Q84252120
red giant branch star in the constellation Cassiopeia
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Q84252120
Summary
Q84252120 is a red giant branch star[1].
Key Facts
- Q84252120's instance of is recorded as red giant branch star[2].
- Q84252120's constellation is recorded as Cassiopeia[3].
- Q84252120's catalog code is recorded as 2MASS J00304554+5506469[4].
- Q84252120's catalog code is recorded as Gaia DR2 418224918654493440[5].
- Q84252120's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.522'}[6].
- Q84252120's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.985'}[7].
- Q84252120's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.840'}[8].
- Q84252120's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.3089'}[9].
- Q84252120's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6475'}[10].
- Q84252120's metallicity is recorded as {'unit': '1', 'amount': '-0.247'}[11].
- Q84252120's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1544.4015'}[12].
- Q84252120's SIMBAD ID is recorded as 2MASS J00304554+5506469[13].
- Q84252120's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+7.68976762952740'}[14].
- Q84252120's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+55.11303190693740'}[15].
- Q84252120's epoch is recorded as J2000.0[16].
- Q84252120's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4818'}[17].
- Q84252120's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+1288'}[18].
- Q84252120's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.344'}[19].
- Q84252120's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+6.748'}[20].
- Q84252120's Gaia ID is recorded as 418224918654493440[21].