NASA Payload Aims to Probe Moon’s Depths to Study Heat Flow

NASA Payload Aims to Probe Moon’s Depths to Study Heat Flow

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Preparations for Next Moonwalk Simulations Underway (and Underwater)

A science instrument flying aboard the next delivery for NASA’s CLPS (Commercial Lunar Payload Services) initiative could help improve our understanding of the Moon. The Lunar Instrumentation for Subsurface Thermal Exploration with Rapidity, or LISTER, is one of 10 payloads set to be carried to the Moon by the Blue Ghost 1 lunar lander in 2025. The instrument sits upon a white table.
LISTER (Lunar Instrumentation for Subsurface Thermal Exploration with Rapidity) is one of 10 payloads flying aboard the next delivery for NASA’s CLPS (Commercial Lunar Payload Services) initiative. The instrument is equipped with a drilling system and thermal probe designed to dig into the lunar surface.
Photo courtesy: Firefly Aerospace

Earth’s nearest neighboring body in the solar system is its Moon, yet to date humans have physically explored just 5% of its surface. It wasn’t until 2023 – building on Apollo-era data and more detailed studies made in 2011-2012 by NASA’s automated GRAIL (Gravity Recovery and Interior Laboratory) mission – that researchers conclusively determined that the Moon has a liquid outer core surrounding a solid inner core.

As NASA and its industry partners plan for continued exploration of the Moon under Artemis in preparation for future long-duration missions to Mars, improving our understanding of Earth’s 4.5-billion-year-old Moon will help teams of researchers and astronauts find the safest ways to study and live and work on the lunar surface.

That improved understanding is  the primary goal of a state-of-the-art science instrument called LISTER (Lunar Instrumentation for Subsurface Thermal Exploration with Rapidity), one of 10 NASA payloads flying aboard the next delivery for the agency’s CLPS (Commercial Lunar Payload Services) initiative and set to be carried to the surface by Firefly Aerospace’s Blue Ghost 1 lunar lander.

Developed jointly by Texas Tech University in Lubbock and Honeybee Robotics of Altadena, California, LISTER will measure the flow of heat from the Moon’s interior. Its sophisticated pneumatic drill will penetrate to a depth of three meters into the dusty lunar regolith. Every half-meter it descends, the drilling system will pause and extend a custom-built thermal probe into the lunar regolith. LISTER will measure two different aspects of heat flow: thermal gradient, or the changes in temperature at various depths, and thermal conductivity, or the subsurface material’s ability to let heat pass through it.

“By making similar measurements at multiple locations on the lunar surface, we can reconstruct the thermal evolution of the Moon,” said Dr. Seiichi Nagihara, principal investigator for the mission and a geophysics professor at Texas Tech. “That will permit scientists to retrace the geological processes that shaped the Moon from its start as a ball of molten rock, which gradually cooled off by releasing its internal heat into space.”

Demonstrating the drill’s effectiveness could lead to more innovative drilling capabilities, enabling future exploration of the Moon, Mars, and other celestial bodies.. The science collected by LISTER aims to contribute to our knowledge of lunar geology, improving our ability to establish a long-term presence on the Moon under the Artemis campaign.

Under the CLPS model, NASA is investing in commercial delivery services to the Moon to enable industry growth and support long-term lunar exploration. As a primary customer for CLPS deliveries, NASA aims to be one of many customers on future flights. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the development of seven of the 10 CLPS payloads carried on Firefly’s Blue Ghost lunar lander.

Learn more about CLPS and Artemis at:

https://www.nasa.gov/clps

Alise Fisher
Headquarters, Washington
202-358-2546
Alise.m.fisher@nasa.gov

Corinne Beckinger 
Marshall Space Flight Center, Huntsville, Ala. 
256-544-0034  
corinne.m.beckinger@nasa.gov 

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Dec 18, 2024

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Beth Ridgeway
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NASA Knows: How Does the Sun Behave? (Grades 5-8)

NASA Knows: How Does the Sun Behave? (Grades 5-8)

This article is for students grades 5-8.

The Sun is the star of our solar system. Its gravity holds Earth and our planetary neighbors in its orbit. At 865,000 miles (1.4 million km) in diameter, it’s the largest object in our solar system. On Earth, its influence is felt in our weather, seasons, climate, and more. Let’s learn about our dynamic star and its connections to life on Earth.

