An Apollo 11 astronaut stands on the Moon and one of the legs of the lunar module can be seen in the corner of the image

Fifty years ago this week, the Apollo 11 astronauts launched on their history-making mission. Saturday, July 20, is the anniversary of that first landing of humans on the Moon; a great milestone to reflect on, as well as an opportunity to look ahead. Read on for some of the ways you can celebrate and learn with NASA!

An audience wears 3-D glasses while in a darkened theater

Go Places

It’s not just science centers that are celebrating the 50th anniversary of humans landing on the Moon. There are events taking place worldwide at libraries, concert halls, baseball stadiums, National Parks, art museums, and on city streets. Find anniversary events near you with this searchable map and calendar.

Sketch of a lunar lander on graph paper with marshmallows, rubber bands and straws scattered around

Do Things

This collection of hands-on activities for all ages will have you throwing water balloons to learn about craters on the Moon, helping actual NASA scientists by mapping the Moon from your own computer, building a model of the Earth-Moon system and seeing what it takes to investigate strange new planets. You can even make your own lunar spacecraft.

The Forward to the Moon With Artemis activity book is a fun way to learn about the Apollo mission that first put people on the Moon and what’s in store for the future. Also, check out these hands-on activities, building challenges and online games!

Animated image of the Moon phases

Focus On the Moon

Love observing the Moon and the rest of the night sky? The Night Sky Network will help you find local astronomy clubs and events. Save the date for International Observe the Moon Night, October 5. If you’re clouded out, you can always make your own Moon to enjoy!

Blue starry background with type that reads Apollo 50 Next Giant Leap

Watch These

NASA TV has a full lineup of Apollo programming. On July 19 at 3 p.m. (EDT), you can watch STEM Forward to the Moon. The half-hour show will feature students enacting simulations of a return to the Moon with NASA’s Artemis program. The accompanying Educator’s Guide has all you need to try the activities from the show at home or in the classroom.

Also fun to watch are vintage recordings from the Apollo program, as well as archived lectures and the kid-friendly “STEM in 30” video series from the National Air And Space Museum.

Scissors, pencils, tape, paper and other materials scattered around. Text overlay reads: Join in July 18, #VirtualMoonshot, A virtual mission to the Moon designed by you! Instagram, Facebook & Twitter

Get Social

Join NASA and educational centers nationwide to build a virtual mission to the Moon on July 18. Follow #VirtualMoonshot on Instagram, Facebook and Twitter to take part – or follow along with a host center near you.

Finally, if you’ve wondered what it would have been like to have social media 50 years ago, be sure to follow Relive Apollo 11 for tweets that tell the story of the mission in real time, starting with its July 16 launch!

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TAGS: Apollo 50th, Events, Activities, Education, STEM, Science, Museums,

  • Amelia Chapman
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Amiee Quon points to a small rover built out of legos as her team stands in a circle around her examining the rover.

Last week, 40 community college students landed at NASA's Jet Propulsion Laboratory to accept the challenge of building miniature Mars rovers over the course of four days, from July 9-12, putting their designs to the test in a series of competitions on simulated Martian terrain.

The challenge is part of the National Community College Aerospace Scholar, or NCAS, program, which hosts hundreds of students across multiple NASA centers for a twice-yearly educational workshop and engineering competition. The activity provides students with an up-close and intimate look at NASA missions, and an opportunity to present their work to a panel of judges.

Several students stand against a wall while another sets a miniature rover on a red surface meant to simulate Martian terrain

Students ready their rover to compete in one of two challenges that took place during the activity at JPL. Image credit: NASA/JPL-Caltech/Lyle Tavernier | + Expand image

One key part of their week here: The students, who are divided into four teams, are mentored by NASA scientists and engineers. And at JPL – where the competition is organized by the Education Office – nobody knows the mentorship experience better than Amiee Quon and Otto Polanco, JPL's two longest-serving NCAS mentors.

In 2012, Quon – who participated in the high school version of NCAS when she was 16 – saw an email circulated at JPL requesting mentors for the competition. She signed up and has been a mentor ever since.

“It’s so rewarding to see how excited they are about engineering, and when they work hard on something and collaborate, that things work out for them,” says Quon, a mechanical integration engineer who has worked on the Mars 2020 helicopter and the Juno mission orbiting Jupiter, and is currently working on the Europa Clipper mission.

10 students and Quon stand in two rows smiling with their winnings, including a padfolio and a Hot Wheels rover

Quon's team poses for a photo with their winnings from the summer 2019 competition. Image credit: NASA/JPL-Caltech/Kim Orr | + Expand image

Things worked out especially well for Quon's mentees this session: The 10 students on her team were named the winners of the summer 2019 competition.

“My team was very cohesive, and I was impressed by how well they worked together to design, build and operate their successful rover,” she says. “All the teams did a great job on the toughest competition course I’ve ever seen.”

For Polanco, being a mentor is a capstone on his own experience as a community college student. He started his undergraduate studies at Santa Monica College, transferred to Cal State L.A. to earn his bachelor’s and master’s degrees in mechanical engineering, and eventually landed an internship at JPL. He's been at JPL for 15 years and has worked as an optical-mechanical engineer on the Mars Science Laboratory mission, Starshade project and more.

The NCAS competition is an opportunity for Polanco to encourage students to go after what they want to do – including helping one female college freshman, whose family expected her to marry and have children instead of chasing a STEM career. Polanco guided her during an NCAS competition and stayed in touch throughout her college years; today, she’s pursuing a Ph.D. at Caltech and studying global climate change.

Polanco makes a claw motion with his hands, while three students stand in a semi circle around him with one student mimicking the claw motion

Polanco speaks with several of his mentees during the summer 2019 session of NCAS. Image credit: NASA/JPL-Caltech/Lyle Tavernier | + Expand image

“The most rewarding part is influencing people’s perspectives about what their engineering futures might be,” he says. “It’s about convincing them to pursue their dreams and passions and seeing them grow over the years.”

While Quon and Polanco play a big part in helping guide the students through various Mars rover challenges and their final presentations, they both recognize that their ultimate roles lie in reminding students that they deserve to achieve anything they set their minds to.

“A lot of our mentorship is raising the confidence levels of individuals,” Polanco says. “It’s through these side conversations that you often hear, ‘I’m not qualified or worthy enough to work here.’” And I always ask them, ‘Why do you put a ceiling on yourself?’”

Adds Quon: “We talked to somebody during the competition who felt they would be at a disadvantage going to career fairs because they transferred [into their current university]. But you’ve worked hard to get to where you are. There’s absolutely no reason to feel 'less than.'”

To that end, Polanco encourages more people at JPL to mentor when they can.

“I think it’s a really good experience for JPL employees to go through, to see how their own experience can help others,” he says. “My little path is a good example of what people can do. There are so many students in community college who struggle to see that end achievement. But the institution is good about hiring talent and [individuals with] strong work ethic, no matter where you went to school.”


The NCAS program is funded by the NASA Minority University Research and Education Program. Learn more and apply, here.

TAGS: Higher Education, Community College, NCAS, Mentors, Students, STEM, Engineering

  • Celeste Hoang
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Buzz Aldrin stands on the moon in his puffy, white spacesuit next to an American flag waving in the wind. The command module casts a long, dark shadow nearby.

