SaSa NASA Partners

SaSa NASA Partners

2 min read

SaSa NASA Partners

NASA Langley

  • NASA Langley Aerosol Research Group (LARGE)
    • LARGE specializes in making in situ aerosol and cloud measurements and conducting research to improve understanding of atmospheric aerosols and their interactions with water vapor. 
    • LARGE aims to contribute directly to NASA and the Langley Science Directorate goals of translating atmospheric discovery into better solutions to protect the Earth and its people. This is accomplished through investments in people and infrastructure, technology development, and stewardship/dissemination of high-quality data during scientific missions like DISCOVER-AQ and SEAC4RS. To learn more, check out the LARGE website.

Research Group

 The research group supporting the SaSa program includes:  

Instrumentation

Below is a snapshot of instruments and tools Langley uses to support SaSa student projects and the summer airborne science campaigns. More information can be found on the NASA Langley Aerosol Research Group (LARGE) Instruments page.

NASA Goddard

NASA Goddard Space Flight Center (GSFC) has unique assets – aircraft, aircraft sensors and experts – to help create an effective learning environment for students.

Research group

GSFC scientists and engineers support the SaSa program, especially in the maintenance of the CAR instrument. The CAR was designed and operated at NASA GSFC until August 2022, when it was transferred to NASA Ames Research Center. This team is lead by:

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Last Updated

Nov 21, 2023

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Milan Loiacono

Space Biology, Manufacturing Research Helping Plan Future Long-Term Missions

Space Biology, Manufacturing Research Helping Plan Future Long-Term Missions

Astronaut Andreas Mogensen operates a microscope to capture imagery of brain cell-like samples for the Cerebral Ageing space biology study.
Astronaut Andreas Mogensen operates a microscope to capture imagery of brain cell-like samples for the Cerebral Ageing space biology study.

Astronaut health, an aging study, and cargo operations kept the Expedition 70 crew busy on Tuesday. The International Space Station residents also explored space manufacturing and downloaded radiation data.

Scientists representing NASA and its international partners are collecting a multitude of physiological and psychological data from crew members living on the orbital outpost. The observations from the CIPHER suite of 14 human research experiments will help researchers and mission planners understand health issues astronauts may face on future missions. Insights from the space biology study will be especially useful when crews begin traveling longer and farther away from Earth toward the Moon, Mars, and beyond.

NASA astronaut Loral O’Hara spent most of Tuesday contributing to the CIPHER study processing blood and urine samples and participating in a cognition test. She processed the samples in a centrifuge and stowed them in a science freezer for later analysis. Results from the sample analyses and cognition tests will help doctors and astronauts prepare for long-term radiation exposure, isolation, extreme distances, and closed environments.

Aging is a key research topic aboard the space station as researchers study microgravity’s affect on brain cell-like samples. NASA Flight Engineer Jasmin Moghbeli was busy during the morning treating some of those samples inside the Kibo laboratory module’s Life Science Glovebox. The Cerebral Ageing study may provide insights unachievable on Earth into accelerated ageing symptoms, neurodegenerative diseases, and hypersensitivity to ultraviolet radiation on a molecular level. Results may promote advanced health treatments on Earth and in space.

Morale is also a very important characteristic to ensure mission success during long periods in deep space. Scientists are exploring the hypothesis that virtual reality experiences onboard a spacecraft may lead to less stress and greater mental relaxation. Commander Andreas Mogensen from ESA (European Space Agency) took part in that study today, VR Mental Care, wearing VR goggles and a controller, and watching a 360-degree movie to understand its stabilizing effect on the nervous system.

Astronaut Satoshi Furukawa from JAXA (Japan Aerospace Exploration Agency) worked inside the SpaceX Dragon Endurance crew spacecraft checking orbital plumbing gear with assistance from Mogensen. In the Harmony module’s port adjacent to Endurance, Moghbeli worked on cargo transfers inside the Dragon cargo spacecraft as O’Hara photographed some of the specially delivered gear.

3D printing in space is critical as crews traveling farther in space will be less dependent on cargo missions launched from Earth. Veteran cosmonaut Oleg Kononenko printed test samples in a 3D printer to learn how to manufacture tools and supplies on demand in microgravity. The five-time station resident also attached sensors to himself measuring his cardiac activity for a long-running Roscosmos experiment.

