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By NASA
This artist’s illustration represents the results from a new study that examines the effects of X-ray and other high-energy radiation unleashed on potential exoplanets from Wolf 359, a nearby red dwarf star. Researchers used Chandra and XMM-Newton to study the impact of steady X-ray and energetic ultraviolet radiation from Wolf 359 on the atmospheres of planets that might be orbiting the star. They found that only a planet with greenhouse gases like carbon dioxide in its atmosphere and at a relatively large distance away from Wolf 359 would have a chance to support life as we know it.X-ray: NASA/CXC/SAO/S.Wolk, et al.; Illustration: NASA/CXC/SAO/M.Weiss; Image processing: NASA/CXC/SAO/N. Wolk Planets around other stars need to be prepared for extreme weather conditions, according to a new study from NASA’s Chandra X-ray Observatory and ESA’s (European Space Agency’s) XMM-Newton that examined the effects of X-rays on potential planets around the most common type of stars.
Astronomers found that only a planet with greenhouse gases in its atmosphere like Earth and at a relatively large distance away from the star they studied would have a chance to support life as we know it around a nearby star.
Wolf 359 is a red dwarf with a mass about a tenth that of the Sun. Red dwarf stars are the most common stars in the universe and live for billions of years, providing ample time for life to develop. At a distance of only 7.8 light-years away, Wolf 359 is also one of the closest stars to the solar system.
“Wolf 359 can help us unlock the secrets around stars and habitability,” said Scott Wolk of the Center for Astrophysics | Harvard & Smithsonian (CfA), who led the study. “It’s so close and it belongs to such an important class of stars – it’s a great combination.”
Because red dwarfs are the most prevalent types of stars, astronomers have looked hard to find exoplanets around them. Astronomers have found some evidence for two planets in orbit around Wolf 359 using optical telescopes, but those conclusions have been challenged by other scientists.
“While we don’t have proof of planets around Wolf 359 yet, it seems very possible that it hosts multiple planets,” Wolk added. “This makes it an excellent test bed to look at what planets would experience around this kind of star.”
Wolk and his colleagues used Chandra and XMM to study the amounts of steady X-rays and extreme ultraviolet (UV) radiation – the most energetic type of UV radiation – that Wolf 359 would unleash on the possible planets around it.
They found that Wolf 359 is producing enough damaging radiation that only a planet with greenhouse gases like carbon dioxide in its atmosphere – and located at a relatively large distance from the star – would likely be able to sustain life.
“Just being far enough away from the star’s harmful radiation wouldn’t be enough to make it habitable,” said co-author Vinay Kashyap, also of CfA. “A planet around Wolf 359 would also need to be blanketed in greenhouse gases like Earth is.”
To study the effects of energetic radiation on the habitability of the planet candidates, the team considered the star’s habitable zone – the region around a star where liquid water could exist on a planet’s surface.
The outer limit of the habitable zone for Wolf 359 is about 15% of the distance between Earth and the Sun, because the red dwarf is much less bright than the Sun. Neither of the planet candidates for this system is located in Wolf 359’s habitable zone, with one too close to the star and the other too far out.
“If the inner planet is there, the X-ray and extreme UV radiation it is subjected to would destroy the atmosphere of this planet in only about a million years,” said co-author Ignazio Pillitteri of CfA and the National Institute for Astrophysics in Palermo, Italy.
The team also considered the effects of radiation on as-yet undetected planets within the habitable zone. They concluded that a planet like the Earth in the middle of the habitable zone should be able to sustain an atmosphere for almost two billion years, while one near the outer edge could last indefinitely, helped by the warming effects of greenhouse gases.
Another big danger for planets orbiting stars like Wolf 359 is from X-ray flares, or occasional bright bursts of X-rays, on top of the steady, everyday output from the star. Combining observations made with Chandra and XMM-Newton resulted in the discovery of 18 X-ray flares from Wolf 359 over 3.5 days.
Extrapolating from these observed flares, the team expects that much more powerful and damaging flares would occur over longer periods of time. The combined effects of the steady X-ray and UV radiation and the flares mean that any planet located in the habitable zone is unlikely to have a significant atmosphere long enough for multicellular life, as we know it on Earth, to form and survive. The exception is the habitable zone’s outer edge if the planet has a significant greenhouse effect.