In the News

This year marks the 50th anniversary of humans landing on the Moon. Now NASA is headed to the Moon once again, using it as a proving ground for a future human mission to Mars. Use this opportunity to get students excited about Earth's natural satellite, the amazing feats accomplished 50 years ago and plans for future exploration.

How They Did It

When NASA was founded in 1958, scientists were unsure whether the human body could even survive orbiting Earth. Space is a demanding environment. Depending on where in space you are, it can lack adequate air for breathing, be very cold or hot, and have dangerous levels of radiation. Additionally, the physics of space travel make everything inside a space capsule feel weightless even while it's hurtling through space. Floating around inside a protective spacecraft may sound fun, and it is, but it also can have detrimental effects on the human body. Plus, it can be dangerous with the hostile environment of space lurking on the other side of a thin metal shell.

In 1959, NASA's Jet Propulsion Laboratory began the Ranger project, a mission designed to impact the Moon – in other words, make a planned crash landing. During its descent, the spacecraft would take pictures that could be sent back to Earth and studied in detail. These days, aiming to merely impact a large solar system body sounds rudimentary. But back then, engineering capabilities and course-of-travel, or trajectory, mathematics were being developed for the first time. A successful impact would be a major scientific and mathematical accomplishment. In fact, it took until July 1964 to achieve the monumental task, with Ranger 7 becoming the first U.S. spacecraft to impact the near side of the Moon, capturing and returning images during its descent.

Side-by-side images of a model of the Ranger 7 spacecraft in color and a black and white image of the Moon taken by Ranger 7.

These side-by-side images show a model of the Ranger 7 spacecraft (left) and an image the spacecraft took of the Moon (right) before it impacted the surface. Image credit: NASA/JPL-Caltech | › + Expand image

After the successful Ranger 7 mission, two more Ranger missions were sent to the Moon. Then, it was time to land softly. For this task, JPL partnered with Hughes Aircraft Corporation to design and operate the Surveyor missions between 1966 and 1968. Each of the seven Surveyor landers were equipped with a television camera – with later landers carried scientific instruments, too – aimed at obtaining up-close lunar surface data to assess the Moon's suitability for a human landing. The Surveyors also demonstrated in-flight maneuvers and in-flight and surface-communications capabilities.

Side-by-side image of an astronaut next to the Surveyor 7 lander and a mosaic of images from Surveyor 3

These side-by-side images show Apollo 12 Commander Charles Conrad Jr. posing with the Surveyor 7 spacecraft on the Moon (left) and a mosaic of images taken by Surveyor 3 on the lunar surface (right). Image credits: NASA/JPL-Caltech | › + Expand image

In 1958, at the same time JPL was developing the technological capabilities to get to the Moon, NASA began the Mercury program to see if it was possible for humans to function in space. The success of the single-passenger Mercury missions, with six successful flights that placed two astronauts into suborbital flight and four astronauts into Earth orbit, kicked off the era of U.S. human spaceflight.

Cutaway illustration of the Mercury capsule with a single astronaut inside.

The success of the single-passenger Mercury capsule, shown in this illustrated diagram, proved that humans could live and work in space, paving the way for future human exploration. Image credit: NASA | › Full image and caption

In 1963, NASA's Gemini program proved that a larger capsule containing two humans could orbit Earth, allowing astronauts to work together to accomplish science in orbit for long-duration missions (up to two weeks in space) and laying the groundwork for a human mission to the Moon. With the Gemini program, scientists and engineers learned how spacecraft could rendezvous and dock while in orbit around Earth. They were also able to perfect re-entry and landing methods and began to better understand the effects of longer space flights on astronauts. After the successful Gemini missions, it was time to send humans to the Moon.

Cutaway illustration of the Gemini spacecraft with two astronauts inside.

The Gemini spacecraft, shown in this illustrated cutaway, paved the way for the Apollo missions. Image credit: NASA | › Full image and caption

The Apollo program officially began in 1963 after President John F. Kennedy directed NASA in September of 1962 to place humans on the Moon by the end of the decade. This was a formidable task as no hardware existed at the time that would accomplish the feat. NASA needed to build a giant rocket, a crew capsule and a lunar lander. And each component needed to function flawlessly.

Rapid progress was made, involving numerous NASA and contractor facilities and hundreds of thousands of workers. A crew capsule was designed, built and tested for spaceflight and landing in water by the NASA contractor North American Aviation, which eventually became part of Boeing. A lunar lander was developed by the Grumman Corporation. Though much of the astronaut training took place at or near the Manned Spacecraft Center, now known as NASA’s Johnson Space Center, in Texas, astronauts practiced lunar landings here on Earth using simulators at NASA's Dryden (now Armstrong) Flight Research Center in California and at NASA's Langley Research Center in Virginia. The enormous Saturn V rocket was a marvel of complexity. Its first stage was developed by NASA's Marshall Space Flight Center in Alabama. The upper-stage development was managed by the Lewis Flight Propulsion Center, now known as NASA's Glenn Research Center, in Ohio in partnership with North American Aviation and Douglas Aircraft Corporation, while Boeing integrated the whole vehicle. The engines were tested at what is now NASA's Stennis Space Center in Mississippi, and the rocket was transported in pieces by water for assembly at Cape Kennedy, now NASA's Kennedy Space Center, in Florida. As the Saturn V was being developed and tested, NASA also developed a smaller, interim vehicle known as the Saturn I and started using it to test Apollo hardware. A Saturn I first flew the Apollo command module design in 1964.

Unfortunately, one crewed test of the Apollo command module turned tragic in February 1967, when a fire erupted in the capsule and killed all three astronauts who had been designated as the prime crew for what became known as Apollo 1. The command module design was altered in response, delaying the first crewed Apollo launch by 21 months. In the meantime, NASA flew several uncrewed Apollo missions to test the Saturn V. The first crewed Apollo launch became Apollo 7, flown on a Saturn IB, and proved that the redesigned command module would support its crew while remaining in Earth orbit. Next, Earth-Moon trajectories were calculated for this large capsule, and the Saturn V powered Apollo 8 set off for the Moon, proving that the calculations were accurate, orbiting the Moon was feasible and a safe return to Earth was possible. Apollo 8 also provided the first TV broadcast from lunar orbit. The next few Apollo missions further proved the technology and allowed humans to practice procedures that would be needed for an eventual Moon landing.

On July 16, 1969, a Saturn V rocket launched three astronauts to the Moon on Apollo 11 from Cape Kennedy. The Apollo 11 spacecraft had three parts: a command module, called "Columbia," with a cabin for the three astronauts; a service module that provided propulsion, electricity, oxygen and water; and a lunar module, "Eagle," that provided descent to the lunar surface and ascent back to the command and service modules.

Collage of three images showing the lunar module during its descent to the Moon, on the lunar surface and during its ascent.

In this image collage, the Apollo 11 lunar module is shown on its descent to the Moon (left), on the lunar surface as Buzz Aldrin descends the stairs (middle), and on its ascent back to the command module (right). Image credit: NASA | › View full image collection

On July 20, while astronaut and command module pilot Michael Collins orbited the Moon, Neil Armstrong and Buzz Aldrin landed Eagle on the Moon and set foot on the surface, accomplishing a first for humankind. They collected regolith (surface "dirt") and rock samples, set up experiments, planted an American flag and left behind medallions honoring the Apollo 1 crew and a plaque that read, "We came in peace for all mankind."

