Q89770158

Summary

Q89770158 is a star^[1].

Key Facts

• Q89770158's instance of is recorded as star^[2].
• Q89770158's constellation is recorded as Volans^[3].
• Q89770158's spectral class is recorded as K3/4(III)^[4].
• Q89770158's catalog code is recorded as CCDM J07595-6909AB^[5].
• Q89770158's catalog code is recorded as CD-68 516^[6].
• Q89770158's catalog code is recorded as CPC 21.1 1242^[7].
• Q89770158's catalog code is recorded as CPD-68 705^[8].
• Q89770158's catalog code is recorded as GSC 09180-00558^[9].
• Q89770158's catalog code is recorded as HD 66659^[10].
• Q89770158's catalog code is recorded as HIC 39060^[11].
• Q89770158's catalog code is recorded as HIP 39060^[12].
• Q89770158's catalog code is recorded as IDS 07594-6852 AB^[13].
• Q89770158's catalog code is recorded as PPM 776859^[14].
• Q89770158's catalog code is recorded as TYC 9180-558-1^[15].
• Q89770158's catalog code is recorded as WDS J07595-6909AB^[16].
• Q89770158's catalog code is recorded as Gaia DR2 5270582796760365440^[17].
• Q89770158's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.21'}^[18].
• Q89770158's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.67'}^[19].
• Q89770158's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.7121'}^[20].
• Q89770158's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9013'}^[21].
• Q89770158's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+3.27'}^[22].
• Q89770158's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1109.5085'}^[23].
• Q89770158's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+119.86584152811790'}^[24].
• Q89770158's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-69.15204862132490'}^[25].
• Q89770158's epoch is recorded as J2000.0^[26].

Body

Definition and Type

Q89770158's instance of is recorded as star^[2].