Astronomy:41 Lyncis
  Location of 41 Lyncis (circled) | |
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Ursa Major |
| Pronunciation | /ˈɪntərkrʌs/,[1] |
| Right ascension | 09h 28m 39.9889s[2] |
| Declination | +45° 36′ 05.3353″[2] |
| Apparent magnitude (V) | 5.413[3] |
| Characteristics | |
| Spectral type | K0 III[4] |
| U−B color index | 0.74 |
| B−V color index | 0.983[5] |
| Astrometry | |
| Radial velocity (Rv) | +38.44[5] km/s |
| Proper motion (μ) | RA: −7.297±0.140[2] mas/yr Dec.: −129.582±0.130[2] mas/yr |
| Parallax (π) | 11.6388 ± 0.1063[2] mas |
| Distance | 280 ± 3 ly (85.9 ± 0.8 pc) |
| Absolute magnitude (MV) | 0.675[5] |
| Details | |
| Mass | 2.07+0.14 −0.16[6] M☉ |
| Radius | 11[7] R☉ |
| Luminosity | 55[7] L☉ |
| Surface gravity (log g) | 2.30[5] cgs |
| Temperature | 4,789[5] K |
| Metallicity [Fe/H] | –0.23[5] dex |
| Rotational velocity (v sin i) | [7] km/s |
| Age | 4.07±2.24[5] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | The star |
| planet b | |
41 Lyncis (abbreviated 41 Lyn), also designated HD 81688 and named Intercrus /ˈɪntərkrʌs/, is a fifth-magnitude star located in the northern constellation of Ursa Major. An extrasolar planet (designated 41 Lyncis b or HD 81688 b, later named Arkas) is thought to be orbiting the star.
Properties
It is estimated using parallax measurements to be approximately 280 light-years (86 parsecs) from the Sun.[2] The spectrum of this star matches a stellar classification of K0 III,[4] with the luminosity class of III suggesting it is a giant star. This star has about double the mass of the Sun, although a re-evaluation of evolutionary tracks published in 2011 gives a lower estimate of 1.1+0.3
−0.2 solar masses.[6] It has expanded to 11 times the Sun's radius and is radiating 55 times as much as the Sun from its outer atmosphere at an effective temperature of 4,789 K.[7] This temperature gives it the orange-hued glow of a K-type star.[8]
This star is following an orbit through the Milky Way with an eccentricity of 0.21. This will take it as close to the Galactic Center as 18.5 kly (5.7 kpc) and as far as 28.2 kly (8.6 kpc). The inclination of this orbit will carry it as much as 1,800 ly (550 pc) away from the galactic plane. For this reason, it is uncertain whether this star is a member of the thin disk population.[5]
41 Lyncis is listed in the Washington Double Star Catalog as having two visual companions, the 8th-magnitude F-type subgiant HD 81704 72″ away, and an 11th-magnitude star 84″ away.[9] Both are background objects, more distant than 41 Lyncis itself, but the two share a common proper motion and are at the same distance as each other.[10]
Nomenclature
41 Lyncis is the Flamsteed designation.[11] Typically, 'Lyncis' is the genitive for a star found in the constellation of Lynx. However, when the constellation boundaries were officially established by the International Astronomical Union (IAU) in 1930, this star was located within Ursa Major. HD 81688 is the entry in the Henry Draper Catalogue. Following its discovery the planet was designated 41 Lyncis b or alternatively HD 81688 b.
In July 2014 the IAU launched NameExoWorlds, a process for giving proper names to certain exoplanets and their host stars.[12] The process involved public nomination and voting for the new names.[13] In December 2015, the IAU announced the winning names were Intercrus for this star and Arkas for its planet.[14] The winning names were those submitted by the Okayama Astro Club of Japan . Intercrus means "between the legs" in Latin style, referring to the star's position in the constellation Ursa Major. Arkas was the son of Callisto (Ursa Major) in Greek mythology.[15]
The International Astronomical Union Working Group on Star Names (WGSN) has approved the proper name Intercrus for 41 Lyncis.[16]
Planetary system
On 19 February 2008 a planet was announced orbiting the star. It has a minimum mass 2.7 times that of Jupiter and completes an orbit every 184 days.[17]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b (Arkas) | >2.7 MJ | 0.81 | 184.02 ± 0.18 | 0 (fixed) | — | — |
References
- ↑ inter-, crus (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=inter-%2C+crus (Subscription or UK public library membership required.)