Collage of images showing Buzz Aldrin doing various activities on the Moon.

This collage of images from the Apollo 11 Moon landing shows Buzz Aldrin posing for a photo on the Moon (left), and setting up the solar wind and seismic experiments (middle). The image on the right shows the plaque the team placed on Moon to commemorate the historic event. Image credit: NASA | › View full image collection

After 21.5 hours on the lunar surface, Armstrong and Aldrin rejoined Collins in the Columbia command module and, on July 21, headed back to Earth. On July 24, after jettisoning the service module, Columbia entered Earth's atmosphere. With its heat shield facing forward to protect the astronauts from the extreme friction heating outside the capsule, the craft slowed and a series of parachutes deployed. The module splashed down in the South Pacific Ocean, 380 kilometers (210 nautical miles) south of Johnston Atoll. Because scientists were uncertain about contamination from the Moon, the astronauts donned biological-isolation garments delivered by divers from the recovery ship, the aircraft carrier the USS Hornet. The astronauts boarded a life raft and then the USS Hornet, where the outside of their biological-isolation suits were washed down with disinfectant. To be sure no contamination was brought back to Earth from the Moon, the astronauts were quarantined until Aug. 10, at which point scientists determined the risk was low that biological contaminants or microbes had returned with the astronauts. Columbia was also disinfected and is now part of the National Air and Space Museum in Washington, D.C.

On the left, a capsule floats in the ocean while astronauts sit in a raft in a gray suits. On the right, the three astronauts smile while looking out of a small window and while Nixon faces them with a microphone in front of him.

These side-by-side images show the Apollo 11 astronauts leaving the capsule in their biological isolation garments after successfully splashing down in the South Pacific Ocean (left). At right, President Richard M. Nixon welcomes the Apollo 11 astronauts, (left to right) Neil A. Armstrong, Michael Collins and Buzz Aldrin, while they peer through the window of the Mobile Quarantine Facility aboard the USS Hornet. Image credit: NASA | › View full image collection

The Apollo program continued with six more missions to the Moon over the next three years. Astronauts placed seismometers to measure "moonquakes" and other science instruments on the lunar surface, performed science experiments, drove a carlike moon buggy on the surface, planted additional flags and returned more lunar samples to Earth for study.

Why It's Important

Apollo started out as a demonstration of America's technological, economic and political prowess, which it accomplished with the first Moon landing. But the Apollo missions accomplished even more in the realm of science and engineering.

Some of the earliest beneficiaries of Apollo research were Earth scientists. The Apollo 7 and 9 missions, which stayed in Earth orbit, took photographs of Earth in different wavelengths of light, highlighting things that might not be seen on the ground, like diseased trees and crops. This research led directly to the joint NASA-U.S. Geological Survey Landsat program, which has been studying Earth's resources from space for more than 45 years.

Samples returned from the Moon continue to be studied by scientists around the world. As new tools and techniques are developed, scientists can learn even more about our Moon, discovering clues to our planet's origins and the formation of the solar system. Additionally, educators can be certified to borrow lunar samples for use in their classrooms.

The Apollo 11 astronauts crowd around a lunar sample contained in a protective case.

The Apollo 11 astronauts take a closer look at a sample they brought back from the Moon. Image credit: NASA | › View full image collection

Perhaps the most important scientific finding came from comparing similarities in the composition of lunar and terrestrial rocks and then noting differences in the amount of specific substances. This suggested a new theory of the Moon's formation: that it accreted from debris ejected from Earth by a collision with a Mars-size object early in our planet's 4.5-billion-year history.

The 12 astronauts who walked on the Moon are the best-known faces of the Apollo program, but in numbers, they were also the smallest part of the program. About 400,000 men and women worked on Apollo, building the vehicles, calculating trajectories, even making and packing food for the crews. Many of them worked on solving a deceptively simple question: "How do we guide astronauts to the Moon and back safely?" Some built the spacecraft to carry humans to the Moon, enable surface operations and safely return astronauts to Earth. Others built the rockets that would launch these advanced spacecraft. In doing all this, NASA engineers and scientists helped lead the computing revolution from transistors to integrated circuits, the forebears to the microchip. An integrated circuit – a miniaturized electronic circuit that is used in nearly all electronic equipment today – is lighter weight, smaller and able to function on less power than the older transistors and capacitors. To suit the needs of the space capsule, NASA developed integrated circuits for use in the capsule's onboard computers. Additionally, computing advancements provided NASA with software that worked exactly as it was supposed to every time. That software lead to the development of the systems used today in retail credit-card swipe devices.

Some lesser-known benefits of the Apollo program include the technologies that commercial industries would then further advance to benefit humans right here on Earth. These "spinoffs" include technology that improved kidney dialysis, modernized athletic shoes, improved home insulation, advanced commercial and residential water filtration, and developed the freeze-drying technique for preserving foods.

Apollo was succeeded by missions that have continued to build a human presence in space and advance technologies on Earth. Hardware developed for Apollo was used to build America's first Earth-orbiting space station, Skylab. After Skylab, during the Apollo-Soyuz test project, American and Soviet spacecraft docked together, laying the groundwork for international cooperation in human spaceflight. American astronauts and Soviet cosmonauts worked together aboard the Soviet space station Mir, performing science experiments and learning about long-term space travel's effects on the human body. Eventually, the U.S. and Russia, along with 13 other nations, partnered to build and operate the International Space Station, a world-class science laboratory orbiting 400 kilometers (250 miles) above Earth, making a complete orbit every 90 minutes.

Graphic showing a possible configuration for the future lunar gateway

Although the configuration is not final, this infographic shows the current lineup of parts comprising the lunar Gateway. Image credit: NASA | › Full image and caption

And the innovations continue today. NASA is planning the Artemis mission to put humans on the Moon again in 2024 with innovative new technologies and the intent of establishing a permanent human presence. Working in tandem with commercial and international partners, NASA will develop the Space Launch System launch vehicle, Orion crew capsule, a new lunar lander and other operations hardware. The lunar Gateway – a small spaceship that will orbit the Moon and include living quarters for astronauts, a lab for science, and research and ports for visiting spacecraft – will provide access to more of the lunar surface than ever before. While at the Moon, astronauts will research ways to use lunar resources for survival and further technological development. The lessons and discoveries from Artemis will eventually pave a path for a future human mission to Mars.

Teach It

Use these standards-aligned lessons to help students learn more about Earth's only natural satellite:

As students head out for the summer, get them excited to learn more about the Moon and human exploration using these student projects:

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TAGS: K-12 Education, Teachers, Educators, Classroom, Engineering, Science, Students, Projects, Moon, Apollo, Summer

  • Ota Lutz
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Brittney Cooper stands in a sandy area holding a controller attached to a rover

Brittney Cooper loves studying weather – and she's taking that passion all the way to Mars. A graduate student at York University in Toronto, Cooper has spent the past two years working with the science team for NASA's Mars rover Curiosity. In January, she authored her first science paper on a study she designed with the Curiosity team that looked at how clouds scatter light and what that tells us about the shapes of their ice crystals. Despite her involvement in the Curiosity mission, the Canada native has never actually been to a NASA center. But that's about to change this summer when she'll embark on her first internship at JPL in Pasadena, California. We caught up with Cooper to find out what she's looking forward to most about her internship and how she's planning to take her studies of Martian clouds even farther.