These results were presented at the 245th meeting of the American Astronomical Society in National Harbor, Maryland, and are being prepared for publication in a journal. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
Read more from NASA’s Chandra X-ray Observatory.
Learn more about the Chandra X-ray Observatory and its mission here:
https://www.nasa.gov/chandra
https://chandra.si.edu
News Media Contact
Megan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998
mwatzke@cfa.harvard.edu
Lane Figueroa
Marshall Space Flight Center, Huntsville, Alabama
256-544-0034
lane.e.figueroa@nasa.gov
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By European Space Agency
Last night a crucial step in the European Space Agency’s eclipse-making Proba-3 mission was completed: the two spacecraft, flying jointly since launch, have successfully separated. This leaves them ready to begin their cosmic dance in the world’s first-ever precision formation-flying mission.
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By NASA
Firefly Aerospace’s Blue Ghost lander getting encapsulated in SpaceX’s rocket fairing ahead of the planned liftoff for 1:11 a.m. EST Jan. 15 from Launch Complex 39A at NASA’s Kennedy Space Center in FloridaSpaceX As part of NASA’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign, the agency is preparing to fly ten instruments aboard Firefly Aerospace’s first delivery to the Moon. These science payloads and technology demonstrations will help advance our understanding of the Moon and planetary processes, while paving the way for future crewed missions on the Moon and beyond, for the benefit of all.
Firefly’s lunar lander, named Blue Ghost, is scheduled to launch on a SpaceX Falcon 9 rocket Wednesday, Jan.15, from Launch Complex 39A at NASA’s Kennedy Space Center in Florida. After a 45-day cruise phase, Blue Ghost is targeted to land near a volcanic feature called Mons Latreille within Mare Crisium, a basin approximately 340 miles wide (550 kilometers) located in the northeast quadrant of the Moon’s near side.
How can we enable more precise navigation on the Moon? How do spacecraft interact with the lunar surface? How does Earth’s magnetic field influence the effects of space weather on our home planet? NASA’s instruments on this flight will conduct first-of-their-kind demonstrations to help answer these questions and more, including testing regolith sampling technologies, lunar subsurface drilling capabilities, increasing precision of positioning and navigation abilities, testing radiation tolerant computing, and learning how to mitigate lunar dust during lunar landings.
The ten NASA payloads aboard Firefly’s Blue Ghost lander include:
Lunar Instrumentation for Subsurface Thermal Exploration with Rapidity (LISTER) will measure heat flow from the Moon’s interior by measuring the thermal gradient, or changes in temperature at various depths, and thermal conductivity, or the subsurface material’s ability to let heat pass through it. LISTER will take several measurements up to 10 feet deep using pneumatic drilling technology with a custom heat flow needle instrument at its tip. Data from LISTER will help scientists retrace the Moon’s thermal history and understand how it formed and cooled. Lead organization: Texas Tech University
Lunar PlanetVac (LPV) is designed to collect regolith samples from the lunar surface using a burst of compressed gas to drive the regolith into a sample chamber (sieving) for collection and analysis by various instruments. Additional instrumentation will then transmit the results back to Earth. The LPV payload is designed to help increase the science return from planetary missions by testing low-cost technologies for collecting regolith samples in-situ. Lead organization: Honeybee Robotics
Next Generation Lunar Retroreflector (NGLR) serves as a target for lasers on Earth to precisely measure the distance between Earth and the Moon by reflecting very short laser pulses from Earth-based Lunar Laser Ranging Observatories. The laser pulse transit time to the Moon and back is used to determine the distance. Data from NGLR could improve the accuracy of our lunar coordinate system and contribute to our understanding of the inner structure of the Moon and fundamental physics questions. Lead organization: University of Maryland
Regolith Adherence Characterization (RAC) will determine how lunar regolith sticks to a range of materials exposed to the Moon’s environment throughout the lunar day. RAC will measure accumulation rates of lunar regolith on surfaces (for example, solar cells, optical systems, coatings, and sensors) through imaging to determine their ability to repel or shed lunar dust. The data captured will help test, improve, and protect spacecraft, spacesuits, and habitats from abrasive regolith. Lead organization: Aegis Aerospace
