HAT-P-38#Planetary system

{{Short description|Star in the constellation Traingulum.}}

{{Starbox begin

| name = HAT-P-38/Horna

}}

{{Starbox observe

| epoch = J2000.0 (ICRS)

| constell = Triangulum

| ra = {{RA|02|21|31.98035}}

| dec = {{DEC|+32|14|46.0933}}

| appmag_v = 12.51{{±|0.02}}

}}

{{Starbox character

| class = G5

| b-v = +0.83

}}

{{Starbox astrometry

| radial_v = −19.85{{±|0.73}}

| parallax = 3.9747

| p_error = 0.0134

| parallax_footnote =

| prop_mo_ra = +47.671

| prop_mo_dec = −21.594

| pm_footnote =

}}

{{Starbox detail

| mass = 0.886{{±|0.044}}

| radius = 1.01{{±|0.07|0.05}}

| luminosity = 0.6772{{±|0.007|0.008}}

| gravity = 4.46{{±|0.08}}

| temperature = 5,330{{±|100}}

| metal_fe = +0.06{{±|0.10}}

| rotational_velocity = 0.4{{±|0.5}}

| age_gyr = 10.1{{±|3.9|4.8}}

}}

{{Starbox catalog

| names = {{odlist | name=Horna | GSC=02314-00559 | TIC=285272237 | TOI=3681 }}

}}

{{Starbox reference

| Simbad = HAT-P-38

| NSTED = HAT-P-38

}}

{{Starbox end}}

HAT-P-38, formally named Horna, is a star located in the northern constellation Triangulum. It has an apparent magnitude of 12.51, making it readily visible in amateur telescopes but not to the naked eye. The object is located relatively far at a distance of 821 light-years based on Gaia DR3 parallax measurements, but it is drifting closer with a spectroscopic radial velocity of {{val|-19.85|ul=km/s}}.

HAT-P-38 has a stellar classification of G5, indicating that it is a G-type star. It has 88.6% the mass of the Sun and 101% the radius of the Sun. It radiates 67.72% the luminosity of the Sun from its photosphere at an effective temperature of {{val|5330|ul=K|fmt=commas}}, giving it a yelllowish-orange hue. HAT-P-38 is slightly metal enriched with an iron abundance 115% that of the Sun's. It is estimated to be approximately 10.1 billion years old, which is more than twice the age of the Sun. It spins modestly with a projected rotational velocity of {{val|0.4|ul=km/s}}.

Planetary system

In 2012, a hot Saturn was detected on a tight 4-day orbit via the transit method; the planet has a similar mass and radius to Saturn. A 2017 paper comparing HAT-P-38b and WASP-67b found that there was water vapor in the planet's atmosphere. HAT-P-38b had a higher water vapor abundance compared to the latter, indicating that the planet is free of clouds or hazes in its upper atmosphere.

In 2019, the system was selected for the second NameExoWorlds campaign for Finland as part of the IAU's 100th anniversary. The approved name for the star is Horna, which is hell or the underworld from Finnic mythology..

{{Orbitbox planet begin

| name = HAT-P-38

| table_ref =

}}

{{Orbitbox planet

| exoplanet = b (Hiisi)

| mass = 0.267{{±|0.020}}

| semimajor = 0.05231{{±|0.00085|0.00089}}

| period = 4.6403288{{±|0.0000011}}

| eccentricity = <0.055

| inclination = 88.3{{±|0.7}}

| radius = 0.825{{±|0.092|0.063}}

}}

{{Orbitbox end}}

References

{{reflist||refs=

{{Cite DR3|324889227693298560}}

{{cite journal |last1=Zacharias |first1=N. |last2=Finch |first2=C. T. |last3=Girard |first3=T. M. |last4=Henden |first4=A. |last5=Bartlett |first5=J. L.|author5-link=Jennifer Bartlett (astronomer) |last6=Monet |first6=D. G. |last7=Zacharias |first7=M. I. |title=The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4) |journal=The Astronomical Journal |date=January 14, 2013 |volume=145 |issue=2 |pages=44 |doi=10.1088/0004-6256/145/2/44 |issn=0004-6256|arxiv=1212.6182 |bibcode=2013AJ....145...44Z |s2cid=119299381 |doi-access = free}}