Roscosmos Flight Engineer Konstantin Borisov assisted Kononenko with the cardiac sensor attachments, checked camera hardware, then downloaded monthly radiation detection data. Flight Engineer Nikolai Chub explored how spaceflight conditions such as spacecraft vibrations, electric fields, and magnetic fields affect fluid systems.


Learn more about station activities by following the space station blog, @space_station and @ISS_Research on X, as well as the ISS Facebook and ISS Instagram accounts.

Get weekly video highlights at: https://roundupreads.jsc.nasa.gov/videoupdate/

Get the latest from NASA delivered every week. Subscribe here: www.nasa.gov/subscribe

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Mark Garcia

What Is a Black Hole? (Grades 5-8)

What Is a Black Hole? (Grades 5-8)

This article is for students grades 5-8

Black hole with spinning material around it

A black hole is a region in space where the pulling force of gravity is so strong that light is not able to escape. The strong gravity occurs because matter has been pressed into a tiny space. This compression can take place at the end of a star’s life. Some black holes are a result of dying stars.

Because no light can escape, black holes are invisible. However, space telescopes with special instruments can help find black holes. They can observe the behavior of material and stars that are very close to black holes.

High energy light

How Big Are Black Holes?

Black holes can come in a range of sizes, but there are three main types of black holes. The black hole’s mass and size determine what kind it is.

The smallest ones are known as primordial black holes. Scientists believe this type of black hole is as small as a single atom but with the mass of a large mountain.

The most common type of medium-sized black holes is called “stellar.” The mass of a stellar black hole can be up to 20 times greater than the mass of the sun and can fit inside a ball with a diameter of about 10 miles. Dozens of stellar mass black holes may exist within the Milky Way galaxy.

The largest black holes are called “supermassive.” These black holes have masses greater than 1 million suns combined and would fit inside a ball with a diameter about the size of the solar system. Scientific evidence suggests that every large galaxy contains a supermassive black hole at its center. The supermassive black hole at the center of the Milky Way galaxy is called Sagittarius A. It has a mass equal to about 4 million suns and would fit inside a ball with a diameter about the size of the sun.

Close-up of black hole

How Do Black Holes Form?

Primordial black holes are thought to have formed in the early universe, soon after the big bang.

Stellar black holes form when the center of a very massive star collapses in upon itself. This collapse also causes a supernova, or an exploding star, that blasts part of the star into space.

Scientists think supermassive black holes formed at the same time as the galaxy they are in. The size of the supermassive black hole is related to the size and mass of the galaxy it is in.

Black hole Sagittarius A

If Black Holes Are “Black,” How Do Scientists Know They Are There?

A black hole can not be seen because of the strong gravity that is pulling all of the light into the black hole’s center. However, scientists can see the effects of its strong gravity on the stars and gases around it. If a star is orbiting a certain point in space, scientists can study the star’s motion to find out if it is orbiting a black hole.

When a black hole and a star are orbiting close together, high-energy light is produced. Scientific instruments can see this high-energy light.

A black hole’s gravity can sometimes be strong enough to pull off the outer gases of the star and grow a disk around itself called the accretion disk. As gas from the accretion disk spirals into the black hole, the gas heats to very high temperatures and releases X-ray light in all directions. NASA telescopes measure the X-ray light. Astronomers use this information to learn more about the properties of a black hole.

A disk of hot material around a supermassive black hole emits a burst of visible light, which travels out to a ring of dust that subsequently emits infrared light.

Could a Black Hole Destroy Earth?

Black holes do not wander around the universe, randomly swallowing worlds. They follow the laws of gravity just like other objects in space. The orbit of a black hole would have to be very close to the solar system to affect Earth, which is not likely.

If a black hole with the same mass as the sun were to replace the sun, Earth would not fall in. The black hole with the same mass as the sun would keep the same gravity as the sun. The planets would still orbit the black hole as they orbit the sun now.

Flaring, active regions of our sun are highlighted in this image combining observations from NASA's NuSTAR. During the observations, microflares went off, which are smaller versions of the larger flares that also erupt from the sun surface.

Will the Sun Ever Turn Into a Black Hole?