Radiation Tolerant Computer (RadPC) will demonstrate a computer that can recover from faults caused by ionizing radiation. Several RadPC prototypes have been tested aboard the International Space Station and Earth-orbiting satellites, but this flight will provide the biggest trial yet by demonstrating the computer’s ability to withstand space radiation as it passes through Earth’s radiation belts, while in transit to the Moon, and on the lunar surface. Lead organization: Montana State University
Electrodynamic Dust Shield (EDS) is an active dust mitigation technology that uses electric fields to move and prevent hazardous lunar dust accumulation on surfaces. EDS is designed to lift, transport, and remove particles from surfaces with no moving parts. Multiple tests will demonstrate the feasibility of the self-cleaning glasses and thermal radiator surfaces on the Moon. In the event the surfaces do not receive dust during landing, EDS has the capability to re-dust itself using the same technology. Lead organization: NASA’s Kennedy Space Center
Lunar Environment heliospheric X-ray Imager (LEXI) will capture a series of X-ray images to study the interaction of solar wind and Earth’s magnetic field that drives geomagnetic disturbances and storms. Deployed and operated on the lunar surface, this instrument will provide the first global images showing the edge of Earth’s magnetic field for critical insights into how space weather and other cosmic forces surrounding our planet impact Earth. Lead organizations: Boston University, NASA’s Goddard Space Flight Center, and Johns Hopkins University
Lunar Magnetotelluric Sounder (LMS) will characterize the structure and composition of the Moon’s mantle by measuring electric and magnetic fields. This investigation will help determine the Moon’s temperature structure and thermal evolution to understand how the Moon has cooled and chemically differentiated since it formed. Lead organization: Southwest Research Institute
Lunar GNSS Receiver Experiment (LuGRE) will demonstrate the possibility of acquiring and tracking signals from GNSS (Global Navigation Satellite System) constellations, specifically GPS and Galileo, during transit to the Moon, during lunar orbit, and on the lunar surface. If successful, LuGRE will be the first pathfinder for future lunar spacecraft to use existing Earth-based navigation constellations to autonomously and accurately estimate their position, velocity, and time. Lead organizations: NASA Goddard, Italian Space Agency
Stereo Camera for Lunar Plume-Surface Studies (SCALPSS) will use stereo imaging photogrammetry to capture the impact of the rocket exhaust plume on lunar regolith as the lander descends on the Moon’s surface. The high-resolution stereo images will aid in creating models to predict lunar regolith erosion, which is an important task as bigger, heavier spacecraft and hardware are delivered to the Moon in close proximity to each other. This instrument also flew on Intuitive Machines’ first CLPS delivery. Lead organization: NASA’s Langley Research Center
Through the CLPS initiative, NASA purchases lunar landing and surface operations services from American companies. The agency uses CLPS to send scientific instruments and technology demonstrations to advance capabilities for science, exploration, or commercial development of the Moon. By supporting a robust cadence of lunar deliveries, NASA will continue to enable a growing lunar economy while leveraging the entrepreneurial innovation of the commercial space industry.
Learn more about CLPS and Artemis at: http://www.nasa.gov/clps
Alise Fisher
Headquarters, Washington
202-358-2546
alise.m.fisher@nasa.gov
Natalia Riusech / Nilufar Ramji
Johnson Space Center, Houston
281-483-5111
natalia.s.riusech@nasa.gov / nilufar.ramji@nasa.gov
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By USH
The crew of a Surjet private air service flight had an unusual encounter on December 23 while returning to Fort Lauderdale. Flight attendant Cassandra Martin, along with two pilots, was onboard the aircraft flying over the Bahamas when an unexpected event caught their attention.
“I suddenly heard air traffic control say, ‘We have a foreign object; can you please identify it?'” Martin recounted to NBC Miami.
Curious, she looked out the window. “I glanced to the left, and the pilot noticed three objects, though I only saw one. I quickly grabbed my phone, pressed it against the window, and tried to record a video of the object,” she explained.
