Friends of NASA (FoN) is an independent non-governmental organization (NGO) dedicated to building international support for peaceful space exploration, commerce, scientific discovery, and STEM education.
Maximum Afterburner: NASA's X-59 Supersonic Research Aircraft | Lockheed Martin
NASA's X-59 fires up its jet engine against a darkening sky, showcasing its unique Mach diamonds, also known as shock diamonds, during maximum afterburning testing at Lockheed Martin Skunk Works in Palmdale, California. The test demonstrated the engine's ability to generate the thrust required for supersonic flight, advancing NASA's Quesst Mission.
A closer view of the powerful afterburner exhaust coming from the tail of NASA's X-59 supersonic technology demonstrator, its characteristic Mach diamonds—also known as shock diamonds—visible in the superhot plume.
The nearly 100-foot-long X-59 sits partially inside a large run stall with the rear of the aircraft and its engine extending outside the run stall’s open bay door. Flames are visible from the engine, producing additional thrust during full afterburner tests.
NASA’s X-59 quiet supersonic research aircraft completed its first maximum afterburner test at Lockheed Martin’s Skunk Works facility in Palmdale, California on Dec. 12, 2024. This full-power test, during which the engine generates additional thrust, validates the additional power needed for meeting the testing conditions of the aircraft. The X-59 is the centerpiece of NASA’s Quesst mission. It aims to overcome a major barrier to supersonic flight over land by reducing the noise of sonic booms. This marks a significant milestone as the X-59 team progresses toward flight.
An afterburner is a component of jet engines that generates additional thrust. Running the engine, an F414-GE-100, with afterburner will allow the X-59 to meet its supersonic speed requirements. The test demonstrated the engine’s ability to operate within temperature limits and with adequate airflow for flight. It also showed the engine’s ability to operate in sync with the aircraft’s other subsystems.
The X-59’s first flight is expected to occur in 2025.
The engine, a modified F414-GE-100, packs 22,000 pounds of thrust. This will enable the X-59 to achieve the desired cruising speed of Mach 1.4 (925 miles per hour) at an altitude of approximately 55,000 feet. It sits in a nontraditional spot–atop the aircraft—to aid in making the X-59 quieter.
The X-59's goal is to help change existing national and international aviation rules that ban commercial supersonic flight over land.
Since it arrived at Jupiter in 2016, NASA’s Juno spacecraft has been probing beneath the dense, forbidding clouds encircling the giant planet—the first orbiter to peer so closely. It seeks answers to questions about the origin and evolution of Jupiter, our solar system, and giant planets across the cosmos. Each perijove passes near a new part of Jupiter's cloud tops. A perijove indicates the point in the Juno spacecraft's orbit when it comes closest to planet Jupiter's center.
The Jet Propulsion Laboratory (JPL), a division of Caltech in Pasadena, California, manages the Juno mission for the principal investigator, Scott J. Bolton, of the Southwest Research Institute in San Antonio. Juno is part of NASA’s New Frontiers Program. This is managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington. Lockheed Martin Space in Denver built and operates the spacecraft.
China's FAST Radio Telescope Discovers over 1,000 Pulsars in 2024
China’s Five-hundred-meter Aperture Spherical Telescope (FAST), the world's largest radio telescope, keeps scanning the stars from the remote mountains of Guizhou as the country celebrates Spring Festival. Nicknamed "Sky Eye", FAST runs 24/7, helping scientists uncover the mysteries of space, from faint neutron stars (pulsars) and cosmic radio bursts to low frequency gravitational waves. At least 10 per cent of the available observation time is reserved for international astronomers.
Maintaining a 500-meter telescope, the size of 30 football fields, is a big job.
By November 2024, China’s FAST telescope has found over 1,000 pulsars, more than all other telescopes combined. These spinning stars flash like cosmic lighthouses, sending steady signals that could one day help guide our spaceships through the universe.
The telescope is located in a naturally deep and round karst depression in China's southwestern province of Guizhou.
The primary driving force behind the FAST project was Nan Rendong, a researcher with the Chinese National Astronomical Observatory, part of the Chinese Academy of Sciences. He held the positions of chief scientist and chief engineer of the project. He died September 15, 2017, in Boston, United States due to lung cancer.
Wilmore & Williams on Spacewalk—EVA 274 | International Space Station
NASA astronaut and Expedition 72 Commander Suni Williams' camera is reflected in her spacesuit helmet's visor as she points it toward herself and takes an out-of-this-world "space-selfie" during a five-hour and 26-minute spacewalk. The International Space Station was orbiting 263 miles above the Pacific Ocean at the time of this photograph.
