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!

Explore More

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

Pi in the Sky 2 Infographic

UPDATE - March 16, 2015: The pi challenge answer key is now available for download.

In honor of the "Pi Day of the Century" (3/14/15), the Education Office at NASA's Jet Propulsion Laboratory has crafted another stellar math challenge to show students of all ages how NASA scientists and engineers use the mathematical constant pi.

The 2015 problem set -- available as a web infographic and printable handouts -- features four real-world, NASA math problems for students in grades 4 through 11, including: calculating the dizzying number of times a Mars rover's wheels have rotated in 11 years; finding the number of images it will take the Dawn spacecraft to map the entire surface of the dwarf planet Ceres (the first dwarf planet to be explored); learning the potential volume of water on Jupiter's moon Europa; and discovering what fraction of a radio beam from our most distant spacecraft reaches Earth.

The word problems, which were crafted by NASA/JPL education specialists with the help of scientists and engineers, give students insight into the real calculations space explorers use every day and a chance to see some of the real-world applications of the math they're learning in school.

"Pi in the Sky 2" Downloads:

TAGS: Pi Day, Infographics, Mars Rover, Dawn, Ceres, Europa, Voyager, K-12

  • Kim Orr

Jason Carlton, Andrew Crawford and Scott Maxwell

At one point, a large potato-sized rock became embedded in the Mars rover Spirit's wheel, rendering it useless until it could somehow be removed. The team was able to use this facility and test a "pop a wheelie" move, which helped the team navigating through the problem in style! (From left: Jason Carlton, Andrew Crawford and Scott Maxwell). Image credit: NASA/JPL-Caltech

To help set the stage for this special blog post, it seems fitting to start with a great piece of advice given to me by Scott Maxwell, a Mars rover driver at NASA's Jet Propulsion Laboratory: "There will come a time, possibly more than once, but at least once, where you feel like you simply can't go on -- you're too tired, it's too hard. When that happens, go on. You can do it. You can do it."

An enormous sense of dedication had already become abundantly clear by the time I sent out an email request to interview the team that drives the rovers on Mars. I received the immediate response of "yes!" at 3:45 a.m. from an enthusiastic Scott Maxwell - who clearly not only loves his job, but also loves sharing it with others. I instantly recognized his name and was eager to see if he was the same engaging "voice of Mars" who I had seen in so many NASA stories. As it turned out, he was not only gracious and helpful in lining up the interview, but he was also passionate about sharing his work with others.

After making an entrance up two floors and badge access doors, we were happily greeted by the same Scott who I had pictured, smiling from ear to ear, as well as a room full of rover drivers who he had arranged for me to interview. It was a tremendous surprise and delight, as I looked around the room and instantly recognized a few of the faces from television and various NASA documentaries.

Andrew with the Mars Exploration Rover Team
Not only were we to meet many of the Mars rover drivers, but also it would later turn out that we were fortunate enough to talk with some of the software developers and original founders of the Mars Exploration Rover project. (From left: Paolo Bellutta, Brian Cooper, Vandi Verma, Jason Carlton, Scott Maxwell, Andrew Crawford and John Wright). Image credit: NASA/JPL-Caltech

Scott is the poster child for being passionate about something and making it happen. From an early age, he wanted to explore far-off worlds, and he worked hard to make those dreams come true. Scott's dedication and brilliance has helped in developing much of the software, operating procedures and commands that are used for the rovers on Mars today. (I encourage you to watch the charismatic interviews Scott has done on the Mars rovers and JPL as well as check out his ongoing five-year blog about his adventures with the Mars rovers at:

Within a matter of minutes, Scott brought us up to speed on a brief history of Mars, the rovers and other expeditions NASA has sent and will send to the Red Planet. It was immediately clear that Scott lives, eats and breathes rover driving. The way he explained the technicalities and details of the Martian missions and rovers with such precision, spot-on memory and passion, made me feel as though I was part of this exclusive group of brilliant individuals.

One of the faces in the room I instantly recognized was rover driver Vandi Verma, whose interesting background and childhood story I had seen on television. I remembered how passionate she was about robotics from an early age. When she completed all the schooling and learning she could in her native India, she set her sights on the United States to get the education and experience that would take her to the pinnacle of robotics: working with and driving rovers on Mars. She went through the citizenship process necessary to work for the U.S. government all while earning her Doctorate and pursing top-level robotics research until being hired by JPL for flight operations with the Mars Exploration Rover project. (For a fascinating look at her history, read her bio.) I had no idea I would be lucky enough to interview Vandi, let alone receive a behind-the-scenes tour of what she was working on.

