Q84043464
long period variable
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Q84043464
Summary
Q84043464 is a long-period variable star[1].
Key Facts
- Q84043464's instance of is recorded as long-period variable star[2].
- Q84043464's constellation is recorded as Cygnus[3].
- Q84043464's spectral class is recorded as M6.5[4].
- Q84043464's catalog code is recorded as AN 182.1928[5].
- Q84043464's catalog code is recorded as GSC 02655-00668[6].
- Q84043464's catalog code is recorded as IRAS 19319+3001[7].
- Q84043464's catalog code is recorded as IRC +30372[8].
- Q84043464's catalog code is recorded as 2MASS J19335432+3008256[9].
- Q84043464's catalog code is recorded as Gaia DR2 2032597194181737984[10].
- Q84043464's catalog code is recorded as EF Cyg[11].
- Q84043464's type of variable star is recorded as SRb semi-regular variable star[12].
- Q84043464's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.740'}[13].
- Q84043464's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.641'}[14].
- Q84043464's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.161'}[15].
- Q84043464's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.0428'}[16].
- Q84043464's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.1025'}[17].
- Q84043464's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+907.0295'}[18].
- Q84043464's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+293.47632570859010'}[19].
- Q84043464's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+30.14044542772990'}[20].
- Q84043464's epoch is recorded as J2000.0[21].
- Q84043464's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.415'}[22].
- Q84043464's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.830'}[23].
Body
Definition and Type
Q84043464's instance of is recorded as long-period variable star[2].