Monday, June 11, 2007

Merope Reflection

The Merope Reflection Nebula
Credit & Copyright: Jean-Charles Cuillandre (CFHT), Hawaiian Starlight, CFHT

Reflection nebulas reflect light from a nearby star. Many small carbon grains in the nebula reflect the light.

The blue colour 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 colour and brightness of the neighbouring 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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