Q89382620
star in the constellation Hydrus
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Q89382620
Summary
Q89382620 is a star[1].
Key Facts
- Q89382620's instance of is recorded as star[2].
- Q89382620's constellation is recorded as Hydrus[3].
- Q89382620's spectral class is recorded as G0IV[4].
- Q89382620's catalog code is recorded as 2MASS J02254380-7048575[5].
- Q89382620's catalog code is recorded as CD-71 110[6].
- Q89382620's catalog code is recorded as CPC 21.1 353[7].
- Q89382620's catalog code is recorded as CPD-71 131[8].
- Q89382620's catalog code is recorded as GSC 09147-01450[9].
- Q89382620's catalog code is recorded as HD 15484[10].
- Q89382620's catalog code is recorded as PPM 367654[11].
- Q89382620's catalog code is recorded as TYC 9147-1450-1[12].
- Q89382620's catalog code is recorded as Gaia DR2 4645287991421509120[13].
- Q89382620's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.263'}[14].
- Q89382620's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.977'}[15].
- Q89382620's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.889'}[16].
- Q89382620's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.37'}[17].
- Q89382620's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.94'}[18].
- Q89382620's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.2079'}[19].
- Q89382620's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.9460'}[20].
- Q89382620's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+34.29'}[21].
- Q89382620's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+202.1836'}[22].
- Q89382620's SIMBAD ID is recorded as HD 15484[23].
- Q89382620's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+36.43256725788410'}[24].
- Q89382620's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-70.81598588572380'}[25].
- Q89382620's epoch is recorded as J2000.0[26].