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Astronomy Picture of the Day
Index - Nebulae: Reflection Nebulae

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Editor's choices for the most educational Astronomy Pictures of the Day about reflection nebulae:

Thumbnail image.  Click to load APOD for this date. APOD: 1999 October 31 - The Witch Head Nebula
Explanation: Double, double toil and trouble; Fire burn, and cauldron bubble ... Maybe Macbeth should have consulted the Witch Head Nebula. This suggestively shaped reflection nebula is associated with the bright star Rigel in the constellation Orion. More formally known as IC 2118, the Witch Head Nebula glows primarily by light reflected from Rigel. Rigel is located about one photo-width off the image to the right. Fine dust in the nebula reflects the light. The blue colour is caused not only by Rigel's blue colour but because the dust grains reflect blue light more efficiently than red. The same physical process causes Earth's daytime sky to appear blue, although the scatterers here are molecules of nitrogen and oxygen. The nebula lies about 1000 light-years away.

Thumbnail image.  Click to load APOD for this date. APOD: 1999 March 1 - Reflection Nebula NGC 1435
Explanation: Reflection nebulae 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. The unusual area on the far left, known as Bernard's Merope Nebula (IC 349), reflects visible light with unusually high efficiency.

Thumbnail image.  Click to load APOD for this date. APOD: 2000 March 2 - NGC 1999: Reflection Nebula In Orion
Explanation: A dusty bright nebula contrasts dramatically with a dusty dark nebula in this Hubble Space Telescope image recorded shortly after December's orbital servicing mission. The nebula, catalogued as NGC 1999, is a reflection nebula, which shines by reflecting light from a nearby star. Unlike emission nebulae, whose reddish glow comes from excited atoms of gas, reflection nebulae have a bluish cast as their interstellar dust grains preferentially reflect blue starlight. While perhaps the most famous reflection nebulae surround the bright young stars of the Pleiades star cluster, NGC 1999's stellar illumination is provided by the embedded variable star V380 Orionis, seen here just left of centre. Extending right of centre, the ominous dark nebula is actually a condensation of cold molecular gas and dust so thick and dense that it blocks light. >From our perspective it lies in front of the bright nebula, silhouetted against the ghostly nebular glow. New stars will likely form within the dark cloud, called a Bok globule, as self-gravity continues to compress its dense gas and dust. Reflection nebula NGC 1999 lies about 1500 light-years away in the constellation Orion, just south of Orion's well known emission nebula, M42.

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