Sols 4239-4240: ‘Vuggin’ Out’

Sols 4239-4240: ‘Vuggin’ Out’

2 min read

Sols 4239-4240: ‘Vuggin’ Out’

On a Martian surface covered in fine, powdery, brownish-orange soil, a large pockmarked rock – resembling a natural sponge – dominates half of the frame, extending from the upper-right corner to the center.
NASA’s Mars rover Curiosity acquired this image of a target named “Glacier Notch” on July 6, 2024, Sol 4236 of the Mars Science Laboratory Mission, at 16:55:06 UTC. Curiosity used its Mars Hand Lens Imager (MAHLI), located on the turret at the end of the rover’s robotic arm, capturing the image from 32 centimeters (about 13 inches) away.

Earth planning date: Monday, July 8, 2024

And just like we planned, Curiosity successfully drove about 11 meters (about 36 feet) after a 27-sol drill campaign at Mammoth Lakes! Not so fast, though, these rocks are just too interesting to leave behind so quickly. Instead of high-tailing it uphill like we usually do after a drill campaign, we’re staying put for another plan to get as much contact science on these diversely-toned rocks with mysterious origins and vugs (geologic term for the cavities in the rock) galore. It’s been a high priority to get as much color documentation of the clasts in the area, so a plan like this has kept my team busy commanding the Mastcams!

The first sol of this plan includes a long, 90-minute remote science block including about 50 minutes of ChemCam LIBS and RMI, about 32 minutes of Mastcam images, and a six-minute dust devil movie taken by Navcam. ChemCam is using its one-LIBS-per-sol on a conglomeratic block target named “Mount  Baxter,” and an RMI of Echo Ridge to the south. Mastcam is taking a 12-image mosaic of Mount Baxter after the LIBS work is done, and a huge 54-image mosaic to the east of Echo Ridge called “Stubblefield Canyon.” After the mast instruments are done, our rover will take about a four-hour long nap and wake up to unstow our arm. Arm activities this plan include two vug-tastic targets named “Lake Dorothy” and “Palisade Glacier,” both imaged by MAHLI and investigated by APXS. Curiosity is back to sleep by about 22:50, which sounds like my perfect sleep schedule.

The second sol of this plan includes a 60-minute remote science block containing about 45 minutes of ChemCam LIBS and RMI, only about six minutes of Mastcam images, and a whopping two hours of dust devil and environmental monitoring by Navcam. With 27 sols at our last location, we noticed significant wind motion between repeated images, and Navcam monitoring helps us keep track of how windy it is. Our rover will take another midday nap and wake up in the evening for a bonus APXS integration on Lake Dorothy, helping raise the signal-to-noise ratio and uncover more secrets (and questions) these Martian rocks have been keeping for millions of years.

Written by Natalie Moore, Mission Operations Specialist at Malin Space Science Systems

Share

Details

Last Updated
Jul 10, 2024

Related Terms

Powered by WPeMatico

Get The Details…

NASA’s Hubble Finds Strong Evidence for Intermediate-Mass Black Hole in Omega Centauri

NASA’s Hubble Finds Strong Evidence for Intermediate-Mass Black Hole in Omega Centauri

4 Min Read

NASA’s Hubble Finds Strong Evidence for Intermediate-Mass Black Hole in Omega Centauri

A Hubble image of the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space.
This NASA Hubble Space Telescope image features the globular star cluster, Omega Centauri.
Credits:
ESA/Hubble, NASA, Maximilian Häberle (MPIA)

Most known black holes are either extremely massive, like the supermassive black holes that lie at the cores of large galaxies, or relatively lightweight, with a mass of under 100 times that of the Sun. Intermediate-mass black holes (IMBHs) are scarce, however, and are considered rare “missing links” in black hole evolution.

Now, an international team of astronomers has used more than 500 images from NASA’s Hubble Space Telescope — spanning two decades of observations — to search for evidence of an intermediate-mass black hole by following the motion of seven fast-moving stars in the innermost region of the globular star cluster Omega Centauri.