You're currently earning your master's at York University in Toronto. What are you studying and what got you interested in that field?

I'm doing my master's in Earth and space science. But if you really want an interesting story [laughs] … I've always been interested in astronomy, space and science, but I also really love art. Coming to the end of high school, I realized that maybe it was going to be too hard for me to pursue science. Maybe I was a little scared and I didn't really think I was going to be able to do it. So I went to university for photography for two years. After two years, I realized photography wasn't challenging me in the right ways and wasn't what I wanted to do for the rest of my life. So I left. I did night school to get credits for calculus and all the grade-12 physics and chemistry that I needed to pursue a degree in atmospheric science, which is not even remotely astronomy, but I've also always loved weather – pretty much anything in the sky. I still had a passion for astronomy, so I started volunteering at the Allan I. Carswell observatory at York. There, I met a professor who I ended up doing research with for many years. He told me, "There's the field called planetary science, where you can study the atmospheres of other planets and you can kind of marry those two fields that you're interested in [astronomy and atmospheric science]." So I ended up adding an astronomy major.

Brittney Copper stands in the snow surrounded by pine trees and holds out a device to measure the flux of solar radiation

Cooper measures the downward flux of solar radiation during a winter snow survey. Image courtesy Brittney Cooper | + Expand image

Later, I started doing research with this professor, John Moores, as an undergrad. In my last year, there was a Ph.D. student who was a participating scientist on NASA's Mars Science Laboratory mission and he was graduating. John had said something along the lines of, "There's an opening, and I know it's always been your dream to work in mission control, so do you want to be on the mission?" And I was, like, "Yes, I definitely do!" I couldn't believe it. And I was never intending to do a master's, but then I realized I really loved the work I was doing, working on constraining physical properties of Martian water-ice clouds using the Mars Curiosity rover. We got to design this observation, which ran on the rover, and then I got to work with the data from it, which was really cool. So I stayed on to do my master's, and I'm still on the mission, which is pretty awesome.

In January you authored your first science paper on that research. Tell me more about that.

A black and white animated image showing light, wispy clouds moving across the Martian sky

Wispy clouds float across the Martian sky in this accelerated sequence of images from NASA's Curiosity Mars rover. Image credit: NASA/JPL-Caltech/York University | › Full image and caption

My research focuses on the physical scattering properties of Martian water-ice clouds. A lot of people don't even realize that there are clouds on Mars, which I totally get because Mars doesn't have much of an atmosphere. But it does have enough of an atmosphere to create very thin, wispy, almost cirrus-like clouds similar to the ones we have on Earth. They're made up of small, water-ice crystals. These kinds of clouds do have a noticeable impact on Earth's climate, so we have now started thinking about what these clouds are doing in Mars' climate. The scattering properties can tell us a bit about that. They can tell us how much radiation is scattered back to space by these clouds or kept in Mars' atmosphere and whether or not we can see really fun things like halos, glories and different types of optical phenomena that we can see here on Earth.

We designed this observation that uses the Navcam imager on Curiosity. The engineering folks with the mission helped us design it. I got to present at a science discussion, which was superscary, but everyone was so kind. And then the observation was approved to run on Mars once a week from September 2017 to March 2018. During this observation window, Curiosity would take images of the sky to capture clouds at as many different scattering angles as possible. Once we got all the data back, we were able to constrain the dominant ice crystal shapes in the clouds based upon this thing called the phase function, which tells you how these clouds scatter light and radiation. I was the lead author on the research paper that came from that, and it got accepted. We started working on this right when I was really new to the mission, and it was my first paper. I couldn't believe everyone wasn't, like, "Who the heck are you? Why are we going to let you do anything?" But everyone was so kind, and it was just such a great experience.

What was the hardest part about writing that first paper?

The hardest part was probably just getting over the fear of thinking people aren't going to listen to you or you aren't going to be smart enough or you won't be able to answer questions. It was really just getting over my own fears and worries and not holding myself back because of them. I have a really great mentor who pushed me to do all these things, so I was able to suck it up and say, "If he believes in me and he thinks I can do it, maybe he's right." Every time I did a presentation or I would talk about the observation or try to advocate for it, I was just met with such positivity that I was, like, "OK, these fears are rooted in nothing."

In July, you're coming to JPL for your first internship here. What will you be working on?

Yes, I'm so excited! I'll be working with two scientists, Michael Mischna and Manuel de la Torre Juarez. We're going to be working with the Rover Environmental Monitoring Station, or REMS, which is an instrument on Curiosity that measures the temperature, relative humidity and pressure around the rover on Mars. From those measurements, we're going to try to infer the presence of clouds at night. So far, the way we've used Curiosity to study clouds is with optical instruments [or cameras]. So we take pictures of the clouds. But that's not really something we can do at night. So using REMS and its temperature sensors at night, we can try to see if clouds around the rover are emitting infrared radiation, heating up the atmosphere around the rover. We can try to detect them that way. So that's what we're going to try to do – look for some patterns and see what we can come up with. We'll also be comparing what we find with data from NASA's Mars Climate Sounder, which is in orbit around Mars and takes nighttime measurements of the atmosphere.

What are you most excited about coming to JPL?

I would be lying if I said it wasn't just getting to come to a NASA center – especially as a Canadian. It's every little space enthusiast's dream. I'm also excited to meet all the people who I've been working with for the last two years. The people are such an awesome part of this mission that I've been a part of. So I'm looking forward to meeting them in person and working with them in a closer way.

What do you see as the ultimate goal of your research?

We're just trying to better understand Mars. It's kind of a crazy place. There is a lot of evidence that shows us that there's a lot more going on than we know now and it's just about trying to put the pieces of the puzzle together. There are also a lot of similarities to Earth. So we can try to take what we learn about Mars and apply it to our planet as well.

What's your ultimate career goal?

What I would really love is to work in spacecraft operations. I absolutely love working in science and working with data, but getting a chance to be a part of this mission and do operations – be part of a team and do multidisciplinary work – it's so exciting, and it's something that I never thought that I'd get to experience. And now that I've had a bit of a taste, I'm wanting more. So that's what I'm hoping for in the future.

Do you ever think about how you moved away from studying photography but are using photography to do science on Mars?

Yes! Every once in a while, that hits me, and I think to myself, "That's so cool." It's just very, very cool. Ten years ago, I never thought I'd be where I am now. But also just to know that there's that connection, that I'm working with visual data, with optical data – I don't think it's a coincidence. I really love working with images, so I think it's pretty cool that I get to do that.

Just one last fun question: If you could travel to any place in space, where would you go and what would you do there?

Without a doubt, it would have to be [Saturn's moon] Titan. I actually would probably go there to study the atmosphere. The first research project that I ever did was trying to find methane and ethane fog on Titan and the surface data was quite limited, so I would like to go there. I want to see water-ice rocks. I want to see methane lakes and methane rain, set up a little vacation spot there [laughs].


