Q75173106
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Q75173106
Summary
Q75173106 is an emission-line star[1].
Key Facts
- Q75173106's instance of is recorded as emission-line star[2].
- Q75173106's catalog code is recorded as IRAS 09042-2844[3].
- Q75173106's catalog code is recorded as AKARI-IRC-V1 J0906213-285613[4].
- Q75173106's catalog code is recorded as RAVE J090621.4-285614[5].
- Q75173106's catalog code is recorded as WRAY 15-328[6].
- Q75173106's catalog code is recorded as Gaia DR2 5635672299869382912[7].
- Q75173106's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.80'}[8].
- Q75173106's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.6504'}[9].
- Q75173106's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.5518'}[10].
- Q75173106's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+80.702'}[11].
- Q75173106's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+80.70'}[12].
- Q75173106's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2222.35'}[13].
- Q75173106's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+136.58919614868360'}[14].
- Q75173106's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-28.93713767033450'}[15].
- Q75173106's epoch is recorded as J2000.0[16].
- Q75173106's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+3400'}[17].
- Q75173106's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+3'}[18].
- Q75173106's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+3.193'}[19].
- Q75173106's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.461'}[20].
Body
Definition and Type
Q75173106's instance of is recorded as emission-line star[2].