Q87071456
classical Cepheid variable star in the constellation Cassiopeia
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Q87071456
Summary
Q87071456 is a classical Cepheid variable[1].
Key Facts
- Q87071456's instance of is recorded as classical Cepheid variable[2].
- Q87071456's instance of is recorded as double star[3].
- Q87071456's instance of is recorded as near-infrared source[4].
- Q87071456's instance of is recorded as variable star[5].
- Q87071456's constellation is recorded as Cassiopeia[6].
- Q87071456's spectral class is recorded as F8[7].
- Q87071456's catalog code is recorded as 2MASS J02444330+6127528[8].
- Q87071456's catalog code is recorded as GSC 04047-00461[9].
- Q87071456's catalog code is recorded as HIC 12817[10].
- Q87071456's catalog code is recorded as HIP 12817[11].
- Q87071456's catalog code is recorded as Gaia DR1 465719178109147136[12].
- Q87071456's catalog code is recorded as Gaia DR2 465719182408723072[13].
- Q87071456's catalog code is recorded as DF Cas[14].
- Q87071456's catalog code is recorded as TYC 4047-461-1[15].
- Q87071456's catalog code is recorded as WDS J02447+6128A[16].
- Q87071456's catalog code is recorded as TIC 50608476[17].
- Q87071456's catalog code is recorded as Gaia DR3 465719182408723072[18].
- Q87071456's type of variable star is recorded as classical Cepheid variable[19].
- Q87071456's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.80'}[20].
- Q87071456's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.525'}[21].
- Q87071456's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.114'}[22].
- Q87071456's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.959'}[23].
- Q87071456's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.74'}[24].
- Q87071456's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.471635'}[25].
- Q87071456's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3445'}[26].
Body
Definition and Type
Recorded instance of include classical Cepheid variable[2], double star[3], near-infrared source[4], and variable star[5].