40 Years Ago: STS-41D – First Space Shuttle Launch Pad Abort

40 Years Ago: STS-41D – First Space Shuttle Launch Pad Abort

In 1983, NASA received delivery of Discovery, the third space qualified vehicle in the agency’s space shuttle fleet. During the launch attempt for the STS-41D mission on June 26, 1984, Discovery’s onboard computers halted the countdown four seconds before liftoff, and after two of its main engines had already ignited. The six astronauts safely egressed the orbiter. This first on-the-pad abort of the shuttle program required the vehicle’s return to its assembly building for replacement of the faulty engine that caused the shutdown. The resulting two-month delay caused a shuffling of the mission’s payloads, but Discovery finally lifted off on Aug. 30, and the astronauts completed a successful six-day mission, deploying three commercial satellites, testing a new solar array, and conducting a commercial biotechnology experiment.

Space shuttle Discovery rolls out of Rockwell’s Palmdale facility Discovery atop the Shuttle Carrier Aircraft during the cross-country ferry flight Discovery arrives at NASA’s Kennedy Space Center in Florida
Left: Space shuttle Discovery rolls out of Rockwell’s Palmdale facility. Middle: Discovery atop the Shuttle Carrier Aircraft during the cross-country ferry flight. Right: Discovery arrives at NASA’s Kennedy Space Center in Florida.

Discovery rolled out of Rockwell International’s plant in Palmdale, California, on Oct. 16, 1983. Five of the six crew members assigned to its first flight attended the ceremony. Workers trucked Discovery overland from Palmdale to NASA’s Dryden, now Armstrong, Flight Research Center at Edwards Air Force Base (AFB). Discovery arrived at NASA’s Kennedy Space Center (KSC) on Nov. 9 after a cross-country ferry flight from Edwards, following a two-day stopover at Vandenberg Air Force, now Space Force, Base in California, atop the Shuttle Carrier Aircraft, a modified Boeing 747. Discovery, named after several historical ships of exploration, incorporated manufacturing lessons learned from the first orbiters as well as through the use of more advanced materials. The new vehicle weighed nearly 8,000 pounds less than its sister ship Columbia and 700 pounds less than Challenger.

The STS-41D crew patch The STS-41D crew of R. Michael “Mike” Mullane, front row left, Steven A. Hawley, Henry W. “Hank” Hartsfield, and Michael D. Coats; and Charles D. Walker, back row left, and Judith A. Resnik
Left: The STS-41D crew patch. Right: The STS-41D crew of R. Michael “Mike” Mullane, front row left, Steven A. Hawley, Henry W. “Hank” Hartsfield, and Michael D. Coats; and Charles D. Walker, back row left, and Judith A. Resnik.

To fly Discovery’s first flight, originally designated STS-12 and later renamed STS-41D, in February 1983 NASA assigned Commander Henry W. Hartsfield, a veteran of STS-4, and first-time flyers Pilot Michael L. Coats, and Mission Specialists R. Michael Mullane, Steven A. Hawley, and Judith A. Resnik, all from the 1978 class of astronauts. In May 1983, NASA announced the addition of Charles D. Walker, an employee of the McDonnell Douglas Corporation, to the crew, flying as the first commercial payload specialist. He would operate the company’s Continuous Flow Electrophoresis System (CFES) experiment. The mission’s primary payloads included the Leasat-1 (formerly known as Syncom IV-1) commercial communications satellite and OAST-1, three experiments from NASA’s Office of Aeronautics and Space Technology, including the Solar Array Experiment, a 105-foot long lightweight deployable and retractable solar array.

Workers in the Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center in Florida lift Discovery to mate it with its external tank and solid rocket boosters Initial rollout of Discovery from the VAB to Launch Pad 39A on May 19, 1984 The Flight Readiness Firing on June 2
Left: Workers in the Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center in Florida lift Discovery to mate it with its external tank and solid rocket boosters. Middle: Initial rollout of Discovery from the VAB to Launch Pad 39A on May 19, 1984. Right: The Flight Readiness Firing on June 2.

The day after its arrival at KSC, workers towed Discovery from the SLF to the Orbiter Processing Facility (OPF) to being preparing it for its first space flight. Between Dec. 9, 1983, and Jan. 10, 1984, it entered temporary storage in the Vehicle Assembly Building (VAB) to allow postflight processing of Columbia in the OPF following STS-9. Workers returned Discovery to the OPF for final processing, towing it to the VAB on May 12 for mating with its External Tank (ET) and Solid Rocket Boosters (SRBs). The completed stack rolled out to Launch Pad 39A on May 19. On June 2, engineers successfully completed an 18-second Flight Readiness Firing of the shuttle main engines. Post test inspections revealed a debonding of a thermal shield in main engine number 1’s combustion chamber, requiring its replacement at the pad. The work pushed the planned launch date back three days to June 25.

