Q78474259
red giant branch star in the constellation Monoceros
Press Enter · cited answer in seconds
0 sources
Q78474259
Summary
Q78474259 is a red giant branch star[1].
Key Facts
- Q78474259's instance of is recorded as red giant branch star[2].
- Q78474259's constellation is recorded as Monoceros[3].
- Q78474259's catalog code is recorded as 2MASS J06512952+0220047[4].
- Q78474259's catalog code is recorded as Gaia DR2 3126290859219425024[5].
- Q78474259's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.217'}[6].
- Q78474259's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.366'}[7].
- Q78474259's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.120'}[8].
- Q78474259's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.7893'}[9].
- Q78474259's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2473'}[10].
- Q78474259's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+74.77'}[11].
- Q78474259's metallicity is recorded as {'unit': '1', 'amount': '-0.139'}[12].
- Q78474259's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+102.87302931203470'}[13].
- Q78474259's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+2.33464240363590'}[14].
- Q78474259's epoch is recorded as J2000.0[15].
- Q78474259's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4302'}[16].
- Q78474259's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+44'}[17].
- Q78474259's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.655'}[18].
- Q78474259's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.245'}[19].
Body
Definition and Type
Q78474259's instance of is recorded as red giant branch star[2].