Nov 23, 2019 Kaʻohe, Mauna Kea, HI (map)
8x42mm Nikon Prostaff 3S Binoculars @ 8x
Large, bright, a misshapen clump of glow about 1° in extent, modestly brighter to the center, easily found off the tip of Triangulum
Aug 21, 2017 Grants Spring, OR (map)
76mm f/6 APO, TeleVue-76 @ 30x
Large, round, about 20' across, gradually brighter to the center fading smoothly into the background at the margins, easily found sweeping north from αTri
Oct 21, 2006 TIMPA, Avra Valley, AZ (map)
12x36 Canon Image Stabilized Binoculars
Large, an oblong hazy patch with no obvious core, just slightly brighter to the center, about 1° across
Oct 24, 2003 Farnsworth Ranch, Pima Co., AZ (map)
46cm f/4.5 Deep Violet
Fantastic! A large diffuse object with a large core, some structure visible at 60x with averted vision, at 175x much of the structure is obvious, particularly the main arms extending north-south from the core and several HII regions with separate designations NGC588, NGC592, NGC595, NGC604, as well as IC137 and IC143, on the whole a sublime and complex scene, a whole new galaxy with the 18
Rev. T.W. Webb
May 19, 1885 Hardwick, Herefordshire, England (map)
Very large, faint, ill defined, visible from its great size (h., nearly ½° n and s, in finder). A very curious object, only fit for low powers, being actually imperceptible, from want of contrast, with my 144. E.of Rosse, who saw it full of knots, found spiral arrangement; two similar curves like an S cross in the centre. Ritchey, who photographed it with the 24-in. at the Yerkes Observatory, with 4 hours' exposure, notes the central parts appear decidedly nebulous, the outer parts parts consist of very faint nebulosity, and numerous curved streams, or wisps of nebulous stars; hundreds of the star-like condensations are shown in the original negative. Closely nf is H. III 150 [NGC604], a small, bright, round neb. with gaseous spect.
― Celestial Objects for Common Telescopes, T. W. Webb, 1917
Sep 15, 1828
Enormously large; very gradually brighter toward the middle. The nucleus taken; has a star of 12 m, north following of the nucleus. The diffused nebula extends 15' south and as much nearly to the north. It has irregularities of light, and even feeble subordinate nuclei and many small stars. Probably H V.17 is part of the diffuse nebula of M33.
Aug 25, 1764
Nebula discovered between the head of the Northern Fish & the great Triangle, a bit distant from a star of 6th magnitude: The nebula is of a whitish light of almost even density, however a little brighter along two-third of its diameter, & contains no star. One sees it with difficulty with an ordinary telescope of 1-foot. Its position was determined from α Trianguli. Seen again September 27, 1780."
― Connaissance des Temps, 1781
Drawings, descriptions, and CCD photos are copyright Andrew Cooper unless otherwise noted, no usage without permission.
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