Q84245489
red giant branch star in the constellation Orion
Press Enter · cited answer in seconds
0 sources
Q84245489
Summary
Q84245489 is a red giant branch star[1].
Key Facts
- Q84245489's instance of is recorded as red giant branch star[2].
- Q84245489's constellation is recorded as Orion[3].
- Q84245489's catalog code is recorded as 2MASS J05543532-0453465[4].
- Q84245489's catalog code is recorded as Gaia DR2 3022614437499479040[5].
- Q84245489's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.637'}[6].
- Q84245489's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.978'}[7].
- Q84245489's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.818'}[8].
- Q84245489's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.6339'}[9].
- Q84245489's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3301'}[10].
- Q84245489's metallicity is recorded as {'unit': '1', 'amount': '-0.254'}[11].
- Q84245489's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3029.3850'}[12].
- Q84245489's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+88.64718612311740'}[13].
- Q84245489's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-4.89628004300490'}[14].
- Q84245489's epoch is recorded as J2000.0[15].
- Q84245489's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4705'}[16].
- Q84245489's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+263'}[17].
- Q84245489's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.677'}[18].
- Q84245489's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.666'}[19].
Body
Definition and Type
Q84245489's instance of is recorded as red giant branch star[2].