NASA astronaut and Expedition 72 Flight Engineer Butch Wilmore works outside the International Space Station during a five-hour and 26-minute spacewalk. Wilmore swabbed external surfaces searching for microorganisms that may survive and reproduce near vents on the exterior of the orbital outpost. The space station was orbiting into a sunset 259 miles above Eastern Europe at the time of this photograph.
NASA astronaut and Expedition 72 Flight Engineer Butch Wilmore works outside the International Space Station during a five-hour and 26-minute spacewalk. Wilmore swabbed external surfaces searching for microorganisms that may survive and reproduce near vents on the exterior of the orbital outpost.
NASA astronaut and Expedition 72 Flight Engineer Butch Wilmore works outside the International Space Station during a five-hour and 26-minute spacewalk. Wilmore swabbed external surfaces searching for microorganisms that may survive and reproduce near vents on the exterior of the orbital outpost. The space station was orbiting 260 miles above Eastern Europe at the time of this photograph.
NASA astronaut and Expedition 72 Flight Engineer Butch Wilmore works outside the International Space Station during a five-hour and 26-minute spacewalk. Wilmore swabbed external surfaces searching for microorganisms that may survive and reproduce near vents on the exterior of the orbital outpost.
NASA astronaut and Expedition 72 Flight Engineer Butch Wilmore works outside the International Space Station during a five-hour and 26-minute spacewalk. Wilmore swabbed external surfaces searching for microorganisms that may survive and reproduce near vents on the exterior of the orbital outpost.
NASA astronauts Suni Williams and Butch Wilmore concluded their spacewalk at 1:09 p.m. Eastern Standard Time (EST) Jan. 30, 2025. It was the ninth spacewalk for Williams and the fifth for Wilmore, and it was the 274th spacewalk in support of space station assembly, maintenance, and upgrades. Williams surpassed former NASA astronaut Peggy Whitson’s record for total spacewalking time by a female astronaut. Williams now has 62 hours, 6 minutes of total spacewalk time, fourth on NASA’s all-time list.
Williams and Wilmore completed their primary objectives, including removing a radio frequency group antenna assembly from the station’s truss and collecting samples of surface material for analysis from the Destiny laboratory and the Quest airlock.
Station Commander: Suni Williams Roscosmos (Russia) Flight Engineers: Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov NASA Flight Engineers: Butch Wilmore, Don Pettit, Nick Hague
An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.
Image Credit: NASA's Johnson Space Center (JSC) Capture Date: Jan. 30, 2025
Europe's Gaia Mission Finds a Mysterious Planet and Brown Dwarf | ESA
New research, published on February 4, 2025, uses data collected by the European Space Agency’s Gaia spacecraft to confirm the existence of two mysterious celestial objects. Gaia-4b is a ‘Super-Jupiter’ exoplanet, and Gaia-5b a brown dwarf. These massive objects are unexpectedly orbiting low-mass stars.
Gaia-4b is a planet orbiting the previously unremarkable star Gaia-4 around 244 light-years away. Gaia-5b orbits the Gaia-5 star, around 134 light-years away from Earth. These two newly discovered objects are nearby, in our own galactic neighborhood. Their existence challenges current theories of planet formation, and Gaia's ongoing mission will provide valuable data to help us understand these intriguing objects.
“Gaia-4b is about twelve times more massive than Jupiter. With an orbital period of 570 days, it is a relatively cold gas giant planet,” explains first author Guðmundur Stefánsson of the University of Amsterdam, the Netherlands, and first author of the new study.
“With a mass of around 21 Jupiters, Gaia-5b is a brown dwarf, more massive than a planet but too light to sustain nuclear fusion to be a star,” Guðmundur adds.
This is the first time a planet has been uniquely discovered by Gaia’s ability to sense the gravitational tug or ‘wobble’ the planet induces on a star.
Grand Canyons on The Moon's Far Side: Vallis Schrödinger & Vallis Planck | NASA LRO
The Schrödinger impact crater sits near to the Moon’s south pole. Sprouting off it are two canyons—called Vallis Schrödinger and Vallis Planck—each comparable in size to the Grand Canyon here on Earth. These were formed when debris, thrown up by a meteor or comet hitting the Moon, crashed back into the surface.
Now, analysis suggests that these high-energy streams of rock could have excavated the canyons in under ten minutes.
Vallis Schrödinger (Latin for "Schrödinger Valley") is a long, nearly linear valley that lies on the far side of the Moon. It is oriented radially to the huge Schrödinger basin and most likely was formed during the original impact that created Schrödinger.
