Six NASA Instruments Will Fly to Moon on Intuitive Machines Lander

Six NASA Instruments Will Fly to Moon on Intuitive Machines Lander

The Nova-C lunar lander is seen in the high bay of Intuitive Machines Headquarters in Houston, before it shipped to NASA’s Kennedy Space Center in Florida for integration with a SpaceX Falcon 9 rocket for launch as part of NASA’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign.
The Nova-C lunar lander is seen in the high bay of Intuitive Machines Headquarters in Houston, before it shipped to NASA’s Kennedy Space Center in Florida for integration with a SpaceX Falcon 9 rocket for launch as part of NASA’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign.
Credit: Intuitive Machines

NASA is gearing up for a commercial robotic flight to the Moon under the agency’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign. Intuitive Machines will launch its Nova-C lander on a SpaceX Falcon 9 rocket no earlier than Wednesday, Feb. 14, from Cape Canaveral, Florida. The Intuitive Machines IM-1 mission will carry six NASA payloads targeted for the South Polar region.

The group of NASA instruments aboard IM-1 will conduct scientific research and demonstrate technologies to help us better understand the Moon’s environment and improve landing precision and safety in the challenging conditions of the lunar south polar region, paving the way for future Artemis astronaut missions. The payloads will collect data on how the plume of engine gasses interacts with the Moon’s surface and kicks up lunar dust, investigate radio astronomy and space weather interactions with the lunar surface, test precision landing technologies, and measure the quantity of liquid propellant in Nova-C propellant tanks in the zero gravity of space. The Nova-C lander will also carry a retroreflector array that will contribute to a network of location markers on the Moon that will be used as a position marker for decades to come

The Nova-C lander is targeted to land Thursday, Feb. 22, in a relatively flat and safe area near the Malapert A crater, in the south polar region of the Moon.

The six NASA payloads aboard Intuitive Machines’ IM-1 mission include:

  • LN-1 (Lunar Node 1 Navigation Demonstrator)
    A small, CubeSat-sized flight hardware experiment that integrates navigation and communication functionality for autonomous navigation to support future surface and orbital operations. Principal investigator: Dr. Evan Anzalone, NASA’s Marshall Space Flight Center
  • LRA (Laser Retroreflector Array)
    A collection of eight retroreflectors that enable precision laser ranging, which is a measurement of the distance between an orbiting or landing spacecraft to the reflector on the lander. LRA is a passive optical instrument and will function as a permanent location marker on the Moon for decades to come.
    Principal investigator: Dr. Xiaoli Sun, NASA’s Goddard Space Flight Center
  • NDL (Navigation Doppler Lidar for Precise Velocity and Range Sensing)
    A Lidar-based (Light Detection and Ranging) descent and landing sensor. This instrument operates on the same principles of radar but uses pulses from a laser emitted through three optical telescopes. NDL will measure vehicle velocity (speed and direction) and altitude (distance to surface) with high precision during descent to touchdown. Principal investigator: Dr. Farzin Amzajerdian, NASA’s Langley Research Center
  • RFMG (Radio Frequency Mass Gauge)
    A rocket propellant gauge used to measure the amount of spacecraft propellant in a low-gravity space environment. Using sensor technology, RFMG will measure the amount, or mass, of cryogenic propellants in Nova-C’s tanks, providing data that can help predict propellant usage on future missions. Principal investigator: Dr. Greg Zimmerli, NASA’s Glenn Research Center
  • ROLSES (Radio-wave Observations at the Lunar Surface of the Photoelectron Sheath)
    Four antennas and a low-frequency radio receiver system designed to study the dynamic radio energy environment near the lunar surface and determine how natural and human-generated activity near the surface interacts with science investigations. It will also detect radio emissions from the Sun, Jupiter, and Earth, as well as dust impacting the surface of the Moon. Principal investigator: Dr. Nat Gopalswamy, NASA Goddard
  • SCALPSS (Stereo Cameras for Lunar Plume-Surface Studies)
    A suite of four cameras to capture stereo and still images of the dust plume created by the lander’s engine as it begins its descent to the lunar surface until after the engine shuts off. Principal investigator: Michelle Munk, NASA Langley

Intuitive Machines is one of 14 vendors eligible to carry NASA payloads to the Moon through the agency’s CLPS initiative, which began in 2018. CLPS is an innovative approach connecting NASA with commercial solutions from American companies to deliver scientific, exploration, and technology payloads to the Moon’s surface and into lunar orbit. Through CLPS, NASA aims to gain new insights into the lunar environment and expand the lunar economy to support future crewed missions under the Artemis campaign.

