Q79777205
red giant branch star in the constellation Hydra
Press Enter · cited answer in seconds
0 sources
Q79777205
Summary
Q79777205 is a red giant branch star[1].
Key Facts
- Q79777205's instance of is recorded as red giant branch star[2].
- Q79777205's constellation is recorded as Hydra[3].
- Q79777205's catalog code is recorded as 2MASS J09002548+0445122[4].
- Q79777205's catalog code is recorded as Gaia DR2 580212526495741184[5].
- Q79777205's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.689'}[6].
- Q79777205's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.141'}[7].
- Q79777205's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.048'}[8].
- Q79777205's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.2759'}[9].
- Q79777205's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2854'}[10].
- Q79777205's metallicity is recorded as {'unit': '1', 'amount': '-0.477'}[11].
- Q79777205's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3503.8542'}[12].
- Q79777205's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+135.10617808825700'}[13].
- Q79777205's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+4.75339084063510'}[14].
- Q79777205's epoch is recorded as J2000.0[15].
- Q79777205's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4709'}[16].
- Q79777205's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+339'}[17].
- Q79777205's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.684'}[18].
- Q79777205's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.979'}[19].
Body
Definition and Type
Q79777205's instance of is recorded as red giant branch star[2].