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Rho Cassiopeiae

Index Rho Cassiopeiae

Rho Cassiopeiae (ρ Cas, ρ Cassiopeiae) is a yellow hypergiant star in the constellation Cassiopeia. [1]

32 relations: Alpha Lacertae, Beta Lacertae, Cassiopeia (constellation), Cassiopeia in Chinese astronomy, Epsilon Cephei, HR 5171, Hypergiant, Iota Andromedae, Kappa Andromedae, Lambda Andromedae, List of brightest stars and other record stars, List of largest stars, List of most luminous stars, List of semiregular variable stars, List of stars in Cassiopeia, List of supernova candidates, Luminous blue variable, Phi Cassiopeiae, Pi1 Cygni, Pi2 Cygni, Psi Andromedae, Semiregular variable star, Sigma Cassiopeiae, Supergiant star, Supernova, Table of stars with Bayer designations, Table of stars with Flamsteed designations, Tau Cassiopeiae, V382 Carinae, V509 Cassiopeiae, Variable star, Yellow hypergiant.

Alpha Lacertae

Alpha Lacertae (Alpha Lac, α Lacertae, α Lac) is an A-type main sequence star in the constellation of Lacerta.

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Beta Lacertae

Beta Lacertae (Beta Lac, β Lacertae, β Lac) is the fourth-brightest star in the constellation of Lacerta.

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Cassiopeia (constellation)

Cassiopeia is a constellation in the northern sky, named after the vain queen Cassiopeia in Greek mythology, who boasted about her unrivalled beauty.

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Cassiopeia in Chinese astronomy

The modern constellation Cassiopeia lies across two of the quadrants symbolized by the Black Tortoise of the North (北方玄武, Běi Fāng Xuán Wǔ), The White Tiger of the West (西方白虎, Xī Fāng Bái Hǔ) and Three Enclosures (三垣, Sān Yuán), that divide the sky in traditional Chinese uranography.

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Epsilon Cephei

Epsilon Cephei, Latinized from ε Cephei, is a star in the northern constellation of Cepheus.

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HR 5171

HR 5171, also known as V766 Centauri, is a triple star system in the constellation Centaurus, around 12,000 light years from Earth.

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Hypergiant

A hypergiant (luminosity class 0 or Ia+) is among the very rare kinds of stars that typically show tremendous luminosities and very high rates of mass loss by stellar winds.

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Iota Andromedae

Iota Andromedae (ι And, ι Andromedae) is a star in the constellation Andromeda.

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Kappa Andromedae

Kappa Andromedae (κ And, κ Andromedae) is the Bayer designation for a bright star in the constellation of Andromeda.

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Lambda Andromedae

Lambda Andromedae (λ And, λ Andromedae) is the Bayer designation for a binary star in the northern constellation of Andromeda.

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List of brightest stars and other record stars

This is a list of the brightest stars together with record holders of other categories with many details in compact form that can be compared.

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List of largest stars

Below is an ordered list of the largest stars currently known by radius.

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List of most luminous stars

Below is a list of stars arranged in order of decreasing luminosity (increasing bolometric magnitude).

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List of semiregular variable stars

This is a list of semiregular variable stars.

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List of stars in Cassiopeia

This is the list of notable stars in the constellation Cassiopeia, sorted by decreasing brightness.

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List of supernova candidates

This is a list of supernova candidates, or stars that astronomers have suggested are supernova progenitors.

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Luminous blue variable

Luminous blue variables (LBVs) are massive evolved stars that show unpredictable and sometimes dramatic variations in both their spectra and brightness.

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Phi Cassiopeiae

Phi Cassiopeiae (φ Cas, φ Cassiopeiae) is a star in the constellation Cassiopeia.

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Pi1 Cygni

Pi¹ Cygni (π¹ Cygni, abbreviated Pi¹ Cyg, π¹ Cyg) is a binary star in the northern constellation of Cygnus.

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Pi2 Cygni

Pi2 Cygni, Latinized from π2 Cygni, is a triple star system in the northern constellation of Cygnus.

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Psi Andromedae

Psi Andromedae (ψ And, ψ Andromedae) is the Bayer designation for a triple star system in the northern constellation of Andromeda.

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Semiregular variable star

Semiregular variable stars are giants or supergiants of intermediate and late spectral type showing considerable periodicity in their light changes, accompanied or sometimes interrupted by various irregularities.

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Sigma Cassiopeiae

Sigma Cassiopeiae (σ Cas, σ Cassiopeiae) is a binary star in the constellation Cassiopeia.

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Supergiant star

Supergiants are among the most massive and most luminous stars.

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Supernova

A supernova (plural: supernovae or supernovas, abbreviations: SN and SNe) is a transient astronomical event that occurs during the last stellar evolutionary stages of a star's life, either a massive star or a white dwarf, whose destruction is marked by one final, titanic explosion.

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Table of stars with Bayer designations

This table lists those stars or other objects which have Bayer designations by the constellation in which those stars or objects lie.

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Table of stars with Flamsteed designations

This table lists those stars/objects which have Flamsteed designations by the constellation in which those stars/objects lie.

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Tau Cassiopeiae

Tau Cassiopeiae (τ Cassiopeiae) is a solitary, orange hued star in the northern constellation of Cassiopeia.

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V382 Carinae

V382 Carinae, also known as x Carinae (x Car), is a yellow hypergiant in the constellation Carina.

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V509 Cassiopeiae

V509 Cassiopeiae (V509 Cas or HR 8752) is one of two yellow hypergiant stars found in the constellation Cassiopeia, which also contains Rho Cassiopeiae.

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Variable star

A variable star is a star whose brightness as seen from Earth (its apparent magnitude) fluctuates.

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Yellow hypergiant

A yellow hypergiant is a massive star with an extended atmosphere, a spectral class from A to K, and an initial mass of about 20–60 solar masses but having lost as much as half that mass.

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Redirects here:

7 Cas, 7 Cassiopeiae, HD 224014, Rho Cas, Ρ Cassiopeiae.

References

[1] https://en.wikipedia.org/wiki/Rho_Cassiopeiae

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