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By NASA
11 Min Read Former Space Communications, Navigation Interns Pioneer NASA’s Future
Interns from the SCaN Internship Project visiting NASA's Wallops Flight Facility in Wallops Island, Virginia. Credits: NASA For over a decade, NASA’s SCaN (Space Communications and Navigation) Internship Project alumni have played important roles in extending the agency’s long-term vision for exploration. For National Intern Day on Thursday, July 25, previous program interns reflect on their journeys to and through NASA and offer advice for current and future interns.
Every summer interns join NASA’s SIP (SCaN Internship Project) program to advance the capabilities of the agency’s Deep and Near Space Networks that enable missions to communicate and navigate.
The SIP intern program develops the future workforce that will imagine, maintain, and operate the next generation of communications and navigation systems. In addition to interns’ main projects, which can range from network engineering and orbital mathematics to mission awareness campaigns and graphic design, SIP interns participate in programming that enhances their professional development and networking skills.
Justin Long
Justin Long was a SIP intern in 2017 while earning his degree in electrical engineering.
Before he applied for an internship, Long was set on working in space communications at NASA and looked out for opportunities to deepen his aerospace experience. Long attributes his work at the University of Alaska Fairbanks’ CubeSat lab for his acceptance into the intern program, as well as his university’s unique partnership with NASA.
“On my morning walks, I would pass by several of the Near Space Network ground stations operated by the Alaska Satellite Facility at the University of Alaska Fairbanks,” Long said. “At the time I was working on a ground station for our CubeSat program, so I went to intern.nasa.gov and searched anything space communications-related.”
Long was selected for a project at NASA’s Wallops Flight Facility in Virginia focused on ground station improvements to the agency’s Near Space Network. In addition to looking at hardware upgrades for NASA-owned ground stations, Long also explored opportunities to expand the network by integrating commercial and university assets.
Justin Long, 2017 SCaN Internship Project (SIP) Intern Courtesy of Justin Long Now, Long works as a telecommunications engineer at NASA Goddard, designing antennas and communication systems for spacecraft. His experience with ground stations at NASA Wallops influences his work on spacecraft today.
“Working on communications systems means figuring out what the end-to-end system for a spacecraft looks like, from the radio to the antenna,” Long said. “The internship prepared me to answer questions about how we’re transmitting the data, how fast we can transmit it, and how much data we can receive in one day.”
The major difference between his current role and his intern project is that the hardware he is developing will fly on a spacecraft rather than remain on Earth as part of a ground station antenna. Long will also test his hardware to ensure it functions as expected in orbit. The reward for this rigorous testing is the knowledge that the communications hardware he designed is a critical part of ensuring the spacecraft’s successful operation.
“There is nothing more exciting than working hands-on with a spacecraft,” Long said. “Getting to see the hardware integrated onto the spacecraft — watching the whole thing come together — is my favorite part of the job.”
While Long’s internship allowed him to come into his current position with a broader knowledge base than other engineers at his level of experience, he stresses that the networking opportunities he had with SIP were more important than the intern project itself.
“Even if you have an internship that’s not directly in your field of expertise, the opportunity to network with NASA professionals and meet different groups can have impact on your career,” Long said. “I’m still in contact with people I met as an intern.”
Thomas Montano
Thomas Montano was completing his bachelor’s degree in electrical engineering during his SIP internships in 2019 and 2020. In his current role as an electrical engineer in NASA’s Search and Rescue office at Goddard, Montano supports human spaceflight recovery efforts as well as the development of a lunar search and rescue system.
Thomas Montano during Artemis II Underway Recovery Test 10.NASA Montano was initially interested in digital signal processing and communication systems, so he decided to apply for a SCaN internship.
“It wasn’t really a contest between NASA and other internship programs,” Montano said. “I got to work on cool projects. I got to work with cool people. Goddard is just a place that makes you want to do better and learn things.”
Montano’s first internship was rewriting a software tool for running link budgets, a log of signal gains and losses in a radio communications system. In his second internship, Montano developed a virtual model of the physical transmission environment for lunar communications systems that could combine with the link budget tool to create an end-to-end communication channel simulation.
