luminosity class वाक्य
उदाहरण वाक्य
मोबाइल
- The spectral luminosity class is of a bright supergiant, indicating the rarefied nature of its atmosphere and low surface gravity.
- Although it is given a supergiant luminosity class, it is effectively a main sequence star still burning hydrogen in its core.
- There is an MKK luminosity class 0 ( zero ) for hypergiants, but this is rarely seen in published spectral classifications.
- The giant phase for such stars is a brief phase of slightly increased size and luminosity before developing a supergiant spectral luminosity class.
- It is an asymptotic giant branch star of spectral type M6S, with a luminosity class of Ib, indicating a supergiant luminosity.
- Alpha Leporis has a stellar classification of F0 Ib, with the Ib luminosity class indicating that it is a lower luminosity supergiant star.
- The stellar classification of this star is K3 IIIa, where the luminosity class of III indicates that this is an evolved giant star.
- The spectrum of ? Aql A matches a stellar classification of F3, with the luminosity class of Ib indicating this is a supergiant.
- Synthetic spectra indicate that it would never have a main sequence luminosity class ( V ), or even a normal O type spectrum.
- Classical Cepheid variables typically have supergiant luminosity classes, although only the most luminous and massive will actually go on to develop an iron core.
- The spectrum matches a stellar classification of K0 III-IV, with the luminosity class of III-IV corresponding to an giant stages.
- The Ib luminosity class indicates this a lower luminosity supergiant star that has consumed the hydrogen fuel at its core, K-type star.
- The brightest O7-8V main sequence stars in Wd1 have luminosity class Ib and II ( V-band magnitudes of 18 20 ).
- Some of these features are used to determine the luminosity class, for example certain near-infrared cyanogen band strengths and the Ca II triplet.
- A luminosity class V star belongs on the main sequence, which means it is generating energy through the thermonuclear fusion of hydrogen at its core.
- The spectrum of this star matches a stellar classification of B5 III, with the luminosity class of III indicating that this is a giant star.
- The spectrum of the primary component matches a stellar classification of K0 IV, with the luminosity class of IV indicating this is a subgiant star.
- The luminosity class'V'means this is a main sequence star that is generating energy through the thermonuclear fusion of hydrogen at its core.
- They have supergiant spectral luminosity classes despite their modest masses and actual luminosities, because they are highly inflated evolved stars with very low surface gravities.
- Luminosity class V, main-sequence stars, generally have weak or missing emission lines, with giants and supergiants showing increasing emission line strength.
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