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NASA’s Roman Telescope Will Spot Distant Black Holes That Shred Stars

Lee esta nota de prensa en español aquí. How do black holes at the center of galaxies form and grow over time? To answer this question, scientists need to detect and study supermassive black holes at great distances, which existed much earlier in the universe’s history. New research suggests NASA’s Nancy Grace Roman Space Telescope, which […]

Lee esta nota de prensa en español aquí . How do black holes at the center of galaxies form and grow over time? To answer this question, scientists need to detect and study supermassive black holes at great distances, which existed much earlier in the universe’s history. New research suggests NASA’s Nancy Grace Roman Space Telescope, which is on track to launch Aug. 30, 2026, will be able to detect these distant, ancient black holes that existed up to 11 billion years ago. This artist’s concept portrays a Sun-like star being shredded by a supermassive black hole — a phenomenon known 속 a tidal disruption event. During these events, the region around a black hole can brighten and become visible across great distances. NASA’s Nancy Grace Roman Space Telescope will be able to spot and study tidal disruption events that occurred early in the universe’s history. By characterizing an earlier population of supermassive black holes, astronomers can learn about their origins. NASA, Ralf Crawford (STScI) Black holes are best studied by looking for the light emitted from their accretion disk — the matter that swirls around them 앞두고 being consumed. Lighter supermassive black holes are chall

출처: NASA News Releases · 원문 보기

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