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Stellar atmosphere information


Photo taken in France during the 1999 solar eclipse

The stellar atmosphere is the outer region of the volume of a star, lying above the stellar core, radiation zone and convection zone.

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Stellar atmosphere

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The stellar atmosphere is the outer region of the volume of a star, lying above the stellar core, radiation zone and convection zone. The stellar atmosphere...

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Atmosphere

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object. A planet retains an atmosphere when the gravity is great and the temperature of the atmosphere is low. A stellar atmosphere is the outer region of...

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Saha ionization equation

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disappearances of absorption lines in the stellar sequence, assuming an order of magnitude for the pressure in a stellar atmosphere and calculating the temperature...

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Star

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of the photosphere is the stellar atmosphere. In a main sequence star such as the Sun, the lowest level of the atmosphere, just above the photosphere...

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Stellar wind

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A stellar wind is a flow of gas ejected from the upper atmosphere of a star. It is distinguished from the bipolar outflows characteristic of young stars...

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Astrophysics

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Radcliffe College, in which she applied Saha's ionization theory to stellar atmospheres to relate the spectral classes to the temperature of stars. Most...

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Stellar core

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the stellar envelope, which transports energy from the core to the stellar atmosphere where it is radiated away into space. Main sequence stars are distinguished...

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Stellar classification

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In astronomy, stellar classification is the classification of stars based on their spectral characteristics. Electromagnetic radiation from the star is...

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Molecules in stars

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been found on the Sun, and there is evidence of H2 in white dwarf stellar atmospheres. Cooler stars include absorption band spectra that are characteristic...

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Astrophysical maser

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emission may arise in molecular clouds, comets, planetary atmospheres, stellar atmospheres, or various other conditions in interstellar space. Like a...

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Effective temperature

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certain value of the Rosseland optical depth (usually 1) within the stellar atmosphere. The effective temperature and the bolometric luminosity are the two...

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Edward Arthur Milne

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outer layers known as stellar atmospheres that produce the radiation observed from the Earth. He considered a grey atmosphere, a simplifying approximation...

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Star lifting

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reverse the stations' fall. This would "squeeze" the star, propelling stellar atmosphere through the polar magnetic nozzles. The ring current would be shut...

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Glossary of astronomy

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the stellar atmosphere; or another name for the stellar atmosphere itself. 2.  The common envelope of gases encompassing a binary star system. stellar evolution...

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Variable star

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indication of a hot stellar atmosphere, or gas clouds surrounding the star. In very few cases it is possible to make pictures of a stellar disk. These may...

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Dubhe

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1990), "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances", Astrophysical Journal Supplement Series...

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Eddington luminosity

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charges, which are typically free protons under the conditions in stellar atmospheres. When the outward electric field is sufficient to levitate the protons...

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Binary star

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close enough they can gravitationally distort each other's outer stellar atmospheres. In some cases, these close binary systems can exchange mass, which...

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Flare star

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flash phase is primarily due to thermal radiation from the heated stellar atmosphere. As the material reaches the corona, the intensive release of energy...

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Grey atmosphere

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grey atmosphere (or gray) is a useful set of approximations made for radiative transfer applications in studies of stellar atmospheres (atmospheres of stars)...

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Atmosphere of Pluto

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temperatures. Existence of the atmosphere of Pluto was proven via stellar occultation. If a star is occulted by a body without an atmosphere, its light disappears...

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Procyon

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within 10 to 100 million years. The effective temperature of the stellar atmosphere is an estimated 6,530 K, giving Procyon A a white hue. It is 1.5 times...

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Spectral signature

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The spectral signature of stars indicates the composition of the stellar atmosphere. The spectral signature of an object is a function of the incidental...

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Radiative equilibrium

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star, but not in a planet's atmosphere. Subrahmanyan Chandrasekhar (1950, page 290) writes of a model of a stellar atmosphere in which "there are no mechanisms...

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Stellar nucleosynthesis

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star. Later in its life, a low-mass star will slowly eject its atmosphere via stellar wind, forming a planetary nebula, while a higher–mass star will...

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