Celestial hemisphere:  Northern  ·  Constellation: Orion (Ori)  ·  Contains:  HD290829  ·  HD290830  ·  HD290859  ·  HD290862  ·  HD290864  ·  HD290865  ·  HD290883  ·  HD290889  ·  HD290890  ·  HD38238  ·  HD38248  ·  HD38311  ·  HD38563  ·  LDN 1627  ·  M 78  ·  NGC 2064  ·  NGC 2067  ·  NGC 2068  ·  NGC 2071  ·  PGC 3085073  ·  PGC 3085076
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M78 in RGB, Mau_Bard
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M78 in RGB

Getting plate-solving status, please wait...
M78 in RGB, Mau_Bard
Powered byPixInsight

M78 in RGB

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Description

This is one of my first recordings with my 200mm f/5 Newtonian, made on the nights of 28 February, 6 and 7 March 2021. At that time, notwithstanding the effort infused into it, I was not able to get a satisfactory result, therefore I never published it. I have completely reprocessed it now, after two years, with the help of better tools and with a bit more experience.

My favorite place in this image is the dark nebula south of M78: a stellar nursery hosting a quantity of young stellar objects (YSO), Herbig Haro and T Tauri stars.

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Messier 78, 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.

M78 is the brightest diffuse reflection nebula of a group of nebulae that includes NGC 2064, NGC 2067 and NGC 2071, all visible in the picture here. This group belongs to the Orion B molecular cloud complex and is about 1,350 light-years distant from Earth. M78 is easily found in small telescopes as a hazy patch and involves two stars of 10th and 11th magnitude. These two B-type stars, HD 38563 A and HD 38563 B, are responsible for making the cloud of dust in M78 visible by reflecting their light.

The M78 cloud contains a cluster of stars that is visible in the infrared. Due to gravity, the molecular gas in the nebula has fragmented into a hierarchy of clumps, whose cores have masses ranging from 0.3 M☉ to 5 M☉. About 45 variable stars of the T Tauri type, young stars still in the process of formation, are members as well. Similarly, 17 Herbig–Haro objects are known in M78.

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