Update: Dec. 15, 2022 – NASA, the French space agency, and SpaceX are now targeting 3:46 a.m. PST (6:46 a.m. EST) on Friday, Dec.16, for the launch of the Surface Water and Ocean Topography (SWOT) satellite. Visit NASA's SWOT launch blog for the latest updates.

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NASA is launching an Earth-orbiting mission that will map the planet’s surface water resources better than ever before. Scheduled to launch on Dec. 16 from Vandenberg Space Force Base in California, the Surface Water and Ocean Topography, or SWOT mission is the latest international collaboration designed to monitor and report on our home planet. By providing us with a highly detailed 3D view of rivers, lakes, and oceans, SWOT promises to improve our understanding of Earth’s water cycle and the role oceans play in climate change, as well as help us better respond to drought and flooding.

Read on to find out why we're hoping to learn more about Earth's surface water, get to know the science behind SWOT's unique design, and follow along with STEM teaching and learning resources.

Why It's Important

Observing Earth from space provides scientists with a global view that is important for understanding the whole climate system. In the case of SWOT, we will be able to monitor Earth’s surface water with unprecedented detail and accuracy. SWOT will provide scientists with measurements of water volume change and movement that will inform our understanding of fresh water availability, flood hazards, and the mechanisms of climate change.

Scientists and engineers provide an overview of the SWOT mission. Credit: NASA/JPL-Caltech | Watch on YouTube

Water Flow

Scientists use a variety of methods to track Earth’s water. These include stream and lake gauges and even measurements from space such as sea surface altimetry and gravitational measurements of aquifer volumes. Monitoring of river flow and lake volume is important because it can tell us how much freshwater is readily available and at what locations. River flow monitoring can also help us make inferences about the downstream environmental impact. But monitoring Earth’s surface water in great detail with enough frequency to track water movement has proven challenging. Until now, most monitoring of river flow and lake levels has relied on water-flow and water-level gauges placed across Earth, which requires that they be accessible and maintained. Not all streams and lakes have gauges and previous space-based altimetry and gravitational measurements, though useful for large bodies of water, have not been able to adequately track the constant movement of water through smaller rivers or lakes.

Here's why understanding Earth’s "water budget" is an important part of understanding our planet and planning for future water needs.

SWOT will be able to capture these measurements across the globe in 3D every 21 days. The mission will monitor how much water is flowing through hundreds of thousands of rivers wider than 330 feet (100 meters) and keep a close watch on the levels of more than a million lakes larger than 15 acres (6 hectares). Data from the mission will be used to create detailed maps of rivers, lakes, and reservoirs that will enable accurate monitoring to provide a view of freshwater resources that is not reliant on physical access. Meanwhile, SWOT’s volumetric measurements of rivers, lakes, and reservoirs will help hydrologists better track drought and flooding impacts in near-real-time.

Coastal Sea Level Rise

SWOT will measure our oceans with unprecedented accuracy, revealing details of ocean features as small as 9 miles (15 kilometers) across. SWOT will also monitor sea levels and tides. Though we have excellent global sea level data, we do not have detailed sea level measurements near coastlines. Coastal sea levels vary across the globe as a result of ocean currents, weather patterns, land changes, and other factors. Sea levels are rising faster than ever, and higher sea levels also mean that hurricane storm surges will reach farther inland than ever before, causing substantially more damage than the same category of hurricanes in the past. SWOT will be able to monitor coastal sea level variations and fill gaps in the observations we currently have from other sources.

What is sea level rise and what does it mean for our planet? | › View Transcript

Ocean Heat Sinks

Further contributing to our understanding of the role Earth’s oceans play in climate change, SWOT will explore how the ocean absorbs atmospheric heat and carbon, moderating global temperatures and climate change. Scientists understand ocean circulation on a large scale and know that ocean currents are driven by temperature and salinity differences. However, scientists do not currently have a good understanding of fine-scale ocean currents, where most of the ocean's motion-related energy is stored and lost. Circulation at these fine scales is thought to be responsible for transporting half of the heat and carbon from the upper ocean to deeper layers. Such downward ocean currents have helped to mitigate the decades-long rise in global air temperatures by absorbing and storing heat and carbon away from the atmosphere. Knowing more about this process is critical for understanding the mechanisms of global climate change.

JPL scientist Josh Willis uses a water balloon to show how Earth's oceans are absorbing most of the heat being trapped on our warming world. | › Related lesson

These fine-scale ocean currents also transport nutrients to marine life and circulate pollutants such as crude oil and debris. Understanding nutrient transport helps oceanographers assess ocean health and the productivity of fisheries. And tracking pollutants aids in natural hazard assessment, prediction, and response.

How It Works

A joint effort between NASA and the French space agency – with contributions from the Canadian and UK space agencies – SWOT will continue NASA’s decades-long record of monitoring sea surface height across the globe. But this mission will add a level of detail never before achieved.

SWOT will measure more than 90% of Earth’s surface water, scanning the planet between 78°N latitude and 78°S latitude within 1 centimeter of accuracy and retracing the same path every 21 days. Achieving this level of accuracy from a spacecraft height of 554 miles (891 kilometers) requires that the boom using radar to measure water elevation remain stable within 2 microns – or about 3% of the thickness of a human hair.

This visualization shows ocean surface currents around the world during the period from June 2005 through December 2007. With its new, high resolution wide-swath measurements, SWOT will be able to observe eddies and current features at greater resolution than previously possible. Credit: NASA Scientific Visualization Studio | Watch on YouTube

Prior to SWOT, spacecraft have used conventional nadir, or straight-down, altimetry to measure sea surface height. Conventional nadir altimetry sends a series of radar or laser pulses down to the surface and measures the time it takes for each signal to return to the spacecraft, thus revealing distances to surface features. To acquire more detailed information on surface water, SWOT will use an innovative instrument called the Ka-band Radar Interferometer, or KaRIn, to measure water height with exceptional accuracy. Ka-band is a portion of the microwave part of the electromagnetic spectrum. SWOT uses microwaves because they can penetrate clouds to return data about water surfaces.

The KaRIn instrument uses the principles of synthetic aperture radar combined with interferometry to measure sea surface height. A radar signal is emitted from the end of the 10-meter-wide boom on the spacecraft. The reflected signal is then received by antennas on both ends of the boom, capturing data from two 30-mile (50-kilometer) wide swaths on either side of the spacecraft. The received signals will be slightly out of sync, or phase, from one another because they will travel different distances to return to the receivers on either end of the boom. Knowing the phase difference, the distance between the antennas, and the radar wavelength allows us to calculate the distance to the surface.

The observations acquired by the two antennas can be combined into what is known as an interferogram. An interferogram is a pattern of wave interference that can reveal more detail beyond the 1-centimeter resolution captured by the radar. To explain how it works, we'll recall a couple of concepts from high school physics. When out-of-phase waves from the two antennas are combined, constructive and destructive interference patterns result in some wave crests being higher and some wave troughs being lower than those of the original waves. The patterns that result from the combination of the waves reveal more detail with resolution better than the 1-centimeter wavelength of the original Ka-band radar waves because the interference occurs over a portion of a wavelength. An interferogram can be coupled with elevation data to reveal a 3D representation of the water’s surface.

This highly accurate 3D view of Earth’s surface water is what makes SWOT so unique and will enable scientists to more closely monitor the dynamics of the water cycle. In addition to observing ocean currents and eddies that will inform our understanding of the ocean’s role in climate change, SWOT's use of interferometry will allow scientists to track volumetric changes in lakes and quantify river flooding, tasks that cannot yet be done on a wide scale in any other way.

Follow Along

SWOT is scheduled to launch no earlier than Dec. 16, 2022, on a SpaceX Falcon 9 rocket from Vandenberg Space Force Base in California. Tune in to watch the launch on NASA TV.

After launch, the spacecraft will spend 6-months in a calibration and validation phase, during which it will make a full orbit of Earth every day at an altitude of 553 miles (857 kilometers). Upon completion of this phase, SWOT will increase its altitude to 554 miles (891 kilometers) and assume a 21-day repeat orbit for the remainder of its mission.

Visit the mission website to follow along as data are returned and explore the latest news, images, and updates as SWOT provides a new view on one of our planet's most important resources.

Teach It

The SWOT mission is the perfect opportunity to engage students in studying Earth’s water budget and water cycle. Explore these lessons and resources to get students excited about the STEM involved in studying Earth’s water and climate change from space.

Educator Resources

• 
  Collection

  SWOT Mission Lessons for Educators

  Explore the science and engineering behind the SWOT mission with this collection of standards-aligned lessons all about water.

• 
  Collection

  Climate Change Lessons for Educators

  Explore a collection of standards-aligned STEM lessons for students that get them investigating climate change along with NASA.

• 
  Collection

  Teachable Moments in Climate Change

  Explore this collection of Teachable Moments articles to get a primer on the latest NASA Earth science missions, plus find related education resources you can deploy right away!

• 
  Expert Talk

  Teaching Space With NASA – Monitoring Earth from Space

  In this educational talk, NASA experts discuss how we build spacecraft to study climate, then answer audience questions.

Student Activities

• 
  Collection

  SWOT Mission Activities for Students

  Explore projects, videos, slideshows, and games for students all about the water cycle and sea level rise.

• 
  Collection

  Climate Change Activities for Students

  Learn about climate change and its impacts with these projects, videos, and slideshows for students.

• 
  Collection

  Earth Minute Video Series

  This series of animated white-board videos for students of all ages explains key concepts about Earth science, missions, and climate change.

Explore More

Activities for Kids

• Download: SWOT Launch Bingo
• Video: How Much Water is on Earth?
• Game: Go With the Flow – An Ocean Currents Game

Websites

• SWOT Mission Website
• NASA Climate Change
• NASA Earth Observatory
• NASA Climate Kids
• NASA Sea Level Change
• NASA Cambio Climático en Español

Facts & Figures

• NASA Climate Change: Evidence
• NASA Earth Science Missions

Videos

• Mission Makers - SWOT
• SWOT Mission - YouTube Playlist

Interactives

• Earth Now
• SWOT Swath Visualizer
• Sea Level Evaluation and Assessment Tool

Image Gallery

• NASA climate images, videos, and graphics
• Images of Change

Articles

• Climate articles from NASA
• Ask NASA Climate
• NASA People - Earth
• Water Mission to Gauge Alaskan Rivers on Front Lines of Climate Change

Podcast

• On a Mission

TAGS: K-12 Education, Teachers, Educators, Earth Science, Earth, Climate Change, Climate, Satellites, Teachable Moments

• 

  ABOUT THE AUTHOR

  Ota Lutz, K-12 Education Group Manager, NASA-JPL Education Office

  Ota Lutz is the manager of the K-12 Education Group at NASA’s Jet Propulsion Laboratory. When she’s not writing new lessons or teaching, she’s probably cooking something delicious, volunteering in the community, or dreaming about where she will travel next.

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Update: Oct. 20, 2022 – The DART spacecraft successfully impacted the asteroid Dimorphos on September 26, reducing the period of the asteroid's orbit by 32 minutes. Scientists considered a change of 73 seconds to be the minimum amount for success. This article has been updated to reflect the latest data and images from the impact.

