Q88351960
high proper-motion star in the constellation Virgo
Press Enter · cited answer in seconds
0 sources
Q88351960
Summary
Q88351960 is a high proper-motion star[1].
Key Facts
- Q88351960's instance of is recorded as high proper-motion star[2].
- Q88351960's constellation is recorded as Virgo[3].
- Q88351960's spectral class is recorded as K0[4].
- Q88351960's catalog code is recorded as AG+07 1730[5].
- Q88351960's catalog code is recorded as AGKR 12017[6].
- Q88351960's catalog code is recorded as BD+08 2711[7].
- Q88351960's catalog code is recorded as GSC 00306-00689[8].
- Q88351960's catalog code is recorded as HD 116912[9].
- Q88351960's catalog code is recorded as HIC 65580[10].
- Q88351960's catalog code is recorded as HIP 65580[11].
- Q88351960's catalog code is recorded as PMC 90-93 3741[12].
- Q88351960's catalog code is recorded as PPM 159754[13].
- Q88351960's catalog code is recorded as SAO 119927[14].
- Q88351960's catalog code is recorded as TYC 306-689-1[15].
- Q88351960's catalog code is recorded as YZ 7 6402[16].
- Q88351960's catalog code is recorded as 2MASS J13264213+0727115[17].
- Q88351960's catalog code is recorded as Gaia DR2 3719114577922414976[18].
- Q88351960's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.221'}[19].
- Q88351960's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.681'}[20].
- Q88351960's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.493'}[21].
- Q88351960's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.14'}[22].
- Q88351960's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.28'}[23].
- Q88351960's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.8113'}[24].
- Q88351960's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.4684'}[25].
- Q88351960's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+1.56'}[26].
Body
Definition and Type
Q88351960's instance of is recorded as high proper-motion star[2].