Celestial hemisphere:  Northern  ·  Constellation: Cassiopeia (Cas)  ·  Contains:  4 Cas  ·  Bubble Nebula  ·  M 52  ·  NGC 7538  ·  NGC 7635  ·  NGC 7654  ·  PK112-00.1  ·  Sh2-157  ·  Sh2-158  ·  Sh2-159  ·  Sh2-161  ·  Sh2-162  ·  The star 4Cas
The Bubble, M52, Et Al., schmaks
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The Bubble, M52, Et Al.

The Bubble, M52, Et Al., schmaks
Powered byPixInsight

The Bubble, M52, Et Al.

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Description

Most nebulae can be described as diffuse nebulae, which means that they are extended and contain no well-defined boundaries. In visible light these nebulae may be divided into emission and reflection nebulae. Emission nebulae emit spectral line radiation from ionized gas (mostly ionized hydrogen); they are often called HII regions.

Reflection nebulae themselves do not emit significant amounts of visible light, but are near stars and reflect light from them. Similar nebulae not illuminated by stars do not exhibit visible radiation, but may be detected as opaque clouds blocking light from luminous objects behind them; they are called “dark nebulae.”

Although these nebulae have different visibility at optical wavelengths, they are all bright sources of infrared emission, chiefly from dust within the nebulae.

Famed examples of emission nebulae include the Orion Nebula and Carina Nebula, both of which are stellar nurseries with hot O and B type stars.

The Pleiades in Taurus are an open star cluster passing through a dust cloud which scatters their blue light back to Earth in the form of a reflection nebula.

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