Q92294748
long period variable
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Q92294748
Summary
Q92294748 is a long-period variable star[1].
Key Facts
- Q92294748's instance of is recorded as long-period variable star[2].
- Q92294748's constellation is recorded as Cepheus[3].
- Q92294748's spectral class is recorded as K4[4].
- Q92294748's catalog code is recorded as WISE J002515.23+735411.4[5].
- Q92294748's catalog code is recorded as AAVSO 0019+73[6].
- Q92294748's catalog code is recorded as CSI+73-00222[7].
- Q92294748's catalog code is recorded as GCRV 225[8].
- Q92294748's catalog code is recorded as IRAS 00222+7337[9].
- Q92294748's catalog code is recorded as SV* HV 3549[10].
- Q92294748's catalog code is recorded as 2MASS J00251524+7354113[11].
- Q92294748's catalog code is recorded as TYC 4307-1248-1[12].
- Q92294748's catalog code is recorded as Gaia DR1 537816869958285056[13].
- Q92294748's catalog code is recorded as WEB 378[14].
- Q92294748's catalog code is recorded as [WWV2004] J0025154+735410[15].
- Q92294748's catalog code is recorded as Gaia DR2 537816874256537216[16].
- Q92294748's catalog code is recorded as TZ Cep[17].
- Q92294748's type of variable star is recorded as SRd semi-regular variable star[18].
- Q92294748's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.58'}[19].
- Q92294748's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.030'}[20].
- Q92294748's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.247'}[21].
- Q92294748's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.916'}[22].
- Q92294748's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.38'}[23].
- Q92294748's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.7939'}[24].
- Q92294748's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.8833'}[25].
- Q92294748's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-7.42'}[26].
Body
Definition and Type
Q92294748's instance of is recorded as long-period variable star[2].