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Created page with 'File:lighterstill.jpgright|frame ==Etymology== Latin accretion-, accretio, from accrescere *Date: [http://www.wikipedia/org/wiki/17th_Century...'
[[File:lighterstill.jpg]][[File:AccretionDisk.jpg|right|frame]]

==Etymology==
[[Latin]] accretion-, accretio, from accrescere
*Date: [http://www.wikipedia/org/wiki/17th_Century 1615]
==Definitions==
*1 : the process of growth or enlargement by a gradual buildup: as a : increase by external addition or accumulation (as by adhesion of external parts or particles) b : the increase of land by the action of natural forces
*2 : a product of accretion; especially : an extraneous addition <accretions of grime>
==Description (Physics)==
An '''accretion disc''' is a [[structure]] (often a circumstellar disk) formed by [[diffuse]] [[material]] in orbital [[motion]] around a central [[body]]. The central body is typically a young [[star]], a [http://en.wikipedia.org/wiki/Protostar protostar], a [http://en.wikipedia.org/wiki/White_dwarf white dwarf], a [http://en.wikipedia.org/wiki/Neutron_star neutron star], or a [http://en.wikipedia.org/wiki/Black_hole black hole]. [[Gravity]] causes material in the disc to spiral inward towards the central body. Gravitational [[forces]] compress the material causing the emission of [http://www.wikipedia.org/wiki/Electromagnetic_Radiation electromagnetic radiation]. The [[frequency]] range of that radiation depends on the central object. Accretion discs of young stars and protostars radiate in the infrared; those around neutron stars and black holes in the x-ray part of the [[spectrum]].[http://en.wikipedia.org/wiki/Accretion_disk]

[[Category: Physics]]
[[Category: General Reference]]

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