Примеры использования Main sequence на Английском языке и их переводы на Русский язык
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It is effectively a main sequence star.
Stars in the main sequence are mainly composed of hydrogen in its plasma state.
The two stars are both on the main sequence.
The internal structure of a main sequence star depends upon the mass of the star.
It is in a very close orbit with an O9.5 main sequence star.
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The cooling star is now off the main sequence and is known as a helium white dwarf.
The primary has a stellar classification of G3V,which is a G-type main sequence star.
COROT-1 is a yellow dwarf main sequence star similar to our Sun.
On a Hertzsprung-Russell diagram subdwarfs appear to lie below the main sequence.
It has sometimes been classified as a main sequence star and sometimes as a giant star.
The brightest is an O8 star just beginning to evolve away from the main sequence.
The primary component is a white A-type main sequence star with an apparent magnitude of +7.48.
The team investigating M85 OT2006-1 believe it to have formed when two main sequence stars merged.
The third component is a B0.5 main sequence star in a long eccentric orbit around the close pair.
This lifespan greatly exceeds the current age of the universe,therefore all red dwarfs are main sequence stars.
This marks the end of the Sun's main sequence lifetime, and thereafter it will pass through the subgiant stage and evolve into a red giant.
The sun has all the properties of a main sequence dwarf star.
Even without circumstellar dust, regions undergoing star formation exhibit high infrared luminosities compared to stars on the main sequence.
Gliese 667 is a triple star system with two K-type main sequence stars and a red dwarf.
Young stellar groups can contain a number of infant T Tauri stars that are still in the process of entering the main sequence.
The primary component, Theta Virginis Aa, is a white-hued A-type main sequence star with a stellar classification of A1Vs.
The energy source of these objects is gravitational contraction,as opposed to hydrogen burning in main sequence stars.
Individually each star is a fairly unremarkable A class main sequence star, but as a binary pair they are unusual.
In particular, during their hydrogen burning period,stars lie along a curve in the diagram called the main sequence.
It orbits HD 195689(or KELT-9), a late B-type main sequence star about 620 light-years(190 parsecs) from Earth.
To compensate for the temperature increase,the outer envelope expanded to many times the radius it possessed as a main sequence star.
Its companion(IK Pegasi B) is a massive white dwarf-a star that has evolved past the main sequence and is no longer generating energy through nuclear fusion.
A pre-main-sequence star(also known as a PMS star and PMS object)is a star in the stage when it has not yet reached the main sequence.
The protostar then becomes a star and joins the main sequence on the HR diagram.
Unresolved binary stars, which appear photometrically to be points,have been identified by studying color-color outliers in cases where one member is off the main sequence.