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

The laboratory’s STEM internship and fellowship programs are managed by the JPL Education Office. Extending the NASA Office of Education’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, College, Internships, Interns, Students, Science, Mars, Rovers, Weather

  • Kim Orr
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The Millennium Falcon takes on TIE fighters in a scene from 'Star Wars: The Force Awakens.'

This feature was originally published on May 3, 2016.


In the News

What do "Star Wars," NASA's Dawn spacecraft and Newton's Laws of Motion have in common? An educational lesson that turns science fiction into science fact using spreadsheets – a powerful tool for developing the scientific models addressed in the Next Generation Science Standards.

The TIE (Twin Ion Engine) fighter is a staple of the "Star Wars" universe. Darth Vader flew one in "A New Hope." Poe Dameron piloted one in "The Force Awakens." And many, many Imperial pilots met their fates in them. While the fictional TIE fighters in "Star Wars" flew a long time ago in a galaxy far, far away, ion engines are a reality in this galaxy today – and have a unique connection to NASA’s Jet Propulsion Laboratory.

Launched in 1998, the first spacecraft to use an ion engine was Deep Space 1, which flew by asteroid 9969 Braille and comet Borrelly. Fueled by the success of Deep Space 1, engineers at JPL set forth to develop the next spacecraft that would use ion propulsion. This mission, called Dawn, would take ion-powered spacecraft to the next level by allowing Dawn to go into orbit twice – around the two largest objects in the asteroid belt: Vesta and Ceres.

How Does It Work?

Ion engines rely on two principles that Isaac Newton first described in 1687. First, a positively charged atom (ion) is pushed out of the engine at a high velocity. Newton’s Third Law of Motion states that for every action there is an equal and opposite reaction, so then a small force pushes back on the spacecraft in the opposite direction – forward! According to Newton’s Second Law of Motion, there is a relationship between the force (F) exerted on an object, its mass (m) and its acceleration (a). The equation F=ma describes that relationship, and tells us that the small force applied to the spacecraft by the exiting atom provides a small amount of acceleration to the spacecraft. Push enough atoms out, and you'll get enough acceleration to really speed things up.


Why is It Important?

Compared with traditional chemical rockets, ion propulsion is faster, cheaper and safer:

  • Faster: Spacecraft powered by ion engines can reach speeds of up to 90,000 meters per second (more than 201,000 mph!)
  • Cheaper: When it comes to fuel efficiency, ion engines can reach more than 90 percent fuel efficiency, while chemical rockets are only about 35 percent efficient.
  • Safer: Ion thrusters are fueled by inert gases. Most of them use xenon, which is a non-toxic, chemically inert (no risk of exploding), odorless, tasteless and colorless gas.

These properties make ion propulsion a very attractive solution when engineers are designing spacecraft. While not every spacecraft can use ion propulsion – some need greater rates of acceleration than ion propulsion can provide – the number and types of missions using these efficient engines is growing. In addition to being used on the Dawn spacecraft and communication satellites orbiting Earth, ion propulsion could be used to boost the International Space Station into higher orbits and will likely be a part of many future missions exploring our own solar system.

Teach It

Newton’s Laws of Motion are an important part of middle and high school physical science and are addressed specifically by the Next Generation Science Standards as well as Common Core Math standards. The lesson "Ion Propulsion: Using Spreadsheets to Model Additive Velocity" lets students study the relationship between force, mass and acceleration as described by Newton's Second Law as they develop spreadsheet models that apply those principles to real-world situations.

This lesson meets the following Next Generation Science and Common Core Math Standards:

NGSS Standards:

  • MS-PS2-2: Plan an investigation to provide evidence that the change in an object’s motion depends on the sum of the forces on the object and the mass of the object.
  • HS-PS2-1: Analyze data to support the claim that Newton’s second law of motion describes the mathematical relationship among the net force on a macroscopic object, its mass, and its acceleration.
  • HS-PS2-1: Use mathematical representations to support the claim that the total momentum of a system of objects is conserved when there is no net force on the system.

Common Core Math Standards:

  • Grade 8: Expressions and Equations A.4: Perform operations with numbers expressed in scientific notation, including problems where both decimal and scientific notation are used. Use scientific notation and choose units of appropriate size for measurements of very large or very small quantities (e.g., use millimeters per year for seafloor spreading). Interpret scientific notation that has been generated by technology.
  • High School: Algebra CED.A.4: Rearrange formulas to highlight a quantity of interest, using the same reasoning as in solving equations.
  • High School: Functions LE.A: Construct and compare linear, quadratic, and exponential models and solve problems.
  • High School: Functions BF.A.1: Write a function that describes a relationship between two quantities.
  • High School: Statistics and Probability ID.C: Interpret linear Models
  • High School: Number and Quantity Q.A.1: Use units as a way to understand problems and to guide the solution of multi-step problems; choose and interpret units consistently in formulas; choose and interpret the scale and the origin in graphs and data displays."

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TAGS: May the Fourth, Star Wars Day, F=ma, ion propulsion, Dawn, Deep Space 1, lesson, classroom activity, NGSS, Common Core Math

  • Lyle Tavernier
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A glowing, orange ring outlines a black hole.

In the News

Accomplishing what was previously thought to be impossible, a team of international astronomers has captured an image of a black hole’s silhouette. Evidence of the existence of black holes – mysterious places in space where nothing, not even light, can escape – has existed for quite some time, and astronomers have long observed the effects on the surroundings of these phenomena. In the popular imagination, it was thought that capturing an image of a black hole was impossible because an image of something from which no light can escape would appear completely black. For scientists, the challenge was how, from thousands or even millions of light-years away, to capture an image of the hot, glowing gas falling into a black hole. An ambitious team of international astronomers and computer scientists has managed to accomplish both. Working for well over a decade to achieve the feat, the team improved upon an existing radio astronomy technique for high-resolution imaging and used it to detect the silhouette of a black hole – outlined by the glowing gas that surrounds its event horizon, the precipice beyond which light cannot escape. Learning about these mysterious structures can help students understand gravity and the dynamic nature of our universe, all while sharpening their math skills.

How They Did It

Though scientists had theorized they could image black holes by capturing their silhouettes against their glowing surroundings, the ability to image an object so distant still eluded them. A team formed to take on the challenge, creating a network of telescopes known as the Event Horizon Telescope, or the EHT. They set out to capture an image of a black hole by improving upon a technique that allows for the imaging of far-away objects, known as Very Long Baseline Interferometry, or VLBI.

Telescopes of all types are used to see distant objects. The larger the diameter, or aperture, of the telescope, the greater its ability to gather more light and the higher its resolution (or ability to image fine details). To see details in objects that are far away and appear small and dim from Earth, we need to gather as much light as possible with very high resolution, so we need to use a telescope with a large aperture.

That’s why the VLBI technique was essential to capturing the black hole image. VLBI works by creating an array of smaller telescopes that can be synchronized to focus on the same object at the same time and act as a giant virtual telescope. In some cases, the smaller telescopes are also an array of multiple telescopes. This technique has been used to track spacecraft and to image distant cosmic radio sources, such as quasars.

