A small piece of the ISS is visible in the top corner of this view looking down from space station over Earth. A large cloud of dust takes half the view over Earth's surface.

A data map overlaid on the globe shows thick swirls of dust traveling from West Africa, across the Atlantic Ocean and all the way to the Caribbean and Southern U.S.

Learn about the role that dust plays in Earth's climate, why scientists are interested in studying dust from space, and how to engage students in the science with STEM resources from JPL.


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.

Sharp mountain peaks are covered in splotches of snow with a fine coating of dust visible on top of the snow.

A coating of dust on snow speeds the pace of snowmelt in the spring. Credit: NASA | + Expand image

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.

A plume of dust eminates from over the Copper River in Alaska, spreading out as this series of overhead satellite images progresses.

A plume of dust is shown emanating from over Alaska's Copper River in October 2016 in these images captured by the Moderate Resolution Imaging Spectroradiometer, or MODIS, instrument on NASA’s Terra and Aqua satellites. Dust storms play a key role in fueling phytoplankton blooms by delivering iron to the Gulf of Alaska. Credit: NASA | › Full image and caption

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.

An overhead view of a swirl of clouds mixed with a streak of dust like a swirl of milk froth in a cappuccino

A swirl of dust mixes with the clouds in a low-pressure storm over the Gobi desert between Mongolia and China. This image was captured by the MODIS instrument on the Terra satellite in May 2019. Credit: NASA | › Full image and caption

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?
A picture of the EMIT instrument, shaped like a small megaphone, is overlaid on an picture of the International Space Station flying above Earth.

The EMIT instrument will fly aboard the International Space Station, which orbits Earth about once every 90 minutes, completing about 16 orbits per day. Credit: NASA | + Expand image

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.

Bands of satellite images looking at a seciton of Earth are highlighted in different colors to reveal different concentrations of minerals.

This example spectra shows how scientists will be able to identify different concentrations of minerals and elements in data collected by EMIT. Credit: NASA/JPL-Caltech | + Expand image

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

Student Activities

Articles

Websites

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

  • Brandon Rodriguez
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Collage of photos featured in this story.

We went behind the scenes with three interns on NASA’s Earth System Observatory team to learn how they're devoting their future careers to putting our planet first.


Leave it to the interns at NASA's Jet Propulsion Laboratory to school the full-timers. Case in point: JPL intern Joalda Morancy knows exactly how to explain—in bite-sized, plain English—NASA’s latest multi-missioned initiative to study our home planet.

“The Earth System Observatory aims to tackle one of the biggest issues we’re facing today—climate change,” they say of NASA's ESO. “We need to have multiple missions that look at the Earth system as a whole in order to tackle the issue of climate change in the next couple of decades.”

The observatory will be made up of an array of satellites, instruments, and missions to form a well-rounded collection of observations meant to offer crucial and precise measurements of our environment. As NASA puts it: “Taken together, as a single observatory, we will have a holistic, 3-dimensional understanding of our Earth’s systems—how they work together, how one change can influence another.”

While the ESO is in its early stages, it’s a crucial time for interns to be involved, as their generation will most likely face the most pressing challenges resulting from climate change. We spoke to three JPL interns getting first-hand experience with the observatory's missions and projects to learn why, to them, Earth is the most important planet to study right now.

Joalda Morancy

Joalda Morancy smiles in a close-up photo.

Image courtesy: Joalda Morancy | + Expand image

Morancy first became fascinated by space exploration in high school thanks to a YouTube video on how to make a peanut butter and honey sandwich in space.

“I love telling that story,” Morancy says with a laugh. “It was so random, and I was so intrigued. I watched the entire video and thought, ‘This is amazing.’ I did a lot more research about what NASA does and that was my gateway to space.”

Flash forward a few years to college at the University of Chicago, where Morancy discovered there was one planet in particular that really captured their attention: Earth.

“I was initially interested in space exploration, and while [majoring in] astrophysics, I took a class on what makes a planet habitable,” they recall. “It taught me everything about basic Earth sciences and how that ties into Earth and the big picture of how a habitable environment operates.”

Morancy found it so interesting and—combined with their growing alarm about climate change—wanted a hand in studying how to preserve our planet. So Morancy took more classes in geophysics and geophysical sciences, including courses on atmosphere, glaciology, and physical geology.

“I wanted to give myself the foundational knowledge,” Morancy says. “And right after that, I started at JPL.”

They had originally searched JPL’s careers site for internships with the Perseverance Mars rover mission but noticed an opening with the Earth Science team.

“I didn’t know JPL did Earth science; I thought it was mostly Mars and robotic exploration,” they say. “When I saw that opening, I knew it was the perfect opportunity for me to learn more about Earth.”

For the past year-and-a-half, Morancy has worked on ECOSTRESS, an ESO-related experiment aboard the International Space Station designed to measure water stress among plants. Now, they are interning with the ESO successor to ECOSTRESS, the Surface Biology and Geology, or SBG, mission.

A heatmap showing land surface temperatures in California as measured by the ECOSTRESS mission.

A graphic developed by Morancy during their internship with the ECOSTRESS mission shows the land surface temperatures at different locations throughout California. Image credit: NASA/JPL-Caltech | › Full image and caption

“I help with a lot of project management since SBG is in its early stages,” they say. “A lot of things are starting to cook up, and a lot of engineers and scientists are being onboarded to the team. I’m working with the team to help onboard, and I’m also helping with the science instruments for SBG.”

The magnitude of being part of SBG and the observatory team in their early stages is not lost on Morancy.

“I really believe it will have a long-lasting impact on how we look at climate change and how we target those specific issues to fix,” they say. “It'll be a major driver for future researchers and scientists.”

While Morancy hopes to combine Earth sciences and space exploration for their future career, they’re invested in studying our blue planet for the long run.

“I think Earth science is incredibly important because this is our only home,” they say. “Even though people are looking to settle on Mars and other celestial bodies ... I think it’s important to take care of this rock we’ve been given to live on. It’s crucial to make sure we take care of it for future generations.”

Rebecca Gustine

Rebecca Gustine smiles for a photo atop an elephant.

Image courtesy: Rebecca Gustine | + Expand image

When Rebecca Gustine studied abroad in Thailand during her junior year of college, she didn’t realize it would alter the course of her studies and her future career path.

“I had a lightbulb moment realizing how human development and access to water go hand in hand,” she says.

Gustine went on to Washington State University, where she is now a Ph.D. student studying civil engineering with a focus on water resources engineering.

“A lot of my undergraduate research had to do with water,” she explains. “It was from a global health perspective and had to do with access to clean water, hygiene, and gender dynamics in developing countries. I also really like math and physics, so combining global health with water resources engineering was very interesting.”

Gustine was so fascinated by water research, she knew she wanted to find an internship that would let her focus on just that. When she saw an open call for internships at JPL, she submitted her resume and was contacted by Gregory Halverson and Christine Lee, JPL scientists focused on using remote sensing measurements to study water quality, water resources, and ecosystems management.

Gustine started at JPL as an intern in August 2020, supporting the Earth science team by looking at how ECOSTRESS data could be used to preserve habitats in the California Bay Delta system, where the Sacramento and the San Joaquin Rivers meet. For the past year, she has focused on processing remote-sensing data and engaging with stakeholders. She was even first-author on a peer-reviewed paper.

“My work is basically using pictures [taken] from the sky that tell us information about the Earth and then making decisions about how to manage water resources and protect critical habitats,” she says.

Gustine is also well aware that her research comes at a pivotal time in the global conversation around Earth’s future.

