Q84249409
red giant branch star in the constellation Lyra
Press Enter · cited answer in seconds
0 sources
Q84249409
Summary
Q84249409 is a red giant branch star[1].
Key Facts
- Q84249409's instance of is recorded as red giant branch star[2].
- Q84249409's constellation is recorded as Lyra[3].
- Q84249409's catalog code is recorded as 2MASS J19220455+4303342[4].
- Q84249409's catalog code is recorded as Gaia DR2 2102046506083763968[5].
- Q84249409's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.016'}[6].
- Q84249409's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.362'}[7].
- Q84249409's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.204'}[8].
- Q84249409's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.9697'}[9].
- Q84249409's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2533'}[10].
- Q84249409's metallicity is recorded as {'unit': '1', 'amount': '+0.263'}[11].
- Q84249409's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3947.8879'}[12].
- Q84249409's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+290.51898442767840'}[13].
- Q84249409's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+43.05949780063570'}[14].
- Q84249409's epoch is recorded as J2000.0[15].
- Q84249409's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4400'}[16].
- Q84249409's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+257'}[17].
- Q84249409's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-6.718'}[18].
- Q84249409's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.328'}[19].
Body
Definition and Type
Q84249409's instance of is recorded as red giant branch star[2].