What is the Sun, and what is it made of?

The Sun is a yellow dwarf star. It is approximately 4.5 billion years old and is in its “main sequence” phase. This means it is partway through its lifecycle with a few billion more years ahead of it.

The Sun is made of hydrogen and helium gases. At its core, hydrogen is fused to form helium. This nuclear reaction creates the Sun’s heat and light. That energy moves outward through the Sun’s radiative zone and convective zone. It then reaches the Sun’s visible surface and lower atmosphere, called the photosphere. Above the photosphere lies the chromosphere, which forms the Sun’s middle atmosphere, and beyond that is the corona, the Sun’s outermost atmosphere.

Spherical diagram of the sun, with a corner area cut out and different internal layers shown in various colors and labeled. Layers, from outer layer to center, are chromosphere, photosphere, subsurface flows, convection zone, radiative zone, core. Surface features labeled include prominence, coronal hole, corona, flare, sun spots
The Sun is a yellow dwarf star with a complex series of layers and features.
NASA

What is the solar cycle?

The Sun goes through a pattern of magnetic activity known as the solar cycle. During each cycle, the Sun experiences a very active period called “solar maximum” and a less active period called “solar minimum.”

During solar maximum, increased magnetic activity creates sunspots. These appear as darker, cooler spots on the Sun’s surface. The more sunspots we can see, the more active the Sun is.

The solar cycle begins at solar minimum, peaks at solar maximum, and then returns to solar minimum. This cycle is driven by the Sun’s magnetic polarity, which flips – north becomes south, and vice versa – every 11 years. It takes two cycles – or 22 years – to complete the full magnetic cycle where the poles return to their original positions.  

A side-by-side view of the rotating Sun, showing solar minimum on the left with a quiet, uniform surface, and solar maximum on the right with multiple solar flares and bright spots visible across the Sun’s surface
The Sun’s level of magnetic activity changes throughout its 11-year solar cycle. During each cycle, the Sun experiences a less-active period called “solar minimum” (left) and a very active period called “solar maximum” (right).
NASA

Wait. The Sun’s magnetic poles can flip??

Yes! Like Earth, the Sun has north and south magnetic poles. But unlike Earth, the Sun’s poles flip regularly. Each 11-year solar cycle is marked by the flipping of the Sun’s poles. The increased magnetic activity during solar maximum makes the north and south poles less defined. As the cycle moves back to solar minimum, the polarization of the poles returns – with flipped polarity.

View of the Sun with magnetic lines around it, blue on top and red on the bottom, with a rectangular magnet in the center with a South pole at the top and North pole at the bottom
Unlike Earth, the Sun’s poles regularly flip with each 11-year solar cycle.
NASA

What is space weather?

Space weather includes phenomena such as solar wind, solar storms, and solar flares. When space weather conditions are calm, there may be little noticeable effect on Earth. But when the Sun is more active, space weather has real impacts on Earth and in space.

Let’s explore these phenomena and how they affect our planet.

Illustration of solar energy radiating from the Sun into space towards Earth, with a blue magnetic field around our planet to protect it
Periods of increased solar activity can cause noticeable effects on Earth and in space.
NASA

What is solar wind?

Solar wind is a stream of charged particles that flow outward from the Sun’s corona. It extends far beyond the orbit of the planets in our solar system. When solar wind reaches Earth, its charged particles interact with Earth’s magnetic field. This causes colorful streams of moving light at Earth’s north and south poles called aurora.

Animation of charged solar particles streaming out into space past Earth. Our planet’s magnetic shield acts as a barrier redirecting particles out and around Earth
Earth’s magnetic field protects our planet from the charged solar particles of the solar wind.
NASA

What are solar storms, solar flares, and coronal mass ejections?

The Sun’s magnetic fields are a tangle of constant motion. These fields twist and stretch to the point that they snap and reconnect. When this magnetic reconnection occurs, it releases a burst of energy that can cause a solar storm.

Solar storms can include phenomena such as solar flares or coronal mass ejections. They happen more frequently around the solar maximum of the Sun’s cycle. A solar flare is an intense burst of light and energy from the Sun’s surface. Solar flares tend to happen near sunspots where the Sun’s magnetic fields are strongest. A coronal mass ejection is a massive cloud of material flowing outward from the Sun. These can occur on their own or along with solar flares.