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 3.0 3.1 "* 41 Lyn". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=%2A+41+Lyn.
- ↑ 4.0 4.1 Sato, K.; Kuji, S. (1990), "MK classification and photometry of stars used for time and latitude observations at Mizusawa and Washington", Astronomy and Astrophysics Supplement Series 85: 1069, Bibcode: 1990A&AS...85.1069S
- ↑ 5.0 5.1 5.2 5.3 5.4 5.5 5.6 5.7 Soubiran, C. et al. (2008), "Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants", Astronomy and Astrophysics 480 (1): 91–101, doi:10.1051/0004-6361:20078788, Bibcode: 2008A&A...480...91S
- ↑ 6.0 6.1 Kunitomo, M. et al. (August 2011), "Planet Engulfment by ~1.5-3 M sun Red Giants", The Astrophysical Journal 737 (2): 66, doi:10.1088/0004-637X/737/2/66, Bibcode: 2011ApJ...737...66K
- ↑ 7.0 7.1 7.2 7.3 Massarotti, Alessandro et al. (January 2008), "Rotational and radial velocities for a sample of 761 HIPPARCOS giants and the role of binarity", The Astronomical Journal 135 (1): 209–231, doi:10.1088/0004-6256/135/1/209, Bibcode: 2008AJ....135..209M
- ↑ "The Colour of Stars", Australia Telescope, Outreach and Education (Commonwealth Scientific and Industrial Research Organisation), December 21, 2004, http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html, retrieved 2012-01-16
- ↑ Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001), "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog", The Astronomical Journal 122 (6): 3466–3471, doi:10.1086/323920, Bibcode: 2001AJ....122.3466M
- ↑ Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G.
- ↑ Kostjuk, N. D. (April 2004), "HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index (Kostjuk, 2002)", VizieR On-line Data Catalog: IV/27A (Institute of Astronomy of Russian Academy of Sciences), Bibcode: 2004yCat.4027....0K
- ↑ NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars. IAU.org. 9 July 2014
- ↑ "NameExoWorlds The Process". http://nameexoworlds.iau.org/process.
- ↑ Final Results of NameExoWorlds Public Vote Released, International Astronomical Union, 15 December 2015.
- ↑ "NameExoWorlds The Approved Names". http://nameexoworlds.iau.org/names.
- ↑ IAU Catalog of Star Names, http://www.pas.rochester.edu/~emamajek/WGSN/IAU-CSN.txt, retrieved 28 July 2016
- ↑ 17.0 17.1 Sato, Bun'ei et al. (2008), "Planetary Companions around Three Intermediate-Mass G and K Giants: 18 Delphini, ξ Aquilae and HD 81688", Publications of the Astronomical Society of Japan 60 (3): 539–550, doi:10.1093/pasj/60.3.539, Bibcode: 2008PASJ...60..539S
External links
- "Image HD 81688". http://aladin.u-strasbg.fr/AladinPreview?-c=09+28+39.9893%2B45+36+05.339&ident=HD++81688&submit=Aladin+previewer.
- "Notes for star HD 81688". Extrasolar Planets Encyclopaedia. http://exoplanet.eu/star.php?st=HD+81688.
- "HR 3743 – Star in double system". http://webviz.u-strasbg.fr/viz-bin/VizieR-S?HR%203743.
- "CCDM J09287 +4536 – Star in double system". http://webviz.u-strasbg.fr/viz-bin/VizieR-S?CCDM%20J09287%2b4536A.
Coordinates: 
09h 28m 40s, +45° 36′ 05″
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