Suggested Searches

CP-22 Science

The Intuitive Machines Nova-C lander (IM-3) will deliver six NASA CLPS science payloads to Mons Mouton.

A rendering of the Intuitive Machines lunar lander Nova-C slowly lowering itself to the lunar surface. There is a plume of fire underneath that signifies the counter-boost to ensure a soft landing.

The Marvelous Mons Mouton

At about 4.3 billion years old, over 20,000 feet high, and with a high likelihood of containing life-sustaining materials, Mons Mouton is practically begging to be studied — and we’re happy to oblige. CP-22 will set up camp in this lunar science wonderland, where its payloads will collect data on everything from the Moon’s history to its material composition to human habitability.

Science, Exploration, and Technology Goals

  • Study Deep Space’s Effect on Humans

    Deep space radiation just hits different.

    The Earth’s atmosphere and magnetosphere are very kind to the human body. Deep space? Not so much. As humans prepare to spend more and more time far away from our planet, it’s vital we protect our astronauts by establishing a more thorough understanding of how the deep space environment influences the human body. One clever and helpful way we can do this without humans being physically present is by studying the effects that radiation and the lunar environment have on yeast cells using LEIA.

  • Investigate Magnetic Anomalies

    Our attraction to lunar science is downright magnetic. The Moon almost certainly used to have a magnetic field, but now it doesn’t. Interestingly though, there are magnetic anomalies scattered across the lunar surface. Researching these anomalies using MAG will unlock more insights about the geological history of our Moon and help us better understand the potential effects of changes to the Earth’s magnetosphere.

  • Study the Impact of Lunar Landings

    Subtlety is not exactly lunar landings’ strong suit. Heat, chemicals, and regolith displacement from the thrusters alter the local environment in a way that can affect data being collected by instruments. In turn, this data changes our understanding of everything from the Earth-Moon history to the habitability of the lunar surface. To make our data collection near landing spots more accurate, we need to study the effects of landing on the lunar surface and exosphere using tools like SEAL.

  • Hunt for Essential Materials

    We want to establish a consistent human presence on the lunar surface, and unless we’ve really missed something with LRO, there doesn’t seem to be any grocery or hardware stores on the Moon. This means we have to create and maintain a life-sustaining environment using locally sourced materials. Remote sensing data tells us that there are some crucial elements hiding under the Moon’s hood. We will use PROSPECT and L-CIRiS to help locate nearby chemical compounds that could provide water, oxygen, fuel, and building materials that could allow humans to establish permanent settlements on the Moon.

Because Mons Mouton is relatively untouched by bombardments, scientists believe it is much more ancient – possibly billions of years older — than its surroundings.
NASA's Scientific Visualization Studio

LEIA

Lunar Explorer Instrument for space biology Applications

PIs: Andrew Mark Settles, Dr. Sergio Santa Maria. NASA Ames Research Center

You might not know by looking at it, but the DNA in human cells has a lot in common with the DNA in yeast. So in our quest to better understand the effects of the lunar environment and deep space on the human body, we’re sending LEIA to the lunar surface.

LEIA will house yeast cells along with three small payloads that scientists can use to remotely monitor the yeast. One will nourish the cells and measure the responses, another will measure their radiation exposure, and a third will measure radiation levels on the lunar surface.

Our findings should help us maintain safe and lengthy stays in deep space for humans.

Pair of gloved hands holding a rectangular clear manifold containing two black square fluidic cards. Tubes filled with blue dye are connected to the manifold.
On Lunar Explorer Instrument for space biology Applications (LEIA), a microfluidic card houses dry yeast cells in tiny compartments between electronics that control temperature and optics.
NASA/Dominic Hart

PROSPECT

Package for Resource Observation and in-Situ Prospecting for Exploration, Commercial exploitation and Transportation

European Space Agency (ESA)

PROSPECT, developed by the European Space Agency (ESA)e, is much more than an ordinary drill; it’s a highly advanced multi-function tool used to capture images of the surrounding area, pierce the rough lunar surface, measure depth temperatures, extract material samples, and analyze the materials during and after drilling. To put it very simply, when it comes to collection and analysis of lunar surface material, PROSPECT does it all.