{{cite journal |last1=Luo |first1=A. -L. |last2=Zhao |first2=Y. -H. |last3=Zhao |first3=G. |title=VizieR Online Data Catalog: LAMOST DR4 catalogs (Luo+, 2018) |journal=VizieR Online Data Catalog |date=August 2018 |volume=5153 |pages=V/153 |bibcode=2018yCat.5153....0L}}

{{cite journal | display-authors=1 | last1=Sato | first1=Bun'ei | last2=Hartman | first2=Joel D. | last3=Bakos | first3=Gáspár Á. | last4=Béky | first4=Bence | last5=Torres | first5=Guillermo | last6=Latham | first6=David W. | last7=KovÁcs | first7=Géza | last8=Csubry | first8=Zoltán | last9=Penev | first9=Kaloyan | last10=Noyes | first10=Robert W. | last11=Buchhave | first11=Lars A. | last12=Quinn | first12=Samuel N. | last13=Everett | first13=Mark | last14=Esquerdo | first14=Gilbert A. | last15=Fischer | first15=Debra A. | last16=Howard | first16=Andrew W. | last17=Johnson | first17=John A. | last18=Marcy | first18=Geoff W. | last19=Sasselov | first19=Dimitar D. | last20=Szklenár | first20=Tamás | last21=Lázár | first21=József | last22=Papp | first22=István | last23=Sári | first23=Pál | title=HAT-P-38b: A Saturn-Mass Planet Transiting a Late G Star | journal=Publications of the Astronomical Society of Japan | volume=64 | issue=5 | date=October 25, 2012 | issn=2053-051X | doi=10.1093/pasj/64.5.97 | s2cid = 119186118 | page= 97| bibcode = 2012PASJ...64...97S | arxiv = 1201.5075 | doi-access = free}}

{{cite journal | display-authors = 1 | last1=Bonomo | first1=A. S. | last2=Desidera | first2=S. | last3=Benatti | first3=S. | last4=Borsa | first4=F. | last5=Crespi | first5=S. | last6=Damasso | first6=M. | last7=Lanza | first7=A. F. | last8=Sozzetti | first8=A. | last9=Lodato | first9=G. | last10=Marzari | first10=F. | last11=Boccato | first11=C. | last12=Claudi | first12=R. U. | last13=Cosentino | first13=R. | last14=Covino | first14=E. | last15=Gratton | first15=R. | last16=Maggio | first16=A. | last17=Micela | first17=G. | last18=Molinari | first18=E. | last19=Pagano | first19=I. | last20=Piotto | first20=G. | last21=Poretti | first21=E. | last22=Smareglia | first22=R. | last23=Affer | first23=L. | last24=Biazzo | first24=K. | last25=Bignamini | first25=A. | last26=Esposito | first26=M. | last27=Giacobbe | first27=P. | last28=Hébrard | first28=G. | last29=Malavolta | first29=L. | last30=Maldonado | first30=J. | last31=Mancini | first31=L. | last32=Martinez Fiorenzano | first32=A. | last33=Masiero | first33=S. | last34=Nascimbeni | first34=V. | last35=Pedani | first35=M. | last36=Rainer | first36=M. | last37=Scandariato | first37=G. | title=The GAPS Programme with HARPS-N at TNG: XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets⋆ | journal=Astronomy & Astrophysics | volume=602 | date=June 2017 | issn=0004-6361 | doi=10.1051/0004-6361/201629882 | s2cid = 118923163 | page=A107 | bibcode = 2017A&A...602A.107B | arxiv = 1704.00373 | doi-access = free}}

{{cite journal | last1=Magrini | first1=L. | last2=Danielski | first2=C. | last3=Bossini | first3=D. | last4=Rainer | first4=M. | last5=Turrini | first5=D. | last6=Benatti | first6=S. | last7=Brucalassi | first7=A. | last8=Tsantaki | first8=M. | last9=Delgado Mena | first9=E. | last10=Sanna | first10=N. | last11=Biazzo | first11=K. | last12=Campante | first12=T. L. | last13=Van der Swaelmen | first13=M. | last14=Sousa | first14=S. G. | last15=Hełminiak | first15=K. G. | last16=Neitzel | first16=A. W. | last17=Adibekyan | first17=V. | last18=Bruno | first18=G. | last19=Casali | first19=G. | title=Ariel stellar characterisation: I. Homogeneous stellar parameters of 187 FGK planet host stars: Description and validation of the method | journal=Astronomy & Astrophysics | volume=663 | date=July 2022 | issn=0004-6361 | doi=10.1051/0004-6361/202243405 | s2cid = 248240168 | page=A161 | bibcode = 2022A&A...663A.161M | arxiv = 2204.08825 | doi-access = free}}