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In a successful attempt to alter the orbit of an asteroid for the first time in history, NASA crashed a spacecraft into the asteroid Dimorphos on Sept. 26, 2022. The mission, known as the Double Asteroid Redirection Test, or DART, took place at an asteroid that posed no threat to our planet. Rather, it was an ideal target for NASA to test an important element of its planetary defense plan.

Read further to learn about DART, how it worked, and how the science and engineering behind the mission can be used to teach a variety of STEM topics.

Why It's Important

The vast majority of asteroids and comets are not dangerous, and never will be. Asteroids and comets are considered potentially hazardous objects, or PHOs, if they are 100-165 feet (30-50 meters) in diameter or larger and their orbit around the Sun comes within five million miles (eight million kilometers) of Earth’s orbit. NASA's planetary defense strategy involves detecting and tracking these objects using telescopes on the ground and in space. In fact, NASA’s Center for Near Earth Object Studies, or CNEOS, monitors all known near-Earth objects to assess any impact risk they may pose. Any relatively close approach is reported on the Asteroid Watch dashboard.

While there are no known objects currently posing a threat to Earth, scientists continue scanning the skies for unknown asteroids. NASA is actively researching and planning for ways to prevent or reduce the effects of a potential impact, should one be discovered. The DART mission was the first test of such a plan – in this case, whether it was possible to divert an asteroid from its predicted course by slamming into it with a spacecraft.

Eyes on Asteroids is a real-time visualization of every known asteroid or comet that is classified as a near-Earth object, or NEO. Asteroids are represented as blue dots and comets as shown as white dots. Use your mouse to explore the interactive further and learn more about the objects and how we track them. Credit: NASA/JPL-Caltech | Explore the full interactive

With the knowledge gained from the demonstration, similar techniques could be used in the future to deflect an asteroid or comet away from Earth if it were deemed hazardous to the planet.

How It Worked

With a diameter of about 525 feet (160 meters) – the length of 1.5 football fields – Dimorphos is the smaller of two asteroids in a double-asteroid system. Before DART's impact, Dimorphos orbited the larger asteroid called Didymos (Greek for "twin"), every 11 hours and 55 minutes.

Neither asteroid poses a threat to our planet, which is one reason why this asteroid system was the ideal place to test asteroid redirection techniques. At the time of DART's impact, the asteroid pair was 6.8 million miles (11 million kilometers) away from Earth as they traveled on their orbit around the Sun.

The DART spacecraft was designed to collide head-on with Dimorphos to alter its orbit, shortening the time it takes the small asteroid to travel around Didymos. Compared with Dimorphos, which has a mass of about 11 billion pounds (five billion kilograms), the DART spacecraft was light. It weighed just 1,210 pounds (550 kilograms) at the time of impact. So how did such a light spacecraft affect the orbit of a relatively massive asteroid?

You can use your mouse to explore this interactive view of DART's impact with Dimorphos from NASA's Eyes on the Solar System. Credit: NASA/JPL-Caltech | Explore the full interactive

DART was designed as a kinetic impactor, meaning it transferred its momentum and kinetic energy to Dimorphos upon impact, altering the asteroid's orbit in return. Scientists were able to make predictions about some of these effects thanks to principles described in Newton's laws of motion.

Newton’s first law told us that the asteroid’s orbit would remain unchanged until something acted upon it. Using the formula for linear momentum (p = m * v), we could calculate that the spacecraft, which at the time of impact would be traveling at 3.8 miles (6.1 kilometers) per second, would have about 0.5% of the asteroid’s momentum. The momentum of the spacecraft may seem small in comparison, but calculations suggested it would be enough to make a detectable change in the speed of Dimorphos' orbit. However, mission planners felt that changing Dimorphos’ orbit by at least 73 seconds would be enough to consider the test a success.

But there was more to consider in testing whether the technique could be used in the future for planetary defense. For example, the formula for kinetic energy (KE = 0.5 * m * v2) tells us that a fast moving spacecraft possesses a lot of energy.

When DART hit the surface of the asteroid, its kinetic energy was 10 billion joules! A crater was formed and material known as ejecta was blasted out as a result of the impact. Scientists are still studying the data returned from the mission to determine the amount of material ejected out of the crater, but estimates prior to impact put the number at 10-100 times the mass of the spacecraft itself. The force needed to push this material out was then matched by an equal reaction force pushing on the asteroid in the opposite direction, as described by Newton’s third law.

This animation shows conceptually how DART's impact is predicted to change Dimorphos' orbit from a larger orbit to a slightly smaller one that's several minutes shorter than the original. Credit: NASA/Johns Hopkins APL/Jon Emmerich | Watch on YouTube

How much material was ejected and its recoil momentum is still unknown. A lot depends on the surface composition of the asteroid, which scientists are still investigating. Laboratory tests on Earth suggested that if the surface material was poorly conglomerated, or loosely formed, more material would be blasted out. A surface that was well conglomerated, or densely compacted, would eject less material.

After the DART impact, scientists used a technique called the transit method to see how much the impact changed Dimorphos' orbit. As observed from Earth, the Didymos pair is what’s known as an eclipsing binary, meaning Dimorphos passes in front of and behind Didymos from our view, creating what appears from Earth to be a subtle dip in the combined brightness of the pair. Scientists used ground-based telescopes to measure this change in brightness and calculate how quickly Dimorphos orbits Didymos. By comparing measurements from before and after impact, scientists determined that the orbit of Dimorphos had slowed by 32 minutes to 11 hours and 23 minutes.

One of the biggest challenges of the DART mission was navigating a small spacecraft to a head-on collision with a small asteroid millions of miles away. To solve that problem, the spacecraft was equipped with a single instrument, the DRACO camera, which worked together with an autonomous navigation system called SMART Nav to guide the spacecraft without direct control from engineers on Earth. About four hours before impact, images captured by the camera were sent to the spacecraft's navigation system, allowing it to identify which of the two asteroids was Dimorphos and independently navigate to the target.

DART was not just an experimental asteroid impactor. The mission also used cutting-edge technology never before flown on a planetary spacecraft and tested new technologies designed to improve how we power and communicate with spacecraft.

Learn more about the engineering behind the DART mission, including the innovative Roll Out Solar Array and NEXT-C ion propulsion system, in this video featuring experts from the mission. Credit: APL | Watch on YouTube

One such technology that was first tested on the International Space Station and was later used on the solar-powered DART spacecraft, is the Roll Out Solar Array, or ROSA, power system. As its name suggests, the power system consisted of flexible solar panel material that was rolled up for launch and unrolled in space.

Some of the power generated by the solar array was used for another innovative technology, the spacecraft's NEXT-C ion propulsion system. Rather than using traditional chemical propulsion, DART was propelled by charged particles of xenon pushed from its engine. Ion propulsion has been used on other missions to asteroids and comets including Dawn and Deep Space 1, but DART's ion thrusters had higher performance and efficiency.

Follow Along

In the days following the event, NASA received images of the impact from a cubesat, LICIACube, that was deployed by DART before impact. The cubesat, which was provided by the Italian Space Agency, captured images of the impact and the ejecta cloud.

Meanwhile, the James Webb Space Telescope, the Hubble Space Telescope, and the Lucy spacecraft observed Didymos to monitor how soon reflected sunlight from the ejecta plume could be seen. Going forward, DART team members will continue observing the asteroid system to measure the change in Dimorphos’ orbit and determine what happened on its surface. And in 2024, the European Space Agency plans to launch the Hera spacecraft to conduct an in-depth post-impact study of the Didymos system.

Continue following along with all the science from DART, including the latest images and updates on the mission website. Plus, explore even more resources on this handy page.

Teach It

The mission is a great opportunity to engage students in the real world applications of STEM topics. Start exploring these lessons and resources to get students engaging in STEM along with the mission.

Educator Guides

• 
  Collection

  DART Lessons for Educators

  Use these standards-aligned lessons for grades K-12 to get students exploring the engineering and science behind the DART mission.

Expert Talks

• 
  Teaching Space With NASA

  Tracking Asteroids

  In this educational talk, NASA experts will discuss how we track and study comets and asteroids. Plus, we'll answer your questions!

Student Activities

• 
  Collection

  DART Activities for Students

  Explore STEM projects, slideshows and videos for students related to the DART mission.

Articles

• 
  Teachable Moments

  How NASA Studies and Tracks Asteroids Near and Far

  Here’s how NASA uses math and science to track the movements of asteroids and find out what they’re made of – and students can, too.

• 
  Meet JPL Interns

  From Island Life to Spotting Asteroids for NASA

  Meet a JPL intern whose journey took her from the remote island of Saipan to a team helping track asteroids at NASA.

Resources for Kids

Check out these related resources for kids from NASA Space Place:

• Article for Kids: Asteroid or Meteor: What's the Difference?
• Article for Kids: What Is an Asteroid?
• Article for Kids: Why Does the Moon Have Craters?
• Article for Kids: What Is an Impact Crater?

Explore More

• Facts & Figures: Didymos In Depth
• Facts & Figures: DART Mission
• Website: DART Mission
• Gallery: DART Mission Images and Videos
• Facts & Figures: Asteroid Watch
• Gallery: Next Five Asteroid Approaches
• Articles: Asteroid News and Images from JPL
• Eyes on Asteroids
• Eyes on the Solar System - DART Impact
• Quiz: Are You a Planetary Defnder?
• Center for Near-Earth Object Studies

TAGS: Asteroids and Comets, DART, near-Earth objects, planetary defense, Science, K-12 Education, Teachers, Educators, Parents, Teachable Moments

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  ABOUT THE AUTHOR

  Lyle Tavernier, Educational Technology Specialist, NASA-JPL Education Office

  Lyle Tavernier is an educational technology specialist at NASA's Jet Propulsion Laboratory. When he’s not busy working in the areas of distance learning and instructional technology, you might find him running with his dog, cooking or planning his next trip.

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Our home galaxy, the Milky Way, has a supermassive black hole at its center, but we’ve never actually seen it – until now. The Event Horizon Telescope, funded by the National Science Foundation, has released the first image of our galactic black hole, Sagittarius A* (pronounced “Sagittarius A-star” and abbreviated Sgr A*).

Read on to find out how the image was acquired and learn more about black holes and Sagittarius A*. Then, explore resources to engage learners in the exciting topic of black holes.

How Black Holes Work

A black hole is a location in space with a gravitational pull so strong that nothing, not even light, can escape it. A black hole’s outer edge, called its event horizon, defines the spherical boundary where the velocity needed to escape exceeds the speed of light. Matter and radiation fall in, but they can’t get out. Because not even light can escape, a black hole is literally black. Contrary to their name’s implication, black holes are not empty. In fact, a black hole contains a great amount of matter packed into a relatively small space. Black holes come in various sizes and can exist throughout space.

We can surmise a lot about the origin of black holes from their size. Scientists know how some types of black holes form, yet the formation of others is a mystery. There are three different types of black holes, categorized by their size: stellar-mass, intermediate-mass, and supermassive black holes.

