35 Years Ago: STS-32 Returns the Long Duration Exposure Facility

35 Years Ago: STS-32 Returns the Long Duration Exposure Facility

On Jan. 9, 1990, space shuttle Columbia took off on its ninth flight, STS-32, from NASA’s Kennedy Space Center (KSC) in Florida. Its five-person crew of Commander Daniel Brandenstein, Pilot James Wetherbee, and Mission Specialists Bonnie Dunbar, Marsha Ivins, and David Low flew a then record-breaking 11-day mission to deploy the Syncom IV-F5 communications satellite for the U.S. Navy and retrieve the Long-Duration Exposure Facility (LDEF). Astronauts aboard a shuttle mission in 1984 deployed the LDEF and scientists eagerly awaited the return of their 57 experiments to study the effects of nearly six years exposure to the low Earth orbit environment. The crew also conducted several middeck experiments in biotechnology and materials processing and used an echocardiograph to study changes in their hearts. 

In November 1988, NASA announced Brandenstein, Wetherbee, Dunbar, Ivins, and Low as the STS-32 crew for the flight then planned for November 1989. Brandenstein, from the Class of 1978, had flown twice before, as pilot on STS-8 in August-September 1983 and commander of STS-51G in June 1985. Dunbar, selected in 1980, had flown once before on STS-61A in October-November 1985. For Wetherbee, Ivins, and Low, all selected in 1984, STS-32 marked their first spaceflight. During the second day of their planned 10-day mission, the astronauts would deploy the Syncom IV-F5, also known as Leasat-5, communications satellite for the U.S. Navy. The main focus of the flight involved the retrieval of LDEF, deployed by the STS-41C crew in April 1984. The original plan had LDEF, containing 57 science and technology experiments, retrieved by the STS-51D crew in February 1985. Delays in the shuttle program first pushed the retrieval to STS-61I in September 1986, and then the Challenger accident delayed it to STS-32. The facility ended up staying in orbit nearly six years instead of the originally intended 10 months. The crew rounded out the mission by conducting a series of middeck science and medical experiments. 

Columbia returned to KSC on Aug. 21, 1989, following STS-28’s landing at Edwards Air Force Base (AFB) in California, and workers towed it to the Orbiter Processing Facility (OPF) the next day. They made 26 modifications to the orbiter, including the installation of the Remote Manipulator System (RMS), or robotic arm, and a fifth set of liquid hydrogen and liquid oxygen tanks to extend the vehicle’s duration in space. Rollover to the nearby Vehicle Assembly Building took place on Nov. 16, where Columbia joined its External Tank and twin Solid Rocket Boosters (SRB) on refurbished Mobile Launch Platform 3, last used in 1975. Rollout took place on Nov. 28 to Launch Pad 39A, newly refurbished since its previous launch in 1986.  

On Dec. 1, engineers and the astronaut crew completed the Terminal Countdown Demonstration Test, a dress rehearsal for the planned Dec. 18 launch. Based on that date and the mission’s planned 10-day duration, the STS-32 crew would have spent Christmas in space, only the third American crew and the first space shuttle crew to do so. However, unfinished work on Pad 39A delayed the launch into January 1990. Trajectory specialists had estimated that due to orbital decay, LDEF would reenter the Earth’s atmosphere by March 1990, so a timely launch remained crucial for mission success. The countdown began on Jan. 4 for an expected Jan. 8 launch, with the crew arriving at KSC on Jan. 5. 

Cloudy skies scrubbed the first launch attempt on Jan. 8. Liftoff took place the next day at 7:35 a.m. EST from Launch Pad 39A, with LDEF 1,500 miles ahead of Columbia. The powered ride to space took 8.5 minutes, placing Columbia into a 215-by-38-mile orbit. A burn of the two Orbiter Maneuvering System (OMS) engines 40 minutes later changed the orbit to the desired 222-by-180-mile altitude. The crew opened the shuttle’s payload bay doors and deployed its radiators. The major activities for the first day in space involved the checkout of the RMS and the first rendezvous maneuver in preparation for the LDEF grapple three days later. The astronauts also activated four of the middeck experiments. On the mission’s second day, Low deployed the 15,000-pound Syncom satellite, releasing it in a frisbee motion out of the payload bay. The satellite extended its antenna, stabilized itself, and 40 minutes after deployment, fired its engine for the first burn to send it to its geostationary orbit. 

