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SuperStar

[jù xīng]
term in astronomy
open 9 entries with the same name
Giant stars are a form of stars in the process of evolution fixed star When old, its size and brightness will become very large, which will form a giant star. [1]
Chinese name
SuperStar
Features
Large luminosity, large volume and small density
Properties
fixed star
Other definitions
Is compared to a great man with outstanding achievements in some aspects

Basic characteristics

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Giant stars are very large in size, but their mass is only a few to dozens of times that of the sun, and they are much brighter than the sun. Interestingly, although the giant star is very bright, its surface temperature is still similar to that of ordinary stars. [1]

classification

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stay Herotu On Main star order Above and below the supergiant branch. Photometric level It belongs to Grade II - Ⅲ. The surface temperature is 2500k~7000k. A few blue giants have higher temperatures, while Cold giant The lowest temperature is only 1000K. ordinary Red Giant Its mass is 1.5~4 times that of the sun, and its radius is about 10 times that of the sun, which is a relatively late stage in the evolution of stars. In the Ming Dynasty of China, the saying of superstar has been widely used《 Public Biography of Jie Huan and Yuan 》:“( Yuan Keli Death The night before last, a giant star fell to the southwest with sound. "
Stars with luminosity level II are called Bright superstar Bright stars Herotu Distribution area on is between Supergiant And superstars. For a certain surface Effective temperature For bright giant stars, their luminosity is stronger than that of giant stars and weaker than that of supergiant stars. The famous bright stars are Orion δ、 Gradual Stage II The bright star of scorpio 19、 leo ε、 Auriga Southern cross γ, etc.
Comparison between planets in the solar system and other stars

Superstars list

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Superstars list
name
(Sun=1)
2150-2158
1260-1738
one thousand and five hundred
one thousand four hundred and twenty
1600-1900
1570±400
one thousand six hundred and fifty
one thousand five hundred and forty
one thousand five hundred and twenty
one thousand four hundred and twenty
one thousand four hundred and sixty
1260-1610
one thousand one hundred and eighty
832-1200
eight hundred
seven hundred and fifty-five
seven hundred and forty-seven
Rho Cassiopeiae (Cassiopeia ρ)
seven hundred and thirty-eight
Pegasus S
five hundred and eighty
five hundred and fifty
Cepheus T
five hundred and forty
five hundred and thirty
Serpentine W
five hundred and twenty
Auriga Y1
five hundred and eleven
five hundred and ten
Cassiopeia R
five hundred
Wezen (Canis Major δ/Bezen)
four hundred and eighty-two
four hundred and seventy
Cassiopeia J
four hundred and sixty
Throne (Hercules alpha/Ras Algethi)
four hundred and sixty
four hundred
Haishan II ( Bottom seat η )
four hundred
400-910
three hundred and seventy
Hull base HR
three hundred and fifty
three hundred and fifty
Pistol Star (Pistol Star)
three hundred and forty
Beagle Y (La Superba)
three hundred
Tianjin IV (Cygnus alpha)
two hundred and twenty
two hundred
Column I ( Epsilon Aurigae )
one hundred and seventy-five
Zeta Auriga
one hundred and sixty
Endangered Sleeping Three (Pegasus ε/Enif)
one hundred and fifty
Southern cross γ (Gacrux)
one hundred and thirteen
one hundred and nine
one hundred
Andromeda gamma
eighty-three
seventy-seven
seventy
Bottom seat ε
seventy
R variable star of northern corona
sixty-five
sixty-five
sixty
Orion δ (Mintaka)
sixty
Zeta Orion ( Alnitak )
sixty
Tianchuan Three (Perseus alpha/Mirfak)
sixty
Gemini ζ (Mekbuda)
sixty
Eagle η
sixty
Eltanin (Draco γ/Eltanin)
fifty
forty-three
emperor Arctic II (Little Bear β/Kochab)
forty-one