The June 26 launch abort Discovery’s three main engines hours after the launch abort
Left: The June 26 launch abort. Right: Discovery’s three main engines hours after the launch abort.

The failure of the shuttle’s backup General Purpose Computer (GPC) caused a one-day delay of the first launch attempt on June 25. On June 26, the countdown proceeded smoothly and at T minus 6.6 seconds the orbiter’s GPCs began the serial ignition sequence of the three main engines. Normally, the three engines ignite at 0.12-second intervals to ease stress on the system and to allow onboard computers to diagnose any problems. Engines number 2 and 3, forming the base of the triangle closest to the body flap, ignited as planned, but engine number 1 at the apex of the triangle and nearest the vertical tail, did not ignite at all. This caused the Redundant Set Launch Sequencer (RSLS) to shut the two working engines down, calling an abort to the countdown at T minus 4 seconds. To ease the tension, Hawley reportedly said, “Gee, I thought we’d be a little higher at main engine cutoff.” The fact that engine number 1 had never ignited caused some momentary confusion as displays showed that the RSLS had not shut it down. A single engine still burning with the shuttle still on the pad would have led to a disaster. Once controllers and the onboard crew realized what had actually happened, they calmed down somewhat. What no one realized at the time is that a hydrogen fire, invisible to the naked eye, had broken out at the aft end of the orbiter. Had the crew evacuated at that time, they would have run through the invisible flames. The pad’s fire suppression system came on to deal with the fire, and when the crew did finally egress the shuttle, they received a good dousing of water. The crew returned safely, if a little drenched, to crew quarters. After ground teams assessed the cause of the abort, they made the decision to roll the stack back to the VAB, demate Discovery from the ET and SRBs and tow it back to the OPF. Workers replaced the faulty engine, and Discovery rolled back out to the launch pad on Aug. 9 for another launch attempt 20 days later, delayed by one day due to a software issue, and finally on Aug. 30, Discovery roared off its launch pad on a pillar of flame and within 8 minutes, NASA’s newest orbiter reached low Earth orbit.

Gemini VI launch pad abort in December 1965 Gemini VI crew of Thomas P. Stafford, left, and Walter M. Schirra
Left: Gemini VI launch pad abort in December 1965. Right: Gemini VI crew of Thomas P. Stafford, left, and Walter M. Schirra.

Although the first on the pad abort of the space shuttle program, the June 1984 attempt to launch Discovery on STS-41D represented the second such incident in the American human spaceflight program. The dubious honor of the first on the pad abort belongs to Gemini VI. On Dec. 12, 1965, astronauts Walter M. Schirra and Thomas P. Stafford strapped into the spacecraft for their second launch attempt to rendezvous with Gemini VII. The countdown clock ticked down to zero, and the Titan-II rocket’s first stage engines ignited. And shut off after just 1.2 seconds. Although the mission clock aboard the spacecraft had started, the rocket had not lifted off, and Schirra made the split-second decision not to eject himself and Stafford from the spacecraft. Engineers later traced the cause of the abort to a dust cap inadvertently left in the engine compartment. After workers took care of that issue, Schirra and Stafford tried to launch again on Dec. 15, and the third time proved to be the charm. 

STS-51F in August 1985 STS-55 in March 1993 STS-51 in August 1993 STS-68 in August 1994
Four space shuttle on-the-pad aborts. STS-51F in August 1985, left, STS-55 in March 1993, STS-51 in August 1993, and STS-68 in August 1994.

In the 10 years following the June 1984 abort, four additional shuttle launch attempts ended with an RSLS abort after at least one main engine had ignited.

July 12, 1985, STS-51F space shuttle Challenger

The RSLS executed a shutdown at T minus 3 seconds, after all three main engines had ignited, because the number two main engine’s chamber coolant valve did not close as rapidly as needed for startup. Investigations revealed a faulty sensor as the real culprit, and workers replaced it at the pad. Challenger launched successfully on July 29, but during ascent engine number 1 shut down, the only inflight failure of a main engine, resulting in the only abort to orbit of the program. Although the shuttle achieved a slightly lower than planned orbit, the mission met most of its science objectives.

