Q85067692
star in the constellation Lacerta
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Q85067692
Summary
Q85067692 is a star[1].
Key Facts
- Q85067692's instance of is recorded as star[2].
- Q85067692's constellation is recorded as Lacerta[3].
- Q85067692's spectral class is recorded as G0[4].
- Q85067692's catalog code is recorded as GSC 03987-02233[5].
- Q85067692's catalog code is recorded as LF 4 +54 1009[6].
- Q85067692's catalog code is recorded as 2MASS J22344962+5438323[7].
- Q85067692's catalog code is recorded as Gaia DR2 2003370354021219328[8].
- Q85067692's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.9'}[9].
- Q85067692's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.761'}[10].
- Q85067692's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.437'}[11].
- Q85067692's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.39'}[12].
- Q85067692's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.9990'}[13].
- Q85067692's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.6902'}[14].
- Q85067692's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-27.17'}[15].
- Q85067692's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+591.6460'}[16].
- Q85067692's SIMBAD ID is recorded as GSC 03987-02233[17].
- Q85067692's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+338.70677628357020'}[18].
- Q85067692's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+54.64232633557170'}[19].
- Q85067692's epoch is recorded as J2000.0[20].
- Q85067692's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-16.259'}[21].
- Q85067692's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-12.603'}[22].
- Q85067692's Gaia ID is recorded as 2003370354021219328[23].