55 Years Ago: Nine Months Before the Moon Landing

55 Years Ago: Nine Months Before the Moon Landing

In October 1968, the American human spaceflight program took significant steps toward achieving President John F. Kennedy’s goal of landing a man on the Moon and returning him safely to the Earth before the end of the decade. American astronauts returned to space after a 23-month hiatus. The success of the 11-day Apollo 7 mission heralded well for NASA to decide to send the next mission, Apollo 8, to orbit the Moon in December. The Saturn V rocket for that flight rolled out to its seaside launch pad two days before Apollo 7 lifted off. Preparations for later missions to test the Lunar Module (LM) in Earth orbit and around the Moon continued in parallel, as did work in anticipation of astronauts and their lunar samples returning from the Moon. Meanwhile, the Soviet Union also resumed its human spaceflight program.

Apollo 7 astronauts Donn F. Eisele,Walter M. Schirra, and R. Walter Cunningham review flight trajectories with Director of Flight Crew Operations Donald K. “Deke” Slayton shortly before launch Schirra, Eisele, and Cunningham suit up for launch Liftoff of Apollo 7, returning American astronauts to space
Left: Apollo 7 astronauts Donn F. Eisele, left, Walter M. Schirra, and R. Walter Cunningham review flight trajectories with Director of Flight Crew Operations Donald K. “Deke” Slayton shortly before launch. Middle: Schirra, left, Eisele, and Cunningham suit up for launch. Right: Liftoff of Apollo 7, returning American astronauts to space!

The liftoff of Apollo 7 astronauts Walter M. Schirra, Donn F. Eisele, and R. Walter Cunningham on Oct. 11, 1968, signaled the end of a 23-month hiatus in American human spaceflights resulting from the tragic Apollo 1 fire. To prevent a recurrence of the fire and to increase overall safety, NASA and North American Rockwell in Downey, California, redesigned the Apollo spacecraft, and Schirra, Eisele, and Cunningham spent months training to test it in Earth orbit. By the time they lifted off from Launch Pad 34 at NASA’s Kennedy Space Center (KSC) in Florida, the Saturn V rocket for the Apollo 8 mission had already rolled out to Launch Pad 39A a few miles away.

View of Apollo 7 lifting off from Launch Pad 34 The Apollo 7 S-IVB third stage, used as a rendezvous target Apollo 7 astronauts Donn F. Eisele, Walter M. Schirra, and R. Walter Cunningham on the prime recovery U.S.S. Essex
Left: View of Apollo 7 lifting off from Launch Pad 34, with the Saturn V for Apollo 8 on Launch Pad 39A in the background. Middle: The Apollo 7 S-IVB third stage, used as a rendezvous target. Right: Apollo 7 astronauts Donn F. Eisele, left, Walter M. Schirra, and R. Walter Cunningham on the prime recovery U.S.S. Essex following their successful 11-day mission.

During their 11-day mission, Schirra, Eisele, and Cunningham thoroughly tested the redesigned Apollo spacecraft. Early in the mission, they performed rendezvous maneuvers with their rocket’s S-IVB second stage, a maneuver planned for later missions to retrieve the LM. They thoroughly tested the Service Propulsion System engine, critical on later lunar missions for getting into and out of lunar orbit, by firing it on eight occasions, including the critical reentry burn to bring them home. The three astronauts conducted the first live television broadcasts from an American spacecraft, providing viewers on the ground with tours of their spacecraft. Teams from the U.S.S. Essex (CV-9) recovered Schirra, Eisele, and Cunningham and their Command Module (CM) from the Atlantic Ocean on Oct. 22. Apollo program managers declared that Apollo 7 “accomplished 101%” of its planned objectives. 

Apollo 8 astronauts James A. Lovell, William A. Anders, and Frank Borman attend the rollout of their Saturn V from the Vehicle Assembly Building to Launch Pad 39A The Apollo 8 Saturn V at Launch Pad 39A Borman, left, Lovell, and Anders pose with their Saturn V
Left: Apollo 8 astronauts James A. Lovell, left, William A. Anders, and Frank Borman attend the rollout of their Saturn V from the Vehicle Assembly Building to Launch Pad 39A. Middle: The Apollo 8 Saturn V at Launch Pad 39A. Right: Borman, left, Lovell, and Anders pose with their Saturn V following a crew egress exercise from their spacecraft.

