Eta Herculis
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Hercules |
| Right ascension | 16h 42m 53.7653s[1] |
| Declination | 38° 55′ 20.116″[1] |
| Apparent magnitude (V) | 3.487[1] |
| Characteristics | |
| Spectral type | G7.5 IIIb[1] |
| U−B color index | -0.58 |
| B−V color index | -0.91[2] |
| Astrometry | |
| Radial velocity (Rv) | 8.3[1] km/s |
| Proper motion (μ) | RA: 35.58[1] mas/yr Dec.: -84.98[1] mas/yr |
| Parallax (π) | 29.11 ± 0.52 mas[3] |
| Distance | 112 ± 2 ly (34.4 ± 0.6 pc) |
| Absolute magnitude (MV) | +0.84[4] |
| Details | |
| Mass | 2.13[4] M☉ |
| Radius | 8.9 ± 0.3[5] R☉ |
| Luminosity | 50[6] L☉ |
| Temperature | 4,900[6] K |
| Metallicity [Fe/H] | -0.28[7] dex |
| Rotational velocity (v sin i) | 8[8] km/s |
| Age | 1[6] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Eta Herculis (η Her, η Herculis) is a fourth-magnitude star in the constellation Hercules. It has the traditional name Sophian, possibly from the Arabic نقي meaning "pure"" or from the Greek σοφία meaning "wisdom".
Properties
Sophian is a G-Type star. With a stellar classification G7.5IIIb, it is yet considerably larger having a mass that is 2.3 times solar and a radius 9.8 times.[6] Though it only shines with an apparent magnitude of 3.48, it is part of the "Keystone" asterism, visible overhead in the mid-summer night sky to northern observers, allowing it to be easily recognized. Sophian is 50 times more luminous than the Sun.[6] The Hipparcos satellite mission estimated its distance at roughly 34.4 parsecs[3] from Earth, or 112 light years away.
If one follows the line connecting Eta Herculis with Zeta Herculis one comes across one of the earliest and most stunning globular clusters in the nighttime sky, M13, discovered in 1714 by Edmond Halley.
Eta Herculis is a double star once thought to be part of a binary star system.[6]
See also
- Lists of stars in the constellation Hercules
- Class G Stars
- Double star
References
- ^ a b c d e f g "SIMBAD query result: eta Her -- Star in double system". Centre de Données astronomiques de Strasbourg. Retrieved 2010-06-09.
- ^ Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV data. Bibcode:1986EgUBV........0M.
{{cite journal}}:|format=requires|url=(help) - ^ a b Perryman, M. A. C.; Lindegren, L.; Kovalevsky, J.; Hoeg, E.; et al. (1997). "The HIPPARCOS Catalogue". Astronomy and Astrophysics. 323: L49–L52. Bibcode:1997A&A...323L..49P.
{{cite journal}}:|format=requires|url=(help); Explicit use of et al. in:|author=(help)CS1 maint: multiple names: authors list (link) - ^ a b Pizzolato, N.; Maggio, A.; Sciortino, S. (September 2000), "Evolution of X-ray activity of 1-3 Msun late-type stars in early post-main-sequence phases", Astronomy and Astrophysics, 361: 614–628, Bibcode:2000A&A...361..614P
- ^ Nordgren, Tyler E.; et al. (December 1999), "Stellar Angular Diameters of Late-Type Giants and Supergiants Measured with the Navy Prototype Optical Interferometer", The Astronomical Journal, 118 (6): 3032–3038, Bibcode:1999AJ....118.3032N, doi:10.1086/301114
{{citation}}: CS1 maint: multiple names: authors list (link) - ^ a b c d e f Kaler, James B. "ETA HER (Eta Herculis)". Stars. University of Illinois. Retrieved 2010-06-09.
- ^ Soubiran, C.; Bienaymé, O.; Mishenina, T. V.; Kovtyukh, V. V. (2008). "Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants" (PDF). Astronomy and Astrophysics. 480 (1): 91–101. arXiv:0712.1370. Bibcode:2008A&A...480...91S. doi:10.1051/0004-6361:20078788. Retrieved 2010-06-09.
{{cite journal}}: CS1 maint: multiple names: authors list (link) - ^ Bernacca, P. L.; Perinotto, M. (1970). "A catalogue of stellar rotational velocities". Contr. Oss. Astrof. Padova in Asiago. 239. Bibcode:1970CoAsi.239....1B.
{{cite journal}}: CS1 maint: multiple names: authors list (link)
External links
- Jim Kaler's Stars:Eta Herculis