Following the Syncom deploy, the crew turned its attention to the rendezvous with LDEF while also continuing the middeck experiments. On Flight Day 3, they completed three rendezvous burns as they steadily continued their approach to LDEF. Soon after awakening on Flight Day 4, the astronauts spotted LDEF appearing as a bright star. After the first of four rendezvous burns, Columbia’s radar locked onto the satellite. As they continued the approach, with three more burns carried out successfully, Dunbar activated the RMS in preparation for the upcoming grapple. Brandenstein took over manual control of Columbia for the final approach and parked the shuttle close enough to LDEF for Dunbar to reach out with the 50-foot arm and grapple the satellite. Brandenstein reported, “We have LDEF.”  

For the next four hours, with Wetherbee flying the orbiter and Dunbar operating the arm, Ivins performed a comprehensive photo survey of LDEF, documenting the effects of nearly six years of space exposure on the various experiments. The survey completed, Dunbar slowly and carefully lowered LDEF into the payload bay, and five latches secured it in place for the ride back to Earth. With the two major goals of their mission completed, the astronauts settled down for the remainder of their 10-day mission conducting science experiments. 

During the mission, the STS-32 crew conducted several middeck experiments. The Protein Crystal Growth experiment used vapor diffusion to grow 120 crystals of 24 different proteins, for study by scientists following their return to Earth. The Characterization of Neurospora Circadian Rhythm experiment studied whether spaceflight affected the daily cycles of pink bread mold. The Fluid Experiment Apparatus performed materials processing research in the microgravity environment. The astronauts used the American Flight Echocardiograph (AFE) to study changes in their hearts as a result of weightlessness. The crew used the large format IMAX camera to film scenes inside the cabin as well as through the windows, such as the capture of LDEF. 

On Jan. 17, Brandenstein celebrated his 47th birthday, the fifth American astronaut to do so in space. His crew presented him with an inflatable plastic cake including candles while controllers in Mission Control passed on their birthday wishes as did his wife and teenage daughter. On the same day, NASA announced the selection of its 13th group of astronauts. Among them, engineer Ronald Sega, Dunbar’s husband, as well as the first female shuttle pilot, Eileen Collins, and the first Hispanic woman astronaut, Ellen Ochoa. 

On Jan. 19, the astronauts awakened for their planned final day in space. However, due to fog at their landing site, Edwards AFB in California, Mission Control first informed them that they would have to spend an extra orbit in space, and finally decided to delay the landing by an entire day. With their experiments already packed, the crew spent a quiet day, looking at the Earth and using up what film still remained. As they slept that night, they passed the record for the longest space shuttle mission, set by STS-9 in 1983.  

In preparation for reentry, the astronauts donned their orange spacesuits and closed the payload bay doors. A last-minute computer problem delayed reentry by one orbit, then Brandenstein and Wetherbee oriented Columbia into the deorbit attitude, with the OMS engines facing in the direction of travel. Over the Indian Ocean, they fired the two engines for 2 minutes 48 seconds to bring the spacecraft out of orbit. They reoriented the orbiter to fly with its heat shield exposed to the direction of flight as it encountered Earth’s atmosphere at 419,000 feet. The buildup of ionized gases caused by the heat of reentry prevented communications for about 15 minutes but provided the astronauts a great light show. After completing the Heading Alignment Circle turn, Brandenstein aligned Columbia with the runway, and Wetherbee lowered the landing gear. Columbia touched down and rolled to a stop, making the third night landing of the shuttle program and ending a 10-day 21-hour 1-minute flight, the longest shuttle flight up to that time, having completed 172 orbits of the Earth.  

Other records set by the astronauts on this mission included Brandenstein as the new record holder for most time spent in space by a shuttle crew member – 24 days – and Dunbar accumulating the most time in space by a woman – 18 days – up to that time. Following eight hours of postflight medical testing, the astronauts boarded a jet bound for Houston’s Ellington Field, where they reunited with their families and took part in a welcome home ceremony led by Aaron Cohen, director of NASA’s Johnson Space Center. 

Following postlanding inspections, workers placed Columbia, with LDEF still cradled in its payload bay, atop a Shuttle Carrier Aircraft, a modified Boeing-747, and the combination left Edwards on Jan. 25. Following a refueling stop at Monthan Davis AFB in Tucson, an overnight stay at Kelly AFB in San Antonio, and another refueling stop at Eglin AFB in Fort Walton Beach, Florida, Columbia and LDEF arrived back at KSC on Jan. 26. The next day, workers towed Columbia to the OPF and on Jan. 30 lifted LDEF out of its payload bay, in preparation for the detailed study of the effects of nearly six years in space on the 57 experiments it carried. Meanwhile, workers began to prepare Columbia for its next flight, STS-35 in December 1990. 