The success of Apollo 7 gave NASA the confidence to announce in November that the next mission, Apollo 8, would attempt to enter orbit around the Moon. In early October, workers in High Bay 2 of KSC’s Vehicle Assembly Building (VAB) completed the stacking of the Saturn V rocket for Apollo 8 by adding the Command and Service Module (CSM). On Oct. 9, two days before Apollo 7 lifted off, as the Apollo 8 crew of Frank Borman, James A. Lovell, and William A. Anders and other NASA officials looked on, the completed Saturn V rolled out from the VAB to begin its eight-hour journey to Launch Pad 39A, three and a half miles away. After the rocket arrived at the pad and engineers began testing it, on Oct. 23, Borman, Lovell, and Anders suited up and practiced emergency egress from the spacecraft, as did their backups Neil A. Armstrong, Edwin E. “Buzz” Aldrin, and Fred W. Haise.

Apollo 8 astronauts Frank Borman, William A. Anders, and James A. Lovell on the deck of the M/V Retriever prepare for their water egress test Anders, Lovell, and Borman inside the boilerplate Apollo spacecraft during the water egress test Anders, Lovell, and Borman in the life raft after egressing from their spacecraft
Left: Apollo 8 astronauts Frank Borman, left, William A. Anders, and James A. Lovell on the deck of the M/V Retriever prepare for their water egress test. Middle: Anders, left, Lovell, and Borman inside the boilerplate Apollo spacecraft during the water egress test. Right: Anders, left, Lovell, and Borman in the life raft after egressing from their spacecraft.

As part of their training, Borman, Lovell, and Anders conducted water egress training in the Gulf of Mexico near Galveston, Texas. On Oct. 25, sailors aboard the Motor Vessel M/V Retriever lowered a mockup CM with the crew inside into the water in a nose-down position. Flotation bags inflated to right the spacecraft to a nose-up position. The astronauts then exited the capsule onto life rafts and recovery personnel hoisted them aboard a helicopter. The next day, backups Armstrong, Aldrin, and Haise repeated the test. 

Workers in the Vehicle Assembly Building at NASA’s Kennedy Space Center (KSC) in Florida lower the S-IVB third stage onto the S-II second stage during stacking operations of the Apollo 9 Saturn V Apollo 9 astronaut Russell L. Schweickart practices entering and leaving the Command Module while wearing a pressure suit during brief periods of weightlessness aboard a KC-135 aircraft Engineers conduct a docking test between the Apollo 9 CM, bottom, and Lunar Module in an altitude chamber in KSC’s Manned Spacecraft Operations Building
Left: Workers in the Vehicle Assembly Building at NASA’s Kennedy Space Center (KSC) in Florida lower the S-IVB third stage onto the S-II second stage during stacking operations of the Apollo 9 Saturn V. Middle: Apollo 9 astronaut Russell L. Schweickart practices entering and leaving the Command Module while wearing a pressure suit during brief periods of weightlessness aboard a KC-135 aircraft. Right: Engineers conduct a docking test between the Apollo 9 CM, bottom, and Lunar Module in an altitude chamber in KSC’s Manned Spacecraft Operations Building.

Preparations for Apollo 9 included training for the first spacewalk of the Apollo program. According to the mission plan, with the LM and CM docked, crew members in both spacecraft would open their hatches. During the spacewalk, one astronaut would transfer from the LM to the CM using handrails for guidance and enter the CM in a test of an emergency rescue capability. The training for this activity took place aboard a KC-135 aircraft from Patrick Air Force Base (AFB) in Florida. By flying repeated parabolic trajectories, the aircraft could simulate 20-30 seconds of weightlessness at a time, during which the astronauts wearing space suits practiced entering and exiting a mockup of the CM. Backup crew members Alan L. Bean and Richard F. Gordon completed the training on Oct. 9 followed by David R. Scott and Russell L. Schweickart of the prime crew the next day. North American Rockwell delivered the Apollo 9 CSM to KSC in early October. At the end the month, technicians in KSC’s Manned Spacecraft and Operations Building (MSOB) conducted a docking test of the Apollo 9 LM and CSM to verify the interfaces between the two vehicles. In the VAB’s High Bay 3, workers stacked the three stages of the Saturn V rocket for Apollo 9 during the first week of October.

Workers in the Manned Spacecraft Operations Building (MSOB) at NASA’s Kennedy Space Center in Florida uncrate the Apollo 10 Lunar Module (LM) descent stage shortly after its arrival MSOB workers unwrap the Apollo 10 LM ascent stage MSOB workers prepare to mate the Apollo 10 LM ascent stage to its descent stage
Left: Workers in the Manned Spacecraft Operations Building (MSOB) at NASA’s Kennedy Space Center in Florida uncrate the Apollo 10 Lunar Module (LM) descent stage shortly after its arrival. Middle: MSOB workers unwrap the Apollo 10 LM ascent stage. Right: MSOB workers prepare to mate the Apollo 10 LM ascent stage to its descent stage.

