Q79772590
red giant branch star in the constellation Monoceros
Press Enter · cited answer in seconds
0 sources
Q79772590
Summary
Q79772590 is a red giant branch star[1].
Key Facts
- Q79772590's instance of is recorded as red giant branch star[2].
- Q79772590's constellation is recorded as Monoceros[3].
- Q79772590's catalog code is recorded as 2MASS J07195950-0514062[4].
- Q79772590's catalog code is recorded as Gaia DR2 3058432982983402496[5].
- Q79772590's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.494'}[6].
- Q79772590's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.772'}[7].
- Q79772590's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.555'}[8].
- Q79772590's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.7465'}[9].
- Q79772590's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2085'}[10].
- Q79772590's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+91.70'}[11].
- Q79772590's metallicity is recorded as {'unit': '1', 'amount': '-0.300'}[12].
- Q79772590's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+109.99792978117430'}[13].
- Q79772590's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-5.23508015282730'}[14].
- Q79772590's epoch is recorded as J2000.0[15].
- Q79772590's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4463'}[16].
- Q79772590's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+72'}[17].
- Q79772590's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.640'}[18].
- Q79772590's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.575'}[19].
Body
Definition and Type
Q79772590's instance of is recorded as red giant branch star[2].