411 REFERENCE · Wikibooks
Messier Index/M78
Reference material by Wikibooks contributors. This retains its source identity and is not 411 news reporting.
M78 Reflection J2000.0 05h 46.7m +00° 03′ 1,600 ly 8.3 8′ × 6′ Orion 2 - Part of the Orion Complex NGC 2068, Ced55u
The nebula Messier 78 (also known as M 78 or NGC 2068) is a w:reflection nebula in the w:constellation Orion. It was discovered by w:Pierre Méchain in w:1780 and included by w:Charles Messier in his catalog of w:comet-like objects that same year.
M78 is the brightest diffuse reflection nebula of a group of nebulae that include NGC 2064, NGC 2067 and NGC 2071. This group belongs to the w:Orion Molecular Cloud Complex and is about 1,600 w:light years distant from w:Earth. M78 is easily found in small w:telescopes as a hazy patch and involves two w:stars of 10th magnitude. These two stars, HD 38563A and HD 38563B, are responsible for making the cloud of dust in M78 visible by reflecting their light.
About 45 w:variable stars of the T Tauri type, young stars still in the process of formation as well as some 17 w:Herbig-Haro objects are known in M78.
External links
Messier 78, SEDS Messier pages
M78: Stardust and Starlight
NightSkyInfo.com - M78