XO-6b

{{Short description|Hot Jupiter exoplanet orbiting the star XO-6}}

{{Infobox planet

| extrasolarplanet = yes

| name = XO-6

| image = XO-6 b comparison.png

| caption = Jupiter compared to XO-6b

| apsis = astron

| discovery_ref =

| discoverer =

| discovery_site = Haleakalā Observatory in Maui, Hawaii

| discovered = December 8th, 2016

| discovery_method = Transit

| orbit_ref =

| semimajor = {{val|0.082|0.008|ul=AU}}

| avg_speed =

| eccentricity = 0.00 (fixed)

| period = {{val|3.7649923|(45)|(46)|ul=days}}

| synodic_period =

| inclination = {{val|84.77|0.82|0.66|ul=deg}}

| angular_dist =

| long_periastron =

| time_periastron = {{val|2458843.93943|0.00012|ul=JD|fmt=commas}}

| semi-amplitude = <{{val|450|ul=m/s}}

| star =

| physical_ref =

| mean_radius = {{val|1.52|0.17|ul=Jupiter radius}}

| surface_area =

| volume =

| density =

| mass = {{val|1.73|0.20|ul=Jupiter mass}}

| single_temperature = {{val|1670|25|ul=K|fmt=commas}}

}}

XO-6b is a transiting exoplanet, orbiting the star XO-6 around 760 light years (230 parsecs) away from Earth. It was discovered in 2016 by the XO planet search team.{{Cite encyclopedia |date=2016 |title=The Extrasolar Planet Encyclopaedia — XO-6 b |url=https://exoplanet.eu/catalog/xo_6_b--4076/ |access-date=2021-02-18 |encyclopedia=Extrasolar Planets Encyclopaedia}}

Characteristics

XO-6b is classified as a hot Jupiter. The planet has an orbital period of just 3.8 days and an average orbital separation of 0.082 astronomical units. As of such, it is highly irradiated, with a surface temperature estimated to be around {{convert|1670|K|C}}. The planet's mass is estimated at {{val|1.73|0.20|ul=Jupiter mass}}. The discovery paper suggested a very large radius of {{Val|2.07|0.22|ul=Jupiter radius}}, which would make it among the largest known exoplanets, but more recent papers, considering the measurements of the host star's distance by the Gaia satellite, found the radius to be smaller, at around {{Val|1.5|u=Jupiter radius}}.

Host star

{{Starbox begin|name=XO-6}}

{{Starbox observe

|epoch=J2000

|equinox=J2000

|constell=Camelopardalis

|ra={{RA|06|19|10.3709}}

|dec={{DEC|+73|49|39.587}}

|appmag_v={{val|10.247|0.004}}

}}

{{Starbox character

|type=Main sequence

|class=F5

|variable=Planetary transit variable

}}

{{Starbox astrometry

|radial_v={{Val|2.5|0.9}}

|prop_mo_ra={{val|-16.628}}

|prop_mo_dec={{Val|-22.275}}

|pm_footnote=

|parallax=4.3131

|p_error=0.0232

|parallax_footnote=

|dist_footnote=

}}

{{Starbox detail

|source=

|mass={{Val|1.297|0.040}}

|radius={{Val|1.417|0.029}}

|luminosity=3.36

|gravity={{Val|4.291|0.091}}

|temperature={{Val|6724|164|fmt=commas}}

|age_gyr={{Val|1.89|0.46}}

}}

{{Starbox catalog

|names={{odlist|BD=+73°323|TIC=138168780|TOI=1651}}

}}

{{Starbox reference

| Simbad=XO-6

}}

{{Starbox end}}

XO-6b orbits XO-6, a faint 10th magnitude star in the constellation Camelopardalis.{{Cite constellation|BD+73 323}} Due to its magnitude, this star is too faint to be seen with the naked eye, but can be seen with a telescope.{{Citation needed|date=February 2024}} XO-6 is a F-type main-sequence star with about 1.30 times the mass of the Sun. It is also radiating three times as bright, and is 1.4 times the size of the Sun. It is also hotter, with a temperature of {{val|6724|ul=K}}, which gives it the typical hue of an F-type star. Unlike most other stars of its kind, XO-6 rotates rapidly at a rate of 43 km/s.{{Citation needed|date=May 2025}}

References

{{Reflist|refs=

{{Cite journal |last=Saha |first=Suman |date=2024-09-01 |title=Precise Transit Photometry Using TESS. II. Revisiting 28 Additional Transiting Systems with Updated Physical Properties |bibcode=2024ApJS..274...13S |arxiv= 2407.20846 |journal=The Astrophysical Journal Supplement Series |volume=274 |issue=1 |pages=13 |doi=10.3847/1538-4365/ad6a60 |doi-access=free |issn=0067-0049}}

{{cite journal |title=Discovery of XO-6b: A Hot Jupiter Transiting a Fast Rotating F5 Star on an Oblique Orbit |last1=Crouzet |first1=N. |last2=McCullough |first2=P. R. |last3=Long |first3=D. |last4=Montanes Rodriguez |first4=P. |last5=Lecavelier Des Etangs |first5=A. |last6=Ribas |first6=I. |last7=Bourrier |first7=V. |last8=Hébrard |first8=G. |last9=Vilardell |first9=F. |last10=Deleuil | first10=M. |last11=Herrero |first11=E. |last12=Garcia-Melendo |first12=E. |last13=Akhenak |first13=L. |last14=Foote |first14=J. |last15=Gary |first15=B. |last16=Benni |first16=P. |last17=Guillot |first17=T. |last18=Conjat |first18=M. |last19=Mékarnia |first19=D. |last20=Garlitz |first20=J. |last21=Burke |first21=C. J. |last22=Courcol |first22=B. |last23=Demangeon |first23=O. |display-authors=1 |journal=The Astronomical Journal |volume=153 |issue=3 |at=94 |year=2017 |arxiv=1612.02776 |bibcode=2017AJ....153...94C |doi=10.3847/1538-3881/153/3/94 |s2cid=119082666 |doi-access=free }}