A Hubble image of the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space.
Omega Centauri is about 10 times as massive as other big globular clusters – almost as massive as a small galaxy – and consists of roughly 10 million stars that are gravitationally bound.
ESA/Hubble, NASA, Maximilian Häberle (MPIA)

These stars provide new compelling evidence for the presence of the gravitational pull from an intermediate-mass black hole tugging on them. Only a few other IMBH candidates have been found to date.

Omega Centauri consists of roughly 10 million stars that are gravitationally bound. The cluster is about 10 times as massive as other big globular clusters — almost as massive as a small galaxy.

Among the many questions scientists want to answer: Are there any IMBHs, and if so, how common are they? Does a supermassive black hole grow from an IMBH? How do IMBHs themselves form? Are dense star clusters their favored home?

The astronomers have now created an enormous catalog for the motions of these stars, measuring the velocities for 1.4 million stars gleaned from the Hubble images of the cluster. Most of these observations were intended to calibrate Hubble’s instruments rather than for scientific use, but they turned out to be an ideal database for the team’s research efforts.

The central region of the globular star cluster Omega Centauri. It appears as a collection of myriad stars colored red, white, and blue on the black background of space.
This image shows the central region of the Omega Centauri globular cluster, where NASA’s Hubble Space Telescope found strong evidence for an intermediate-mass black hole candidate.
ESA/Hubble, NASA, Maximilian Häberle (MPIA)

“We discovered seven stars that should not be there,” explained Maximilian Häberle of the Max Planck Institute for Astronomy in Germany, who led this investigation. “They are moving so fast that they would escape the cluster and never come back. The most likely explanation is that a very massive object is gravitationally pulling on these stars and keeping them close to the center. The only object that can be so massive is a black hole, with a mass at least 8,200 times that of our Sun.”

Several studies have suggested the presence of an IMBH in Omega Centauri. However, other studies proposed the mass could be contributed by a central cluster of stellar-mass black holes, and had suggested the lack of fast-moving stars above the necessary escape velocity made an IMBH less likely in comparison.

This image includes three panels. The first image at left shows the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space. The second image, middle, zooms in on details of the central region of this cluster, with a closer view of the individual stars. The third image, at right, zooms in further to show the location of the intermediate-mass black hole candidate in the cluster. A dark region is circled and labeled
An international team of astronomers used more than 500 images from NASA’s Hubble Space Telescope – spanning two decades of observations – to detect seven fast-moving stars in the innermost region of Omega Centauri, the largest and brightest globular cluster in the sky. These stars provide compelling new evidence for the presence of an intermediate-mass black hole (IMBH) tugging on them. Only a few other IMBH candidates have been found to date. This image shows the location of the IMBH in Omega Centauri. If confirmed, at its distance of 17,700 light-years the candidate black hole resides closer to Earth than the 4.3-million-solar-mass black hole in the center of the Milky Way, which is 26,000 light-years away. Besides the Galactic center, it would also be the only known case of a number of stars closely bound to a massive black hole. This image includes three panels. The first image at left shows the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space. The second image shows the details of the central region of this cluster, with a closer view of the individual stars. The third image shows the location of the IMBH candidate in the cluster.
ESA/Hubble, NASA, Maximilian Häberle (MPIA)

“This discovery is the most direct evidence so far of an IMBH in Omega Centauri,” added team lead Nadine Neumayer of the Max Planck Institute for Astronomy in Germany, who initiated the study, together with Anil Seth from the University of Utah, Salt Lake City. “This is exciting because there are only very few other black holes known with a similar mass. The black hole in Omega Centauri may be the best example of an IMBH in our cosmic neighborhood.”

If confirmed, at a distance of 17,700 light-years the candidate black hole resides closer to Earth than the 4.3-million-solar-mass black hole in the center of the Milky Way, located 26,000 light-years away.

