Surprise Planet Around a Young Star express

Original: "Thermal Eclipse Observation of the Young Hot Neptune AU Mic b with Spitzer"
arXiv:2602.05168 · 2026-02-05 · CC BY 4.0 · 1 min
The young planet AU Mic b is hotter than it should be, and that's a new mystery.

Astronomers caught the young planet AU Mic b in the act of hiding behind its star. The Spitzer telescope tracked its infrared glow: as the planet slipped behind, the system's total light dimmed slightly. The dip was just 171 parts per million, like a single drop of ink in ten buckets of water. But that was enough to measure the dayside temperature of this distant world.

The planet turns out to be scorching at 1031 Kelvin (about 758°C). For comparison, if it were heated only by its star's radiation, it would be around 606 Kelvin. That's the difference between a hot cup of tea and a sizzling skillet. The planet is clearly getting extra heat, but where from is a puzzle.

AU Mic b is a "hot Neptune": a gas giant the size of Neptune but orbiting very close to its star. Such planets are common, but this one is among the youngest known, at just about 23 million years old.

The scientists tested several explanations: maybe heat isn't distributed well across the planet, or it's contracting under its own gravity and warming up, or the star's pulsations are to blame, or even instrument errors. None fit. So we'll have to wait for new observations from the James Webb Space Telescope, which could peer into the planet's atmosphere and maybe find the source of the mysterious heat.

The dayside temperature of AU Mic b is higher than that of some stars — red dwarfs that merely smolder in space.

In the novel "The Three-Body Problem," a planet in a three-sun system experiences chaotic temperature swings — AU Mic b also throws surprises, but for now it stays steadily hot.

Scientists
Adam RiessBrian SchmidtEdwin HubbleGeorges LemaîtreMaarten SchmidtSaul Perlmutter
Concepts
neptune hot jupiter atmospheres james webb space telescope miri mercury kepler telescope nirspec jwst exoplanet atmospheres tess transit method eclipse sub neptune nicer icecube type ia supernova JWST hot jupiter infrared telescope neutron star light emission