Learn more about NASA’s CLPS initiative at:

https://www.nasa.gov/clps/

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Jeffery Rubio

Spiral Galaxy NGC 4254’s Dazzling Swirls

Spiral Galaxy NGC 4254’s Dazzling Swirls

Webb’s image of NGC 4254 shows a densely populated face-on spiral galaxy anchored by its central region, which has a light blue haze that takes up about a quarter of the view. In this circular core is the brightest blue area. Within the core are populations of older stars, represented by many pinpoints of blue light. Spiny spiral arms made of stars, gas, and dust also start at the center, largely starting in the wider area of the blue haze. The spiral arms extend to the edges, rotating counterclockwise. The spiraling filamentary structure looks somewhat like a cross section of a nautilus shell. The arms of the galaxy are largely orange, ranging from dark to bright orange. Scattered across the packed scene are some additional bright blue pinpoints of light, which are stars spread throughout the galaxy. In areas where there is less orange, it is darker, and some dark regions look more circular.
It’s oh-so-easy to be mesmerized by this spiral galaxy. Follow its clearly defined arms, which are brimming with stars, to its center, where there may be old star clusters and – sometimes – active supermassive black holes. NASA’s James Webb Space Telescope delivered highly detailed scenes of this and other nearby spiral galaxies in a combination of near- and mid-infrared light.
NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), and the PHANGS team

NGC 4254, a spiral galaxy, is resplendent in orange and blue in this Jan. 29, 2024, image from the James Webb Space Telescope. This is one of 19 nearby spiral galaxies recently imaged by the telescope as part of the long-standing Physics at High Angular resolution in Nearby GalaxieS (PHANGS) program supported by more than 150 astronomers worldwide.

Webb’s Near-Infrared Camera captured millions of stars in these images, which sparkle in blue tones, while the telescope’s Mid-Infrared Instrument data highlights glowing dust, showing us where it exists around and between stars.

Explore the intricacies of spiral galaxies in this deep dive.

Image Credit: NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), and the PHANGS team

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Monika Luabeya

Into the Belly of the Rover: VIPER’s Final Science Instrument Installed 

Into the Belly of the Rover: VIPER’s Final Science Instrument Installed 

A team of engineers prepares to integrate TRIDENT – short for The Regolith Ice Drill for Exploring New Terrain – into the belly of NASA’s first robotic Moon rover, VIPER – short for the Volatiles Investigating Polar Exploration Rover.
NASA/Bill Stafford

A team of engineers prepares to integrate TRIDENT – short for The Regolith Ice Drill for Exploring New Terrain – into the belly of NASA’s first robotic Moon rover, VIPER (Volatiles Investigating Polar Exploration Rover). 

TRIDENT, designed and developed by engineers at Honeybee Robotics in Altadena, California, is the fourth and final science instrument to be installed into VIPER. NASA engineers have already successfully integrated VIPER’s three other science instruments into the rover. These include: the MSOLO (Mass Spectrometer Observing Lunar Operations), NIRVSS (Near-Infrared Volatiles Spectrometer System), and NSS (Neutron Spectrometer System). 

Shortly after TRIDENT was integrated in the clean room at NASA’s Johnson Space Center in Houston, the team also successfully tested its ability to power on, release the locks that hold the drill in place during launch, extend to its full depth of more than three feet (one meter), perform percussive drilling, and return to its stowed position inside the rover.

TRIDENT will dig up soil from 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 also carries a temperature sensor to take readings below the surface. 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. Scientists will work with these four instruments to better understand the origin of water and other resources on the Moon, which could support human exploration as part of NASA’s Artemis campaign.

