Jump to content

NASA’s Curiosity Rover Captures a Martian Day, From Dawn to Dusk


Recommended Posts

  • Publishers
Posted

4 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Mars solar conjunction in November 2023
While stationary for two weeks during Mars solar conjunction in November 2023, NASA’s Curiosity rover used its front and rear black-and-white Hazcams to capture 12 hours of a Martian day. The rover’s shadow is visible on the surface in these images taken by the front Hazcam.

Videos from the rover show its shadow moving across the Martian surface during a 12-hour sequence while Curiosity remained parked.

When NASA’s Curiosity Mars rover isn’t on the move, it works pretty well as a sundial, as seen in two black-and-white videos recorded on Nov. 8, the 4,002nd Martian day, or sol, of the mission. The rover captured its own shadow shifting across the surface of Mars using its black-and-white Hazard-Avoidance Cameras, or Hazcams.

Instructions to record the videos were part of the last set of commands beamed up to Curiosity just before the start of Mars solar conjunction, a period when the Sun is between Earth and Mars. Because plasma from the Sun can interfere with radio communications, missions hold off on sending commands to Mars spacecraft for several weeks during this time. (The missions weren’t totally out of contact: They still radioed back regular health check-ins throughout conjunction.)

Rover drivers normally rely on Curiosity’s Hazcams to spot rocks, slopes, and other hazards that may be risky to traverse. But because the rover’s other activities were intentionally scaled back just prior to conjunction, the team decided to use the Hazcams to record 12 hours of snapshots for the first time, hoping to capture clouds or dust devils that could reveal more about the Red Planet’s weather.

When the images came down to Earth after conjunction, scientists didn’t see any weather of note, but the pair of 25-frame videos they put together do capture the passage of time. Extending from 5:30 a.m. to 5:30 p.m. local time, the videos show Curiosity’s silhouette shifting as the day moves from morning to afternoon to evening.

The first video, featuring images from the front Hazcam, looks southeast along Gediz Vallis, a valley found on Mount Sharp. Curiosity has been ascending the base of the 3-mile-tall (5-kilometer-tall) mountain, which sits in Gale Crater, since 2014.

As the sky brightens during sunrise, the shadow of the rover’s 7-foot (2-meter) robotic arm moves to the left, and Curiosity’s front wheels emerge from the darkness on either side of the frame. Also becoming visible at left is a circular calibration target mounted on the shoulder of the robotic arm. Engineers use the target to test the accuracy of the Alpha Particle X-ray Spectrometer, an instrument that detects chemical elements on the Martian surface.

In the middle of the day, the front Hazcam’s autoexposure algorithm settles on exposure times of around one-third of a second. By nightfall, that exposure time grows to more than a minute, causing the typical sensor noise known as “hot pixels” that appears as white snow across the final image.

e1-pia26209-fig-a-curiositys-hazcams-cap
Curiosity’s rear Hazcam captured the shadow of the back of the rover in this 12-hour view looking toward the floor of Gale Crater. A variety of factors caused several image artifacts, including a black speck, the distorted appearance of the Sun, and the rows of white pixels that streak out from the Sun.
NASA/JPL-Caltech

The second video shows the view of the rear Hazcam as it looks northwest down the slopes of Mount Sharp to the floor of Gale Crater. The rover’s right rear wheel is visible, along with the shadow of Curiosity’s power system. A small black artifact that appears at the left midway through the video, during the 17th frame, resulted from a cosmic ray hitting the camera sensor. Likewise, the bright flashing and other noise at the end of the video are the result of heat from the spacecraft’s power system affecting the Hazcam’s image sensor.

These images have been re-projected to correct the wide-angle lenses of the Hazcams. The speckled appearance of the images, especially prominent in the rear-camera video, is due to 11 years of Martian dust settling on the lenses.

More About the Mission

Curiosity was built by NASA’s Jet Propulsion Laboratory, which is managed by Caltech in Pasadena, California. JPL leads the mission on behalf of NASA’s Science Mission Directorate in Washington.

For more about Curiosity, visit:

http://mars.nasa.gov/msl

News Media Contacts

Andrew Good
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-2433
andrew.c.good@jpl.nasa.gov

Karen Fox / Alana Johnson
NASA Headquarters, Washington
301-286-6284 / 202-358-1501
karen.c.fox@nasa.gov / alana.r.johnson@nasa.gov

2023-189

Share

Details

Last Updated
Dec 28, 2023

View the full article

Join the conversation

You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.

