Object: M36 Camera: Meade DSI-Pro II
Date: 11/10/2007 Telescope: Meade 80mm APO refractor @ f/6
Total Exposure: RGB:30'40'40' Subexposures: 1 minutes each
Location: West Boylston, MA
Processing: Description:
M36
Discovered by Giovanni Batista Hodierna before 1654.

M36 is about 4,100 light years distant (only Kenneth Glyn Jones disagrees and has 3,700), so that its angular diameter of 12' corresponds to about 14 light years (Wallenquist gives an apparent diameter of 19', corresponding to over 20 light years). It has about 60 proven members, the brightest of which are of apparent mag 9 and spectral type B2; the luminosity of the brightest member is about 360 times that of the Sun. Many of these bright stars are rapidly rotating, as shown by their broadened spectral lines, an effect which is also found for the bright type B members of the Pleiades (M45). If it were at the same distance (i.e., 10 times closer), this cluster would look as conspicuous as and very similar to the Pleiades.