Both tools continue to be used at the agency today, though Montano’s current position has shifted his focus to the special realities of human spaceflight. Now, Montano is helping NASA test location beacons for the Artemis II astronauts. He describes meeting the Artemis crew while practicing capsule recovery on a U.S. Navy ship as an exciting and sobering reminder of the importance of his work.
“Nothing can top putting boots on the ground,” Montano said. “Meeting the crew made the work all the more real. My work isn’t hypothetical or theoretical. These are real people going to the Moon. My system cannot fail. The search and rescue system cannot go down. Failure really is not an option.”
Nothing can top putting boots on the ground. Meeting the Artemis crew mad the work all the more real.
THomas Montano
Electrical Engineer at NASA's Goddard Space Flight Center
Montano advises new interns to explore the center, ask questions, and learn how the agency works. He encourages anyone considering an internship to apply.
“The biggest reason that people don’t get NASA internships is because they don’t apply,” he said. “They count themselves out, and that’s nonsense. If you have good qualifications, go submit your résumé.”
Katrina Lee
Before becoming the engagement coordinator for NASA’s Commercialization, Innovation, and Synergies (CIS) office at Goddard, Katrina Lee was a communications intern with SIP.
For her project, Lee wrote promotional materials highlighting NASA’s then-upcoming LCRD (Laser Communications Relay Demonstration), which launched Dec. 7, 2021. The role required her to research the science behind laser communications and understand the role the technology is playing in advancing communications at NASA. The following summer, Lee applied her experience to writing and producing promotional materials for Integrated LCRD Low Earth Orbit User Modem and Amplifier Terminal (ILLUMA-T) — LCRD’s first in-space user.
When Lee first joined the program in 2021, she was planning to work in national security. Her internship experience shifted her attention to pursuing a degree in marketing and business. She also joined her student newspaper as a contributing writer.
“The project I was covering resonated with me. I learned that I was really interested in writing and communications,” said Lee. “I homed in on my interest in public-facing opportunities to share very technical information in a digestible way.”
Katrina Lee, SCaN Internship Project (SIP) Intern Summer 2021 and 2022.Courtesy of Katrina Lee In her current role, Lee applies the skills she developed as an intern to promote the Near Space Network’s commercialization opportunities. In addition to writing promotional and informational material, Lee manages event logistics, plans and guides center tours for the public and potential partners, attends conferences, and generates ideas for promoting the CIS office.
Lee’s work gives her special insight into the continuing development of the Near Space Network.
“I get to see the future of space exploration in real time,” Lee said. “There’s a greater emphasis on collaboration than we’ve seen in the past, and that collaboration is going to help space communications capabilities go further than ever before.”
When Lee reflects on what aspects of her internship were most important, she returns to the value of her work and her mentor-mentee relationship.
“I felt challenged here,” Lee said. “It was an opportunity to build confidence and learn from your mistakes beside someone who wants you to succeed. It really helped me grow as a professional.”
Lee advises new interns and students considering an internship to remember that mistakes are a valuable part of the experience. “No one at NASA expects you to know everything right away,” Lee said. “They recognize that you’re an intern and you are here to learn. This is a place where you can learn something new every day.”
Unsh Rawal
Unsh Rawal joined SIP in 2022 as a rising high school senior. He came to the program with a passion for robotics and a desire to expand his interests and try new things.
Rawal’s project contributed to the development of an interface that allows students to control robots over local and remote wireless connections. The interface is part of an educational activity for Amateur Radio on the International Space Station (ARISS) exploring telerobotics, or the distant remote control of a robot.
Unsh Rawal, SCaN Internship Project (SIP) Intern Summer 2022.Courtesy of Unsh Rawal Rawal continued to develop his project with ARISS beyond his internship. He spent the past winter porting the activity’s code to a Raspberry Pi, a palm-sized minicomputer, while broadening its functionality. His work is key to ARISS’s efforts to distribute accessible, interactive educational tools.
Rawal hopes to return to the intern program to continue his NASA project alongside his educational pursuits. While Rawal came to the intern program planning to pursue a degree in robotics, his project ignited his passion for a new field. “I learned a lot about networking, gained UI and API experience, learned about sockets,” he said. “I learned I really enjoy computer science.”
When asked to share his advice with interns new to the program, Rawal recommends scheduling regular meetings with your project mentor.