Guest
Reply to this topic...

×   Pasted as rich text.   Paste as plain text instead

  Only 75 emoji are allowed.

×   Your link has been automatically embedded.   Display as a link instead

×   Your previous content has been restored.   Clear editor

×   You cannot paste images directly. Upload or insert images from URL.

  • Similar Topics

    • By NASA
      3 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      NASA’s Curiosity Mars rover sees its tracks receding into the distance at a site nicknamed “Ubajara” on April 30, 2023. This site is where Curiosity made the discovery of siderite, a mineral that may help explain the fate of the planet’s thicker ancient atmosphere.Credit: NASA/JPL-Caltech/MSSS New findings from NASA’s Curiosity Mars rover could provide an answer to the mystery of what happened to the planet’s ancient atmosphere and how Mars has evolved over time.
      Researchers have long believed that Mars once had a thick, carbon dioxide-rich atmosphere and liquid water on the planet’s surface. That carbon dioxide and water should have reacted with Martian rocks to create carbonate minerals. Until now, though, rover missions and near-infrared spectroscopy analysis from Mars-orbiting satellites haven’t found the amounts of carbonate on the planet’s surface predicted by this theory.
      Reported in an April paper in Science, data from three of Curiosity’s drill sites revealed the presence of siderite, an iron carbonate mineral, within the sulfate-rich rocky layers of Mount Sharp in Mars’ Gale Crater.
      “The discovery of abundant siderite in Gale Crater represents both a surprising and important breakthrough in our understanding of the geologic and atmospheric evolution of Mars,” said Benjamin Tutolo, associate professor at the University of Calgary, Canada, and lead author of the paper.
      To study the Red Planet’s chemical and mineral makeup, Curiosity drills three to four centimeters down into the subsurface, then drops the powdered rock samples into its CheMin instrument. The instrument, led by NASA’s Ames Research Center in California’s Silicon Valley, uses X-ray diffraction to analyze rocks and soil. CheMin’s data was processed and analyzed by scientists at the Astromaterials Research and Exploration Science (ARES) Division at NASA’s Johnson Space Center in Houston.
      “Drilling through the layered Martian surface is like going through a history book,” said Thomas Bristow, research scientist at NASA Ames and coauthor of the paper. “Just a few centimeters down gives us a good idea of the minerals that formed at or close to the surface around 3.5 billion years ago.”
      The discovery of this carbonate mineral in rocks beneath the surface suggests that carbonate may be masked by other minerals in near-infrared satellite analysis. If other sulfate-rich layers across Mars also contain carbonates, the amount of stored carbon dioxide would be a fraction of that needed in the ancient atmosphere to create conditions warm enough to support liquid water. The rest could be hidden in other deposits or have been lost to space over time.
      In the future, missions or analyses of other sulfate-rich areas on Mars could confirm these findings and help us better understand the planet’s early history and how it transformed as its atmosphere was lost.
      Curiosity, part of NASA’s Mars Exploration Program (MEP) portfolio, was built by NASA’s Jet Propulsion Laboratory, which is managed by Caltech in Pasadena, California. JPL leads the mission on behalf of NASA’s Science Mission Directorate in Washington.
      For more information on Curiosity, visit: 
      https://science.nasa.gov/mission/msl-curiosity
      News Media Contacts 
      Karen Fox / Molly Wasser 
      NASA Headquarters, Washington
      202-358-1600
      karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov 

