Tag: NASA

  • What Are Asteroids? (Ages 14-18)

    5 Min Read

    What Are Asteroids? (Ages 14-18)

    An asteroid

    What are asteroids?

    Asteroids are rocky objects that orbit the Sun just like planets do. In fact, sometimes asteroids are called “minor planets.” These space rocks were left behind after our solar system formed about 4.6 billion years ago.

    Asteroids are found in a wide range of sizes. For example, one small asteroid, 2015 TC25, has a diameter of about 6 feet – about the size of a small car – while the asteroid Vesta is nearly 330 miles in diameter, almost as wide as the U.S. state of Arizona. Some asteroids even have enough gravity to have one or two small moons of their own.

    There are more than a million known asteroids. Many asteroids are given names. An organization called the International Astronomical Union is responsible for assigning names to objects like asteroids and comets.

    This illustration depicts NASA's Psyche spacecraft as it approaches the asteroid Psyche.
    This illustration depicts NASA’s Psyche spacecraft as it approaches the asteroid Psyche. Once it arrives in 2029, the spacecraft will orbit the metal-rich asteroid for 26 months while it conducts its science investigation.
    NASA/JPL-Caltech/ASU

    What’s the difference between asteroids, meteors, and comets?

    Although all of these celestial bodies orbit the Sun, they are not the same. Unlike asteroids, which are rocky, comets are a mix of dust and ice. Meteors are small space rocks that get pulled close enough to enter Earth’s atmosphere, where they either burn up as a shooting star or land on the ground as a meteorite.

    What are asteroids made of?

    Different types of asteroids are composed of different mixes of materials. Most of them are made of chondrites, which are combinations of materials such as rocks and clay. These are called “C-type” asteroids. Some, called “S-type,” are made of stony materials, while “M-type” asteroids are composed of metallic elements.

    NASA’s Dawn spacecraft captured this image of Vesta as it left the giant asteroid’s orbit in 2012. The framing camera was looking down at the north pole, which is in the middle of the image.
    NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

    How did the asteroids form?

    Asteroids formed around the same time and in the same way as the planets in our solar system. A massive, dense cloud of gas and dust collapsed into a spinning disk, and the gravity in the disk’s center pulled more and more material toward it. Over time, these pieces repeatedly collided with each other, sometimes resulting in smaller fragments and other times clumping together, resulting in much bigger objects.

    Objects with a lot of mass – like planets – produced enough gravity to pull themselves into spheres, but many smaller objects didn’t. These ended up becoming comets, small moons, and, yes, asteroids. Although some asteroids have a spherical shape, most have irregular shapes – sometimes oblong, bumpy, or jagged.

    illustration depicting groupings of asteroids in the solar sytsem
    The main asteroid belt lies between Mars and Jupiter, and Trojan asteroids both lead and follow Jupiter. Scientists now know that asteroids were the original “building blocks” of the inner planets. Those that remain are airless rocks that failed to adhere to one another to become larger bodies as the solar system was forming 4.6 billion years ago.
    Credits: NASA, ESA and J. Olmsted (STScI)

    Where are asteroids found?

    Most of the asteroids we know about are located in an area called the main asteroid belt, which is found in the space between Mars and Jupiter. But asteroids are found in other parts of the solar system, too.

    Trojan asteroids orbit the Sun on the same orbital path as a planet. They’re found at two specific points on the planetary orbit called Lagrange points. At these points, the gravitational pull of the planet and the Sun are in balance, making these points gravity-neutral and stable. Many planets have been found to have Trojan asteroids, including Earth.

    An asteroid’s location can also be influenced by the gravity of planets it passes and end up pushed or pulled onto a path that brings it close to Earth. When asteroids or comets are on an orbital path that comes within 30 million miles of Earth’s orbit, we call them near-Earth objects.

    Illustration of NASA’s DART spacecraft and the Italian Space Agency’s (ASI) LICIACube, with images of the asteroids Dimorphos and Didymos obtained by the DART spacecraft.
    Credit: NASA/Johns Hopkins APL/Joshua Diaz

    Could an asteroid come close enough to hit Earth?

    Yes! Throughout history, asteroids or pieces of asteroids have collided with Earth, our Moon, and the other planets, too. The effects of some of these impacts are still visible. For example, Chicxulub Crater was created 65 million years ago when a massive asteroid struck Mexico’s Yucatan Peninsula. The resulting cloud of dust and gas released into Earth’s atmosphere blocked sunlight, leading to a mass extinction that included the dinosaurs. More recently, in 2013, people in Chelyabinsk, Russia, witnessed an asteroid almost as wide as a tennis court explode in the atmosphere above them. That event produced a powerful shockwave that caused injuries and damaged structures.

    This is why NASA’s Planetary Defense Coordination Office keeps a watchful eye on near-Earth objects. The Planetary Defense team relies on telescopes and observatories on Earth and in space to detect and monitor objects like these that could stray too close to our planet.

    The agency is working on planetary defense strategies to use if an asteroid is discovered to be heading our way. For example, NASA’s DART (Double Asteroid Redirection Test) mission in 2022 was a first-of-its-kind test: an uncrewed spacecraft with an autonomous targeting system intentionally flew into the asteroid Dimorphos, successfully changing its orbit.

    A scientist in a white coat, mask, hair net, and purple gloves holds up a clear vial with a black substance inside near the camera.
    Jason Dworkin, OSIRIS-REx mission project scientist, holds up a vial containing part of the sample from asteroid Bennu in 2023.
    Credit: NASA/James Tralie

    How does NASA study asteroids?