“Given that climate change is having a profound impact on human and natural systems, we have to understand those changes and protect critical habitats and resources for the well-being of humans everywhere,” she says. “Changes in one component of a system can have cascading consequences for other parts of the system.”

While she works alongside others exploring the mysteries of worlds beyond Earth, Gustine is particularly proud to be part of pioneering research that could alter the future of our planet.

“Observing Earth is still space exploration, just from a different vantage point,” she says. “Given that NASA is the major proprietor of space, to look back at Earth using the same technology we use to go farther into space is important.”

Jonathan Vellanoweth

Jonathan Vellanoweth stands in a grassy field holding a phone in one hand and with a grasshopper balancing on his other hand.

Image courtesy: Jonathan Vellanoweth | + Expand image

What will be the future, long-term impacts of power plants on our environment? Jonathan Vellanoweth is spending his time as a JPL intern working with a team to try to help answer that very question.

Vellanoweth is a student at Cal State University, Los Angeles, where he’s earning his master’s degree in environmental science with an emphasis in geospatial science. In his internship with the Surface Biology and Geology team at JPL, he's using data and satellite imagery from ECOSTRESS and the Landsat mission to detect thermal plumes emitted by power plants.

Vellanoweth’s work currently focuses on the Diablo Canyon Power Plant in San Luis Obispo, California.

“We’re looking at power plants that intake coastal waters to cool their reactors, then discharge it at a higher temperature back into the same water body,” he explains. “I’m using satellite imagery to detect that thermal change and outline the area of what is classified as a plume, or anywhere thermal discharge is heating up the ocean or the coast. We can see where this plume is moving over the year or several seasons, and other studies can use this data to see what the actual effects are on coastal communities.”

Vellanoweth has been fascinated by Earth science since as early as 7th grade, when he took his first environmental science class where he learned all about the scientific method and later went out into nature to collect soil samples and study them.

As a JPL intern, Vellanoweth has been particularly grateful for the variety of knowledge his colleagues provide him.

“The amount of support that you have from all these great scientists that work here is really what attracted me,” he says. “You can intern for a lot of places, but at JPL, you have all these colleagues you can meet with who have a lot of feedback they can give you. There are people on your team studying similar and dissimilar things as you, so they can provide you with something you might not have thought about and help expand your research.”

Most importantly, Vellanoweth is looking forward to the information everyone will have access to in the future thanks to the efforts of all the missions and projects within the Earth Science Observatory.

“I’m excited about getting things out there and making them accessible to the public. I’m really big on that because there are a lot of people who want to do this kind of research, but a lot of times, it can be hard to find the data or algorithm you need, and it’s a lot of trial and error,” he says. “SBG and ESO bring all of these things together and make it available for everyone.”


The laboratory’s STEM internship and fellowship programs are managed by the JPL Education Office. Extending the NASA Office of STEM Engagement’s reach, JPL Education seeks to create the next generation of scientists, engineers, technologists and space explorers by supporting educators and bringing the excitement of NASA missions and science to learners of all ages.

Career opportunities in STEM and beyond can be found online at jpl.jobs. Learn more about careers and life at JPL on LinkedIn and by following @nasajplcareers on Instagram.

TAGS: Interns, Colleges, Universities, Students, Higher Education, Internships, Student Programs, Year-Round Internship Program, Summer Internship Program, Earth Science, Earth, Climate Change, Earth System Observatory

  • Celeste Hoang
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Just beyond the wing of a plane, the edge of a tall glacier is visible through the plane's window. At the bottom of the glacier, bits of ice surround an elliptical pool of brown water at the glacier's edge.

Explore how the OMG mission discovered more about what's behind one of the largest contributors to global sea level rise. Plus, learn what it means for communities around the world and how to get students engaged.


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

An animation shows a ship passing over the ocean directly in front of a glacier and scanning the sea floor followed by a plane flying overhead and scanning the air.

This animation shows how the OMG mission created a map of the ocean floor, known as a bathymetric map, to determine the geometry around Greenland's glaciers. Image credit: NASA/JPL-Caltech | + Expand image

An animation shows a plan flying over a glacier and scanning the ground below followed by a plane flying over the ocean shelf next to the glacier and dropping probes into the water.

This animation shows how the OMG mission used radar to measure changes in the thickness and retreat of Greenland's glaciers as well as probes to measure ocean temperature and salinity. Credit: NASA/JPL-Caltech | + Expand image

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

Student Projects

Articles

Explore More

Websites

Facts & Figures

Videos

Interactives

Image Gallery

Articles

Podcast

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

  • Ota Lutz
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Photo collage of interns who participated in JPL's HBCU/URM initiative in 2021

Five years in, a JPL initiative forging relationships with students and faculty at historically Black colleges and universities continues expanding its reach, hosting 48 interns this year.


Brandon Ethridge, a flight systems engineer at NASA’s Jet Propulsion Laboratory in Southern California, has had a year to remember. The 24-year-old got engaged, became a father, and is celebrating the one-year anniversary of starting full time at JPL – his self-described dream job.

“Definitely the most eventful year of my life,” Ethridge said.

Brandon Ethridge stands in front of a mural made to look like a blueprint on the Mechanical Design Building at JPL.

Brandon Ethridge poses in front of the Mechanical Design Center at JPL during his internship in 2019. Image credit: NASA/JPL-Caltech/Kim Orr | + Expand image

While he’s been gaining experience testing systems used to build spacecraft, Ethridge has spent minimal time at the Laboratory due to the pandemic. But the North Carolina native already had plenty of first-hand knowledge of JPL thanks to his summer 2019 internship – an opportunity that presented itself at a JPL informational session that spring at his alma mater, North Carolina A&T State University.

“That allowed me the chance to speak one-on-one with Jenny Tieu and Roslyn Soto [JPL Education project managers],” Ethridge said. “They were incredibly generous with their time and provided resume critiques, feedback, and general advice about how to get an opportunity at JPL.”

Since 2017, Tieu has been leading JPL’s Historically Black Colleges and Universities/Underrepresented Minorities, or HBCU/URM, initiative – an effort to increase and foster a more diverse workforce in technical roles at the Laboratory. It’s one of many programs facilitating the more than 550 internship opportunities offered through the Education Office this year.

Now in its fifth year, the program has seen rapid growth; from seven interns in its first year, to 24 interns in 2020. This year, JPL is welcoming 48 students interning remotely from institutions including Howard, North Carolina A&T, Tuskegee, and Prairie View A&M universities, along with underrepresented-minority students from universities including UCLA, USC, UC Riverside, Duke, Cal Poly Pomona, and more.

The initiative includes funding and support to bring in faculty from the schools to take part in research with the students, building in a cohort model that facilitates sustainable interactions with JPL.

“We’re intentional about addressing the culture shock that some of these students may experience,” Tieu said. “With the cohort model, the faculty members can provide guidance to the students while they are navigating new relationships, connections, and a new city.”

Additionally, interns are invited to participate in roundtable conversations in groups where they can share concerns and openly discuss their experiences at JPL. Tieu has also set up virtual meet-ups where students can get to know employees from outside their groups and hear talks from members of JPL’s Black Excellence Strategic Team and past HBCU alumni.

For Ethridge, being in a position to give back to the program was something he prioritized.

“I wanted to repay some of the many kindnesses that were afforded to me,” Ethridge said. “I also feel that I am in a unique position because I just recently went through the process.”

For Howard University junior Kyndall Jones, the draw to JPL came following a fellow student’s acceptance into the program.

Kyndall Jones sits in the cockpit of a plane and looks back at the camera while making the peace sign with her left hand.

