Examples of using Main sequence in English and their translations into Portuguese
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Colloquial
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Official
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Medicine
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Financial
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Ecclesiastic
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Ecclesiastic
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Computer
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Official/political
Below approximately spectral type K3 the region between the main sequence and red giants is entirely empty, with no subgiants.
the period of stay in the main sequence of stars only about 100 million years.
Stars that begin with more than 50 can lose over half their total mass while on the main sequence.
will remain on the main sequence for about 10 billion years.
known as the main sequence.
More than 90,000 are G-type stars(similar to the Sun) on or near the main sequence.
More-massive stars already have cores above the Schönberg-Chandrasekhar mass when they leave the main sequence.
including main sequence and giants, using the spectroscope.
The system andromedae was the first multiplo system discovered whose the central body belong to the main sequence.
a halfway through their life on the main sequence.
These stars are chemically peculiar main sequence stars of spectral class B8p to A7p.
The Sun is a main sequence"G2V" yellow dwarf of intermediate temperature
Alpha Circini, a white main sequence star with an apparent magnitude of 3.19,
However, even perfect observation would show a fuzzy main sequence because mass is not the only parameter that affects a star's color and luminosity.
identifying it as a type of main sequence star known as a red dwarf.
The star reaches the main sequence when the core reaches a temperature high enough to begin fusing hydrogen(a few million kelvin)
a white main sequence star of apparent(visual) magnitude 3.3 around 97 light-years away from Earth.
Beta Pictoris is another white main sequence star of spectral type A6V and apparent magnitude 3.86.
In the lower main sequence, energy is primarily generated as the result of the proton-proton chain,
HD 102195 is an orange main sequence star about 94 light years away in the constellation of Virgo.