      Andrew Good 
      Jet Propulsion Laboratory, Pasadena, Calif.
      818-393-2433
      andrew.c.good@jpl.nasa.gov
      Share
      Details
      Last Updated Apr 17, 2025 Related Terms
      Ames Research Center Astromaterials Curiosity (Rover) General Jet Propulsion Laboratory Mars Science Laboratory (MSL) Explore More
      7 min read NASA’s SpaceX 32nd Commercial Resupply Mission Overview
      NASA and SpaceX are targeting no earlier than 4:15 a.m. EDT on Monday, April 21,…
      Article 21 hours ago 6 min read NASA’s Chandra Releases New 3D Models of Cosmic Objects
      Article 24 hours ago 3 min read NASA Sees Progress on Blue Origin’s Orbital Reef Design Development
      Article 1 day ago Keep Exploring Discover Related Topics
      Curiosity Rover (MSL)
      Ames Research Center
      Mars
      Mars is the fourth planet from the Sun, and the seventh largest. It’s the only planet we know of inhabited…
      Curiosity Science Instruments
      Curiosity’s scientific instruments are the tools that bring us stunning images of Mars and ground-breaking discoveries.
      View the full article
    • By NASA
      To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
      NASA has announced the winners of it’s 31st Human Exploration Rover Challenge . The annual engineering competition – one of the agency’s longest standing student challenges – wrapped up on April 11 and April 12, at the U.S. Space & Rocket Center in Huntsville, Alabama, near NASA’s Marshall Space Flight Center. NASA NASA has announced the winning student teams in the 2025 Human Exploration Rover Challenge. This year’s competition challenged teams to design, build, and test a lunar rover powered by either human pilots or remote control. In the human-powered division, Parish Episcopal School in Dallas, Texas, earned first place in the high school division, and the Campbell University in Buies Creek, North Carolina, captured the college and university title. In the remote-control division, Bright Foundation in Surrey, British Columbia, Canada, earned first place in the middle and high school division, and the Instituto Tecnologico de Santa Domingo in the Dominican Republic, captured the college and university title.
      The annual engineering competition – one of NASA’s longest standing student challenges – wrapped up on April 11 and April 12, at the U.S. Space & Rocket Center in Huntsville, Alabama, near NASA’s Marshall Space Flight Center. The complete list of 2025 award winners is provided below:
      Human-Powered High School Division 
      First Place: Parish Episcopal School, Dallas, Texas Second Place: Ecambia High School, Pensacola, Florida Third Place: Centro Boliviano Americano – Santa Cruz, Bolivia Human-Powered College/University Division 
      First Place: Campbell University, Buies Creek, North Carolina Second Place: Instituto Tecnologico de Santo Domingo, Dominican Republic Third Place: University of Alabama in Huntsville Remote-Control Middle School/High School Division
      First Place: Bright Foundation, Surrey, British Columbia, Canada Second Place: Assumption College, Brangrak, Bangkok, Thailand Third Place: Erie High School, Erie, Colorado Remote-Control College/University Division
      First Place: Instituto Tecnologico de Santo Domingo, Dominican Republic Second Place: Campbell University, Buies Creek, North Carolina Third Place: Tecnologico de Monterey – Campus Cuernvaca, Xochitepec, Morelos, Mexico Ingenuity Award 
       Queen’s University, Kingston, Ontario, Canada Phoenix Award 
      Human-Powered High School Division: International Hope School of Bangladesh, Uttara, Dhaka, Bangladesh College/University Division: Auburn University, Auburn, Alabama Remote-Control Middle School/High School Division: Bright Foundation, Surrey, British Columbia, Canada College/University Division: Southwest Oklahoma State University, Weatherford, Oklahoma Task Challenge Award 
      Remote-Control Middle School/High School Division: Assumption College, Bangrak, Bangkok, Thailand College/University Division: Instituto Tecnologico de Santo Domingo, Dominican Republic Project Review Award 
      Human-Powered High School Division: Parish Episcopal School, Dallas, Texas College/University Division: Campbell University, Buies Creek, North Carolina Remote-Control Middle School/High School Division: Bright Foundation, Surrey, British Columbia, Canada College/University Division: Instituto Tecnologico de Santo Domingo, Dominican Republic Featherweight Award 
      Campbell University, Buies Creek, North Carolina Safety Award 
      Human-Powered High School Division: Parish Episcopal School, Dallas, Texas College/University Division: University of Alabama in Huntsville Crash and Burn Award 
      Universidad de Monterrey, Nuevo Leon, Mexico (Human-Powered Division) Team Spirit Award 
      Instituto Tecnologico de Santo Domingo, Dominican Republic (Human-Powered Division) STEM Engagement Award 
      Human-Powered High School Division: Albertville Innovation School, Albertville, Alabama College/University Division: Instituto Tecnologico de Santo Domingo, Dominican Republic Remote-Control Middle School/High School Division: Instituto Salesiano Don Bosco, Santo Domingo, Dominican Republic College/University Division: Tecnologico de Monterrey, Nuevo Leon, Mexico Social Media Award
      Human-Powered High School Division: International Hope School of Bagladesh, Uttara, Dhaka, Bangladesh College/University Division: Universidad Catolica Boliviana “San Pablo” La Paz, Bolivia Remote-Control Middle School/High School Division: ATLAS SkillTech University, Mumbai, Maharashtra, India College/University Division: Instituto Salesiano Don Bosco, Santo Domingo, Dominican Republic Most Improved Performance Award
      Human-Powered High School Division: Space Education Institute, Leipzig, Germany College/University Division: Purdue University Northwest, Hammond, Indiana Remote-Control Middle School/High School Division: Erie High School, Erie, Colorado College/University Division: Campbell University, Buies Creek, North Carolina Pit Crew Award
      Human-Powered High School Division: Academy of Arts, Career, and Technology, Reno, Nevada College/University Division: Queen’s University, Kingston, Ontario, Canada Artemis Educator Award
      Fabion Diaz Palacious from Universidad Catolica Boliviana “San Pablo” La Paz, Bolivia Rookie of the Year
      Deira International School, Dubai, United Arab Emirates

