Credit & Copyright: R Jay GaBany
(Cosmotography.com)
Explanation:
One of the nearest supernovas of recent years was
discovered late last month in the bright nearby galaxy
M51.
It is visible on the right of the
above before and after images of the
picturesque spiral.
Can you spot it?
The supernova, discovered originally by
Wolfgang Kloehr and now dubbed 2005cs,
is still near its maximum brightness and visible
with a telescope toward the constellation of the Hunting Dogs (Canes Venatici).
The supernova has been identified as a
Type II but has an unusual brightness history,
creating speculation that is similar in nature to the
brightest supernova of modern times:
1987A.
The progenitor star has been
identified as a bright blue star.
Although hundreds of supernovas are discovered each year by automated searches,
nearby supernova are rare and important because they
frequently become bright enough to be studied by many telescopes and are near enough
for their (former) host star and immediate surroundings to be spatially resolved.
Supernova 2005cs may have left behind a core that has been
compressed into a
neutron star or
black hole.
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Publikacii s klyuchevymi slovami:
supernova - M 51 - Sverhnovye
Publikacii so slovami: supernova - M 51 - Sverhnovye | |
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