Q90770259
star in the constellation Hydrus
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Q90770259
Summary
Q90770259 is a star[1].
Key Facts
- Q90770259's instance of is recorded as star[2].
- Q90770259's constellation is recorded as Hydrus[3].
- Q90770259's spectral class is recorded as K3III[4].
- Q90770259's catalog code is recorded as CD-76 54[5].
- Q90770259's catalog code is recorded as CPC 21.3 153[6].
- Q90770259's catalog code is recorded as CPD-76 100[7].
- Q90770259's catalog code is recorded as GSC 09348-00826[8].
- Q90770259's catalog code is recorded as HD 9249[9].
- Q90770259's catalog code is recorded as PPM 367278[10].
- Q90770259's catalog code is recorded as TYC 9348-826-1[11].
- Q90770259's catalog code is recorded as 2MASS J01273069-7604259[12].
- Q90770259's catalog code is recorded as Gaia DR2 4637639616740638720[13].
- Q90770259's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.355'}[14].
- Q90770259's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.813'}[15].
- Q90770259's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.635'}[16].
- Q90770259's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.26'}[17].
- Q90770259's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.42'}[18].
- Q90770259's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.9499'}[19].
- Q90770259's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.2453'}[20].
- Q90770259's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+40.03'}[21].
- Q90770259's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+445.3748'}[22].
- Q90770259's SIMBAD ID is recorded as HD 9249[23].
- Q90770259's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+21.87784553557630'}[24].
- Q90770259's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-76.07383782385090'}[25].
- Q90770259's epoch is recorded as J2000.0[26].