     NASA detects and tracks asteroids using telescopes on the ground and in space, radar observations, and computer modeling. The agency also has launched several robotic explorers to learn more about asteroids. Some missions study asteroids from above, such as the Psyche mission, launched in 2023 to study the asteroid Psyche beginning in 2029. Other missions have actually made physical contact with asteroids. For example, the DART mission mentioned above impacted an asteroid to change its orbit, and the OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification and Security – Regolith Explorer) spacecraft collected a sample of material from the surface of asteroid Bennu and delivered the sample to Earth in 2023 for scientists to study.

    Career Corner

    Want a career where you get to study asteroids? Here are some jobs at NASA that do just that:

    • Astronomer: These scientists observe and study planets, stars, and galaxies. Astronomers make discoveries that help us understand how the universe works and how it is changing. This job requires a strong educational background in science, math, and computer science.
    • Geologist: Asteroids are made of different types of rock, clay, or metallic materials. Geologists study the properties and composition of these materials to learn about the processes that have shaped Earth and other celestial bodies, like planets, moons, and asteroids.

    More About Asteroids

    Asteroid Facts
    Gallery: What’s That Space Rock?
    Center for Near Earth Object Studies
    Planetary Defense at NASA
    Asteroid Watch: Keeping an Eye on Near-Earth Objects

  • John Casani, Former Manager of Multiple NASA Missions, Dies

    6 min read

    Preparations for Next Moonwalk Simulations Underway (and Underwater)

    With Voyager 2 in the background, John Casani holds a small U.S. flag
    With Voyager 2 in the background, John Casani holds a small U.S. flag that was sewn into the spacecraft’s thermal blankets before its 1977 launch. Then Voyager’s project manager, Casani was first to envision the mission’s Golden Record, which lies before him with its cover at right.
    NASA/JPL-Caltech

    During his work on several historic missions, Casani rose through a series of technical and management positions, making an indelible mark on the nation’s space program.  

    John R. Casani, a visionary engineer who served a central role in many of NASA’s historic deep space missions, died on Thursday, June 19, 2025, at the age of 92. He was preceded in death by his wife of 39 years, Lynn Casani, in 2008 and is survived by five sons and their families.

    Casani started at the Jet Propulsion Laboratory in Southern California in 1956 and went on to work as an electronics engineer on some of the nation’s earliest spacecraft after NASA’s formation in 1958. Along with leading the design teams for both the Ranger and Mariner series of spacecraft, he held senior project positions on many of the Mariner missions to Mars and Venus, and was project manager for three trailblazing space missions: Voyager, Galileo, and Cassini.

    His work helped advance NASA spacecraft in areas including mechanical technology, system design and integration, software, and deep space communications. No less demanding were the management challenges of these multifaceted missions, which led to innovations still in use today.

    JPL's John Casani receives the National Air & Space Museum's Lifetime Achievement Award.
    JPL’s John Casani receives the National Air & Space Museum’s Lifetime Achievement Award.
    Carolyn Russo/NASM, National Air and Space Museum, Smithsonian Institution

    John had a major influence on the development of spacecraft that visited almost every planet in our solar system, as well as the people who helped build them,” said JPL director Dave Gallagher. “He played an essential role in America’s first attempts to reach space and then the Moon, and he was just as crucial to the Voyager spacecraft that marked humanity’s first foray into interplanetary — and later, interstellar — space. That Voyager is still exploring after nearly 50 years is a testament to John’s remarkable engineering talent and his leadership that enabled others to push the boundaries of possibility.”

    Born in Philadelphia in 1932, Casani studied electrical engineering at the University of Pennsylvania. After a short stint at an Air Force research lab, he moved to California in 1956 and was hired to work at JPL, a division of Caltech, on the guidance system for the U.S. Army Ballistic Missile Agency’s Jupiter-C and Sergeant missile programs.

    In 1957, the Soviet Union launched Sputnik 1, the first human-made Earth satellite, alarming America and changing the trajectory of both JPL and Casani’s career. With the 1958 launch of Explorer 1, America’s first satellite, the lab transitioned to concentrating on robotic space explorers, and Casani segued from missiles to spacecraft.

    One of his jobs as payload engineer on Pioneer 3 and 4, NASA’s first missions to the Moon, was to carry each of the 20-inch-long (51-cm-long) probes in a suitcase from JPL to the launch site at Cape Canaveral, Florida, where he installed them in the rocket’s nose cone.

    At the dawn of the 1960s, Casani served as spacecraft systems engineer for the agency’s first two Ranger missions to the Moon, then joined the Mariner project in 1965, earning a reputation for being meticulous. Four years later, he was Mariner project manager.

    Asked to share some of his wisdom in a 2009 NASA presentation, Casani said, “The thing that makes any of this work … is toughness. Toughness because this is a tough business, and it’s a very unforgiving business. You can do 1,000 things right, but if you don’t do everything right, it’ll come back and bite you.”

    Casani’s next role: project manager for NASA’s high-profile flagship mission to the outer planets and beyond — Voyager. He not only led the mission from clean room to space, he was first to envision attaching a message representing humanity to any alien civilization that might encounter humanity’s first interstellar emissaries. 

