Q89370289
star in the constellation Ara
Press Enter · cited answer in seconds
0 sources
Q89370289
Summary
Q89370289 is a star[1].
Key Facts
- Q89370289's instance of is recorded as star[2].
- Q89370289's constellation is recorded as Ara[3].
- Q89370289's spectral class is recorded as K0[4].
- Q89370289's catalog code is recorded as CD-50 10887[5].
- Q89370289's catalog code is recorded as CF 15654[6].
- Q89370289's catalog code is recorded as CPD-50 9741[7].
- Q89370289's catalog code is recorded as GC 22727[8].
- Q89370289's catalog code is recorded as GSC 08339-00257[9].
- Q89370289's catalog code is recorded as PPM 345507[10].
- Q89370289's catalog code is recorded as SAO 244260[11].
- Q89370289's catalog code is recorded as TYC 8339-257-1[12].
- Q89370289's catalog code is recorded as 2MASS J16541469-5048535[13].
- Q89370289's catalog code is recorded as Gaia DR1 5936707240548967552[14].
- Q89370289's catalog code is recorded as Gaia DR2 5936707240548967552[15].
- Q89370289's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.491'}[16].
- Q89370289's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.921'}[17].
- Q89370289's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.775'}[18].
- Q89370289's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.67'}[19].
- Q89370289's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.70'}[20].
- Q89370289's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.2478'}[21].
- Q89370289's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.2922'}[22].
- Q89370289's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-3.08'}[23].
- Q89370289's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+436.2621'}[24].
- Q89370289's SIMBAD ID is recorded as CD-50 10887[25].
- Q89370289's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+253.56121850170840'}[26].