In preparation for Apollo 10, planned as a test of the CSM and LM in lunar orbit, the Grumman Aircraft Engineering Corporation in Bethpage, New York, delivered the LM for that mission to KSC. The descent stage arrived Oct. 11, followed by the ascent stage five days later. Technicians in the MSOB mated the two stages and installed the assembled vehicle into a vacuum chamber on Nov. 2 to begin a series of altitude tests.

A flight of the Lunar Landing Training Vehicle at Ellington Air Force Base in Houston The forward instrument panel of the Lunar Module Test Article-8 Richard Wright, administrative assistant for the Lunar Receiving Laboratory, gives astronaut Michael Collins a tour of the gloveboxes for examining lunar samples
Left: A flight of the Lunar Landing Training Vehicle at Ellington Air Force Base in Houston. Middle: The forward instrument panel of the Lunar Module Test Article-8. Right: Richard Wright, administrative assistant for the Lunar Receiving Laboratory, gives astronaut Michael Collins a tour of the gloveboxes for examining lunar samples.

The Lunar Landing Training Vehicle (LLTV), built by Bell Aerosystems of Buffalo, New York, allowed Apollo astronauts to master the intricacies of landing on the Moon by simulating the LM’s performance in the final few hundred feet of the descent to the surface. Although an excellent training tool, the LLTV and its predecessor the Lunar Landing Research Vehicle (LLRV) also carried some risk. Astronaut Armstrong ejected from an LLRV on May 6, 1968, moments before it crashed at Houston’s Ellington AFB. The final accident investigation report, issued on Oct. 17, cited a loss of helium pressure that caused depletion of the fuel used for the reserve attitude thrusters, with inadequate warning to the pilot as a contributing factor. By that time, Chief of Aircraft Operations Joseph S. “Joe” Algranti piloted the properly modified LLTV during its first flight on Oct 3. Algranti and NASA pilot H.E. “Bud” Ream completed 14 checkout flights before a crash in December grounded the LLTV. In October, NASA began a series of critical thermal-vacuum tests to certify the Apollo LM for lunar missions. The tests, conducted in the Space Environment Simulation Laboratory (SESL), at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston, involved Grumman pilots Gerald P. Gibbons and Glennon M. Kingsley and astronaut James B. Irwin. The tests using Lunar Module Test Article-8, concluded in November, and simulated the temperatures expected during a typical flight to the Moon and descent to the surface.

To receive astronauts and their lunar samples after their return from the Moon, NASA built the Lunar Receiving Laboratory (LRL) in MSC’s Building 37. The LRL’s special design isolated astronauts and rock samples returning from the Moon to prevent back-contamination of the Earth by any possible lunar micro-organisms. By October 1968, with the Moon landing likely less than a year away, the LRL had reached a state of readiness that warranted a simulation of some its capabilities. Between Oct. 22 and Nov. 1, managers, scientists, and technicians carried out a 10-day simulation of LRL operations following a lunar landing mission. Although the exercise uncovered many deficiencies, enough time remained to correct them before the actual Moon landing.

Lift off of Soyuz 3 from the Baikonur Cosmodrome carrying cosmonaut Georgi T. Beregovoi Beregovoi during a television broadcast from Soyuz 3 The Soyuz 3 spacecraft carrying Beregovoi descends under its parachute for a soft-landing
Left: Lift off of Soyuz 3 from the Baikonur Cosmodrome carrying cosmonaut Georgi T. Beregovoi. Middle: Beregovoi during a television broadcast from Soyuz 3. Right: The Soyuz 3 spacecraft carrying Beregovoi descends under its parachute for a soft-landing. Image credits: courtesy Roscosmos.

As a reminder that a race to the Moon still existed, the Soviet Union also resumed crewed missions, halted in April 1967 by the death of Soyuz 1 cosmonaut Vladimir M. Komarov. Just three days after the Apollo 7 splashdown, the Soviets launched Soyuz 2, but without a crew. The next day, Soyuz 3 lifted off with cosmonaut Georgi T. Beregovoi aboard, at 47 the oldest person to fly in space up to that time. Although Beregovoi brought the two spacecraft close together, he could not achieve the intended docking. Soyuz 2 landed on Oct. 28 and Beregovoi in Soyuz 3 two days later. Following the Zond 5 circumlunar flight in September, rumors persisted that the next Zond mission may soon carry two cosmonauts on a similar circumlunar flight. The apparently successful Zond 5 mission coupled with the rumors of an imminent Soviet crewed lunar mission possibly contributed to the decision to send Apollo 8 on its historic circumlunar flight in December 1968.