Martin described the orb as white, later shifting to a faint green hue, almost as though surrounded by an electric field. The object followed their flight for about 45 minutes before disappearing.
What made the sighting extraordinary was the altitude. The jet was cruising at approximately 43,000 to 45,000 feet, yet the orb was far above the aircraft and still managed to track it for the extended duration.
The orb’s speed and maneuverability ruled out possibilities such as a balloon or a consumer drone. Unless the orb is of extraterrestrial origin, the orb might be a craft or drone equipped with highly advanced technology not yet publicly known, akin to recent reports of sophisticated drones spotted across the U.S.
This remarkable incident follows a December 16, 2024 sighting aboard United Airlines flight UA2359 from Chicago to Newark. During that flight, a passenger filmed several unidentified orbs at altitudes between 40,000 and 50,000 feet. Additionally, reports surfaced from at least four commercial airline pilots who witnessed mysterious, colorful, circular lights moving at extreme speeds over Oregon in the same month.
These repeated sightings raise questions: Are they advanced black projects hidden from public knowledge or evidence of something extraterrestrial? Regardless of their origin, the increasing reports of advanced drones and strange orbs suggest that something significant is occurring. View the full article
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By NASA
NASA’s Office of STEM Engagement at Johnson Space Center in Houston offers students a unique gateway to opportunity through the High School Aerospace Scholars (HAS) program. The initiative provides Texas juniors with hands-on experience in space exploration, working on projects ranging from rocket building to problem-solving in collaborative teams.
The stories of HAS alumni highlight the program’s impact, showcasing how it has opened doors to diverse careers in STEM and inspired graduates to empower others.
Johnson Community Engagement Lead Jessica Cordero, who served as the manager of the HAS program from 2018 to 2021, reflected on her time with the students:
“I had the privilege of working with so many incredible students who brought imagination and determination to their dreams,” she said. “During HAS, they connected with peers who shared their passion for NASA and STEM, and by the time they completed the program, they had a clear vision of the degrees they would pursue in college. These students are the Artemis Generation—we are in great hands!”
Meet Former HAS Student Neel Narayan
For Neel Narayan, NASA’s HAS program was a transformative experience that reshaped his understanding of space exploration and his place within it.
Through his time in the program, Narayan learned to navigate complex challenges with confidence. “My experience working with difficult information at HAS, combined with having mentors explain the unknown, taught me to be okay with confusion and comfortable with solving hard problems,” he said. “That’s what STEM is all about.”
Neel Narayan at NASA’s High School Aerospace Scholars (HAS) 20th anniversary ceremony. Before participating in the program, Narayan had a narrow view of what a STEM career entailed: long equations and solitary hours behind a computer. HAS completely dismantled that misconception. He said the program, “broke the most complex concepts into granular bites of digestible information, showing that complexity can be distilled if done correctly.”
“During the one-week onsite experience, I was talking to scientists, building rockets, and exploring NASA facilities—none of which involved equations!” he said. “HAS taught me that STEM is not confined to technical work.”
Narayan describes HAS as an eye-opening experience that redefined his approach to problem-solving. “Most of us are unaware of what we don’t know,” he said. “In collaborating with others, I was made aware of solutions that I didn’t know existed. The greatest asset you can have when solving a problem is another person.”
He credits the HAS community, especially his fellow scholars, with shaping his academic and professional growth. “I benefited most from the networking opportunities, particularly with the other HAS scholars in my cohort,” he said. “For those of us studying together in California, we’ve met up to discuss work, school, and external opportunities. Everyone in the program comes out very successful, and I’m grateful to have met those people and to still stay in touch with them.”
For high school students considering STEM but unsure of their direction, Narayan offers simple advice: keep exploring. “You don’t need to know your career path yet—in fact, you shouldn’t,” he said. “There is no better field to explore than STEM because of its vastness.”
Neel Narayan, University of Stanford. Narayan is currently pursuing a master’s degree in computational and mathematical engineering at Stanford University after earning an undergraduate degree in computer science. With his graduate program, Narayan is building on the foundation he developed through NASA’s HAS program.
