Q66612561
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Q66612561
Summary
Q66612561 is a high proper-motion star[1].
Key Facts
- Q66612561's instance of is recorded as high proper-motion star[2].
- Q66612561's spectral class is recorded as F3V[3].
- Q66612561's catalog code is recorded as HD 92210[4].
- Q66612561's catalog code is recorded as CPC 22 1318[5].
- Q66612561's catalog code is recorded as GSC 09405-01434[6].
- Q66612561's catalog code is recorded as HIC 51713[7].
- Q66612561's catalog code is recorded as HIP 51713[8].
- Q66612561's catalog code is recorded as 2MASS J10335656-8031004[9].
- Q66612561's catalog code is recorded as PPM 377227[10].
- Q66612561's catalog code is recorded as SAO 258585[11].
- Q66612561's catalog code is recorded as TD1 15013[12].
- Q66612561's catalog code is recorded as uvby98 100092210[13].
- Q66612561's catalog code is recorded as TYC 9405-1434-1[14].
- Q66612561's catalog code is recorded as RX J1033.8-8030[15].
- Q66612561's catalog code is recorded as Gaia DR1 5198748158767676672[16].
- Q66612561's catalog code is recorded as Gaia DR2 5198748163065619328[17].
- Q66612561's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.57'}[18].
- Q66612561's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.18'}[19].
- Q66612561's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.0747'}[20].
- Q66612561's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.390'}[21].
- Q66612561's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.251'}[22].
- Q66612561's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.161'}[23].
- Q66612561's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+10.5085'}[24].
- Q66612561's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+26.86'}[25].
- Q66612561's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+95.1611'}[26].
Body
Definition and Type
Q66612561's instance of is recorded as high proper-motion star[2].