“Having consistent meetings with the people supervising the project helps you stay on track and better understand the project requirements,” Rawal said. “They’re an opportunity to learn new things from someone willing to give you one-on-one guidance.”
Lindsay White
Lindsay White was a SIP intern in 2018 and 2019 before joining NASA’s Pathways program in 2020. She completed her internship while earning her master’s degree in electrical engineering, specifically applied electromagnetics.
During her SIP internship, White programmed software-defined radios, a communication system where computer software is used to replace physical radio hardware like modulators and amplifiers, to create test benches for the development of novel signals. That internship evolved into learning more about Field Programmable Gate Arrays (FPGAs) in her second summer, a customizable hardware that can be reconfigured into different digital circuits. White then applied her FPGA knowledge to laser communications missions.
White’s first summer in the internship program confirmed that she wanted to work for NASA. “The environment is so welcoming and supportive,” she said. “People want to answer your questions and help you. I enjoyed the work I was doing and learned a ton.”
White sees a direct relationship between the work she completed as an intern and her current role as a signal analysis engineer at NASA’s Jet Propulsion Laboratory in Southern California. “The work I do now is an evolution of all the work I did as an intern. I’m applying the skills I gained by working in laser communications to my current work in radio communications.”
Lindsay White, SCaN Internship Project (SIP) Intern in 2018 and 2019.NASA White works on the digital signal processing inside the Mars Sample Return mission’s radio, as well as a research and development project called Universal Space Transponder Lite, a flexible, modular radio with a broad series of potential applications. Sometimes even she is surprised by the importance of her role to NASA’s commitment to space exploration.
“The impact is astonishing,” White said. “My work is essential to a Mars mission. Something I’m touching is going to end up on Mars.”
The impact is astonishing. My work is essential to a Mars mission. Something I'm touching is going to end up on Mars.
Lindsay White
Signal Analysis Engineer at NASA's Jet Propulsion Laboratory
White advises incoming interns to use their time in the program to develop their understanding of the agency’s personnel and projects. “SIP provides an opportunity to talk with people you otherwise wouldn’t meet,” said White. “Learning the different things NASA is working on can be even more important than hitting stretch goals on your technical project.”
White’s advice for students considering a SIP internship is straightforward: “Do it! Even if you don’t have a technical background, there’s a spot for you at NASA.”
By Korine Powers
NASA’s Goddard Space Flight Center, Greenbelt, Md.
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Last Updated Jul 25, 2024 EditorKatherine SchauerContactKatherine Schauerkatherine.s.schauer@nasa.govLocationGoddard Space Flight Center Related Terms
Space Communications & Navigation Program Communicating and Navigating with Missions Goddard Space Flight Center Space Communications Technology View the full article
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By European Space Agency
30 years ago, on 16 July 1994, astronomers watched in awe as the first of many pieces of the Shoemaker-Levy 9 comet slammed into Jupiter with incredible force. The event sparked intense interest in the field of planetary defence as people asked: “Could we do anything to prevent this happening to Earth?”
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By NASA
The Goldstone Solar System Radar, part of NASA’s Deep Space Network, made these observations of the recently discovered 500-foot-wide (150-meter-wide) asteroid 2024 MK, which made its closest approach — within about 184,000 miles (295,000 kilometers) of Earth — on June 29.NASA/JPL-Caltech The Deep Space Network’s Goldstone planetary radar had a busy few days observing asteroids 2024 MK and 2011 UL21 as they safely passed Earth.
Scientists at NASA’s Jet Propulsion Laboratory in Southern California recently tracked two asteroids as they flew by our planet. One turned out to have a little moon orbiting it, while the other had been discovered only 13 days before its closest approach to Earth. There was no risk of either near-Earth object impacting our planet, but the radar observations taken during these two close approaches will provide valuable practice for planetary defense, as well as information about their sizes, orbits, rotation, surface details, and clues as to their composition and formation.
Passing Earth on June 27 at a distance of 4.1 million miles (6.6 million kilometers), or about 17 times the distance between the Moon and Earth, the asteroid 2011 UL21 was discovered in 2011 by the NASA-funded Catalina Sky Survey, in Tucson, Arizona. But this is the first time it has come close enough to Earth to be imaged by radar. While the nearly mile-wide (1.5-kilometer-wide) object is classified as being potentially hazardous, calculations of its future orbits show that it won’t pose a threat to our planet for the foreseeable future.
