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C83

NGC 4945

Proper NameNone
Caldwell NumberC83
NGC/IC NumberNGC 4945
ConstellationCentaurus
Right Ascension13h 5m 27s
Declination-49° 28' 4"
Distancec.10,500,000 light years
c.3,200,000 parsecs
MagnitudeApparent: +7.91
Absolute: -19.63
Mean DiameterApparent: 23.3'
Actual: 71,200 light years
Hubble TypeSBc barred spiral
Optimum VisibilityApril (Usually visible from southern latitudes)

A galaxy in the central regions of Centaurus with a loosely barred spiral form, C83 has a structure comparable to that of the Milky Way Galaxy, though with a diameter of some 71,200 light years it is somewhat smaller. C83 lies at a distance of 10.5 million light years from the Milky Way.

The disc of C83 is angled so that it appears nearly edge-on as seen from Earth. The stars in this image are all within the Milky Way Galaxy, and hence in the near foreground compared with the distant galaxy beyond (the bright star to the west of C83 is fifth-magnitude Xi1 Centauri). Imagery provided by Aladin sky atlas

As viewed from Earth, the galaxy is almost edge-on and so appears as a narrow ellipse, though its spiral structure is still clearly visible, as is a dark lane of dust running around much of its outer edge. The galaxy's nucleus is unusually active, implying that C83 hosts a supermassive black hole at its core.

C83 is one of the most prominent of a group of about forty galaxies that span the sky northward from Centaurus, known collectively as the Centaurus A/M83 Group. C83 belongs to the southern lobe of this group, associated with Centaurus A, the most massive of the group's galaxies. Indeed C83 and Centaurus A are relatively close together, on a galactic scale. They lie about two million light years apart, a distance comparable with the Milky Way's distance from the Andromeda Galaxy.

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