Iota Virginis
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Virgo |
| Right ascension | 14h 16m 00.9s |
| Declination | −6° 00′ 02″ |
| Apparent magnitude (V) | +4.07[1] |
| Absolute magnitude (V) | +2.44[2] |
| Distance | 69.8 ± 1.3 ly (21.4 ± 0.4 pc) |
| Spectral type | F6 III[citation needed] |
| Other designations | |
Iota Virginis (
Syrma is a yellow star of apparent magnitude 4.08 and spectral class F6 III about 70 light years from Earth. This star has 1.52 times the mass of the Sun,[3] with a projected rotational velocity of 14.8 km s–1.[2] It is radiating 8.6 times the luminosity of the Sun from its outer atmosphere at an effective temperature of 6,282 K.[1] The radius is about 2.5 times that of the Sun.[4]
In culture
The name Syrma is from the Arabic (سرما (تطريز sirmā "train" (of a garment).
USS Syrma (AK-134) was a United States Navy Crater class cargo ship named after the star.
References
- ^ a b Mallik, Sushma V. (1999), "Lithium abundance and mass", Astronomy and Astrophysics, 352: 495–507, Bibcode:1999A&A...352..495M
{{citation}}: Unknown parameter|month=ignored (help) - ^ a b Pizzolato, N.; Maggio, A.; Sciortino, S. (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
{{citation}}: Unknown parameter|month=ignored (help) - ^ Shaya, Ed J.; Olling, Rob P. (2011), "Very Wide Binaries and Other Comoving Stellar Companions: A Bayesian Analysis of the Hipparcos Catalogue", The Astrophysical Journal Supplement, 192 (1): 2, Bibcode:2011ApJS..192....2S, doi:10.1088/0067-0049/192/1/2
{{citation}}: Unknown parameter|month=ignored (help) - ^ Malagnini, M. L.; Morossi, C. (1990), "Accurate absolute luminosities, effective temperatures, radii, masses and surface gravities for a selected sample of field stars", Astronomy and Astrophysics Supplement Series, 85 (3): 1015–1019, Bibcode:1990A&AS...85.1015M
{{citation}}: Unknown parameter|month=ignored (help)