Because close approaches by asteroids the size of 2024 MK are relatively rare, JPL’s planetary radar team gathered as much information about the near-Earth object as possible. This mosaic shows the spinning asteroid in one-minute increments about 16 hours after its closest approach with Earth.NASA/JPL-Caltech Using the Deep Space Network’s 230-foot-wide (70-meter) Goldstone Solar System Radar, called Deep Space Station 14 (DSS-14), near Barstow, California, JPL scientists transmitted radio waves to the asteroid and received the reflected signals by the same antenna. In addition to determining the asteroid is roughly spherical, they discovered that it’s a binary system: A smaller asteroid, or moonlet, orbits it from a distance of about 1.9 miles (3 kilometers).
“It is thought that about two-thirds of asteroids of this size are binary systems, and their discovery is particularly important because we can use measurements of their relative positions to estimate their mutual orbits, masses, and densities, which provide key information about how they may have formed,” said Lance Benner, principal scientist at JPL who helped lead the observations.
These seven radar observations by the Deep Space Network’s Goldstone Solar System Radar shows the mile-wide asteroid 2011 UL21 during its June 27 close approach with Earth from about 4 million miles away. The asteroid and its small moon (a bright dot at the bottom of the image) are circled in white.NASA/JPL-Caltech Second Close Approach
Two days later, on June 29, the same team observed the asteroid 2024 MK pass our planet from a distance of only 184,000 miles (295,000 kilometers), or slightly more than three-quarters of the distance between the Moon and Earth. About 500 feet (150 meters) wide, this asteroid appears to be elongated and angular, with prominent flat and rounded regions. For these observations, the scientists also used DSS-14 to transmit radio waves to the object, but they used Goldstone’s 114-foot (34-meter) DSS-13 antenna to receive the signal that bounced off the asteroid and came back to Earth. The result of this “bistatic” radar observation is a detailed image of the asteroid’s surface, revealing concavities, ridges, and boulders about 30 feet (10 meters) wide.
Close approaches of near-Earth objects the size of 2024 MK are relatively rare, occurring about every couple of decades, on average, so the JPL team sought to gather as much data about the object as possible. “This was an extraordinary opportunity to investigate the physical properties and obtain detailed images of a near-Earth asteroid,” said Benner.
This sunset photo shows NASA’s Deep Space Station 14 (DSS-14), the 230-foot-wide (70-meter) antenna at the Goldstone Deep Space Communications Complex near Barstow, California.NASA/JPL-Caltech The asteroid 2024 MK was first reported on June 16 by the NASA-funded Asteroid Terrestrial-impact Last Alert System (ATLAS) at Sutherland Observing Station in South Africa. Its orbit was changed by Earth’s gravity as it passed by, reducing its 3.3-year orbital period around the Sun by about 24 days. Although it is classified as a potentially hazardous asteroid, calculations of its future motion show that it does not pose a threat to our planet for the foreseeable future.
The Goldstone Solar System Radar Group is supported by NASA’s Near-Earth Object Observations Program within the Planetary Defense Coordination Office at the agency’s headquarters in Washington. Managed by JPL, the Deep Space Network receives programmatic oversight from Space Communications and Navigation program office within the Space Operations Mission Directorate, also at NASA Headquarters.
More information about planetary radar and near-Earth objects can be found at:
https://www.jpl.nasa.gov/asteroid-watch
News Media Contact
Ian J. O’Neill
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-2649
ian.j.oneill@jpl.nasa.gov
2024-097
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Last Updated Jul 03, 2024 Related Terms
Near-Earth Asteroid (NEA) Asteroids Deep Space Network Jet Propulsion Laboratory Planetary Defense Planetary Defense Coordination Office Potentially Hazardous Asteroid (PHA) Space Communications & Navigation Program Explore More
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By NASA
5 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
This artist’s concept depicts an asteroid drifting through space. Many such objects frequently pass Earth. To help prepare for the discovery of one with a chance of impacting our planet, NASA leads regular exercises to figure out how the international community could respond to such a threat.NASA/JPL-Caltech The fifth Planetary Defense Interagency Tabletop Exercise focused on an asteroid impact scenario designed by NASA JPL’s Center for Near Earth Object Studies.