Enjoy the crew narrate a video of the STS-32 mission. Read Brandenstein‘s and Dunbar‘s recollections of the STS-32 mission in their oral histories with the JSC History Office. For an overview of the LDEF project, enjoy this video. For detailed information on the results of the LDEF experiments, follow this link

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John J. Uri

Helicopter Removes Artifact from NASA Armstrong Rooftop

Helicopter Removes Artifact from NASA Armstrong Rooftop

3 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

NASA/Lori Losey

What do the X-15 and the space shuttles have in common? Information from the rocket plane and the spacecraft, as well as many experimental aircraft, were tracked from a pedestal and telemetry dish during key eras in flight history at or near NASA’s Armstrong Flight Research Center in Edwards, California.

When the NASA facility’s administration Building 4800 was built in the 1950s, the infrastructure was included to anchor the rooftop pedestal and dish as the primary way to gather data from aircraft during flights. It was retired in 2015, but a recent roofing project enabled relocation of the artifact to a new place of honor for its support of many experimental aircraft such as the lifting body aircraft, the reverse swept wing X-29, and the highly maneuverable X-31.

“Gathering telemetry data from aircraft on missions is at the core of what we do. Close proximity to the back ramp was one of the big advantages of having the telemetry antenna on the roof in the early days,” said Bob Guere, NASA Armstrong Range Operations chief, referring to the area where aircraft taxi from the hangar to the flightline. “You were able to support ground tests and check airplanes before they taxied without having to use telemetry antennas positioned further away.”

A man secures a cable to a rooftop pedestal.
A cable is secured on a rooftop pedestal located on Building 4800 at NASA’s Armstrong Flight Research Center in Edwards, California, on Oct. 4, 2024. The pedestal, which was prepared for a helicopter lift to remove it from the roof, was used since the 1950s until 2015 to enable different telemetry dishes to collect data from research aircraft.
NASA/Carla Thomas

The rooftop pedestal was key in the early days of the center and its refurbishment in 2003 restored its value. The transformation also included certification to meet Space Shuttle Program landing requirements.

“When a space shuttle deorbited from space it was coming over the top of Edwards,” Guere said. “Telemetry antennas on the hill near NASA Armstrong looked down and with dirt and concrete in the background there were reflections. The rooftop antenna was closer to ground level and looked up as the orbiter was coming in for a landing. It provided an excellent link for shuttle landings.”

The pedestal and dish were not removed when it was decommissioned because of the cost. Now, it’s economical to use a helicopter to remove the pedestal from the roof compared to other options as part of a major project focusing primarily on re-roofing Building 4800. The helicopter lift of the pedestal took a month to plan, plus time to obtain airspace operation and landing permits from the Air Force for the removal project, said Bryan Watters, NASA Armstrong roof project manager.

A helicopter is positioned to carry a rooftop pedestal.
A helicopter is positioned to remove a rooftop pedestal from Building 4800 at NASA’s Armstrong Flight Research Center in Edwards, California, on Oct. 4, 2024. The pedestal was used since the 1950s to 2015 to house different telemetry dishes to collect data from research aircraft.
NASA/Carla Thomas

The pedestal and riser measured 16 feet tall above the rooftop and housed an assembly for the 12-foot dish to rotate. The pedestal and dish together weight about 2,500 pounds and were removed separately. Crews checked the eight bolts anchoring the pedestal and dish to infrastructure on the roof prior to the arrival of a helicopter Oct. 3 before the helicopter arrived.

The following day, after additional briefings, the helicopter was positioned over Building 4800 and a cable was lowered and attached to the pedestal. Once secured, the helicopter slowly gained altitude and took its passenger to the south side of the building. There it was released from the cable and taken to a nearby warehouse for storage. Roofers demolished the steel platform on which the pedestal was located to prepare the area for new roofing materials.

Officials have not determined where the pedestal will be displayed. There are several options to place the pedestal and dish by the famous retired research aircraft on display near the entrance of NASA Armstrong.