News from around the world in October 1968:

Oct. 2 – Redwood National Park established to preserve the tallest trees on Earth.

Oct. 7 – The Motion Picture Association of America adopts a film rating system.

Oct. 12 – Equatorial Guinea gains independence from Spain.

Oct. 12 – The XIX Olympic Games open in Mexico City, the first time the games held in Latin America.

Oct. 14 – The Beatles finish recording the double “White Album.”

Oct. 16 – The Jimi Hendrix Experience releases its last studio album “Electric Ladyland.”

Oct. 17 – Release of the film “Bullitt,” starring Steve McQueen.

Oct. 20 – American high jumper Dick Fosbury introduces the Fosbury Flop technique at the Mexico City Olympics.

Oct. 24 – The 199th and last flight of the X-15 hypersonic rocket plane takes place at Edwards Air Force Base in California, piloted by NASA pilot William H. Dana.

Oct. 25 – Led Zeppelin gives its first concert, at Surrey University in England.

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Kelli Mars

International Ocean Satellite Monitors How El Niño Is Shaping Up

International Ocean Satellite Monitors How El Niño Is Shaping Up

The maps above show sea levels in the Pacific Ocean
The maps above show sea levels in the Pacific Ocean during early October of 1997, 2015, and 2023, in the run up to El Niño events. Higher-than-average ocean heights appear red and white, and lower-than-average heights are in blue and purple.
NASA/JPL-Caltech

Sentinel-6 Michael Freilich is the latest satellite contributing to a 30-year sea level record that researchers are using to compare this year’s El Niño with those of the past.

Not all El Niño events are created equal. Their impacts vary widely, and satellites like the U.S.-European Sentinel-6 Michael Freilich help anticipate those impacts on a global scale by tracking changes in sea surface height in the Pacific Ocean.

Water expands as it warms, so sea levels tend to be higher in places with warmer water. El Niños are characterized by higher-than-normal sea levels and warmer-than-average ocean temperatures along the equatorial Pacific. These conditions can then propagate poleward along the western coasts of the Americas. El Niños can bring wetter conditions to the U.S. Southwest and drought to regions in the western Pacific, including Indonesia. This year’s El Niño is still developing, but researchers are looking to the recent past for clues as to how it is shaping up.

There have been two extreme El Niño events in the past 30 years: the first from 1997 to 1998 and the second from 2015 to 2016. Both caused shifts in global air and ocean temperatures, atmospheric wind and rainfall patterns, and sea level. The maps above show sea levels in the Pacific Ocean during early October of 1997, 2015, and 2023, with higher-than-average ocean heights in red and white, and lower-than-average heights in blue and purple. Sentinel-6 Michael Freilich captured the 2023 data, the TOPEX/Poseidon satellite collected data for the 1997 image, and Jason-2 gathered data for the 2015 map.

By October 1997 and 2015, large areas of the central and eastern Pacific had sea levels more than 7 inches (18 centimeters) higher than normal. This year, sea levels are about 2 or 3 inches (5 to 8 centimeters) higher than average and over a smaller area compared to the 1997 and 2015 events. Both of the past El Niños reached peak strength in late November or early December, so this year’s event may still intensify.

“Every El Niño is a little bit different,” said Josh Willis, Sentinel-6 Michael Freilich project scientist at NASA’s Jet Propulsion Laboratory in Southern California. “This one seems modest compared to the big events, but it could still give us a wet winter here in the Southwest U.S. if conditions are right.”

More About the Mission

Launched in November 2020, Sentinel-6 Michael Freilich is named after former NASA Earth Science Division Director Michael Freilich. The satellite is one of two that compose the Copernicus Sentinel-6/Jason-CS (Continuity of Service) mission.

Sentinel-6/Jason-CS was jointly developed by ESA (European Space Agency), the European Organisation for the Exploitation of Meteorological Satellites (EUMETSAT), NASA, and the U.S. National Oceanic and Atmospheric Administration, with funding support from the European Commission and technical support on performance from the French space agency CNES (Centre National d’Études Spatiales).

