Q85608735
classical Cepheid variable star in the constellation Cetus
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Q85608735
Summary
Q85608735 is a classical Cepheid variable[1].
Key Facts
- Q85608735's instance of is recorded as classical Cepheid variable[2].
- Q85608735's instance of is recorded as near-infrared source[3].
- Q85608735's instance of is recorded as variable star[4].
- Q85608735's instance of is recorded as astrophysical X-ray source[5].
- Q85608735's constellation is recorded as Cetus[6].
- Q85608735's catalog code is recorded as GSC 00019-00392[7].
- Q85608735's catalog code is recorded as ASAS J010516+0159.2[8].
- Q85608735's catalog code is recorded as UCAC3 184-3071[9].
- Q85608735's catalog code is recorded as 2MASS J01051593+0159141[10].
- Q85608735's catalog code is recorded as Gaia DR1 2539054201469245568[11].
- Q85608735's catalog code is recorded as Gaia DR2 2539054201469245568[12].
- Q85608735's catalog code is recorded as GT Cet[13].
- Q85608735's catalog code is recorded as TYC 19-392-1[14].
- Q85608735's catalog code is recorded as EPIC 220269465[15].
- Q85608735's catalog code is recorded as TIC 344754529[16].
- Q85608735's catalog code is recorded as Gaia DR3 2539054201469245568[17].
- Q85608735's type of variable star is recorded as classical Cepheid variable[18].
- Q85608735's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.70'}[19].
- Q85608735's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.11'}[20].
- Q85608735's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.777'}[21].
- Q85608735's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.127'}[22].
- Q85608735's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.995'}[23].
- Q85608735's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.35'}[24].
- Q85608735's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.417065'}[25].
- Q85608735's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6471'}[26].
Body
Definition and Type
Recorded instance of include classical Cepheid variable[2], near-infrared source[3], variable star[4], and astrophysical X-ray source[5].