She showed us a detailed 3D contour map of the Martian landscape and Husband Hill, a legendary Martian landform for Mars Exploration Rover drivers. She had been re-driving the particularly challenging and difficult terrain of Husband Hill -- which took the Mars rover Spirit a full year to successfully climb in 2005 -- in preparation for the arrival of the rover Opportunity at a similar feature called the Highlands. All the while, Vandi's fingers seemed to navigate the keyboard with lightning speed, entering commands that exposed breathtaking images and grids of the Martian terrain.

Andrew with the Mars Exploration Rover Team
It was Husband Hill -- which is named in remembrance of Rick Husband, the commander of NASA's Space Shuttle Columbia -- that took the Mars rover Spirit a full year to successfully and triumphantly climb in 2005. The rover made groundbreaking scientific discoveries all along the way. (From left: Jason Carlton, Vandi Verma, Chris Leger and Andrew Crawford). Image credit: NASA/JPL-Caltech

Sitting directly beside her was another face that I instantly recognized from years of following Mars exploration missions. Chris Leger, a youthful, hip-looking and brilliant member of the team who's responsible for some of Mars robotics and space-robotics most significant advancements and undertakings. Chris was part of the original driving team that took Spirit up Husband Hill's incredibly challenging 30-degree, boulder-laden slopes; he also does his own bouldering and climbing here on Earth twice a week. (For a mind-blowing description of all he's done, visit: )

We were joined by even more legendary rover drivers, and the room was alive with varying generations of drivers and programmers reaching back to the days of NASA's Mars Pathfinder mission. The conversation was in full swing.

The moment seemed fitting to ask if the team had ever seen anything strange that made the hair rise on the back of their necks, and if so, what did they do? One of the gentlemen seated at the table wearing a big smile, shorts and a cool Hawaiian shirt, spoke up about a strange event involving what looked like a "white rabbit" on the surface of Mars. I listened intently to John Wright, an engaging and cool dude who used to work at Hughes Aircraft, founded by one of my personal favorite heroes and explorers, Howard Hughes.

John drove Spirit for six years and is one of the five developers of the software that the rover drivers use to build command sequences and visualize and rehearse the rovers' activities. He tells great stories, including this one about the "white rabbit." He said one day an image came through from Spirit showing a feature that looked an awful lot like a white rabbit in the distance, and in the preceding pictures, it was gone! The group immediately called up a team of engineers and scientists to examine the finding. It was later concluded that the "white rabbit" was simply a small piece of fabric from the rover's atmospheric descent landing bags that had blown past in the wind. It was a story and lesson that the whole team could relate to with many adding that they feel as though they've earned a degree in geology because they can now quickly identify rocks or anomalies, know what to steer clear of and avoid, and what to investigate.

We said goodbye to Chris and Vandi as they were late for a meeting, which I could only imagine was highly technical and dealt with strategically planning future movements for billion-dollar spacecraft. We were then joined by two more rover drivers coming straight from the driving room. It seemed that once again, Scott had gone a step above in rallying all the troops for this interview, and I couldn't seem to stop smiling. Paolo Bellutta and Khaled Ali wcgere just as charismatic and enthusiastic as the rest of the team, and instantly, they started sharing stories that had us on the edge of our seats.

Paolo's introduction said it all: "My name is Paolo, and I am from Italy, and please no jokes about driving." The room erupted. What followed was a mesmerizing story about a treacherous navigation next to an 80 meter cliff in Victoria Crater on Mars with Paolo at the helm. Due to the estimations of the terrain combined with the long response time of sending and receiving data and commands between Earth and Mars, there was a period when Paolo had to wait in utter silence wondering if a valuable supplier of otherworldly exploration and knowledge had gone off the radar ... Then, after a grueling two-hour silence, the images and data started to appear again with huge relief.

