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Messier 78 or M78, also known as NGC 2068, is a reflection nebula in the constellation Orion. It was discovered by Pierre Méchain in 1780 and included by Charles Messier in his catalog of comet-like objects that same year. [4] M78 is the brightest diffuse reflection nebula of a group of nebulae that includes NGC 2064, NGC 2067 and NGC 2071.
Charles Messier. The first edition of 1774 covered 45 objects (M1 to M45).The total list published by Messier in 1781 contained 103 objects, but the list was expanded through successive additions by other astronomers, motivated by notes in Messier's and Méchain's texts indicating that at least one of them knew of the additional objects.
Germain Amphitheater (originally Polaris Amphitheater) was a 20,000-seat outdoor entertainment venue located in Columbus, Ohio, near the suburb of Westerville. The venue opened as part of a large development venture off of Interstate Highway I-71. There were 6,700 seats in an open-air pavilion—much of it under cover—and room for another ...
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Images Names and designations 6: Bug Nebula: Sh2-6, NGC 6302, Bug Nebula, PK 349+01 1, Butterfly Nebula, RCW 124, Gum 60, Caldwell 69 8: NGC 6334: ESO 392-EN 009, Sharpless 8, RCW 127, Gum 64, NGC 6334 11: War and Peace Nebula: Sh2-11, NGC 6357, RCW 131, Gum 66, War and Peace Nebula 25: Lagoon Nebula: Sh2 25, RCW 146, Gum 72, Messier 8 29 ...
The M81 Group is a galaxy group in the constellations Ursa Major and Camelopardalis that includes the galaxies Messier 81 and Messier 82, as well as several other galaxies with high apparent brightnesses. [1] The approximate center of the group is located at a distance of 3.6 Mpc, making it one of the nearest groups to the Local Group. [1]
NGC 2071 with Euclid in the infrared. NGC 2071 is a reflection nebula in the constellation Orion.It was discovered on January 1, 1784, by William Herschel. [1] It is part of a group of nebulae that also includes Messier 78, NGC 2064, and NGC 2067.
Infrared images of the Trapezium are better able to penetrate the surrounding clouds of dust, and have located many more stellar components. About half the stars within the cluster exhibit circumstellar disks that are dwindling, a likely precursor to planetary formation.
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