Q85811741
star in the constellation Fornax
Press Enter · cited answer in seconds
0 sources
Q85811741
Summary
Q85811741 is a star[1].
Key Facts
- Q85811741's instance of is recorded as star[2].
- Q85811741's constellation is recorded as Fornax[3].
- Q85811741's spectral class is recorded as F7V[4].
- Q85811741's catalog code is recorded as 2MASS J03184244-3248082[5].
- Q85811741's catalog code is recorded as CD-33 1166[6].
- Q85811741's catalog code is recorded as CPD-33 345[7].
- Q85811741's catalog code is recorded as GSC 07023-00022[8].
- Q85811741's catalog code is recorded as HD 20684[9].
- Q85811741's catalog code is recorded as PPM 278921[10].
- Q85811741's catalog code is recorded as TYC 7023-22-1[11].
- Q85811741's catalog code is recorded as RAVE J031842.5-324808[12].
- Q85811741's catalog code is recorded as USNO-B1.0 0571-00034417[13].
- Q85811741's catalog code is recorded as DENIS J031842.4-324808[14].
- Q85811741's catalog code is recorded as Gaia DR1 5054389806822843008[15].
- Q85811741's catalog code is recorded as Gaia DR2 5054389811119207296[16].
- Q85811741's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.947'}[17].
- Q85811741's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.621'}[18].
- Q85811741's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.576'}[19].
- Q85811741's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.616'}[20].
- Q85811741's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.7'}[21].
- Q85811741's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.06'}[22].
- Q85811741's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.64'}[23].
- Q85811741's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.774'}[24].
- Q85811741's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.9146'}[25].
- Q85811741's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.1835'}[26].
Body
Definition and Type
Q85811741's instance of is recorded as star[2].