To learn more about Sentinel-6 Michael Freilich, visit:

https://www.nasa.gov/sentinel-6

News Media Contacts

Jane J. Lee / Andrew Wang
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-0307 / 626-379-6874
jane.j.lee@jpl.nasa.gov / andrew.wang@jpl.nasa.gov

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Anthony Greicius

NASA Employees Win Top Federal Award for Asteroid Deflection Mission

NASA Employees Win Top Federal Award for Asteroid Deflection Mission

Scott Bellamy, left, and Brian Key, right, stop for a photo moments after receiving the Samuel J. Heyman Service to America Medals. Bellamy and Key accepted on behalf of the entire DART team during a ceremony at the John F. Kennedy Center for Performing Arts in Washington on Oct. 17.
Scott Bellamy, left, and Brian Key, right, received the Samuel J. Heyman Service to America Medals. Bellamy and Key accepted on behalf of the entire DART team during a ceremony at the John F. Kennedy Center for Performing Arts in Washington on Oct. 17.
Allison Shelley for the Partnership for Public Service

NASA’s Brian Key and Scott Bellamy accepted the Samuel J. Heyman Service to America Medal on behalf of a mission team for the first planetary defense test during a ceremony at the John F. Kennedy Center for Performing Arts in Washington on Oct. 17.

The awards program for career federal employees, known as the Sammies, aims to highlight key accomplishments that benefit the nation, seeks to build trust in government, and inspire people to consider careers in public service.

Known as DART, NASA’s Double Asteroid Redirection Test mission successfully impacted a known asteroid in September 2022 and altered its orbit, demonstrating one planetary defense method that could be used to protect Earth from a potentially hazardous asteroid on a collision course with our home planet if one were ever discovered.

Key and Bellamy served as program manager and mission manager for DART, respectively, and are based in the Planetary Missions Program Office at NASA’s Marshall Space Flight Center in Huntsville, Alabama. For their work on the mission, the team was honored in the Science, Technology, and Environment category of the Heyman awards.

“DART was a first-of-its-kind mission that marked a watershed moment for planetary defense. The DART team members are some of the very best of NASA, and we are so excited to see Brian Key and Scott Bellamy recognized for their contributions and leadership,” NASA Administrator Bill Nelson said. “Brian, Scott, and the entire DART team have shaped the course of human space exploration, inspiring people around the world through innovation. Thanks to their dedication and hard work, NASA is better prepared to defend our home planet, and will be ready for whatever the universe throws at us.”

In his role on DART, Key maintained budget, staff, and schedule oversight for the mission and worked directly with DART spacecraft developers at Johns Hopkins Applied Physics Laboratory in Laurel, Maryland.

“I’m elated to see our team honored with this award and hope it will bring more attention to the valuable work NASA does to defend our home world,” Key said, who oversees management of NASA’s $2 billion portfolio spanning the Discovery Program, the New Horizons Program, and the Solar System Exploration Program, which covers the full range of large and small science missions exploring the planets, moons, asteroids, comets and other destinations of interest in the solar system.

Bellamy was tasked with keeping the team on track to launch and operate the mission. He echoed Key’s praise for the entire DART team.

“We’re just the managers,” Bellamy said. “Our role has been to serve the team, keeping things moving forward as smoothly as possible to enable them to do the actual hands-on, pencilwork-to-hardware that brought this mission from concept to reality.”

That mission could not have gone more flawlessly, they agreed. Launched in November 2021, the DART spacecraft traveled to more than 6.8 million miles from Earth with one simple goal: to intentionally impact into Dimorphos, a 492-foot-diameter asteroid, at roughly 14,000 miles per hour, thus altering its orbit around its much larger parent asteroid, Didymos. DART’s collision with Dimorphos altered the asteroid’s roughly 12-hour orbit period around its parent by about a half-hour.

“I don’t even have the words to describe the release of emotion in the control room when we got confirmation that DART had impacted,” Bellamy said. “The whole team went from nail-biting suspense to unbelievable excitement in a matter of seconds.”

As for future planetary defense activities, NASA and its partners will build on DART’s success. A follow-up mission by ESA (European Space Agency), called Hera, is scheduled to launch in 2024 to further assess DART’s impact on Dimorphos. NASA also is developing the NEO Surveyor mission, which is designed to accelerate the rate at which the agency can discovery potentially hazardous near-Earth objects, asteroids and comets which can come close to Earth and could pose an impact risk.