More than a dozen antennas pointing forward sit on barren land surrounded by red and blue-purple mountains in the distance.

Making up one piece of the EHT array of telescopes, the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile has 66 high-precision antennas. Image credit: NRAO/AUI/NSF | + Expand image

The aperture of a giant virtual telescope such as the Event Horizon Telescope is as large as the distance between the two farthest-apart telescope stations – for the EHT, those two stations are at the South Pole and in Spain, creating an aperture that’s nearly the same as the diameter of Earth. Each telescope in the array focuses on the target, in this case the black hole, and collects data from its location on Earth, providing a portion of the EHT’s full view. The more telescopes in the array that are widely spaced, the better the image resolution.

This video shows the global network of radio telescopes in the EHT array that performed observations of the black hole in the galaxy M87. Credit: C. Fromm and L. Rezzolla (Goethe University Frankfurt)/Black Hole Cam/EHT Collaboration | Watch on YouTube

To test VLBI for imaging a black hole and a number of computer algorithms for sorting and synchronizing data, the Event Horizon Telescope team decided on two targets, each offering unique challenges.

The closest supermassive black hole to Earth, Sagittarius A*, interested the team because it is in our galactic backyard – at the center of our Milky Way galaxy, 26,000 light-years (156 quadrillion miles) away. (An asterisk is the astronomical standard for denoting a black hole.) Though not the only black hole in our galaxy, it is the black hole that appears largest from Earth. But its location in the same galaxy as Earth meant the team would have to look through “pollution” caused by stars and dust to image it, meaning there would be more data to filter out when processing the image. Nevertheless, because of the black hole’s local interest and relatively large size, the EHT team chose Sagittarius A* as one of its two targets.

An image showing a smattering of orange stars against the black backdrop of space with a small black circle in the middle and a rectangle identifying the location of the M87 black hole.

A close-up image of the core of the M87 galaxy, imaged by the Chandra X-ray Observatory. Image credit: NASA/CXC/Villanova University/J. Neilsen | + Expand image

A blue jet extends from a bright yellow point surrounded by smaller yellow stars.

This image from NASA's Hubble Space Telescope shows a jet of subatomic particles streaming from the center of M87*. Image credits: NASA and the Hubble Heritage Team (STScI/AURA) | + Expand image

The second target was the supermassive black hole M87*. One of the largest known supermassive black holes, M87* is located at the center of the gargantuan elliptical galaxy Messier 87, or M87, 53 million light-years (318 quintillion miles) away. Substantially more massive than Sagittarius A*, which contains 4 million solar masses, M87* contains 6.5 billion solar masses. One solar mass is equivalent to the mass of our Sun, approximately 2x10^30 kilograms. In addition to its size, M87* interested scientists because, unlike Sagittarius A*, it is an active black hole, with matter falling into it and spewing out in the form of jets of particles that are accelerated to velocities near the speed of light. But its distance made it even more of a challenge to capture than the relatively local Sagittarius A*. As described by Katie Bouman, a computer scientist with the EHT who led development of one of the algorithms used to sort telescope data during the processing of the historic image, it’s akin to capturing an image of an orange on the surface of the Moon.

By 2017, the EHT was a collaboration of eight sites around the world – and more have been added since then. Before the team could begin collecting data, they had to find a time when the weather was likely to be conducive to telescope viewing at every location. For M87*, the team tried for good weather in April 2017 and, of the 10 days chosen for observation, a whopping four days were clear at all eight sites!

Each telescope used for the EHT had to be highly synchronized with the others to within a fraction of a millimeter using an atomic clock locked onto a GPS time standard. This degree of precision makes the EHT capable of resolving objects about 4,000 times better than the Hubble Space Telescope. As each telescope acquired data from the target black hole, the digitized data and time stamp were recorded on computer disk media. Gathering data for four days around the world gave the team a substantial amount of data to process. The recorded media were then physically transported to a central location because the amount of data, around 5 petabytes, exceeds what the current internet speeds can handle. At this central location, data from all eight sites were synchronized using the time stamps and combined to create a composite set of images, revealing the never-before-seen silhouette of M87*’s event horizon. The team is also working on generating an image of Sagittarius A* from additional observations made by the EHT.

This zoom video starts with a view of the ALMA telescope array in Chile and zooms in on the heart of M87, showing successively more detailed observations and culminating in the first direct visual evidence of a supermassive black hole’s silhouette. Credit: ESO/L. Calçada, Digitized Sky Survey 2, ESA/Hubble, RadioAstron, De Gasperin et al., Kim et al., EHT Collaboration. Music: Niklas Falcke | Watch on YouTube

As more telescopes are added and the rotation of Earth is factored in, more of the image can be resolved, and we can expect future images to be higher resolution. But we might never have a complete picture, as Katie Bouman explains here (under “Imaging a Black Hole”).

To complement the EHT findings, several NASA spacecraft were part of a large effort to observe the black hole using different wavelengths of light. As part of this effort, NASA’s Chandra X-ray Observatory, Nuclear Spectroscopic Telescope Array (NuSTAR) and Neil Gehrels Swift Observatory space telescope missions – all designed to detect different varieties of X-ray light – turned their gaze to the M87 black hole around the same time as the EHT in April 2017. NASA’s Fermi Gamma-ray Space Telescope was also watching for changes in gamma-ray light from M87* during the EHT observations. If the EHT observed changes in the structure of the black hole’s environment, data from these missions and other telescopes could be used to help figure out what was going on.

Though NASA observations did not directly trace out the historic image, astronomers used data from Chandra and NuSTAR satellites to measure the X-ray brightness of M87*’s jet. Scientists used this information to compare their models of the jet and disk around the black hole with the EHT observations. Other insights may come as researchers continue to pore over these data.

Why It's Important

Learning about mysterious structures in the universe provides insight into physics and allows us to test observation methods and theories, such as Einstein’s theory of general relativity. Massive objects deform spacetime in their vicinity, and although the theory of general relativity has directly been proven accurate for smaller-mass objects, such as Earth and the Sun, the theory has not yet been directly proven for black holes and other regions containing dense matter.

One of the main results of the EHT black hole imaging project is a more direct calculation of a black hole’s mass than ever before. Using the EHT, scientists were able to directly observe and measure the radius of M87*’s event horizon, or its Schwarzschild radius, and compute the black hole’s mass. That estimate was close to the one derived from a method that uses the motion of orbiting stars – thus validating it as a method of mass estimation.

The size and shape of a black hole, which depend on its mass and spin, can be predicted from general relativity equations. General relativity predicts that this silhouette would be roughly circular, but other theories of gravity predict slightly different shapes. The image of M87* shows a circular silhouette, thus lending credibility to Einstein’s theory of general relativity near black holes.

An illustration of a black hole surrounded by a bright, colorful swirl of material. Text describes each part of the black hole and its surroundings.

This artist’s impression depicts a rapidly spinning supermassive black hole surrounded by an accretion disc. Image credit: ESO | + Expand image

The data also offer some insight into the formation and behavior of black hole structures, such as the accretion disk that feeds matter into the black hole and plasma jets that emanate from its center. Scientists have hypothesized about how an accretion disk forms, but they’ve never been able to test their theories with direct observation until now. Scientists are also curious about the mechanism by which some supermassive black holes emit enormous jets of particles traveling at near light-speed.