    “I approached Carl Sagan,” he said in a 2007 radio interview, “and asked him if he could come up with something that would be appropriate that we could put on our spacecraft in a way of sending a message to whoever might receive it.” Sagan took up the challenge, and what resulted was the Golden Record, a 12-inch gold-plated copper disk containing sounds and images selected to portray the diversity of life and culture on Earth.

    Once Voyager 1 and 2 and their Golden Records launched in 1977, JPL wasted no time in pointing their “engineer’s engineer” toward Galileo, which would become the first mission to orbit a gas giant planet. As the mission’s initial project manager, Casani led the effort from inception to assembly. Along the way, he had to navigate several congressional attempts to end the project, necessitating multiple visits to Washington. The 1986 loss of Space Shuttle Challenger, from which Galileo was to launch atop a Centaur upper-stage booster, led to mission redesign efforts before its 1989 launch.

    After 11 years leading Galileo, Casani became deputy assistant laboratory director for flight projects in 1988, received a promotion just over a year later and then, from 1990 to 1991, served as project manager of Cassini, NASA’s first flagship mission to orbit Saturn.

    Casani became JPL’s first chief engineer in 1994, retiring in 1999 and serving on several nationally prominent committees, including leading the investigation boards of both the Mars Climate Orbiter and the Mars Polar Lander failures, and also leading the James Webb Space Telescope Independent Comprehensive Review Panel.

    In early 2003, Casani returned to JPL to serve as project manager for NASA’s Project Prometheus, which would have been the nation’s first nuclear-powered, electric-propulsion spacecraft. In 2005, he became manager of the Institutional Special Projects Office at JPL, a position he held until retiring again in 2012.

    “Throughout his career, John reflected the true spirit of JPL: bold, innovative, visionary, and welcoming,” said Charles Elachi, JPL’s director from 2001 to 2016. “He was an undisputed leader with an upbeat, fun attitude and left an indelible mark on the laboratory and NASA. I am proud to have called him a friend.”

    Casani received many awards over his lifetime, including NASA’s Exceptional Achievement Medal, the Management Improvement Award from the President of the United States for the Mariner Venus Mercury mission, and the Air and Space Museum Trophy for Lifetime Achievement.

    News Media Contacts

    Matthew Segal / Veronica McGregor
    Jet Propulsion Laboratory, Pasadena, Calif.
    818-354-8307 / 818-354-9452
    matthew.j.segal@jpl.nasa.gov / veronica.c.mcgregor@jpl.nasa.gov

    Details

    Last Updated

    Jun 25, 2025

  • NASA to Welcome Fourth Private Astronaut Mission to Space Station

    The SpaceX Dragon spacecraft carrying the Axiom Mission 4 crew launches atop the Falcon 9 rocket from NASA's Kennedy Space Center to the International Space Station.
    The SpaceX Dragon spacecraft carrying the Axiom Mission 4 crew launches atop the Falcon 9 rocket from NASA’s Kennedy Space Center to the International Space Station.
    Credit: NASA

    As part of NASA’s efforts to expand access to space, four private astronauts are in orbit following the successful launch of the fourth all private astronaut mission to the International Space Station.

    A SpaceX Dragon spacecraft lifted off at 2:31 a.m. EDT Wednesday from Launch Complex 39A at NASA’s Kennedy Space Center in Florida, carrying Axiom Mission 4 crew members Peggy Whitson, former NASA astronaut and director of human spaceflight at Axiom Space as commander, ISRO (Indian Space Research Organisation) astronaut and pilot Shubhanshu Shukla, and mission specialists ESA (European Space Agency) project astronaut Sławosz Uznański-Wiśniewski of Poland and HUNOR (Hungarian to Orbit) astronaut Tibor Kapu of Hungary.

    “Congratulations to Axiom Space and SpaceX on a successful launch,” said NASA acting Administrator Janet Petro. “Under President Donald Trump’s leadership, America has expanded international participation and commercial capabilities in low Earth orbit. U.S. industry is enabling astronauts from India, Poland, and Hungary to return to space for the first time in over forty years. It’s a powerful example of American leadership bringing nations together in pursuit of science, discovery, and opportunity.”

    A collaboration between NASA and ISRO allowed Axiom Mission 4 to deliver on a commitment highlighted by President Trump and Indian Prime Minister Narendra Modi to send the first ISRO astronaut to the station. The space agencies are participating in five joint science investigations and two in-orbit science, technology, engineering, and mathematics demonstrations. NASA and ISRO have a long-standing relationship built on a shared vision to advance scientific knowledge and expand space collaboration.

    This mission serves as an example of the success derived from collaboration between NASA’s international partners and American commercial space companies.

    Live coverage of the spacecraft’s arrival will begin at 5 a.m., Thursday, June 26, on NASA+. Learn how to watch NASA content through a variety of platforms, including social media.

    The spacecraft is scheduled to autonomously dock at approximately 7 a.m. to the space-facing port of the space station’s Harmony module.

    Once aboard the station, Expedition 73 crew members, including NASA astronauts, Nicole Ayers, Anne McClain, and Jonny Kim, JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi, and Roscosmos cosmonauts Kirill Peskov, Sergey Ryzhikov, and Alexey Zubritsky will welcome the astronauts.

    The crew is scheduled to remain at the space station, conducting microgravity research, educational outreach, and commercial activities for about two weeks before a return to Earth and splashdown off the coast of California.

