Book contents
- Frontmatter
- Dedication
- Contents
- Foreword
- Preface
- User Guide
- Charles Messier
- The Observations
- The Catalog
- Statistics of the Messier objects
- Visual observation of the Messier objects
- Photography of the Messier objects
- The 110 Messier objects
- M 1
- M 2
- M 3
- M 4
- M 5
- M 6
- M 7
- M 8
- M 9
- M 10
- M 11
- M 12
- M 13
- M 14
- M 15
- M 16
- M 17
- M 18
- M 19
- M 20
- M 21
- M 22
- M 23
- M 24
- M 25
- M 26
- M 27
- M 28
- M 29
- M 30
- M 31
- M 32
- M 33
- M 34
- M 35
- M 36
- M 37
- M 38
- 39
- M 40
- M 41
- M 42
- M 43
- M 44
- M 45
- M 46
- M 47
- M 48
- M 49
- M 50
- M 51
- M 52
- M 53
- M 54
- M 55
- M 56
- M 57
- M 58
- M 59
- M 60
- M 61
- M 62
- M 63
- M 64
- M 65
- M 66
- M 67
- M 68
- M 69
- M 70
- M 71
- M 72
- M 73
- M 74
- M 75
- M 76
- M 77
- M 78
- M 79
- M 80
- M 81
- M 82
- M 83
- M 84
- M 85
- M 86
- M 87
- M 88
- M 89
- M 90
- M 91
- M 92
- M 93
- M 94
- M 95
- M 96
- M 97
- M 98
- M 99
- M 100
- M 101
- M 102
- M 103
- M 104
- M 105
- M 106
- M 107
- M 108
- M 109
- M 110
- Glossary of technical terms
- Index of figures
- Index of sources
M 37
from The 110 Messier objects
Published online by Cambridge University Press: 05 August 2015
- Frontmatter
- Dedication
- Contents
- Foreword
- Preface
- User Guide
- Charles Messier
- The Observations
- The Catalog
- Statistics of the Messier objects
- Visual observation of the Messier objects
- Photography of the Messier objects
- The 110 Messier objects
- M 1
- M 2
- M 3
- M 4
- M 5
- M 6
- M 7
- M 8
- M 9
- M 10
- M 11
- M 12
- M 13
- M 14
- M 15
- M 16
- M 17
- M 18
- M 19
- M 20
- M 21
- M 22
- M 23
- M 24
- M 25
- M 26
- M 27
- M 28
- M 29
- M 30
- M 31
- M 32
- M 33
- M 34
- M 35
- M 36
- M 37
- M 38
- 39
- M 40
- M 41
- M 42
- M 43
- M 44
- M 45
- M 46
- M 47
- M 48
- M 49
- M 50
- M 51
- M 52
- M 53
- M 54
- M 55
- M 56
- M 57
- M 58
- M 59
- M 60
- M 61
- M 62
- M 63
- M 64
- M 65
- M 66
- M 67
- M 68
- M 69
- M 70
- M 71
- M 72
- M 73
- M 74
- M 75
- M 76
- M 77
- M 78
- M 79
- M 80
- M 81
- M 82
- M 83
- M 84
- M 85
- M 86
- M 87
- M 88
- M 89
- M 90
- M 91
- M 92
- M 93
- M 94
- M 95
- M 96
- M 97
- M 98
- M 99
- M 100
- M 101
- M 102
- M 103
- M 104
- M 105
- M 106
- M 107
- M 108
- M 109
- M 110
- Glossary of technical terms
- Index of figures
- Index of sources
Summary
Degree of difficulty 2 (of 5)
Minimum aperture Naked eye
Designation NGC 2099
Type Open cluster
Class I2r
Distance 4510 ly (K2005) 6720 ly (2004) 4510 ly (proper motion, 2002) 6660 ly (CMD, 2001)
Size 33 ly
Constellation Auriga
R.A. 5h 52,5min
Decl. +32° 33′
Magnitude 5.6
Surface brightness –
Apparent diameter 25′
Discoverer Hodierna, 1654
History M 37 was discovered before 1654 by Giovanni Batista Hodierna, who saw a “nebulous patch.” Unaware of Hodierna's observation, Messier made an independent discovery of M 37 on the 2nd of September 1764, and described a “cluster of faint stars, at little distance from the previous [M 36]; the stars are very faint, close, and contain some nebulosity.”
Around 1830, Smyth noted enthusiastically: “The whole field being strewed as it were with sparkling gold-dust; and the group is resolvable into about 500 stars, from the 10th to the 14th magnitudes, besides the outliers.” John Herschel, too, saw a “very fine large cluster, all resolved into stars of 10th to 13th magnitude. It fills 1½ fields, but the straggling stars extend very far. There may be 500 stars.” Heinrich d'Arrest even believed he saw “wonderful loops and curved star patterns,” while Mädler remarked: “no particular compression can be noticed toward the middle.”
Leo Brenner described M 37 in detail in his observing guide for amateur astronomers, about 100 years ago: “A splendid object for small scopes. Visible already in small finder scopes as a nebulous star, 24′ diameter. The larger the telescope, the more splendid the view. With a 27-inch telescope, I estimated the number of visible stars 10th to 14th magnitude to about 600, but also in a 7-inch we see about 550, and a 4-inch at 120× magnification still shows nearly 500. Stars are more crowded towards the middle.”
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- Information
- Atlas of the Messier ObjectsHighlights of the Deep Sky, pp. 164 - 165Publisher: Cambridge University PressPrint publication year: 2008