{{Cite journal |last1=Collaboration |first1=Gaia |last2=Creevey |first2=O. L. |last3=Sarro |first3=L. M. |last4=Lobel |first4=A. |last5=Pancino |first5=E. |last6=Andrae |first6=R. |last7=Smart |first7=R. L. |last8=Clementini |first8=G. |last9=Heiter |first9=U. |last10=Korn |first10=A. J. |last11=Fouesneau |first11=M. |last12=Frémat |first12=Y. |last13=De Angeli |first13=F. |last14=Vallenari |first14=A. |last15=Harrison |first15=D. L. |date=June 2023 |title=Gaia Data Release 3. A golden sample of astrophysical parameters |bibcode=2023A&A...674A..39G |journal=Astronomy and Astrophysics |language=en |volume=674 |pages=A39 |doi=10.1051/0004-6361/202243800 |arxiv=2206.05870 |issn=0004-6361}}

{{Cite journal |last1=Johns |first1=Daniel |last2=Marti |first2=Connor |last3=Huff |first3=Madison |last4=McCann |first4=Jacob |last5=Wittenmyer |first5=Robert A. |last6=Horner |first6=Jonathan |last7=Wright |first7=Duncan J. |date=November 2018 |title=Revised Exoplanet Radii and Habitability Using Gaia Data Release 2 |bibcode=2018ApJS..239...14J |journal=The Astrophysical Journal Supplement Series |language=en |volume=239 |issue=1 |pages=14 |doi=10.3847/1538-4365/aae5fb |doi-access=free |arxiv=1808.04533 |issn=0067-0049}}

{{cite web | title=The Colour of Stars | date=December 21, 2004 | work=Australia Telescope, Outreach and Education | publisher=Commonwealth Scientific and Industrial Research Organisation | url=http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html | accessdate=2012-01-16 | archive-date=2013-12-03 | archive-url=https://web.archive.org/web/20131203222826/http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html | url-status=dead }}

{{Cite DR3|1114308481603347584}}

{{cite journal |title=Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties |url=https://www.aanda.org/articles/aa/full_html/2016/11/aa29512-16/aa29512-16.html |journal=Astronomy and Astrophysics |volume=595 |at=A2 |year=2016 |last1=Brown |first1=A. G. A |last2=Vallenari |first2=A |last3=Prusti |first3=T |last4=De Bruijne |first4=J. H.J |last5=Mignard |first5=F |last6=Drimmel |first6=R |last7=Babusiaux |first7=C |last8=Bailer-Jones |first8=C. A.L |last9=Bastian |first9=U |last10=Biermann |first10=M |last11=Evans |first11=D. W |last12=Eyer |first12=L |last13=Jansen |first13=F |last14=Jordi |first14=C |last15=Katz |first15=D |last16=Klioner |first16=S. A |last17=Lammers |first17=U |last18=Lindegren |first18=L |last19=Luri |first19=X |last20=o'Mullane |first20=W |last21=Panem |first21=C |last22=Pourbaix |first22=D |last23=Randich |first23=S |last24=Sartoretti |first24=P |last25=Siddiqui |first25=H. I |last26=Soubiran |first26=C |last27=Valette |first27=V |last28=Van Leeuwen |first28=F |last29=Walton |first29=N. A |last30=Aerts |first30=C |display-authors=1 |arxiv=1609.04172 |bibcode=2016A&A...595A...2G |doi=10.1051/0004-6361/201629512 |s2cid=1828208 }}[http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=I/337/tgas&recno=284654 Gaia Data Release 1 catalog entry]

{{Cite journal |last1=Simpson |first1=Emilie R. |last2=Fetherolf |first2=Tara |last3=Kane |first3=Stephen R. |last4=Pepper |first4=Joshua |last5=Močnik |first5=Teo |last6=Dalba |first6=Paul A. |date=August 2023 |title=Variability of Known Exoplanet Host Stars Observed by TESS |bibcode=2023AJ....166...72S |journal=The Astronomical Journal |language=en |volume=166 |issue=2 |pages=72 |doi=10.3847/1538-3881/acda26 |doi-access=free |arxiv=2305.09687 |issn=0004-6256}}

}}

Further reading

  • {{cite journal |title=Periodic transit timing variations and refined system parameters of the exoplanet XO-6b |last1=Garai |first1=Zoltán |display-authors=et al |journal=Monthly Notices of the Royal Astronomical Society |volume=491 |issue=2 |pages=2760–2769 |doi=10.1093/mnras/stz3235 |arxiv=1911.07054 |bibcode=2020MNRAS.491.2760G |date=January 2020|doi-access=free }}
  • {{cite journal |title=TESS Observations of the Hot Jupiter Exoplanet XO-6b: No Evidence of Transit Timing Variations |journal=The Astronomical Journal |volume=160 |issue=6 |date=December 2020 |doi=10.3847/1538-3881/abba1e |arxiv=2009.10781 |bibcode=2020AJ....160..249R |last1=Ridden-Harper |first1=Andrew |last2=Turner |first2=Jake D. |last3=Jayawardhana |first3=Ray |page=249 |s2cid=221856652 |doi-access=free}}

{{Stars of Camelopardalis}}

Category:Exoplanets discovered in 2016

Category:Transiting exoplanets

Category:Hot Jupiters

Category:Camelopardalis