Examples of using Main sequence in English and their translations into Swedish
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Most of the stars are main sequence binaries.
The table below shows typical values for stars along the main sequence.
HD 12661 is a G-type main sequence star in the northern constellation of Aries.
Stars within the portion of the instability strip that crosses the main sequence are called Delta Scuti variables.
Most stars belong to the main sequence, which consists of ordinary hydrogen-burning stars.
People also translate
In about four billion years from now, component A will evolve off the main sequence into a giant.
V Cephei is a white main sequence star in the constellation Cepheus.
moving off the main sequence.
This is a hot, core hydrogen-fusing B-type main sequence star of spectral class B2 Vp.
This is a main sequence star of spectral type K7.5 Ve, having just 67% of the Sun's mass.
The Lantean Star in the Lantean system is a regular main sequence star with at least seven planets in its orbit.
The Sun is a main sequence G2V yellow dwarf of intermediate temperature
With the hydrogen supply exhausted at its core, the Sun leaves the main sequence and begins to evolve into a red giant.
This is an F-type main sequence star with a stellar classification of F5 V. It is chromospherically active.
It was noted that its color indices are incompatible with a main sequence object, but are consistent with a white dwarf.
This is an A-type main sequence star with a stellar classification of A5 V. Some sources list it as A8 V.
either a star that has not yet reached the main sequence or a small, low-temperature star.
As an O-class main sequence star, it would be 8 times the solar radius
in the spectral type, with classifications ranging from a main sequence star to a giant.
This indicates that the star has left the main sequence and has begun the final stages in its stellar evolution.
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.
Component Ab has a main sequence luminosity class,
although it is already in the main sequence stage of its evolution.
This is curious, because most main sequence stars with planets tend to have a higher abundance of metals.
although it is already in the main sequence stage of its evolution.
The secondary is likely to be a main sequence star slightly cooler than the primary,
To compensate for the temperature increase, the outer envelope expanded to many times the radius it possessed as a main sequence star.
This is an F-type main sequence star with a stellar classification of F5 V. It is younger than the Sun at an age of about 2.6 billion years.
can be on the main sequence, a degenerate dwarf(white dwarf),
This is an F-type main sequence star with a stellar classification of F5 V Fe-0.8,