Vallis Planck is a long, linear valley located on the far side of the Moon. It is oriented radially to the huge Schrödinger basin, and was most likely formed by that impact. The selenographic coordinates of this feature are 58.4°S 126.1°E, and it has a length of 451 km.
Understanding this area of the Moon is important as the region has been selected for investigation as part of NASA’s Artemis missions.
This year, NASA's Lunar Reconnaissance Orbiter (LRO) will celebrate its 16th anniversary orbiting the Moon (2009-2025). This mission has given scientists the largest volume of data ever collected by a planetary science mission at NASA. Considering that success and the continuing functionality of the spacecraft and its instruments, NASA awarded the mission an extended mission phase to continue operations. This is LRO's 5th extended science mission (ESM5). LRO continues to be one of NASA's most valuable tools for advancing lunar science.
Video Credit: Science Journal Nature
Image Credits: NASA, LRO, Arizona State University (ASU)
NASA’s PUNCH Solar Wind Mission | Goddard Space Flight Center
NASA’s Polarimeter to Unify the Corona and Heliosphere, or PUNCH Mission, is a constellation of four small satellites in low Earth orbit that will make global, 3D observations of the Sun’s corona to better understand how the mass and energy there becomes the solar wind that fills the solar system.
Watch the video to learn how imaging the Sun’s corona and the solar wind together will help scientists better understand the entire inner heliosphere—Sun, solar wind, and Earth—as a single connected system.
Since it arrived at Jupiter in 2016, NASA’s Juno spacecraft has been probing beneath the dense, forbidding clouds encircling the giant planet—the first orbiter to peer so closely. It seeks answers to questions about the origin and evolution of Jupiter, our solar system, and giant planets across the cosmos. Each perijove passes near a new part of Jupiter's cloud tops. A perijove indicates the point in the Juno spacecraft's orbit when it comes closest to planet Jupiter's center.
The Jet Propulsion Laboratory (JPL), a division of Caltech in Pasadena, California, manages the Juno mission for the principal investigator, Scott J. Bolton, of the Southwest Research Institute in San Antonio. Juno is part of NASA’s New Frontiers Program. This is managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington. Lockheed Martin Space in Denver built and operates the spacecraft.
China Commercial Startup Building Reusable Passenger Spaceplane: Flight Animation
China commercial startup Space Transportation, also known as Lingkong Tianxing Technology, tested a hypersonic prototype of their passenger spaceplane during late January 2025. This vehicle design involves two reusable rocket boosters and a reusable rocket plane, combining vertical takeoff and landing operations. It would be capable of a 1-hour trip from Shanghai, China, to Dubai in the United Arab Emirates—a distance of over 6,400 km or nearly 4,000 miles. Founded in 2018 by Yudong Wang, Space Transportation focuses on reducing the costs of space exploration and on developing spaceplanes, plus hypersonic and supersonic aircraft. As testing continues, Space Transportation’s ambitious goal is to make commercial spaceplane, along with supersonic and hypersonic travel, an everyday reality. It may soon help to introduce a new era in global transportation.
This vehicle is being developed by Sichuan Lingkong Tianxing Technology as part of a parallel effort to develop a supersonic passenger jet capable of Mach 4.1, over twice as fast as the British-French Concorde supersonic plane, according to the company. Supersonic aircraft development has been delayed for decades due to challenges, such as noise, economic feasibility, and a lack of mature technology.
The Bullseye Galaxy: LEDA 1313424 in Pisces | Hubble Space Telescope
High-resolution imagery from the NASA/European Space Agency Hubble Space Telescope has allowed researchers to hone in on more of the Bullseye galaxy’s rings—and helped confirm the galaxy that dove through its core.
LEDA 1313424, aptly nicknamed the Bullseye, is two and a half times the size of our Milky Way and has nine rings—six more than any other known galaxy. Hubble has confirmed eight rings, and data from the W. M. Keck Observatory in Hawaii confirmed a ninth. Hubble and Keck also identified the galaxy thatdove through the Bullseye, creating these rings: the blue dwarf galaxy sitting to its immediate center-left. This relatively tiny interloper traveled like a dart through the core of the Bullseye about 50 million years ago, leaving rings in its wake like ripples in a pond. A thin trail of gas now links the pair, though they are currently separated by 130,000 light-years.
Ax-4 Mission | Crew Press Conference | Axiom Space
Axiom Space held a virtual press conference with the astronauts of Axiom Mission 4 (Ax-4), the company’s fourth commercial astronaut mission to the International Space Station. The Ax-4 crew presented their training and experience, preparedness, and mission objectives. This was the first opportunity for reporters to talk with the full Ax-4 crew.