Stellar-mass black holes are found throughout our Milky Way galaxy and have masses less than about 100 times that of our Sun. They comprise one of the possible endpoints of the lives of high-mass stars. Stars are fueled by the nuclear fusion of hydrogen, which forms helium and other elements deep in their interiors. The outflow of energy from the central regions of the star provides the pressure necessary to keep the star from collapsing under its own weight.

Once the fuel in the core of a high-mass star has completely burned out, the star collapses, sometimes producing a supernova explosion that releases an enormous amount of energy, detectable across the electromagnetic spectrum. If the star’s mass is more than about 25 times that of our Sun, a stellar-mass black hole can form.

Intermediate-mass black holes have masses between about 100 and 100,000 times that of our Sun. Until recently, the existence of intermediate-mass black holes had only been theorized. NASA’s Chandra X-ray Observatory has identified several intermediate-mass black hole candidates by observing X-rays emitted by the gas surrounding the black hole. The Laser Interferometer Gravitational Wave Observatory, or LIGO, funded by the National Science Foundation, detected the merger of two stellar-mass black holes with masses 65 and 85 times that of our Sun forming an intermediate-mass black hole of 142 solar masses. (Some of the mass was converted to energy and about nine solar masses were radiated away as gravitational waves.)

Supermassive black holes contain between a million and a billion times as much mass as a stellar-mass black hole. Scientists are uncertain how supermassive black holes form, but one theory is that they result from the combining of stellar-mass black holes.

Our local galactic center’s black hole, Sagittarius A*, is a supermassive black hole with a mass of about four million suns, which is fairly small for a supermassive black hole. NASA’s Hubble Space Telescope and other telescopes have determined that many galaxies have supermassive black holes at their center.

Why They're Important

Black holes hold allure for everyone from young children to professional astronomers. For astronomers, in particular, learning about Sagittarius A* is important because it provides insights into the formation of our galaxy and black holes themselves.

Understanding the physics of black hole formation and growth, as well as their surrounding environments, gives us a window into the evolution of galaxies. Though Sagittarius A* is more than 26,000 light years (152 quadrillion miles) away from Earth, it is our closest supermassive black hole. Its formation and physical processes influence our galaxy as galactic matter continually crosses the event horizon, growing the black hole’s mass.

Studying black holes also helps us further understand how space and time interact. As one gets closer to a black hole, the flow of time slows down compared with the flow of time far from the black hole. In fact, according to Einstein’s theory of general relativity, the flow of time slows near any massive object. But it takes an incredibly massive object, such as a black hole, to make an appreciable difference in the flow of time. There's still much to learn about what happens to time and space inside a black hole, so the more we study them, the more we can learn.

How Scientists Imaged Sagittarius A*

Black holes, though invisible to the human eye, can be detected by observing their effects on nearby space and matter. As a result of their enormous mass, black holes have extremely high gravity, which pulls in surrounding material at rapid speeds, causing this material to become very hot and emit X-rays.

This video explains how Sagittarius A* appears to still have the remnants of a blowtorch-like jet dating back several thousand years. Credit: NASA | Watch on YouTube

X-ray-detecting telescopes such as NASA’s Chandra X-ray Observatory can image the material spiraling into a black hole, revealing the black hole’s location. NASA’s Hubble Space Telescope can measure the speed of the gas and stars orbiting a point in space that may be a black hole. Scientists use these measurements of speed to determine the mass of the black hole. Hubble and Chandra are also able to image the effects of gravitational lensing, or the bending of light that results from the gravitational pull of black holes or other high-mass objects such as galaxies.

To directly image the matter surrounding a black hole, thus revealing the silhouette of the black hole itself, scientists from around the world collaborated to create the Event Horizon Telescope. The Event Horizon Telescope harnesses the combined power of numerous telescopes around the world that can detect radio-wave emissions from the sky to create a virtual telescope the size of Earth.

Narrated by Caltech’s Katie Bouman, this video explains how she and her fellow teammates at the Event Horizon Telescope project managed to take a picture of Sagittarius A* (Sgr A*), a beastly black hole lying 27,000 light-years away at the heart of our Milky Way galaxy. Credit: Caltech | Watch on YouTube

In 2019, the team released the first image of a black hole's silhouette when they captured the glowing gasses surrounding the M87* galactic black hole nearly 53 million light-years (318 quintillion miles) away from Earth. The team then announced that one of their next endeavors was to image Sagittarius A*.

To make the newest observation, the Event Horizon Telescope focused its array of observing platforms on the center of the Milky Way. A telescope array is a group of telescopes arranged so that, as a set, they function similarly to one giant telescope. In addition to the telescopes used to acquire the M87* image, three additional radio telescopes joined the array to acquire the image of Sagittarius A*: the Greenland Telescope, the Kitt Peak 12-meter Telescope in Arizona, and the NOrthern Extended Millimeter Array, or NOEMA, in France.

This image of the center of our Milky Way galaxy representing an area roughly 400 light years across, has been translated into sound. Listen for the different instruments representing the data captured by the Chandra X-ray Observatory, Hubble Space Telescope, and Spitzer Space Telescope. The Hubble data outline energetic regions where stars are being born, while Spitzer's data captures glowing clouds of dust containing complex structures. X-rays from Chandra reveal gas heated to millions of degrees from stellar explosions and outflows from Sagittarius A*. Credit: Chandra X-ray Observatory | Watch on YouTube

The distance from the center of Sagittarius A* to its event horizon, a measurement known as the Schwarzschild radius, is enormous at seven million miles (12,000,000 kilometers or 0.08 astronomical units). But its apparent size when viewed from Earth is tiny because it is so far away. The apparent Schwarzschild radius for Sagittarius A* is 10 microarcseconds, about the angular size of a large blueberry on the Moon.

Acquiring a good image of a large object that appears tiny when viewed from Earth requires a telescope with extraordinarily fine resolution, or the ability to detect the smallest possible details in an image. The better the resolution, the better the image and the more detail the image will show. Even the best individual telescopes or array of telescopes at one location do not have a good enough resolution to image Sagittarius A*.

The addition of the 12-meter Greenland Telescope, though a relatively small instrument, widened the diameter, or aperture, of the Event Horizon Telescope to nearly the diameter of Earth. And NOEMA – itself an array of twelve 15-meter antennas with maximum separation of 2,500 feet (760 meters) – helped further increase the Event Horizon Telescope’s light-gathering capacity.

Altogether, when combined into the mighty Event Horizon Telescope, the virtual array obtained an image of Sagittarius A* spanning about 50 microarcseconds, or about 1/13th of a billionth the span of the night sky.

While the Event Horizon Telescope was busy capturing the stunning radio image of Sagittarius A*, an additional worldwide contingent of astronomical observatories was also focused on the black hole and the region surrounding it. The aim of the team, known as the Event Horizon Telescope Multiwavelength Science Working Group, was to observe the black hole in other parts of the electromagnetic spectrum beyond radio. As part of the effort, X-ray data were collected by NASA’s Chandra X-ray Observatory, Nuclear Spectroscopic Telescope (NuSTAR), and Neil Gehrels Swift Observatory, additional radio data were collected by the East Asian Very Long-Baseline Interferometer (VLBI) network and the Global 3 millimeter VLBI array, and infrared data were collected by the European Southern Observatory’s Very Large Telescope.

The data from these multiple platforms will allow scientists to continue building their understanding of the behavior of Sagittarius A* and to refine their models of black holes in general. The data collected from these multiwavelength observations are crucial to the study of black holes, such as the Chandra data revealing how quickly material falls in toward the disk of hot gas orbiting the black hole’s event horizon. Data such as these will hopefully help scientists better understand black hole accretion, or the process by which black holes grow.

Teach It

Check out these resources to bring the real-life STEM of black holes into your teaching, plus learn about opportunities to involve students in real astronomy research.

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  Educator Guide: Dropping In With Gravitational Waves

  Students develop a model to represent the collision of two black holes, the gravitational waves that result and the waves' propagation through spacetime.

  Subject Science

  Grades 6-8

  Time 30-60 mins

• 
  Teachable Moments: How Scientists Captured the First Image of a Black Hole

  Find out how scientists created a virtual telescope as large as Earth itself to capture the first image of a black hole's silhouette.

• 
  Teachable Moments: Gravitational Waves Detected for the First Time

  Find out how researchers proved part of Albert Einstein’s Theory of General Relativity, then create a model of the Nobel Prize-winning experiment in the classroom.

Explore More

Articles

• 
  Teachable Moments: Learn About the Universe With the James Webb Space Telescope

  Get a look into the science and engineering behind the largest and most powerful space telescope ever built while exploring ways to engage learners in the mission.

• 
  JPL Education ‘Teachable Moment’ Inspires Winning Science Fair Project

  A “teachable moment” turned into a science fair win for an eighth-grader in Ontario, Canada, who based his project on a classroom activity from NASA’s Jet Propulsion Laboratory.

Educator Guides

• 
  How Do We See Dark Matter?

  Students will make observations of two containers and identify differences in content, justify their claims and make comparisons to dark matter observations.

  Subject Science

  Grades 6-12

  Time < 30 mins

Student Activities

• 
  Black Holes: By the Numbers

  What are black holes and how do they form?

  Subject Science

  Grades 4-12

  Time Less than 30 mins

Check out these related resources for students from NASA’s Space Place

• What is a Black Hole?

Across the NASA-Verse

• Educator Guide: Black Hole Math
• NASA/IPAC TeacherArchive Research Program
• Student Resources: Chandra
• Articles: Hubble - Black Holes
• Audio: Sonification of the Milky Way galactic center
• Audio: Sonification of the M87 black hole
• Interactive: Sagittarius A*
• Videos: Hubble - Black Holes
• Website: NASA Science - Black Holes
• Download: A Galaxy Full of Black Holes Presentation
• Expert Talk: Imaging a Black Hole Lecture
• Website: NASA - Black Holes
• Article: Black Hole Image Makes History
• Graphic: Anatomy of a Black Hole

---

This Teachable Moment was created in partnership with NASA’s Universe of Learning. Universe of Learning materials are based upon work supported by NASA under award number NNX16AC65A to the Space Telescope Science Institute, working in partnership with Caltech/IPAC, Center for Astrophysics | Harvard & Smithsonian, and the Jet Propulsion Laboratory.

TAGS: Black hole, Milky Way, galaxy, universe, stars, teachers, educators, lessons, Teachable Moments, K-12, science

• 

  ABOUT THE AUTHOR

  Ota Lutz, K-12 Education Group Manager, NASA-JPL Education Office

  Ota Lutz is the manager of the K-12 Education Group at NASA’s Jet Propulsion Laboratory. When she’s not writing new lessons or teaching, she’s probably cooking something delicious, volunteering in the community, or dreaming about where she will travel next.

---

A NASA instrument launched to the International Space Station this summer will explore how dust impacts global temperatures, cloud formation, and the health of our oceans. The Earth Surface Mineral Dust Source Investigation, or EMIT, is the first instrument of its kind, designed to collect measurements from space of some of the most arid regions on Earth to understand the composition of soils that generate dust and the larger role dust plays in climate change.

Read on to find out how the instrument works and why scientists are hoping to learn more about the composition of dust. Then, explore how to bring the science into your classroom with related climate lessons that bridge physical sciences with engineering practices.

