Q85821504

Summary

Q85821504 is a high proper-motion star^[1].

Key Facts

• Q85821504's instance of is recorded as high proper-motion star^[2].
• Q85821504's constellation is recorded as Cetus^[3].
• Q85821504's catalog code is recorded as NLTT 8744^[4].
• Q85821504's catalog code is recorded as LP 590-431^[5].
• Q85821504's catalog code is recorded as HD 16886B^[6].
• Q85821504's catalog code is recorded as TYC 4699-978-2^[7].
• Q85821504's catalog code is recorded as ADS 2068 B^[8].
• Q85821504's catalog code is recorded as BD-02 476B^[9].
• Q85821504's catalog code is recorded as CCDM J02423-0221B^[10].
• Q85821504's catalog code is recorded as CSI-02 476 2^[11].
• Q85821504's catalog code is recorded as IDS 02372-0247 B^[12].
• Q85821504's catalog code is recorded as WDS J02423-0221B^[13].
• Q85821504's catalog code is recorded as Gaia DR2 2495889539626436864^[14].
• Q85821504's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.5573'}^[15].
• Q85821504's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+24.8809'}^[16].
• Q85821504's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+34.47'}^[17].
• Q85821504's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+40.1915'}^[18].
• Q85821504's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+40.57993410832540'}^[19].
• Q85821504's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-2.35178562041790'}^[20].
• Q85821504's epoch is recorded as J2000.0^[21].
• Q85821504's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+22.482'}^[22].
• Q85821504's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+174.971'}^[23].

Body

Definition and Type

Q85821504's instance of is recorded as high proper-motion star^[2].