Q78758029
red giant branch star in the constellation Monoceros
Press Enter · cited answer in seconds
0 sources
Q78758029
Summary
Q78758029 is a red giant branch star[1].
Key Facts
- Q78758029's instance of is recorded as red giant branch star[2].
- Q78758029's constellation is recorded as Monoceros[3].
- Q78758029's catalog code is recorded as 2MASS J06412213+1106042[4].
- Q78758029's catalog code is recorded as Gaia DR2 3351087828286351872[5].
- Q78758029's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.832'}[6].
- Q78758029's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.76'}[7].
- Q78758029's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.292'}[8].
- Q78758029's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.6025'}[9].
- Q78758029's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0974'}[10].
- Q78758029's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+41.59'}[11].
- Q78758029's metallicity is recorded as {'unit': '1', 'amount': '-0.036'}[12].
- Q78758029's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+100.34222108973280'}[13].
- Q78758029's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+11.10116888253680'}[14].
- Q78758029's epoch is recorded as J2000.0[15].
- Q78758029's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4634'}[16].
- Q78758029's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+219'}[17].
- Q78758029's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.266'}[18].
- Q78758029's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.171'}[19].
Body
Definition and Type
Q78758029's instance of is recorded as red giant branch star[2].