Bright flashes and ribbons of super-heated materials snake around the Sun’s surface and arc out into space in this pair of close-up videos of solar flares
The Sun’s magnetic field is strongest near sunspots. These active regions of the Sun’s surface release energy in the form of solar flares and coronal mass ejections like these.
NASA

How do these phenomena affect Earth?

When a solar storm erupts towards Earth, our atmosphere and magnetic field protect us from significant harm. However, some impacts are possible, both on Earth and in space. For example, strong solar storms can cause power outages and radio blackouts. GPS signals can be disrupted. Satellite electronics can be affected. And astronauts working outside of the International Space Station could be exposed to dangerous radiation. NASA monitors and forecasts space weather to protect the safety and health of astronauts and spacecraft.

Colorful aurora in hues of green, yellow, purple, and pink seem to cascade over the landscape near Saskatoon in Saskatchewan, Canada
When charged particles from intense solar storms interact with Earth’s magnetic fields, colorful auroras like this one captured in Saskatchewan, Canada, can occur.
NASA

Learn more about the Sun

NASA’s Parker Solar Probe launched in 2018 on the first-ever mission to fly into the Sun’s corona. Since its first pass through the corona in 2021, every orbit has brought it closer to the Sun. On Dec. 24, 2024, it makes the first of its three final, closest solar approaches of its primary mission. Test your knowledge with NASA’s new quiz, Kahoot! Parker Solar Probe trivia.

Visit these resources for more details about the Sun:

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Sandra May

NASA, CU Enact Collaborative Space Act Agreement

NASA, CU Enact Collaborative Space Act Agreement

Jeanette Wing and Christa Peters-Lidard sit at a table draped with a black tablecloth with the NASA logo. They are both holding pens and large white documents with the NASA meatball logo sit in front of each of them. They are mid-conversation and both smiling.
Dr. Jeannette Wing and Dr. Christa Peters-Lidard sign a collaborative Space Act Agreement at NASA’s Goddard Space Flight Center on Monday, Dec. 16, 2024.
NASA/Travis Wohlrab

NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and Columbia University in New York, New York, enacted a collaborative Space Act Agreement to advance research and education opportunities during a signing ceremony Monday, Dec. 16, at Goddard.

Presiding over the ceremony were Dr. Christa Peters-Lidard, director of Goddard’s Sciences and Exploration directorate, and Dr Jeannette Wing, executive vice president for research and professor of computer science at Columbia University.

Columbia University has been a trusted partner for many years and has a long history of interactions with Goddard Space Flight Center. Notably, the Goddard Institute for Space Studies (GISS) is located at Columbia University serving as a laboratory in Goddard’s Earth Sciences Division and is affiliated with the Columbia Climate School and School of Engineering and Applied Science.

The agreement expands NASA’s CU partnership to Goddard’s Greenbelt campus and will be centered around collaborative research, education, technology development, workforce development, science and engineering exchanges, applied science, commercial as well as nonprofit research along with technology infusion.

Areas of mutual interest include but are not limited to: artificial intelligence, foundation models, machine learning, and data science; climate sustainability, justice, adaptation, and resilience; materials and sensors; quantum sensing and computing; Earth science, planetary science, heliophysics, physics and astrophysics.

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Dec 18, 2024

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Katy Mersmann
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OTPS Releases Its 2024 Annual Report

OTPS Releases Its 2024 Annual Report

1 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

OTPS Releases its 2024 Annual Report

NASA’s Office of Technology, Policy, and Strategy, shares highlights from the office in 2024, including key accomplishments and collaborations that support the NASA mission. Read the full report, NASA’s Office of Technology, Policy, and Strategy: A Year in Review 2024

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Dec 18, 2024

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NASA’s Agency Chief Technologist Presents Their Annual Year in Review 2024

NASA’s Agency Chief Technologist Presents Their Annual Year in Review 2024

1 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

OTPS shares an annual letter from the Agency Chief Technologist (ACT), updates on various studies in the technology domain within OTPS, overviews of the center chief technologists, and vignettes of various technology projects across the agency. Read the full report, A Year in Review 2024 from NASA’s Agency Chief Technologist.

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Dec 18, 2024

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