The Lagoon Nebula, M8 // RichR
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The Lagoon Nebula, M8 // RichR

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Sketches of Messier 42 and More
More astronomy posting! This time! Emission Nebulae.
Emission nebulae are where gas and dust in the galaxy collapses under gravity to form new stars, with new planets around those stars. Each of these objects are in the process of forming solar systems. When especially hot stars are formed in these nebulae, they emit ultraviolet radiation which 'powers' the nebula, and causes it to glow in visible light.
Let's look at the best such nebula in the sky visible from the northern hemisphere: Messier 42, aka The Great Nebula in Orion. It is seen in winter or early spring evenings in the northern hemisphere, or summer and early autumn in the southern hemisphere. (It is near enough to the equator to be visible from most latitudes.)
We'll zoom in starting from binoculars, moving up to a small toy telescope, and then a large 10" reflector.
Text transcription, and more sketches including a beautiful view with a large telescope, below the read-more!
स्वर्गम्🌌🌈
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This is the Lagoon Nebula! 💗💗💗
The beautiful lagoon shaped portion is created from aggressive stellar winds pushing the nebulae’s gas and dust aside. Many of the stars here are young, hot O-type stars that are more than 200,000 times brighter than the Sun! ✨✨✨
Taken by me (Michelle Park) using the Slooh Canary Two telescope on July 23rd, 2022 at 22:31 UTC.
The Trifid (M20, NGC 6514) & The Lagoon Nebula ( M8, NGC 6523)
Constellation Sagittarius.
Distance to Earth: 5.200 & 4.100 light years.
DSLR Canon Rebel T3i
Montcada i Reixac (Bortle 8)

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LAGOON NEBULA Messier 8, or the Lagoon Nebula, is visible just above the Saggitarius star cloud. What appears as a grey patch to viewers from Earth is actually a vast stellar nursery 100 light-years across teeming with massive young stars and delicate wisps of glowing hydrogen-rich gas.
Lagoon Nebula (M8, Messier 8)
Starry night
4,000 light years from Earth, the Lagoon Nebula is seen with its swirling clouds of gas and dust in a pattern reminiscent of Van Gogh. This nebula provides astronomers an excellent opportunity to study the properties of very young stars. Many infant stars give off copious amounts of high-energy light including X-rays, which are seen in the Chandra X-ray data (in pink) to reveal the infant stars budding in the surreal nightscape. The X-ray data have been combined with an optical image of Messier 8 from the Mt. Lemmon Sky Center in Arizona. Credit: X-ray: NASA/CXC/SAO; Optical: Adam Block/Mount Lemmon SkyCenter/University of Arizona