Kyndall Jones at the NASA Armstrong Flight Research Center. Image courtesy: Kyndall Jones | + Expand image

“I was so amazed that he had an internship with NASA, and it really sparked my interest,” Jones said. “After doing my research on the program, I submitted my resume and heard back after a few months, landed an interview, and now here I am [virtually]!”

Despite the telework nature of this summer’s internship, Jones said that even from her home in Dayton, Ohio, she has been able to foster connections with JPL employees and gain valuable experience in her role working on software for an Earth-science instrument that will help NASA understand how different types of air pollution, which can cause serious health problems, affect human health.

And thanks to her mentor, Operations Systems Engineer Janelle Wellons, Jones was able to get the type of hands-on NASA experience that’s been hard to come by since the pandemic.

“My mentor Janelle suggested that I come visit Los Angeles for a few days this summer, and I was finally able to visit and explore the city for the first time,” Jones said. “I am also super grateful for her setting up a tour at the NASA Armstrong Flight Research Center where we were able to view, tour, and learn lots of interesting facts about NASA’s historical aircraft.”

Wellons – who splits her time operating instruments aboard several Earth-observing missions – had been involved in previous years’ roundtable discussions with HBCU interns, but this year, she had the opportunity to hire her own interns through the program. Being from the East Coast herself, Wellons remembers having little awareness of JPL as a potential career landing spot while studying at Massachusetts Institute of Technology.

“Getting visibility and actually partnering with these schools to make these internships happen is so important,” Wellons said. “Actively interacting with HBCUs is only going to do good for people we would otherwise potentially never get an application from, and it benefits JPL by broadening the talent pool and diversity of our workforce.”

As for the future, Jones sees the initiative as one step of many for her and fellow interns toward careers in engineering and science.

“I know a lot of Howard students that are interning or have interned with JPL, and the love from our College of Engineering and Architecture is especially high,” Jones said. “The info sessions, resume workshops, and networking workshops that JPL has been able to put on have been great, and the more they can do, the better for students.”

Tieu agrees, adding, "We are happy to see the growth of the initiative but look forward to making further progress. There's so much more we would like to accomplish in the years ahead."

To learn more about the HBCU/URM initiative and apply, see the Maximizing Student Potential in STEM program page. The HBCU/URM initiative resides within this program.

This Q&A is part of an ongoing series highlighting the stories and experiences of students and faculty who came to JPL as part of the laboratory's collaboration with historically black colleges and universities, or HBCUs. › Read more from the series

Explore More

The laboratory’s STEM internship and fellowship programs are managed by the JPL Education Office. Extending the NASA Office of STEM Engagement’s reach, JPL Education seeks to create the next generation of scientists, engineers, technologists and space explorers by supporting educators and bringing the excitement of NASA missions and science to learners of all ages.

Career opportunities in STEM and beyond can be found online at jpl.jobs. Learn more about careers and life at JPL on LinkedIn and by following @nasajplcareers on Instagram.

TAGS: HBCU, Internships, College Students, Faculty, Research, Careers, Earth Science, Black History Month, Engineering, Intern, Higher Education

  • Taylor Hill
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Collage of images and graphics representing the science goals of the Sentinel-6 Michael Freilich mission

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


In the News

A new spacecraft that will collect vital sea-surface measurements for better understanding climate change and improving weather predictions is joining the fleet of Earth science satellites monitoring our changing planet from space. A U.S.-European partnership, the Sentinel-6 Michael Freilich satellite continues a long tradition of collecting scientific data from Earth orbit. It’s named in honor of NASA’s former Earth Science Division director and a leading advocate for ocean measurements from space.

Read on to find out how the mission will measure sea-surface height for the next 10 years and provide atmospheric data to help better predict weather. Plus, find out how to watch the launch online and explore related teaching resources to bring NASA Earth science into the classroom and incorporate sea level data into your instruction.

How It Works

The Sentinel-6 Michael Freilich satellite is designed to measure sea-surface height and improve weather predictions. Once in orbit, it will be able to measure sea-surface height – with accuracy down to the centimeter – over 90% of the world’s oceans every 10 days. It will do this using a suite of onboard science tools, or instruments.

To measure sea-surface height, a radar altimeter will send a pulse of microwave energy to the ocean’s surface and record how long it takes for the energy to return. The time it takes for the signal to return varies depending on the height of the ocean – a higher ocean surface results in a shorter return time, while a lower ocean surface results in a longer return time. A microwave radiometer will measure delays that take place as the signal travels through the atmosphere to correct for this effect and provide an even more precise measurement of sea-surface height.

A blue beam extends from the spacecraft down toward Earth as a red dot pulses back and forth between the spacecraft and the surface of the planet.

This animation shows the radar pulse from the Sentinel-6 Michael Freilich satellite's altimeter bouncing off the sea surface in order to measure the height of the ocean. Image credit: NASA/JPL-Caltech | + Expand image

To measure atmospheric data, Sentinel-6 Michael Freilich is equipped with the Global Navigation Satellite System - Radio Occultation, or GNSS-RO, instrument, which will measure signals from GPS satellites – the same ones you use to navigate on Earth. As these satellites move below or rise above the horizon from Sentinel-6 Michael Freilich's perspective, their signals slow down, change frequency and bend as a result of the phenomenon known as refraction. Scientists can use these changes in the GPS signal to measure small shifts in temperature, moisture content, and density in the atmosphere. These measurements can help meteorologists improve weather forecasts.

Why It's Important

Scientists from around the world have been collecting sea level measurements for more than a century. The data – gathered from tide gauges, sediment cores, and space satellites – paint a clear picture: sea level is rising. Looking at the average height of the sea across the planet, we see that in the last 25 years global sea level has been rising an average of 0.13 inches (3.3 mm) per year. This average is increasing each year (in the 2000s, it was 0.12 inches, or 3.0 mm, per year) as is the rate at which it’s increasing. That means that sea level is rising, and it’s rising faster and faster. Since 1880, global sea level has risen more than eight inches (20 cm). By 2100, it is projected to rise another one to four feet (30 to 122 cm).

This satellite data show the change in Earth's global sea level since 1993. Roll over the chart to see the various data points. For more Earth vital signs, visit NASA's Global Climate Change website

Measuring sea level from space provides scientists with global measurements of Earth’s oceans in a matter of days, including areas far from shore where measurements aren’t practical or possible. Starting in 1992 with the launch of the TOPEX/Poseidon mission, the record of sea level measurements from space has continued uninterrupted, providing an increasingly detailed picture of Earth’s rising seas. The Sentinel-6 Michael Freilich satellite – and its twin, which will launch in 2025 – will extend those measurements to 2030, allowing scientists to continue collecting vital information about Earth’s changing oceans and climate.

Unlike previous satellites that measured sea level, Sentinel-6 Michael Freilich has the capability to measure sea level variations more accurately near coastlines, giving scientists insight into changes that can have direct impacts on communities and livelihoods, such as commercial fishing and ship navigation.

This playlist for students and teachers features explainers about the causes and effects of sea level rise and how NASA is studying our changing planet – plus related STEM activities and experiments for students. | Watch on YouTube

With rising seas already impacting people and communities, it's important to understand not just how much seas are rising, but also where and how quickly they are rising. Data from instruments on Sentinel-6 Michael Freilich can be combined with data from other satellites to get a clearer picture of what's contributing to sea level rise and where. For example, by looking at the satellite's radar altimeter measurements along with gravity measurements from the GRACE-FO mission, scientists can better determine how melting ice and thermal expansion are contributing to sea level rise. And by tracking the movement of warm water (which stands taller than cold water), scientists can better predict the rapid expansion of hurricanes.