    The International Space Station is a springboard for developing a low Earth economy. NASA’s goal is to achieve a strong economy off the Earth where the agency can purchase services as one of many customers to meet its science and research objectives in microgravity. NASA’s commercial strategy for low Earth orbit provides the government with reliable and safe services at a lower cost, empowers U.S. industry, and enables the agency to focus on Artemis missions to the Moon in preparation for Mars while also continuing to use low Earth orbit as a training and proving ground for those deep space missions.

    Learn more about NASA’s commercial space strategy at:

    https://www.nasa.gov/commercial-space

    -end-

    Josh Finch
    Headquarters, Washington
    202-358-1100
    joshua.a.finch@nasa.gov

    Anna Schneider
    Johnson Space Center, Houston
    281-483-5111
    anna.c.schneider@nasa.gov

  • NASA Astronaut Zena Cardman

    NASA Astronaut Zena Cardman

    NASA astronaut Zena Cardman inspects her spacesuit’s wrist mirror at the NASA Johnson Space Center photo studio on March 22, 2024.

  • NASA Sets Coverage for Axiom Mission 4 Launch, Arrival at Station

    A white spacecraft faces the camera with its nose cone open, with Earth in the background.
    The SpaceX Dragon spacecraft carrying the Axiom Mission 3 crew is pictured approaching the International Space Station on Jan. 20, 2024.
    Credit: NASA

    NASA, Axiom Space, and SpaceX are targeting 2:31 a.m. EDT, Wednesday, June 25, for launch of the fourth private astronaut mission to the International Space Station, Axiom Mission 4.

    The mission will lift off from Launch Complex 39A at NASA’s Kennedy Space Center in Florida. The crew will travel to the orbiting laboratory on a new SpaceX Dragon spacecraft after launching on the company’s Falcon 9 rocket. The targeted docking time is approximately 7 a.m. Thursday, June 26.

    This launch opportunity comes after NASA and Roscosmos officials discussed the status of the recent repair work in the transfer tunnel at the aft (back) most segment of the orbital laboratory’s Zvezda service module. Based on the evaluations, NASA and Roscosmos agreed to further lower the pressure in the transfer tunnel to 100 millimeters of mercury, and teams will continue to evaluate going forward. Safety remains a top priority for NASA and Roscosmos.

    “NASA and Roscosmos have a long history of cooperation and collaboration on the International Space Station. This professional working relationship has allowed the agencies to arrive at a shared technical approach and now Axiom Mission 4 launch and docking will proceed,” said acting NASA Administrator Janet Petro. “We look forward to the launch with Axiom Space and SpaceX for this commercial international mission.”

    For this mission, NASA is responsible for integrated operations, which begins during the spacecraft’s approach to the space station, continues during the crew’s stay aboard the orbiting laboratory conducting science, education, and commercial activities, and concludes once the spacecraft departs the station.

    Live coverage of launch and arrival activities will stream on NASA+. Learn how to watch NASA content through a variety of platforms, including social media.

    Peggy Whitson, former NASA astronaut and director of human spaceflight at Axiom Space, will command the commercial mission, while ISRO (Indian Space Research Organisation) astronaut Shubhanshu Shukla will serve as pilot. The two mission specialists are ESA (European Space Agency) project astronaut Sławosz Uznański-Wiśniewski of Poland, and HUNOR (Hungarian to Orbit) astronaut Tibor Kapu of Hungary.

    Once docked, the private astronauts plan to spend about two weeks aboard the orbiting laboratory, conducting a mission comprised of science, outreach, and commercial activities.

    As part of a collaboration between NASA and ISRO, Axiom Mission 4 delivers on a commitment highlighted by President Donald Trump and Indian Prime Minister Narendra Modi to send the first ISRO astronaut to the station. The space agencies are participating in five joint science investigations and two in-orbit STEM (science, technology, engineering, and mathematics) demonstrations. NASA and ISRO have a long-standing relationship built on a shared vision to advance scientific knowledge and expand space collaboration.

    The private mission also carries the first astronauts from Poland and Hungary to stay aboard the International Space Station.

    NASA’s mission coverage is as follows (all times Eastern and subject to change based on real-time operations):

    Wednesday, June 25

    12:30 a.m. – Axiom Space and SpaceX launch coverage begins.

    1:40 a.m. – NASA joins the launch coverage on NASA+.

    2:31 a.m. – Launch

    NASA will end coverage following orbital insertion, which is approximately 15 minutes after launch. As it is a commercial launch, NASA will not provide a clean launch feed on its channels.

    Thursday, June 26

    5 a.m. – Arrival coverage begins on NASA+, Axiom Space, and SpaceX channels.

    7 a.m. – Targeted docking to the space-facing port of the station’s Harmony module.

    Arrival coverage will continue through hatch opening and welcome remarks.

    All times are estimates and could be adjusted based on real-time operations after launch. Follow the space station blog for the most up-to-date operations information.

    The International Space Station is a springboard for developing a low Earth economy. NASA’s goal is to achieve a strong economy off the Earth where the agency can purchase services as one of many customers to meet its science and research objectives in microgravity. NASA’s commercial strategy for low Earth orbit provides the government with reliable and safe services at a lower cost, enabling the agency to focus on Artemis missions to the Moon in preparation for Mars while also continuing to use low Earth orbit as a training and proving ground for those deep space missions.

