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Search resuls for: "Mark Garlick"


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In the event of an impending hazardous asteroid strike, NASA already has its plan in place to alert the public. NASA’s Planetary Defense Coordination Office is tasked with finding, tracking, and assessing the risk associated with potentially hazardous asteroids in our solar system. To do that, NASA works with a global coalition of astronomers called the International Asteroid Warning Network (IAWN). There are about 2,300 known potentially hazardous asteroids out there, and roughly 153 of them are larger than 0.6 miles across. If Bennu does head toward Earth, NASA has a few tricks up its sleeve to defend our planet.
Persons: , ROGER HARRIS, , Lindley Johnson, ” Johnson, IAWN, Johnson, MARK GARLICK, NASA wouldn’t, they’re Organizations: NASA, Service, Defense, Office, Planetary Defense, Warning, White, United Nations Office, Outer Space Affairs, Minor Planet
These black holes get kicked into space, moving as fast as 1,000 kilometers per second. AdvertisementScientists studying how supernovas explode may have discovered a new process for how certain black holes form. Turns out, some baby black holes hit the ground running at colossal speeds just moments after they take shape. Asymmetrical explosions can lead to powerful kicks that send black holes shooting into space at over 2 million mph. AdvertisementIf the black holes are movingIf you hear blazing-fast black holes and start to panic, don't.
Persons: , MARK GARLICK, GARLICK, Adam Burrows, Burrows, Vijay Varma, Ivo Labbe, Swinburne, Rachel Bezanson, Varma Organizations: Service, Princeton University, University of Massachusetts Dartmouth, NASA, ESA, CSA, University of Pittsburgh
Planets beyond our solar system have a size gap, where worlds seem to shrink past a certain range. Scientists think this is because some sub-Neptunes shrink — losing their atmospheres and speeding through the size gap until they are as small as a super-Earth. AdvertisementThe planets themselves may be pushing their atmospheres awayShrinking exoplanets may lack the mass (and therefore the gravity) to hold their atmospheres close. AdvertisementThe other hypothesis, called photoevaporation, says that a planet's atmosphere is dissipated by the radiation of its host star. AdvertisementThe scientists found that most of the planets there retained their atmosphere, making the core-powered mass loss a more likely cause of eventual atmosphere loss.
Persons: , Jessie Christiansen, Mark Garlick, NASA's, Christiansen Organizations: NASA, Service, JPL, Caltech, Kepler Space, Harvard
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