Watch the Launch

Scheduled to launch at 9:17 a.m. PST (12:17 p.m. EST) on November 21, Sentinel-6 Michael Freilich will launch atop a SpaceX Falcon 9 rocket from Vandenberg Air Force Base in California.

Watch a live broadcast of the launch from the Vandenberg Air Force Base on NASA TV and the agency’s website. Visit the Sentinel-6 Michael Freilich website to explore more news about the mission. Follow launch updates on NASA's Twitter, Facebook and Instagram accounts.

Teach It

Make classroom connections to NASA Earth science with lessons about rising seas, thermal expansion and ice melt, data collection and graphing, and engineering. Plus explore independent activities and experiments students can do at home, video playlists, and more:

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Recursos en Español

TAGS: Teachable Moments, Educators, Teachers, Parents, K-12 Education, Launch, Mission, Earth, Satellite, Earth Science, Climate Change, Sentinel-6 Michael Freilich, Sea Level, Sea Level Rise, Climate TM

  • Lyle Tavernier
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Satellite Image of smoke above the Western U.S.

Data overlayed on a satellite image of the United States shows a thick cloud of aerosols over the western US

Animated satellite image of Earth

Update: Sept. 14, 2020 – This feature, originally published on Aug. 23, 2016, has been updated to include information on the 2020 fires and current fire research.


In the News

Once again, it’s fire season in the western United States with many citizens finding themselves shrouded in wildfire smoke. Late summer in the West brings heat, low humidity, and wind – optimal conditions for fire. These critical conditions have resulted in the August Complex Fire, the largest fire in California's recorded history. Burning concurrently in California are numerous other wildfires, including the SCU Lightning Complex fire, the third-largest in California history.

Fueled by high temperatures, low humidity, high winds, and years of vegetation-drying drought, more than 7,700 fires have engulfed over 3 million acres across California already this year. And the traditional fire season – the time of year when fires are more likely to start, spread, and consume resources – has only just begun.

Because of their prevalence and effects on a wide population, wildfires will remain a seasonal teachable moment for decades to come. Keep reading to find out how NASA studies wildfires and their effects on climate and communities. Plus, explore lessons to help students learn more about fires and their impacts.

How It Works

With wildfires starting earlier in the year and continuing to ignite throughout all seasons, fire season is now a year-round affair not just in California, but also around the world. In fact, the U.S. Forest Service found that fire seasons have grown longer in 25 percent of Earth's vegetation-covered areas.

Animation of the FireSat network of satellites capturing wildfires on Earth

This animation shows how FireSat would use a network of satellites around the Earth to detect fires faster than ever before. | + Expand image

For NASA's Jet Propulsion Laboratory, which is located in Southern California, the fires cropping up near and far are a constant reminder that its efforts to study wildfires around the world from space, the air, and on the ground are as important as ever.

JPL uses a suite of Earth satellites and airborne instruments to help better understand fires and aide in fire management and mitigation. By looking at multiple images and types of data from these instruments, scientists compare what a region looked like before, during, and after a fire, as well as how long the area takes to recover.

While the fire is burning, scientists watch its behavior from an aerial perspective to get a big-picture view of the fire itself and the air pollution it is generating in the form of smoke filled with carbon monoxide and carbon dioxide.

Natasha Stavros, a wildfire expert at JPL, joined Zach Tane with the U.S. Forest Service during a Facebook Live event to discuss some of these technologies and how they're used to understand wildfire behavior and improve wildfire recovery.

Additionally, JPL worked with a startup in San Francisco called Quadra Pi R2E to develop FireSat, a global network of satellites designed to detect wildfires and alert firefighting crews faster. 

Using these technologies, NASA scientists are gaining a broader understanding of fires and their impacts.

Why It's Important

One of the ways we often hear wildfires classified is by how much area they have burned. Though this is certainly of some importance, of greater significance to fire scientists is the severity of the fire. Wildfires are classified as burning at different levels of severity: low, medium, and high. Severity is a function of intensity, or how hot the fire was, and its spread rate, or the speed at which it travels. A high-severity fire is going to do some real damage. (Severity is measured by the damage left after the fire, but can be estimated during a fire event by calculating spread rate and measuring flame height which indicates intensity.)

Google Earth image showing fire severity
This image, created using data imported into Google Earth, shows the severity of the 2014 King Fire. Green areas are unchanged by the fire; yellow equals low severity; orange equals moderate severity; and red equals high severity. A KMZ file with this data is available in the Fired Up Over Math lesson linked below. Credit: NASA/JPL-Caltech/E. Natasha Stavros.

The impacts of wildfires range from the immediate and tangible to the delayed and less obvious. The potential for loss of life, property, and natural areas is one of the first threats that wildfires pose. From a financial standpoint, fires can lead to a downturn in local economies due to loss of tourism and business, high costs related to infrastructure restoration, and impacts to federal and state budgets.

The release of greenhouse gases like carbon dioxide and carbon monoxide is also an important consideration when thinking about the impacts of wildfires. Using NASA satellite data, researchers at the University of California, Berkeley, determined that between 2001 and 2010, California wildfires emitted about 46 million tons of carbon, around five to seven percent of all carbon emitted by the state during that time period.

Animation showing Carbon Dioxide levels rising from the Station Fire in Southern California.
This animation from NASA's Eyes on the Earth visualization program shows carbon monoxide rising (red is the highest concentration) around Southern California as the Station Fire engulfed the area near JPL in 2009. Image credit: NASA/JPL-Caltech

In California and the western United States, longer fire seasons are linked to changes in spring rains, vapor pressure, and snowmelt – all of which have been connected to climate change. Wildfires serve as a climate feedback loop, meaning certain effects of wildfires – the release of CO2 and CO – contribute to climate change, thereby enhancing the factors that contribute to longer and stronger fire seasons.

While this may seem like a grim outlook, it’s worth noting that California forests still act as carbon sinks – natural environments that are capable of absorbing carbon dioxide from the atmosphere. In certain parts of the state, each hectare of redwood forest is able to store the annual greenhouse gas output of 500 Americans.

Studying and managing wildfires is important for maintaining resources, protecting people, properties, and ecosystems, and reducing air pollution, which is why JPL, NASA, and other agencies are continuing their study of these threats and developing technologies to better understand them.

Teach It

Have your students try their hands at solving some of the same fire-science problems that NASA scientists do with these two lessons that get students in grades 3 through 12 using NASA data, algebra, and geometry to approximate burn areas, fire-spread rate and fire intensity:

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Lyle Tavernier contributed to this feature.

TAGS: teachable moments, wildfires, science, Earth Science, Earth, Climate Change, Climate TM

  • Ota Lutz
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Collage of intern photos that appear in this article

Most years, summertime at NASA's Jet Propulsion Laboratory arrives with an influx of more than 800 interns, raring to play a hands-on role in exploring Earth and space with robotic spacecraft.

Perhaps as exciting as adding NASA to their resumes and working alongside the scientists and engineers they have long admired is the chance to explore the laboratory's smorgasbord of science labs, spacecraft assembly facilities, space simulators, the historic mission control center and a place called the Mars Yard, where engineers test drive Mars rovers.

But this year, as the summer internship season approached with most of JPL's more than 6,000 employees still on mandatory telework, the laboratory – and the students who were offered internships at the Southern California center – had a decision to make.

