Q91390201
high proper-motion star in the constellation Cetus
Press Enter · cited answer in seconds
0 sources
Q91390201
Summary
Q91390201 is a high proper-motion star[1].
Key Facts
- Q91390201's instance of is recorded as high proper-motion star[2].
- Q91390201's constellation is recorded as Cetus[3].
- Q91390201's spectral class is recorded as G2V[4].
- Q91390201's catalog code is recorded as 2MASS J00102306-1359023[5].
- Q91390201's catalog code is recorded as BD-14 11[6].
- Q91390201's catalog code is recorded as GSC 05267-00434[7].
- Q91390201's catalog code is recorded as HD 603[8].
- Q91390201's catalog code is recorded as HIC 846[9].
- Q91390201's catalog code is recorded as HIP 846[10].
- Q91390201's catalog code is recorded as LTT 70[11].
- Q91390201's catalog code is recorded as NLTT 477[12].
- Q91390201's catalog code is recorded as PPM 208438[13].
- Q91390201's catalog code is recorded as SAO 147123[14].
- Q91390201's catalog code is recorded as TYC 5267-434-1[15].
- Q91390201's catalog code is recorded as YZ 104 29[16].
- Q91390201's catalog code is recorded as Gaia DR1 2417943682864218368[17].
- Q91390201's catalog code is recorded as Gaia DR2 2417943687160001536[18].
- Q91390201's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.92'}[19].
- Q91390201's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.51'}[20].
- Q91390201's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.825'}[21].
- Q91390201's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.590'}[22].
- Q91390201's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.501'}[23].
- Q91390201's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.7811'}[24].
- Q91390201's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+14.5068'}[25].
- Q91390201's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.58'}[26].
Body
Definition and Type
Q91390201's instance of is recorded as high proper-motion star[2].