March 22, 1993, STS-55 space shuttle Columbia

Following a trouble-free countdown, Columbia’s three main engines came to life at as planned, but three seconds later, the RSLS shut them all down when it detected that engine number 3 had not come up to full power. A tiny fragment of rubber caused a valve in the liquid oxygen system to leak, preventing the engine from fully starting. Columbia borrowed three main engines from Endeavour, and STS-55 took off on April 26 to carry out its German Spacelab-D2 mission.

Aug. 12, 1993, STS-51 space shuttle Discovery

After a trouble-free preflight processing and countdown, Discovery’s three main engines ignited as planned at T minus 6.6 seconds. Three seconds later, all three engines shut down. Investigation revealed the cause as a faulty sensor that monitors fuel flow through main engine number 2. Workers replaced all three engines at the pad, and Discovery took off on Sept. 12 to carry out its mission.

Aug. 18, 1994, STS-68 space shuttle Endeavour

Following a smooth countdown, Endeavour’s three main engines began their startup sequence at T minus 6.6 seconds. The GLS computers detected a problem with the No. 3 main engine’s High Pressure Oxidizer Turbine. One of its sensors detected a dangerously high discharge temperature, exceeding the rules of the Launch Commit Criteria, and Endeavour’s computers halted the countdown a mere 1.9 seconds before liftoff. Workers rolled Endeavour back to the VAB, replacing its three main engines with ones borrowed from Atlantis. STS-68 finally took off on Sept. 30 and successfully completed its radar mapping mission. NASA astronaut Daniel W. Bursch holds the distinction as the only person to have experienced two on-the-pad aborts, as he served as a mission specialist on both STS-51 and STS-68.

The lessons learned from these on-the-pad abort experiences can inform current and future programs. For example, the Space Launch System (SLS) uses main engines leftover from the space shuttle program to power its booster stage. And operationally, other launcher systems can learn from these experiences and safely manage similar future events.

Read recollections of the STS-41D mission by Hartsfield, Coats, Mullane, Hawley, and Walker in their oral histories with the JSC History Office.

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Kelli Mars

Detective Work Enables Perseverance Team to Revive SHERLOC Instrument

Detective Work Enables Perseverance Team to Revive SHERLOC Instrument

5 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Imagery captured by a navigation camera aboard NASA’s Perseverance rover on Jan. 23 shows the position of a cover on the SHERLOC instrument. The cover had become stuck several weeks earlier but the rover team has since found a way to address the issue so the instrument can continue to operate.
NASA/JPL-Caltech

After six months of effort, an instrument that helps the Mars rover look for potential signs of ancient microbial life has come back online.

The SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals) instrument aboard NASA’s Perseverance Mars rover has analyzed a rock target with its spectrometer and camera for the first time since encountering an issue this past January. The instrument plays a key role in the mission’s search for signs of ancient microbial life on Mars. Engineers at NASA’s Jet Propulsion Laboratory in Southern California confirmed on June 17 that the instrument succeeded in collecting data.

“Six months of running diagnostics, testing, imagery and data analysis, troubleshooting, and retesting couldn’t come with a better conclusion,” said SHERLOC principal investigator Kevin Hand of JPL.

Position of a cover on the SHERLOC instrument
Imagery captured by a navigation camera aboard NASA’s Perseverance rover on Jan. 23 shows the position of a cover on the SHERLOC instrument. The cover had become stuck several weeks earlier but the rover team has since found a way to address the issue so the instrument can continue to operate.
NASA/JPL-Caltech

Mounted on the rover’s robotic arm, SHERLOC uses two cameras and a laser spectrometer to search for organic compounds and minerals in rocks that have been altered in watery environments and may reveal signs of past microbial life. On Jan. 6, a movable lens cover designed to protect the instrument’s spectrometer and one of its cameras from dust became frozen in a position that prevented SHERLOC from collecting data.

Analysis by the SHERLOC team pointed to the malfunction of a small motor responsible for moving the protective lens cover as well as adjusting focus for the spectrometer and the Autofocus and Context Imager (ACI) camera. By testing potential solutions on a duplicate SHERLOC instrument at JPL, the team began a long, meticulous evaluation process to see if, and how, the lens cover could be moved into the open position.

