Q79777318
red giant branch star in the constellation Lacerta
Press Enter · cited answer in seconds
0 sources
Q79777318
Summary
Q79777318 is a red giant branch star[1].
Key Facts
- Q79777318's instance of is recorded as red giant branch star[2].
- Q79777318's constellation is recorded as Lacerta[3].
- Q79777318's catalog code is recorded as 2MASS J22101219+5029486[4].
- Q79777318's catalog code is recorded as Gaia DR2 1976988809464956800[5].
- Q79777318's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.175'}[6].
- Q79777318's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.358'}[7].
- Q79777318's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.149'}[8].
- Q79777318's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.5933'}[9].
- Q79777318's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0875'}[10].
- Q79777318's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-65.70'}[11].
- Q79777318's metallicity is recorded as {'unit': '1', 'amount': '+0.074'}[12].
- Q79777318's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+332.55081489521640'}[13].
- Q79777318's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+50.49682587225010'}[14].
- Q79777318's epoch is recorded as J2000.0[15].
- Q79777318's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4299'}[16].
- Q79777318's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+60'}[17].
- Q79777318's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.463'}[18].
- Q79777318's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.408'}[19].
Body
Definition and Type
Q79777318's instance of is recorded as red giant branch star[2].