Q80687395
star in the constellation Cetus
Press Enter · cited answer in seconds
0 sources
Q80687395
Summary
Q80687395 is a star[1].
Key Facts
- Q80687395's instance of is recorded as star[2].
- Q80687395's constellation is recorded as Cetus[3].
- Q80687395's spectral class is recorded as F6V[4].
- Q80687395's catalog code is recorded as 2MASS J01173127-0924331[5].
- Q80687395's catalog code is recorded as BD-10 272[6].
- Q80687395's catalog code is recorded as GSC 05274-01059[7].
- Q80687395's catalog code is recorded as HD 7807[8].
- Q80687395's catalog code is recorded as PPM 183260[9].
- Q80687395's catalog code is recorded as SAO 129213[10].
- Q80687395's catalog code is recorded as TYC 5274-1059-1[11].
- Q80687395's catalog code is recorded as YZ 0 4878[12].
- Q80687395's catalog code is recorded as YZ 99 261[13].
- Q80687395's catalog code is recorded as Gaia DR1 2471556419590029824[14].
- Q80687395's catalog code is recorded as Gaia DR2 2471556423886109056[15].
- Q80687395's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.625'}[16].
- Q80687395's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.457'}[17].
- Q80687395's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.381'}[18].
- Q80687395's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.57'}[19].
- Q80687395's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.08'}[20].
- Q80687395's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.4694'}[21].
- Q80687395's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.0380'}[22].
- Q80687395's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+0.66'}[23].
- Q80687395's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+329.1639'}[24].
- Q80687395's SIMBAD ID is recorded as HD 7807[25].
- Q80687395's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+19.38028671991380'}[26].