Q78480837
red giant branch star in the constellation Lyra
Press Enter · cited answer in seconds
0 sources
Q78480837
Summary
Q78480837 is a red giant branch star[1].
Key Facts
- Q78480837's instance of is recorded as red giant branch star[2].
- Q78480837's constellation is recorded as Lyra[3].
- Q78480837's catalog code is recorded as 2MASS J19114754+2904083[4].
- Q78480837's catalog code is recorded as Gaia DR2 2039076032058636800[5].
- Q78480837's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.464'}[6].
- Q78480837's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.892'}[7].
- Q78480837's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.748'}[8].
- Q78480837's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.2347'}[9].
- Q78480837's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2693'}[10].
- Q78480837's metallicity is recorded as {'unit': '1', 'amount': '-0.313'}[11].
- Q78480837's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3713.3309'}[12].
- Q78480837's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+287.94811387620130'}[13].
- Q78480837's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+29.06898674437200'}[14].
- Q78480837's epoch is recorded as J2000.0[15].
- Q78480837's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4695'}[16].
- Q78480837's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+490'}[17].
- Q78480837's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.719'}[18].
- Q78480837's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.621'}[19].
Body
Definition and Type
Q78480837's instance of is recorded as red giant branch star[2].