The stellar atmosphere is the outer region of the volume of a star, lying above the stellar core, radiation zone and convection zone.
OverviewEdit
The stellar atmosphere is divided into several regions of distinct character:
- The photosphere, which is the atmosphere's lowest and coolest layer, is normally its only visible part.<ref name="BrightPS"/> Light escaping from the surface of the star stems from this region and passes through the higher layers. The Sun's photosphere has a temperature in the Template:Cvt range.<ref name="lowTemp">Template:Cite book</ref><ref name = "higherTemp"/> Starspots, cool regions of disrupted magnetic field, lie in the photosphere.<ref name = "higherTemp">Template:Cite book</ref>
- Above the photosphere lies the chromosphere. This part of the atmosphere first cools down and then starts to heat up to about 10 times the temperature of the photosphere.
- Above the chromosphere lies the transition region, where the temperature increases rapidly on a distance of only around Template:Cvt.<ref>Template:Cite book</ref>
- Additionally, many stars have a molecular layer (MOLsphere) above the photosphere and just beyond or even within the chromosphere.<ref>Template:Cite journal</ref> The molecular layer is cool enough to contain molecules rather than plasma, and may consist of such components as carbon monoxide, water vapor, silicon monoxide, and titanium oxide.
- The outermost part of the stellar atmosphere, or upper stellar atmosphere, is the corona, a tenuous plasma which has a temperature above one million Kelvin.<ref>Template:Cite journal</ref> While all stars on the main sequence feature transition regions and coronae, not all evolved stars do so. It seems that only some giants, and very few supergiants, possess coronae. An unresolved problem in stellar astrophysics is how the corona can be heated to such high temperatures. The answer is believed to lie in magnetic fields, but the exact mechanism remains unclear.<ref>{{#invoke:citation/CS1|citation
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- The astrosphere, which is in the case of the Sun the heliosphere,<ref name="Sterken Baalmann Draine Godenko 2022 p. ">Template:Cite journal</ref> can be in a broader understanding considered the furthest part of a stellar atmosphere,<ref name="NASA Science 2017 b915">{{#invoke:citation/CS1|citation
|CitationClass=web }}</ref><ref name="NASA 2013 z570">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> before interstellar space begins at the heliopause. The astrosphere is not to be confused with the Solar System and its outermost region the Oort cloud, which extends much further than the astrosphere, therefore far into interstellar space.
During a total solar eclipse, the photosphere of the Sun is obscured, revealing its atmosphere's other layers.<ref name = "BrightPS"> {{#invoke:citation/CS1|citation |CitationClass=web }}</ref> Observed during eclipse, the Sun's chromosphere appears (briefly) as a thin pinkish arc,<ref> Template:Cite book </ref> and its corona is seen as a tufted halo. The same phenomenon in eclipsing binaries can make the chromosphere of giant stars visible.<ref> Template:Cite book
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See alsoEdit
- Cecilia Payne-Gaposchkin, who first proposed the presently-accepted composition of stellar atmospheres
- Circumstellar envelope
- Heliosphere