A man helps guide a pedestal hanging from a helicopter to a safe position on the ground.
A pedestal carried by a helicopter is positioned for a gentle placement on the ground. The helicopter removed the pedestal from the rooftop of Building 4800 at NASA’s Armstrong Flight Research Center in Edwards, California, on Oct. 4, 2024. The pedestal was used since the 1950s to 2015 to house different telemetry dishes to collect data from research aircraft.
NASA/Carla Thomas
A pedestal and dish are positioned on a rooftop.
A rooftop pedestal and telemetry dish gathered information from research aircraft at Building 4800 at NASA’s Armstrong Flight Research Center in Edwards, California. The pedestal was used since the 1950s to 2015 to house different dishes to collect data from research aircraft. On Oct. 4, 2024, a helicopter was used to remove the pedestal from the roof.
NASA/Jim Ross

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Jan 08, 2025

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Dede Dinius

Achieving Instrument High Accuracy In-Orbit

Achieving Instrument High Accuracy In-Orbit

The ARCSTONE observatory is shown in low Earth orbit with the spectrometer viewing the Sun and Moon. The spacecraft rotates in order to view the Moon or the Sun.

One of the most challenging tasks in remote sensing from space is achieving required instrument calibration accuracy on-orbit. The Moon is considered to be an excellent exoatmospheric calibration source. However, the current accuracy of the Moon as an absolute reference is limited to 5 – 10%, and this level of accuracy is inadequate to meet the challenging objective of Earth Science observations. ARCSTONE is a mission concept that provides a solution to this challenge. An orbiting spectrometer flying on a small satellite in low Earth orbit will provide lunar spectral reflectance with accuracy sufficient to establish an SI-traceable absolute lunar calibration standard for past, current, and future Earth weather and climate sensors.

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Joshua Lee Kinne

NASA’s Kennedy Marks New Chapter for Florida Space Industry

NASA’s Kennedy Marks New Chapter for Florida Space Industry

Kennedy Space Center Director and charter members of the Florida University Space Research Consortium signed a memorandum of understanding on Jan. 8, 2025. Comprised of the University of Florida, Embry-Riddle Aeronautical University, and University of Central Florida, the consortium was designated in 2024 as the state’s official space research entity, making Florida the only state with a university consortium affiliated with one of NASA’s centers. This critical milestone in a one-of-a-kind partnership to advance research, technology development, education, and communication between the spaceport and the state’s growing space industry. From left: Jennifer Kunz, Associate Director, Technical, Kennedy Space Center; Kelvin Manning, Deputy Director, Kennedy Space Center; Dr. Kent Fuchs, Interim President, University of Florida; Janet Petro, Director, Kennedy Space Center; Jeanette Nuñez, Florida Lieutenant Governor; Dr. Alexander Cartwright, President, University of Central Florida; Dr. Barry Butler, President, Embry-Riddle Aeronautical University.
Kennedy Space Center Director and charter members of the Florida University Space Research Consortium signed a memorandum of understanding on Jan. 8, 2025. From left: Jennifer Kunz, Associate Director, Technical, Kennedy Space Center; Kelvin Manning, Deputy Director, Kennedy Space Center; Dr. Kent Fuchs, Interim President, University of Florida; Janet Petro, Director, Kennedy Space Center; Jeanette Nuñez, Florida Lieutenant Governor; Dr. Alexander Cartwright, President, University of Central Florida; Dr. Barry Butler, President, Embry-Riddle Aeronautical University.
NASA/Kim Shiflett

The future of research and technology at NASA’s Kennedy Space Center in Florida is expanding Wednesday, as Kennedy’s center director and charter members in the Florida University Space Research Consortium signed a memorandum of understanding in research and development to assist with missions and contribute to NASA’s Moon to Mars exploration approach.

Officials from the consortium – designated in 2024 as the state’s official space research entity – NASA leaders, and guests participated in the signing ceremony held at Kennedy, marking a critical milestone in a partnership to advance research, technology development, education, and communication between the spaceport and the state’s growing space industry.

“Through this agreement, NASA will benefit in new and exciting ways from our longtime partnership with the universities that make Florida shine,” said NASA Administrator Bill Nelson. “As we move deeper into this golden era of space exploration, a new generation of thinkers and leaders will lead the way – thinkers and leaders like the researchers, faculty, and students of the Artemis Generation, whom we are pleased to work with through the consortium.”