SHERLOC instrument’s Autofocus and Context Imager to capture this image of its calibration target
Perseverance’s team used the SHERLOC instrument’s Autofocus and Context Imager to capture this image of its calibration target on May 11 to confirm an issue with a stuck lens cover had been resolved. A silhouette of the fictional detective Sherlock Holmes is at the center of the target.
NASA/JPL-Caltech

SHERLOC Sleuthing

Among many other steps taken, the team tried heating the lens cover’s small motor, commanding the rover’s robotic arm to rotate the SHERLOC instrument under different orientations with supporting Mastcam-Z imagery, rocking the mechanism back and forth to loosen any debris potentially jamming the lens cover, and even engaging the rover’s percussive drill to try jostling it loose. On March 3, imagery returned from Perseverance showed that the ACI cover had opened more than 180 degrees, clearing the imager’s field of view and enabling the ACI to be placed near its target.

“With the cover out of the way, a line of sight for the spectrometer and camera was established. We were halfway there,” said Kyle Uckert, SHERLOC deputy principal investigator at JPL. “We still needed a way to focus the instrument on a target. Without focus, SHERLOC images would be blurry and the spectral signal would be weak.”

Like any good ophthalmologist, the team set about figuring out SHERLOC’s prescription. Since they couldn’t adjust the focus of the instrument’s optics, they relied on the rover’s robotic arm to make minute adjustments in the distance between SHERLOC and its target in order to get the best image resolution. SHERLOC was commanded to take pictures of its calibration target so that the team could check the effectiveness of this approach.

NASA’s Perseverance rover gathering data on the “Walhalla Glades” abrasion
This image of NASA’s Perseverance rover gathering data on the “Walhalla Glades” abrasion was taken in the “Bright Angel” region of Jezero Crater by one of the rover’s front hazard avoidance cameras on June 14. The WATSON camera on the SHERLOC instrument is closest to the Martian surface.
NASA/JPL-Caltech

“The rover’s robotic arm is amazing. It can be commanded in small, quarter-millimeter steps to help us evaluate SHERLOC’s new focus position, and it can place SHERLOC with high accuracy on a target,” said Uckert. “After testing first on Earth and then on Mars, we figured out the best distance for the robotic arm to place SHERLOC is about 40 millimeters,” or 1.58 inches. “At that distance, the data we collect should be as good as ever.”

Confirmation of that fine positioning of the ACI on a Martian rock target came down on May 20. The verification on June 17 that the spectrometer is also functional checked the team’s last box, confirming that SHERLOC is operational.

“Mars is hard, and bringing instruments back from the brink is even harder,” said Perseverance project manager Art Thompson of JPL. “But the team never gave up. With SHERLOC back online, we’re continuing our explorations and sample collection with a full complement of science instruments.”

Perseverance is in the later stages of its fourth science campaign, looking for evidence of carbonate and olivine deposits in the “Margin Unit,” an area along the inside of Jezero Crater’s rim. On Earth, carbonates typically form in the shallows of freshwater or alkaline lakes. It’s hypothesized that this also might be the case for the Margin Unit, which formed over 3 billion years ago.

 

More About the Mission

A key objective of Perseverance’s mission on Mars is astrobiology, including caching samples that may contain signs of ancient microbial life. The rover will characterize the planet’s geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith.

Subsequent NASA missions, in cooperation with ESA (European Space Agency), would 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 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, which is managed for the agency by Caltech, built and manages operations of the Perseverance rover.

For more about Perseverance:

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 / Charles Blue
NASA Headquarters
202-385-1600 / 202-802-5345
karen.c.fox@nasa.gov / charles.e.blue@nasa.gov

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Jun 26, 2024

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Anthony Greicius

NOAA’s GOES-U Satellite Launches

NOAA’s GOES-U Satellite Launches

Looking down a runway, we see clouds of vapor billowing outward as a rocket takes off. A black tower structure called the gantry is on the left of the rocket's flames, and further in the distance on the right is a white water tower.
SpaceX

A SpaceX Falcon Heavy rocket with the National Oceanic and Atmospheric Administration’s GOES-U (Geostationary Operational Environmental Satellite) satellite lifts off from NASA’s Kennedy Space Center in Florida on June 25, 2024. GOES-U is the fourth and final satellite in the current series of advanced weather satellites; it will provide continuous coverage of weather and hazardous environmental conditions across much of the Western Hemisphere.

In addition to its critical role in predicting weather on Earth, the GOES series of satellites helps forecasters predict space weather near Earth that can interfere with satellite electronics, GPS, and radio communications. The GOES-U satellite has a new space weather instrument, the Compact Coronograph-1, which blocks the Sun’s bright light so scientists can observe the relatively fainter solar atmosphere.

GOES-U will take about two weeks to reach geostationary orbit. Once there, the satellite will be renamed GOES-19. Follow GOES-U’s journey.