Paolo's story triggered a conversation on safety parameter software programs, which are always evolving and incorporated into rover planning and mission architecture -- usually written and constructed by the drivers and planners themselves. Little did I know that seated at our table, quiet but insightful, was Brian Cooper, who was one of the original software developers and Mars Exploration Rover mission architects. He was also responsible for hiring most of the drivers there with us that day. He said that at the beginning of the Mars rover missions, it was difficult to know exactly what terrain and routes were secure and what parameters to observe. But over time, the parameter software development and safety autonomy programs have been getting better and better, incorporating gridlines with built-in "keep-out zones" and danger-sensing abilities.

Next, we heard from rover driver Khaled Ali, whose personal background made me want to never stop learning. While listening to Khaled explain how he eventually landed a job as a rover driver, Scott interjected excitedly saying, "Khaled sometimes goes off and takes on other jobs around JPL, such as building test-beds for testing Moonrise, stuff like that. And we always welcome him back with open arms!" This resonates as a prime example of the collaborative, never-stop-learning attitude that seems to be especially prevalent within this team and at JPL.

The last of the usual five rover driving meetings per day was about to begin, and Scott suggested we boogie to the command room and catch the tail end of the meeting. As we walked into the room -- "quiet as mice," per Scott's advice -- the first thing I saw was a table laden with coffee, computers, papers and many of the same people that were just in the other room with us discussing various commands and undecipherable software language displayed on a screen up front. Scott whispered to us that they were reviewing the day's planned movements and trajectory for the rover Opportunity. Every day there are multiple meetings and checks, then double checks, ensuring that the scientific goals, safety parameters and command sequences are exactly on target to provide 100 percent safety and redundancy for the mission. Paolo and John were stationed at computers typing what appeared to my eyes as a foreign language and discussing and answering questions from all angles of the room. We exited the room as it was clear they were in the midst of highly technical planning. And my mentor Jason and I just smile at each other like little kids in a candy store.

Just when I didn't think my brain could absorb any more, Scott had more adventures and stops planned for us, including another room where Bubba, a full-size replica of a Mars Exploration Rover (like the twin rovers Spirit and Opportunity) was located. Scott gave us such a detailed breakdown of the rover components and functionalities that I felt like a VIP with a backstage pass.

Andrew with the Mars Exploration Rover Team
The suspension I'm marveling at here was designed by my mentor's mentor, Don Bickler, and it really hits home what a tight-knit, cooperative and dedicated group exists here at JPL. Image credit: NASA/JPL-Caltech

Our last stop was the rover testing facility, located in a building specially designed with soil and rocks mimicking Martian terrain and housing full-size, functional rovers. The Planetary Science Summer School group was taking a tour and peering down at the rovers through the glass as we walked in. Within seconds Scott had the full attention of the group and was telling them stories. It wasn't long before he was convincing the whole group to join us downstairs inside the testing room. There was no stopping Scott then, and to the sheer delight of the group, as well as myself, we saw a green light flash on the badge reader and heard the door click open: access granted! Three feet in front of me, in the soil, was where the very engineers, scientists, drivers, and programmers who are responsible for the rovers do their testing!

One of the group-members asked Scott what his "Free Spirit!" shirt meant and he explained that after six years of what was planned as a three-month mission, Spirit had become trapped in a very fine soil, granular sediment, which is much like powder. And making things more difficult was the fact that only four of her six wheels could help in the exit strategy. After months of testing and brainstorming right in that very room, using those very rovers, they were unable to free Spirit from her Martian trap. She lost her ability to align her solar panels with the sun, and after a long winter, the signal was lost.

Andrew, Jason and Scott
Scott explains how the driving team used this facility to test strategies for freeing the Mars rover Spirit from her Martian trap, while a model of the next Mars rover, Curiosity, looks primed for exploration in the background. Image credit: NASA/JPL-Caltech

The loss of Spirit, however, in no way marks the end a continually busy schedule for Scott, Vandi, Chris, Paolo, John, Brian and Khaled. In fact, the team just celebrated the arrival of Spirit's twin rover, Opportunity, at Endeavor crater after a three-year trek across the Red Planet. It's a major milestone for the Mars Exploration Rover mission and one that will continue the Mars rovers' amazing history of discovery.

We said goodbye to Scott and expressed our gratitude as best we could. I couldn't help but think that he and his team are some of JPL's most valuable assets, and I blurted it out as Scott crossed the street, like a little kid cheering for his favorite team. He laughed, smiled and swiped his badge, entering another world.

TAGS: Rover Driver, Mars Rover, Engineering, Science

  • Andrew Crawford