Q85701687
long period variable
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Q85701687
Summary
Q85701687 is a long-period variable star[1].
Key Facts
- Q85701687's instance of is recorded as long-period variable star[2].
- Q85701687's instance of is recorded as near-infrared source[3].
- Q85701687's constellation is recorded as Cygnus[4].
- Q85701687's spectral class is recorded as C:[5].
- Q85701687's catalog code is recorded as GSC 02711-00059[6].
- Q85701687's catalog code is recorded as 2MASS J21193994+3500111[7].
- Q85701687's catalog code is recorded as Gaia DR2 1867446046528158080[8].
- Q85701687's catalog code is recorded as V2337 Cyg[9].
- Q85701687's catalog code is recorded as TIC 117394956[10].
- Q85701687's catalog code is recorded as Gaia DR3 1867446046528158080[11].
- Q85701687's type of variable star is recorded as long-period variable star[12].
- Q85701687's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.521'}[13].
- Q85701687's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.556'}[14].
- Q85701687's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.181'}[15].
- Q85701687's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.595643'}[16].
- Q85701687's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2836'}[17].
- Q85701687's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-29.67'}[18].
- Q85701687's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+319.9164175239'}[19].
- Q85701687's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+35.00308010616'}[20].
- Q85701687's epoch is recorded as J2000.0[21].
- Q85701687's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.924'}[22].
- Q85701687's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.477'}[23].
Body
Definition and Type
Recorded instance of include long-period variable star[2] and near-infrared source[3].