Q91702954
star in the constellation Ara
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Q91702954
Summary
Q91702954 is a star[1].
Key Facts
- Q91702954's instance of is recorded as star[2].
- Q91702954's constellation is recorded as Ara[3].
- Q91702954's catalog code is recorded as IRAS 17542-5300[4].
- Q91702954's catalog code is recorded as AKARI-IRC-V1 J1758146-530058[5].
- Q91702954's catalog code is recorded as RAVE J175814.6-530059[6].
- Q91702954's catalog code is recorded as 2MASS J17581463-5300590[7].
- Q91702954's catalog code is recorded as Gaia DR2 5944909773388124672[8].
- Q91702954's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.113'}[9].
- Q91702954's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.24'}[10].
- Q91702954's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.661'}[11].
- Q91702954's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.1508'}[12].
- Q91702954's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3419'}[13].
- Q91702954's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-423.82'}[14].
- Q91702954's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+269.56101516072180'}[15].
- Q91702954's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-53.01643895052450'}[16].
- Q91702954's epoch is recorded as J2000.0[17].
- Q91702954's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4500'}[18].
- Q91702954's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+58'}[19].
- Q91702954's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.009'}[20].
- Q91702954's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.247'}[21].
Body
Definition and Type
Q91702954's instance of is recorded as star[2].