HAT-P-30#Planetary system

{{Starbox observe

| epoch = J2000

| constell = Hydra

| ra = {{RA|08|15|47.9802}}

| dec = {{DEC|+05|50|12.351}}

| appmag_v = 10.35

}}

{{Starbox character

| type=main sequence

| class = G0

}}

{{Starbox astrometry

| radial_v = 44.14

| prop_mo_ra = −17.231

| prop_mo_dec = +23.875

| parallax = 4.8037

| p_error = 0.0099

| parallax_footnote = {{cite Gaia DR3|3096441729861716224}}

}}

{{Starbox detail

| mass = 1.175{{±|0.025}}

| radius = 1.314{{±|0.015}}

| gravity = 4.270{{±|0.007}}

| luminosity = 2.37{{±|0.01}}

| temperature = 6,252{{±|100}}

| metal_fe = −0.079{{±|0.079}}

| rotation =

| rotational_velocity = 3.6{{±|0.4}}

| age_gyr = {{val|4.1|0.6}}

}}

{{Starbox catalog

| names = {{odlist|BD=+06 1909|GSC=00208-00722|2MASS=J08154797+0550121|TOI=490|WASP=51}}

}}

{{Starbox reference

| Simbad = HAT-P-30

}}

HAT-P-30, also known as WASP-51, is the primary of a binary star system about 700 light-years away. It is a G-type main-sequence star. HAT-P-30 has a similar concentration of heavy elements compared to the Sun.

The faint stellar companion was detected in 2013 at a projected separation of 3.842{{±|0.007}}″.

Planetary system

In 2011 a transiting hot Jupiter planet b was independently detected by two teams.

The planetary orbit is strongly misaligned with the equatorial plane of the star, the misalignment angle being equal to 73.5{{±|9.0}}°.

Since 2022, an additional planet in the system is suspected based on transit timing variations.

{{OrbitboxPlanet begin

| table_ref =

}}

{{OrbitboxPlanet

| exoplanet = b

| mass = 0.723{{±|0.023}}

| radius = 1.426{{±|0.020}}

| semimajor = 0.04114{{±|0.00030}}

| period = 2.8106006{{±|0.0000004}}

| eccentricity = 0

| inclination = 82.56{{±|0.08}}

}}

References

{{Reflist|refs=

{{citation | 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. | title = The Tycho-2 catalogue of the 2.5 million brightest stars |journal=Astronomy and Astrophysics | date = March 2000 | volume = 355 | pages = L27–L30 | bibcode = 2000A&A...355L..27H | issn = 0004-6361}}

{{citation|arxiv=2203.02866|year=2022|title=WASP-35 and HAT-P-30/WASP-51: Reanalysis using TESS and Ground-based Transit Photometry|doi=10.3847/1538-3881/ac5b6a |last1=Bai |first1=Lu |last2=Gu |first2=Shenghong |last3=Wang |first3=Xiaobin |last4=Sun |first4=Leilei |last5=Kwok |first5=Chi-Tai |last6=Hui |first6=Ho-Keung |journal=The Astronomical Journal |volume=163 |issue=5 |page=208 |bibcode=2022AJ....163..208B |s2cid=247292453 |doi-access=free }}

{{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=1103.3825|title=HAT-P-30b: A transiting hot Jupiter on a highly oblique orbit|year=2011|doi=10.1088/0004-637X/735/1/24|last1=Johnson|first1=John Asher|last2=Winn|first2=J. N.|last3=Bakos|first3=G. Á.|last4=Hartman|first4=J. D.|last5=Morton|first5=T. D.|last6=Torres|first6=G.|last7=Kovács|first7=Géza|last8=Latham|first8=D. W.|last9=Noyes|first9=R. W.|last10=Sato|first10=B.|last11=Esquerdo|first11=G. A.|last12=Fischer|first12=D. A.|last13=Marcy|first13=G. W.|last14=Howard|first14=A. W.|last15=Buchhave|first15=L. A.|last16=Fűrész|first16=G.|last17=Quinn|first17=S. N.|last18=Béky|first18=B.|last19=Sasselov|first19=D. D.|last20=Stefanik|first20=R. P.|last21=Lázár|first21=J.|last22=Papp|first22=I.|last23=Sári|first23=P.|journal=The Astrophysical Journal|volume=735|issue=1|page=24|bibcode=2011ApJ...735...24J|s2cid=53689766}}

{{citation |doi=10.1088/0004-6256/142/3/86 |title=WASP-35b, WASP-48b, and HAT-P-30b/WASP-51b: Two New Planets and an Independent Discovery of a Hat Planet |year=2011 |last1=Enoch |first1=B. |last2=Anderson |first2=D. R. |last3=Barros |first3=S. C. C. |last4=Brown |first4=D. J. A. |last5=Cameron |first5=A. Collier |last6=Faedi |first6=F. |last7=Gillon |first7=M. |last8=Hébrard |first8=G. |last9=Lister |first9=T. A. |last10=Queloz |first10=D. |last11=Santerne |first11=A. |last12=Smalley |first12=B. |last13=Street |first13=R. A. |last14=Triaud |first14=A. H. M. J. |last15=West |first15=R. G. |last16=Bouchy |first16=F. |last17=Bento |first17=J. |last18=Butters |first18=O. |last19=Fossati |first19=L. |last20=Haswell |first20=C. A. |last21=Hellier |first21=C. |last22=Holmes |first22=S. |last23=Jehen |first23=E. |last24=Lendl |first24=M. |last25=Maxted |first25=P. F. L. |last26=McCormac |first26=J. |last27=Miller |first27=G. R. M. |last28=Moulds |first28=V. |last29=Moutou |first29=C. |last30=Norton |first30=A. J. |journal=The Astronomical Journal |volume=142 |issue=3 |page=86 |arxiv=1104.2827 |bibcode=2011AJ....142...86E |s2cid=63996398 |display-authors=29 }}

{{citation |bibcode=2013A&A...559A..71G |doi=10.1051/0004-6361/201322274 |title=The multiplicity status of three exoplanet host stars |author1=Ginski, C. |author2=Mugrauer, M. |author3=Seeliger, M. |author4=Löhne, T. |journal=Astronomy & Astrophysics |volume=559 |pages=6 |date=November 2013 |doi-access=free }}

}}

Category:Hydra (constellation)

Category:G-type main-sequence stars

Category:Binary stars

Category:Planetary systems with one confirmed planet

Category:Planetary transit variables

J08154797+0550121

Category:Durchmusterung objects