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Description: Observations of Nebulae and Clusters of Stars, Made at Slough, with a Twenty-Feet Reflector, between the Years 1825 and 1833 in Philosophica Transactions of the Royal Society, London, 1833
The Dumbbell Nebula (M27), is a large, bright planetary nebula which was discovered by the French astronomer Charles Messier in 1764 as the very first object of its kind. [12] It can be seen with good binoculars in a dark sky location, appearing as a dimly glowing disk approximately 8 arcminutes in diameter. [13] The nebula is approximately ...
English: HaRGB image of The Little Dumbbell Nebula (M76). Data from the Liverpool Telescope (a 2 m RC telescope on La Palma) processed by Göran Nilsson and Wim van Berlo. 150 exposures totalling 4.2 hours
To mark 34 years of service, the Hubble Space Telescope captured an image of the Little Dumbbell Nebula, which may contain evidence of one star devouring another.
The Dumbbell Nebula (also known as the Apple Core Nebula, Messier 27, and NGC 6853) is a planetary nebula (nebulosity surrounding a white dwarf) in the constellation Vulpecula, at a distance of about 1360 light-years. [1] It was the first such nebula to be discovered, by Charles Messier in 1764.
In 1991, Newton became the first amateur astrophotographer to make full color CCD images of celestial objects using a Santa Barbara Instruments Group ST-4 camera, making a full color CCD image of M57, the "Ring Nebula" and M27, the "Dumbbell Nebula".
The Little Dumbbell Nebula, also known as Messier 76, NGC 650/651, the Barbell Nebula, or the Cork Nebula, [1] is a planetary nebula in the northern constellation of Perseus. It was discovered by Pierre Méchain in 1780 and included in Charles Messier 's catalog of comet -like objects as number 76.
This is a list of NGC objects 6001–7000 from the New General Catalogue (NGC). The astronomical catalogue is composed mainly of star clusters, nebulae, and galaxies.Other objects in the catalogue can be found in the other subpages of the list of NGC objects.