"We asked the students and the mentors [the employees bringing them in] whether their projects could still be achieved remotely and provide the educational component we consider to be so crucial to these experiences," said Adrian Ponce, deputy section manager of JPL's Education Office, which runs the laboratory's STEM internship programs.

The answer was a resounding yes, which meant the laboratory had just a matter of weeks to create virtual alternatives for every aspect of the internship experience, from accessing specialized software for studying Earth and planetary science to testing and fine-tuning the movements of spacecraft in development and preparing others for launch to attending enrichment activities like science talks and team building events.

“We were able to transition almost all of the interns to aspects of their projects that are telework-compatible. Others agreed to a future start date,” said Ponce, adding that just 2% of the students offered internships declined to proceed or had their projects canceled.

Now, JPL's 600-plus summer interns – some who were part-way through internships when the stay-at-home orders went into effect, others who are returning and many who are first-timers – are getting an extended lesson in the against-the-odds attitude on which the laboratory prides itself.

We wanted to hear about their experiences as JPL's first class of remote interns. What are their routines and home offices like in cities across the country? How have their teams adapted to building spacecraft and doing science remotely? Read a collection of their responses below to learn how JPL interns are finding ways to persevere, whether it's using their engineering skills to fashion homemade desks, getting accustomed to testing spacecraft from 2,000 miles away or working alongside siblings, kids, and pets.


In the image on the left, Jennifer Brag stands in front of a series of observatories. In the image on the right, her bird is pirched on top of open laptop.

Courtesy of Jennifer Bragg | + Expand image

"I am working with an astronomer on the NEOWISE project, which is an automated system that detects near-Earth objects, such as asteroids. The goal of my project is to identify any objects missed by the automated system and use modeling to learn more about their characteristics. My average day consists of writing scripts in Python to manipulate the NEOWISE data and visually vet that the objects in the images are asteroids and not noise or stars.

My office setup consists of a table with scattered books, papers, and pencils, a laptop, television, a child in the background asking a million questions while I work, and a bird on my shoulder that watches me at times."

– Jennifer Bragg will be studying optics at the University of Arizona as an incoming graduate student starting this August. She is completing her summer internship from Pahoa, Hawaii.


Radina Yanakieva poses in front of a model of the Curiosity Mars rover at JPL

Courtesy of Radina Yanakieva | + Expand image

"I'm helping support the Perseverance Mars rover launch this summer. So far, I have been working remotely, but I'm lucky enough to have the opportunity to go to Pasadena, California, in late July to support the launch from JPL! On launch day, I will be in the testbed, where myself and a few other members of my group will be 'shadowing' the spacecraft. This means that when operators send their commands to the actual spacecraft, when it’s on the launch pad and during its first day or so in space, we'll send the same instructions to the test-bed version. This way, if anything goes wrong, we'll have a high-fidelity simulation ready for debugging.

I have a desk in my bedroom, so my office setup is decent enough. I bought a little whiteboard to write myself notes. As for my average working day, it really depends on what I'm doing. Some days, I'm writing procedures or code, so it's a text editor, a hundred internet tabs, and a messenger to ask my team members questions. Other days, I'm supporting a shift in the test bed, so I'm on a web call with a few other people talking about the test we're doing. Luckily, a large portion of my team's work can be done on our personal computers. The biggest change has been adding the ability to operate the test bed remotely. I'm often amazed that from New York, I can control hardware in California.

I was ecstatic that I was still able to help with the Perseverance Mars rover mission! I spent the second half of 2019 working on launch and cruise testing for the mission, so I'm happy to be able to see it through."

– Radina Yanakieva is an undergraduate student studying aerospace engineering at Georgia Tech and interning from Staten Island, New York.


Aditya Khuller stands with his arms outstretched and poses in front of a model Mars rover in a garage at JPL.

Courtesy of Aditya Khuller | + Expand image

"Our team is using radar data [from the European Space Agency’s Mars Express spacecraft] to find out what lies beneath the large icy deposits on Mars' south pole. My average day consists of analyzing this radar data on my computer to find and map the topography of an older surface that lies below the ice on Mars’ south pole, while my plants look on approvingly.

I was delighted to be offered the chance to work at JPL again. (This is my fourth JPL internship.) Even though it's better to be 'on lab,' it is an honor to get to learn from the coolest and smartest people in the world."

– Aditya Khuller is a graduate student working toward a Ph.D. in planetary science at Arizona State University and interning from Tempe, Arizona.


Breanna Ivey wears a Georgia Tech T-Shirt and poses in front of a river with her arms outstretched on concrete railing.

Courtesy of Breanna Ivey | + Expand image

"I am working on the Perseverance Mars rover mission [launching this summer]. As a member of the mobility team, I am testing the rover's auto-navigation behaviors. If given a specific location, flight software should be able to return data about where that location is relative to the rover. My project is to create test cases and develop procedures to verify the data returned by the flight software when this feature is used.

My average day starts with me eating breakfast with my mom who is also working from home. Then, I write a brief plan for my day. Next, I meet with my mentor to discuss any problems and/or updates. I spend the rest of my day at my portable workstation working on code to test the rover's behaviors and analyzing the data from the tests. I have a mini desk that I either set up in my bedroom in front of my Georgia Tech Buzz painting or in the dining room.

If I could visit in person, the first thing I would want to see is the Mars rover engineering model "Scarecrow." I would love to visit the Mars Yard [a simulated Mars environment at JPL] and watch Scarecrow run through different tests. It would be so cool to see a physical representation of the things that I've been working on."

– Breanna Ivey is an undergraduate student studying electrical engineering at the Georgia Institute of Technology and interning from Macon, Georgia.


Kaelan Oldani wears her graduation gown and holds her cap while posing in front of a sign that reads 'Michigan Union.'

Courtesy of Kaelan Oldani | + Expand image

"I am working on the Psyche mission as a member of the Assembly Test and Launch Operations team, also known as ATLO. (We engineers love our acronyms!) Our goal is to assemble and test the Psyche spacecraft to make sure everything works correctly so that the spacecraft will be able to orbit and study its target, a metal asteroid also called Psyche. Scientists theorize that the asteroid is actually the metal core of what was once another planet. By studying it, we hope to learn more about the formation of Earth.

I always start out my virtual work day by giving my dog a hug, grabbing a cup of coffee and heading up to my family's guest bedroom, which has turned into my office for the summer. On the window sill in my office are a number of space-themed Lego sets including the 'Women of NASA' set, which helps me get into the space-exploration mood! Once I have fueled up on coffee, my brain is ready for launch, and I log in to the JPL virtual network to start writing plans for testing Psyche's propulsion systems. While the ATLO team is working remotely, we are focused on writing test plans and procedures so that they can be ready as soon as the Psyche spacecraft is in the lab for testing. We have a continuous stream of video calls set up throughout the week to meet virtually with the teams helping to build the spacecraft."

– Kaelan Oldani is a master's student studying aerospace engineering at the University of Michigan and interning from Ann Arbor, Michigan. She recently accepted a full-time position at JPL and is starting in early 2021.


In the image on the left, Richardo Isai Melgar poses in front of a model of the Curiosity Mars rover at JPL. In the image on the right, he kneels in front of a model Mars rover in the Mars Yard at JPL.

Courtesy of Ricardo Isai Melgar | + Expand image

"NASA's Deep Space Network is a system of antennas positioned around the world – in Australia, Spain, and Goldstone, California – that's used to communicate with spacecraft. My internship is working on a risk assessment of the hydraulic system for the 70-meter antenna at the Goldstone facility. The hydraulic system is what allows the antenna and dish surrounding it to move so it can accurately track spacecraft in flight. The ultimate goal of the work is to make sure the antenna's hydraulic systems meet NASA standards.