Omega Centauri is visible from Earth with the naked eye and is one of the favorite celestial objects for stargazers living in the southern hemisphere. Located just above the plane of the Milky Way, the cluster appears almost as large as the full Moon when seen from a dark rural area. It was first listed in Ptolemy’s catalog nearly 2,000 years ago as a single star. Edmond Halley reported it as a nebula in 1677. In the 1830s the English astronomer John Herschel was the first to recognize it as a globular cluster.

The discovery paper led by Häberle et al. is published online today in the journal Nature.

Scientists think a massive object is gravitationally pulling on the stars within Omega Centauri, keeping them close to its center. Credit: NASA’s Goddard Space Flight Center, Lead Producer: Paul Morris

The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, Colorado, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, Maryland, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.

Media Contacts:

Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov

Ray Villard
Space Telescope Science Institute, Baltimore, MD

Bethany Downer
ESA/Hubble.org

Science Contact:
Maximilian Häberle
Max Planck Institute for Astronomy, Heidelberg, Germany

Powered by WPeMatico

Get The Details…

NASA Administrator, Leaders to Discuss Space-Based Cancer Research

NASA Administrator, Leaders to Discuss Space-Based Cancer Research

NASA Administrator Bill Nelson delivers remarks to an audience that includes NASA astronauts during an event with Department of Health and Human Services Secretary Xavier Becerra to highlight how the agencies are making progress toward President Joe Biden and First Lady Jill Biden’s Cancer Moonshot initiative, March 21, 2024, in the Earth Information Center at the Mary W. Jackson NASA Headquarters building in Washington.
NASA Administrator Bill Nelson delivers remarks during an event with Department of Health and Human Services Secretary Xavier Becerra to highlight how the agencies are making progress toward the Biden Cancer Moonshot on March 21 in the Earth Information Center at the Mary W. Jackson NASA Headquarters building in Washington. NASA is working with agencies and researchers across the federal government to help cut the nation’s cancer death rate by at least 50% in the next 25 years, a goal of the Cancer Moonshot Initiative.
Credits: NASA/Keegan Barber

As part of the Biden Cancer Moonshot, NASA will virtually host an event at 2 p.m. EDT Thursday, July 11, to highlight how the agency is working to end cancer for the benefit of humanity by conducting research aboard the International Space Station.

The event will stream on NASA Television and the agency’s website. Learn how to stream NASA TV through a variety of platforms, including social media.

Additional participants include:

  • Dr. Michael Roberts, chief scientific officer, International Space Station National Laboratory
  • Dr. Catriona Jamieson, director, Sanford Stem Cell Institute at the University of California San Diego

As a member of the Cancer Cabinet, NASA is working with agencies and researchers across the federal government to reduce the nation’s cancer death rate by at least 50% in the next 25 years, one of the ambitious but achievable goals of the Cancer Moonshot.

Learn more about the Biden Cancer Moonshot at:

https://www.whitehouse.gov/cancermoonshot/

-end-

Faith McKie
Headquarters, Washington
202-358-1600
faith.d.mckie@nasa.gov

Share

Details

Last Updated

Jul 10, 2024

Powered by WPeMatico

Get The Details…
Tiernan P. Doyle

First Mars Crew Completes Yearlong Simulated Red Planet NASA Mission

First Mars Crew Completes Yearlong Simulated Red Planet NASA Mission

The inaugural CHAPEA (Crew Health and Performance Exploration Analog) crew is “back on Earth” after walking out of their simulated Martian habitat at NASA’s Johnson Space Center in Houston on July 6. The first of three simulated missions, CHAPEA Mission 1 was designed to help scientists, engineers, and mission planners better understand how living on another world could affect human health and performance.

Kelly Haston, commander, Ross Brockwell, flight engineer, Nathan Jones, medical officer, and Anca Selariu, science officer, lived and worked in an isolated 1,700-square-foot, 3D-printed habitat to support human health and performance research to prepare for future missions to Mars.

