Celestial hemisphere:  Northern  ·  Constellation: Virgo (Vir)  ·  Contains:  M 87  ·  NGC 4425  ·  NGC 4429  ·  NGC 4435  ·  NGC 4438  ·  NGC 4452  ·  NGC 4459  ·  NGC 4461  ·  NGC 4473  ·  NGC 4477  ·  NGC 4486  ·  NGC 4503  ·  NGC 4531  ·  Virgo Galaxy
M87, Jason Lichter
M87
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M87

M87, Jason Lichter
M87
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M87

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Description

Streaming out from the center of the galaxy M87 like a cosmic searchlight is one of nature's most amazing phenomena, a black-hole-powered jet of electrons and other sub-atomic particles. Lying at the center of M87 is a supermassive black hole, which has swallowed up a mass equivalent to 2 billion times the mass of our Sun. The jet originates in the disk of superheated gas swirling around this black hole and is propelled and concentrated by the intense, twisted magnetic fields trapped within this plasma. The light that we see (and the radio emission) is produced by electrons twisting along magnetic field lines in the jet, a process known as synchrotron radiation, which gives the jet its bluish tint. At a distance of 50 million light-years, M87 is too distant for Hubble to discern individual stars. The dozens of star-like points swarming about M87 are, instead, themselves clusters of hundreds of thousands of stars each. An estimated 15,000 globular clusters formed very early in the history of this galaxy and are older than the second generation of stars, which huddle closer to the center of the galaxy.

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M87, Jason Lichter

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