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Climate satellite MethaneSAT backed by Bezos and Google fails in space after just 1 year
To the Spacemobile!
To the Spacemobile!
In this Nov. 1, 1964, image, three members of NASA’s Lewis Research Center’s (now NASA’s Glenn Research Center in Cleveland) Educational Services Office pose with one of the center’s Spacemobile space science demonstration units. Once the NACA (National Advisory Committee for Aeronautics) became NASA, public outreach became one of the agency’s core tenets. Lewis, which had previously been a closed laboratory, began hosting open houses and elaborate space fairs in the early 1960s.
In addition, the center initiated educational programs that worked with local schools and a robust speaker’s bureau that explained NASA activities to the community. One aspect of these efforts was the Spacemobile Program. These vehicles included a delegated speaker, exhibits, models, and other resources. The Spacemobiles, which made forays across the Midwest, were extremely active throughout the 1960s.
Image credit: NASA
To the Spacemobile!
In this Nov. 1, 1964, image, three members of NASA’s Lewis Research Center’s (now NASA’s Glenn Research Center in Cleveland) Educational Services Office pose with one of the center’s Spacemobile space science demonstration units. Once the NACA (National Advisory Committee for Aeronautics) became NASA, public outreach became one of the agency’s core tenets. Lewis, which had previously been a closed laboratory, began hosting open houses and elaborate space fairs in the early 1960s.
In addition, the center initiated educational programs that worked with local schools and a robust speaker’s bureau that explained NASA activities to the community. One aspect of these efforts was the Spacemobile Program. These vehicles included a delegated speaker, exhibits, models, and other resources. The Spacemobiles, which made forays across the Midwest, were extremely active throughout the 1960s.
Image credit: NASA
New Horizons images enable first test of interstellar navigation
New Horizons images enable first test of interstellar navigation
Vegan cheese could be about to get a lot closer to the real thing
Vegan cheese could be about to get a lot closer to the real thing
An ancient Egyptian's complete genome has been read for the first time
An ancient Egyptian's complete genome has been read for the first time
You’ve been sold a giant myth when it comes to improving your health
You’ve been sold a giant myth when it comes to improving your health
Discovery Alert: Flaring Star, Toasted Planet
A giant planet some 400 light-years away, HIP 67522 b, orbits its parent star so tightly that it appears to cause frequent flares from the star’s surface, heating and inflating the planet’s atmosphere.
Key FactsOn planet Earth, “space weather” caused by solar flares might disrupt radio communications, or even damage satellites. But Earth’s atmosphere protects us from truly harmful effects, and we orbit the Sun at a respectable distance, out of reach of the flares themselves.
Not so for planet HIP 67522 b. A gas giant in a young star system – just 17 million years old – the planet takes only seven days to complete one orbit around its star. A “year,” in other words, lasts barely as long as a week on Earth. That places the planet perilously close to the star. Worse, the star is of a type known to flare – especially in their youth.
In this case, the proximity of the planet appears to result in fairly frequent flaring.
DetailsThe star and the planet form a powerful but likely a destructive bond. In a manner not yet fully understood, the planet hooks into the star’s magnetic field, triggering flares on the star’s surface; the flares whiplash energy back to the planet. Combined with other high-energy radiation from the star, the flare-induced heating appears to have increased the already steep inflation of the planet’s atmosphere, giving HIP 67522 b a diameter comparable to our own planet Jupiter despite having just 5% of Jupiter’s mass.
This might well mean that the planet won’t stay in the Jupiter size-range for long. One effect of being continually pummeled with intense radiation could be a loss of atmosphere over time. In another 100 million years, that could shrink the planet to the status of a “hot Neptune,” or, with a more radical loss of atmosphere, even a “sub-Neptune,” a planet type smaller than Neptune that is common in our galaxy but lacking in our solar system.
Fun FactsFour hundred light-years is much too far away to capture images of stellar flares striking orbiting planets. So how did a science team led by Netherlands astronomer Ekaterina Ilin discover this was happening? They used space-borne telescopes, NASA’s TESS (Transiting Exoplanet Survey Satellite) and the European Space Agency’s CHEOPS (CHaracterising ExoPlanets Telescope), to track flares on the star, and also to trace the path of the planet’s orbit.
Both telescopes use the “transit” method to determine the diameter of a planet and the time it takes to orbit its star. The transit is a kind of mini-eclipse. As the planet crosses the star’s face, it causes a tiny dip in starlight reaching the telescope. But the same observation method also picks up sudden stabs of brightness from the star – the stellar flares. Combining these observations over five years’ time and applying rigorous statistical analysis, the science team revealed that the planet is zapped with six times more flares than it would be without that magnetic connection.