“Congratulations to the crew of CHAPEA Mission 1 on their completion of a year in a Mars-simulated environment,” said NASA Administrator Bill Nelson. “Through the Artemis missions, we will use what we learn on and around the Moon to take the next giant leap: sending the first astronauts to Mars. The CHAPEA missions are critical to developing the knowledge and tools needed for humans to one day live and work on the Red Planet.”

The crew stepped out of the habitat and back into the arms of family and friends after a 378-day simulated Mars surface mission that began June 25, 2023.

This high-fidelity simulation involved the crew carrying out different types of mission objectives, including simulated “marswalks,” robotic operations, habitat maintenance, exercise, and crop growth. The crew also faced intentional environmental stressors in their habitat such as resource limitations, isolation, and confinement. For the next two weeks, the volunteers will complete post-mission data collection activities before returning home.

“We planned the last 378 days with many of the challenges crews could face on Mars and this crew dedicated their lives over that time to achieve these unprecedented operational objectives,” said CHAPEA Principal Investigator Grace Douglas. “I am looking forward to diving into the data we have gathered, preparing for CHAPEA Mission 2 and eventually, a human presence on Mars.”

As NASA works to establish a long-term presence for scientific discovery and exploration on the Moon through the Artemis campaign, analog missions like CHAPEA provide scientific data to validate systems and develop technological solutions for future missions to Mars.

Two additional one-year CHAPEA missions are planned, with the next targeted to begin in 2025. The subsequent missions will be nearly identical, allowing researchers to collect data from more participants to expand the dataset and provide a broader perspective on the impacts of Mars-realistic resource limitations, isolation and confinement on human health and performance.

NASA has several other avenues for gathering isolation research, including the Human Exploration Research Analog, Antarctica, and other analogs, as well as human spaceflight missions to the International Space Station to ensure key research goals can be completed to inform future human missions to the Moon and Mars.

The CHAPEA simulated missions are unique because they test the impacts of extended isolation and confinement with the addition of Mars-realistic time delays of communicating to Earth – up to 44-minutes roundtrip – along with resource limitations relevant to Mars, including a more limited food system that can be supported on the space station and in other analogs.

To view the ceremony of crew exiting their habitat, visit here.

Under NASA’s Artemis campaign, the agency will establish the foundation for long-term scientific exploration at the Moon, land the first woman, first person of color, and its first international partner astronaut on the lunar surface, and prepare for human expeditions to Mars for the benefit of all.

Learn more about CHAPEA at:

www.nasa.gov/humans-in-space/chapea/

Powered by WPeMatico

Get The Details…
Kelli Mars

30 Years Ago: STS-65, the Second International Microgravity Lab Mission

30 Years Ago: STS-65, the Second International Microgravity Lab Mission

On July 8, 1994, space shuttle Columbia took to the skies on its 17th trip into space, on the second International Microgravity Laboratory (IML-2) mission. Six space agencies sponsored 82 life and microgravity science experiments. The seven-person crew consisted of Commander Robert D. Cabana, Pilot James D. Halsell, Payload Commander Richard J. Hieb, Mission Specialists Carl E. Walz, Leroy Chiao, and Donald A. Thomas, and Payload Specialist Chiaki Mukai representing the National Space Development Agency (NASDA) of Japan, now the Japan Aerospace Exploration Agency. Jean-Jacques H. Favier of the French space agency CNES served as a backup payload specialist. During their then-record setting 15-day shuttle flight, the international team of astronauts successfully completed the science program. They returned to earth on July 23.