A large asteroid impacting Earth is highly unlikely for the foreseeable future. But because the damage from such an event could be great, NASA leads hypothetical asteroid impact “tabletop” exercises every two years with experts and decision-makers from federal and international agencies to address the many uncertainties of an impact scenario. The most recent exercise took place this past April, with a preliminary report being issued on June 20.
Making such a scenario realistic and useful for all involved is no small task. Scientists from the Center for Near Earth Object Studies (CNEOS) at NASA’s Jet Propulsion Laboratory in Southern California, which specializes in the tracking and orbital determination of asteroids and comets and finding out if any are hazards to Earth, have played a major role in designing these exercises since the first 11 years ago.
“These hypothetical scenarios are complex and take significant effort to design, so our purpose is to make them useful and challenging for exercise participants and decision-makers to hone their processes and procedures to quickly come to a plan of action while addressing gaps in the planetary defense community’s knowledge,” said JPL’s Paul Chodas, the director of CNEOS.
The Impact Scenario
This year’s scenario: A hypothetical asteroid, possibly several hundred yards across, has been discovered, with an estimated 72% chance of impacting Earth in 14 years. Potential impact locations include heavily populated areas in North America, Southern Europe, and North Africa, but there is still a 28% chance the asteroid will miss Earth. After several months of being tracked, the asteroid moves too close to the Sun, making further observations impossible for another seven months. Decision-makers must figure out what to do.
Explore asteroids and near-Earth objects in real-time 3D Leading the exercise was NASA’s Planetary Defense Coordination Office (PDCO), the Federal Emergency Management Agency Response Directorate, and the Department of State Office of Space Affairs. Over the course of two days in April, participants gathered at the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, which hosted the event, to consider the potential national and global responses to the scenario.
“This was a very successful tabletop exercise, with nearly 100 participants from U.S. government agencies and, for the first time, international planetary defense experts,” said Terik Daly from APL, who coordinated the exercise. “An asteroid impact would have severe national and international ramifications, so should this scenario play out for real, we’d need international collaboration.”
Reality Informs Fiction
In real life, CNEOS calculates the orbit of every known near-Earth object to provide assessments of future potential impact hazards in support of NASA’s planetary defense program. To make this scenario realistic, the CNEOS team simulated all the observations in the months leading up to the exercise and used orbital determination calculations to simulate the probability of impact.
“At this point in time, the impact was likely but not yet certain, and there were significant uncertainties in the object’s size and the impact location,” said Davide Farnocchia, a navigation engineer at JPL and CNEOS, who led the design of the asteroid’s orbit. “It was interesting to see how this affected the decision-makers’ choices and how the international community might respond to a real-world threat 14 years out.”
Options to Deflect
Preparation, planning, and decision-making have been key focal points of all five exercises that have taken place over the past 11 years. For instance, could a reconnaissance spacecraft be sent to the asteroid to gather additional data on its orbit and better determine its size and mass? Would it also be feasible to attempt deflecting the asteroid so that it would miss Earth? The viability of this method was recently demonstrated by NASA’s Double Asteroid Redirection Test (DART), which impacted the asteroid moonlet Dimorphos on Sept. 26, 2022, slightly changing its trajectory. Other methods of deflection have also been considered during the exercises.
But any deflection or reconnaissance mission would need many years of preparation, requiring the use of advanced observatories capable of finding hazardous asteroids as early as possible. NASA’s Near-Earth Object Surveyor, or NEO Surveyor, is one such observatory. Managed by JPL and planned for launch in late 2027, the infrared space telescope will detect light and dark asteroids, including those that orbit near the Sun. In doing so, NEO Surveyor will support PDCO’s objectives to discover any hazardous asteroids as early as possible so that there would be more time to launch a deflection mission to potential threats.
To find out the outcome of the exercise, read NASA’s preliminary summary.
For more information about CNEOS, visit:
https://cneos.jpl.nasa.gov/
NASA Study: Asteroid’s Orbit, Shape Changed After DART Impact NASA Program Predicted Impact of Small Asteroid Over Ontario, Canada Classroom Activity: Modeling an Asteroid News Media Contacts
Ian J. O’Neill
Jet Propulsion Laboratory, Pasadena, Calif.
