The stellar atmosphere is the outer region of the volume of a
star
A star is an astronomical object comprising a luminous spheroid of plasma held together by its gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye at night, but their immense distances from Earth make ...
, lying above the
stellar core,
radiation zone and
convection zone.
Overview
The stellar atmosphere is divided into several regions of distinct character:
* The
photosphere
The photosphere is a star's outer shell from which light is radiated.
The term itself is derived from Ancient Greek roots, φῶς, φωτός/''phos, photos'' meaning "light" and σφαῖρα/''sphaira'' meaning "sphere", in reference to it ...
, which is the atmosphere's lowest and coolest layer, is normally its only visible part.
Light
Light or visible light is electromagnetic radiation that can be perceived by the human eye. Visible light is usually defined as having wavelengths in the range of 400–700 nanometres (nm), corresponding to frequencies of 750–420 te ...
escaping from the surface of the star stems from this region and passes through the higher layers. The
Sun's photosphere has a
temperature
Temperature is a physical quantity that expresses quantitatively the perceptions of hotness and coldness. Temperature is measured with a thermometer.
Thermometers are calibrated in various temperature scales that historically have relied on ...
in the 5,770
K to 5,780 K range.
Starspot
Starspots are stellar phenomena, so-named by analogy with sunspots.
Spots as small as sunspots have not been detected on other stars, as they would cause undetectably small fluctuations in brightness. The commonly observed starspots are in gen ...
s, cool regions of disrupted
magnetic field
A magnetic field is a vector field that describes the magnetic influence on moving electric charges, electric currents, and magnetic materials. A moving charge in a magnetic field experiences a force perpendicular to its own velocity and t ...
lie on the photosphere.
* 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 100 km.
* The outermost part of the stellar atmosphere is the
corona, a tenuous
plasma which has a temperature above one million Kelvin. While all stars on the
main sequence
In astronomy, the main sequence is a continuous and distinctive band of stars that appears on plots of stellar color versus brightness. These color-magnitude plots are known as Hertzsprung–Russell diagrams after their co-developers, Ejnar Her ...
feature transition regions and coronae, not all
evolved stars do so. It seems that only some
giants, and very few
supergiant
Supergiants are among the most massive and most luminous stars. Supergiant stars occupy the top region of the Hertzsprung–Russell diagram with absolute visual magnitudes between about −3 and −8. The temperature range of supergiant stars s ...
s, possess coronae.
An unresolved problem in stellar
astrophysics
Astrophysics is a science that employs the methods and principles of physics and chemistry in the study of astronomical objects and phenomena. As one of the founders of the discipline said, Astrophysics "seeks to ascertain the nature of the he ...
is how the corona can be heated to such high temperatures. The answer lies in
magnetic field
A magnetic field is a vector field that describes the magnetic influence on moving electric charges, electric currents, and magnetic materials. A moving charge in a magnetic field experiences a force perpendicular to its own velocity and t ...
s, but the exact mechanism remains unclear.
During a total
solar eclipse
A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of the Earth, totally or partially. Such an alignment occurs during an eclipse season, approximately every six mo ...
, the photosphere of the Sun is
obscured, revealing its atmosphere's other layers.
[
] Observed during eclipse, the Sun's chromosphere appears (briefly) as a thin pinkish
arc, and its corona is seen as a tufted
halo
Halo, halos or haloes usually refer to:
* Halo (optical phenomenon)
* Halo (religious iconography), a ring of light around the image of a head
HALO, halo, halos or haloes may also refer to:
Arts and entertainment Video games
* Halo (franchise), ...
. The same phenomenon in
eclipsing binaries
A binary star is a system of two stars that are gravitationally bound to and in orbit around each other. Binary stars in the night sky that are seen as a single object to the naked eye are often resolved using a telescope as separate stars, in ...
can make the chromosphere of giant stars visible.
[
]
See also
*
Cecilia Payne-Gaposchkin, who first proposed the presently-accepted composition of stellar atmospheres
*
Circumstellar envelope
Notes
{{Star
Atmosphere
An atmosphere () is a layer of gas or layers of gases that envelop a planet, and is held in place by the gravity of the planetary body. A planet retains an atmosphere when the gravity is great and the temperature of the atmosphere is low. ...