WASP-12b

Lore & Background

WASP-12b orbits its star at a distance of about 3.5 million kilometers, just 1/43 of Earth's distance from the Sun. Its proximity causes tidal forces to distort it into a prolate spheroid and pull away its atmosphere at a rate of about 189 quadrillion tons per year. In December 2013, the Hubble Space Telescope detected water in its atmosphere, and in July 2014, NASA reported very dry atmospheres on WASP-12b and two other exoplanets.

Reader's Guide

WASP-12b is significant as one of the most extreme hot Jupiters known, demonstrating the effects of tidal heating and atmospheric stripping. Its low albedo (6% reflectivity) and carbon-rich atmosphere challenge models of planetary formation and composition. The detection of water and carbon monoxide in its atmosphere, along with evidence of a possible plasma torus from a candidate exomoon, make WASP-12b a key object for studying exoplanetary atmospheres and orbital dynamics.

Did You Know?

• WASP-12b reflects only 6% of light, described as 'black as asphalt'.
• It is being consumed by its star, losing about 189 quadrillion tons of atmosphere per year.
• Its orbit is decaying by about 29.81 milliseconds per year, with an estimated lifetime of 3.16 million years.
• It has an enhanced carbon-to-oxygen ratio, possibly indicating a carbon-rich composition like diamond or graphite.

Discovery & Orbital Profile

Its orbital radius of roughly 3.5 million kilometres—about one forty-third of the Earth-Sun gap—places it in an extremely tight embrace around WASP-12, with an eccentricity comparable to Jupiter's own orbit. Despite carrying 40 percent more mass than Jupiter, the planet's atmosphere has swelled to nearly three times Jupiter's radius, giving it one of the lowest known densities among all exoplanets. This pronounced inflation is attributed to the relentless flood of stellar energy it receives. The combination of a bloated envelope and a compact orbit makes WASP-12b a textbook example of how close-in giant planets can be puffed up by their host star's radiation.

Atmospheric Chemistry & the Carbon Question

The chemical makeup of WASP-12b's atmosphere has generated both excitement and confusion among astronomers. In December 2013, a team using the Hubble Space Telescope reported the detection of water vapour in the planet's upper atmosphere. Yet just seven months later, in July 2014, NASA announced that WASP-12b—alongside HD 189733b and HD 209458b—possessed a remarkably dry atmosphere, a finding that seemed to complicate the earlier water detection. The excess carbon resides in the atmosphere primarily as carbon monoxide and methane. One of the study's authors noted that a world with more carbon than oxygen could, in principle, produce solid bodies of pure carbon such as diamond or graphite. The claim quickly captured media attention, with some outlets dubing WASP-12b a "diamond planet," though the carbon in question is gaseous and atmospheric rather than solid planetary material.

A Dying Orbit and Stellar Consumption

WASP-12b is on a slow but irreversible path toward destruction. A 2012 analysis of the Rossiter-McLaughlin effect showed its orbit is tilted roughly 59 degrees relative to the star's equatorial plane. This steady decay, driven by tidal interactions between planet and star, implies an orbital lifetime of only about 3.16 million years. Earlier estimates placed the planet's remaining lifespan at three to ten million years, a window that is now steadily closing.

A Black, Blazing, Tidally Warped World

Despite its enormous size, WASP-12b is almost impossibly dark. In September 2017, Hubble-based researchers measured its albedo at just six percent, meaning it bounces back only a tiny fraction of the starlight that strikes it. Descriptions in the literature have called its surface "black as asphalt" and "pitch black." Yet the planet is simultaneously so scorching hot that it radiates its own reddish glow, a direct consequence of tidal heating and its blistering proximity to WASP-12. Because it is tidally locked—much like the Moon always showing Earth the same face—one hemisphere is locked in perpetual daylight while the other endures endless night. This extreme temperature gradient drives ferocious winds that sweep heat from the irradiated day side toward the cooler night side. Physicists Taylor Bell and Nicolas Cowan have further argued that hydrogen atoms become ionised on the blazing day face and then recombine into neutral atoms as they travel to the cooler hemisphere, amplifying the planet's internal heat transport. The relentless tidal pull also stretches the planet into a visibly elongated, prolate spheroid shape.