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ian.j.oneill@jpl.nasa.gov
Karen Fox / Charles Blue
NASA Headquarters
202-358-1600 / 202-802-5345
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2024-094
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Last Updated Jul 02, 2024 Related Terms
Asteroids NEA Scout (Near Earth Asteroid Scout) NEO Surveyor (Near-Earth Object Surveyor Space Telescope) Planetary Defense Planetary Defense Coordination Office Potentially Hazardous Asteroid (PHA) Explore More
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By NASA
6 Min Read Surprising Phosphate Finding in NASA’s OSIRIS-REx Asteroid Sample
A microscope image of a dark Bennu particle, about a millimeter long, with a crust of bright phosphate. To the right is a smaller fragment that broke off. Credits: From Lauretta & Connolly et al. (2024) Meteoritics & Planetary Science, doi:10.1111/maps.14227. Early analysis of the asteroid Bennu sample returned by NASA’s OSIRIS-REx mission has revealed dust rich in carbon, nitrogen, and organic compounds, all of which are essential components for life as we know it. Dominated by clay minerals, particularly serpentine, the sample mirrors the type of rock found at mid-ocean ridges on Earth. The magnesium-sodium phosphate found in the sample hints that the asteroid could have splintered off from an ancient, small, primitive ocean world. The phosphate was a surprise to the team because the mineral had not been detected by the OSIRIS-REx spacecraft while at Bennu. While a similar phosphate was found in the asteroid Ryugu sample delivered by JAXA’s (Japan Aerospace Exploration Agency) Hayabusa2 mission in 2020, the magnesium-sodium phosphate detected in the Bennu sample stands out for its purity (that is, the lack of other materials included in the mineral) and the size of its grains, unprecedented in any meteorite sample. Scientists have eagerly awaited the opportunity to dig into the 4.3-ounce (121.6-gram) pristine asteroid Bennu sample collected by NASA’s OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security – Regolith Explorer) mission since it was delivered to Earth last fall. They hoped the material would hold secrets of the solar system’s past and the prebiotic chemistry that might have led to the origin of life on Earth. An early analysis of the Bennu sample, published June 26 in Meteoritics & Planetary Science, demonstrates this excitement was warranted.
The OSIRIS-REx Sample Analysis Team found that Bennu contains the original ingredients that formed our solar system. The asteroid’s dust is rich in carbon and nitrogen, as well as organic compounds, all of which are essential components for life as we know it. The sample also contains magnesium-sodium phosphate, which was a surprise to the research team, because it wasn’t seen in the remote sensing data collected by the spacecraft at Bennu. Its presence in the sample hints that the asteroid could have splintered off from a long-gone, tiny, primitive ocean world.
A Phosphate Surprise
Analysis of the Bennu sample unveiled intriguing insights into the asteroid’s composition. Dominated by clay minerals, particularly serpentine, the sample mirrors the type of rock found at mid-ocean ridges on Earth, where material from the mantle, the layer beneath Earth’s crust, encounters water.
This interaction doesn’t just result in clay formation; it also gives rise to a variety of minerals like carbonates, iron oxides, and iron sulfides. But the most unexpected discovery is the presence of water-soluble phosphates. These compounds are components of biochemistry for all known life on Earth today.
A tiny fraction of the asteroid Bennu sample returned by NASA’s OSIRIS-REx mission, shown in microscope images. The top-left pane shows a dark Bennu particle, about a millimeter long, with an outer crust of bright phosphate. The other three panels show progressively zoomed-in views of a fragment of the particle that split off along a bright vein containing phosphate, captured by a scanning electron microscope.From Lauretta & Connolly et al. (2024) Meteoritics & Planetary Science, doi:10.1111/maps.14227. While a similar phosphate was found in the asteroid Ryugu sample delivered by JAXA’s (Japan Aerospace Exploration Agency) Hayabusa2 mission in 2020, the magnesium-sodium phosphate detected in the Bennu sample stands out for its purity — that is, the lack of other materials in the mineral — and the size of its grains, unprecedented in any meteorite sample.
