Q75130631
classical Cepheid variable star in the constellation Centaurus
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Q75130631
Summary
Q75130631 is a classical Cepheid variable[1].
Key Facts
- Q75130631's instance of is recorded as classical Cepheid variable[2].
- Q75130631's instance of is recorded as near-infrared source[3].
- Q75130631's instance of is recorded as variable star[4].
- Q75130631's constellation is recorded as Centaurus[5].
- Q75130631's spectral class is recorded as G8Iab+B6.0V[6].
- Q75130631's catalog code is recorded as GSC 08999-02332[7].
- Q75130631's catalog code is recorded as HIC 66383[8].
- Q75130631's catalog code is recorded as HIP 66383[9].
- Q75130631's catalog code is recorded as KN Cen[10].
- Q75130631's catalog code is recorded as 2MASS J13363690-6433298[11].
- Q75130631's catalog code is recorded as WDS J13366-6433AB[12].
- Q75130631's catalog code is recorded as Gaia DR1 5864135315581474176[13].
- Q75130631's catalog code is recorded as Gaia DR2 5864135319959353600[14].
- Q75130631's catalog code is recorded as TYC 8999-2332-1[15].
- Q75130631's catalog code is recorded as TIC 317502464[16].
- Q75130631's catalog code is recorded as Gaia DR3 5864135319959353600[17].
- Q75130631's type of variable star is recorded as classical Cepheid variable[18].
- Q75130631's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.300'}[19].
- Q75130631's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.645'}[20].
- Q75130631's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.364'}[21].
- Q75130631's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.86'}[22].
- Q75130631's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.22'}[23].
- Q75130631's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.240802'}[24].
- Q75130631's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2272'}[25].
- Q75130631's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-37.81'}[26].
Body
Definition and Type
Recorded instance of include classical Cepheid variable[2], near-infrared source[3], and variable star[4].