Lunar ice and oxygen are at the top of PROSPECT’s wish list. Humans require water and oxygen to survive (we’re so high maintenance), so if we’re able to generate drinkable water, breathable air, or even rocket fuel from materials that already exist on the Moon, it would allow for permanent human settlements there.

A close-up image of the Prospect drill head. There are heating coils wrapped around the drill bit.
ESA’s Prospect payload package is a comprehensive suite of hardware designed around a drill that will allow extraction of samples at the Moon’s poles in search of icy volatiles such as water ice.
Leonardo Space

L-CIRiS

Lunar Compact Infrared Imaging System

PI: Dr. Paul Hayne, University of Colorado

Imagine if you could look around and accurately identify the material and temperature of everything you see. That’s exactly what L-CIRiS will do on the lunar surface.

L-CIRiS is a multispectral imaging radiometer, which is basically a substance-identifier, thermal camera, and regular camera rolled into one. It will perform 360° panoramic scans and provide in-depth analysis of the surroundings, measuring temperatures from -170°C (-274°F) to +100°C (212°F) and mineral composition at an unprecedented resolution.

Data from L-CIRiS aims to provide insight into the Moon’s formation and geologic evolution, identify potential exploration hazards, and help us discover the ultimate treasure — water ice.

A well-lit laboratory photo of a small covered octogonal instrument situated on a mounting plate.
The Compact Infrared Imaging System (LV-CIRiS) is a multispectral imaging radiometer used to map variations in silicate composition and thermophysical properties of rocks and regolith at high spatial resolution.
Ball Aerospace

SEAL

Surface and Exosphere Alterations by Landers

PI: Dr. Mehdi Benna, NASA Goddard Space Flight Center

Lunar landings have some massive effects on the lunar surface. SEAL is an instrument designed to help us understand these effects. It will analyze regolith (think of it like “Moon dirt”) before, during, and after descent. It works like a molecular detector that can “sniff out” different gases and particles by their unique signatures by measuring changes in heat, chemical exhaust, and physical behavior.

Data provided by SEAL will allow scientists to better distinguish between natural lunar materials and contamination from human activities. This ensures more accurate analysis of lunar samples and will advance scientific context for past and future specimens.

A close up photo of a small device with electronic parts assembled in a rectangular block, and topped with a small metallic cylindrical protector.
Surface and Exosphere Alterations by Landers (SEAL) aims to investigate the interaction of lunar regolith with volatiles from the lander's rocket exhaust.
NASA Goddard Space Flight Center

MAG

Fluxgate Magnetometer

NASA Goddard Space Flight Center

A Fluxgate Magnetometer (MAG) measures the magnetic field of a planetary body like the Earth or Moon. It essentially acts as a high-tech compass, but instead of using a magnetized needle to point you home, it has a magnetically sensitive core wrapped in sets of coils to provide precise measurements. These sensitive instruments can magnetic anomalies on the lunar surface.

While the Moon no longer has a complete magnetic field, it may have had one billions of years ago, and MAG can still help us understand the history of the Moon, its inner structure, and its surface features. And, in many ways, the study of the Moon is the study of the Earth — we’ll better understand our own planet and history by studying our nearest neighbor.

An octagonal device about the size of a small toaster sits on a laboratory table before a worker wearing a white full-body covering in a clean room at NASA's Jet Propulsion Laboratory.
The Fluxgate Magnetometer (MAG) will characterize certain magnetic fields to improve the understanding of energy and particle pathways at the lunar surface.
NASA/JPL-Caltech

LRA

Laser Retroreflector Array

PI: Dr. Xiaoli Sun, GSFC

The Laser Retroreflector Array (LRA) is the ultimate sidekick to any lunar surface payload. Payload-collected data needs precise locations to maximize its effectiveness and accuracy, and LRA does exactly that. LRA uses reflected laser light from orbiting spacecraft to determine its exact location, including a precise distance to Earth.

Laser Retroreflector Array (LRA) payload
The Laser Retroreflector Array (LRA) has eight retroreflectors inside. It will be mounted on Astrobotic’s Peregrine lander deck and help provide precision measurements of distances between orbiting or landing spacecraft.
NASA / GSFC