The sun does not have enough mass to collapse into a black hole. In billions of years, when the sun is at the end of its life, it will become a red giant star. Then, when it has used the last of its fuel, it will throw off its outer layers and turn into a glowing ring of gas called a planetary nebula. Finally, all that will be left of the sun is a cooling white dwarf star.

This week in 2008, the Fermi Gamma-ray Space Telescope was launched aboard a Delta II rocket.

How Is NASA Studying Black Holes?

NASA is learning about black holes using spacecraft like the Chandra X-ray Observatory, the Swift satellite and the Fermi Gamma-ray Space Telescope. Fermi launched in 2008 and is observing gamma rays – the most energetic form of light – in search of supermassive black holes and other astronomical phenomena. Spacecraft like these help scientists answer questions about the origin, evolution and destiny of the universe.

_________________________________________________________________________________________

Words to Know

mass: the measurement for the amount of matter in an object

red giant star: a star that is larger than the sun and red
because it has a lower temperature

white dwarf star: a small star, about the size of Earth;
one of the last stages of a star’s life
_________________________________________________________________________________________

More About Black Holes

Space Place in a Snap: What Is a Black Hole?
Black Hole Rescue
Fall Into a Black Hole
Black Holes: By the Numbers Slideshow
Black Hole Travel Postcards

Read What Is a Black Hole? (Grades K-4)

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Sandra May

What Is a Black Hole? (Grades K – 4)

What Is a Black Hole? (Grades K – 4)

This article is for students grades K-4.
 

A black hole is a place in space where gravity pulls so much that even light can not get out. The gravity is so strong because matter has been squeezed into a tiny space. This can happen when a star is dying.

Because no light can get out, people can’t see black holes. They are invisible. Space telescopes with special tools can help find black holes. The special tools can see how stars that are very close to black holes act differently than other stars.

Close-up of a black hole

How Big Are Black Holes?

Black holes can be big or small. Scientists think the smallest black holes are as small as just one atom. These black holes are very tiny but have the mass of a large mountain. Mass is the amount of matter, or “stuff,” in an object.

Another kind of black hole is called “stellar.” Its mass can be up to 20 times more than the mass of the sun. There may be many, many stellar mass black holes in Earth’s galaxy. Earth’s galaxy is called the Milky Way.

The largest black holes are called “supermassive.” These black holes have masses that are more than 1 million suns together. Scientists have found proof that every large galaxy contains a supermassive black hole at its center.

The supermassive black hole at the center of the Milky Way galaxy is called Sagittarius A. It has a mass equal to about 4 million suns and would fit inside a very large ball that could hold a few million Earths.

Black hole with spinning material around it

How Do Black Holes Form?

Scientists think the smallest black holes formed when the universe began.

Stellar black holes are made when the center of a very big star falls in upon itself, or collapses. When this happens, it causes a supernova. A supernova is an exploding star that blasts part of the star into space.

Scientists think supermassive black holes were made at the same time as the galaxy they are in.

Black hole Sagittarius A

If Black Holes Are “Black,” How Do Scientists Know They Are There?

A black hole can not be seen because strong gravity pulls all of the light into the middle of the black hole. But scientists can see how the strong gravity affects the stars and gas around the black hole. Scientists can study stars to find out if they are flying around, or orbiting, a black hole.

When a black hole and a star are close together, high-energy light is made. This kind of light can not be seen with human eyes. Scientists use satellites and telescopes in space to see the high-energy light.

High energy light

Could a Black Hole Destroy Earth?

Even if a black hole the same mass as the sun were to take the place of the sun, Earth still would not fall in. The black hole would have the same gravity as the sun. Earth and the other planets would orbit the black hole as they orbit the sun now.

Black holes do not go around in space eating stars, moons and planets. Earth will not fall into a black hole because no black hole is close enough to the solar system for Earth to do that.

The sun will never turn into a black hole. The sun is not a big enough star to make a black hole.

This week in 2008, the Fermi Gamma-ray Space Telescope was launched aboard a Delta II rocket.

How Is NASA Studying Black Holes?

NASA is using satellites and telescopes that are traveling in space to learn more about black holes. These spacecraft help scientists answer questions about the universe.