My average day starts by getting ready for work (morning routine), accessing my work computer through a virtual interface and talking with my mentor on [our collaboration tool]. Then, I dive into work, researching hydraulic schematics, JPL technical drawings of the antenna, and NASA standards, and adding to a huge spreadsheet that I use to track every component of the antenna's hydraulic system. Currently, I'm tracking every flexible hydraulic fluid hose on the system and figuring out what dangers a failure of the hose could have on personnel and the mission."

– Ricardo Isai Melgar is an undergraduate student studying mechanical engineering at East Los Angeles College and interning from Los Angeles.


Susanna Eschbach poses in front of a mirrored background.

Courtesy of Susanna Eschbach | + Expand image

"My project this summer is to develop a network of carbon-dioxide sensors to be used aboard the International Space Station for monitoring the levels of carbon dioxide that crewmembers experience.

My 'office setup' is actually just a board across the end of my bed balanced on the other side by a small dresser that I pull into the middle of the room every day so that I can sit and have a hard surface to work on.

At first I wasn't sure if I was interested in doing a virtual engineering internship. How would that even work? But after talking to my family, I decided to accept. Online or in person, getting to work at JPL is still a really cool opportunity."

– Susanna Eschbach is an undergraduate student studying electrical and computer engineering at Northern Illinois University and interning from DeKalb, Illinois.


Izzie Torres poses in front of an ancient pyramid.

Courtesy of Izzie Torres | + Expand image

"I'm planning test procedures for the Europa Clipper mission [which is designed to make flybys of Jupiter's moon Europa]. The end goal is to create a list of tests we can perform that will prove that the spacecraft meets its requirements and works as a whole system.

I was very excited when I got the offer to do a virtual internship at JPL. My internship was originally supposed to be with the Perseverance Mars rover mission, but it required too much in-person work, so I was moved to the Europa Clipper project. While I had been looking forward to working on a project that was going to be launching so soon, Jupiter's moon Europa has always captured my imagination because of the ocean under its surface. It was an added bonus to know I had an internship secured for the summer."

– Izzie Torres is an undergraduate student studying aerospace engineering and management at MIT and interning from Seattle.


Jared Blanchard poses in front of a visualization in the VIVID lab at JPL.

Courtesy of Jared Blanchard | + Expand image

"I am investigating potential spacecraft trajectories to reach the water worlds orbiting the outer planets, specifically Jupiter's moon Europa. If you take both Jupiter and Europa into account, their gravitational force fields combine to allow for some incredibly fuel-efficient maneuvers between the two. The ultimate goal is to make it easier for mission designers to use these low-energy trajectories to develop mission plans that use very little fuel.

I'm not a gamer, but I just got a new gaming laptop because it has a nice graphics processing unit, or GPU. During my internship at JPL last summer, we used several GPUs and a supercomputer to make our trajectory computations 10,000 times faster! We plan to use the GPU to speed up my work this summer as well. I have my laptop connected to a second monitor up in the loft of the cabin where my wife and I are staying. We just had a baby two months ago, so I have to make the most of the quiet times when he's napping!"

– Jared Blanchard is a graduate student working toward a Ph.D. in aeronautics and astronautics at Stanford University.


Yohn Ellis, wearing a suit and tie, poses in front of yellow and gold balloons.

Courtesy of Yohn I. Ellis Jr. | + Expand image

"I'm doing a theory-based project on the topic of nanotechnology under the mentorship of Mohammad Ashtijou and Eric Perez.

I vividly remember being infatuated with NASA as a youth, so much so that my parents ordered me a pamphlet from Space Center Houston with posters and stickers explaining all of the cool things happening across NASA. I will never forget when I was able to visit Space Center Houston on spring break in 2009. It was by far the most amazing thing I have ever witnessed as a youth. When I was offered the internship at JPL, I was excited, challenged, and motivated. There is a great deal of respect that comes with being an NASA intern, and I look forward to furthering my experiences.

But the challenges are prevalent, too. Unfortunately, the internship is completely virtual and there are limitations to my experience. It is hard working at home with the multiple personalities in my family. I love them, but have you attempted to conduct research with a surround system of romantic comedies playing in the living room, war video games blasting grenades, and the sweet voice of your grandmother asking for help getting pans from the top shelf?"

– Yohn I. Ellis Jr. is a graduate student studying electrical engineering at Prairie View A&M University and interning from Houston.


Mina Cezairli wears a NASA hat and poses in front of a landscape of green mountains a turqoise ocean and puffy white and grey clouds.

Courtesy of Mina Cezairli | + Expand image

"This summer, I am supporting the proposal for a small satellite mission concept called Cupid’s Arrow. Cupid’s Arrow would be a small probe designed to fly through Venus’ atmosphere and collect samples. The ultimate goal of the project is to understand the “origin story” of Venus' atmosphere and how, despite their comparable sizes, Earth and Venus evolved so differently geologically, with the former being the habitable, friendly planet that we call home and the latter being the hottest planet in our solar system with a mainly carbon dioxide atmosphere.

While ordinary JPL meetings include discussions of space probes, rockets, and visiting other planets, my working day rarely involves leaving my desk. Because all of my work can be done on my computer, I have a pretty simple office setup: a desk, my computer, and a wall full of posters of Earth and the Solar System. An average day is usually a combination of data analysis, reading and learning about Venus, and a number of web meetings. The team has several different time zones represented, so a morning meeting in Pacific time accommodates all of Pacific, Eastern and European time zones that exist within the working hours of the team."

– Mina Cezairli is an undergraduate student studying mechanical engineering at Yale University and is interning from New Haven, Connecticut.


Izabella Zamora sits on steps leading up to a building with pumpkins decorating the steps to her right.

Courtesy of Izabella Zamora | + Expand image

“I'm characterizing the genetic signatures of heat-resistant bacteria. The goal is to improve the techniques we use to sterilize spacecraft to prevent them from contaminating other worlds or bringing contaminants back to Earth. Specifically, I'm working to refine the amount of time spacecraft need to spend getting blasted by dry heat as a sanitation method.

"As someone who has a biology-lab heavy internship, I was quite skeptical of how an online internship would work. There was originally supposed to be lab work, but I think the project took an interesting turn into research and computational biology. It has been a really cool intersection to explore, and I have gained a deeper understanding of the math and analysis involved in addition to the biology concepts."

– Izabella Zamora is an undergraduate student studying biology and computer science at the Massachusetts Institute of Technology and interning from Brimfield, Massachusetts.


Leilani Trautman poses for a photo at an outside table. The back of her open laptop has dozens of stickers attached to it, including a NASA meatball.

Courtesy of Leilani Trautman | + Expand image

"I am working on the engineering operations team for the Perseverance Mars rover. After the rover lands on Mars, it will send daily status updates. Every day, an engineer at JPL will need to make sure that the status update looks healthy so that the rover can continue its mission. I am writing code to make that process a lot faster for the engineers.

When I was offered the internship back in November, I thought I would be working on hardware for the rover. Once the COVID-19 crisis began ramping up and I saw many of my friends' internships get cancelled or shortened, I was worried that the same would happen to me. One day, I got a call letting me know that my previous internship wouldn't be possible but that there was an opportunity to work on a different team. I was so grateful to have the opportunity to retain my internship at JPL and get the chance to work with my mentor, Farah Alibay, who was once a JPL intern herself."

– Leilani Trautman is an undergraduate student studying electrical engineering and computer science at MIT and interning from San Diego, California.