The creation of the consortium was the result of more than a year of effort by leaders at Kennedy, the University of Florida, the University of Central Florida, and Embry-Riddle Aeronautical University. The agreement highlights the partnership and serves as the official start to partnering activities, with Florida now the only state with a university consortium affiliated with one of NASA’s centers.

Present at the event was Florida Governor Ron DeSantis. “It was great to visit the Space Coast Jan. 8 to announce the Florida University Space Research Consortium—our state’s official space research entity. Home to a thriving aerospace industry and world-class higher education institutions, Florida is the ideal place to launch this initiative. We are primed to lead the nation in developing a blueprint for state-space partnerships into the future.”

The mission of the consortium is to foster a symbiotic relationship between NASA Kennedy and Florida’s universities to drive innovation in space exploration, research, and technology through academic collaboration, joint projects, and workforce development.

“The launch of the Florida University Space Research Consortium is a significant milestone for our state’s aerospace sector, bringing together our world-class education system with cutting edge research and development,” said Lieutenant Governor Jeanette Nuñez. “This consortium will undoubtedly further strengthen and deepen Florida’s position as the leader in the global aerospace economy.”

The memorandum of understanding marks the dawn of a new era of cooperation between the Florida spaceport and the state’s university system, starting with the three charter universities with plans to expand to other state universities interested in participating. The push to enhance research and technological collaboration with universities has been a priority at NASA for years and has seen success at other NASA centers across the country.

While Kennedy becomes the first NASA center affiliated with a university consortium, recently NASA’s Ames Research Center in California’s Silicon Valley partnered with University of California, Berkeley, on development of the Berkeley Space Center at NASA Research Park, located at Ames. Still in development, the project is envisioned as a 36-acre discovery and innovation hub to include educational spaces, labs, offices, student housing, and a new conference center. More recently, NASA’s Johnson Space Center in Houston teamed up with Texas A&M University to break ground on a building that will become a testing laboratory for apparatuses in development for NASA’s Moon to Mars plans. In attendance for the groundbreaking was Kennedy Space Center Director Janet Petro, who was one of the signatories on the agreement.

Kennedy Space Center Janet Petro signs a memorandum of understanding between Kennedy Space Center and the Florida University Space Research Consortium on Jan. 8, 2025. Comprised of the University of Florida, Embry-Riddle Aeronautical University, and University of Central Florida, the consortium was designated in 2024 as the state’s official space research entity, making Florida the only state with a university consortium affiliated with one of NASA’s centers. This critical milestone in a one-of-a-kind partnership to advance research, technology development, education, and communication between the spaceport and the state’s growing space industry.
NASA’s Kennedy Space Center Director Janet Petro signs a memorandum of understanding between Kennedy Space Center and the Florida University Space Research Consortium on Jan. 8, 2025.
NASA/Kim Shiflett

“This agreement is a shining example of what it looks like when we link arms and create a space for the whole to be greater than all our parts,” said Petro. “This symbiotic partnership makes way for collaborative research opportunities and increased exposure to advanced technology, significantly enhancing NASA’s research output in fields such as aerospace engineering, materials science, robotics, and environmental science, all of which are necessary for long-term human exploration as we learn to live and work deeper into space than ever before.”

For more information about NASA Kennedy, visit:

https://www.nasa.gov/kennedy

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Jason Costa

A Rover Retrospective: Turning Trials to Triumphs in 2024

A Rover Retrospective: Turning Trials to Triumphs in 2024

3 min read

A Rover Retrospective: Turning Trials to Triumphs in 2024

A look back at a few Mars 2020 mission highlights of 2024  

Perseverance’s past year operating on the surface of Mars was filled with some of the mission’s highest highs, but also some of its greatest challenges. True to its name and its reputation as a mission that overcomes challenges, Perseverance and its team of scientists and engineers turned trials to triumphs in yet another outstanding year for the mission. There’s a lot to celebrate about Perseverance’s past year on Mars, but here are three of my top mission moments this year, in the order in which they happened. 

