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Starlink and OneWeb Satellites: An Unexpected Swap in Brightness ⚡ экспресс

Original: "Secular Brightness Trends of Starlink and OneWeb Satellites"
· Anthony Mallama
arXiv:2604.13145 · 2026-04-14 · CC BY 4.0 · ⏱ 1 min · Instrumentation
Over five years, Starlink got brighter while OneWeb got dimmer.
Abstract

Astronomers analyzed 1.6 million brightness measurements of Starlink VisorSat and OneWeb satellites from 2021 to 2026. It turned out that Starlink became brighter by 0.6 magnitudes (in this scale, the smaller the number, the brighter the object), while OneWeb, on the contrary, dimmed by 0.4 magnitudes. Both trends are statistically significant—the probability of a random coincidence is less than 0.3% (three sigma). These data will help better assess the impact of satellite constellations on astronomical observations.

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For five consecutive years, the automated MMT9 observatory measured the brightness of Starlink and OneWeb satellites using photometry (precise light measurement). The results were surprising: VisorSats, equipped with visors to reduce glare, became brighter by 0.6 magnitudes, while OneWeb, on the contrary, dimmed by 0.4. The scale is inverted: the smaller the number, the brighter the object. So "increased brightness" actually means the number got smaller.

These changes are like headlights on a dark road: some suddenly shine brighter while others grow dim. Such instability hampers astronomers: they search for exoplanets by detecting faint dips in starlight during a transit, but a passing satellite can flood the frame, mimicking a false signal. Projects like the Kepler telescope, launched under the leadership of William Borucki, and modern observations following the methods of David Charbonneau, may lose precious data because of this.

Satellite operators should take long-term trends into account and make their spacecraft darker and more stable. Otherwise, celestial traffic risks turning from an annoying nuisance into a real obstacle for science.

🎯 The astronomical brightness scale works backward: the brighter the object, the smaller its number. So, "a brightness increase of 0.6" means the numerical value dropped by 0.6. This system was invented by ancient astronomers, who divided visible stars into six magnitudes—from first (brightest) to sixth (dimmest).

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterDavid Charbonneau
Tags
photometry exoplanet transit method
Laws
Doppler effectKepler's third lawStefan–Boltzmann lawKepler's first lawKepler's second lawLaw of Universal Gravitation
Original: arXiv:2604.13145 · CC BY 4.0 · bridge42worlds