Q89220427
long period variable
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Q89220427
Summary
Q89220427 is a long-period variable star[1].
Key Facts
- Q89220427's instance of is recorded as long-period variable star[2].
- Q89220427's constellation is recorded as Camelopardalis[3].
- Q89220427's catalog code is recorded as 2MASS J04344197+5542316[4].
- Q89220427's catalog code is recorded as GSC 03736-00376[5].
- Q89220427's catalog code is recorded as Gaia DR2 277188496271213056[6].
- Q89220427's catalog code is recorded as V363 Cam[7].
- Q89220427's type of variable star is recorded as semiregular variable star[8].
- Q89220427's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.0'}[9].
- Q89220427's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.626'}[10].
- Q89220427's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.615'}[11].
- Q89220427's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.295'}[12].
- Q89220427's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.0542'}[13].
- Q89220427's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.8359'}[14].
- Q89220427's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-11.48'}[15].
- Q89220427's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1196.3153'}[16].
- Q89220427's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+68.67487957023230'}[17].
- Q89220427's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+55.70881607434650'}[18].
- Q89220427's epoch is recorded as J2000.0[19].
- Q89220427's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.181'}[20].
- Q89220427's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+8.427'}[21].
Body
Definition and Type
Q89220427's instance of is recorded as long-period variable star[2].