The Ax-4 mission will “realize the return” to human spaceflight for India, Poland, and Hungary, with each nation’s first and only government-sponsored flight taking place more than 40 years ago. While Ax-4 marks each nation’s second human spaceflight mission in history, it will be the first time all three nations will execute a mission on board the space station. This historic mission underscores how Axiom Space is redefining the pathway to low-Earth orbit and elevating national space programs globally.
The Ax-4 crew includes Commander Peggy Whitson of the United States, Mission Pilot Shubhanshu Shukla of India, Mission Specialist Sławosz Uznański-Wiśniewski of the European Space Agency (ESA)/Poland, and Mission Specialist Tibor Kapu of Hungary.
A SpaceX Falcon 9 rocket will launch the Ax-4 crew aboard a SpaceX Dragon spacecraft to the space station from Florida no earlier than spring 2025. Once docked, the Ax-4 astronauts plan to spend up to 14 days on board implementing a full mission comprised of microgravity research, technology demonstrations, educational outreach, and media events.
The star that should have exploded already: T Coronae Borealis | ESO
T Coronae Borealis, nicknamed the Blaze Star, erupts every 80 years or so, becoming visible to the naked eye. Based on recent behavior the star should have flared again in late 2024, but it did not! Astronomers are thus eagerly waiting for this imminent explosion. In this episode of Chasing Starlight we tell you how professional telescopes can quickly react to sudden cosmic events like this one.
T Coronae Borealis (T CrB), nicknamed the Blaze Star, is a binary star and a recurrent nova about 3,000 light-years (920 pc) away in the constellation Corona Borealis.
Video Credits: European Southern Observatory (ESO) Directed by: L. Calçada, M. Kornmesser Hosted by: S. Randall Written by: H. Huysegoms Editing: M. Kornmesser, L. Calçada Videography: A. Tsaousis Animations & footage: ESO, M. Kornmesser, Liam Young, B. Tafreshi, ESA/Hubble, VPHAS+ team, P. Horálek, L. Calçada, H. Zodet Scientific Consultant: P. Amico Filming Locations: ESO Supernova Duration: 5 minutes Release Date: Jan. 31, 2025
What is happening to Comet G3 ATLAS? After passing near the Sun in mid-January 2025, the head of the comet has become dimmer and dimmer. By late January, the comet had become a headless wonder—although it continued to show impressive tails after sunset in the skies of Earth's Southern Hemisphere. A key reason is likely that the comet's nucleus of ice and rock, at the head's center, has fragmented. Comet G3 ATLAS passed well inside the orbit of planet Mercury when at its solar closest, a distance that where heat destroys many comets. Some of comet G3 ATLAS' scattering remains will continue to orbit the Sun . . .
Image Description: In a gradient from orange-red to green-blue, this image captures the Comet C/2024 G3 around dusk. The background is covered by countless stars of all sizes. At the forefront, the comet appears as a white feather-shaped object. The core of the comet (its tip) is bright white. From there, two tails originate: towards the right projects a fainter tail, almost like a veil. Approaching the top, it projects a brighter tail, almost looking like the bushy tail of a cat. It becomes fainter the further you go from the comet’s core.
This impressive image of comet C/2024 G3 ATLAS was captured on January 29, 2025, from the European Southern Observatory's Paranal Observatory by Abel de Burgos Sierra, ESO Fellow in Chile. Gas and dust particles are ejected from the nucleus and pushed away from the Sun by the solar wind and radiation, creating a spectacular display with multiple tails.
Credit: A. de Burgos Sierra/European Southern Observatory (ESO) Release Date: Feb. 3, 2025
China commercial startup Space Transportation, also known as Lingkong Tianxing Technology, tested a prototype of their hypersonic passenger spaceplane during late January 2025, as shown in a released clip of a vertical takeoff. Founded in 2018 by Yudong Wang, Space Transportation focuses on reducing the costs of space exploration and on developing hypersonic aircraft. As testing continues, Space Transportation’s ambitious goal is to make commercial hypersonic travel a reality. It may soon introduce a new era in global transportation. The vehicle design involves two reusable rocket boosters and a reusable rocket plane. It would be capable of a 1-hour trip from Shanghai, China, to Dubai in the United Arab Emirates—a distance of over 6,400 km or nearly 4,000 miles.
This vehicle is being developed by Sichuan Lingkong Tianxing Technology as part of a parallel effort to develop a supersonic passenger jet capable of Mach 4.1, over twice as fast as the British-French Concorde supersonic plane, according to the company. Supersonic aircraft development has been delayed for decades due to challenges, such as noise, economic feasibility, and a lack of mature technology.