The STS-65 crew patch Official photo of the STS-65 crew of Richard J. Hieb, seated left, Robert D. Cabana, and Donald A. Thomas; Leroy Chiao, standing left, James D. Halsell, Chiaki Mukai of Japan, and Carl E. Walz The payload patch for the International Microgravity Laboratory-2
Left: The STS-65 crew patch. Middle: Official photo of the STS-65 crew of Richard J. Hieb, seated left, Robert D. Cabana, and Donald A. Thomas; Leroy Chiao, standing left, James D. Halsell, Chiaki Mukai of Japan, and Carl E. Walz. Right: The payload patch for the International Microgravity Laboratory-2.

In August 1973, NASA and the European Space Research Organization, reorganized as the European Space Agency (ESA) in 1975, agreed to build a reusable laboratory called Spacelab to fly in the space shuttle’s cargo bay. As part of the agreement, ESA built two pressurized modules in addition to other supporting hardware. First flying on STS-9 in 1983, the 18-foot-long pressurized Spacelab module made its 10th flight on STS-65. In September 1992 NASA named Hieb as the IML-2 payload commander and Mukai and Favier as prime and backup payload specialists, respectively, adding Chiao and Thomas as mission specialists in October 1992, finally designating Cabana, Halsell, and Walz as the orbiter crew in August 1993. For Cabana and Hieb, both selected as astronauts in 1985, STS-65 marked their third spaceflight.  NASA selected Halsell, Walz, Chiao, and Thomas in 1990, in the class nicknamed The Hairballs. Walz would make his second flight, with the other three making their first. NASDA selected Mukai in 1985 and she holds the distinction as the first Japanese woman in space. Chiao and Mukai as part of the STS-65 crew marked the first time that two Asians flew on the shuttle at the same time, and with Kazakh cosmonaut Talgat A. Musbayev aboard Mir, the first time that three people of Asian origins flew in space at the same time.

The STS-65 crew during preflight training at NASA’s Johnson Space Center in Houston Workers at NASA’s Kennedy Space Center in Florida prepare the Spacelab module for the STS-65 mission
Left: The STS-65 crew during preflight training at NASA’s Johnson Space Center in Houston. Right: Technicians at NASA’s Kennedy Space Center in Florida prepare the Spacelab module for the STS-65 mission.

Columbia returned to NASA’s Kennedy Space Center (KSC) in Florida following its previous flight, STS-62, in March 1994. Technicians in KSC’s Orbiter Processing Facility (OPF) serviced the orbiter, removed the previous payload, and installed the Spacelab module in the payload bay. Following a successful leak check of the Spacelab module, rollover of Columbia from the OPF to the Vehicle Assembly Building (VAB) took place on June 8, where workers mated it with an external tank (ET) and two solid rocket boosters (SRBs). Following integrated testing, the stack rolled out to Launch Pad 39A seven days later. The crew participated in the Terminal Countdown Demonstration Test on June 22.

Liftoff of space shuttle Columbia on STS-65 carrying the second International Microgravity Laboratory
Liftoff of space shuttle Columbia on STS-65 carrying the second International Microgravity Laboratory.

On July 8, 1994, precisely on time, Columbia thundered off KSC’s Launch Pad 39A to begin the STS-65 mission. For the first time in shuttle history, a video camera recorded the liftoff from the orbiter’s flight deck, showing the vibrations during the first two minutes while the SRBs fired, smoothing out once the shuttle main engines took over. Mounted inside Columbia’s payload bay, the Spacelab 18-foot-long module provided a shirt-sleeve environment for the astronauts to conduct the scientific experiments. As during many Spacelab missions, the STS-65 crew carried out science operations 24-hours a day, divided into two teams – the red shift comprised Cabana, Halsell, Hieb, and Mukai, while Chiao, Thomas, and Walz made up the blue shift.

Still image from video recorded on the shuttle’s flight deck during powered ascent James D. Halsell, left, and Carl E. Walz moments after Columbia reached orbit View of the Spacelab module in the shuttle’s payload bay
Left: Still image from video recorded on the shuttle’s flight deck during powered ascent. Middle: James D. Halsell, left, and Carl E. Walz moments after Columbia reached orbit. Right: View of the Spacelab module in the shuttle’s payload bay.

