Q85178853
long period variable
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Q85178853
Summary
Q85178853 is a long-period variable star[1].
Key Facts
- Q85178853's instance of is recorded as long-period variable star[2].
- Q85178853's constellation is recorded as Cygnus[3].
- Q85178853's catalog code is recorded as CSV 5159[4].
- Q85178853's catalog code is recorded as GSC 03937-00655[5].
- Q85178853's catalog code is recorded as SV* SON 3829[6].
- Q85178853's catalog code is recorded as 2MASS J20233139+5411132[7].
- Q85178853's catalog code is recorded as Gaia DR2 2185037781189821568[8].
- Q85178853's catalog code is recorded as V772 Cyg[9].
- Q85178853's type of variable star is recorded as slow irregular variable[10].
- Q85178853's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.399'}[11].
- Q85178853's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.873'}[12].
- Q85178853's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.773'}[13].
- Q85178853's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8776'}[14].
- Q85178853's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.3654'}[15].
- Q85178853's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+15.85'}[16].
- Q85178853's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+229.0741'}[17].
- Q85178853's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+305.88081774601950'}[18].
- Q85178853's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+54.18698491946620'}[19].
- Q85178853's epoch is recorded as J2000.0[20].
- Q85178853's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.757'}[21].
- Q85178853's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.410'}[22].
Body
Definition and Type
Q85178853's instance of is recorded as long-period variable star[2].