{{cite journal | display-authors = 1 | last1 = Stassun | first1 = Keivan G. | last2 = Oelkers | first2 = Ryan J. | last3 = Paegert | first3 = Martin | last4 = Torres | first4 = Guillermo | last5 = Pepper | first5 = Joshua | last6 = Lee | first6 = Nathan De | last7 = Collins | first7 = Kevin | last8 = Latham | first8 = David W. | last9 = Muirhead | first9 = Philip S. | last10 = Chittidi | first10 = Jay | last11 = Rojas-Ayala | first11 = Bárbara | last12 = Fleming | first12 = Scott W. | last13 = Rose | first13 = Mark E. | last14 = Tenenbaum | first14 = Peter | last15 = Ting | first15 = Eric B. | last16 = Kane | first16 = Stephen R. | last17 = Barclay | first17 = Thomas | last18 = Bean | first18 = Jacob L. | last19 = Brassuer | first19 = C. E. | last20 = Charbonneau | first20 = David | last21 = Ge | first21 = Jian | last22 = Lissauer | first22 = Jack J. | last23 = Mann | first23 = Andrew W. | last24 = McLean | first24 = Brian | last25 = Mullally | first25 = Susan | last26 = Narita | first26 = Norio | last27 = Plavchan | first27 = Peter | last28 = Ricker | first28 = George R. | last29 = Sasselov | first29 = Dimitar | last30 = Seager | first30 = S. | last31 = Sharma | first31 = Sanjib | last32 = Shiao | first32 = Bernie | last33 = Sozzetti | first33 = Alessandro | last34 = Stello | first34 = Dennis | last35 = Vanderspek | first35 = Roland | last36 = Wallace | first36 = Geoff | last37 = Winn | first37 = Joshua N. | title = The Revised TESS Input Catalog and Candidate Target List | journal = The Astronomical Journal | date = 9 September 2019 | volume = 158 | issue = 4 | page = 138 | eissn = 1538-3881 | doi = 10.3847/1538-3881/ab3467 | bibcode = 2019AJ....158..138S | arxiv = 1905.10694 | s2cid = 166227927 | hdl = 1721.1/124721 | hdl-access = free | doi-access = free}}