Narayan aspires to contribute to the agency’s innovation and groundbreaking work. “NASA’s research changes the world, and being part of that mission is a dream I’ve had for a while,” he said.
Meet Sarah Braun
NASA’s HAS program solidified Sarah Braun’s understanding of how a STEM career could encompass her diverse interests, from design and education to plotting spacecraft orbits and planning launches. From her time in HAS to her current space exploration career, Braun believes STEM can be as multifaceted as the people who pursue it.
“HAS showed me the options ahead were as endless as my imagination,” she said. “The program convinced me that all my skills would be put to use in STEM, including getting to be creative and artistic.”
Sarah Braun engages in science, technology, engineering, and mathematics outreach at the Air Zoo Aerospace & Science Museum in Portage, Michigan, standing beside a Gemini model. The program gave her the opportunity to network, problem-solve, and collaborate with students from various backgrounds. “Learning how to communicate designs I could picture in my head was the biggest challenge, but by observing my teammates and mentors, I built the skills I needed.”
The networking opportunities she gained through HAS have also been instrumental to her academic and career growth. “The mentors I met through HAS have supported me throughout college and into my early career,” she said. “They taught me countless technical skills and how to best take advantage of my college years. I would never have made it to where I am today without HAS!”
After completing the HAS program, Braun interned with NASA, where she worked on space systems and paved the way for her career at Collins Aerospace.
Sarah Braun at the National Museum of the U.S. Air Force in Dayton, Ohio. She stands in front of the hardware she now works on at Collins Aerospace. Braun advises high school students uncertain about their career paths to get engaged and ask questions. “There are so many people out there who pursue STEM to follow a passion or challenge themselves,” she said. “Talking with people about what they have experienced and learned has been a huge help and inspiration for me throughout the years.”
She is also passionate about inspiring and educating others. “Whether I’m leading after-school STEM clubs or mentoring students, outreach and teaching have become my biggest contributions to NASA’s mission of exploration and discovery,” said Braun.
Meet Audrey Scott
Audrey Scott credits the HAS program with giving her a chance to explore science in the real world. “I experienced the excitement space could bring through livestream events like the landing of NASA’s InSight Lander mission and Cassini’s Grand Finale,” she said.
Audrey Scott, front, with fellow 2019 HAS graduates. Scott shared that the HAS program opened her eyes to the vast possibilities within STEM fields. Seeing the many ways to apply a STEM degree in practice broadened her perspective and inspired her to pursue her passion.
After HAS, Scott chose to study astrophysics at the University of Chicago in Illinois, where she is now pursuing her Ph.D. in experimental cosmology and laying the groundwork for a future in space exploration.
“My time with HAS and its encouragement of STEM excellence gave me the confidence I needed to take the plunge,” said Scott.
The program also transformed her approach to teamwork and exposed her to fast-paced problem-solving. “My school didn’t prioritize group projects, so working with people from all different backgrounds and personalities was informative for my future work in college,” she said. “HAS was a safe space to experiment with being both a leader and collaborator.”
She encourages high school students uncertain of their path to “try everything.” Scott advises, “If you have a moment of fascination, take advantage of that intellectual and creative energy, and learn something new. Time spent realizing you don’t like something is just as useful as time spent realizing you do.” She also recommends seeking out resources, finding mentors, and talking to everyone.
Scott continues to connect with some of her HAS cohort, especially young women navigating STEM paths alongside her. “We’ve been able to support each other through challenges,” she said. “Being part of HAS made me, in a way, part of the NASA family.”
Audrey Scott, front, with fellow 2019 HAS graduates. Scott’s HAS experience opened doors to opportunities like the Brooke Owens Fellowship, where she worked on a satellite in partnership with NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and later the Illinois Space Grant award, which took her to NASA’s Jet Propulsion Laboratory in Southern California. She envisions part of her thesis research as a Ph.D. candidate taking place at a NASA center and remains open to a future at the agency.
“I’ll continue advocating for space exploration and pushing the boundaries of what’s known,” she said. “In my research, I’m driven by questions like, ‘What did the beginning of the universe look like—and why are we here?’”
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