PBS Space Time

The New Physics of Black Hole Star Capture | Extreme Tidal Disruption Events

If you track the motion of individual stars in the ultra-dense star cluster at the very center of the Milky Way you’ll see that they swing in sharp orbits around some vast but invisible mass—that’s the Sagittarius A* supermassive black hole. These are perilous orbits, and sometimes a star wanders just a little too close to that lurking monster, leading to a tidal disruption event.

The New Physics of Black Hole Star Capture | Extreme Tidal Disruption Events

17m 44s

If you track the motion of individual stars in the ultra-dense star cluster at the very center of the Milky Way you’ll see that they swing in sharp orbits around some vast but invisible mass—that’s the Sagittarius A* supermassive black hole. These are perilous orbits, and sometimes a star wanders just a little too close to that lurking monster, leading to a tidal disruption event.

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  • The New Physics of Black Hole Star Capture | Extreme Tidal Disruption Events: asset-mezzanine-16x9

    The New Physics of Black Hole Star Capture | Extreme Tidal Disruption Events

    S10 E21 - 17m 44s

    If you track the motion of individual stars in the ultra-dense star cluster at the very center of the Milky Way you’ll see that they swing in sharp orbits around some vast but invisible mass—that’s the Sagittarius A* supermassive black hole. These are perilous orbits, and sometimes a star wanders just a little too close to that lurking monster, leading to a tidal disruption event.

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