These questions and others will be answered as more data is acquired by the EHT and synthesized in computer algorithms. Be sure to stay tuned for that and the next expected image of a black hole – our Milky Way’s own Sagittarius A*.

Teach It

Capture your students’ enthusiasm about black holes by challenging them to solve these standards-aligned math problems.

Model black-hole interaction with this NGSS-aligned lesson:

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

TAGS: Black Hole, Teachable Moments, Science, K-12 Education, Teachers, Educators

  • Ota Lutz
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Illustration of spacecraft against a starry background

Update: March 15, 2019 – The answers to the 2018 NASA Pi Day Challenge are here! View the illustrated answer key


In the News

The excitement of Pi Day – and our annual excuse to chow down on pie – is upon us! The holiday celebrating the mathematical constant pi arrives on March 14, and with it comes the sixth installment of the NASA Pi Day Challenge from the Jet Propulsion Laboratory’s Education Office. This challenge gives students in grades 6-12 a chance to solve four real-world problems faced by NASA scientists and engineers. (Even if you’re done with school, they’re worth a try for the bragging rights.)

https://www.jpl.nasa.gov/edu/teach/activity/pi-in-the-sky-6/

Visit the "Pi in the Sky 6" lesson page to explore classroom resources and downloads for the 2019 NASA Pi Day Challenge. Image credit: NASA/JPL-Caltech/Kim Orr | + Expand image

Why March 14?

Pi, the ratio of a circle’s circumference to its diameter, is what is known as an irrational number. As an irrational number, its decimal representation never ends, and it never repeats. Though it has been calculated to trillions of digits, we use far fewer at NASA. In fact, 3.14 is a good approximation, which is why March 14 (or 3/14 in U.S. month/day format) came to be the date that we celebrate this mathematical marvel.

The first-known Pi Day celebration occurred in 1988. In 2009, the U.S. House of Representatives passed a resolution designating March 14 as Pi Day and encouraging teachers and students to celebrate the day with activities that teach students about pi.

The 2019 Challenge

This year’s NASA Pi Day Challenge features four planetary puzzlers that show students how pi is used at the agency. The challenges involve weathering a Mars dust storm, sizing up a shrinking storm on Jupiter, estimating the water content of a rain cloud on Earth and blasting ice samples with lasers!

›Take on the 2019 NASA Pi Day Challenge!

The Science Behind the Challenge

In late spring of 2018, a dust storm began stretching across Mars and eventually nearly blanketed the entire planet in thick dust. Darkness fell across Mars’ surface, blocking the vital sunlight that the solar-powered Opportunity rover needed to survive. It was the beginning of the end for the rover’s 15-year mission on Mars. At its height, the storm covered all but the peak of Olympus Mons, the largest known volcano in the solar system. In the Deadly Dust challenge, students must use pi to calculate what percentage of the Red Planet was covered by the dust storm.

The Terra satellite, orbiting Earth since 1999, uses the nine cameras on its Multi-Angle Imaging SpectroRadiometer, or MISR, instrument to provide scientists with unique views of Earth, returning data about atmospheric particles, land-surface features and clouds. Estimating the amount of water in a cloud, and the potential for rainfall, is serious business. Knowing how much rain may fall in a given area can help residents and first responders prepare for emergencies like flooding and mudslides. In Cloud Computing, students can use their knowledge of pi and geometric shapes to estimate the amount of water contained in a cloud.

Jupiter’s Great Red Spot, a giant storm that has been fascinating observers since the early 19th century, is shrinking. The storm has been continuously observed since the 1830s, but measurements from spacecraft like Voyager, the Hubble Space Telescope and Juno indicate the storm is getting smaller. How much smaller? In Storm Spotter, students can determine the answer to that very question faced by scientists.

Scientists studying ices found in space, such as comets, want to understand what they’re made of and how they interact and react with the environment around them. To see what molecules may form in space when a comet comes into contact with solar wind or sunlight, scientists place an ice sample in a vacuum and then expose it to electrons or ultraviolet photons. Scientists have analyzed samples in the lab and detected molecules that were later observed in space on comet 67P/Churyumov-Gerasimenko. To analyze the lab samples, an infrared laser is aimed at the ice, causing it to explode. But the ice will explode only if the laser is powerful enough. Scientist use pi to figure out how strong the laser needs to be to explode the sample – and students can do the same when they solve the Icy Intel challenge.

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Participate

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

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TAGS: Pi Day, K-12, STEM, Science, Engineering, Technology, Math, Pi, Educators, Teachers, Informal Education, Museums

  • Lyle Tavernier
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In the News

This summer, a global dust storm encircled Mars, blocking much of the vital solar energy that NASA’s Opportunity rover needs to survive. After months of listening for a signal, the agency has declared that the longest-lived rover to explore Mars has come to the end of its mission. Originally slated for a three-month mission, the Opportunity rover lived a whopping 14.5 years on Mars. Opportunity beat the odds many times while exploring the Red Planet, returning an abundance of scientific data that paved the way for future exploration.

Scientists and engineers are celebrating this unprecedented mission success, still analyzing data collected during the past decade and a half and applying lessons learned to the design of future spacecraft. For teachers, this historic mission provides lessons in engineering design, troubleshooting and scientific discovery.

How They Did It

Launched in 2003 and landed in early 2004, the twin Mars Exploration Rovers, Spirit and Opportunity, were the second spacecraft of their kind to land on our neighboring planet.

Preceded by the small Sojourner rover in 1997, Spirit and Opportunity were substantially larger, weighing about 400 pounds, or 185 kilograms, on Earth (150 pounds, or 70 kilograms, on Mars) and standing about 5 feet tall. The solar-powered rovers were designed for a mission lasting 90 sols, or Mars days, during which they would look for evidence of water on the seemingly barren planet.

Dust in the Wind

Scientists and engineers always hope a spacecraft will outlive its designed lifetime, and the Mars Exploration Rovers did not disappoint. Engineers at NASA’s Jet Propulsion Laboratory in Pasadena, California, expected the lifetime of these sun-powered robots to be limited by dust accumulating on the rovers’ solar panels. As expected, power input to the rovers slowly decreased as dust settled on the panels and blocked some of the incoming sunlight. However, the panels were “cleaned” accidentally when seasonal winds blew off the dust. Several times during the mission, power levels were restored to pre-dusty conditions. Because of these events, the rovers were able to continue their exploration much longer than expected with enough power to continue running all of their instruments.