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Rachel Hoover

Team Assessing SHERLOC Instrument on NASA’s Perseverance Rover

Team Assessing SHERLOC Instrument on NASA’s Perseverance Rover

3 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

NASA’s Perseverance puts its robotic arm to work
NASA’s Perseverance puts its robotic arm to work around a rocky outcrop called “Skinner Ridge” in a set of images captured in June and July 2022 by the rover’s Mastcam-Z camera system. SHERLOC is mounted on the end of the arm.
NASA/JPL-Caltech/ASU/MSSS

Engineers are working to stabilize a dust cover on one of the science instrument’s cameras.

Data and imagery from NASA’s Perseverance Mars rover indicate one of two covers that keep dust from accumulating on the optics of the SHERLOC instrument remains partially open. In this position, the cover interferes with science data collection operations. Mounted on the rover’s robotic arm, SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals) uses cameras, a spectrometer, and a laser to search for organic compounds and minerals that have been altered in watery environments and may be signs of past microbial life.

The mission determined on Jan. 6 that the cover was oriented in such a position that some of its operation modes could not successfully operate. An engineering team has been investigating to determine the root cause and possible solutions. Recently, the cover partially opened. To better understand the behavior of the cover’s motor, the team has been sending commands to the instrument that alter the amount of power being fed to it.

With the cover in its current position, the instrument cannot use its laser on rock targets, and cannot collect spectroscopy data. However, imaging microscopy can still be acquired with WATSON, a color camera on SHERLOC used for taking close-up images of rock grains and surface textures. WATSON (Wide Angle Topographic Sensor for Operations and eNgineering) operates through a different aperture.

SHERLOC is part of a seven-instrument suite on Perseverance. During development of the mission, the team designed the instrument suite such that the rover could still achieve its science objectives should any single instrument fail, as there is some overlap among the capabilities of the instruments. Along with SHERLOC, PIXL (Planetary Instrument for X-ray Lithochemistry) and SuperCam also perform spectroscopy.

Currently making its way to explore an area nicknamed “Beehive Geyser,” the rover marked its 1,000th Martian day, or sol, on the Red Planet on Dec. 12, 2023 – more than 300 sols beyond its initial prime mission. Since the rover’s landing Feb. 18, 2021, SHERLOC has scanned and provided rich data on 34 rock targets, creating a total of 261 hyperspectral maps of those targets. Featuring a radioisotope power system, Perseverance’s design is based on the agency’s Curiosity Mars rover, which is still going strong after more than 11 years (4,000 sols) on the Red Planet.

More About the Mission

A key objective for Perseverance’s mission on Mars is astrobiology, including the search for 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.

JPL, which is managed for NASA by Caltech in Pasadena, California, built and manages operations of the Perseverance rover.

For more about Perseverance:

mars.nasa.gov/mars2020/

News Media Contacts

Karen Fox / Alana Johnson
NASA Headquarters, Washington
301-286-6284 / 202-358-1501
karen.c.fox@nasa.gov / alana.r.johnson@nasa.gov

DC Agle
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-9011
agle@jpl.nasa.gov

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Anthony Greicius

55 Years Ago: President Nixon Establishes Space Task Group to Chart Post-Apollo Plans

55 Years Ago: President Nixon Establishes Space Task Group to Chart Post-Apollo Plans

In early 1969, the goal set by President John F. Kennedy to land a man on the Moon seemed within reach. A new president, Richard M. Nixon, now sat in the White House and needed to chart America’s course in space in the post-Apollo era. President Nixon directed his science advisor to evaluate proposals for America’s next steps in space. He established a Space Task Group (STG), chaired by Vice President Spiro T. Agnew, to report back to him with their recommendations. The STG delivered its report to President Nixon on Sept. 15, 1969, who declined to select any of the options proposed. Instead, more than two years later, he directed NASA to build the space shuttle, just one element of the ambitious plans the STG had proposed.

President John F. Kennedy announces his goal of a Moon landing during a Joint Session of Congress in May 1961 President Kennedy reaffirms the goal during his address at Rice University in Houston in September 1962
Left: President John F. Kennedy announces his goal of a Moon landing during a Joint Session of Congress in May 1961. Right: President Kennedy reaffirms the goal during his address at Rice University in Houston in September 1962.

