My Astrophotography – Lynds Nebulae (LBN/LDN)

Lynds Nebulae Objects
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LBN are a fascinating collection of luminous nebulae catalogued by American astronomer Beverly Turner Lynds in 1965.
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The catalogue includes 1,126 bright nebulae observed using the 48-inch Palomar Schmidt telescope, and each entry is designated with the prefix LBN followed by a number.
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Lynds’ Bright Objects are a catalog of glowing clouds in space that helps astronomers find and study places where stars are forming.
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The Lynds Bright Nebulae (LBN) and Lynds Dark Nebulae (LDN) catalogues
both come from Beverly Turner Lynds, but they focus on very two different types of nebulae:

1) Bright – LBN objects are bright glowing clouds in space.
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2 ) Dark – LDN objects are dark dust clouds that block the light from stars behind them.
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1) Bright (LBN)

Lynds Bright Nebulae (LBN)
Emission and reflection nebulae that emit or reflect light, helping by regions of active star formation and ionized gas.

2) Dark (LDN)

Lynds Dark Nebulae (LDN)
Dense clouds of dust that block light from stars behind them.

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(See an example of clouds into two main types)
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Lynds Bright & Dark Nebulae (LBN/LDN)

Beverly Lynds created both catalogs to help astronomers identify and study these amazing clouds.
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Each object has its own number, such as LBN 438 or LDN 1622.

LBD & LDN in the California Nebula (NGC1499)

Lynds Bright & Dark Nebulae in
the California Nebula Region 👆🏻

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My archived astrophotography – Lynds Bright & Dark Nebulae (LBN/LDN)
Click the image below to view a larger version with the explanation.
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