stellar classification oor Spaans
stellar classification
Vertalings in die woordeboek Engels - Spaans
clasificación estelar
en
classification of stars based on their spectral characteristics
es
clasificación de estrellas sobre la base de sus características espectrales
Geskatte vertalings
Vertoon algoritmies gegenereerde vertalings
voorbeelde
Advanced filtering
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The stellar classification of this star has been rated from M1.5V to M4.0V by various sources.
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This is the most common stellar classification system used by astronomers today.
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They are also used in astrographic telescopes where multiple single narrow wavelength images are used in stellar classification .
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Other modern stellar classification systems, such as the UBV system, are based on color indexes—the measured differences in three or more color magnitudes.
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Kappa Andromedae has a stellar classification of B9 IVn, indicating that it is a subgiant star in the process of evolving away from the main sequence.
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The MK system remains the standard stellar spectral classification system used by astronomers today.
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The Hertzsprung–Russell diagram, abbreviated as H–R diagram, HR diagram or HRD, is a scatter plot of stars showing the relationship between the stars' absolute magnitudes or luminosities versus their stellar classifications or effective temperatures.
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Keenan was an American spectroscopist who collaborated with William Wilson Morgan and Edith Kellman (1911–2007) to develop the MKK stellar spectral classification system between 1939 and 1943.
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Libraries of stellar spectra by D. Montes, UCM Spectral Types for Hipparcos Catalogue Entries Stellar Spectral Classification by Richard O. Gray and Christopher J. Corbally Spectral models of stars by P. Coelho Merrifield, Michael; Bauer, Amanda; Häußler, Boris (2010).
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This Wikipedia article on stellar classification lists types of stars based on their temperature.
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Stellar classification In astronomy, stellar classification is the classification of stars based on their spectral characteristics.
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Stellar classification In astronomy, stellar classification is the classification of stars based on their spectral characteristics.
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The Hertzsprung–Russell diagram relates stellar classification with absolute magnitude, luminosity, and surface temperature.
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The Hertzsprung-Russell diagram relates stellar classification with absolute magnitude, luminosity, and surface temperature.
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You can read an explanation of this classification system in the Wikipedia: Stellar classification
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The primary, component A, is a magnitude 4.95 evolved giant star with a stellar classification of G8 III.
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Included in the category are white dwarfs, and as can be seen from the radically different classification scheme for class D, non-stellar objects are difficult to fit into the MK system.
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O and B are the two hottest stellar classifications and most stars of these types are very brilliant blue-white stars, and relatively young.
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Several spectral types, all previously used for non-standard stars in the mid-20th century, have been replaced during revisions of the stellar classification system.
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Edit Annie Jump Cannon (/ˈkænən/; December 11, 1863 – April 13, 1941) was an American astronomer whose cataloging work was instrumental in the development of contemporary stellar classification.
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Also known as Harvard spectral classification. It is the most used stellar classification in astronomy where the different types are sorted according to the temperature of the star.
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Temperature classification The current stellar classification system originated in the early 20th century, when stars were classified from A to Q based on the strength of the hydrogen line.
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Using the newfound oscillator strengths the researchers identified key atomic transitions important in classification of the previously poorly understood atmospheric components of cool stellar and substellar objects.
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The Hertzsprung–Russell diagram, abbreviated H–R diagram or HRD, is a scatter plot of stars showing the relationship between the stars' absolute magnitudes or luminosities versus their stellar classifications or effective temperatures.
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This team included Annie Jump Cannon, who developed the stellar classification system, and Henrietta Swan Leavitt, who discovered the means to measure the distance from a star to the earth by its spectra, later used to identify other galaxies in the universe.
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