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The Hunt for Moons of Rogue Planets ⚡ экспресс

Original: "A Deep Search for Exomoons Around WISE 0855 With JWST"
arXiv:2510.24575 · 2025-10-28 · CC BY 4.0 · ⏱ 1 min · Exoplanets Instrumentation Stellar
For the first time, the James Webb Space Telescope tested a method to find moons around lonely planets drifting without stars.
Abstract

Observations of the free-floating planetary-mass object WISE 0855 (T≈250–285 K, M≈6.5±3.5 M_Jup, d=2.3 pc) over 11 hours with JWST/NIRSpec enabled an exomoon search via the transit method. The spectrograph's sensitivity combined with Gaussian process modeling allowed separation of transit signals from the object's intrinsic variability. No statistically significant transit evidence was found. Tests with injected artificial signals at depths of 0.1–1% (0.35–1.12 R⊕) showed that for depths ≥0.5% (1.96 R_Titan) detection reliability reaches 96%; this corresponds to a satellite-to-planet mass ratio akin to Titan and Saturn. Given the sensitivity, transit probabilities, and observation durations, the chance to register a Titan analogue after 18 such sessions is ~91% if each system hosts such a moon in a Galilean-like configuration. This work first demonstrates JWST's ability to detect Galilean-mass satellites around free-floating planets.

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In the vast darkness of interstellar space, the rogue planet WISE 0855 flickers with a barely perceptible heat glow, like a cooling ember. Its temperature is only a few dozen degrees above freezing — if life existed there, it would see a sunless sky, in an eternal icy haze. The James Webb telescope stared intently at this faint light for 11 hours, hoping to catch the shadow of a passing moon — as if a microscopic soot particle momentarily eclipsed a smoldering ember.

The transit method can detect even slight dips in brightness when a satellite blocks part of the planet. The main challenge is telling such a shadow from the object’s natural shimmer: an ember already flickers unevenly on its own.

Astronomers built a model predicting the “ember’s” wavering and hunted in the data for dips — moon traces. No direct finds occurred, but the researchers tested their method by injecting artificial moons into the data. If a shadow dimmed the light by at least 0.5%, the detector triggered in 96% of cases, corresponding to a Titan-sized moon.

So, if rogue planets often carry giant moons, after 18 observing sessions Webb has a 91% chance of spotting at least one. Further observations will show whether moons are common in the interstellar night.

🎯 WISE 0855 is one of the coldest objects known beyond the Solar System: its temperature is just a few dozen degrees above freezing. If intelligent life were there, it would see a sky without any sun, perpetually shrouded in water-ice fogs.

🎬 Rogue planets with moons are almost a ready-made illustration for Isaac Asimov’s story “The Wanderer”: the characters live on a moon of an orphan planet, warmed only by internal heat.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterAlbert Einstein
Tags
exoplanet JWST transit method
Laws
Doppler effectgravitational lensingKepler's third lawKepler's first lawKepler's second lawLaw of Universal Gravitation
Original: arXiv:2510.24575 · CC BY 4.0 · bridge42worlds