Image Credit: SpaceX

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Monika Luabeya

NASA Advances Research to Grow Habitats in Space from Fungi

NASA Advances Research to Grow Habitats in Space from Fungi

Bricks produced using mycelium, yard waste and wood chips as a part of the myco-architecture project. Similar materials could be used to build habitats on the Moon or Mars.
Credits: NASA

As NASA prepares for long-duration missions to the Moon and Mars for the benefit of all, a habitat-growing concept selected Wednesday by the agency could help “grow” homes using fungi for future explorers. A team of researchers at NASA Ames Research Center in California’s Silicon Valley will receive new funding under the NASA’s Innovative Advanced Concepts (NIAC) program to propel their habitat research.

The Phase III NIAC award will provide $2 million over two years to continue technology development of the Mycotecture Off Planet project in preparation for a potential future demonstration mission. The work is led by Lynn Rothschild, a senior research scientist at NASA Ames.

“As NASA prepares to explore farther into the cosmos than ever before, it will require new science and technology that doesn’t yet exist” said NASA Administrator Bill Nelson. “NASA’s space technology team and the NIAC program unlock visionary ideas – ideas that make the impossible, possible. This new research is a steppingstone to our Artemis campaign as we prepare to go back to the Moon to live, to learn, to invent, to create – then venture to Mars and beyond.”

Some habitats, such as landers and rovers, will be delivered to planetary surfaces. However, the mycotecture project team is developing technologies that could “grow” habitats on the Moon, Mars, and beyond using fungi and the underground threads that comprise the main part of fungi, known as mycelia. With this development, explorers could travel with a compact habitat built out of lightweight material containing dormant fungi. By adding water, fungi can potentially grow around that framework into a fully functional human habitat, while being safely contained to avoid contaminating the environment.

“We are committed to advancing technologies to transport our astronauts, house our explorers, and facilitate valuable research,” said Walt Engelund, associate administrator for Programs in the Space Technology Mission Directorate at NASA Headquarters in Washington. “We invest in these technologies throughout their lifecycle, recognizing their potential to help us accomplish our goals – benefiting industry, our agency, and humanity.”

The mycotecture project could enable a new, multi-use material for in-space construction, reducing mass and saving resources for additional mission priorities. The proof of concept for this technology was demonstrated through earlier NIAC awards. The team created multiple combinations of fungal-based biocomposites, fabricated prototypes, tested materials in a planetary simulator, evaluated enhancements including incorporating radiation protection, and drafted detailed mycelium-based Moon habitat designs. This project also has uses on Earth in addition to applications on other worlds. Mycelia could be used for water filtration and systems that extract minerals from wastewater.

From deep space human exploration to advanced propulsion and robotics, NASA aims to change the possible by supporting early-stage space technology research that could radically change the future.

“Mycotecture Off Planet exemplifies how advanced concepts can change how we envision future exploration missions,” said John Nelson, NIAC Program Executive. “As NASA embarks on the next era of space exploration, NIAC helps the agency lay the necessary groundwork to bring innovative visions to life.”

Work under the Phase III award will allow the research team to optimize material properties. It also will enable the team to progress toward testing in low Earth orbit. Future applications of this project could include integration into commercial space stations or infusion into missions to the Moon with the ultimate goal of use on Mars.

NASA Innovative Advanced Concepts supports visionary, early-stage research ideas through multiple progressive phases of study. In January 2024, NASA announced 19 Phase I and Phase II proposal selections. NASA’s Space Technology Mission Directorate, which is responsible for developing the new cross-cutting technologies and capabilities the agency needs to achieve its current and future missions, funds NIAC activities.

For more information about NASA’s investments in space technology, visit:

https://www.nasa.gov/space-technology-mission-directorate

-end-

Jasmine Hopkins
Headquarters, Washington
202-358-1600
jasmine.s.hopkins@nasa.gov

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Tiernan P. Doyle

Surprising Phosphate Finding in NASA’s OSIRIS-REx Asteroid Sample

Surprising Phosphate Finding in NASA’s OSIRIS-REx Asteroid Sample

6 Min Read

Surprising Phosphate Finding in NASA’s OSIRIS-REx Asteroid Sample

Mineral fragment from OSIRIS-REx's asteroid Bennu sample, seen against a black background. The pieces are predominantly gray, with notable light blue hues flecked throughout. The biggest fragment, triangular, is about a millimeter on a side.

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, Tucson

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.
301-332-6975
rani.c.gran@nasa.gov

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Rob Garner