    Learn more about NASA’s commercial space strategy at:

    https://www.nasa.gov/commercial-space

    -end-

    Joshua Finch
    Headquarters, Washington
    202-358-1100
    joshua.a.finch@nasa.gov

    Anna Schneider
    Johnson Space Center, Houston
    281-483-5111
    anna.c.schneider@nasa.gov

  • NASA Astronaut Zena Cardman

    A white woman's eye and nose are reflected in a diamond-shaped mirror attached to the wrist of her spacesuit. The mirror and white spacesuit glove are in focus, while the astronaut's blonde hair is in the foreground, out of focus.
    NASA/Josh Valcarcel

    NASA astronaut Zena Cardman inspects her spacesuit’s wrist mirror in this portrait taken at NASA’s Johnson Space Center in Houston on March 22, 2024. Cardman will launch to the International Space Station as part of NASA’s SpaceX Crew-11 mission. This will be her first spaceflight.

    Cardman was selected by NASA as a member of the 2017 “Turtles” Astronaut Class. The Virginia native holds a bachelor’s degree in biology and a master’s degree in marine sciences from the University of North Carolina, Chapel Hill. Her research focused primarily on geobiology and geochemical cycling in subsurface environments, from caves to deep sea sediments. Cardman’s experience includes multiple Antarctic expeditions. Since completing initial training, Cardman has supported real-time station operations and lunar surface exploration planning.

    This photo was one of the winners of NASA’s 2024 Photos of the Year.

  • Live or Fly a Plane in California? Help NASA Measure Ozone Pollution!

    Ozone high in the stratosphere protects us from the Sun’s ultraviolet light. But ozone near the ground is a pollutant that harms people and plants. The San Joaquin Valley has some of the most polluted air in the country, and NASA scientists with the new Ozone Where We Live (OWWL) project are working to measure ozone and other pollutants there. They need your help!  

    Do you live or work in Bakersfield, CA? Sign up to host an ozone sensor! It’s like a big lunch box that you place in your yard, but it’s not packed with tuna and crackers. It’s filled with sensors that measure temperature and humidity and sniff out dangerous gases like methane, carbon monoxide, carbon dioxide, and of course, ozone. 

    Can you fly a plane? Going to the San Joaquin Valley? Sign up to take an ozone sensor on your next flight! You can help measure ozone levels in layers of the atmosphere that are hard for satellites to investigate. Scientists will combine the data you take with data from NASA’s TEMPO satellite to improve air quality models and measurements within the region. Find out more here or email: Emma.l.yates@nasa.gov

    The Ozone Where We Live project logo, which shows a sunlit multi-story building with a small aircraft flying over it leaving a yellow contrail in a blue sky. In white letters on a blue field circling the image are the words “OWWL Ozone Where We Live.”
    Join the Ozone Where We Live (OWWL) project and help NASA scientists protect the people of the San Joaquin Valley!
    Credit: Emma Yates
  • NASA’s SLS Solid Rocket Boosters: What is DM-1?

    An infographic titled “What is DM-1” offers a detailed visual and textual breakdown of the Demonstration Motor-1 test at Northrop Grumman’s facility in Promontory, Utah. The left side features a Q&A section that explains the purpose of the event and outlines key testing objectives, such as evaluating upgraded booster components for NASA’s SLS (Space Launch System). On the right, the infographic highlights the critical role SLS boosters play during Artemis missions, emphasizing their immense thrust and engineering significance. At the bottom right, a silhouette of the state of Utah includes an arrow pinpointing the location of Promontory, visually grounding the event’s geographic setting.
    NASA/Kevin O’Brien

    Demonstration Motor-1 (DM-1) is the first full-scale ground test of the evolved five-segment solid rocket motor of NASA’s SLS (Space Launch System) rocket. The event will take place in Promontory, Utah, and will be used as an opportunity to test several upgrades made from the current solid rocket boosters. Each booster burns six tons of solid propellant every second and together generates almost eight million pounds of thrust.

    News Media Contact

    Jonathan Deal
    Marshall Space Flight Center, Huntsville, Ala. 
    256-544-0034 
    jonathan.e.deal@nasa.gov

  • Mission Accomplished! Artemis ROADS III National Challenge Competitors Celebrate their Achievements

    5 min read

    Mission Accomplished! Artemis ROADS III National Challenge Competitors Celebrate their Achievements

    The NASA Science Activation program’s Northwest Earth and Space Sciences Pathways (NESSP) team has successfully concluded the 2024–2025 Artemis ROADS III National Challenge, an educational competition that brought real NASA mission objectives to student teams (and reached more than 1,500 learners) across the country. From December 2024 through May 2025, over 300 teams of upper elementary, middle, and high school students from 22 states participated, applying STEM (Science, Technology, Engineering, and Mathematics) skills in exciting and creative ways.

    Participants tackled eight Mission Objectives inspired by NASA’s Artemis missions, which aim to return humans to the Moon. Students explored challenges such as:

    • Designing a water purification system for the Moon inspired by local water cycles
    • Developing a Moon-based agricultural plan based on experimental results
    • Programming a rover to autonomously navigate lunar tunnels
    • Engineering and refining a human-rated water bottle rocket capable of safely returning a “chip-stronaut” to Earth
    • Envisioning their future careers through creative projects like graphic novels or video interviews
    • Exploring NASA’s Artemis program through a new Artemis-themed Lotería game

    In-person hub events were hosted by Northern Arizona University, Central Washington University, and Montana State University, where teams from Washington, Montana, and Idaho gathered to present their work, collaborate with peers, and experience life on a college campus. Students also had the chance to connect virtually with NASA scientists and engineers through NESSP’s NASA Expert Talks series.