Why It’s Important

Scientists have long studied the movements of dust. The fact that dust storms can carry tiny particles great distances was reported in the scientific literature nearly two centuries ago by none other than Charles Darwin as he sailed across the Atlantic on the HMS Beagle. What still remains a mystery all these years later is what that dust is made of, how it moves, and how that affects the health of our planet.

For example, we now know that dust deposited on snow speeds up snow melt even more than increased air temperature. That is to say, that dust traveling to cold places can cause increased snow melt.

Dust can affect air temperatures as well. For example, dust with more iron absorbs light and can cause the air to warm, while dust with less iron reflects light and is responsible for local cooling. Iron in dust can also act as a fertilizer for plankton in oceans, supplying them with nutrients needed for growth and reproduction.

Floating dust potentially alters the composition of clouds and how quickly or slowly they form, which can ultimately impact weather patterns, including the formation of hurricanes. That’s because clouds need particles to act as seeds around which droplets of moisture in the atmosphere can form. This process of coalescing water particles, called nucleation, is one factor in how clouds form.

Thanks to EMIT, we’ll take the first steps in understanding how the movements of dust particles contribute to local and global changes in climate by producing “mineral maps”. These mineral maps will reveal differences in the chemical makeup of dust, providing essential information to help us model the way dust can transform Earth’s climate.

› Learn more about what EMIT will do from JPL News

How It Works

NASA has been exploring how dust moves across the globe by combining on-the-ground field studies with cutting-edge technology.

Dr. Olga Kalashnikova, an aerosol scientist at NASA's Jet Propulsion Laboratory and a co-investigator for EMIT, has been using satellite data to study atmospheric mineral dust for many years, including tracking the movements of dust and investigating trends in the frequency of dust storms.

As Dr. Kalashnikova describes, “From the ground, we can see what types of dusts are lifted into the atmosphere by dust storms on a local scale, but with EMIT, we can understand how they differ and where they originally came from.”

EMIT is the first instrument designed to observe a key part of the mineral dust cycle from space, allowing scientists to track different dust compositions on a global scale, instead of in just one region at a time. To understand dust’s impact on Earth’s climate, scientists will use EMIT to answer key questions, including:

• How does dust uplifted in the atmosphere alter global temperatures?
• What role do dusts play in fertilizing our oceans when they are deposited?
• How do dust particles in the atmosphere affect cloud nucleation; the process by which clouds are ‘seeded’ and begin to coalesce into larger clouds?

To achieve its objectives, EMIT will spend 12 months collecting what are called “hyperspectral images” of some of the most arid regions of our planet selected by scientists and engineers as areas of high dust mobility, such as Northern Africa, the Middle East, and the American Southwest.

These images are measurements of light reflected from the Earth below, calibrated to the distinct patterns, or spectra, of light we see when certain minerals are present. The EMIT team has identified 10 minerals that are most common, including gypsum, hematite, and kaolinite.

Why are these minerals important? One key reason is the presence or absence of the element iron, found in some minerals but not others.

Dr. Bethany Ehlmann is a planetary scientist and co-investigator for the EMIT project at Caltech and explains that when it comes to heating, “a little bit of iron goes a long way.” Iron in minerals absorbs visible and infrared light, meaning that even if only a small amount is present, it will result in a much warmer dust particle. Large amounts of warm dust in our atmosphere may have an impact on temperatures globally since those dust particles radiate heat as they travel, sometimes as far as across oceans!

Collecting images from space is, of course, no easy task, especially when trying to look only at the ground below. Yet it does allow scientists to get a global picture that's not possible to capture from the ground. Field studies allow us to take individual samples from tiny places of interest, but from space, we can scan the entire planet in remote places where no scientist can visit.

Of course, there are some complications in trying to study the light reflected off the surface of Earth, such as interference from clouds. To prevent this problem, the EMIT team plans to collect data at each location several times to ensure that the images aren’t being obscured by clouds between the instrument and the minerals we’re looking for.

The data collected by EMIT will provide a map of the compositions of dust from dry, desert environments all over the world, but the team involved won’t stop there. Knowing more about what the dust is made of sets the stage for a broader understanding of a few more of the complex processes that make up our global climate cycle. Upon completion of this study, EMIT's mineral maps will support further campaigns to complete our global dust picture. For example, NASA hopes to couple the data from EMIT with targeted field campaigns, in which scientists can collect wind-blown dust from the ground to learn more about where dust particles move over time and answer questions about what types of dust are on the go.

Furthermore, missions such as the Multiangle Imager for Aerosols, or MAIA, will allow us to better understand the effects of these dust particles on air-quality and public health.

Teach it

Studying Earth’s climate is a complex puzzle, consisting of many trackable features. These can range from sea level to particles in our atmosphere, but each makes a contribution to measuring the health of our planet. Bring EMIT and NASA Earth Science into your classroom with these lessons, articles, and activities to better understand how we’re exploring climate change.

Educator Guides

• 
  Ocean World: Earth Globe Toss Game

  Students use NASA images and a hands-on activity to compare the amounts of land and surface water on our planet.

  Subject Science

  Grades K-6

  Time Less than 30 mins

• 
  Modeling the Water Budget

  Students use a spreadsheet model to understand droughts and the movement of water in the water cycle.

  Subject Science

  Grades 5-8

  Time 30-60 mins

• 
  Graphing Global Temperature Trends

  Students use global temperature data to create models and compare short-term trends to long-term trends.

  Subject Math

  Grades 5-12

  Time 1-2 hrs

• 
  Using Light to Study Planets

  Students build a spectrometer using basic materials as a model for how NASA uses spectroscopy to determine the nature of elements found on Earth and other planets.

  Subject Science

  Grades 6-11

  Time > 2 hrs

• 
  Cloud Computing: A 'Pi in the Sky' Math Challenge

  In this illustrated math problem, students use pi to calculate how much water could be contained within a cloud.

  Subject Math

  Grades 6-12

  Time Less than 30 mins

• 
  More Earth Science Lessons for Educators

  Explore a collection of standards-aligned STEM lessons for students that get them investigating Earth science along with NASA.

Student Activities

• 
  The Types of Clouds and What They Mean

  Learn about cloud types and how they form. Then help NASA scientists studying clouds.

  Subject Science

  Grades K-3

  Time 30-60 mins

• 
  Make a Cloud in a Bottle

  Have you ever wondered how clouds form? In this activity, you can make your own cloud to see for yourself!

  Subject Science

  Grades 4-12

  Time < 30 mins

• 
  Video Series: NASA's Earth Minute

  Learn about the science behind climate change and the NASA missions studying it in these short videos.

  Subject Science

  Grades 2-12

  Time < 30 mins

• 
  The Change of Seasons: Views from Space

  See how seasonal changes affect our planet.

  Subject Science

  Grades 2-12

  Time < 30 mins

• 
  More Earth Science Activities for Students

  Explore Earth science with these projects, videos, and slideshows for students.

Articles

• 
  Teachable Moments

  Reflecting On Greenland’s Melting Glaciers as OMG Mission Concludes

  Explore how the OMG mission discovered more about what's behind one of the largest contributors to global sea level rise.

• 
  Teachable Moments

  Earth Satellite Joins NASA Fleet to Monitor Sea Level, Improve Weather Forecasts

  Learn about the mission and find out how to make classroom connections to NASA Earth science – plus explore related teaching and learning resources.

• 
  Teachable Moments

  Climate Change Collection

  Explore this collection of Teachable Moments articles to get a primer on the latest NASA Earth science missions, plus find related education resources you can deploy right away!

Websites

• NASA Climate Change
• NASA Earth Observatory - Images of Dust and Haze
• NASA Climate Kids
• Recursos En Español: NASA Climate Change

TAGS: Earth, climate, geology, weather, EMIT, Teachers, Classroom, Lessons, Earth Science, Climate Change, Dust, Global Warming, Educators, K-12, Teachable Moments, Climate TM

• 

  ABOUT THE AUTHOR

  Brandon Rodriguez, Educator Professional Development Specialist, NASA-JPL Education Office

  Brandon Rodriguez is the educator professional development specialist at NASA’s Jet Propulsion Laboratory. Outside of promoting STEM education, he enjoys reading philosophy, travel and speaking to your dog like it's a person.

Update: March 15, 2022 – The answers are here! Visit the NASA Pi Day Challenge slideshow to view the illustrated answer keys for each of the problems in the 2022 challenge.

In the News

No matter what Punxsutawney Phil saw on Groundhog Day, a sure sign that spring approaches is Pi Day. Celebrated on March 14, it’s the annual holiday that pays tribute to the mathematical constant pi – the number that results from dividing any circle's circumference by its diameter.

Every year, Pi Day gives us a reason to not only celebrate the mathematical wonder that helps NASA explore the universe, but also to enjoy our favorite sweet and savory pies. Students can join in the fun by using pi to explore Earth and space themselves in our ninth annual NASA Pi Day Challenge.

Read on to learn more about the science behind this year's challenge and find out how students can put their math mettle to the test to solve real problems faced by NASA scientists and engineers as we explore Earth, the Moon, Mars, and beyond!

How It Works

Dividing any circle’s circumference by its diameter gives you an answer of pi, which is usually rounded to 3.14. Because pi is an irrational number, its decimal representation goes on forever and never repeats. In 2021, a supercomputer calculated pi to more than 62 trillion digits. But you might be surprised to learn that for space exploration, NASA uses far fewer digits of pi.

Here at NASA, we use pi to understand how much signal we can receive from a distant spacecraft, to calculate the rotation speed of a Mars helicopter blade, and to collect asteroid samples. But pi isn’t just used for exploring the cosmos. Since pi can be used to find the area or circumference of round objects and the volume or surface area of shapes like cylinders, cones, and spheres, it is useful in all sorts of ways. Architects use pi when designing bridges or buildings with arches; electricians use pi when calculating the conductance of wire; and you might even want to use pi to figure out how much frozen goodness you are getting in your ice cream cone.

In the United States, March 14 can be written as 3.14, which is why that date was chosen for celebrating all things pi. In 2009, the U.S. House of Representatives passed a resolution officially designating March 14 as Pi Day and encouraging teachers and students to celebrate the day with activities that teach students about pi. And that's precisely what the NASA Pi Day Challenge is all about!

The Science Behind the 2022 NASA Pi Day Challenge

This ninth installment of the NASA Pi Day Challenge includes four brain-busters that get students using pi to measure frost deep within craters on the Moon, estimate the density of Mars’ core, calculate the water output from a dam to assess its potential environmental impact, and find how far a planet-hunting satellite needs to travel to send data back to Earth.

Read on to learn more about the science and engineering behind the problems or click the link below to jump right into the challenge.

› Take the NASA Pi Day Challenge

› Educators, get the lesson here!

Lunar Logic

NASA’s Lunar Flashlight mission is a small satellite that will seek out signs of frost in deep, permanently shadowed craters around the Moon’s south pole. By sending infrared laser pulses to the surface and measuring how much light is reflected back, scientists can determine which areas of the lunar surface contain frost and which are dry. Knowing the locations of water-ice on the Moon could be key for future crewed missions to the Moon, when water will be a precious resource. In Lunar Logic, students use pi to find out how much surface area Lunar Flashlight will measure with a single pulse from its laser.

