Q78484187
red giant branch star in the constellation Aquila
Press Enter · cited answer in seconds
0 sources
Q78484187
Summary
Q78484187 is a red giant branch star[1].
Key Facts
- Q78484187's instance of is recorded as red giant branch star[2].
- Q78484187's constellation is recorded as Aquila[3].
- Q78484187's catalog code is recorded as 2MASS J19142330-0530063[4].
- Q78484187's catalog code is recorded as Gaia DR2 4212032203385238528[5].
- Q78484187's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.720'}[6].
- Q78484187's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.900'}[7].
- Q78484187's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.708'}[8].
- Q78484187's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.1085'}[9].
- Q78484187's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3095'}[10].
- Q78484187's metallicity is recorded as {'unit': '1', 'amount': '-0.141'}[11].
- Q78484187's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3231.0178'}[12].
- Q78484187's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+288.59710740223340'}[13].
- Q78484187's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-5.50173959210270'}[14].
- Q78484187's epoch is recorded as J2000.0[15].
- Q78484187's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4270'}[16].
- Q78484187's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+47'}[17].
- Q78484187's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.592'}[18].
- Q78484187's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.176'}[19].
Body
Definition and Type
Q78484187's instance of is recorded as red giant branch star[2].