Syrma, 99 Vir, BD−05°3843, FK5 525, GJ 9473, HD 124850, HIP 69701, HR 5338, SAO 139824
Database references
SIMBAD
data
Iota Virginis (ι Virginis, abbreviated Iota Vir, ι Vir) is a binary star in the constellation of Virgo. Its apparent magnitude is 4.08.[2] Based on its parallax, it is assumed to be relatively nearby, at 71.8 light-years (22.0 parsecs).[1]
Its two components are designated Iota Virginis A (officially named Syrma/ˈsɜːrmə/,[7] the traditional name for the system)[8] and B.
^ abcdefVallenari, 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.
^ abGray, R. O.; Napier, M. G.; Winkler, L. I. (2001). "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars". The Astronomical Journal. 121 (4): 2148. Bibcode:2001AJ....121.2148G. doi:10.1086/319956.
^ abcdeGontcharov, G.A.; Kiyaeva, O.V. (2010). "Photocentric orbits from a direct combination of ground-based astrometry with Hipparcos II. Preliminary orbits for six astrometric binaries". New Astronomy. 15 (3): 324–331. arXiv:1606.08182. Bibcode:2010NewA...15..324G. doi:10.1016/j.newast.2009.09.006. S2CID 119252073.
^ abMermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.
^ abAguilera-Gómez, Claudia; Ramírez, Iván; Chanamé, Julio (2018-06-01). "Lithium abundance patterns of late-F stars: an in-depth analysis of the lithium desert". Astronomy and Astrophysics. 614: A55. arXiv:1803.05922. Bibcode:2018A&A...614A..55A. doi:10.1051/0004-6361/201732209. ISSN 0004-6361. Iota Virginis' databasee entry at VizieR.
^ abcdBaines, Ellyn K.; Clark, James H., III; Schmitt, Henrique R.; Stone, Jordan M.; von Braun, Kaspar (2023-12-01). "33 New Stellar Angular Diameters from the NPOI, and Nearly 180 NPOI Diameters as an Ensemble". The Astronomical Journal. 166 (6): 268. Bibcode:2023AJ....166..268B. doi:10.3847/1538-3881/ad08be. ISSN 0004-6256.{{cite journal}}: CS1 maint: multiple names: authors list (link)
^"syrma". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
^"Naming Stars". IAU.org. Retrieved 16 December 2017.
IotaVirginis (ι Virginis, abbreviated Iota Vir, ι Vir) is a binary star in the constellation of Virgo. Its apparent magnitude is 4.08. Based on its parallax...
an asterism consisting of Kappa Virginis, IotaVirginis, Phi Virginis and Lambda Virginis. Consequently, Kappa Virginis itself is known as 亢宿一 (Káng Sù...
Phi Virginis (φ Virginis, abbreviated Phi Vir, φ Vir) is a binary star in the zodiac constellation of Virgo. It can be seen with the naked eye, having...
Lambda Virginis (λ Virginis, abbreviated Lambda Vir, λ Vir) is a binary star system in the zodiac constellation of Virgo. With an apparent visual magnitude...
the Almagest) Chi Andromedae (one of adhil in the Almagest) Syrma (IotaVirginis) "Naming Stars". IAU.org. Retrieved 18 June 2018. Peters, C. H. F. and...
Beta Virginis, a name Latinised from β Virginis, is a star in the equatorial constellation of Virgo. It has the proper name Zavijava (/ˌzævɪˈdʒævə/), and...
Star Slightly variable 3.38 3.32 Delta Virginis Star 3.38 Epsilon Hydrae Quintuple star system 3.38 Zeta Virginis Binary star system Slightly variable 3...
Iota Leonis, Latinized from ι Leonis, is a triple star system in the constellation Leo. The system is fairly close to the Sun, at only 79 light-years (24...
synthesis of an image of Mizar; then a first-ever six-way synthesis of Eta Virginis in 2002; and most recently "closure phase" as a step to the first synthesized...
Angle of the Barking Dog زاوية العواء Beta Virginis Zawiah aka Zaniah az-Zāwiyah The angle الزاوية Eta Virginis Zubenelgenubi az-Zubān ul-Janūbiy Southern...
examples include Polaris, Alpha Leporis, Alpha Persei, Delta Canis Majoris and Iota¹ Scorpii. Many of them are variable stars, mostly pulsating Cepheids such...
five stars, the largest depicting Sirius Canopus (α Carinae) Spica (α Virginis) Hydra: two stars, the larger being Alphard Crux Australis: five stars...
object) Cepheid W Virginis, a class of Cepheids named after W Virginis, the archetype for the class CWA – (celestial object) Cepheid W Virginis A, a subclass...
Enclosure, refers to an asterism consisting of Theta Leonis, Beta Virginis, Sigma Leonis, Iota Leonis and Delta Leonis. Consequently, the Chinese name for Theta...
Bibcode:2003ApJ...599.1383H. doi:10.1086/379281. S2CID 11506537. "The planet-host star Iota Horologii". Kiefer, Flavien (17 October 2019). "Determining the mass of the...
stars found that 75% of the Mira stars which could be resolved using the IOTA telescope are not spherically symmetric, a result which is consistent with...
L. (1986). "Heavy-element abundances in the mild barium stars Omicron Virginis and 16 Serpentis". The Astrophysical Journal. 311: 819. Bibcode:1986ApJ...
its structure modeled as stratospheric. Iota Draconis b: The first planet discovered around the giant star Iota Draconis, an orange giant. This provides...
21 confirmed and 139 candidates. The most massive confirmed exoplanet is Iota Draconis b, which masses 9.40 MJ (i.e. 9.4 times the mass of Jupiter); the...
Wall Gamma Virginis Porrima 東上相 Dōng Shàng Xiàng The First Eastern Minister 太微左垣三 Tài Wēi Zuǒ Yuán sān the Third Star of Left Wall Delta Virginis Minelauva...
catalogue, plus 77 candidates and 61 poor or rejected stars. Six stars, namely Iota Herculis, 53 Piscium, Nu Eridani, Gamma Pegasi, HD 13745 (V354 Persei) and...
(2009-02-11). "The radius and other fundamental parameters of the F9 V star beta Virginis". Monthly Notices of the Royal Astronomical Society. 393 (1): 245–252....