WASP-75

{{Starbox observe

| epoch = J2000

| constell = Aquarius

| ra = {{RA|22|49|32.5676}}

| dec = {{DEC|-10|40|31.926}}

| appmag_v = 11.299

}}

{{Starbox character

| type=Main sequence{{cite thesis |bibcode=2015PhDT.........5I |date=2015 |title=Analysis of Angular Momentum in Planetary Systems and Host Stars |last1=Irwin |first1=Stacy Ann }}

| class = F9

}}

{{Starbox astrometry

| radial_v = 2.7{{±|0.8}}

| prop_mo_ra = 45.892

| prop_mo_dec = 15.428

| parallax = 3.3387

| p_error = 0.0202

| parallax_footnote = {{cite Gaia DR3|2605161444735454464}}

}}

{{Starbox detail

| source = {{citation|arxiv=1711.06377|year=2017|doi=10.3847/1538-3881/aa9b83|last1=Petigura|first1=Erik A.|last2=Crossfield|first2=Ian J. M.|last3=Isaacson|first3=Howard|last4=Beichman|first4=Charles A.|last5=Christiansen|first5=Jessie L.|last6=Dressing|first6=Courtney D.|last7=Fulton|first7=Benjamin J.|last8=Howard|first8=Andrew W.|last9=Kosiarek|first9=Molly R.|last10=Lépine|first10=Sébastien|last11=Schlieder|first11=Joshua E.|last12=Sinukoff|first12=Evan|last13=Yee|first13=Samuel W.|title=Planet Candidates from K2 Campaigns 5–8 and Follow-up Optical Spectroscopy|journal=The Astronomical Journal|volume=155|page=21|s2cid=55674757 |doi-access=free }}

| mass = 1.18

| radius = 1.39

| gravity = 4.233

| luminosity = 1.1{{±|0.01}}{{citation |arxiv=1511.01744 |doi=10.1051/0004-6361/201527297 |title=Age consistency between exoplanet hosts and field stars |year=2016 |last1=Bonfanti |first1=A. |last2=Ortolani |first2=S. |last3=Nascimbeni |first3=V. |journal=Astronomy & Astrophysics |volume=585 |pages=A5 |bibcode=2016A&A...585A...5B |s2cid=53971692 }}

| temperature = 6090

| metal_fe = 0.07{{±|0.09}}

| rotation = 11.2{{±|1.5}} d

| rotational_velocity =

| age_gyr = 2.9{{±|0.2}}

}}

{{Starbox catalog

| names = {{odlist | 2MASS=J22493256-1040320 | BD=−11 5929 | EPIC=206154641 | Gaia DR3=2605161444735454464 | GSC=05816-01135 | K2=40 }}

}}

{{Starbox reference

| Simbad = BD-11+5929

}}

WASP-75 is a F-type main-sequence star about 980 light-years away. The star is much younger than the Sun at approximately {{val|2.9|0.2|u=billion years}}. WASP-75 is similar to the Sun in its concentration of heavy elements.

Planetary system

In 2013 a transiting hot Jupiter planet b was detected on a tight, circular orbit,{{citation |arxiv=1307.6532 |doi=10.1051/0004-6361/201322314 |title=Discovery of WASP-65b and WASP-75b: Two hot Jupiters without highly inflated radii |year=2013 |last1=Gómez Maqueo Chew |first1=Y. |last2=Faedi |first2=F. |last3=Pollacco |first3=D. |last4=Brown |first4=D. J. A. |last5=Doyle |first5=A. P. |last6=Collier Cameron |first6=A. |last7=Gillon |first7=M. |last8=Lendl |first8=M. |last9=Smalley |first9=B. |last10=Triaud |first10=A. H. M. J. |last11=West |first11=R. G. |last12=Wheatley |first12=P. J. |last13=Busuttil |first13=R. |last14=Liebig |first14=C. |last15=Anderson |first15=D. R. |last16=Armstrong |first16=D. J. |last17=Barros |first17=S. C. C. |last18=Bento |first18=J. |last19=Bochinski |first19=J. |last20=Burwitz |first20=V. |last21=Delrez |first21=L. |last22=Enoch |first22=B. |last23=Fumel |first23=A. |last24=Haswell |first24=C. A. |last25=Hébrard |first25=G. |last26=Hellier |first26=C. |last27=Holmes |first27=S. |last28=Jehin |first28=E. |last29=Kolb |first29=U. |last30=Maxted |first30=P. F. L. |journal=Astronomy & Astrophysics |volume=559 |pages=A36 |bibcode=2013A&A...559A..36G |s2cid=1008674 |display-authors=29 }} and the planet was confirmed in 2018.{{citation |arxiv=1802.02132 |doi=10.1088/1538-3873/aaa33e |title=An Analysis of Transiting Hot Jupiters Observed with K2: WASP-55b and WASP-75b |year=2018 |last1=Clark |first1=B. J. M. |last2=Anderson |first2=D. R. |last3=Hellier |first3=C. |last4=Turner |first4=O. D. |last5=Močnik |first5=T. |journal=Publications of the Astronomical Society of the Pacific |volume=130 |issue=985 |page=034401 |bibcode=2018PASP..130c4401C |s2cid=119077382 }} Its equilibrium temperature is {{val|1688|fmt=commas|u=K}}.

{{OrbitboxPlanet begin

| name = WASP-75

| table_ref ={{citation|arxiv=1908.08548|year=2019|title=Estimation of singly-transiting K2 planet periods with Gaia parallaxess|doi=10.1093/mnras/stz2348|last1=Sandford|first1=Emily|last2=Espinoza|first2=Néstor|last3=Brahm|first3=Rafael|last4=Jordán|first4=Andrés|journal=Monthly Notices of the Royal Astronomical Society|volume=489|issue=3|pages=3149–3161|doi-access=free |bibcode=2019MNRAS.489.3149S|s2cid=201645337}}

}}

{{OrbitboxPlanet

| exoplanet = b

| mass = 1.08{{±|0.05}}

| radius = 1.31{{±|0.02}}

| semimajor = 0.0377{{±|0.0006}}

| period =2.484193

| eccentricity = <0.1

| inclination=81.96{{±|0.02}}

}}