Q89878217
Mira variable star in the constellation Lacerta
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Q89878217
Summary
Q89878217 is a Mira variable[1].
Key Facts
- Q89878217's instance of is recorded as Mira variable[2].
- Q89878217's constellation is recorded as Lacerta[3].
- Q89878217's spectral class is recorded as M9[4].
- Q89878217's catalog code is recorded as SV* SON 10094[5].
- Q89878217's catalog code is recorded as SV* VV 424[6].
- Q89878217's catalog code is recorded as IRAS 22394+5623[7].
- Q89878217's catalog code is recorded as AKARI-IRC-V1 J2241272+563908[8].
- Q89878217's catalog code is recorded as UCAC4 734-088857[9].
- Q89878217's catalog code is recorded as 2MASS J22412724+5639091[10].
- Q89878217's catalog code is recorded as WISE J224127.27+563909.0[11].
- Q89878217's catalog code is recorded as [WWV2004] J2241276+563909[12].
- Q89878217's catalog code is recorded as Gaia DR2 2007008088242999424[13].
- Q89878217's catalog code is recorded as GV Lac[14].
- Q89878217's type of variable star is recorded as Mira variable[15].
- Q89878217's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.25'}[16].
- Q89878217's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.21'}[17].
- Q89878217's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.30'}[18].
- Q89878217's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.80'}[19].
- Q89878217's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.8900'}[20].
- Q89878217's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4339'}[21].
- Q89878217's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-38'}[22].
- Q89878217's SIMBAD ID is recorded as V* GV Lac[23].
- Q89878217's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+340.36354037554270'}[24].
- Q89878217's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+56.65254117437180'}[25].
- Q89878217's epoch is recorded as J2000.0[26].