      More than 500 students with 75 teams from around the world participated in the  31st year of the competition. Participating teams represented 35 colleges and universities, 38 high schools, and two middle schools from 20 states, Puerto Rico, and 16 other nations. Teams were awarded points based on navigating a half-mile obstacle course, conducting mission-specific task challenges, and completing multiple safety and design reviews with NASA engineers. 
      NASA expanded the 2025 challenge to include a remote-control division, Remote-Operated Vehicular Research, and invited middle school students to participate. 
      “This student design challenge encourages the next generation of scientists and engineers to engage in the design process by providing innovative concepts and unique perspectives,” said Vemitra Alexander, who leads the challenge for NASA’s Office of STEM Engagement at Marshall. “This challenge also continues NASA’s legacy of providing valuable experiences to students who may be responsible for planning future space missions, including crewed missions to other worlds.”
      The rover challenge is one of NASA’s eight Artemis Student Challenges reflecting the goals of the Artemis campaign, which will land Americans on the Moon while establishing a long-term presence for science and exploration, preparing for future human missions to Mars. NASA uses such challenges to encourage students to pursue degrees and careers in the fields of science, technology, engineering, and mathematics. 
      The competition is managed by NASA’s Southeast Regional Office of STEM Engagement at Marshall. Since its inception in 1994, more than 15,000 students have participated – with many former students now working at NASA, or within the aerospace industry.    
      To learn more about the Human Exploration Rover Challenge, please visit: 
      https://www.nasa.gov/roverchallenge/home/index.html
      News Media Contact
      Taylor Goodwin
      Marshall Space Flight Center, Huntsville, Ala.
      256.544.0034
      taylor.goodwin@nasa.gov
      View the full article
    • By NASA
      Explore Hubble Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts e-Books Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 2 min read
      Hubble Captures a Star’s Swan Song
      This NASA/ESA Hubble Space Telescope image features the planetary nebula Kohoutek 4-55. ESA/Hubble & NASA, K. Noll The swirling, paint-like clouds in the darkness of space in this stunning image seem surreal, like a portal to another world opening up before us. In fact, the subject of this NASA/ESA Hubble Space Telescope image is very real. We are seeing vast clouds of ionized atoms and molecules, thrown into space by a dying star. This is a planetary nebula named Kohoutek 4-55, a member of the Milky Way galaxy situated just 4,600 light-years away in the constellation Cygnus (the Swan).
      Planetary nebulae are the spectacular final display at the end of a giant star’s life. Once a red giant star has exhausted its available fuel and shed its last layers of gas, its compact core will contract further, enabling a final burst of nuclear fusion. The exposed core reaches extremely hot temperatures, radiating ultraviolet light that energizes the enormous clouds of gas cast off by the star. The ultraviolet light ionizes atoms in the gas, making the clouds glow brightly. In this image, red and orange indicate nitrogen, green is hydrogen, and blue shows oxygen. Kohoutek 4-55 has an uncommon, multi-layered form: a faint layer of gas surrounds a bright inner ring, all wrapped in a broad halo of ionized nitrogen. The spectacle is bittersweet, as the brief phase of fusion in the core will end after only tens of thousands of years, leaving a white dwarf that will never illuminate the clouds around it again.
      This image itself was also the final work of one of Hubble’s instruments: the Wide Field and Planetary Camera 2 (WFPC2). Installed in 1993 to replace the original Wide Field and Planetary Camera, WFPC2 was responsible for some of Hubble’s most enduring images and fascinating discoveries. Hubble’s Wide Field Camera 3 replaced WFPC2 in 2009, during Hubble’s final servicing mission. A mere ten days before astronauts removed Hubble’s WFPC2 from the telescope, the instrument collected the data used in this image: a fitting send-off after 16 years of discoveries. Image processors used the latest and most advanced processing techniques to bring the data to life one more time, producing this breathtaking new view of Kohoutek 4-55.
      Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Share