On May 25, 1961, President Kennedy, before a Joint Session of Congress, committed the United States to the goal, before the decade was out, of landing a man on the Moon and returning him safely to the Earth. President Kennedy reaffirmed the commitment during an address at Rice University in Houston in September 1962. Vice President Lyndon B. Johnson, who played a key role in establishing NASA in 1958, and under Kennedy served as the Chair of the National Aeronautics and Space Council, worked with members of Congress to ensure adequate funding for the next several years to provide NASA with the proper resources to meet that goal. Following Kennedy’s assassination in November 1963, now President Johnson continued his strong support of the space program to ensure that his predecessor’s goal of a Moon landing could be achieved within the stipulated time frame. But with increasing competition for scarce federal resources from the conflict in southeast Asia and from domestic programs, Johnson showed less interest in any space endeavors that might follow the Moon landing. The space agency’s annual budget peaked in 1966 and began a steady decline three years before Kennedy’s goal was met. From a budgetary standpoint, the prospects of a vibrant post-Apollo space program did not look too rosy, the Apollo triumphs of 1968 and 1969 notwithstanding.

President Richard M. Nixon, right, meets with his science advisor Lee DuBridge in the Oval Office President Nixon, left, and Vice President Spiro T. Agnew, right, introduce Thomas O. Paine as the nominee to be NASA administrator on March 5, 1969
Left: President Richard M. Nixon, right, meets with his science advisor Lee DuBridge in the Oval Office – note the Apollo 8 Earthrise photo on the wall. Right: President Nixon, left, and Vice President Spiro T. Agnew, right, introduce Thomas O. Paine as the nominee to be NASA administrator on March 5, 1969.

On Feb. 4, just two weeks after taking office, President Nixon directed his Science Advisor Lee A. DuBridge to appoint an interagency committee to advise him on a post-Apollo space program. Nine days later, the President announced the formation of the STG to develop a strategy for America’s space program for the next decade. Vice President Agnew, as the Chair of the National Aeronautics and Space Council, led the group. Other members of the STG included NASA Acting Administrator Thomas O. Paine (the Senate confirmed him as administrator on March 20), the Secretary of Defense, and the Director of the Office of Science and Technology.

Proposed lunar landing sites through Apollo 20, per NASA planning in August 1969 Illustration of the Apollo Applications Program experimental space station
Left: Proposed lunar landing sites through Apollo 20, per NASA planning in August 1969. Right: Illustration of the Apollo Applications Program experimental space station.

At the time, the only approved human space flight programs included lunar missions through Apollo 20 and the Apollo Applications Program (AAP), later renamed Skylab, that involved three flights to an experimental space station based on Apollo technology. Beyond a general vague consensus that the United States human space flight program should continue, no approved projects existed to follow these missions when they ended by about 1975.

Concept of a fully reusable space shuttle system from early 1969 Illustration from early 1969 of low Earth orbit infrastructure, including a large space station supported by space shuttles Cover page of NASA’s report to the interagency Space Task Group
Left: Concept of a fully reusable space shuttle system from early 1969. Middle: Illustration from early 1969 of low Earth orbit infrastructure, including a large space station supported by space shuttles. Right: Cover page of NASA’s report to the interagency Space Task Group.

Within NASA, given the intense focus on achieving the Moon landing within President Kennedy’s time frame, officials paid less attention to what would follow the Apollo Program and AAP. During a Jan. 27, 1969 meeting at NASA chaired by Paine, a general consensus evolved that the next step after the Moon landing should involve the development of a 12-person earth-orbiting space station by 1975, followed by an even larger outpost capable of housing up to 100 people “with a multiplicity of capabilities.” In June, with the goal of the Moon landing about to be realized, NASA’s internal planning added the development of a space shuttle by 1977 to support the space station, and truly optimistically, the development of a lunar base by 1976, among other highly ambitious endeavors that included the idea that the U.S. should begin preparing for a human mission to Mars as early as the 1980s. These proposals were presented to the STG for consideration in early July in a report titled “America’s Next Decade in Space.”

