Q79768476
red giant branch star in the constellation Lynx
Press Enter · cited answer in seconds
0 sources
Q79768476
Summary
Q79768476 is a red giant branch star[1].
Key Facts
- Q79768476's instance of is recorded as red giant branch star[2].
- Q79768476's constellation is recorded as Lynx[3].
- Q79768476's catalog code is recorded as 2MASS J07514200+5332178[4].
- Q79768476's catalog code is recorded as Gaia DR2 984690079459711872[5].
- Q79768476's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.184'}[6].
- Q79768476's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.723'}[7].
- Q79768476's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.629'}[8].
- Q79768476's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.6196'}[9].
- Q79768476's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3422'}[10].
- Q79768476's metallicity is recorded as {'unit': '1', 'amount': '-0.335'}[11].
- Q79768476's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2922.2677'}[12].
- Q79768476's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+117.92500926187170'}[13].
- Q79768476's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+53.53827459146150'}[14].
- Q79768476's epoch is recorded as J2000.0[15].
- Q79768476's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4976'}[16].
- Q79768476's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+1950'}[17].
- Q79768476's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.633'}[18].
- Q79768476's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.278'}[19].
Body
Definition and Type
Q79768476's instance of is recorded as red giant branch star[2].