Astronomy:Lambda2 Fornacis

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Short description: Binary star system in the constellation Fornax


For other stars with this Bayer designation, see λ Fornacis.
Lambda2 Fornacis
250px
λ2 Fornacis on the right of the Fornax Dwarf Galaxy
Credit: ESO/Digitized Sky Survey 2
Observation data
Equinox J2000.0]] (ICRS)
Constellation Fornax
Right ascension  02h 36m 58.60775s[1]
Declination −34° 34′ 40.7113″[1]
Apparent magnitude (V) 5.78[2]
Characteristics
Spectral type G1V[3]
B−V color index +0.653±0.005[2]
Astrometry
Radial velocity (Rv)+11.16±0.12[1] km/s
Proper motion (μ) RA: −18.363[1] mas/yr
Dec.: −259.002[1] mas/yr
Parallax (π)39.2946 ± 0.0305[1] mas
Distance83.00 ± 0.06 ly
(25.45 ± 0.02 pc)
Absolute magnitude (MV)3.74±0.04[4]
Details
A
Mass1.16±0.03[5] M☉
Radius1.63±0.04[5] R☉
Luminosity3.03[2] L☉
Surface gravity (log g)4.12±0.03[5] cgs
Temperature5,829±80[5] K
Metallicity [Fe/H]0.10±0.08[5] dex
Rotational velocity (v sin i)1.4 or 3.2[6] km/s
Age6.3±0.9[5] Gyr
B
Mass0.11[7] M☉
Other designations
λ2 For, CD−5°903, Gaia DR2 5062172841616745856, GC 3153, GJ 105.1, HD 16417, HIP 12186, HR 772, SAO 193811, PPM 278138, LTT 1280, NLTT 8516, 2MASS J02365859-3434404[8]
Database references
SIMBADdata
Exoplanet Archivedata
ARICNSdata
Extrasolar Planets
Encyclopaedia		data

λ2 Fornacis, Latinized as Lambda2 Fornacis, is the primary of a binary star system in the southern constellation of Fornax. It is just visible to the naked eye as a dim, yellow-hued point of light with an apparent visual magnitude of 5.78.[2] It is located 83 light years distant from the Sun, based on stellar parallax, and is drifting further away with a radial velocity of +11.1 km/s.[1]

This object is a G-type main-sequence star with a stellar classification of G1V.[3] It is considered a solar analog, being photometrically-similar to the Sun.[9] The star is an estimated 6.3 billion years old with 1.16 times the mass of the Sun and 1.63 times the Sun's radius.[5] It is radiating three times the luminosity of the Sun from its photosphere[2] at an effective temperature of 5,829 K.[5] The abundance of elements with more mass than helium is 55% higher than in the Sun.[4][10]

There is a faint co-moving companion star located to the east of the main star at an angular separation of 45″. This is most likely an M5–M6 class red dwarf with 0.11 times the Sun's mass. The projected separation between the pair is about 1,000 astronomical unit|AU.[7]

Planetary system

Precision Doppler spectroscopy from an intensive 48 night observing campaign on the Anglo-Australian Telescope has revealed the presence of a low-mass extrasolar planet orbiting the star.[11] This object has an orbital period of 17.25 days and an eccentricity of 0.14. It has a minimum (baseline) mass of 16.8 M🜨.[5]

The Lambda2 Fornacis planetary system[5]
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b ≥16.8+1.2
−1.3 M⊕ 		0.14±0.01[11] 17.251+0.002
−0.003 		0.35±0.05 — —

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A. 
  3. ↑ 3.0 3.1 Gray, R. O. et al. (July 2006). "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample". The Astronomical Journal 132 (1): 161–170. doi:10.1086/504637. Bibcode: 2006AJ....132..161G. 
  4. ↑ 4.0 4.1 da Silva, L. et al. (November 2006). "Basic physical parameters of a selected sample of evolved stars". Astronomy and Astrophysics 458 (2): 609–623. doi:10.1051/0004-6361:20065105. Bibcode: 2006A&A...458..609D. 
  5. ↑ 5.00 5.01 5.02 5.03 5.04 5.05 5.06 5.07 5.08 5.09 Nielsen, M. B.; Ball, W. H.; Standing, M. R.; Triaud, A. H. M. J.; Buzasi, D.; Carboneau, L.; Stassun, K. G.; Kane, S. R. et al. (September 2020). "TESS asteroseismology of the known planet host star λ2 Fornacis". Astronomy & Astrophysics 641: A25. doi:10.1051/0004-6361/202037461. ISSN 0004-6361. Bibcode: 2020A&A...641A..25N. 
  6. ↑ Soto, M. G.; Jenkins, J. S. (July 2018). "Spectroscopic Parameters and atmosphEric ChemIstriEs of Stars (SPECIES). I. Code description and dwarf stars catalogue". Astronomy & Astrophysics 615: 28. doi:10.1051/0004-6361/201731533. A76. Bibcode: 2018A&A...615A..76S. 
  7. ↑ 7.0 7.1 Mugrauer, M. et al. (March 2014). "New wide stellar companions of exoplanet host stars". Monthly Notices of the Royal Astronomical Society 439 (1): 1063–1070. doi:10.1093/mnras/stu044. Bibcode: 2014MNRAS.439.1063M. 
  8. ↑ "lam02 For". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=lam02+For. 
  9. ↑ Datson, Juliet et al. (February 2015). "Spectroscopic study of solar twins and analogues". Astronomy & Astrophysics 574: 12. doi:10.1051/0004-6361/201425000. A124. Bibcode: 2015A&A...574A.124D. 
  10. ↑ 10+0.19 = 1.55
  11. ↑ 11.0 11.1 O’Toole, Simon et al. (2009). "A Neptune-mass Planet Orbiting the Nearby G Dwarf HD16417". The Astrophysical Journal 697 (2): 1263–1268. doi:10.1088/0004-637X/697/2/1263. Bibcode: 2009ApJ...697.1263O. 

Coordinates: Sky map 02h 36m 58.6079s, −34° 34′ 40.717″



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