Richard J. Hieb opens the hatch from the airlock to the tunnel leading to the Spacelab module Hieb and Chiaki Mukai begin activating Spacelab and its experiments The view from the tunnel showing astronauts at work in the Spacelab module
Left: Richard J. Hieb opens the hatch from the airlock to the tunnel leading to the Spacelab module. Middle: Hieb and Chiaki Mukai begin activating Spacelab and its experiments. Right: The view from the tunnel showing astronauts at work in the Spacelab module.

After reaching orbit, the crew opened the payload bay doors and deployed the shuttle’s radiators, and removed their bulky launch and entry suits, stowing them for the remainder of the flight. Shortly after, Hieb opened the hatch to the transfer tunnel and translated through it to enter the Spacelab module for the first time. He and Mukai activated the module and turned on the first experiments. For the next 14 days, the astronauts worked round the clock, with Cabana, Halsell, and Walz managing the shuttle’s systems while Hieb, Chiao, Thomas, and Mukai conducted the bulk of the research. The astronauts commemorated the 25th anniversary of the Apollo 11 launch on July 16 and the Moon landing four days later, recalling that their spacecraft and the Command Module shared the name Columbia.

Chiaki Mukai of the National Space Development Agency of Japan, now the Japan Aerospace Exploration Agency, talks to students in Japan using the shuttle’s amateur radio Richard J. Hieb, left, and Robert D. Cabana take an air sample from an experiment Hieb in the Lower Body Negative Pressure device
Left: Chiaki Mukai of the National Space Development Agency of Japan, now the Japan Aerospace Exploration Agency, talks to students in Japan using the shuttle’s amateur radio. Middle: Richard J. Hieb, left, and Robert D. Cabana take an air sample from an experiment. Right: Hieb in the Lower Body Negative Pressure device.

Donald A. Thomas, left, Leroy Chiao, Richard J. Hieb, and Chiaki Mukai at work in the Spacelab module Chiao, left, and Thomas work on the Biorack instruments Goldfish swim in the Aquatic Animal Experiment Unit
Left: Donald A. Thomas, left, Leroy Chiao, Richard J. Hieb, and Chiaki Mukai at work in the Spacelab module. Middle: Chiao, left, and Thomas work on the Biorack instruments. Right: Goldfish swim in the Aquatic Animal Experiment Unit.

Robert D. Cabana uses the shuttle’s amateur radio Leroy Chiao looks out at the Earth Carl E. Walz working on the shuttle’s flight deck
Left: Robert D. Cabana uses the shuttle’s amateur radio. Middle: Leroy Chiao looks out at the Earth. Right: Carl E. Walz working on the shuttle’s flight deck.

Carl E. Walz flies through the Spacelab module Donald A. Thomas gives two thumbs up for the crew’s performance during the mission Thomas, left, Walz, and Leroy Chiao pay tribute to Apollo 11 on the 25th anniversary of the Moon landing mission
Left: Carl E. Walz flies through the Spacelab module. Middle: Donald A. Thomas gives two thumbs up for the crew’s performance during the mission. Right: Thomas, left, Walz, and Leroy Chiao pay tribute to Apollo 11 on the 25th anniversary of the Moon landing mission.

The first time two Asians fly on the shuttle at the same time – Chiaki Mukai, left, of the National Space Development Agency of Japan, now the Japan Aerospace Exploration Agency, left, and NASA astronaut Leroy Chiao Donald A. Thomas, left, James D. Halsell, Carl E. Walz, and Chiao, all selected in 1990 as part of astronaut class 13, nicknamed The Hairballs Inflight photograph of the STS-65 crew
Left: The first time two Asians fly on the shuttle at the same time – Chiaki Mukai, left, of the National Space Development Agency of Japan, now the Japan Aerospace Exploration Agency, left, and NASA astronaut Leroy Chiao. Middle: Donald A. Thomas, left, James D. Halsell, Carl E. Walz, and Chiao, all selected in 1990 as part of astronaut class 13, nicknamed The Hairballs. Right: Inflight photograph of the STS-65 crew.