Johns Hopkins Applied Physics Laboratory managed the DART mission for NASA’s Planetary Defense Coordination Office. The agency provided support for the mission from several centers, including the Jet Propulsion Laboratory in Southern California; Goddard Space Flight Center in Greenbelt, Maryland; NASA’s Johnson Space Center in Houston; Glenn Research Center in Cleveland; and Langley Research Center in Hampton, Virginia.

Learn more about NASA’s Planetary Missions Program and Planetary Defense Coordination Offices online.

-end-

News Media Contacts

Jackie McGuinness
Headquarters, Washington
202-358-1600
jackie.mcguinness@nasa.gov

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

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Last Updated

Oct 18, 2023

Editor

Claire A. O’Shea

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Claire A. O’Shea

The Start of an Eclipse

The Start of an Eclipse

The Sun appears as a white disc in the darkness of space. The Moon begins to pass in front of it on the left, making it look like there's a circular portion of the Sun missing.
NASA / Jasmin Moghbeli

While aboard the International Space Station, astronaut Jasmin Moghbeli took this picture of the Moon passing in front of the Sun during the annular solar eclipse on Oct. 14, 2023. As the space station orbits Earth, astronauts take images of the planet below and phenomena in space.

Visible in parts of the United States, Mexico, and many countries in South and Central America, millions of people in the Western Hemisphere experienced this eclipse. If you weren’t in the path of the annular eclipse, or you want to relive this exciting event, watch our coverage of the 2023 annular solar eclipse.

Image credit: NASA/Jasmin Moghbeli

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Monika Luabeya

All Together Now: Drill Joins Other Moon Rover Science Instruments

All Together Now: Drill Joins Other Moon Rover Science Instruments

Engineers inspect the TRIDENT drill in a clean room.
A team of engineers from NASA’s Johnson Space Center in Houston and Honeybee Robotics in Altadena, California inspect TRIDENT – short for The Regolith Ice Drill for Exploring New Terrain – shortly after its arrival at the integration and test facility.
NASA/Robert Markowitz

A team of engineers from NASA’s Johnson Space Center in Houston and Honeybee Robotics in Altadena, California, inspect TRIDENT – short for The Regolith Ice Drill for Exploring New Terrain – shortly after its arrival at the integration and test facility. In the coming months, the team will integrate the drill into NASA’s first robotic Moon rover, VIPER – short for the Volatiles Investigating Polar Exploration Rover. 

TRIDENT is the fourth and final science instrument for VIPER to arrive at the clean room, where the vehicle is being built. NASA engineers have already successfully integrated VIPER’s three other science instruments into the rover. These include: the MSOLO (Mass Spectrometer Observing Lunar Operations), which was integrated in  July, and the NSS (Neutron Spectrometer System) and NIRVSS (Near-Infrared Volatiles Spectrometer System) instruments, which were integrated in August. 

TRIDENT will dig up soil cuttings from as much as three feet below the lunar surface using a rotary percussive drill – meaning it both spins to cut into the ground and hammers to fragment hard material for more energy-efficient drilling. In addition to being able to measure the strength and compactedness of the lunar soil, the drill features a tip that carries a temperature sensor to take readings below the surface. 

MSOLO is a commercial off-the-shelf mass spectrometer modified to withstand the harsh lunar environment by engineers and technicians at the agency’s Kennedy Space Center in Florida. MSOLO will help NASA analyze the chemical makeup of the lunar soil and study water on the surface of the Moon. 

NIRVSS will detect which types of minerals and ices are present, if any, and identify the composition of the lunar soil.

NSS will help scientists study the distribution of water and other potential resources on the Moon, by targeting its search for hydrogen – the element that’s the telltale sign of water, or H2O.

Over the past few months, engineers and technicians from the agency’s Johnson, Kennedy, and Ames Research Center, performed pre-integration operations, such as installing external heaters, harnesses, instrumentation sensors, and multi-layer insulation onto the instruments. This critical hardware will help monitor and control how hot or cold the instruments get as the rover encounters different temperature conditions on the Moon; depending on whether the rover is in sunlight or shade, temperatures can vary by as many as 300 degrees Fahrenheit.  

VIPER will launch to the Moon aboard Astrobotic’s Griffin lunar lander on a SpaceX Falcon Heavy rocket as part of NASA’s Commercial Lunar Payload Services initiative. It will reach its destination at Mons Mouton near the Moon’s South Pole in November 2024. During VIPER’s approximately 100-day mission, these four instruments will work together to better understand the origin of water and other resources on the Moon, which could support human exploration as part of NASA’s Artemis program.  

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Rachel Hoover