Q79764003
red giant branch star in the constellation Lacerta
Press Enter · cited answer in seconds
0 sources
Q79764003
Summary
Q79764003 is a red giant branch star[1].
Key Facts
- Q79764003's instance of is recorded as red giant branch star[2].
- Q79764003's constellation is recorded as Lacerta[3].
- Q79764003's catalog code is recorded as 2MASS J22041479+5059198[4].
- Q79764003's catalog code is recorded as Gaia DR2 1980061497787498496[5].
- Q79764003's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.951'}[6].
- Q79764003's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.130'}[7].
- Q79764003's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.887'}[8].
- Q79764003's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.5341'}[9].
- Q79764003's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0986'}[10].
- Q79764003's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-150.90'}[11].
- Q79764003's metallicity is recorded as {'unit': '1', 'amount': '-0.269'}[12].
- Q79764003's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+331.06167619731240'}[13].
- Q79764003's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+50.98885533769680'}[14].
- Q79764003's epoch is recorded as J2000.0[15].
- Q79764003's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4292'}[16].
- Q79764003's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+32'}[17].
- Q79764003's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.765'}[18].
- Q79764003's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.465'}[19].
Body
Definition and Type
Q79764003's instance of is recorded as red giant branch star[2].