    “Artemis ROADS III is NESSP’s eighth ROADS challenge, and I have to say, I think it’s the best one yet. It’s always inspiring to see so many students across the country engage in a truly meaningful STEM experience. I heard from several students and educators that participating in the challenge completely changed their perspective on science and engineering. I believe that’s because this program is designed to let students experience the joy of discovery and invention—driven by both teamwork and personal creativity—that real scientists and engineers love about their work. We also show students the broad range of STEM expertise NASA relies on to plan and carry out a mission like Artemis. Most importantly, it gives them a chance to feel like they are part of the NASA mission, which can be truly transformative.”
     – Dr. Darci Snowden, Director, NESSP

    NESSP proudly recognizes the following teams for completing all eight Mission Objectives and the Final Challenge:

    • Space Pringles, 3rd-5th Grade, San Antonio, TX 
    • Space Axolotls, 3rd-5th Grade, Roberts, MT 
    • TEAM Wild, 6th-8th Grade, Eagle Mountain, UT 
    • Pessimistic Penguins, 6th-8th Grade, Eagle Mountain, UT 
    • Dwarf Planets, 6th-8th Grade, Eagle Mountain, UT 
    • Astronomical Rovers, 6th-8th Grade, Eagle Mountain, UT 
    • Cosmic Honeybuns, 6th-8th Grade, Eagle Mountain, UT 
    • Houston we have a Problem, 6th-8th Grade, Eagle Mountain, UT 
    • FBI Wanted List, 6th-8th Grade, Eagle Mountain, UT 
    • Lunar Legion, 6th-8th Grade, San Antonio, TX 
    • Artemis Tax-Free Space Stallions, 6th-8th Grade, Egg Harbor, NJ 
    • Aquila, 6th-8th Grade, Gooding, ID 
    • Space Warriors, 6th-8th Grade, Wapato, WA 
    • Team Cygnus, 6th-8th Grade, Red Lodge, MT 
    • Maple RocketMen, 6th-8th Grade, Northbrook, IL 
    • RGB Hawks, 6th-8th Grade, Sagle, ID 
    • The Blue Moon Bigfoots, 6th-8th Grade, Medford, OR 
    • W.E.P.Y.C.K., 6th-8th Grade, Roberts, MT 
    • Lunar Dawgz, 6th-8th Grade, Safford, AZ 
    • ROSEBUD ROCKETEERS, 6th-8th Grade, Rosebud, MT 
    • The Cosmic Titans, 6th-8th Grade, Thomson Falls, MT 
    • The Chunky Space Monkeys, 6th-8th Grade, Naches, WA 
    • ROSEBUD RED ANGUS, 9th-12th Grade, Rosebud, MT 
    • Bulky Bisons, 9th-12th Grade, Council Grove, KS 
    • The Falling Stars, 9th-12th Grade, Thomson Falls, MT 
    • The Roadkillers, 9th-12th Grade, Thomson Falls, MT 
    • The Goshawks, 9th-12th Grade, Thomson Falls, MT 
    • Sequim Cosmic Catalysts, 9th-12th Grade, Sequim, WA 
    • Spuddie Buddies, 9th-12th Grade, Moses Lake, WA 
    • Astrocoquí 2, 9th-12th Grade, Mayaguez, PR 
    • Big Sky Celestials, 9th-12th Grade, Billings, MT 
    • TRYOUTS, 9th-12th Grade, Columbus, MT 
    • Cosmonaughts, 9th-12th Grade, Columbus, MT 
    • TCCS 114, 9th-12th Grade, Tillamook, OR 
    • Marvin’s Mighty Martians, 9th-12th Grade, Simms, TX

    You can see highlights of these teams’ work in the Virtual Recognition Ceremony video on the NESSP YouTube channel. The presentation also features the teams selected to travel to Kennedy Space Center in August of 2025, the ultimate prize for these future space explorers!

    In addition to student engagement, the ROADS program provided professional development workshops and NGSS-aligned classroom resources to support K–12 educators. Teachers are invited to explore these materials and register for the next round of workshops, beginning in August 2025: https://nwessp.org/professional-development-registration.

    For more information about NESSP, its programs, partners, and the ROADS National Challenge, visit www.nwessp.org or contact info@nwessp.org.

     ———–

    NASA’s Northwest Earth and Space Science Pathways’ (NESSP) project is supported by NASA cooperative agreement award number 80NSSC22M0006 and is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn/about-science-activation/

    A water bottle rocket takes off in front of a crowd.
    A water bottle rocket launches into the air carrying its precious chip-stronaut cargo.

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    Last Updated

    Jun 23, 2025

    Editor
    NASA Science Editorial Team
  • NASA’s Curiosity Mars Rover Starts Unpacking Boxwork Formations

    5 min read

    Preparations for Next Moonwalk Simulations Underway (and Underwater)

    Drag your mouse or move your phone to pan around within this 360-degree view to explore the boxwork patterns on Mars that NASA’s Curiosity is investigating for the first time. The rover captured the 291 images that make up this mosaic between May 15 and May 18.
    Credit: NASA/JPL-Caltech/MSSS

    The rover recently drilled a sample from a new region with features that could reveal whether Mars’ subsurface once provided an environment suitable for life.

