Hoo-boy! This is a dense cluster. It had a roughly triangular shape, trisected by dark lanes focusing on a bright yellow-orange central star. It was very stunning to look at. I was really struggling with how to sketch it. Plotting star positions wasn’t giving the feel for granularity in the triangular area. In the end, I dashed in boundaries of the grainy regions, and then lightly shaded and stippled these. It looks like a little too blunt of an instrument, but it’s better than no indication at all. The south end of the view was punctuated by a bright yellow star. Going to a 120X view still showed some localized background granularity, but I didn’t indicate this in the close-up sketch.
M37 is the brightest and richest of the three Auriga Messier clusters. It contains 150 stars brighter than mag 12.5, with a possible total of 500 stars altogether. Its age is estimated at 300 million years, and contains at least a dozen red giants. Distance estimates range from 3600 to 4700 light years, with a diameter of 20 to 25 light years. M37 was discovered by Giovanni Batista Hodierna before 1654, and independently re-recorded by Charles Messier in 1764.
|Subject||M37 (NGC 2099)|
|Position*||Auriga [RA: 05:52.4 / Dec: +32:33]|
|Date/Time||February 3, 2005 – 9:30 PM
(February 4, 2005 – 04:30 UT)
|Observing Loc.||Flagstaff, AZ – Home|
|Instrument||Orion SVP 6LT Reflector (150 mm dia./1200 mm F/L)|
|Eyepieces/Mag.||32 mm (37X), 10 mm (120X)|
*Based on published data.