Q79810667
red giant branch star in the constellation Ophiuchus
Press Enter · cited answer in seconds
0 sources
Q79810667
Summary
Q79810667 is a red giant branch star[1].
Key Facts
- Q79810667's instance of is recorded as red giant branch star[2].
- Q79810667's constellation is recorded as Ophiuchus[3].
- Q79810667's catalog code is recorded as 2MASS J17163442-2511179[4].
- Q79810667's catalog code is recorded as Gaia DR2 4109456457213091072[5].
- Q79810667's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.753'}[6].
- Q79810667's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.776'}[7].
- Q79810667's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.418'}[8].
- Q79810667's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.0001'}[9].
- Q79810667's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3372'}[10].
- Q79810667's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-17.57'}[11].
- Q79810667's metallicity is recorded as {'unit': '1', 'amount': '+0.105'}[12].
- Q79810667's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+259.14344013547010'}[13].
- Q79810667's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-25.18831634026410'}[14].
- Q79810667's epoch is recorded as J2000.0[15].
- Q79810667's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4135'}[16].
- Q79810667's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+44'}[17].
- Q79810667's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.221'}[18].
- Q79810667's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.349'}[19].
Body
Definition and Type
Q79810667's instance of is recorded as red giant branch star[2].