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Shadow or Mirage: Hunting a Moon Around a Scorching Jupiter ⚡ экспресс

Original: "A JWST Transit of a Jupiter Analog: II. A Search for Exomoons"
arXiv:2511.15317 · 2025-11-19 · CC BY · ⏱ 1 min · Exoplanets
Instrumental drift turned the moon hunt at Kepler-167e into an open-ended detective story.
Abstract

Using the James Webb Space Telescope, scientists carried out a 60-hour observation of the exoplanet Kepler-167e (a Jupiter-like planet) transiting its star, hoping to find an exomoon. They uncovered strong instrumental trends—a slow drift in brightness in each 10-hour exposure, like a camera lens gradually fogging up. In 7 out of 12 analysis runs, the data hinted at a large moon, but the likely culprit is the planet crossing a starspot mid-transit, backed up by old Kepler observations. Paradoxically, Webb’s superb precision makes a single transit too 'flexible' for moon models, so the mystery will only be solved by another observation in 2027.

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The hunt for exomoons — the search for satellites around planets of other stars — resembles watching shadows in a theater where the spotlight keeps fading and flaring. The planet Kepler-167e, a gas giant near a scorching star, was discovered by William Borucki and his team. Now James Webb watched its passage across the star, hoping to catch a tiny dip in brightness from a moon.

But the telescope faced an invisible foe — its own 'breathing'. The sensitive NIRSpec instrument registered a slow drift, as if someone was smoothly turning a dimmer knob: thermal fluctuations in the camera created the illusion of changing light. Against this shaky background, the moon signal got lost, like a mosquito's shadow in the flickering beam of a spotlight. Out of 12 processing methods, seven pointed to a satellite one-tenth the planet's size. Yet midway through the transit, a double appeared — an event perfectly matching the planet crossing a dark starspot. Such a spot, like a colossal solar storm, could fool the detectors.

An answer will come in October 2027: only then will a new transit show whether it was a moon or a trick of the light.

🎯 The brightness drift is caused not by the star, but by the telescope itself: its camera warms and cools, flickering like a living heart.

🎬 The search for distant moons has long become real, yet still evokes scenes from 'Star Wars': somewhere out there, around gas giants, their own Endors could be hiding.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterAlbert Einstein
Tags
exoplanet JWST transit method spectroscopy
Laws
Doppler effectgravitational lensingKepler's third lawMaxwell's equationsPlanck's lawPlanck–Einstein relation
Original: arXiv:2511.15317 · CC BY · bridge42worlds