    New images from NASA’s Curiosity Mars rover show the first close-up views of a region scientists had previously observed only from orbit. The images and data being collected are already raising new questions about how the Martian surface was changing billions of years ago. The Red Planet once had rivers, lakes, and possibly an ocean. Although scientists aren’t sure why, its water eventually dried up and the planet transformed into the chilly desert it is today.

    By the time Curiosity’s current location formed, the long-lived lakes were gone in Gale Crater, the rover’s landing area, but water was still percolating under the surface­. The rover found dramatic evidence of that groundwater when it encountered crisscrossing low ridges, some just a few inches tall, arranged in what geologists call a boxwork pattern. The bedrock below these ridges likely formed when groundwater trickling through the rock left behind minerals that accumulated in those cracks and fissures, hardening and becoming cementlike. Eons of sandblasting by Martian wind wore away the rock but not the minerals, revealing networks of resistant ridges within.

    The ridges Curiosity has seen so far look a bit like a crumbling curb. The boxwork patterns stretch across miles of a layer on Mount Sharp, a 3-mile-tall (5-kilometer-tall) mountain whose foothills the rover has been climbing since 2014. Intriguingly, boxwork patterns haven’t been spotted anywhere else on the mountain, either by Curiosity or orbiters passing overhead.

    NASA’s Curiosity Mars rover viewed this low ridge on Mars
    NASA’s Curiosity Mars rover viewed this low ridge, which looks a bit like a crumbling curb, on May 16. Scientists think the hardened edges of such ridges — part of the boxwork region the rover is exploring — may have been formed by ancient groundwater.
    NASA/JPL-Caltech/MSSS

    “A big mystery is why the ridges were hardened into these big patterns and why only here,” said Curiosity’s project scientist, Ashwin Vasavada of NASA’s Jet Propulsion Laboratory in Southern California. “As we drive on, we’ll be studying the ridges and mineral cements to make sure our idea of how they formed is on target.”

    Important to the boxwork patterns’ history is the part of the mountain where they’re found. Mount Sharp consists of multiple layers, each of which formed during different eras of ancient Martian climate. Curiosity essentially “time travels” as it ascends from the oldest to youngest layers, searching for signs of water and environments that could have supported ancient microbial life.

    The rover is currently exploring a layer with an abundance of salty minerals called magnesium sulfates, which form as water dries up. Their presence here suggests this layer emerged as the climate became drier. Remarkably, the boxwork patterns show that even in the midst of this drying, water was still present underground, creating changes seen today.

    Panoramic image of Mars captured by Curiosity rover, showing a broad, rocky landscape with layered hills, eroded formations, and scattered loose stones under a hazy, reddish sky.
    NASA’s Curiosity Mars rover captured this scene while looking out across a region filled with boxwork patterns, low ridges that scientists think could have been formed by groundwater billions of years ago.
    NASA/JPL-Caltech/MSSS

    Scientists hope to gain more insight into why the boxwork patterns formed here, and Mars recently provided some unexpected clues. The bedrock between the boxwork ridges has a different composition than other layers of Mount Sharp. It also has lots of tiny fractures filled with white veins of calcium sulfate, another salty mineral left behind as groundwater trickles through rock cracks. Similar veins were plentiful on lower layers of the mountain, including one enriched with clays, but had not been spotted in the sulfate layer until now.

    “That’s really surprising,” said Curiosity’s deputy project scientist, Abigail Fraeman of JPL. “These calcium sulfate veins used to be everywhere, but they more or less disappeared as we climbed higher up Mount Sharp. The team is excited to figure out why they’ve returned now.”

    New Terrain, New Findings

    On June 8, Curiosity set out to learn about the unique composition of the bedrock in this area, using the drill on the end of its robotic arm to snag a sample of a rock nicknamed “Altadena.” The rover then dropped the pulverized sample into instruments within its body for more detailed analysis.

    Drilling additional samples from more distant boxwork patterns, where the mineral ridges are much larger, will help the mission make sense of what they find. The team will also search for organic molecules and other evidence of an ancient habitable environment preserved in the cemented ridges.

    As Curiosity continues to explore, it will be leaving a new assortment of nicknames behind, as well. To keep track of features on the planet, the mission applies nicknames to each spot the rover studies, from hills it views with its cameras to specific calcium sulfate veins it zaps with its laser. (Official names, such as Aeolis Mons — otherwise known as Mount Sharp — are approved by the International Astronomical Union.)

    The previous names were selected from local sites in Southern California, where JPL is based. The Altadena sample, for instance, bears the name of a community near JPL that was severely burned during January’s Eaton Canyon fire. Now on a new part of their Martian map, the team is selecting names from around Bolivia’s Salar de Uyuni, Earth’s largest salt flat. This exceptionally dry terrain crosses into Chile’s Atacama Desert, and astrobiologists study both the salt flat and the surrounding desert because of their similarity to Mars’ extreme dryness.

    More About Curiosity

    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 as part of NASA’s Mars Exploration Program portfolio.

    For more about Curiosity, visit:

    science.nasa.gov/mission/msl-curiosity

    News Media Contacts

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

    Karen Fox / Molly Wasser
    NASA Headquarters, Washington
    202-358-1600
    karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov

    2025-080

  • A Martian Volcano in the Mist

    Arsia Mons, one of the Red Planet’s largest volcanoes, peeks through a blanket of water ice clouds in this image captured by NASA’s 2001 Mars Odyssey orbiter on May 2, 2025.

