Q93438628
classical Cepheid variable star in the constellation Vela
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Q93438628
Summary
Q93438628 is a classical Cepheid variable[1].
Key Facts
- Q93438628's instance of is recorded as classical Cepheid variable[2].
- Q93438628's instance of is recorded as near-infrared source[3].
- Q93438628's instance of is recorded as variable star[4].
- Q93438628's constellation is recorded as Vela[5].
- Q93438628's catalog code is recorded as GSC 08585-00148[6].
- Q93438628's catalog code is recorded as HIC 47177[7].
- Q93438628's catalog code is recorded as HIP 47177[8].
- Q93438628's catalog code is recorded as 2MASS J09365148-5301581[9].
- Q93438628's catalog code is recorded as Gaia DR1 5309174963404492160[10].
- Q93438628's catalog code is recorded as Gaia DR2 5309174967720762496[11].
- Q93438628's catalog code is recorded as AE Vel[12].
- Q93438628's catalog code is recorded as TYC 8585-148-1[13].
- Q93438628's catalog code is recorded as UBV M 6555[14].
- Q93438628's catalog code is recorded as TIC 280287051[15].
- Q93438628's catalog code is recorded as Gaia DR3 5309174967720762496[16].
- Q93438628's type of variable star is recorded as classical Cepheid variable[17].
- Q93438628's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.4'}[18].
- Q93438628's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.5'}[19].
- Q93438628's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.734'}[20].
- Q93438628's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.512'}[21].
- Q93438628's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.103'}[22].
- Q93438628's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.887'}[23].
- Q93438628's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.832482'}[24].
- Q93438628's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3531'}[25].
- Q93438628's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+14.33'}[26].
Body
Definition and Type
Recorded instance of include classical Cepheid variable[2], near-infrared source[3], and variable star[4].