Q78483709
red giant branch star in the constellation Lynx
Press Enter · cited answer in seconds
0 sources
Q78483709
Summary
Q78483709 is a red giant branch star[1].
Key Facts
- Q78483709's instance of is recorded as red giant branch star[2].
- Q78483709's constellation is recorded as Lynx[3].
- Q78483709's catalog code is recorded as 2MASS J07380316+3748330[4].
- Q78483709's catalog code is recorded as Gaia DR2 896073320615653120[5].
- Q78483709's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.339'}[6].
- Q78483709's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.878'}[7].
- Q78483709's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.779'}[8].
- Q78483709's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.7893'}[9].
- Q78483709's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4765'}[10].
- Q78483709's metallicity is recorded as {'unit': '1', 'amount': '-0.282'}[11].
- Q78483709's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2098.6359'}[12].
- Q78483709's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+114.51317277190610'}[13].
- Q78483709's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+37.80919175285180'}[14].
- Q78483709's epoch is recorded as J2000.0[15].
- Q78483709's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4953'}[16].
- Q78483709's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+1288'}[17].
- Q78483709's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.266'}[18].
- Q78483709's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.019'}[19].
Body
Definition and Type
Q78483709's instance of is recorded as red giant branch star[2].