Q84250782
red giant branch star in the constellation Cassiopeia
Press Enter · cited answer in seconds
0 sources
Q84250782
Summary
Q84250782 is a red giant branch star[1].
Key Facts
- Q84250782's instance of is recorded as red giant branch star[2].
- Q84250782's constellation is recorded as Cassiopeia[3].
- Q84250782's catalog code is recorded as 2MASS J00301072+5341479[4].
- Q84250782's catalog code is recorded as Gaia DR2 416543456137138432[5].
- Q84250782's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.740'}[6].
- Q84250782's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.011'}[7].
- Q84250782's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.845'}[8].
- Q84250782's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8201'}[9].
- Q84250782's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2511'}[10].
- Q84250782's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-27.29'}[11].
- Q84250782's metallicity is recorded as {'unit': '1', 'amount': '-0.506'}[12].
- Q84250782's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+7.54470095136120'}[13].
- Q84250782's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+53.69662595806630'}[14].
- Q84250782's epoch is recorded as J2000.0[15].
- Q84250782's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4331'}[16].
- Q84250782's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+49'}[17].
- Q84250782's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.413'}[18].
- Q84250782's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.470'}[19].
Body
Definition and Type
Q84250782's instance of is recorded as red giant branch star[2].