1. SHERLOC’s cover opens 

A close-up photo of an instrument on the Perseverance rover shows — against a blurred background of light tan-orange terrain — a metallic structure at the top of the frame, dusted with fine orange powder in some places. Pointing down from that is a short, barrel-shaped extension. Attached to the bottom of that is a “D”-shaped cover, attached to the mouth of the barrel on the right by a cylindrical hinge, fully opened toward the right, to an angle greater than 180 degrees.
NASA’s Mars Perseverance rover captured this image of its SHERLOC instrument (Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals), showing the cover mechanism of SHERLOC’s Autofocus and Context Imager camera (ACI) in a nearly open configuration. The rover acquired this image using its Left Mastcam-Z camera — one of a pair of cameras located high on the rover’s mast — on March 3, 2024 (sol 1079, or Martian day 1,079 of the Mars 2020 mission), at the local mean solar time of 12:18:41.
NASA/JPL-Caltech/ASU

In early January the SHERLOC instrument’s cover mechanism stopped responding during a routine attempt to acquire data on a rock outcrop in the Margin unit. After six weeks of team diagnostics, the SHERLOC instrument was declared offline and many of us feared that the instrument had met its end. In early March, the team made significant progress in driving the cover to a more open position. Then, to everyone’s surprise, the SHERLOC cover moved unexpectedly to a nearly completely open position during a movement of the arm on sol 1077. I remember staring in wonder at the image of the cover (taken on sol 1079), feeling real optimism for the first time that SHERLOC could be recovered. The team spent the next few months developing a new plan for operating SHERLOC with its cover open, and the instrument was declared back online at the end of June.  

2. A potential biosignature at Cheyava Falls  

A color image of a Mars rock shows a smooth band of orange-tan down the center of the image, flanked by lumpy strips of lighter materials, smooth and in shades of light mint green and turquoise. The center portion shows innumerable small spots — light tan, outlined in very dark gray.
NASA’s Perseverance Mars rover captured this image of “leopard spots” on a rock nicknamed “Cheyava Falls” on July 18, 2024 — sol 1212. or the 1,212th Martian day of the mission. Running the length of the rock are large white calcium sulfate veins. Between those veins are bands of material whose reddish color suggests the presence of hematite, one of the minerals that gives Mars its distinctive rusty hue. Scientists are particularly interested in the millimeter-size, irregularly shaped light patches on the central reddish band (from lower left to upper right of the image) that resemble leopard spots. Perseverance captured the image using a camera called WATSON (Wide Angle Topographic Sensor for Operations and eNgineering), part of the SHERLOC (Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals) instrument suite located on the end of Perseverance’s robotic arm.
NASA/JPL-Caltech/MSSS

No top list would be complete without Perseverance’s discovery in July 2024 of a potential biosignature in the form of sub-millimeter-scale “leopard spots” at an outcrop called Cheyava Falls. These features, which formed during chemical reactions within the rock, have dark rims and light cores and occur together with organic carbon. On Earth, these chemical reactions are often driven by or associated with microbes. Although we can’t say for sure that microbes were involved in the formation of the leopard spots at Cheyava Falls, this question can be answered when Perseverance’s samples are returned to Earth. In the meantime, this rock remains one of the most compelling rocks discovered on Mars.  

3. Arrival at Witch Hazel Hill 

A color image from the Martian surface shows uneven yellow-tan ground leading up to the base of a hill, where the smoother ground dotted with small rocks turns into an outcropping of much larger rocks. That outcropping is on the horizon, which runs diagonally in the image, from the upper left side to the top right of the frame.
NASA’s Mars Perseverance rover acquired this image at the top of Witch Hazel Hill, of the South Arm and Minnie Hill outcrops. Perseverance used its Left Navigation Camera (Navcam) — which also aids in driving — located high on the rover’s mast. The rover captured the image on Dec. 16, 2024 (sol 1359, or Martian day 1,359 of the Mars 2020 mission), at the local mean solar time of 13:26:38.
NASA/JPL-Caltech

Closing out 2024 on a high note, in mid-December Perseverance arrived at the top of a sequence of rock exposed on the western edge of the Jezero crater rim called Witch Hazel Hill. These rocks pre-date the formation of Jezero crater and could be amongst the oldest rocks exposed on the surface of Mars. These rocks have the potential to tell us about a period of solar system history not well-preserved on our own planet Earth, and they may record important clues about the early history and habitability of Mars. Witch Hazel Hill first caught my attention during landing site selection several years ago, when we were debating the merits of landing Perseverance in Jezero versus sites outside the crater. At the time, this area seemed just out of reach for a Jezero-focused mission, so I’m thrilled that the rover is now exploring this site!   

The Mars 2020 mission had its ups and downs and a fair share of surprises during 2024, but we are looking ahead to 2025 with excitement, as Perseverance continues to explore and sample the Jezero crater rim.

Written by Katie Stack Morgan, Mars 2020 Deputy Project Scientist

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Jan 08, 2025

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