      Details
      Last Updated Apr 10, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
      Hubble Space Telescope Astrophysics Astrophysics Division Emission Nebulae Goddard Space Flight Center Nebulae Planetary Nebulae Stars The Universe Keep Exploring Discover More Topics From Hubble
      Hubble Space Telescope


      Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.


      The Death Throes of Stars


      From colliding neutron stars to exploding supernovae, Hubble reveals new details of  some of the mysteries surrounding the deaths of…


      Exploring the Birth of Stars


      Seeing ultraviolet, visible, and near-infrared light helps Hubble uncover the mysteries of star formation.


      Hubble’s Nebulae


      View the full article
    • By NASA
      6 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      This mosaic showing the Martian surface outside of Jezero Crater was taken by NASA’s Perseverance on Dec. 25, 2024, at the site where the rover cored a sample dubbed “Silver Mountain” from a rock likely formed during Mars’ earliest geologic period.NASA/JPL-Caltech/ASU/MSSS The diversity of rock types along the rim of Jezero Crater offers a wide glimpse of Martian history.
      Scientists with NASA’s Perseverance rover are exploring what they consider a veritable Martian cornucopia full of intriguing rocky outcrops on the rim of Jezero Crater. Studying rocks, boulders, and outcrops helps scientists understand the planet’s history, evolution, and potential for past or present habitability. Since January, the rover has cored five rocks on the rim, sealing samples from three of them in sample tubes. It’s also performed up-close analysis of seven rocks and analyzed another 83 from afar by zapping them with a laser. This is the mission’s fastest science-collection tempo since the rover landed on the Red Planet more than four years ago.
      Perseverance climbed the western wall of Jezero Crater for 3½ months, reaching the rim on Dec. 12, 2024, and is currently exploring a roughly 445-foot-tall (135-meter-tall) slope the science team calls “Witch Hazel Hill.” The diversity of rocks they have found there has gone beyond their expectations.
      “During previous science campaigns in Jezero, it could take several months to find a rock that was significantly different from the last rock we sampled and scientifically unique enough for sampling,” said Perseverance’s project scientist, Katie Stack Morgan of NASA’s Jet Propulsion Laboratory in Southern California. “But up here on the crater rim, there are new and intriguing rocks everywhere the rover turns. It has been all we had hoped for and more.”
      One of Perseverance’s hazard cameras captured the rover’s coring drill collecting the “Main River” rock sample on “Witch Hazel Hill” on March 10, 2025, the 1,441st Martian day, or sol, of the mission. NASA/JPL-Caltech That’s because Jezero Crater’s western rim contains tons of fragmented once-molten rocks that were knocked out of their subterranean home billions of years ago by one or more meteor impacts, including possibly the one that produced Jezero Crater. Perseverance is finding these formerly underground boulders juxtaposed with well-preserved layered rocks that were “born” billions of years ago on what would become the crater’s rim. And just a short drive away is a boulder showing signs that it was modified by water nestled beside one that saw little water in its past.
      Oldest Sample Yet?
      Perseverance collected its first crater-rim rock sample, named “Silver Mountain,” on Jan. 28. (NASA scientists informally nickname Martian features, including rocks and, separately, rock samples, to help keep track of them.) The rock it came from, called “Shallow Bay,” most likely formed at least 3.9 billion years ago during Mars’ earliest geologic period, the Noachian, and it may have been broken up and recrystallized during an ancient meteor impact.
      About 360 feet (110 meters) away from that sampling site is an outcrop that caught the science team’s eye because it contains igneous minerals crystallized from magma deep in the Martian crust. (Igneous rocks can form deep underground from magma or from volcanic activity at the surface, and they are excellent record-keepers — particularly because mineral crystals within them preserve details about the precise moment they formed.) But after two coring attempts (on Feb. 4 and Feb. 8) fizzled due to the rock being so crumbly, the rover drove about 520 feet (160 meters) northwest to another scientifically intriguing rock, dubbed “Tablelands.”
