Q85115983
high proper-motion star in the constellation Cetus
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Q85115983
Summary
Q85115983 is a high proper-motion star[1].
Key Facts
- Q85115983's instance of is recorded as high proper-motion star[2].
- Q85115983's constellation is recorded as Cetus[3].
- Q85115983's spectral class is recorded as G1V[4].
- Q85115983 is part of Q85237615[5].
- Q85115983's catalog code is recorded as GSC 05266-00996[6].
- Q85115983's catalog code is recorded as HD 336B[7].
- Q85115983's catalog code is recorded as TYC 5266-996-1[8].
- Q85115983's catalog code is recorded as 2MASS J00075859-1413334[9].
- Q85115983's catalog code is recorded as ADS 92 B[10].
- Q85115983's catalog code is recorded as BD-15 3B[11].
- Q85115983's catalog code is recorded as CCDM J00080-1414B[12].
- Q85115983's catalog code is recorded as CSI-15 3 1[13].
- Q85115983's catalog code is recorded as IDS 00029-1447 B[14].
- Q85115983's catalog code is recorded as SAO 147097[15].
- Q85115983's catalog code is recorded as YZ 104 12[16].
- Q85115983's catalog code is recorded as WDS J00080-1414B[17].
- Q85115983's catalog code is recorded as Gaia DR2 2417571983510423808[18].
- Q85115983's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.220'}[19].
- Q85115983's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.383'}[20].
- Q85115983's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.034'}[21].
- Q85115983's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.991'}[22].
- Q85115983's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.56'}[23].
- Q85115983's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.4342'}[24].
- Q85115983's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+9.8426'}[25].
- Q85115983's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+1.44'}[26].
Body
Definition and Type
Q85115983's instance of is recorded as high proper-motion star[2].
Use and Application
Q85115983 is part of Q85237615[5].