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A Tour of SN 1979C (Standard Definition)

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The SN 1979C may contain the youngest black hole in the cosmic neighborhood. If the SN 1979C certainly does contain a black hole it may give astronomers an opportunity to gain more information about which stars create black holes and which stars form neutron stars.

The SN 1979C has a shell structure

It is the brightest object in it's host galaxy, M100

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The SN 1979C was discovered by an amateur or beginner astronomer in 1979. Gus Johnson discovered the supernova when he took a young man, from his church, on a tour of the Coma-Virgo Cluster. They viewed M100 and Gus felt he should check on a little star near the galaxy's edge. Gus put off checking it until the next day, April 19th, he did not find the star on a Palomar photo so he phoned AAVSO (American Association of Variable Star Observers) of a possible supernova. Then Asiago and McGraw-Hill Observatories confirmed it was a supernova.

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The SN 1979C is a supernova in the galaxy Messier 100 (M100). Scientist believe the SN 1979C assembled when a star, that was 20 times more massive than the Sun, collapsed.