Celestial hemisphere:  Northern  ·  Constellation: Camelopardalis (Cam)  ·  Contains:  NGC 2403
NGC2403, Carl Tanner
NGC2403
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NGC2403

NGC2403, Carl Tanner
NGC2403
Powered byPixInsight

NGC2403

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Description

An outlier of the M81 Group of galaxies, ngc2403, is a galaxy very much like M33 in the Local Group. At 50963.5ly across and containing some 60 billion stars, ngc2403 is around the same size as M33, only a little more massive. Like M33, ngc2403 contains a great number of very prominent HII regions, the largest being ngc2404. ngc2404 is one of the largest HII known and spans 2000ly, a little larger than the Tarantula Nebula in the LMC (1840ly). However, unlike the Tarantula, the central cluster of the nebula is much smaller and looks more like a large OB association, whereas the central cluster of stars in the Tarantula weighs in at some 450K solar masses and resembles a nacent globular cluster. At 8 million ly (2.5Mpc) from Earth, in the constellation of Camelopardalis (the giraffe), the galaxy is closer than main body of the M81 Group, but its membership of the group is seen in their common motion through space Its apparent brightness of 8.9mag makes it the second brightest member of the group and it has a redshift velocity is 131km/s.

The Hubble Classification for the galaxy is SAB(s)cd, making it an intermediate barred spiral galaxy with no central ring and relatively loose arms around a smallish nucleus. The galaxy holds the distinction as being the first galaxy outside the Local Group where Cepheid variable stars were first discovered Two supernovae have been seen in this galaxy, SN1954j, which peaked at 16mag, and SN2004dj, which was the brightest supernova seen for the last 17 years and is still the brightest seen in the 21st Century.

Pic was taken with t68 (iTelescope, NMSO), 10x2min subs.

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NGC2403, Carl Tanner