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Supernova Remnants

A supernova remnant is made of material ejected from an eploding star. A star that is roughly three times more massive than the sun or larger is doomed to end this way. When it does, it ejects most of its material in a rapidly expanding shock wave. This then seeds the surrounding area with heavier elements that go on to be part of new stars, solar systems, planets, trees, and cats. These remnants often contain copious amounts of ionized hydrogen and oxygen, which makes them particularly photogenic to astrophotographers using specialized filters.

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The Lifecycle of Stars – Star birth, Planetary Nebulas, and Supernovas
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Messier 1 - The Crab Nebula
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IC 2118 - Witch Head Nebula & Rigel Mosaic
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Serpens Mosaic (feat. M16 & M17)
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NGC 6974 & 6979
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NGC 6995 (Caldwell 33) – The Bat Nebula
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NGC 6960 (Caldwell 34) – The Witch’s Broom
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NGC 6979 – Pickering’s Triangle
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The Veil Nebula

Gallery

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