Q89078880
star in the constellation Perseus
Press Enter · cited answer in seconds
0 sources
Q89078880
Summary
Q89078880 is a star[1].
Key Facts
- Q89078880's instance of is recorded as star[2].
- Q89078880's constellation is recorded as Perseus[3].
- Q89078880's spectral class is recorded as A0[4].
- Q89078880's catalog code is recorded as 2MASS J04072433+4316410[5].
- Q89078880's catalog code is recorded as AG+43 437[6].
- Q89078880's catalog code is recorded as BD+42 893[7].
- Q89078880's catalog code is recorded as GSC 02889-02919[8].
- Q89078880's catalog code is recorded as HD 25819[9].
- Q89078880's catalog code is recorded as HIC 19239[10].
- Q89078880's catalog code is recorded as HIP 19239[11].
- Q89078880's catalog code is recorded as PPM 46807[12].
- Q89078880's catalog code is recorded as SAO 39321[13].
- Q89078880's catalog code is recorded as TD1 2812[14].
- Q89078880's catalog code is recorded as TYC 2889-2919-1[15].
- Q89078880's catalog code is recorded as Gaia DR1 232269872863340160[16].
- Q89078880's catalog code is recorded as Gaia DR2 232269877166505088[17].
- Q89078880's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.44'}[18].
- Q89078880's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.053'}[19].
- Q89078880's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.096'}[20].
- Q89078880's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.029'}[21].
- Q89078880's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.53'}[22].
- Q89078880's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.3814'}[23].
- Q89078880's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.6332'}[24].
- Q89078880's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-4.30'}[25].
- Q89078880's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+275.2395'}[26].
Body
Definition and Type
Q89078880's instance of is recorded as star[2].