The Space Task Group’s (STG) Report to President Nixon Meeting in the White House to present the STG Report to President Nixon
Left: The Space Task Group’s (STG) Report to President Nixon. Right: Meeting in the White House to present the STG Report to President Nixon. Image credit: courtesy Richard Nixon Presidential Library and Museum.

Still bathing in the afterglow of the successful Moon landing, the STG presented its 29-page report “The Post-Apollo Space Program:  Directions for the Future” to President Nixon on Sep. 15, 1969, during a meeting in the White House Cabinet Room. In its Conclusions and Recommendations section, the report noted that the United States should pursue a balanced robotic and human space program but emphasized the importance of the latter, with a long-term goal of a human mission to Mars before the end of the 20th century. The report proposed that NASA develop new systems and technologies that emphasized commonality, reusability, and economy in its future programs. To accomplish these overall objectives, the report presented three options:

Option I – this option required more than a doubling of NASA’s budget by 1980 to enable a human Mars mission in the 1980s, establishment of a lunar orbiting space station, a 50-person Earth orbiting space station, and a lunar base. A decision would be required by 1971 on development of an Earth-to-orbit transportation system to support the space station. A strong robotic scientific and exploration program would be maintained.

Option II – this option maintained NASA’s budget at then current levels for a few years then anticipated a gradual increase to support the parallel development of both an earth orbiting space station and an Earth-to-orbit transportation system, but deferred a Mars mission to about 1986. A strong robotic scientific and exploration program would be maintained, but smaller than in Option I.

Option III – essentially the same as Option II but deferred indefinitely the human Mars mission.

In separate letters, both Agnew and Paine recommended to President Nixon to choose Option II. 

Illustration of a possible space shuttle orbiter from 1969 Illustration of a possible 12-person space station from 1969
Left: Illustration of a possible space shuttle orbiter from 1969. Right: Illustration of a possible 12-person space station from 1969.

The White House released the report to the public at a press conference on Sep. 17 with Vice President Agnew and Administrator Paine in attendance. Although he publicly supported a strong human spaceflight program and enjoyed the positive press he received when photographed with Apollo astronauts, and initially sounding positive about the STG options, President Nixon ultimately chose not to act on the report’s recommendations. Faced with the still ongoing conflict in southeast Asia and domestic programs competing for scarce federal dollars, the fiscally conservative Nixon decided these plans were just too grandiose and far too expensive. He also believed that NASA should be considered as one America’s domestic programs without the special status it enjoyed during the 1960s, one of the lasting legacies of the Nixon space doctrine. Even some of the already planned remaining Moon landing missions fell victim to the budgetary axe. On Jan. 4, 1970, NASA canceled Apollo 20 since it needed its Saturn V rocket to launch the Skylab experimental space station – NASA Administrator James E. Webb had turned off the Saturn V assembly line in 1968 and none remained beyond the original 15 built under contract. In September 1970, reductions in NASA’s budget forced the cancellation of two more Apollo missions, and for a time in 1971 President Nixon considered cancelling two more but he relented, and they flew as the final two Apollo Moon landing missions in 1972.

NASA Administrator James C. Fletcher, left, and President Richard M. Nixon announce the approval to proceed with space shuttle development in 1972 First launch of the space shuttle in 1981
Left: NASA Administrator James C. Fletcher, left, and President Richard M. Nixon announce the approval to proceed with space shuttle development in 1972. Right: First launch of the space shuttle in 1981.

More than two years after the STG submitted its report, in January 1972 President Nixon directed NASA Administrator James C. Fletcher to develop the Space Transportation System, the formal name for the space shuttle, the only element of the recommendations to survive the budgetary challenges. At that time, the first flight of the program was expected in 1979; in actuality, the first flight occurred two years later. It would be 12 years after Nixon’s shuttle decision before President Ronald W. Reagan approved the development of a space station, the second major component of the STG recommendation, and another 14 years after that before the first element of that program reached orbit. In those intervening years, the original American space station had been redesigned and evolved into the multinational partnership called the International Space Station.

The International Space Station as it appeared in 2021
The International Space Station as it appeared in 2021.

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Feb 13, 2024

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Kelli Mars