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N6946-BH1

N6946-BH1 is a disappearing supergiant star and failed supernova candidate formerly seen in the galaxy NGC 6946, on the northern border of the constellation of Cygnus. The star, either a red supergiant or a yellow hypergiant, was 25 times the mass of the Sun, and was 20 million light years distant from Earth. In March through to May 2009 its bolometric luminosity increased to at least a million solar luminosities, but by 2015 it had disappeared from optical view. In the mid and near infrared an object is still visible; however, it is fading away with a brightness proportional to t−4/3. The brightening was insufficient to be a supernova; the process that created the outburst is still uncertain.

Description
light curve for N6946-BH1, plotted from data published by Adams et al. (2017) Observed type II supernovae do not originate from stars with initial masses greater than about , and the rate of large star formation appears to exceed the rate of supernovae. The expectation is that something else is happening to these extra large stars. Failed supernovae and black hole formation is one proposed explanation. ==See also==
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