Explanation: Reflection nebulas reflect light from a nearby star. Many small carbon grains in the nebula reflect the light. The blue color typical of reflection nebula is caused by blue light being more efficiently scattered by the carbon dust than red light. The brightness of the nebula is determined by the size and density of the reflecting grains, and by the color and brightness of the neighboring star(s). NGC 1435, pictured above, surrounds Merope (23 Tau), one of the brightest stars in the Pleiades (M45). The Pleiades nebulosity is caused by a chance encounter between an open cluster of stars and a molecular cloud.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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NASA Official: Jay Norris. Specific rights apply.
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& Michigan Tech. U.

Publikacii s klyuchevymi slovami: reflection nebula - Merope - otrazhatel'nye tumannosti - otrazhenie Publikacii so slovami: reflection nebula - Merope - otrazhatel'nye tumannosti - otrazhenie
Sm. takzhe: IC 348 i Barnard 3 Prizraki v Kassiopee NGC 6727: tumannost' Buinyi Pavian NGC 7023: tumannost' Iris M78 ot kosmicheskogo teleskopa "Evklid" Svet, temnota i pyl' Otrazheniya tumannosti Prizrak Vse publikacii na tu zhe temu >>