E Ophiuchi

e Ophiuchi (HD 156681) is a star in the constellation Ophiuchus near the border with Hercules, which it had been mistakenly catalogued 66 Herculis.[7] I

E Ophiuchi
e Ophiuchi
Observation data
Epoch J2000.0      Equinox ICRS
Constellation Ophiuchus[1]
Right ascension 17h 18m 36.99s[2]
Declination +10° 51′ 52.1″[2]
Apparent magnitude (V) 5.03[3]
Characteristics
Evolutionary stage red giant branch[4]
Spectral type K4II-III[3]
U−B color index 1.89[3]
B−V color index 1.55[3]
R−I color index 0.83[citation needed]
Astrometry
Radial velocity (Rv)1.89 km/s
Proper motion (μ) RA: +7.676[2] mas/yr
Dec.: −97.830[2] mas/yr
Parallax (π)6.3784±0.1045 mas[2]
Distance511 ± 8 ly
(157 ± 3 pc)
Absolute magnitude (MV)−0.86[1]
Details
Mass1.1[4] M
Radius53[4] R
Luminosity554[4] L
Surface gravity (log g)1.06[4] cgs
Temperature3,836[4] K
Rotational velocity (v sin i)5.47[5] km/s
Age10.3[4] Gyr
Other designations
e Oph, 66 Her, BD+11°3156, HD 156681, HR 6433, SAO 102725[6]
Database references
SIMBADdata

e Ophiuchi (HD 156681) is a star in the constellation Ophiuchus near the border with Hercules, which it had been mistakenly catalogued 66 Herculis.[7] It has an apparent magnitude of 5.03.

References

  1. ^ a b Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. XHIP record for this object at VizieR.
  2. ^ a b c d e Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  3. ^ a b c d "VizieR Detailed Page". Archived from the original on 2016-03-05. Retrieved 2012-07-13.
  4. ^ a b c d e f g Reffert, Sabine; Bergmann, Christoph; Quirrenbach, Andreas; Trifonov, Trifon; Künstler, Andreas (2015). "Precise radial velocities of giant stars. VII. Occurrence rate of giant extrasolar planets as a function of mass and metallicity". Astronomy and Astrophysics. 574: A116. arXiv:1412.4634. Bibcode:2015A&A...574A.116R. doi:10.1051/0004-6361/201322360.
  5. ^ Hekker, S.; Meléndez, J. (2007). "Precise radial velocities of giant stars. III. Spectroscopic stellar parameters". Astronomy and Astrophysics. 475 (3): 1003. arXiv:0709.1145. Bibcode:2007A&A...475.1003H. doi:10.1051/0004-6361:20078233.
  6. ^ "e Ophiuchi". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2025-10-05.
  7. ^ Wagman, M. (August 1987), "Flamsteed's Missing Stars", Journal for the History of Astronomy, 18 (3): 209–223, Bibcode:1987JHA....18..209W, doi:10.1177/002182868701800305, S2CID 118445625.


Content Disclaimer

Informasi ini disarikan dari Wikipedia dan disajikan kembali untuk tujuan edukasi. Konten tersedia di bawah lisensi CC BY-SA 3.0. Kami tidak bertanggung jawab atas ketidakakuratan data yang bersumber dari kontribusi publik tersebut.

  1. The information displayed on this website is sourced in part or in whole from Wikipedia and has been adapted for the purpose of restating it. We strive to provide accurate and relevant information, however:
  2. There is no guarantee of absolute accuracy. Wikipedia is an open, collaborative project that can be edited by anyone, so information is subject to change.
  3. It is not intended to constitute professional advice. The content displayed is for informational and educational purposes only. For important decisions (e.g., medical, legal, or financial), please consult a professional.
  4. Content copyright. Wikipedia is licensed under the Creative Commons Attribution-ShareAlike License (CC BY-SA). This means that content may be reused with appropriate attribution and shared under a similar license.
  5. Responsible use. Any risk arising from the use of information from this website is entirely the responsibility of the user.