{{cite journal | display-authors=1 | last1=Kokori | first1=A. | last2=Tsiaras | first2=A. | last3=Edwards | first3=B. | last4=Rocchetto | first4=M. | last5=Tinetti | first5=G. | last6=Bewersdorff | first6=L. | last7=Jongen | first7=Y. | last8=Lekkas | first8=G. | last9=Pantelidou | first9=G. | last10=Poultourtzidis | first10=E. | last11=Wünsche | first11=A. | last12=Aggelis | first12=C. | last13=Agnihotri | first13=V. K. | last14=Arena | first14=C. | last15=Bachschmidt | first15=M. | last16=Bennett | first16=D. | last17=Benni | first17=P. | last18=Bernacki | first18=K. | last19=Besson | first19=E. | last20=Betti | first20=L. | last21=Biagini | first21=A. | last22=Brandebourg | first22=P. | last23=Bretton | first23=M. | last24=Brincat | first24=S. M. | last25=Caló | first25=M. | last26=Campos | first26=F. | last27=Casali | first27=R. | last28=Ciantini | first28=R. | last29=Crow | first29=M. V. | last30=Dauchet | first30=B. | last31=Dawes | first31=S. | last32=Deldem | first32=M. | last33=Deligeorgopoulos | first33=D. | last34=Dymock | first34=R. | last35=Eenmäe | first35=T. | last36=Evans | first36=P. | last37=Esseiva | first37=N. | last38=Falco | first38=C. | last39=Ferratfiat | first39=S. | last40=Fowler | first40=M. | last41=Futcher | first41=S. R. | last42=Gaitan | first42=J. | last43=Horta | first43=F. Grau | last44=Guerra | first44=P. | last45=Hurter | first45=F. | last46=Jones | first46=A. | last47=Kang | first47=W. | last48=Kiiskinen | first48=H. | last49=Kim | first49=T. | last50=Laloum | first50=D. | last51=Lee | first51=R. | last52=Lomoz | first52=F. | last53=Lopresti | first53=C. | last54=Mallonn | first54=M. | last55=Mannucci | first55=M. | last56=Marino | first56=A. | last57=Mario | first57=J.-C. | last58=Marquette | first58=J.-B. | last59=Michelet | first59=J. | last60=Miller | first60=M. | last61=Mollier | first61=T. | last62=Molina | first62=D. | last63=Montigiani | first63=N. | last64=Mortari | first64=F. | last65=Morvan | first65=M. | last66=Mugnai | first66=L. V. | last67=Naponiello | first67=L. | last68=Nastasi | first68=A. | last69=Neito | first69=R. | last70=Pace | first70=E. | last71=Papadeas | first71=P. | last72=Paschalis | first72=N. | last73=Pereira | first73=C. | last74=Perroud | first74=V. | last75=Phillips | first75=M. | last76=Pintr | first76=P. | last77=Pioppa | first77=J.-B. | last78=Popowicz | first78=A. | last79=Raetz | first79=M. | last80=Regembal | first80=F. | last81=Rickard | first81=K. | last82=Roberts | first82=M. | last83=Rousselot | first83=L. | last84=Rubia | first84=X. | last85=Savage | first85=J. | last86=Sedita | first86=D. | last87=Shave-Wall | first87=D. | last88=Sioulas | first88=N. | last89=Školník | first89=V. | last90=Smith | first90=M. | last91=St-Gelais | first91=D. | last92=Stouraitis | first92=D. | last93=Strikis | first93=I. | last94=Thurston | first94=G. | last95=Tomacelli | first95=A. | last96=Tomatis | first96=A. | last97=Trevan | first97=B. | last98=Valeau | first98=P. | last99=Vignes | first99=J.-P. | last100=Vora | first100=K. | last101=Vrašťák | first101=M. | last102=Walter | first102=F. | last103=Wenzel | first103=B. | last104=Wright | first104=D. E. | last105=Zíbar | first105=M. | title=ExoClock Project. II. A Large-scale Integrated Study with 180 Updated Exoplanet Ephemerides | journal=The Astrophysical Journal Supplement Series | volume=258 | issue=2 | date=February 1, 2022 | issn=0067-0049 | doi=10.3847/1538-4365/ac3a10 | doi-access=free | page=40 | bibcode = 2022ApJS..258...40K | arxiv = 2204.08825 | s2cid = 248240168}}

{{cite journal | last1=Bruno | first1=Giovanni | last2=Lewis | first2=Nikole K. | last3=Stevenson | first3=Kevin B. | last4=Filippazzo | first4=Joseph | last5=Hill | first5=Matthew | last6=Fraine | first6=Jonathan D. | last7=Wakeford | first7=Hannah R. | last8=Deming | first8=Drake | last9=Kilpatrick | first9=Brian | last10=Line | first10=Michael R. | last11=Morley | first11=Caroline V. | last12=Collins | first12=Karen A. | last13=Conti | first13=Dennis M. | last14=Garlitz | first14=Joseph | last15=Rodriguez | first15=Joseph E. | title=A Comparative Study of WASP-67 b and HAT-P-38 b from WFC3 Data | journal=The Astronomical Journal | volume=155 | issue=2 | date=February 1, 2018| issn=0004-6256 | doi=10.3847/1538-3881/aaa0c7 | doi-access=free | page=55 | bibcode = 2018AJ....155...55B | arxiv = 1712.03384}}

{{Cite web|url=http://www.nameexoworlds.iau.org/final-results|title=Approved names|website=NameExoworlds|language=en|access-date=2020-01-02}}

{{Cite constellation|HAT-P-38}}

{{cite web |url=https://www.space.com/37102-hot-jupiter-alien-planets-cloudy-clear.html|last1=Wall |first1=Mike |title=Surprise! Giant Exoplanet 'Cousins' Have Different Atmospheres |website=Space.com |language=en |date=6 June 2017}}

}}

{{Stars of Triangulum}}

Category:G-type main-sequence stars

Category:Planetary systems with one confirmed planet

3681

00285272237

Horna

Category:Triangulum