Visual Astronomy

MESSIER 88
Messie 88
   
RA:
12h 32m 00s
DEC:
+14° 25' 00''
Type:
Spiral galaxy
NGC:
4501
Magnitude:
9.60
Surface brightness :
13.00
Apparent dimensions :
6.8'x3.7'
Distance:
60,000,000 ly
   
 

M88 is one of the eight galaxies found on March 18, 1781 by Charles Messier in the Coma-Virgo region, and described by him as "nebula without stars," "one of the faintest" objects, and similar to M58. On that most successful discovery day, Messier also found globular cluster M92, to bring his daily score to 9 cataloged objects.

M88 is among the first recognized as a spiral galaxy, and listed by Lord Rosse as one of 14 "spiral nebulae" discovered to 1850.

This bright member of the Virgo Cluster of galaxies is nicely symmetrical and of multiple-arm type. As its equatorial plane is inclined by about 30 degrees to the line of sight, its appearance resembles a bit that of the Andromeda galaxy M31, and its outline is an elongated ellipse of angular dimension between 7x4 to 8x3 arc minutes, according to different sources, corresponding to a linear diameter of about 130,000 light years. This is one of the more rewarding galaxies in the Virgo cluster for smaller instruments!

 

VEDRAN VRHOVAC©

2006.-2007.