HD 72659
{{short description|Star in the constellation of Hydra}}
{{Starbox begin}}
{{Starbox observe
| epoch = J2000.0
| constell = Hydra
| dec = {{DEC|-01|34|05.5822}}
}}
{{Starbox character
| u-b =
| variable =
}}
{{Starbox astrometry
| radial_v = {{val|-18.29|0.12}}
| prop_mo_ra = {{val|-112.313|0.026}}
| prop_mo_dec = {{val|-96.386|0.018}}
| parallax = 19.2582
| p_error = 0.0271
}}
{{Starbox detail
| mass = {{val|1.07|0.02}}
| radius = {{val|1.38|0.02}}
| luminosity = {{val|2.16|0.01}}
| gravity = {{val|4.19|0.02}}
| temperature = {{val|5956|43|fmt=commas}}
| metal_fe = {{Val|−0.04|0.01}}
| rotation =
| age_gyr = {{val|7.0|0.7}}
}}
{{Starbox catalog
| names = {{odlist | BD=−01°2075 | HD=72659 | HIP=42030 | SAO=136045|Gaia DR2=3073443760538892032|2MASS=J08340320-0134056}}
}}
{{Starbox reference
| Simbad = HD+72659
}}
{{Starbox end}}
HD 72659 is a star in the equatorial constellation of Hydra. With an apparent visual magnitude of 7.46, his yellow-hued star is too faint to be viewed with the naked eye. Parallax measurements provide a distance estimate of 169.4 light years from the Sun, and it has an absolute magnitude of 3.98. The star is drifting closer with a radial velocity of −18.3 km/s.
This is a Sun-like main sequence star with a stellar classification of G2V, indicating that it is generating energy through core hydrogen fusion. It is older than the Sun with an age of about seven billion years, and is spinning with a projected rotational velocity of 5.1 km/s. The star has 7% greater mass than the Sun and a 38% larger radius. It is radiating more than double the Sun's luminosity from its photosphere at an effective temperature of 5,956 K. The metallicity of the stellar atmosphere is similar to the Sun.
Planetary system
An extrasolar planet was discovered orbiting this star in 2003 via the Doppler method. This is a superjovian planet with an eccentric orbit, completing a lap around its host star every {{Convert|3630|days|years|disp=out|abbr=off}}. In 2022, the inclination and true mass of HD 72659 b were measured via astrometry, along with the detection of a second substellar companion, likely a brown dwarf.
{{OrbitboxPlanet begin
| period_unit = year
}}
{{OrbitboxPlanet
| exoplanet = b
| mass = {{val|2.988|2.586|0.098}}
| period = {{val|9.718|0.052|0.043}}
| semimajor = {{val|4.691|0.185|0.202}}
| eccentricity = {{val|0.257|0.014|0.016}}
| inclination = {{val|77.583|39.898|39.755}}
}}
{{OrbitboxPlanet
| exoplanet = c
| mass = {{val|18.806|4.442|4.796}}
| period = {{val|49.850|3.805|3.287}}
| semimajor = {{val|13.959|0.884|0.861}}
| eccentricity = {{val|0.091|0.055|0.048}}
| inclination = {{val|14.279|4.366|2.678}}
}}
{{Orbitbox end}}
See also
References
{{Reflist|refs=
{{Cite Gaia DR3|3073443760538892032}}
{{cite simbad | title=HD 72659 | access-date=2020-01-24 }}
| title=XHIP: An extended hipparcos compilation
| last1=Anderson | first1=E. | last2=Francis | first2=Ch.
| journal=Astronomy Letters | volume=38
| issue=5 | pages=331 | year=2012
| bibcode=2012AstL...38..331A | arxiv=1108.4971
| doi=10.1134/S1063773712050015 | s2cid=119257644 }}
| title=Michigan catalogue of two-dimensional spectral types for the HD Stars
| last1=Houk | first1=N. | last2=Swift | first2=C.
| journal=Michigan Spectral Survey
| volume=5 | year=1999 | bibcode=1999MSS...C05....0H }}
| title=Revising the ages of planet-hosting stars
| url=http://www.aanda.org/articles/aa/full_html/2015/03/aa24951-14/aa24951-14.html
| last1=Bonfanti | first1=A. | last2=Ortolani | first2=S.
| last3=Piotto | first3=G. | last4=Nascimbeni | first4=V.
| display-authors=1 | journal=Astronomy and Astrophysics
| year=2015 | volume=575 | at=A18
| arxiv=1411.4302 | bibcode=2015A&A...575A..18B
| doi=10.1051/0004-6361/201424951 | s2cid=54555839
}}
| title=Seven New Keck Planets Orbiting G and K Dwarfs
| last1=Butler | first1=R. Paul | last2=Marcy | first2=Geoffrey W.
| last3=Vogt | first3=Steven S. | last4=Fischer | first4=Debra A.
| last5=Henry | first5=Gregory W. | last6=Laughlin | first6=Gregory
| last7=Wright | first7=Jason T. | display-authors=1
| journal=The Astrophysical Journal
| date=2003 | volume=582 | issue=1 | pages=455–466
| doi=10.1086/344570 | bibcode=2003ApJ...582..455B
| citeseerx=10.1.1.7.6988 | s2cid=17608922 }}
| title=Abundances in the Local Region II: F, G, and K Dwarfs and Subgiants
| last1=Luck | first1=R. Earle
| journal=The Astronomical Journal
| volume=153 | issue=1 | id=21 | pages=19 | date=January 2017
| bibcode=2017AJ....153...21L | arxiv=1611.02897
| doi=10.3847/1538-3881/153/1/21 | s2cid=119511744 | doi-access=free }}
{{cite journal |last1=Feng |first1=Fabo |last2=Butler |first2=R. Paul |display-authors=etal |date=August 2022 |title=3D Selection of 167 Substellar Companions to Nearby Stars |journal=The Astrophysical Journal Supplement Series |volume=262 |issue=21 |page=21 |doi=10.3847/1538-4365/ac7e57 |arxiv=2208.12720 |bibcode=2022ApJS..262...21F|s2cid=251864022 |doi-access=free }}
}}
External links
{{Sky|08|34|03.1895|-|01|34|05.583|168}}
{{Stars of Hydra}}
{{DEFAULTSORT:HD 72659}}
Category:G-type main-sequence stars
Category:Planetary systems with one confirmed planet
Category:Hydra (constellation)