Q79818338
red giant branch star in the constellation Cassiopeia
Press Enter · cited answer in seconds
0 sources
Q79818338
Summary
Q79818338 is a red giant branch star[1].
Key Facts
- Q79818338's instance of is recorded as red giant branch star[2].
- Q79818338's constellation is recorded as Cassiopeia[3].
- Q79818338's catalog code is recorded as 2MASS J01401721+6707169[4].
- Q79818338's catalog code is recorded as Gaia DR2 519516568366457728[5].
- Q79818338's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.710'}[6].
- Q79818338's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.745'}[7].
- Q79818338's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.458'}[8].
- Q79818338's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.9174'}[9].
- Q79818338's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2666'}[10].
- Q79818338's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-73.05'}[11].
- Q79818338's metallicity is recorded as {'unit': '1', 'amount': '-0.077'}[12].
- Q79818338's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+25.07171716754050'}[13].
- Q79818338's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+67.12140697080260'}[14].
- Q79818338's epoch is recorded as J2000.0[15].
- Q79818338's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4191'}[16].
- Q79818338's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+43'}[17].
- Q79818338's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.191'}[18].
- Q79818338's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.302'}[19].
Body
Definition and Type
Q79818338's instance of is recorded as red giant branch star[2].