Kathryn Chamberlin poses for an outdoor photo in front of a green hedge.

Courtesy of Kathryn Chamberlin | + Expand image

"I am working on electronics for the coronagraph instrument that will fly aboard the Nancy Grace Roman Space Telescope. The Roman Space Telescope will study dark energy, dark matter, and exoplanets [planets outside our solar system]. The science instrument I'm working on will be used to image exoplanets. It's also serving as a technology demonstration to advance future coronagraphs [which are instruments designed to observe objects close to bright stars].

I was both nervous and excited to have a virtual internship. I’m a returning intern, continuing my work on the coronagraph instrument. I absolutely love my work and my project at JPL, so I was really looking forward to another internship. Since I’m working with the same group, I was relieved that I already knew my team, but nervous about how I would connect with my team, ask questions, and meet other 'JPLers.' But I think my team is just as effective working virtually as we were when working 'on lab.' My mentor and I have even figured out how to test hardware virtually by video calling the engineer in the lab and connecting remotely into the lab computer."

– Kathryn Chamberlin is an undergraduate student studying electrical engineering at Arizona State University and interning from Phoenix.


Daniel Stover is shown in a screengrab from a web meeting app pointing to an illustration of the Perseverance Mars rover.

Courtesy of Daniel Stover | + Expand image

"I am working on the flight system for the Perseverance Mars rover. The first half of my internship was spent learning the rules of the road for the entire flight system. My first task was updating command-line Python scripts, which help unpack the data that is received from the rover. After that, I moved on to testing a part of the flight software that manages which mechanisms and instruments the spacecraft can use at a certain time. I have been so grateful to contribute to the Perseverance Mars rover project, especially during the summer that it launches!

I have always been one to be happy with all the opportunities I am granted, but I do have to say it was hard to come to the realization that I would not be able to step foot on the JPL campus. However, I was truly grateful to receive this opportunity, and I have been so delighted to see the JPL spirit translate to the online video chats and communication channels. It's definitely the amazing people who make JPL into the place that everybody admires. Most important, I would like to thank my mentor, Jessica Samuels, for taking the time to meet with me every day and show me the true compassion and inspiration of the engineers at JPL."

– Daniel Stover is an undergraduate student studying electrical and computer engineering at Virginia Tech and interning from Leesburg, Virginia.


In the image on the left, Sophia Yoo poses for a selfie. In the image on the right, her laptop, mouse, headphones and open notebook are shown at a table outside surrounded by a wooden porch and a green landscape.

Courtesy of Sophia Yoo | + Expand image

"I'm working on a project called the Multi-Angle Imager for Aerosols, or MAIA. It's an instrument that will go into lower Earth orbit and collect images of particulate matter to learn about air pollution and its effects on health. I'm programming some of the software used to control the instrument's electronics. I'm also testing the simulated interface used to communicate with the instrument.

I was ecstatic to still have my internship! I'm very blessed to be able to do all my work remotely. It has sometimes proven to be a challenge when I find myself more than four layers deep in virtual environments. And it can be confusing to program hardware on the West Coast with software that I wrote all the way over here on the East Coast. However, I've learned so much and am surprised by and grateful for the meaningful relationships I've already built."

– Sophia Yoo is an incoming graduate student studying electrical and computer engineering at Princeton University and is interning from Souderton, Pennsylvania.


Natalie Maus can be seen in the right corner of the image as she looks at a graph on her laptop.

Courtesy of Natalie Maus | + Expand image

"My summer research project is focused on using machine-learning algorithms to make predictions about the density of electrons in Earth’s ionosphere [a region of the planet's upper atmosphere]. Our work seeks to allow scientists to forecast this electron density, as it has important impacts on things such as GPS positioning and aircraft navigation.

Despite the strangeness of working remotely, I have learned a ton about the research process and what it is like to be part of a real research team. Working alongside my mentors to adapt to the unique challenges of working remotely has also been educational. In research, and in life, there will always be new and unforeseen problems and challenges. This extreme circumstance is valuable in that it teaches us interns the importance of creative problem solving, adaptability, and making the most out of the situation we are given."

– Natalie Maus is an undergraduate student studying astrophysics and computer science at Colby College and interning from Evergreen, Colorado.


Lucas Lange wears hiking gear and poses next to an American Flag at the top of a mountain with a valley visible in the background.

Courtesy of Lucas Lange | + Expand image

"I have two projects at JPL. My first project focuses on the Europa Clipper mission [designed to make flybys of Jupiter's moon Europa]. I study how the complex topography on the icy moon influences the temperature of the surface. This work is crucial to detect 'hot spots,' which are areas the mission (and future missions) aim to study because they might correspond to regions that could support life! My other work consists of studying frost on Mars and whether it indicates the presence of water-ice below the surface.

JPL and NASA interns are connected through social networks, and it's impressive to see the diversity. Some talks are given by 'JPLers' who make themselves available to answer questions. When I came to JPL, I expected to meet superheroes. This wish has been entirely fulfilled. Working remotely doesn't mean working alone. On the contrary, I think it increases our connections and solidarity."

– Lucas Lange is an undergraduate student studying aerospace engineering and planetary science at ISAE-SUPAERO [aerospace institute in France] and interning from Pasadena, California.


Explore JPL’s summer and year-round internship programs and apply at: jpl.nasa.gov/intern

Career opportunities in STEM and beyond can be found online at jpl.jobs. Learn more about careers and life at JPL on LinkedIn and by following @nasajplcareers on Instagram.

The laboratory’s STEM internship and fellowship programs are managed by the JPL Education Office. Extending the NASA Office of STEM Engagement’s reach, JPL Education seeks to create the next generation of scientists, engineers, technologists and space explorers by supporting educators and bringing the excitement of NASA missions and science to learners of all ages.

TAGS: Higher Education, Internships, STEM, College Students, Virtual Internships, Telework, Mars 2020 interns, Mars 2020, Perseverance, DSN, Deep Space Network, Mars, Asteroids, NEOWISE, Science, Technology, Engineering, Computer Science, Psyche, International Space Station, ISS, Europa, Jupiter, Europa Clipper, trajectory, nanotechnology, Cupid's Arrow, Proposal, Venus, Planetary Protection, Biology, Nancy Grace Roman Space Telescope, Dark Matter, Exoplanets, Multi-Angle Imager for Aerosols, MAIA, Earth, Earth science, air pollution, Hispanic Heritage Month, Black History Month, Asian Pacific American Heritage Month, Earth Science, Earth, Climate Change, Sea Level Rise

  • Kim Orr
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Illustration of spacecraft on a light purple background that reads "NASA Pi Day Challenge"

Update: March 16, 2020 – The answers to the 2020 NASA Pi Day Challenge are here! View the illustrated answer key (also available as a text-only doc).


In the News

Our annual opportunity to indulge in a shared love of space exploration, mathematics and sweet treats has come around again! Pi Day is the March 14 holiday that celebrates the mathematical constant pi – the number that results from dividing any circle's circumference by its diameter.

