WASP-107b Turns Out to be Super-Puff the Size of Jupiter

Jan 20, 2021 | Daily Space, Exoplanets

IMAGE: Artistic rendition of the exoplanet WASP-107b and its star, WASP-107. Some of the star’s light streams through the exoplanet’s extended gas layer. CREDIT: ESA/HUBBLE, NASA, M. KORNMESSER

Jupiter is definitely the Big Planet on Campus here in our solar system, what with that huge moon and its own significant size. But in the wider galaxy, Jupiter is a small fish in a big pond. And it’s not even the most interesting Jupiter-sized planet in that big pond!

In a new paper appearing in The Astronomical Journal, a team led by Caroline Piaulet presents the discovery of a puffed up planet. Roughly the size of Jupiter, the world has ten times less mass than Jupiter. It’s basically just a lot of hot gas with a less than 4.6 Earth-mass core. 

It is thought that it normally takes significantly more mass in the core for a planet to gravitationally pull in enough material to be this big. This object has been cataloged as WASP-107b and has been dubbed a super puff or cotton candy planet. Co-author Bjorn Benneke states: This work addresses the very foundations of how giant planets can form and grow. It provides concrete proof that massive accretion of a gas envelope can be triggered for cores that are much less massive than previously thought.

It’s unclear if the team has considered any other ways of getting a puffed-out planet than forming it that way; this is after all a discovery paper saying, “Hey, look at what we found.” 

I have to admit, this work reminds me of a paper last year that pointed out that Jupiter’s core is fluffier than expected, probably because of a collision between Jupiter and an earlier proto-planet. That paper has me wondering if you can get really fluffy planets with bigger collisions. I can’t wait to see what theorists do with this discovery.

More Information

University of Montreal press release

WASP-107b’s Density Is Even Lower: A Case Study for the Physics of Planetary Gas Envelope Accretion and Orbital Migration,” Caroline Piaulet et al., 2021 January 18, The Astronomical Journal

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