Astronomy Picture of the Day
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2020 September 8
GW190521: Unexpected Black Holes Collide
Illustration Credit: Raśl Rubio (Virgo Valencia Group, The Virgo
Collaboration)
Explanation: How do black holes like this form? The two black holes
that spiraled together to produce the gravitational wave event GW190521
were not only the most massive black holes ever seen by LIGO and VIRGO
so far, their masses -- 66 and 85 solar masses -- were unprecedented
and unexpected. Lower mass black holes, below about 65 solar masses are
known to form in supernova explosions. Conversely, higher mass black
holes, above about 135 solar masses, are thought to be created by very
massive stars imploding after they use up their weight-bearing
nuclear-fusion-producing elements. How such intermediate mass black
holes came to exist is yet unknown, although one hypothesis holds that
they result from consecutive collisions of stars and black holes in
dense star clusters. Featured is an illustration of the black holes
just before collision, annotated with arrows indicating their spin
axes. In the illustration, the spiral waves indicate the production of
gravitational radiation, while the surrounding stars highlight the
possibility that the merger occurred in a star cluster. Seen last year
but emanating from an epoch when the universe was only about half its
present age (z ~ 0.8), black hole merger GW190521 is the farthest yet
detected, to within measurement errors.
Astrophysicists: Browse 2,200+ codes in the Astrophysics Source Code
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Tomorrow's picture: stellar sisters
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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)
NASA Official: Phillip Newman Specific rights apply.
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