WASP-16b

{{Short description|Extrasolar planet}}

{{Infobox planet

| name = WASP-16b

| image = Exoplanet Comparison WASP-16 b.png

| caption = Size comparison of WASP-16b with Jupiter.

| discoverer = Lister et al.

| discovered = August 3, 2009

| discovery_method = Transit and
Radial velocity

| apsis = astron

| semimajor = 0.0421{{±|0.001|0.0018}} AU

| eccentricity = 0

| period = 3.1186009{{±|1.46e-5|1.31e-5}} d

| inclination = 85.22{{±|0.27|0.43}}

| star = WASP-16

| mass = 0.855 ± 0.059 {{Jupiter mass|link=y}}

}}

WASP-16b is an extrasolar planet that travels around its star, WASP-16, every 3.12 days. Likely a hot Jupiter. Its mass is near .855 of Jupiter, the radius is 1.008 of Jupiter. It was discovered in 2009 by a team led by T.A. Lister as part of the Wide Angle Search for Planets project.{{cite journal

| last = Lister | first = Timothy A

| title = WASP-16b: A new Jupiter-like planet transiting a southern solar analog

| date = 3 August 2009

| arxiv = 0908.1553

|display-authors=etal

| doi=10.1088/0004-637X/709/1/159

| volume=709

| journal=The Astrophysical Journal

| issue = 1

| pages=159–167

| bibcode=2010ApJ...709..159A| s2cid = 53628741

}}

Characteriscics

In 2012, it was found from the Rossiter–McLaughlin effect that WASP-16b orbits its slow-rotating and likely old parent star WASP-16 in a prograde direction, with the star's rotational axis inclined to the planetary orbit by {{val|-4.2|11.0|13.9|u=deg}}.

References

{{reflist|refs=

{{cite journal|arxiv=1203.4971|doi=10.1111/j.1365-2966.2012.20973.x|title=Rossiter-McLaughlin Effect Measurements for WASP-16, WASP-25 and WASP-31 |year=2012|last1=Brown|first1=D. J. A.|last2=Cameron|first2=A. Collier|last3=Anderson|first3=D. R.|last4=Enoch|first4=B.|last5=Hellier|first5=C.|last6=Maxted|first6=P. F. L.|last7=Miller|first7=G. R. M.|last8=Pollacco|first8=D.|last9=Queloz|first9=D.|last10=Simpson|first10=E.|last11=Smalley|first11=B.|last12=Triaud|first12=A. H. M. J.|last13=Boisse|first13=I.|last14=Bouchy|first14=F.|last15=Gillon|first15=M.|last16=Hébrard|first16=G.|journal=Monthly Notices of the Royal Astronomical Society|volume=423|issue=2|pages=1503–1520|doi-access=free |bibcode=2012MNRAS.423.1503B|s2cid=53445367 }}

}}