Q89026150
high proper-motion star in the constellation Aquarius
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Q89026150
Summary
Q89026150 is a high proper-motion star[1].
Key Facts
- Q89026150's instance of is recorded as high proper-motion star[2].
- Q89026150's constellation is recorded as Aquarius[3].
- Q89026150's spectral class is recorded as G8II[4].
- Q89026150's catalog code is recorded as BD-12 6343[5].
- Q89026150's catalog code is recorded as GSC 05815-00032[6].
- Q89026150's catalog code is recorded as HD 215555[7].
- Q89026150's catalog code is recorded as HIC 112415[8].
- Q89026150's catalog code is recorded as HIP 112415[9].
- Q89026150's catalog code is recorded as PPM 240726[10].
- Q89026150's catalog code is recorded as SAO 165283[11].
- Q89026150's catalog code is recorded as TYC 5815-32-1[12].
- Q89026150's catalog code is recorded as YZC 11 8017[13].
- Q89026150's catalog code is recorded as [L91b] 370[14].
- Q89026150's catalog code is recorded as 2MASS J22460877-1209314[15].
- Q89026150's catalog code is recorded as Gaia DR1 2604532008688545152[16].
- Q89026150's catalog code is recorded as Gaia DR2 2604532012983927168[17].
- Q89026150's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.947'}[18].
- Q89026150's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.538'}[19].
- Q89026150's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.424'}[20].
- Q89026150's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.36'}[21].
- Q89026150's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.25'}[22].
- Q89026150's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.1560'}[23].
- Q89026150's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+7.6427'}[24].
- Q89026150's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-33.39'}[25].
- Q89026150's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+130.8438'}[26].
Body
Definition and Type
Q89026150's instance of is recorded as high proper-motion star[2].