Q94490449
star in the constellation Libra
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Q94490449
Summary
Q94490449 is a star[1].
Key Facts
- Q94490449's instance of is recorded as star[2].
- Q94490449's constellation is recorded as Libra[3].
- Q94490449's spectral class is recorded as K0III[4].
- Q94490449's catalog code is recorded as BD-14 4229[5].
- Q94490449's catalog code is recorded as GSC 05607-00177[6].
- Q94490449's catalog code is recorded as HD 138613[7].
- Q94490449's catalog code is recorded as PPM 230405[8].
- Q94490449's catalog code is recorded as SAO 159347[9].
- Q94490449's catalog code is recorded as TYC 5607-177-1[10].
- Q94490449's catalog code is recorded as YZ 104 5702[11].
- Q94490449's catalog code is recorded as 2MASS J15334223-1455201[12].
- Q94490449's catalog code is recorded as Gaia DR2 6265041517345159552[13].
- Q94490449's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.99'}[14].
- Q94490449's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.19'}[15].
- Q94490449's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.856'}[16].
- Q94490449's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.269'}[17].
- Q94490449's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.101'}[18].
- Q94490449's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.6160'}[19].
- Q94490449's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.7758'}[20].
- Q94490449's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-3.95'}[21].
- Q94490449's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+360.2565'}[22].
- Q94490449's SIMBAD ID is recorded as HD 138613[23].
- Q94490449's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+233.42595188303280'}[24].
- Q94490449's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-14.92227234922430'}[25].
- Q94490449's epoch is recorded as J2000.0[26].