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 36
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 1960
Type Open cluster
Class I3r
Distance 4300 ly (K2005) 4240 ly (CMD, 2000)
Size 15 ly
Constellation Auriga
R.A. 5h 36.1min
Decl. +34° 8′
Magnitude 6.0
Surface brightness –
Apparent diameter 12′
Discoverer Hodierna, 1654
History M 36 was discovered before 1654 by the Sicilian observer Giovanni Batista Hodierna as a “nebulous patch.” However, his observations were soon forgotten and his notes were rediscovered only in 1984. For this reason, le Gentil must be considered a true independent discoverer of this cluster, which he found in 1749. Messier made his observation on the 2nd of September 1764, and wrote: “Cluster of stars in the Charioteer, with a simple refractor of 3½ foot the stars are barely discerned, the cluster does not contain any nebulosity. 9′ diameter.”
John Herschel called M 36 a “very pretty object which fills the field.” Smyth described it as “the device of a star whose rays are formed by very small stars.” D'Arrest must have had a similar impression when he wrote: “extremely rich and pretty cluster. Originating from the center, many stars are arranged in three thin spirals.”
Leo Brenner recommended the observation of M 36 to his fellow amateur observers, about 100 years ago, with the words: “very large, rich and bright, consisting of somewhat scattered stars of 8th to 10th magnitude, which include the double star Σ 737 of 8th and 9th magnitude stars, separated 10.6". A rewarding object even for 3-inch telescopes and low magnifications.”
Astrophysics M 36 is the least rich of the three Messier clusters in Auriga. Only 178 stars are regarded as physical cluster members. The brightest star (magnitude 8.8) is a blue giant with the early spectral type B2 and 360 times the solar luminosity.
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- Information
- Atlas of the Messier ObjectsHighlights of the Deep Sky, pp. 162 - 163Publisher: Cambridge University PressPrint publication year: 2008