Q75266939
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Q75266939
Summary
Q75266939 is a star[1].
Key Facts
- Q75266939's instance of is recorded as star[2].
- Q75266939's spectral class is recorded as G3IV[3].
- Q75266939's catalog code is recorded as 2MASS J00242663-7815013[4].
- Q75266939's catalog code is recorded as CD-78 13[5].
- Q75266939's catalog code is recorded as CPC 21.3 42[6].
- Q75266939's catalog code is recorded as CPD-78 11[7].
- Q75266939's catalog code is recorded as GSC 09350-01182[8].
- Q75266939's catalog code is recorded as HD 2134[9].
- Q75266939's catalog code is recorded as HIC 1937[10].
- Q75266939's catalog code is recorded as HIP 1937[11].
- Q75266939's catalog code is recorded as PPM 366908[12].
- Q75266939's catalog code is recorded as SRS 18492[13].
- Q75266939's catalog code is recorded as TYC 9350-1182-1[14].
- Q75266939's catalog code is recorded as Gaia DR1 4635564765283483776[15].
- Q75266939's catalog code is recorded as Gaia DR2 4635564769579703936[16].
- Q75266939's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.602'}[17].
- Q75266939's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.313'}[18].
- Q75266939's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.228'}[19].
- Q75266939's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.82'}[20].
- Q75266939's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.50'}[21].
- Q75266939's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.6468'}[22].
- Q75266939's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+13.9811'}[23].
- Q75266939's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+4.39'}[24].
- Q75266939's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+71.5251'}[25].
- Q75266939's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+2.0'}[26].
Body
Definition and Type
Q75266939's instance of is recorded as star[2].