4 Jan 2015 Waikoloa, HI (map)
28cm f/10 SCT, NexStar 11" Gypsy @ 80x
Big, beautiful, rich, a distinct cluster of hundreds of members in a 20' area, quite distinct, fully resolved, a notable orange star at the center (HD 39183 magV 9.16)
21 Oct 2006 TIMPA, Avra Valley, AZ (map)
12x36 Canon Image Stabilized Binoculars
Good sized, bright, easily found, not resolved, a round patch of fuzz, M36 one field west
30 Sep 2005 Gila, New Mexico (map)
90mm F/12 APO Violet Haze
Large! Rich! beautiful cluster of hundreds of well matched stars, a large central group with several clumps to the sides separated by slight rifts
25 Mar 1998 Sycamore House, Tucson, AZ (map)
20cm f/10 SCT
Dimmer than M36 or M38, but far more visible members, yes the magnitude shows brighter, but few bright members gives the eye the impression of a dimmer object, I will not attempt to draw this crowd tonight
2 Jan 1764
Cluster of small stars, little remote from the preceding [M36], above the parallel of chi Aurigae; the stars are smaller, more close together and enclosing some nebulosity; with an ordinary telescope of 3.5 feet, one has pain to see the stars: this cluster is reported on the Chart of the second Comet of 1771, Mem. Acad. 1777."
Rev. T.W. Webb
Hardwick, Herefordshire, England (map)
Sm. calls this 'a magnificent object;' the whole field being strewed, as it were, with sparkling gold dust; the group is resolvable into about 500 stars, from 10 to 14 mg., besides the outliers. Even in smaller instruments extremely beautiful, one of the finest in its class. Gaze at it well and long. K. notices a brighter star near centre, Burton: ruby: 10, Es.: 9.0: pale red. All the stars in the mass must be nearly at the same distance from us, and consequently their real sizes must be different. The aspect of the Nubucula Major in the S. Hemisphere convinced h. of this: it is ocular proof of the incontrovertible, though long discredited fact, that the apparent brightness of stars has very little connection with their distance from the earth. E. of Rosse, wonderful loops and curved lines of stars, first remarked by D'A.
6 objects found within 120'
Drawings, descriptions and CCD photos are copyright Andrew Cooper unless otherwise noted, no usage without permission. Use for non-profit and educational reasons is generally given on request.
Positional and some physical information is from the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Additional object data from the SIMBAD database, operated at CDS, Strasbourg, France.
The Digitized Sky Survey was produced at the Space Telescope Science Institute under U.S. Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope.
Dark nebulae data from E.E. Barnard, A Photographic Atlas of Selected Regions of the Milky Way. Ed. Edwin B. Frost and Mary R. Calvert. Carnegie Institution of Washington, 1927
Object descriptions of Rev. Webb from Celestial Objects for Common Telescopes sixth edition, Rev. T.W. Webb, 1917, edited by Rev T.E.Espin.