Core Conundrum

Since 2018, the InSight lander has studied the interior of Mars by measuring vibrations from marsquakes and the “wobble” of the planet as it rotates on its axis. Through careful analysis of the data returned from InSight, scientists were able to measure the size of Mars’ liquid core for the first time and estimate its density. In Core Conundrum, students use pi to do some of the same calculations, determining the volume and density of the Red Planet’s core and comparing it to that of Earth’s core.

Dam Deduction

The Surface Water and Ocean Topography, or SWOT mission will conduct NASA's first global survey of Earth's surface water. SWOT’s state-of-the-art radar will measure the elevation of water in major lakes, rivers, wetlands, and reservoirs while revealing unprecedented detail on the ocean surface. This data will help scientists track how these bodies of water are changing over time and improve weather and climate models. In Dam Deduction, students learn how data from SWOT can be used to assess the environmental impact of dams. Students then use pi to do their own analysis, finding the powered output of a dam based on the water height of its reservoir and inferring potential impacts of this quick-flowing water.

Telescope Tango

The Transiting Exoplanet Survey Satellite, or TESS, is designed to survey the sky in search of planets orbiting bright, nearby stars. TESS does this while circling Earth in a unique, never-before-used orbit that brings the spacecraft close to Earth about once every two weeks to transmit its data. This special orbit keeps TESS stable while giving it an unobstructed view of space. In its first two years, TESS identified more than 2,600 possible exoplanets in our galaxy with thousands more discovered during its extended mission. In Telescope Tango, students will use pi to calculate the distance traveled by TESS each time it sends data back to Earth.

Teach It

Celebrate Pi Day by getting students thinking like NASA scientists and engineers to solve real-world problems in NASA Pi Day Challenge. Completing the problem set and reading about other ways NASA uses pi is a great way for students to see the importance of the M in STEM.

Pi Day Resources

• 
  Pi in the Sky Lessons

  Here's everything you need to bring the NASA Pi Day Challenge into the classroom.

  Grades 4-12

  Time Varies

• 
  NASA Pi Day Challenge

  The entire NASA Pi Day Challenge collection can be found in one, handy slideshow for students.

  Grades 4-12

  Time Varies

• 
  How Many Decimals of Pi Do We Really Need?

  While you may have memorized more than 70,000 digits of pi, world record holders, a JPL engineer explains why you really only need a tiny fraction of that for most calculations.

• 
  18 Ways NASA Uses Pi

  Whether it's sending spacecraft to other planets, driving rovers on Mars, finding out what planets are made of or how deep alien oceans are, pi takes us far at NASA. Find out how pi helps us explore space.

• 
  10 Ways to Celebrate Pi Day With NASA on March 14

  Find out what makes pi so special, how it’s used to explore space, and how you can join the celebration with resources from NASA.

• 
  Infographic: Planet Pi

  This poster shows some of the ways NASA scientists and engineers use the mathematical constant pi (3.14) and includes common pi formulas.

• 

  Downloads

  Can't get enough pi? Download this year's NASA Pi Day Challenge graphics, including mobile phone and desktop backgrounds:

  • Pi in the Sky 9 Poster (PDF, 11.2 MB)
  • Lunar Flashlight Background: Phone | Desktop
  • Mars InSight Lander Background: Phone | Desktop
  • SWOT Mission Background: Phone | Desktop
  • TESS Mission - Downlink Background: Phone | Desktop
  • TESS Mission - Science Background (not pictured): Phone | Desktop
  • Medley Background (not pictured): Phone | Desktop
• 
  Pi Day: What's Going 'Round

  Tell us what you're up to this Pi Day and share your stories and photos on our showcase page.

Plus, join the conversation using the hashtag #NASAPiDayChallenge on Facebook, Twitter, and Instagram.

Recursos en español

• 
  18 Maneras en Que la NASA Usa Pi

  Pi nos lleva lejos en la NASA. Estas son solo algunas de las formas en que pi nos ayuda a explorar el espacio.

Related Lessons for Educators

• 
  Planetary Egg Wobble and Newton's First Law

  Students try to determine the interior makeup of an egg (hard-boiled or raw) based on their understanding of center of mass and Newton’s first law of motion.

  Grades 3-8

  Time 30 min to 1 hour

• 
  Whip Up a Moon-Like Crater

  Whip up a moon-like crater with baking ingredients as a demonstration for students.

  Grades 1-6

  Time 30 min to 1 hour

• 
  Exploring Exoplanets with Kepler

  Students use math concepts related to transits to discover real-world data about Mercury, Venus and planets outside our solar system.

  Grades 6-12

  Time 30 min to 1 hour

• 
  Tracking Water Using NASA Satellite Data

  Using real data from NASA’s GRACE satellites, students will track water mass changes in the U.S.

  Grades 4-8

  Time 30 min to 1 hour

• 
  Modeling the Water Budget

  Students use a spreadsheet model to understand droughts and the movement of water in the water cycle.

  Grades 5-8

  Time 30 min to 1 hour

Related Activities for Students

• 
  NASA's Earth Minute: Mission to Earth?

  NASA doesn't just explore outer space! It studies Earth, too, with a fleet of spacecraft and scientists far and wide.

  Type Video

  Subject Science

• 
  Look at the Moon! Journaling Project

  Draw what you see in a Moon Journal and see if you can predict the moon phase that comes next.

  Type Project

  Subject Science

• 
  Mars in a Minute: Are There Quakes on Mars?

  Are there earthquakes on Mars – or rather, "marsquakes"? What could they teach us about the Red Planet?

  Type Video

  Subject Science

Explore More

Infographic

• Mars Quick Facts

Facts and Figures

• Earth's Moon
• Mars
• Earth
• Exoplanet Discoveries Dashboard

Missions and Instruments

• Mars InSight Lander
• TESS Mission
• SWOT Mission
• Lunar Flashlight

Websites

• Exoplanets Exploration
• Mars Exploration
• NASA Climate
• NASA Science: Earth's Moon
• Artemis

TAGS: Pi Day, Pi, Math, NASA Pi Day Challenge, Moon, Lunar Flashlight, Mars, InSight, Earth, Climate, SWOT, Exoplanets, Universe, TESS, Teachers, Educators, Parents, Students, Lessons, Activities, Resources, K-12

• 

  ABOUT THE AUTHOR

  Lyle Tavernier, Educational Technology Specialist, NASA-JPL Education Office

  Lyle Tavernier is an educational technology specialist at NASA's Jet Propulsion Laboratory. When he’s not busy working in the areas of distance learning and instructional technology, you might find him running with his dog, cooking or planning his next trip.

---

Grades K-2

• 
  Make a Paper Mars Helicopter

  In this lesson, students build a paper helicopter, then improve the design and compare and measure performance.

  Subject Engineering

  Grades 2-8

  Time 30-60 mins

• 
  Student Project: Make a Paper Mars Helicopter

  Build a paper helicopter, then see if you can improve the design like NASA engineers did when making the first helicopter for Mars.

  Subject Engineering

  Grades 2-8

  Time 30-60 mins

• 
  What Tools Would You Take to Mars?

  Students decide what they want to learn from a robotic mission to Mars and what tools they will put on their robot to accomplish their goals.

  Subject Science

  Grades K-2

  Time 30-60 mins

• 
  Rockets by Size

  Students cut out, color and sequence paper rockets in a simple mathematics lesson on measurement.

  Subject Math

  Grades K-2

  Time 30-60 mins

• 
  Rocket Math

  Students use rocket manipulatives to help them develop number sense, counting, addition and subtraction skills.

  Subject Math

  Grades K-1

  Time 30-60 mins

• 
  Tangram Rocket

  Students use tangrams to create rockets while practicing shape recognition.

  Subject Math

  Grades K-1

  Time 1-2 hrs

• 
  Student Project: Build a Rover and More With Shapes

  Use geometric shapes called tangrams to build a rover and other space-themed designs!

  Subject Math

  Grades K-2

  Time Less than 30 mins

• 
  Student Project: Build a Rocket and More With Shapes

  Use geometric shapes called tangrams to build a rocket and other space-themed designs!

  Subject Math

  Grades K-2

  Time Less than 30 mins

• 
  Mineral Mystery Experiment

  Students explore the science behind an intriguing planetary feature by creating saline solutions and then observing what happens when the solutions evaporate.

  Subject Science

  Grades 2-12

  Time 2 sessions of 30-60 mins

• 
  Student Project: Do a Mineral Mystery Experiment

  Dissolve salts in water, then observe what happens when the water evaporates.

  Subject Science

  Grades 2-12

  Time 2 sessions of 30-60 mins

• 
  What Do You Know About Mars?

  Students decide what they want to learn from a robotic mission to Mars.

  Subject Science

  Grades K-2

  Time Less than 30 mins

• 
  Melting Ice Experiment

  Students make predictions and observations about how ice will melt in different conditions then compare their predictions to results as they make connections to melting glaciers.

  Subject Science

  Grades 2-12

  Time 30-60 mins

• 
  Parachute Design

  Students design and test parachute landing systems to successfully land a probe on target.

  Subject Engineering

  Grades K-2

  Time 1-2 hrs

• 
  Planetary Poetry

  In this cross-curricular STEM and language arts lesson, students learn about planets, stars and space missions and write STEM-inspired poetry to share their knowledge of or inspiration about these topics.

  Subject Science

  Grades 2-12

  Time 1-2 hrs

• 
  Student Project: Write a Poem About Space

  Are you a space poet, and you didn't even know it? Find out how to create your own poems inspired by space!

  Subject Science

  Grades 2-12

  Time 30-60 mins

• 
  Ocean World: Earth Globe Toss Game

  Students use NASA images and a hands-on activity to compare the amounts of land and surface water on our planet.

  Subject Science

  Grades K-6

  Time Less than 30 mins

• 
  Simple Rocket Science Continued

  Students gather data on a balloon rocket launch, then create a simple graph to show the results of the tests.

  Subject Math

  Grades K-2

  Time 30-60 mins

• 
  Spaghetti Anyone? Building with Pasta

  Students use the engineering design process to build a structure to handle the greatest load and gain first-hand experience with compression and tension forces.

  Subject Engineering

  Grades K-8

  Time Less than 30 mins

• 
  Student Project: Building With Spaghetti

  Use spaghetti to build a tower modeled after the giant structures NASA uses to talk to spacecraft.

  Subject Engineering

  Grades K-8

  Time 30-60 mins

• 
  Simple Rocket Science

  Students perform a simple science experiment to learn how a rocket works and demonstrate Newton’s third law of motion.

  Subject Science

  Grades K-2

  Time 30-60 mins

Grades 3-5

• 
  Make a Paper Mars Helicopter

  In this lesson, students build a paper helicopter, then improve the design and compare and measure performance.

  Subject Engineering

  Grades 2-8

  Time 30-60 mins

• 
  Student Project: Make a Paper Mars Helicopter

  Build a paper helicopter, then see if you can improve the design like NASA engineers did when making the first helicopter for Mars.

