Q80431962
Mira variable star in the constellation Pegasus
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Q80431962
Summary
Q80431962 is a Mira variable[1].
Key Facts
- Q80431962's instance of is recorded as Mira variable[2].
- Q80431962's constellation is recorded as Pegasus[3].
- Q80431962's spectral class is recorded as M8/9[4].
- Q80431962's catalog code is recorded as FBS 2305+235[5].
- Q80431962's catalog code is recorded as FBS L 14-109[6].
- Q80431962's catalog code is recorded as IRAS 23051+2330[7].
- Q80431962's catalog code is recorded as 2MASS J23073630+2346565[8].
- Q80431962's catalog code is recorded as CRTS J230736.2+234656[9].
- Q80431962's catalog code is recorded as Gaia DR2 2842409498228308352[10].
- Q80431962's catalog code is recorded as MV Peg[11].
- Q80431962's type of variable star is recorded as long-period variable star[12].
- Q80431962's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.998'}[13].
- Q80431962's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.442'}[14].
- Q80431962's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.60'}[15].
- Q80431962's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.7424'}[16].
- Q80431962's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.7939'}[17].
- Q80431962's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-94'}[18].
- Q80431962's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+346.90127384836700'}[19].
- Q80431962's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+23.78240869422190'}[20].
- Q80431962's epoch is recorded as J2000.0[21].
- Q80431962's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.215'}[22].
- Q80431962's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+3.837'}[23].
Body
Definition and Type
Q80431962's instance of is recorded as Mira variable[2].