Q84620242
high proper-motion star in the constellation Tucana
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Q84620242
Summary
Q84620242 is a high proper-motion star[1].
Key Facts
- Q84620242's instance of is recorded as high proper-motion star[2].
- Q84620242's constellation is recorded as Tucana[3].
- Q84620242's spectral class is recorded as G3V[4].
- Q84620242's spectral class is recorded as G5[5].
- Q84620242's catalog code is recorded as CD-58 8278[6].
- Q84620242's catalog code is recorded as CPC 20 7026[7].
- Q84620242's catalog code is recorded as CPD-58 7932[8].
- Q84620242's catalog code is recorded as GSC 08828-00617[9].
- Q84620242's catalog code is recorded as HD 210769[10].
- Q84620242's catalog code is recorded as HIC 109792[11].
- Q84620242's catalog code is recorded as HIP 109792[12].
- Q84620242's catalog code is recorded as PPM 350076[13].
- Q84620242's catalog code is recorded as SAO 247369[14].
- Q84620242's catalog code is recorded as TYC 8828-617-1[15].
- Q84620242's catalog code is recorded as 2MASS J22142000-5801077[16].
- Q84620242's catalog code is recorded as Gaia DR2 6411547318571790592[17].
- Q84620242's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.333'}[18].
- Q84620242's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.080'}[19].
- Q84620242's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.007'}[20].
- Q84620242's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.47'}[21].
- Q84620242's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.06'}[22].
- Q84620242's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.3148'}[23].
- Q84620242's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+9.3301'}[24].
- Q84620242's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+10.25'}[25].
- Q84620242's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+10.41'}[26].
Body
Definition and Type
Q84620242's instance of is recorded as high proper-motion star[2].