Q86584251
star in the constellation Ara
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Q86584251
Summary
Q86584251 is a star[1].
Key Facts
- Q86584251's instance of is recorded as star[2].
- Q86584251's constellation is recorded as Ara[3].
- Q86584251's catalog code is recorded as IRAS 17350-5514[4].
- Q86584251's catalog code is recorded as AKARI-IRC-V1 J1739102-551630[5].
- Q86584251's catalog code is recorded as RAVE J173910.2-551631[6].
- Q86584251's catalog code is recorded as 2MASS J17391021-5516305[7].
- Q86584251's catalog code is recorded as Gaia DR2 5921184099172456192[8].
- Q86584251's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.078'}[9].
- Q86584251's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.15'}[10].
- Q86584251's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.755'}[11].
- Q86584251's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.0114'}[12].
- Q86584251's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.5313'}[13].
- Q86584251's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+0.96'}[14].
- Q86584251's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+264.79258786693390'}[15].
- Q86584251's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-55.27517937034510'}[16].
- Q86584251's epoch is recorded as J2000.0[17].
- Q86584251's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+3585'}[18].
- Q86584251's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+9500'}[19].
- Q86584251's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.910'}[20].
- Q86584251's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.932'}[21].
Body
Definition and Type
Q86584251's instance of is recorded as star[2].