Rio de Janeiro Barrier islands in Papua New Guinea Hurricane Emilia in the central Pacific Ocean
A selection of the STS-65 crew Earth observation photographs. Left: Rio de Janeiro. Middle: Barrier islands in Papua New Guinea. Right: Hurricane Emilia in the central Pacific Ocean.

James D. Halsell uses the laptop-based PILOT to train for the entry and landing The astronauts close Columbia’s payload bay doors prior to entry Flash of plasma seen through Columbia’s overhead window during reentry
Left: James D. Halsell uses the laptop-based PILOT to train for the entry and landing. Middle: The astronauts close Columbia’s payload bay doors prior to entry. Right: Flash of plasma seen through Columbia’s overhead window during reentry.

At the end of 13 days, the astronauts finished the last of the experiments and deactivated the Spacelab module. Managers waved off the planned landing on July 22 due to cloudy weather at KSC. On July 23, the astronauts closed the hatch to the Spacelab module for the final time, closed Columbia’s payload bay doors, donned their launch and entry suits, and strapped themselves into their seats for entry and landing. Cabana piloted Columbia to a smooth landing on KSC’s Shuttle Landing Facility, completing 236 orbits around the Earth in 14 days, 17 hours, and 55 minutes, at the time the longest shuttle flight. Mukai set a then-record for the longest single flight by a woman. In October 1994, Columbia returned to its manufacturer, Rockwell International in Palmdale, California, for scheduled modification and refurbishment before its next mission, STS-73, in October 1995.

Robert D. Cabana pilots Columbia during the final approach to NASA’s Kennedy Space Center (KSC) in Florida, with the Vehicle Assembly Building visible through the window Columbia touches down on KSC’s Shuttle Landing Facility to end the STS-65 mission Donald A. Thomas, left, and Cabana give a thumbs up after the successful mission
Left: Robert D. Cabana pilots Columbia during the final approach to NASA’s Kennedy Space Center (KSC) in Florida, with the Vehicle Assembly Building visible through the window. Middle: Columbia touches down on KSC’s Shuttle Landing Facility to end the STS-65 mission. Right: Donald A. Thomas, left, and Cabana give a thumbs up after the successful mission.

The two Spacelab modules flew a total of 16 times, the last one during the STS-90 Neurolab mission in April 1998. Visitors can view the module that flew on STS-65 and eight other missions on display at the Stephen F. Udvar-Hazy Center of the Smithsonian Institution’s National Air and Space Museum in Chantilly, Virginia. The other module resides at the Airbus Defence and Space plant in Bremen, Germany, and not accessible to the public.

The Spacelab long module that flew on STS-65 and eight other missions on display at the Stephen F. Udvar-Hazy Center of the Smithsonian Institution’s National Air and Space Museum in Chantilly, Virginia. The Spacelab long module that flew on STS-65 and eight other missions on display at the Stephen F. Udvar-Hazy Center of the Smithsonian Institution’s National Air and Space Museum in Chantilly, Virginia. The Spacelab long module that flew on STS-65 and eight other missions on display at the Stephen F. Udvar-Hazy Center of the Smithsonian Institution’s National Air and Space Museum in Chantilly, Virginia.
The Spacelab long module that flew on STS-65 and eight other missions on display at the Stephen F. Udvar-Hazy Center of the Smithsonian Institution’s National Air and Space Museum in Chantilly, Virginia.

Enjoy the crew narrate a video about the STS-65 mission. Read Cabana’s and Chiao’s recollections of the STS-65 mission in their oral histories with the JSC History Office.

Powered by WPeMatico

Get The Details…
Kelli Mars