  Subject Engineering

  Grades 2-8

  Time 30-60 mins

• 
  Soda-Straw Rockets

  Students study rocket stability as they design, construct and launch paper rockets using soda straws.

  Subject Engineering

  Grades 4-8

  Time Less than 30 mins

• 
  Student Project: Make a Straw Rocket

  Create a paper rocket that can be launched from a soda straw – then, modify the design to make the rocket fly farther!

  Subject Engineering

  Grades 4-8

  Time Less than 30 mins

• 
  Rocket Activity: Heavy Lifting

  Students construct balloon-powered rockets to launch the greatest payload possible to the classroom ceiling.

  Subject Engineering

  Grades 3-8

  Time 30-60 mins

• 
  Design a Robotic Insect

  Students design a robotic insect for an extraterrestrial environment, then compare the process to how NASA engineers design robots for extreme environments like Mars.

  Subject Science

  Grades 3-5

  Time 30-60 mins

• 
  Student Project: Design a Robotic Insect

  Design a robotic insect to go to an extreme environment. Then, compare the design process to what NASA engineers do when building robots for Mars!

  Subject Science

  Grades 3-5

  Time 30-60 mins

• 
  Mineral Mystery Experiment

  Students explore the science behind an intriguing planetary feature by creating saline solutions and then observing what happens when the solutions evaporate.

  Subject Science

  Grades 2-12

  Time 2 sessions of 30-60 mins

• 
  Student Project: Do a Mineral Mystery Experiment

  Dissolve salts in water, then observe what happens when the water evaporates.

  Subject Science

  Grades 2-12

  Time 2 sessions of 30-60 mins

• 
  How Far Away Is Space?

  Students use measurement skills to determine the scale distance to space on a map.

  Subject Math

  Grades 3-7

  Time 30-60 mins

• 
  Student Project: How Far Away Is Space?

  Stack coins and use your measurement skills to figure out the scale distance from Earth's surface to space.

  Subject Math

  Grades 3-7

  Time 30-60 mins

• 
  Melting Ice Experiment

  Students make predictions and observations about how ice will melt in different conditions then compare their predictions to results as they make connections to melting glaciers.

  Subject Science

  Grades 2-12

  Time 30-60 mins

• 
  Planetary Poetry

  In this cross-curricular STEM and language arts lesson, students learn about planets, stars and space missions and write STEM-inspired poetry to share their knowledge of or inspiration about these topics.

  Subject Science

  Grades 2-12

  Time 1-2 hrs

• 
  Student Project: Write a Poem About Space

  Are you a space poet, and you didn't even know it? Find out how to create your own poems inspired by space!

  Subject Science

  Grades 2-12

  Time 30-60 mins

• 
  Planetary Travel Time

  Students will compute the approximate travel time to planets in the solar system using different modes of transportation.

  Subject Math

  Grades 4-6

  Time 30-60 mins

• 
  The Ring Wing Glider

  In this simple engineering design lesson, students turn a piece of paper into an aircraft wing and then try to improve upon their design.

  Subject Engineering

  Grades 3-8

  Time 30-60 mins

• 
  Student Project: Make a Paper Glider

  Turn a piece of paper into a glider inspired by a NASA design.

  Subject Engineering

  Grades 3-8

  Time 30-60 mins

• 
  Ocean World: Earth Globe Toss Game

  Students use NASA images and a hands-on activity to compare the amounts of land and surface water on our planet.

  Subject Science

  Grades K-6

  Time Less than 30 mins

• 
  Spaghetti Anyone? Building with Pasta

  Students use the engineering design process to build a structure to handle the greatest load and gain first-hand experience with compression and tension forces.

  Subject Engineering

  Grades K-8

  Time Less than 30 mins

• 
  Student Project: Building With Spaghetti

  Use spaghetti to build a tower modeled after the giant structures NASA uses to talk to spacecraft.

  Subject Engineering

  Grades K-8

  Time 30-60 mins

Grades 6-8

• 
  Make a Paper Mars Helicopter

  In this lesson, students build a paper helicopter, then improve the design and compare and measure performance.

  Subject Engineering

  Grades 2-8

  Time 30-60 mins

• 
  Student Project: Make a Paper Mars Helicopter

  Build a paper helicopter, then see if you can improve the design like NASA engineers did when making the first helicopter for Mars.

  Subject Engineering

  Grades 2-8

  Time 30-60 mins

• 
  Soda-Straw Rockets

  Students study rocket stability as they design, construct and launch paper rockets using soda straws.

  Subject Engineering

  Grades 4-8

  Time Less than 30 mins

• 
  Student Project: Make a Straw Rocket

  Create a paper rocket that can be launched from a soda straw – then, modify the design to make the rocket fly farther!

  Subject Engineering

  Grades 4-8

  Time Less than 30 mins

• 
  Rocket Activity: Heavy Lifting

  Students construct balloon-powered rockets to launch the greatest payload possible to the classroom ceiling.

  Subject Engineering

  Grades 3-8

  Time 30-60 mins

• 
  Mineral Mystery Experiment

  Students explore the science behind an intriguing planetary feature by creating saline solutions and then observing what happens when the solutions evaporate.

  Subject Science

  Grades 2-12

  Time 2 sessions of 30-60 mins

• 
  Student Project: Do a Mineral Mystery Experiment

  Dissolve salts in water, then observe what happens when the water evaporates.

  Subject Science

  Grades 2-12

  Time 2 sessions of 30-60 mins

• 
  How Far Away Is Space?

  Students use measurement skills to determine the scale distance to space on a map.

  Subject Math

  Grades 3-7

  Time 30-60 mins

• 
  Student Project: How Far Away Is Space?

  Stack coins and use your measurement skills to figure out the scale distance from Earth's surface to space.

  Subject Math

  Grades 3-7

  Time 30-60 mins

• 
  Melting Ice Experiment

  Students make predictions and observations about how ice will melt in different conditions then compare their predictions to results as they make connections to melting glaciers.

  Subject Science

  Grades 2-12

  Time 30-60 mins

• 
  Planetary Poetry

  In this cross-curricular STEM and language arts lesson, students learn about planets, stars and space missions and write STEM-inspired poetry to share their knowledge of or inspiration about these topics.

  Subject Science

  Grades 2-12

  Time 1-2 hrs

• 
  Student Project: Write a Poem About Space

  Are you a space poet, and you didn't even know it? Find out how to create your own poems inspired by space!

  Subject Science

  Grades 2-12

  Time 30-60 mins

• 
  Planetary Travel Time

  Students will compute the approximate travel time to planets in the solar system using different modes of transportation.

  Subject Math

  Grades 4-6

  Time 30-60 mins

• 
  The Ring Wing Glider

  In this simple engineering design lesson, students turn a piece of paper into an aircraft wing and then try to improve upon their design.

  Subject Engineering

  Grades 3-8

  Time 30-60 mins

• 
  Student Project: Make a Paper Glider

  Turn a piece of paper into a glider inspired by a NASA design.

  Subject Engineering

  Grades 3-8

  Time 30-60 mins

• 
  Ocean World: Earth Globe Toss Game

  Students use NASA images and a hands-on activity to compare the amounts of land and surface water on our planet.

  Subject Science

  Grades K-6

  Time Less than 30 mins

• 
  Spaghetti Anyone? Building with Pasta

  Students use the engineering design process to build a structure to handle the greatest load and gain first-hand experience with compression and tension forces.

  Subject Engineering

  Grades K-8

  Time Less than 30 mins

• 
  Student Project: Building With Spaghetti

  Use spaghetti to build a tower modeled after the giant structures NASA uses to talk to spacecraft.

  Subject Engineering

  Grades K-8

  Time 30-60 mins

• 
  How Do We See Dark Matter?

  Students will make observations of two containers and identify differences in content, justify their claims and make comparisons to dark matter observations.

  Subject Science

  Grades 6-12

  Time Less than 30 mins

Grades 9-12

• 
  Mineral Mystery Experiment

  Students explore the science behind an intriguing planetary feature by creating saline solutions and then observing what happens when the solutions evaporate.

  Subject Science

  Grades 2-12

  Time 2 sessions of 30-60 mins

• 
  Student Project: Do a Mineral Mystery Experiment

  Dissolve salts in water, then observe what happens when the water evaporates.

  Subject Science

  Grades 2-12

  Time 2 sessions of 30-60 mins

• 
  Melting Ice Experiment

  Students make predictions and observations about how ice will melt in different conditions then compare their predictions to results as they make connections to melting glaciers.

  Subject Science

  Grades 2-12

  Time 30-60 mins

• 
  Planetary Poetry

  In this cross-curricular STEM and language arts lesson, students learn about planets, stars and space missions and write STEM-inspired poetry to share their knowledge of or inspiration about these topics.

  Subject Science

  Grades 2-12

  Time 1-2 hrs

• 
  Student Project: Write a Poem About Space

  Are you a space poet, and you didn't even know it? Find out how to create your own poems inspired by space!

  Subject Science

  Grades 2-12

  Time 30-60 mins

• 
  Let's Go to Mars! Calculating Launch Windows

  Students use advanced algebra concepts to determine the next opportunity to launch a spacecraft to Mars.

  Subject Math

  Grades 9-12

  Time 30-60 mins

• 
  How Do We See Dark Matter?

  Students will make observations of two containers and identify differences in content, justify their claims and make comparisons to dark matter observations.

  Subject Science

  Grades 6-12

  Time Less than 30 mins

Explore More

Find our full collection of more than 250 STEM educator guides and student activities in Teach and Learn.

For games, articles, and more activities from NASA for kids in upper-elementary grades, visit NASA Space Place and NASA Climate Kids.

Explore more educational resources and opportunities for students and educators from NASA STEM Engagement.

TAGS: Lessons, Teachers, Educators, Parents, Substitutes, Activities, Students, Science, Engineering, Quick and Easy

• 

  ABOUT THE AUTHOR

  Kim Orr, Web Producer, NASA-JPL Education Office

  Kim Orr is a web and content producer for the Education Office at NASA's Jet Propulsion Laboratory. Her pastimes are laughing and going on Indiana Jones style adventures.
  

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After six years investigating the effects of warming oceans on Greenland's ice sheet, the Oceans Melting Greenland, or OMG, mission has concluded. This airborne and seaborne mission studied how our oceans are warming and determined that ocean water is melting Greenland’s glaciers as much as warm air is melting them from above.

Read on to learn more about how OMG accomplished its goals and the implications of what we learned. Then, explore educational resources to engage students in the science of this eye-opening mission.

Why It's Important

Global sea level rise is one of the major environmental challenges of the 21st century. As oceans rise, water encroaches on land, affecting populations that live along shorelines. Around the world – including U.S. regions along the Gulf of Mexico and Eastern Seaboard and in Alaska – residents are feeling the impact of rising seas. Additionally, freshwater supplies are being threatened by encroaching saltwater from rising seas.

Sea level rise is mostly caused by melting land ice (primarily glaciers), which adds water to the ocean, as well as thermal expansion, the increase in volume that occurs when water heats up. Both ice melt and thermal expansion result from rising global average temperatures on land and in the sea – one facet of climate change.