The finding of magnesium-sodium phosphates in the Bennu sample raises questions about the geochemical processes that concentrated these elements and provides valuable clues about Bennu’s historic conditions.
“The presence and state of phosphates, along with other elements and compounds on Bennu, suggest a watery past for the asteroid,” said Dante Lauretta, co-lead author of the paper and principal investigator for OSIRIS-REx at the University of Arizona, Tucson. “Bennu potentially could have once been part of a wetter world. Although, this hypothesis requires further investigation.”
“OSIRIS-REx gave us exactly what we hoped: a large pristine asteroid sample rich in nitrogen and carbon from a formerly wet world,” said Jason Dworkin, a co-author on the paper and the OSIRIS-REx project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
From a Young Solar System
Despite its possible history of interaction with water, Bennu remains a chemically primitive asteroid, with elemental proportions closely resembling those of the Sun.
“The sample we returned is the largest reservoir of unaltered asteroid material on Earth right now,” said Lauretta.
This composition offers a glimpse into the early days of our solar system, over 4.5 billion years ago. These rocks have retained their original state, having neither melted nor resolidified since their inception, affirming their ancient origins.
Hints at Life’s Building Blocks
The team has confirmed the asteroid is rich in carbon and nitrogen. These elements are crucial in understanding the environments where Bennu’s materials originated and the chemical processes that transformed simple elements into complex molecules, potentially laying the groundwork for life on Earth.
“These findings underscore the importance of collecting and studying material from asteroids like Bennu — especially low-density material that would typically burn up upon entering Earth’s atmosphere,” said Lauretta. “This material holds the key to unraveling the intricate processes of solar system formation and the prebiotic chemistry that could have contributed to life emerging on Earth.”
What’s Next
Dozens more labs in the United States and around the world will receive portions of the Bennu sample from NASA’s Johnson Space Center in Houston in the coming months, and many more scientific papers describing analyses of the Bennu sample are expected in the next few years from the OSIRIS-REx Sample Analysis Team.
“The Bennu samples are tantalizingly beautiful extraterrestrial rocks,” said Harold Connolly, co-lead author on the paper and OSIRIS-REx mission sample scientist at Rowan University in Glassboro, New Jersey. “Each week, analysis by the OSIRIS-REx Sample Analysis Team provides new and sometimes surprising findings that are helping place important constraints on the origin and evolution of Earth-like planets.”
Launched on Sept. 8, 2016, the OSIRIS-REx spacecraft traveled to near-Earth asteroid Bennu and collected a sample of rocks and dust from the surface. OSIRIS-REx, the first U.S. mission to collect a sample from an asteroid, delivered the sample to Earth on Sept. 24, 2023.
NASA’s Goddard Space Flight Center in Greenbelt, Maryland, provided overall mission management, systems engineering, and the safety and mission assurance for OSIRIS-REx. Dante Lauretta of the University of Arizona, Tucson, is the principal investigator. The university leads the science team and the mission’s science observation planning and data processing. Lockheed Martin Space in Littleton, Colorado, built the spacecraft and provided flight operations. Goddard and KinetX Aerospace were responsible for navigating the OSIRIS-REx spacecraft. Curation for OSIRIS-REx takes place at NASA Johnson. International partnerships on this mission include the OSIRIS-REx Laser Altimeter instrument from CSA (Canadian Space Agency) and asteroid sample science collaboration with JAXA’s Hayabusa2 mission. OSIRIS-REx is the third mission in NASA’s New Frontiers Program, managed by NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington.
Find more information about NASA’s OSIRIS-REx mission at:
https://www.nasa.gov/osiris-rex
By Mikayla Mace Kelley
University of Arizona, Tuscon
News Media Contacts
Karen Fox / Erin Morton
NASA Headquarters, Washington
202-385-1287 / 202-805-9393
karen.c.fox@nasa.gov / erin.morton@nasa.gov
Rani Gran
NASA’s Goddard Space Flight Center, Greenbelt, Md.
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Last Updated Jun 26, 2024 EditorRob GarnerLocationGoddard Space Flight Center Related Terms
OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer) Asteroids Astrobiology Astromaterials Bennu Goddard Space Flight Center Johnson Space Center Planetary Science The Solar System View the full article
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