Side-by-side images of Opportunity on Mars, showing dust on its solar panels and then relatively clean solar panels

A self-portrait of NASA's Mars Exploration Rover Opportunity taken in late March 2014 (right) shows that much of the dust on the rover's solar arrays was removed since a similar portrait from January 2014 (left). Image Credit: NASA/JPL-Caltech/Cornell Univ./Arizona State Univ. | › Full image and caption

Terrestrial Twin

To troubleshoot and overcome challenges during the rovers’ long mission, engineers would perform tests on a duplicate model of the spacecraft, which remained on Earth for just this purpose. One such instance was in 2005, when Opportunity got stuck in the sand. Its right front wheel dug into loose sand, reaching to just below its axle. Engineers and scientists worked for five weeks to free Opportunity, first using images and spectroscopy obtained by the rover’s instruments to recreate the sand trap on Earth and then placing the test rover in the exact same position as Opportunity. The team eventually found a way to get the test rover out of the sand trap. Engineers tested their commands repeatedly with consistent results, giving them confidence in their solution. The same commands were relayed to Opportunity through NASA’s Deep Space Network, and the patient rover turned its stuck wheel just the right amount and backed out of the trap that had ensnared it for over a month, enabling the mission to continue.

Engineers test moves on a model of the Opportunity rover in the In-Situ Instrument Laboratory at JPL

Inside the In-Situ Instrument Laboratory at JPL, rover engineers check how a test rover moves in material chosen to simulate some difficult Mars driving conditions. | › Full image and caption

A few years later, in 2009, Spirit wasn’t as lucky. Having already sustained some wheel problems, Spirit got stuck on a slope in a position that would not be favorable for the Martian winter. Engineers were not able to free Spirit before winter took hold, denying the rover adequate sunlight for power. Its mission officially ended in 2011. Meanwhile, despite a troubled shoulder joint on its robotic arm that first started showing wear in 2006, Opportunity continued exploring the Red Planet. It wasn’t until a dust storm completely enveloped Mars in the summer of 2018 that Opportunity finally succumbed to the elements.

The Final Act

animation showing a dust storm moving across Mars

This set of images from NASA’s Mars Reconnaissance Orbiter (MRO) shows a giant dust storm building up on Mars in 2018, with rovers on the surface indicated as icons. Image credit: NASA/JPL-Caltech/MSSS | › Full image and caption

simulated views of the sun as the 2018 dust storm darkened from Opportunity's perspective on Mars

This series of images shows simulated views of a darkening Martian sky blotting out the Sun from NASA’s Opportunity rover’s point of view in the 2018 global dust storm. Each frame corresponds to a tau value, or measure of opacity: 1, 3, 5, 7, 9, 11. Image credit: NASA/JPL-Caltech/TAMU | › Full image and caption

Dust storm season on Mars can be treacherous for solar-powered rovers because if they are in the path of the dust storm, their access to sunlight can be obstructed for months on end, longer than their batteries can sustain them. Though several dust storms occurred on Mars during the reign of the Mars Exploration Rovers, 2018 brought a large, thick dust storm that covered the entire globe and shrouded Opportunity’s access to sunlight for four months. Only the caldera of Olympus Mons, the largest known volcano in the solar system, peeked out above the dust.

The transparency or “thickness” of the dust in Mars’ atmosphere is denoted by the Greek letter tau. The higher the tau, the less sunlight is available to charge a surface spacecraft’s batteries. An average tau for Opportunity’s location is 0.5. The tau at the peak of the 2018 dust storm was 10.8. This thick dust was imaged and measured by the Curiosity Mars rover on the opposite side of the planet. (Curiosity is powered by a radioisotope thermoelectric generator.)

Since the last communication with Opportunity on June 10, 2018, NASA has sent more than 1,000 commands to the rover that have gone unanswered. Each of these commands was an attempt to get Opportunity to send back a signal saying it was alive. A last-ditch effort to reset the rover’s mission clock was met with silence.

Why It’s Important

The Mars Exploration Rovers were designed to give a human-height perspective of Mars, using panoramic cameras approximately 5 feet off the surface, while their science instruments investigated Mars’ surface geology for signs of water. Spirit and Opportunity returned more than 340,000 raw images conveying the beauty of Mars and leading to scientific discoveries. The rovers brought Mars into classrooms and living rooms around the world. From curious geologic formations to dune fields, dust devils and even their own tracks on the surface of the Red Planet, the rovers showed us Mars in a way we had never seen it before.

tracks on Mars with a patch of white soil showing

This mosaic shows an area of disturbed soil made by the Spirit rover's stuck right front wheel. The trench exposed a patch of nearly pure silica, with the composition of opal. Image credit: NASA/JPL-Caltech/Cornell | › Full image and caption

Mineral vein on the surface of Mars

This color view of a mineral vein was taken by the Mars rover Opportunity on Nov. 7, 2011. Image credit: NASA/JPL-Caltech/Cornell/ASU | › Full image and caption

The rovers discovered that Mars was once a warmer, wetter world than it is today and was potentially able to support microbial life. Opportunity landed in a crater and almost immediately discovered deposits of hematite, which is a mineral known to typically form in the presence of water. During its travels across the Mars surface, Spirit found rocks rich in magnesium and iron carbonates that likely formed when Mars was warm and wet, and sustained a near-neutral pH environment hospitable to life. At one point, while dragging its malfunctioning wheel, Spirit excavated 90 percent pure silica lurking just below the sandy surface. On Earth, this sort of silica usually exists in hot springs or hot steam vents, where life as we know it often finds a happy home. Later in its mission, near the rim of Endeavor crater, Opportunity found bright-colored veins of gypsum in the rocks. These veins likely formed when water flowed through underground fractures in the rocks, leaving calcium behind. All of these discoveries lead scientists to believe that Mars was once more hospitable to life than it is today, and they laid the groundwork for future exploration.

Imagery from the Mars Reconnaissance Orbiter and Mars Odyssey, both orbiting the Red Planet, has been combined with surface views and data from the Mars Exploration Rovers for an unprecedented understanding of the planet’s geology and environment.

Not only did Spirit and Opportunity add to our understanding of Mars, but also the rovers set the stage for future exploration. Following in their tracks, the Curiosity rover landed in 2012 and is still active, investigating the planet’s surface chemistry and geology, and confirming the presence of past water. Launching in 2020 is the next Mars rover, currently named Mars 2020. Mars 2020 will be able to analyze soil samples for signs of past microbial life. It will carry a drill that can collect samples of interesting rocks and soils, and set them aside in a cache on the surface of Mars. In the future, those samples could be retrieved and returned to Earth by another mission. Mars 2020 will also do preliminary research for future human missions to the Red Planet, including testing a method of producing oxygen from Mars’ atmosphere.

It’s thanks to three generations of surface-exploring rovers coupled with the knowledge obtained by orbiters and stationary landers that we have a deeper understanding of the Red Planet’s geologic history and can continue to explore Mars in new and exciting ways.

Teach It

Use these standards-aligned lessons and related activities to get students doing engineering, troubleshooting and scientific discovery just like NASA scientists and engineers!

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Try these related resources for students from NASA’s Space Place

TAGS: K-12 Education, Teachers, Educators, Students, Opportunity, Mars rover, Rovers, Mars, Lessons, Activities, Missions

  • Ota Lutz
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2019 Los Angeles Regional Science Bowl winners

After a full day of intense competition, a team of students from University High School in Irvine, California, earned first place in a regional round of the U.S. Department of Energy National Science Bowl on Jan. 26, 2019. This is the second consecutive year that the school has placed first in the regional round, and it's the 27th year that NASA's Jet Propulsion Laboratory in Pasadena, California, has hosted the competition.

› Read the full story on JPL News


TAGS: High School, Science Bowl, Student Competitions, Science, Events

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