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HD 99109

Coordinates:Sky map11h 24m 17.358s, −01° 31′ 44.674″
From Wikipedia, the free encyclopedia
Star in the constellation Leo
HD 99109 / Shama
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationLeo
Right ascension11h 24m 17.359s[1]
Declination–01° 31′ 44.67″[1]
Apparent magnitude (V)+9.10[2]
Characteristics
Spectral typeG8/K0IV[3]
B−Vcolor index0.874±0.002[2]
Astrometry
Radial velocity (Rv)+33.060±0.0025[4] km/s
Proper motion (μ)RA: −178.689mas/yr[1]
Dec.: −159.528mas/yr[1]
Parallax (π)18.178±0.017 mas[1]
Distance179.4 ± 0.2 ly
(55.01 ± 0.05 pc)
Absolute magnitude (MV)5.62[2]
Details
Mass0.93±0.02[5] M
Radius0.90±0.03[5] R
Luminosity0.56±0.02[5] L
Surface gravity (log g)4.49±0.03[5] cgs
Temperature5,270±24[5] K
Metallicity [Fe/H]0.315±0.030[6] dex
Rotational velocity (v sin i)1.86±0.50[6] km/s
Age6±3 Gyr[5]
≥ 12.2[7] Gyr
Other designations
Shama,BD−00°2437,HD 99109,HIP 55664,SAO 138182[8]
Database references
SIMBADdata

HD 99109 is an orange-huedstar with anexoplanetary companion in theconstellation ofLeo. It has anabsolute visual magnitude of +9.10,[2] which is too faint to be visible to the naked eye. The distance to this system is 179 light-years based onparallax, and it is drifting further away with aradial velocity of +33 km/s.[1] The star is one and half degrees away from thecelestial equator to the south.

Thestellar classification of this star is G8/K0IV,[3] matching alate G orearlyK-typesubgiant star. It appears to be past the end of itsmain sequence lifetime, having exhausted the supply of hydrogen at itscore.[7] The star is 93% as massive as the Sun and has 90% of the Sun's radius.[5] It is spinning with aprojected rotational velocity of ~2 km/s[6] and has over twice the abundance ofiron relative tohydrogen than the Sun. The star is radiating 56% of the Sun's luminosity from itsphotosphere at aneffective temperature of 5,270 K.[5] As of 2006, oneextrasolar planet has been confirmed to be orbiting the star.[6]

The star HD 99109 is namedShama. The name was selected in theNameExoWorlds campaign byPakistan, during the 100th anniversary of theIAU. Shama (شمع) is anUrdu literary term meaning a smalllamp orflame. The exoplanet companion is calledPerwana, meaning 'moth' in Urdu, alluding to the eternal love of an object circling a source of light.[9][10]

Planetary system

[edit]

The planet HD 99109 b has an orbit comparable in eccentricity to the planetMars in theSolar System but has a mass at least half that ofJupiter. Stability analysis reveals that Earth-size planets could have stable orbits in the planet'sTrojan points, located 60 degrees ahead and behind the planet's position in its orbit.[7]

The HD 99109 planetary system[6]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b / Perwana>0.502 ± 0.070 MJ1.105 ± 0.065439.3 ± 5.60.09 ± 0.16

References

[edit]
  1. ^abcdeVallenari, 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 atVizieR.
  2. ^abcdAnderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5): 331.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.S2CID 119257644.
  3. ^abHouk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars".Michigan Spectral Survey.5.Bibcode:1999MSS...C05....0H.
  4. ^Soubiran, C.; et al. (2018). "Gaia Data Release 2. The catalogue of radial velocity standard stars".Astronomy and Astrophysics.616: A7.arXiv:1804.09370.Bibcode:2018A&A...616A...7S.doi:10.1051/0004-6361/201832795.S2CID 52952408.
  5. ^abcdefghBonfanti, A.; Ortolani, S.; Nascimbeni, V. (2016). "Age consistency between exoplanet hosts and field stars".Astronomy & Astrophysics.585: 14.arXiv:1511.01744.Bibcode:2016A&A...585A...5B.doi:10.1051/0004-6361/201527297.S2CID 53971692. A5.
  6. ^abcdeButler, R. P.; et al. (2006). "Catalog of Nearby Exoplanets".The Astrophysical Journal.646 (1):505–522.arXiv:astro-ph/0607493.Bibcode:2006ApJ...646..505B.doi:10.1086/504701.S2CID 119067572.
  7. ^abcSchwarz, R.; et al. (November 2007)."Survey of the stability region of hypothetical habitable Trojan planets".Astronomy & Astrophysics.474 (3):1023–1029.Bibcode:2007A&A...474.1023S.doi:10.1051/0004-6361:20077994.:HD 93083,HD 17051,HD 28185,HD 27442,HD 188015, HD 99109,HD 221287
  8. ^"HD 99109".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2015-12-21.
  9. ^"Approved names".NameExoworlds. IAU. Retrieved2020-01-02.
  10. ^"International Astronomical Union | IAU".www.iau.org. Retrieved2020-01-02.


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