This short video explains why Greenland's ice sheets are melting and what it means for our planet. Credit: NASA/JPL-Caltech | Watch more from the Earth Minute series

Greenland’s melting glaciers contribute more freshwater to sea level rise than any other source, which is why the OMG mission set out to better understand the mechanisms behind this melting.

How We Did It

The OMG mission used a variety of instruments onboard airplanes and ships to map the ocean floor, measure the behemoth Greenland glaciers, and track nearby water temperature patterns.

Join JPL scientist Josh Willis as he and the NASA Oceans Melting Greenland (OMG) team work to understand the role that ocean water plays in melting Greenland’s glaciers. Credit: NASA/JPL-Caltech | Watch on YouTube

Early on, the mission team created a map of the ocean floor, known as a bathymetric map, by combining multibeam sonar surveys taken from ships and gravity measurements taken from airplanes. Interactions among glaciers and warming seas are highly dependent on the geometry of the ocean floor. For example, continental shelf troughs carved by glaciers allow pathways for water to interact with glacial ice. So understanding Greenland's local bathymetry was crucial to OMG's mission.

To locate the edges of Greenland's glaciers and measure their heights, the mission used a radar instrument known as the Glacier and Ice Surface Topography Interferometer. Every spring during the six-year OMG mission, the radar was deployed on NASA’s Gulfstream III airplane that flew numerous paths over Greenland’s more than 220 glaciers. Data from the instrument allowed scientists to determine how the thickness and area of the glaciers are changing over time.

Finally, to measure ocean temperature and salinity patterns, scientists deployed numerous cylindrical probes. These probes dropped from an airplane and fell through the water, taking measurements from the surface all the way to the ocean floor. Each probe relayed its information back to computers onboard the plane where ocean temperatures and salinity were mapped. Then, scientists took this data back to their laboratories and analyzed it for trends, determining temperature variations and circulation patterns.

What We Discovered

Prior to the OMG mission, scientists knew that warming air melted glaciers from above, like an ice cube on a hot day. However, glaciers also flow toward the ocean and break off into icebergs in a process called calving. Scientists had the suspicion that warmer ocean waters were melting the glaciers from below, causing them to break off more icebergs and add to rising seas. It wasn’t until they acquired the data from OMG, that they discovered the grim truth: Glaciers are melting from above and below, and warming oceans are having a significant effect on glacial melt.

This narrated animation shows warm ocean water is melting glaciers from below, causing their edges to break off in a process called calving. Credit: NASA | Watch on YouTube

What this means for our Earth's climate is that as we continue burning fossil fuels and contributing to greenhouse gas accumulation, the oceans, which store more than 90% of the heat that is trapped by greenhouse gases, will continue to warm, causing glaciers to melt faster than ever. As warming ocean water moves against glaciers, it eats away at their base, causing the ice above to break off. In other words, calving rates increase and sea level rises even faster.

Our oceans control our climate and affect our everyday lives, whether or not we live near them. With the pace of the melt increasing, our shorelines and nearby communities will be in trouble sooner than previously expected. And it’s not just the beaches that will be affected. If Greenland’s glaciers all melt, global sea levels will rise by over 24 feet (7.4 meters), bringing dramatic change to the landscapes of major cities around the world.

› Read more about OMG’s findings and how scientists are continuing their research through ongoing initiatives and projects.

Teach It

Check out these resources to bring the real-life STEM behind the mission into your teaching. With lessons for educators and student projects, engage students in learning about the OMG mission and NASA climate science.

Educator Guides

• 
  Melting Ice Experiment

  Students make predictions and observations about how ice will melt in different conditions then compare their predictions to results as they make connections to melting glaciers.

  Subject Science

  Grades 2-12

  Time 30-60 mins

• 
  What's Causing Sea-Level Rise? Land Ice Vs. Sea Ice

  Students learn the difference between land ice and sea ice and make a model to see how the melting of each impacts global sea level.

  Subject Science

  Grades 2-8

  Time 30-60 mins

• 
  Lessons in Sea-Level Rise

  What is sea-level rise and how does it affect us? This "Teachable Moment" looks at the science behind sea-level rise and offers lessons and tools for teaching students about this important climate topic.

  Subject Science

  Grades 5-12

  Time 30-60 mins

• 
  Collection: Climate Change Lessons for Educators

  Explore a collection of standards-aligned STEM lessons for students that get them investigating climate change along with NASA.

Student Projects

• 
  How Melting Ice Causes Sea Level Rise

  Learn the difference between land ice and sea ice, then do an experiment to see how the melting of each contributes to global sea level rise.

  Subject Science

  Grades 2-8

  Time 30-60 mins

• 
  Collection: Climate Change Activities for Students

  Learn about climate change and its impacts with these projects, videos, and slideshows for students.

Articles

• 

  NASA Greenland Mission Completes Six Years of Mapping Unknown Terrain

  To learn how ocean water is melting glaciers, NASA’s Oceans Melting Greenland mission extensively surveyed the coastline of the world’s largest island.

Explore More

Websites

• NASA Climate Change
• NASA Earth Observatory
• NASA Climate Kids
• OMG Mission Website
• NASA Sea Level Change
• NASA Cambio Climático en Español

Facts & Figures

• NASA Climate Change: Evidence
• NASA Earth Science Missions

Videos

• Earth Minute Video Series
• Teaching Space - Monitoring Earth From Space

Interactives

• Earth Now

Image Gallery

• NASA climate images, videos, and graphics
• Images of Change

Articles

• Climate articles from NASA
• Ask NASA Climate
• NASA People - Josh Willis, Principal Investigator, Oceans Melting Greenland
• NASA People - Earth

Podcast

• On a Mission

TAGS: Teachable Moment, Climate, Earth Science, Glaciers, Greenland, Ice, Sea Level Rise, Teachers, Educators, Parents, Lessons, Missions, Earth, Climate TM

• 

  ABOUT THE AUTHOR

  Ota Lutz, K-12 Education Group Manager, NASA-JPL Education Office

  Ota Lutz is the manager of the K-12 Education Group at NASA’s Jet Propulsion Laboratory. When she’s not writing new lessons or teaching, she’s probably cooking something delicious, volunteering in the community, or dreaming about where she will travel next.

What unique challenges do you face engaging or addressing the needs of your students?

Many of the students I teach face challenges including poverty, homelessness, and learning English as a second language. This year, in particular, has been extremely difficult for all of us dealing with the pandemic and distance learning. As a teacher, I have had to find ways to make sure that my students are engaged in scientific inquiry and have access to resources and materials while learning remotely. This begins and ends with a conscious effort to acknowledge that kids are struggling with this online format and carving out time in every single class to provide the socio-emotional support they have come to expect from a classroom environment. Before we dive into content, this means making time for check-ins and updates. In any in-person classroom, we carve out time to get to know each other, and being online should not diminish that. Of course, as we all learned this year, easier said than done.

Social isolation is another factor that contributes to the challenges of distance learning. Even though students see their peers virtually, it is often difficult for them to open up and talk as freely as they would if they were in a physical classroom. So I have had to find ways to make sure that my students are comfortable with engaging in a virtual setting by allowing them opportunities to talk and collaborate with each other online.

Using breakout sessions was difficult at first, because the students were very self-conscious about speaking to each other on screen and were reluctant to share ideas. So every day, we spent the first few minutes in each class just talking to each other through text-based chat to get them socializing and feeling more comfortable with this new way of interacting. Now they are more comfortable engaging in scientific inquiry with each other and have meaningful discussions to expand their learning. It is not the same as having them physically perform labs together in class but things are definitely improving.

Another challenge has been providing all of my students with access to resources and materials that allow them to simulate a laboratory experience at home. I have been pleasantly surprised at the wealth of resources I have available to me as a teacher to provide virtual labs and activities to my students. Whether it is virtual demonstrations and simulations or scientific investigations that require simple materials that students can find around the house, we have been very resourceful so we can give students the best experience possible through distance learning. Promoting lab science with home supplies has been instrumental in student engagement, as they really get to explore in their own context, expressing themselves creatively with what they have at their disposal instead of being provided the materials.

How have you used lessons from NASA and JPL to keep students engaged while teaching in person and remotely?

I have always been fascinated by outer space and have loved sci-fi TV shows and movies since I was very young. So as a teacher, I was so excited to discover ways to use my love of astronomy to engage my students.

When I discovered NASA and JPL's resources and lessons, I went through them like a kid in a candy store. I found so many different activities that I could adapt to use in my own classroom. Over the past few years, I have used several JPL Education lessons and modified and extended them for my students.

For example, I took JPL's Touchdown lesson and allowed students to create their own planetary lander using materials they could find around their home. I challenged them to create a way to quantify how much impact the touchdown would have on the "astronauts" in their lander. Some students used balls of play dough as their astronauts, and quantified the impact by measuring the dents made in the play dough by paper clips that they had placed on the "seats" of their lander.

Another example was when I combined the Soda-Straw Rocket and Stomp Rockets lessons. I had my students create a straw-stomp rocket to investigate how changing the angle of the rocket launch could have an effect on the distance the rocket traveled.

My students also had the opportunity to participate in engineering activities with JPL and college students from Pasadena City College. The impact that this had on my students was profound and long-lasting. It was inspiring for my students to hear from NASA scientists and student role-models who encouraged them to pursue careers in science, engineering, and technology.

How have students reacted to these lessons?

The biggest payoff for me was seeing students envision themselves as NASA scientists. They learned to collaborate with each other, learn from each other, and challenge each other. They were able to experience every step of the engineering process firsthand. They were actively involved in designing, building, and testing their rockets and landers. They could also gather information from watching other students revise and improve their designs. Learning from each other was so much fun for them. As a teacher, watching my students strengthen their critical thinking, practical engineering, and problem-solving skills is one of the best parts of my job.

You switched from teaching middle school to teaching high school this year. How are you thinking about incorporating NASA resources into lessons for older students?

Growing up, I loved how the technology that I saw in the sci-fi shows I watched as a kid eventually made its way into our reality. I am always amazed at how NASA scientists push the boundaries of technology development and are only limited by the scope of their imagination.

As a high school biology teacher, I'm looking forward to having my students examine the ways that space technology is being used to help humans improve the health of the planet. Investigating climate change and the ecological impact humans have on the environment is so important. Looking at how NASA gathers data to better understand climate change is especially critical at this time because my students' generation is going to play a pivotal role in developing technologies for improving life on Earth. I'm looking forward to continuing to use JPL Education resources to help my students prepare for that challenge.

---

Looking for ways to bring NASA STEM into your classroom or already have a great idea? The Education Office at NASA's Jet Propulsion Laboratory serves educators in the greater Los Angeles area. Contact us at education@jpl.nasa.gov.

Explore More

• 
  Touchdown

  Students design and build a shock-absorbing system that will protect two "astronauts" when they land.

  Grades 3-8

  Time 30-60 mins

• 
  Soda-Straw Rockets

  Students study rocket stability as they design, construct and launch paper rockets using soda straws.

  Grades 4-8

  Time Less than 30 mins

• 
  Stomp Rockets

  In this video lesson, students learn to design, build and launch paper rockets, calculate how high they fly and improve their designs.