More About Black Holes

Space Place in a Snap: What Is a Black Hole?
Black Hole Rescue 
Fall Into a Black Hole

Read What Is a Black Hole? (Grades 5-8)

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Get The Details…
Flint Wild

NASA Selects 11 Space Biology Research Projects to Inform Biological Research During Future Lunar Exploration Missions

NASA Selects 11 Space Biology Research Projects to Inform Biological Research During Future Lunar Exploration Missions

4 min read

NASA Selects 11 Space Biology Research Projects to Inform Biological Research During Future Lunar Exploration Missions

NASA announces the award of eleven grants or cooperative agreements for exciting new Space Biology research that will advance NASA’s understanding of how exposure to lunar dust/regolith impact both plant and animal systems.

As human exploration prepares to go beyond Earth Orbit, Space Biology is advancing its research priorities towards work that will enable organisms to Thrive In DEep Space (TIDES). The ultimate goal of the TIDES initiative is to enable long-duration space missions and improve life on Earth through innovative research. Space Biology supported research will enable the study of the effects of environmental stressors in spaceflight on model organisms, that will both inform future fundamental research, as well as provide valuable information that will better enable human exploration of deep space.

Proposals for these eleven projects were submitted in response to ROSES-2022 Program Element E.9 “Space Biology Research Studies” (NNH22ZDA001N-SBR). This funding opportunity solicited ground studies using plant or animal models (or their associated microbes) to characterize the responses of these organisms to lunar regolith simulant similar to that found at NASA candidate landing sites for future lunar exploration missions. This funding opportunity represents a collaboration between the Space Biology Program and NASA’s Astromaterials Research and Exploration Science (ARES) Division within the Exploration Architecture, Integration, and Science (EAIS) Directorate at the NASA Johnson Space Center, who will be supplying the lunar regolith simulant required for these studies.

Selected studies include (but are not limited to) efforts to 1) test the ability of lunar regolith to act as a growth substrate for crop-producing plants including grains, tomatoes and potatoes, 2) understand how growth in lunar regolith influences plant and microbial interactions, and how in turn, these interactions affect plant development and health, 3) identify and test bioremediation methods/techniques to enhance the ability of regolith to act as a growth substrate, and 4) understand how lunar dust exposure impacts host/microbial interactions in human-analogous model systems under simulated microgravity conditions.

Eleven investigators will conduct these Space Biology investigations from ten institutions in nine states. Eight of these awards are to investigators new to the Space Biology Program. When fully implemented, approximately $2.3 million will be awarded in fiscal years 2024-2027.

Plant Research Investigations

Simon Gilroy, Ph.D. University of Wisconsin, Madison

Tailoring Lunar Regolith to Plant Nutrition

Aymeric Goyer, Ph.D.  Oregon State University

Growth, physiology and nutrition dynamics of potato plants grown on lunar regolith

simulant medium

Christopher Mason, Ph.D. Weill Medical College of Cornell University

Leveraging the microbes of Earth’s extreme environments for sustainable plant growth

in lunar regolith

Thomas Juenger, Ph.D. University of Texas, Austin

Engineering plant-microbial interactions for improved plant growth on simulated lunar regolith

Plant Early Career Research Investigations

Miranda Haus, Ph.D. Michigan State University

The sources and extent of root stunting during growth in lunar highland regolith and its impact on legume symbioses

Joseph Lynch, Ph.D. West Virginia University

The metabolomic impact of lunar regolith-based substrate on tomatoes

Jared Broddrick, Ph.D. NASA Ames Research Center

Phycoremediation of lunar regolith towards in situ agriculture

Shuyang Zhen, Ph.D. Texas A&M AgriLife Research

Investigating the impact of foliar and root-zone exposure to lunar regolith simulant on lettuce growth and stress physiology in a hydroponic system

Plant Small Scale Research Investigations

Kathryn Fixen, Ph.D. University of Minnesota

The impact of lunar regolith on nitrogen fixation in a plant growth promoting rhizobacterium

Animal Research Investigations

Cheryl Nickerson, Arizona State University

Effects of Lunar Dust Simulant on Human 3-D Biomimetic Intestinal Models, Enteric Microorganisms, and Infectious Disease Risks

Afshin Beheshti, Ph.D. NASA Ames Research CenterSpaceflight and Regolith Induced Mitochondrial Stress Mitigated by miRNA-based Countermeasures

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Nov 21, 2023

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