Infographic of all of the Pi in the Sky 7 graphics and problems

Visit the Pi in the Sky 7 lesson page to explore classroom resources and downloads for the 2019 NASA Pi Day Challenge. Image credit: NASA/JPL-Caltech | + Expand image

Overhead view of Mars with a comparison of the smaller landing ellipse made possible by Range Trigger technology

A new Mars landing technique called Range Trigger is reducing the size of the ellipse where spacecraft touch down. Image credit: NASA/JPL-Caltech | › Full image and caption

Composite image of the Kuiper Belt object Arrokoth from NASA's New Horizons spacecraft. Image credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/Roman Tkachenko | › Full image and caption

Diagram of an airplane flying over a section of ocean with an example of the spectral data that CORAL collects

The CORAL mission records the spectra of light reflected from the ocean to study the composition and health of Earth's coral reefs. Image credit: NASA | + Expand image

Rays of bright orange and red shoot out diagonally from a blue circle surrounding the star Beta Pictoris

The star Beta Pictoris and its surrounding debris disk in near-infrared light. Image credit: ESO/A.-M. Lagrange et al. | › Full image and caption

Besides providing an excuse to eat all varieties of pie, Pi Day gives us a chance to appreciate some of the ways NASA uses pi to explore the solar system and beyond. You can do the math for yourself – or get students doing it – by taking part in the NASA Pi Day Challenge. Find out below how to test your pi skills with real-world problems faced by NASA space explorers, plus get lessons and resources for educators.

How It Works

The ratio of any circle's circumference to its diameter is equal to pi, which is often rounded to 3.14. But pi is what is known as an irrational number, so its decimal representation never ends, and it never repeats. Though it has been calculated to trillions of digits, we use far fewer at NASA.

Pi is useful for all sorts of things, like calculating the circumference and area of circular objects and the volume of cylinders. That's helpful information for everyone from farmers irrigating crops to tire manufacturers to soup-makers filling their cans. At NASA, we use pi to calculate the densities of planets, point space telescopes at distant stars and galaxies, steer rovers on the Red Planet, put spacecraft into orbit and so much more! With so many practical applications, it's no wonder so many people love pi!

In the U.S., 3.14 is also how we refer to March 14, which is why we celebrate the mathematical marvel that is pi on that date each year. 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.

The NASA Pi Day Challenge

This year's NASA Pi Day Challenge poses four puzzlers that require pi to compare the sizes of Mars landing areas, calculate the length of a year for one of the most distant objects in the solar system, measure the depth of the ocean from an airplane, and determine the diameter of a distant debris disk. Learn more about the science and engineering behind the problems below or click the link to jump right into the challenge.

› Take the NASA Pi Day Challenge
› Educators, get the lesson here!

Mars Maneuver

Long before a Mars rover touches down on the Red Planet, scientists and engineers must determine where to land. Rather than choosing a specific landing spot, NASA selects an area known as a landing ellipse. A Mars rover could land anywhere within this ellipse. Choosing where the landing ellipse is located requires compromising between getting as close as possible to interesting science targets and avoiding hazards like steep slopes and large boulders, which could quickly bring a mission to its end. In the Mars Maneuver problem, students use pi to see how new technologies have reduced the size of landing ellipses from one Mars rover mission to the next.

Cold Case

In January 2019, NASA's New Horizons spacecraft sped past Arrokoth, a frigid, primitive object that orbits within the Kuiper Belt, a doughnut-shaped ring of icy bodies beyond the orbit of Neptune. Arrokoth is the most distant Kuiper Belt object to be visited by a spacecraft and only the second object in the region to have been explored up close. To get New Horizons to Arrokoth, mission navigators needed to know the orbital properties of the object, such as its speed, distance from the Sun, and the tilt and shape of its orbit. This information is also important for scientists studying the object. In the Cold Case problem, students can use pi to determine how long it takes the distant object to make one trip around the Sun.

Coral Calculus

Coral reefs provide food and shelter to many ocean species and protect coastal communities against extreme weather events. Ocean warming, invasive species, pollutants, and acidification caused by climate change can harm the tiny living coral organisms responsible for building coral reefs. To better understand the health of Earth's coral reefs, NASA's COral Reef Airborne Laboratory, or CORAL, mission maps them from the air using spectroscopy, studying how light interacts with the reefs. To make accurate maps, CORAL must be able to differentiate among coral, algae and sand on the ocean floor from an airplane. And to do that, it needs to calculate the depth of the ocean at every point it maps by measuring how much sunlight passes through the ocean and is reflected upward from the ocean floor. In Coral Calculus, students use pi to measure the water depth of an area mapped by the CORAL mission and help scientists better understand the status of Earth's coral reefs.

Planet Pinpointer

Our galaxy contains billions of stars, many of which are likely home to exoplanets – planets outside our solar system. So how do scientists decide where to look for these worlds? Using data gathered by NASA's Spitzer Space Telescope, researchers found that they're more likely to find giant exoplanets around young stars surrounded by debris disks, which are made up of material similar to what's found in the asteroid belt and Kuiper Belt in our solar system. Sure enough, after discovering a debris disk around the star Beta Pictoris, researchers later confirmed that it is home to at least two giant exoplanets. Learning more about Beta Pictoris' debris disk could give scientists insight into the formation of these giant worlds. In Planet Pinpointer, put yourself in the role of a NASA scientist to learn more about Beta Pictoris' debris disk, using pi to calculate the distance across it.

Participate

Join the conversation and share your Pi Day Challenge answers with @NASAJPL_Edu on social media using the hashtag #NASAPiDayChallenge

Blogs and Features

Related Lessons for Educators

Related Activities for Students

NOAA Video Series: Coral Comeback

Multimedia

Facts and Figures

Missions and Instruments

Websites

TAGS: K-12 Education, Math, Pi Day, Pi, NASA Pi Day Challenge, Events, Space, Educators, Teachers, Parents, Students, STEM, Lessons, Problem Set, Mars 2020, Perseverance, Curiosity, Mars rovers, Mars landing, MU69, Arrokoth, New Horizons, Earth science, Climate change, CORAL, NASA Expeditions, coral reefs, oceans, Spitzer, exoplanets, Beta Pictoris, stars, universe, space telescope, Climate TM

  • Lyle Tavernier
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Animated illustration of Earth orbiting the Sun

You may have noticed that there's an extra day on your calendar this year. That's not a typo; it's leap day! Leap day is another name for Feb. 29, a date that typically comes around every four years, during a leap year. Why doesn't Feb. 29 appear on the calendar every year? Read on to find out how the imperfect match between the length of a calendar year and Earth's orbit results in the need to make small adjustments to our calendar on a regular basis. Explore leap day resources for students, too.

The length of a year is based on how long it takes a planet to revolve around the Sun. Earth takes about 365.2422 days to make one revolution around the Sun. That's about six hours longer than the 365 days that we typically include in a calendar year. As a result, every four years we have about 24 extra hours that we add to the calendar at the end of February in the form of leap day. Without leap day, the dates of annual events, such as equinoxes and solstices, would slowly shift to later in the year, changing the dates of each season. After only a century without leap day, summer wouldn’t start until mid-July!

But the peculiar adjustments don't end there. If Earth revolved around the Sun in exactly 365 days and six hours, this system of adding a leap day every four years would need no exceptions. However, Earth takes a little less time than that to orbit the Sun. Rounding up and inserting a 24-hour leap day every four years adds about 45 extra minutes to every four-year leap cycle. That adds up to about three days every 400 years. To correct for that, years that are divisible by 100 don't have leap days unless they’re also divisible by 400. If you do the math, you'll see that the year 2000 was a leap year, but 2100, 2200 and 2300 will not be.

After learning more about leap years with this article from NASA's Space Place, students can do the math for themselves with this leap day problem set. Follow that up with writing a letter or poem to be opened on the next leap day. And since we've got an extra 24 hours this year, don't forget to take a little time to relax!

Explore More

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

TAGS: K-12 Education, Math, Leap Day, Leap Year, Events, Space, Educators, Teachers, Parents, Students, STEM, Lessons, Earth Science, Earth

  • Lyle Tavernier
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