Q79775776
red giant branch star in the constellation Orion
Press Enter · cited answer in seconds
0 sources
Q79775776
Summary
Q79775776 is a red giant branch star[1].
Key Facts
- Q79775776's instance of is recorded as red giant branch star[2].
- Q79775776's constellation is recorded as Orion[3].
- Q79775776's catalog code is recorded as 2MASS J06182277+0748106[4].
- Q79775776's catalog code is recorded as Gaia DR2 3325254596433466240[5].
- Q79775776's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.780'}[6].
- Q79775776's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.195'}[7].
- Q79775776's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.093'}[8].
- Q79775776's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.6748'}[9].
- Q79775776's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2552'}[10].
- Q79775776's metallicity is recorded as {'unit': '1', 'amount': '-0.514'}[11].
- Q79775776's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3918.4953'}[12].
- Q79775776's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+94.59486294971240'}[13].
- Q79775776's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+7.80294153394280'}[14].
- Q79775776's epoch is recorded as J2000.0[15].
- Q79775776's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4976'}[16].
- Q79775776's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+295'}[17].
- Q79775776's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.635'}[18].
- Q79775776's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.710'}[19].
Body
Definition and Type
Q79775776's instance of is recorded as red giant branch star[2].