  Grades 4-9

  Time 1-2 hrs

• 
  Roving on the Moon

  Students build a rubber-band-powered rover that can scramble across the room.

  Grades 6-12

  Time 30-60 mins

• 
  Global Warming Demonstration

  This demonstration uses a water balloon to show how Earth's oceans are absorbing most of the heat being trapped on our warming world.

  Grades 1-12

  Time Less than 30 mins

TAGS: Teaching, Teachers, K-12, Middle School, High School, Remote Instruction, Classroom, Lessons, Educators, Workshops, Professional Development

• 

  ABOUT THE AUTHOR

  Brandon Rodriguez, Educator Professional Development Specialist, NASA-JPL Education Office

  Brandon Rodriguez is the educator professional development specialist at NASA’s Jet Propulsion Laboratory. Outside of promoting STEM education, he enjoys reading philosophy, travel and speaking to your dog like it's a person.

---

In the News

On Feb. 18, NASA's Perseverance Mars rover touched down on the Red Planet after a seven-month flight from Earth. Only the fifth rover to land on the planet, Perseverance represents a giant leap forward in our scientific and technological capabilities for exploring Mars and the possibility that life may have once existed on the Red Planet.

Here, you will:

• Meet the Perseverance Mars rover and find out what it's designed to do.
• Learn about an exciting opportunity to get your classroom, educational organization, or household involved with the Mission to Mars Student Challenge.

Why It's Important

You might be wondering, "Isn't there already a rover on Mars?” The answer is yes! The Curiosity rover landed on Mars in 2012 and has spent its time on the Red Planet making fascinating discoveries about the planet's geology and environment – setting the stage for Perseverance. So, why send another rover to Mars? The lessons we’ve learned from Curiosity coupled with advancements in technology over the last decade are allowing us to take the next big steps in our exploration of Mars, including looking for signs of ancient microbial life, collecting rock samples to bring to Earth one day, and setting the stage for a potential future human mission to the Red Planet.

More specifically, the Perseverance Mars rover has four science objectives:

• Identify past environments on Mars that could have supported microbial life
• Seek signs of ancient microbial life within the rocks and soil using a new suite of scientific instruments
• Collect rock samples of interest to be stored on the surface for possible return by future missions
• Pave the way for human exploration beyond the Moon

With these science objectives in mind, let's take a look at how the mission is designed to achieve these goals – from its science-rich landing site, Jezero Crater, to its suite of onboard tools and technology.

How It Works

Follow the Water

While present-day Mars is a cold, barren planet, science suggests that it was once very similar to Earth. The presence of clay, dried rivers and lakes, and minerals that formed in the presence of water provide extensive evidence that Mars once had flowing water at its surface. As a result, a mission looking for signs of ancient life, also known as biosignatures, should naturally follow that water. That’s because water represents the essential ingredient for life as we know it on Earth, and it can host a wide variety of organisms.

This is what makes Perseverance's landing site in Jezero Crater such a compelling location for scientific exploration. The crater was originally formed by an ancient meteorite impact about 3.8 billion years ago, and it sits within an even larger, older impact basin. The crater also appears to have once been home to an ancient lake fed by a river that formed the delta where Perseverance will begin its exploration, by exploring the foot of the river delta.

Tools of the Trade

Perseverance will begin its scientific exploration with the assistance of an array of tools, also known as science instruments.

Like its predecessor, Perseverance will have a number of cameras – 23, in fact! – serving as the eyes of the rover for scientists and engineers back on Earth. Nine of these cameras are dedicated to mobility, or tracking the rover's movements; six will capture images and videos as the rover travels through the Martian atmosphere down to the surface, a process known as entry, descent, and landing; and seven are part of the science instrumentation.

Navcam, located on the mast (or "head") of the rover, will capture images to help engineers control the rover. Meanwhile, Mastcam-Z, also on the rover’s mast, can zoom in, focus, and take 3D color pictures and video at high speed to allow detailed examination of distant objects. A third camera, Supercam, fires a small laser burst to excite compounds on the surface and determine their composition using spectroscopy. Supercam is also equipped with a microphone. This microphone (one of two on the rover) will allow scientists to hear the pop the laser makes upon hitting its target, which may give scientists additional information about the hardness of the rock.

Leaning more toward chemistry, the Planetary Instrument for X-Ray Lithochemistry (PIXL) will allow us to look at the composition of rocks and soil down to the size of a grain of salt. Elements respond to different types of light, such as X-rays, in predictable ways. So by shining an X-ray on Martian rocks and soil, we can identify elements that may be part of a biosignature.

Meanwhile, a device called SHERLOC will look for evidence of ancient life using a technique called Deep UV Raman spectroscopy. Raman spectroscopy can help scientists see the crystallinity and molecular structure of rocks and soil. For example, some molecules and crystals luminesce, or emit light, when exposed to ultraviolet – similar to how a blacklight might be used to illuminate evidence in a crime scene. Scientists have a good understanding of how chemicals considered key to life on Earth react to things like ultraviolet light. So, SHERLOC could help us identify those same chemicals on Mars. In other words, it can contribute to identifying those biosignatures we keep talking about.

Rounding out its role as a roving geologist on wheels, Perseverance also has instruments for studying beneath the surface of Mars. An instrument called the Radar Imager of Mars Subsurface Experiment (RIMFAX) will use ground-penetrating radar to analyze depths down to about 100 feet (30 meters) below the surface. Mounted on the rear of the rover, RIMFAX will help us understand geological features that can't be seen by the other cameras and instruments.

The rover's suite of instruments demonstrates how multiple scientific disciplines – chemistry, physics, biology, geology, and engineering – work in concert to further our understanding of Mars and help scientists uncover whether life ever existed on the Red Planet.

Next Generation Tech

At NASA, scientists and engineers are always looking to push the envelope and, while missions such as Perseverance are ambitious in themselves, they also provide an opportunity for NASA to test new technology that could be used for future missions. Two excellent examples of such technology joining Perseverance on Mars are MOXIE and the first ever Mars helicopter, Ingenuity.

MOXIE stands for the Mars Oxygen In-Situ Resource Utilization Experiment. Operating at 800 degrees Celsius, MOXIE takes in carbon dioxide (CO2) from the thin Martian atmosphere and splits those molecules into pure oxygen using what is called a catalyst. A catalyst is a chemical that allows for reactions to take place under conditions they normally wouldn’t. MOXIE provides an incredible opportunity for NASA to create something usable out of the limited resources available on Mars. Over the duration of the rover's mission, MOXIE will run for a total of one hour every time it operates, distributed over the course of the prime mission timeframe, to determine whether it can reliably produce breathable oxygen. The goal of operating this way is to allow scientists to determine the performance across a variety of environmental conditions that a dedicated, human-mission-sized oxygen plant would see during operations - day versus night, winter versus summer, etc. Oxygen is of great interest for future missions not just because of its necessity for future human life support on Mars, but also because it can be used as a rocket propellant, perhaps allowing for future small-scale sample return missions to Earth.

The Mars Ingenuity helicopter is likewise an engineering first. It is a technology demonstration to test powered flight on Mars. Because the Martian atmosphere is so thin, flight is incredibly difficult. So, the four-pound (1.8-kilogram), solar powered helicopter is specially designed with two, four-foot (1.2-meter) long counter-rotating blades that spin at 2,400 rotations per minute. In the months after Perseverance lands, Ingenuity will drop from the belly of the rover. If all goes well, it will attempt test flights of increasing difficulty, covering incrementally greater heights and distances for about 30 days. In the future, engineers hope flying robots can allow for a greater view of the surrounding terrain for robotic and human missions alike.

Teach It

The process of landing on Mars with such an advanced mission is no doubt an exciting opportunity to engage students across all aspects of STEM – and NASA wants to help teachers, educators and families bring students along for the adventure with the Mission to Mars Student Challenge. This challenge will lead students through designing and building a mission to Mars with a guided education plan and resources from NASA, listening to expert talks, and sharing student work with a worldwide audience. 

Learn more about the challenge and explore additional education resources related to the Perseverance Mars rover mission at https://go.nasa.gov/mars-challenge

Watch the Landing

The next chapter of Perseverance’s journey takes place on Feb. 18 at 12 p.m. PST (3 p.m. EST), when the mission reaches Mars after seven months of travelling through space. Join NASA as we countdown to landing with online events for teachers, students, and space enthusiasts! The landing day broadcast can be seen on NASA TV and the agency's website starting at 11:15 a.m. PST (2:15 p.m. EST). For a full listing of online events leading up to and on landing day, visit the mission's Watch Online page.

Follow landing updates on NASA's Twitter, Facebook and Instagram accounts.

Explore More

• 
  NASA's Mission to Mars Student Challenge

  Take part in a worldwide "teachable moment" and bring students along for the ride as NASA lands a rover on Mars February 18!

• 
  Teachable Moment 

  Meet Perseverance, NASA's Next Mars Rover

  Find out how the rover has been "souped up" with science instruments, cameras and technologies to explore Mars in new ways – plus, what to expect on launch day.

• 
  Mission to Mars Unit

  In this standards-aligned unit, students learn about Mars, design a mission to explore the planet, build and test model spacecraft and components, and engage in scientific exploration.

• 
  NASA #CountdownToMars STEM Toolkit

  Explore links to activities, lessons, interactives, social media, and more resources from NASA to participate in the Perseverance Mars rover mission.

• 
  Exploring Mars Lessons

  Get students engaged in the excitement of NASA's next mission to Mars with standards-aligned STEM lessons.

• 

  Meet JPL Interns of Mars 2020

  Read stories about interns helping prepare NASA's next Mars rover for its launch this summer.

• 
  Education Webinars

  Teaching Space With NASA

  Watch education webinars featuring NASA experts and education specialists and register to ask questions during live Q&As. Plus, explore related education resources.

• 
  Exploring Mars Activities

  Make a cardboard rover, design a Mars exploration video game, learn about Mars in a minute and explore more STEM activities for students.

• 
  Resources for Families

  Learning Space With NASA at Home

  Explore space and science activities students can do with NASA at home. Watch video tutorials for making rockets, Mars rovers, Moon landers and more. Plus, find tips for learning at home!

More Resources From NASA

Website: Perseverance Mars Rover

Website: NASA Mars Exploration

Website: Space Place - All About Mars

Video: Perseverance Mission Landing Trailer

Profiles: Meet the Martians

Simulation: Fly Along with Perseverance in Real-Time

Virtual Events: Watch Online – NASA Mars Exploration

Videos: Mars exploration videos from NASA

Images: Mars exploration images and graphics from NASA

Articles: Articles about Mars exploration from NASA

Share: Social Media

TAGS: Mars, Perseverance, Mars 2020, Science, Engineering, Robotics, Educators, Teachers, Students, Teachable Moments, Teach, Learn, Mars Landing

• 

  ABOUT THE AUTHOR

  Brandon Rodriguez, Educator Professional Development Specialist, NASA-JPL Education Office

  Brandon Rodriguez is the educator professional development specialist at NASA’s Jet Propulsion Laboratory. Outside of promoting STEM education, he enjoys reading philosophy, travel and speaking to your dog like it's a person.