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We don’t yet know what dark matter is, yet it makes up 85% of all the matter in the universe. The Roman Space Telescope will aim to unravel the mystery. With a field of view 100 times wider than the Hubble Space Telescope’s, Roman will study in near-infrared light the atmospheres of planets orbiting other stars, making other exoplanet discoveries along the way. The mission is named after Dr. Nancy Grace Roman, NASA’s first chief of astronomy and advocate for the development of the Hubble Space Telescope.

Robots inspired by nature? A novel realm of engineering called soft robotics is being studied at NASA’s Langley Research Center. Engineers are working to understand how soft robotics could one day support space exploration, including missions to the Moon’s surface.

Cleaning scum from bathtubs and pipes can be a costly chore. It’s even more challenging aboard spacecraft. NASA researchers are looking at ways to keep astronauts from having to deal with fungal or bacterial buildup, known as biofilm.

The Internet of Animals, a collaborative research project with the National Oceanographic and Atmospheric Administration, U.S. Geological Survey, and other universities and institutions, is giving insight into the intersection of animal movement patterns and climate. By combining remote sensing data with wildlife tracking tags, experts can get a better idea of scientific needs to manage conservation at the federal level.

In this episode, Dr. Gioia Massa, senior Life Sciences project scientist at NASA’s Kennedy Space Center, outlines the systems and processes used for growing vegetables aboard the International Space Station. The technology could one day support astronauts on long-duration missions in deep space. What we learn can benefit agriculture on Earth as well.

A new NASA report titled "Cost and Benefit Analysis of Mitigating, Tracking, and Remediating Orbital Debris" compares the cost-effectiveness of several strategies that could reduce the risk of collisions between spacecraft, including the space station, and orbital debris.

In this episode, Jacob Bleacher, NASA’s chief exploration scientist, tells us about the science goals of the Artemis Lunar Terrain Vehicle and how NASA is collaborating with industry to explore more of the Moon’s surface than ever before

In this episode, Dr. Chelle Gentemann, Open Science Program Scientist for the Office of the Chief Science Data Officer, explains NASA’s initiative to make science more collaborative, accessible, and inclusive. Known as Transform to Open Science, or TOPS, the program encourages increased access to research and data.

How inflatable habitats moved from concept papers to the International Space Station, and what NASA is doing to eventually put one on the Moon.

Dave Mitchell brings extensive experience as an engineer and project manager to a new position leading a small team with the broad mandate of improving acquisitions and program and project management across NASA.

In this episode we’ll focus on Gateway, a small space station NASA is developing to place in orbit at the Moon. We’ll speak with Mark Wiese, who leads the team that will ensure Gateway will receive the cargo, equipment, and supplies it needs to support Artemis astronauts.

Janet Karika, who retired recently from NASA after 43 years in the aerospace industry, shares career highlights and her approach to leading the Artemis I Lessons Learned process.

Dive deep into the world of in-space manufacturing (ISM) with our guest, Zach Courtright, the In-Space Manufacturing Portfolio Manager at NASA. Zach shares his perspectives on cutting-edge advancements and collaborations in the field and the potential of the technology for game-changing impacts on space exploration and resource utilization.

Today, we look at NASA’s PACE mission, which seeks to unravel some of the mysteries of Earth’s atmosphere and the vital role played by aerosols and clouds. Join us as we delve into this fascinating journey with atmospheric scientist Dr. Kirk Knobelspiesse.

In this episode, we step behind the scenes of NASA's Orion project to explore the remarkable teamwork, leadership, and communication that drive this groundbreaking endeavor. Join us as we sit down with Stu McClung, the NASA Orion Test lead, to talk about the Orion mission and the human side of space exploration.

In this episode, we chat with Dr. Zach Pirtle, a policy analyst for NASA’s Office of Technology, Policy and Strategy about NASA’s Artemis and Ethics workshop, which explored the ethical, legal, and societal implications of its Artemis and Moon to Mars missions.

In this episode, we sit down with Jim Rostohar, Chief Knowledge Officer for NASA's Johnson Space Center, to explore the vital role of knowledge sharing within the organization.

Developing and testing rocket propulsion systems, it’s really foundational to spaceflight and to everything that we’re trying to do with spaceflight.

The data cover the region near the supermassive black hole at the center of the Milky Way galaxy. The black hole, known as Sagittarius A*, is barely seen in the lower right-hand of the visual image that contains X-ray data from IXPE (red-orange) and Chandra (purple). In the sonification of these data, the cursor begins at Sagittarius A* and moves out as a growing circle toward the center of the image. As it encounters IXPE data, the volume of the notes changes according to the brightness of the X-rays. The brighter the Chandra data, the higher the musical pitch and vice versa. When the cursor travels over a large patch of X-rays both from Chandra and IXPE in the center of the image, a rushing sound is heard. This region is where scientists find a “light echo,” a high-energy relic left behind from an eruption from Sagittarius A* about 200 years ago. NASA/CXC/SAO/K.Arcand, SYSTEM Sounds (M. Russo, A. Santaguida)

Messier 104 (M104 for short), located about 28 million light-years from Earth, is one of the largest galaxies in the nearby Virgo cluster. As seen from Earth, the galaxy is angled nearly edge-on allowing a view of its bright core and spiral arms wrapped around it. Spitzer's infrared view of M104 shows a ring of dust circling the galaxy that pierces through the obscuring dust in Hubble’s optical light image. Spitzer also sees an otherwise hidden disk of stars within the dust ring. The Chandra X-ray image shows hot gas in the galaxy and point sources that are a mixture of objects within M104 as well as quasars in the background. The Chandra observations show that diffuse X-ray emission extends over 60,000 light years from the center of the M104. (The galaxy itself spans 50,000 light years across.) In sonifying these data, we can listen to each type of light either separately or together. Either option begins at the top and scans toward the bottom of the image. The brightness controls the volume and the pitch, meaning the brightest sources in the image are the loudest and highest frequencies. The data from the three telescopes are mapped to different types of sounds. The X-rays from Chandra sound like a synthesizer, Spitzer’s infrared data are strings, and optical light from Hubble has bell-like tones. The core of the galaxy, its dust lanes and spiral arms, and point-like X-ray sources are all audible features in the sonification of these data.