  • A Martian Volcano in the Mist

    A black mountain peak shows through water ice clouds on Mars. Just above the clouds is the hazy green Martian atmosphere.
    NASA/JPL-Caltech/ASU

    Arsia Mons, one of the Red Planet’s largest volcanoes, peeks through a blanket of water ice clouds in this image captured by NASA’s 2001 Mars Odyssey orbiter on May 2, 2025. Odyssey used a camera called the Thermal Emission Imaging System (THEMIS) to capture this view while studying the Martian atmosphere, which appears here as a greenish haze above the scene. A large crater known as a caldera, produced by massive volcanic explosions and collapse, is located at the summit. At 72 miles (120 kilometers) wide, the Arsia Mons summit caldera is larger than many volcanoes on Earth.

    Learn more about Arsia Mons and Mars Odyssey.

    Image Credit: NASA/JPL-Caltech/ASU

  • NASA Intern Took Career from Car Engines to Cockpits

    3 min read

    Preparations for Next Moonwalk Simulations Underway (and Underwater)

    Some career changes involve small shifts. But for one NASA engineering intern, the leap was much bigger –moving from under the hood of a car to helping air taxis take to the skies.

    Saré Culbertson spent more than a decade in the auto industry and had been working as a service manager in busy auto repair shops. Today, she supports NASA’s Air Mobility Pathfinders project as a flight operations engineer intern at NASA’s Armstrong Flight Research Center in Edwards, California, through NASA’s Pathways program.

    “NASA has helped me see opportunities I didn’t even know existed

    Saré Culbertson

    Saré Culbertson

    NASA Intern

    “NASA has helped me see opportunities I didn’t even know existed,” she said. “I realized that being good at something isn’t enough – you have to be passionate about it too.”

    With a strong foundation in mechanical engineering – earning a bachelor’s degree from California State University, Long Beach, Antelope Valley Engineering Program – she graduated magna cum laude and delivered her class’s commencement speech. Culbertson also earned two associate’s degrees, one in engineering and one in fine arts.

    NASA Pathways intern, Saré Culbertson, right, wearing a dark blue shirt with a NASA meatball logo, verifies the coordinates for an Emlid Reach RS2+ receiver mounted on a black metal tripod. The equipment is cordoned off with metal stands and black tape. Bright neon green cones mark the corners and orange plastic triangular cups hang from the center of the black tape. NASA operations engineer stands to the right of Culbertson, observing the validation data on the test equipment in her right hand. They are surrounded by desert scrub and sand at NASA’s Armstrong Flight Research Center in Edwards, California on November 7, 2024.
    NASA Pathways intern Saré Culbertson, right, works with NASA operations engineer Jack Hayes at NASA’s Armstrong Flight Research Center in Edwards, California, on Nov. 7, 2024. They are verifying GPS and global navigation satellite system coordinates using Emlid Reach RS2+ receiver equipment, which supports surveying, mapping, and navigation in preparation for future air taxi test flight research.
    NASA/Genaro Vavuris

    Before making the switch to aeronautics, she worked at car dealerships and independent car repair facilities while in college. She also led quality control efforts to help a manufacturer meet international standards for quality.

    “I never thought land surveying would have anything to do with flying. But it’s a key part of supporting our research with GPS and navigation verification,” Culbertson said. “GPS measures exact positions by analyzing how long signals take to travel from satellites to ground receivers. In aviation testing, it helps improve safety by reducing signal errors and ensuring location data of the aircraft is accurate and reliable.”

    A musician since childhood, Culbertson has also performed in 21 states, playing everything from tuba to trumpet, and even appeared on HBO’s “Silicon Valley” with her tuba. She’s played in ska, punk, and reggae bands and now performs baritone in the Southern Sierra Pops Orchestra.

    Surrounded by desert scrub and sand at NASA’s Armstrong Flight Research Center in Edwards, California, NASA Pathways intern Saré Culbertson adjusts a Emlid Reach RS2+ receiver. Wearing a dark blue shirt with the NASA meatball logo, Culbertson holds the black tripod-mounted pole with a white and black receiver attached at the top. Culbertson and the equipment are encircled by black tape and bright neon green cones. Orange cone-shaped cups hang from the center of the black tape warning passersby of the equipment.
    Saré Culbertson, NASA Pathways intern at NASA’s Armstrong Flight Research Center in Edwards, California, adjusts the Emlid Reach RS2+ receiver equipment that connects with GPS and global navigation satellite systems on Nov. 7, 2024, in preparation for future air taxi test flight research.
    NASA/Genaro Vavuris

    The NASA Pathways internship, she says, changed everything. Culbertson was recently accepted into the Master of Science in Flight Test Engineering program at the National Test Pilot School, where she will be specializing in fixed wing performance and flying qualities.

    Her advice for anyone starting out?

    “Listen more than you talk,” she said. “Don’t get so focused on the next promotion that you forget to be great at the job you have now.”

    During her internship, Culbertson is making meaningful contributions toward NASA’s Urban Air Mobility research. She collects location data for test landing sites as part of the first evaluation of an experimental commercial electric vertical takeoff landing aircraft, a significant milestone in the development of next generation aviation technologies. From fixing cars to helping air taxis become a reality, Saré Culbertson is proof that when passion meets persistence, the sky isn’t the limit – it’s just the beginning.

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    Last Updated

    Jun 23, 2025

    Editor
    Dede Dinius
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    Laura Mitchell