The DiscoverersA team of scientists from the Netherlands, Germany, Sweden, and Switzerland, led by Ekaterina Ilin of the Netherlands Institute for Radio Astronomy, published their paper on the planet-star connection, “Close-in planet induces flares on its host star,” in the journal Nature on July 2, 2025.
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Discovery Alert: Flaring Star, Toasted Planet
A giant planet some 400 light-years away, HIP 67522 b, orbits its parent star so tightly that it appears to cause frequent flares from the star’s surface, heating and inflating the planet’s atmosphere.
Key FactsOn planet Earth, “space weather” caused by solar flares might disrupt radio communications, or even damage satellites. But Earth’s atmosphere protects us from truly harmful effects, and we orbit the Sun at a respectable distance, out of reach of the flares themselves.
Not so for planet HIP 67522 b. A gas giant in a young star system – just 17 million years old – the planet takes only seven days to complete one orbit around its star. A “year,” in other words, lasts barely as long as a week on Earth. That places the planet perilously close to the star. Worse, the star is of a type known to flare – especially in their youth.
In this case, the proximity of the planet appears to result in fairly frequent flaring.
DetailsThe star and the planet form a powerful but likely a destructive bond. In a manner not yet fully understood, the planet hooks into the star’s magnetic field, triggering flares on the star’s surface; the flares whiplash energy back to the planet. Combined with other high-energy radiation from the star, the flare-induced heating appears to have increased the already steep inflation of the planet’s atmosphere, giving HIP 67522 b a diameter comparable to our own planet Jupiter despite having just 5% of Jupiter’s mass.
This might well mean that the planet won’t stay in the Jupiter size-range for long. One effect of being continually pummeled with intense radiation could be a loss of atmosphere over time. In another 100 million years, that could shrink the planet to the status of a “hot Neptune,” or, with a more radical loss of atmosphere, even a “sub-Neptune,” a planet type smaller than Neptune that is common in our galaxy but lacking in our solar system.
Fun FactsFour hundred light-years is much too far away to capture images of stellar flares striking orbiting planets. So how did a science team led by Netherlands astronomer Ekaterina Ilin discover this was happening? They used space-borne telescopes, NASA’s TESS (Transiting Exoplanet Survey Satellite) and the European Space Agency’s CHEOPS (CHaracterising ExoPlanets Telescope), to track flares on the star, and also to trace the path of the planet’s orbit.
Both telescopes use the “transit” method to determine the diameter of a planet and the time it takes to orbit its star. The transit is a kind of mini-eclipse. As the planet crosses the star’s face, it causes a tiny dip in starlight reaching the telescope. But the same observation method also picks up sudden stabs of brightness from the star – the stellar flares. Combining these observations over five years’ time and applying rigorous statistical analysis, the science team revealed that the planet is zapped with six times more flares than it would be without that magnetic connection.
The DiscoverersA team of scientists from the Netherlands, Germany, Sweden, and Switzerland, led by Ekaterina Ilin of the Netherlands Institute for Radio Astronomy, published their paper on the planet-star connection, “Close-in planet induces flares on its host star,” in the journal Nature on July 2, 2025.
Keep Exploring Discover More Topics From NASA
Search for Life
Stars
Galaxies
Black Holes
Explore This Section
- Exoplanets Home
- Exoplanets Overview
- Search for Life
- Discoveries
- Immersive
- News
- Resources
- More
The secret of why Mars grew cold and dry may be locked away in its rocks
Near-Earth Asteroids as of July 2025
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Near-Earth Asteroids as of July 2025Each month, NASA’s Planetary Defense Coordination Office releases a monthly update featuring the most recent figures on NASA’s planetary defense efforts, near-Earth object close approaches, and other timely facts about comets and asteroids that could pose an impact hazard with Earth. Here is what we’ve found so far.
Updated: July 2, 2025
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Near-Earth Asteroids as of July 2025
1 min read
Near-Earth Asteroids as of July 2025Each month, NASA’s Planetary Defense Coordination Office releases a monthly update featuring the most recent figures on NASA’s planetary defense efforts, near-Earth object close approaches, and other timely facts about comets and asteroids that could pose an impact hazard with Earth. Here is what we’ve found so far.
Updated: July 2, 2025
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21 hours ago
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AI Could Help Save Patients from Extreme Heat
AI could be used to comb through electronic health records and warn vulnerable people about dangerous heat waves
Astronomers Found the Most Self-Destructive Planet in the Sky
This planet triggers flares on its star—spelling its ultimate doom
Clingy planets can trigger own doom, suspect Cheops and TESS
Astronomers using the European Space Agency’s Cheops mission have caught an exoplanet that seems to be triggering flares of radiation from the star it orbits. These tremendous explosions are blasting away the planet’s wispy atmosphere, causing it to shrink every year.
This is the first-ever evidence for a ‘planet with a death wish’. Though it was theorised to be possible since the nineties, the flares seen in this research are around 100 times more energetic than expected.