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Legacy article – Astronomy and observation

Orion Nebula – M42

Original publication date
6 November 2010
Original section
Astronomy and observation
Original slug / legacy ID
orion-nebula-m42 / 183
Restored on current site
martinpeniak.com/archive/writing/orion-nebula-m42/
Editing scope
Period voice retained; spelling and formatting lightly cleaned.

Originally published 6 November 2010 on the earlier martinpeniak.com site.

Preserved as part of the astronomy and observation thread around cameras, optics, and the sky. The article keeps its period voice, with light formatting cleanup.

The Orion Nebula (also known as Messier 42, M42, or NGC 1976) is a diffuse nebula situated south of Orion's Belt. It is one of the brightest nebulae, and is visible to the naked eye in the night sky. M42 is one of the most scrutinized and photographed objects in the night sky, and is among the most intensely studied celestial features.The nebula has revealed much about the process of how stars and planetary systems are formed from collapsing clouds of gas and dust. Astronomers have directly observed protoplanetary disks, brown dwarfs, intense and turbulent motions of the gas, and the photo-ionizing effects of massive nearby stars in the nebula. There are also supersonic "bullets" of gas piercing the dense hydrogen clouds of the Orion Nebula. Each bullet is ten times the diameter of Pluto's orbit and tipped with iron atoms glowing bright blue. They were probably formed one thousand years ago from an unknown violent event.

M42