WASP-8b

{{Short description|Planet orbiting a star in a binary system in the constellation of Sculptor}}

{{Infobox planet

| name = WASP-8b

| image = Exoplanet Comparison WASP-8 b.png

| caption = Size comparison of WASP-8b with Jupiter.

| discovery_ref =

| discoverer = Cameron et al. (SuperWASP)

| discovered = April 1, 2008

| discovery_method = Transit

| orbit_ref =

| semimajor = {{val|0.0817|0.0006|ul=AU}}

| eccentricity = {{val|0.3057|0.0046}}

| period = {{val|8.158715|0.000016|ul=d}}

| inclination = {{val|88.51|0.09|u=deg}}

| arg_peri = {{val|274.21|0.33|u=deg}}

| semi-amplitude = {{val|221.65|1.39|ul=m/s}}

| star = WASP-8

| physical_ref =

| mean_radius = {{val|1.165|0.032|ul=Jupiter radius}}

| mass = {{val|2.216|0.035|ul=Jupiter mass}}

| density = {{val|1.7370|0.1325|ul=g/cm3}}

| surface_grav = {{val|42.5|2.3|ul=m/s2}} (4.34 g)

| single_temperature = {{val|1552|85|ul=K}} ({{convert|1552|K|C F|disp=out}})

}}

WASP-8b is an exoplanet orbiting the star WASP-8A in the constellation of Sculptor. The star is similar to the Sun and forms a binary star with a red dwarf star (WASP-8B) of half the Sun's mass that orbits WASP-8A 4.5 arcseconds away. The system is {{convert|294|ly|pc|lk=on|abbr=off}} away and is therefore located closer to Earth than many other star systems that are known to feature planets similar to WASP-8b. The planet and its parent star were discovered in the SuperWASP batch -6b to -15b. On 1 April 2008, Dr. Don Pollacco of Queen's University Belfast announced them at the RAS National Astronomy Meeting (NAM 2008).{{Cite web|date=2008-04-01|title=SuperWASP scoops ten exoplanets in six months|url=https://astronomynow.com/news/080401waspplanets/index.html#:~:text=SuperWASP%20(where%20WASP%20is%20an,SuperWASP%20factory%20output%20to%2015.|website=Astronomy Now}}

Orbit

The planet orbits WASP-8A at an average distance of just {{convert|0.08|AU|km|lk=on|abbr=on}} and a year passes in slightly more than 8.1 days on WASP-8b, which is somewhat farther from its parent star than other hot Jupiter planets. However, WASP-8b's orbit also has a relatively high eccentricity of 0.3, which, at periastron, brings it as close to its star as said similar planets are.

One thing that stands out extremely about WASP-8b is its orbit-spin angle to its star of {{Val|123|3.4|4.4|u=°}}: This implies that the planet actually orbits retrograde to the spin of the parent star.{{cite web | url=http://www.eso.org/public/videos/eso1016a/

|title=Artist's impression of an exoplanet WASP 8b in a retrograde orbit

|author= European Southern Observatory

}}

Physical characteristics

WASP-8b belongs to a class of extrasolar planets known as hot Jupiters and has a mass about 2.2 times and a radius slightly bigger than that of the planet Jupiter. Its density is about {{Val|1.737|u=g/cm3}}; this implies that, unlike similar close-orbiting gas giants, the planet is actually denser than Jupiter (which has a density of {{Val|1.326|u=g/cm3}}).

Owing to its close distance to its star, WASP-8b is extremely hot: Its measured dayside temperature is {{convert|1552|K|C}}, this is even hotter than its equilibrium temperature of {{convert|947|K|C}}.

See also

References

{{reflist|refs=

{{cite journal

|author=Didier Queloz

|display-authors=etal

|year=2010

|title=WASP-8b: a retrograde transiting planet in a multiple system

|journal=Astronomy and Astrophysics

|volume=517 |pages=L1

|arxiv=1006.5089

|bibcode=2010A&A...517L...1Q

|doi=10.1051/0004-6361/201014768

|s2cid=35774603

}}

{{citation|arxiv=1206.6105|title=Obliquities of Hot Jupiter Host Stars: Evidence for Tidal Interactions and Primordial Misalignments|year=2012|doi=10.1088/0004-637X/757/1/18 |last1=Albrecht |first1=Simon |last2=Winn |first2=Joshua N. |last3=Johnson |first3=John A. |last4=Howard |first4=Andrew W. |last5=Marcy |first5=Geoffrey W. |last6=Butler |first6=R. Paul |last7=Arriagada |first7=Pamela |last8=Crane |first8=Jeffrey D. |last9=Shectman |first9=Stephen A. |last10=Thompson |first10=Ian B. |last11=Hirano |first11=Teruyuki |last12=Bakos |first12=Gaspar |last13=Hartman |first13=Joel D. |journal=The Astrophysical Journal |volume=757 |issue=1 |page=18 |bibcode=2012ApJ...757...18A |s2cid=17174530 }}

{{cite journal |last1=Cubillos |first1=Patricio |last2=Harrington |first2=Joseph |display-authors=etal |date=May 2013 |title=WASP-8b: Characterization of a Cool and Eccentric Exoplanet with Spitzer |journal=The Astrophysical Journal |volume=768 |issue=1 |pages=42 |doi=10.1088/0004-637X/768/1/42 |arxiv=1303.5468 |bibcode=2013ApJ...768...42C}}

{{cite journal |last1=Bonomo |first1=A. S. |last2=Desidera |first2=S. |display-authors=etal |date=June 2017 |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 |issue= |pages=A107 |doi=10.1051/0004-6361/201629882 |arxiv=1704.00373 |bibcode=2017A&A...602A.107B}}

{{citation|arxiv=2001.08224|year=2020|title=A multiplicity study of transiting exoplanet host stars|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|s2cid=210861118 |bibcode=2020A&A...635A..73B}}

{{citation|arxiv=2001.08225|year=2020|title=A multiplicity study of transiting exoplanet host stars|doi=10.1051/0004-6361/201937334|last1=Southworth|first1=J.|last2=Bohn|first2=A. J.|last3=Kenworthy|first3=M. A.|last4=Ginski|first4=C.|last5=Mancini|first5=L.|journal=Astronomy & Astrophysics|volume=635|pages=A74|bibcode=2020A&A...635A..74S |s2cid=210860775}}

}}