      Data from the rover’s instruments indicates that Tablelands is made almost entirely of serpentine minerals, which form when large amounts of water react with iron- and magnesium-bearing minerals in igneous rock. During this process, called serpentinization, the rock’s original structure and mineralogy change, often causing it to expand and fracture. Byproducts of the process sometimes include hydrogen gas, which can lead to the generation of methane in the presence of carbon dioxide. On Earth, such rocks can support microbial communities.
      Coring Tablelands went smoothly. But sealing it became an engineering challenge.
      Sealing the “Green Gardens” sample — collected by NASA’s Perseverance Mars rover from a rock dubbed “Tablelands” along the rim of Jezero Crater on Feb. 16, 2025 — pre-sented an engineering challenge. The sample was finally sealed on March 2.NASA/JPL-Caltech/ASU/MSSS Flick Maneuver
      “This happened once before, when there was enough powdered rock at the top of the tube that it interfered with getting a perfect seal,” said Kyle Kaplan, a robotics engineer at JPL. “For Tablelands, we pulled out all the stops. Over 13 sols,” or Martian days, “we used a tool to brush out the top of the tube 33 times and made eight sealing attempts. We even flicked it a second time.”
      During a flick maneuver, the sample handling arm — a little robotic arm in the rover’s belly — presses the tube against a wall inside the rover, then pulls the tube away, causing it to vibrate. On March 2, the combination of flicks and brushings cleaned the tube’s top opening enough for Perseverance to seal and store the serpentine-laden rock sample. 
      Eight days later, the rover had no issues sealing its third rim sample, from a rock called “Main River.” The alternating bright and dark bands on the rock were like nothing the science team had seen before.
      Up Next
      Following the collection of the Main River sample, the rover has continued exploring Witch Hazel Hill, analyzing three more rocky outcrops (“Sally’s Cove,” “Dennis Pond,” and “Mount Pearl”). And the team isn’t done yet.  
      “The last four months have been a whirlwind for the science team, and we still feel that Witch Hazel Hill has more to tell us,” said Stack. “We’ll use all the rover data gathered recently to decide if and where to collect the next sample from the crater rim. Crater rims — you gotta love ’em.”
      More About Perseverance
      A key objective for Perseverance’s mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover is characterizing the planet’s geology and past climate, to help pave the way for human exploration of the Red Planet and is the first mission to collect and cache Martian rock and regolith.
      NASA’s Mars Sample Return Program, in cooperation with ESA (European Space Agency), is designed to send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis.
      The Mars 2020 Perseverance mission is part of NASA’s Mars Exploration Program portfolio and the agency’s Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.
      NASA’s Jet Propulsion Laboratory, managed for the agency by Caltech in Pasadena, California, built and manages operations of the Perseverance rover.
      For more about Perseverance:
      https://science.nasa.gov/mission/mars-2020-perseverance
      News Media Contacts
      DC Agle
      Jet Propulsion Laboratory, Pasadena, Calif.
      818-393-9011
      agle@jpl.nasa.gov
      Karen Fox / Molly Wasser
      NASA Headquarters, Washington
      202-358-1600
      karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov  
      2025-051
      Share
      Details
      Last Updated Apr 10, 2025 Related Terms
      Perseverance (Rover) Mars Mars 2020 Explore More
      5 min read Perseverance Rover Witnesses One Martian Dust Devil Eating Another
      Article 7 days ago 6 min read How NASA’s Perseverance Is Helping Prepare Astronauts for Mars
      Article 2 weeks ago 6 min read NASA’s Curiosity Rover Detects Largest Organic Molecules Found on Mars
      Lee esta historia en español aquí. Researchers analyzing pulverized rock onboard NASA’s Curiosity rover have found…
      Article 2 weeks ago Keep Exploring Discover Related Topics
      Missions
      Humans in Space
      Climate Change
      Solar System
      View the full article
    • By European Space Agency
      This new snapshot from the European Space Agency’s Mars Express deftly captures the two distinct faces of Mars: ridged and rugged versus smooth and unmarked.
      View the full article
  • Check out these Videos

×
×
  • Create New...