Q85477955
star in the constellation Vela
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Q85477955
Summary
Q85477955 is a star[1].
Key Facts
- Q85477955's instance of is recorded as star[2].
- Q85477955's constellation is recorded as Vela[3].
- Q85477955's spectral class is recorded as K[4].
- Q85477955's catalog code is recorded as CD-53 2803[5].
- Q85477955's catalog code is recorded as CPD-53 2234[6].
- Q85477955's catalog code is recorded as GSC 08583-01978[7].
- Q85477955's catalog code is recorded as HD 299922[8].
- Q85477955's catalog code is recorded as PPM 768559[9].
- Q85477955's catalog code is recorded as TYC 8583-1978-1[10].
- Q85477955's catalog code is recorded as Gaia DR1 5311450918113929472[11].
- Q85477955's catalog code is recorded as Gaia DR2 5311450922437905024[12].
- Q85477955's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.97'}[13].
- Q85477955's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.02'}[14].
- Q85477955's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.6709'}[15].
- Q85477955's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.5264'}[16].
- Q85477955's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+2.30'}[17].
- Q85477955's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+655.1363'}[18].
- Q85477955's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+138.49399456125450'}[19].
- Q85477955's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-54.05756802027530'}[20].
- Q85477955's epoch is recorded as J2000.0[21].
- Q85477955's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.817'}[22].
- Q85477955's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.131'}[23].
Body
Definition and Type
Q85477955's instance of is recorded as star[2].