BD+00 316
{{Short description|F-class main sequence star in the constellation Cetus}}
{{Starbox begin
| name = BD+00 316 / Mpingo
}}
{{Starbox observe
| epoch = J2000
| constell = Cetus
| ra = {{RA|01|57|03.204}}{{Cite Gaia DR3|2507901914613201024}}
| appmag_v = 10.56{{Cite journal
| title=The Tycho-2 catalogue of the 2.5{{nbsp}}million brightest stars
| last1=Høg | first1=E. | last2=Fabricius | first2=C.
| last3=Makarov | first3=V. V. | last4=Urban | first4=S.
| last5=Corbin | first5=T. | last6=Wycoff | first6=G.
| last7=Bastian | first7=U. | last8=Schwekendiek | first8=P.
| last9=Wicenec | first9=A. | display-authors=1
| journal=Astronomy and Astrophysics
| volume=355 | page=L27 | date=2000
| bibcode=2000A&A...355L..27H | doi=10.1888/0333750888/2862
| isbn=978-0333750889 }}
}}
{{Starbox character
| type=
}}
{{Starbox astrometry
| radial_v = 7.690{{±|0.004}}{{Cite Gaia DR2|2507901914613005056}}
| prop_mo_ra = 23.418
| prop_mo_dec = −6.844
| parallax = 2.8158
| p_error = 0.0265
}}
{{Starbox detail
| mass = 1.53{{±|0.07|0.06}}
| radius = 2.17{{±|0.18|0.10}}
| gravity = 3.944{{±|0.036|0.050}}
| luminosity =
| temperature = 6,050{{±|100}}
| metal_fe = 0.15{{±|0.07}}
| rotation =
| rotational_velocity = 7.8{{±|0.3}}
| age_gyr = 3.6{{±|1.6|1.0}}
}}
{{Starbox catalog
| names = {{odlist | name=Mpingo | BD=+00 316 | WASP=71 | TYC=30-116-1 | 2MASS=J01570320+0045318 | Gaia DR2=2507901914613005056 }}
}}
{{Starbox reference
| Simbad = BD-07 436
}}
{{Starbox end}}
BD+00 316 is an ordinary star with a close-orbiting planetary companion in the equatorial constellation of Cetus. It is also known as WASP-71 since 2019; BD+00 316 is the stellar identifier from the Bonner Durchmusterung catalogue. With an apparent visual magnitude of 10.56, it is too faint to be visible to the naked eye. This star is located at a distance of 1,160 light-years based on parallax measurements, and is drifting further away with a heliocentric radial velocity of 7.7 km/s.
This is classified as an F-type star with a stellar classification of F8. It is more than double the diameter of the Sun with 1.5 times the Sun's mass. The star is younger than the Sun at about 3.6 billion years, yet is already evolving away from the main sequence. BD+00 316 is enriched in heavy elements, having 140% of the solar abundance of iron. Imaging surveys in 2015 and 2020 failed to find any stellar companions for BD+00 316.{{citation|arxiv=1506.05456|title=A Lucky Imaging search for stellar sources near 74 transit hosts|year=2015|doi=10.1051/0004-6361/201526525|last1=Wöllert|first1=Maria|last2=Brandner|first2=Wolfgang|journal=Astronomy & Astrophysics|volume=579|pages=A129|bibcode=2015A&A...579A.129W |s2cid=118903879}}{{citation|arxiv=2001.08224|title=A multiplicity study of transiting exoplanet host stars. I. High-contrast imaging with VLT/SPHERE|year=2020|doi=10.1051/0004-6361/201937127|last1=Bohn|first1=A. J.|last2=Southworth|first2=J.|last3=Ginski|first3=C.|last4=Kenworthy|first4=M. A.|last5=Maxted|first5=P. F. L.|last6=Evans|first6=D. F.|journal=Astronomy & Astrophysics|volume=635|pages=A73|bibcode=2020A&A...635A..73B |s2cid=210861118}}
The star was named Mpingo by Tanzanian amateur astronomers in 2020 as part of the NameExoWorlds contest, after the mpingo tree (Dalbergia melanoxylon) whose wood is a type of ebony used in musical instruments.
Planetary system
In 2012 a transiting superjovian planet, designated component b, was detected on a tight, circular orbit.{{citation|arxiv=1211.3045|title=WASP-71b: a bloated hot Jupiter in a 2.9-day, prograde orbit around an evolved F8 star|year=2013|doi=10.1051/0004-6361/201220727|last1=Smith|first1=A. M. S.|last2=Anderson|first2=D. R.|last3=Bouchy|first3=F.|last4=Collier Cameron|first4=A.|last5=Doyle|first5=A. P.|last6=Fumel|first6=A.|last7=Gillon|first7=M.|last8=Hébrard|first8=G.|last9=Hellier|first9=C.|last10=Jehin|first10=E.|last11=Lendl|first11=M.|last12=Maxted|first12=P. F. L.|last13=Moutou|first13=C.|last14=Pepe|first14=F.|last15=Pollacco|first15=D.|last16=Queloz|first16=D.|last17=Santerne|first17=A.|last18=Segransan|first18=D.|last19=Smalley|first19=B.|last20=Southworth|first20=J.|last21=Triaud|first21=A. H. M. J.|last22=Udry|first22=S.|last23=West|first23=R. G.|journal=Astronomy & Astrophysics|volume=552|pages=A120|bibcode=2013A&A...552A.120S |s2cid=118575479}} The planetary orbit is well aligned with the equatorial plane of the star, the misalignment angle being equal to −1.9{{±|7.1|7.5}}°.{{citation|arxiv=1610.00600|title=Rossiter–McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems|year=2016|doi=10.1093/mnras/stw2316|last1=Brown|first1=D. J. A.|last2=Triaud|first2=A. H. M. J.|last3=Doyle|first3=A. P.|last4=Gillon|first4=M.|last5=Lendl|first5=M.|last6=Anderson|first6=D. R.|last7=Collier Cameron|first7=A.|last8=Hébrard|first8=G.|last9=Hellier|first9=C.|last10=Lovis|first10=C.|last11=Maxted|first11=P. F. L.|last12=Pepe|first12=F.|last13=Pollacco|first13=D.|last14=Queloz|first14=D.|last15=Smalley|first15=B.|journal=Monthly Notices of the Royal Astronomical Society|volume=464|issue=1 |pages=810–839|doi-access=free |bibcode=2017MNRAS.464..810B |s2cid=53497449}} Its equilibrium temperature is 2,016.1{{±|67.0|52.5}} K.
The planet was named Tanzanite by Tanzanian amateur astronomers in 2020 as part of the NameExoWorlds contest, after the mineral also known as tanzanite.[https://wasp-planets.net/2020/01/05/the-iau-announces-names-for-wasp-exoplanets/ The IAU announces names for WASP exoplanets]
{{OrbitboxPlanet begin
| name = WASP-71
}}
{{OrbitboxPlanet
| exoplanet = b (Tanzanite)
| mass = 2.14{{±|0.08}}
| radius = 1.35{{±|0.13|0.07}}
| semimajor = 0.0460{{±|0.0006}}
| period = 2.903676{{±|0.000008}}
| inclination = 85.8{{±|2.4|2.1}}
}}
{{Orbitbox end}}
References
{{Reflist|refs=
{{Cite constellation|WASP-71}}
{{cite simbad |title=BD+00 316}}
}}
{{Sky|01|57|03.2041|+|00|45|31.8789}}
{{Cetus}}
{{DEFAULTSORT:BD+00 316}}
Category:Planetary systems with one confirmed planet
Category:Planetary transit variables