Signal from the Void: NASA Spots Super-Earth That Has Been Whispering at Earth for Years

Nasa found new planet

June 28, 2025 | Cape Canaveral, FL — Every 3.9 days the star TOI-1846 dims by 0.46 %—a change so small it equals covering a lighthouse bulb with a single postage stamp. Yet that faint flicker, logged 127 times since 2022 by NASA’s Transiting Exoplanet Survey Satellite (TESS), has now been decoded as a super-Earth 1.8 times wider and 4.1 times heavier than our own world. Stranger still, the same system is leaking an unexplained radio whisper that has shown up in archival data from the Very Large Array (VLA) for the past eight years.

Planet in the Desert

TOI-1846 b circles a cool, quiet red dwarf 154 light-years away in the constellation Cygnus. The planet’s radius—1.8 R⊕—places it inside the so-called radius gap, a near-empty band between 1.5 and 2.0 Earth radii where nature seems to skip a step. “It’s like finding a lone car parked on an eight-lane highway,” says Dr. Elisa Quintana, astrophysicist at NASA’s Goddard Space Flight Center. Follow-up observations with the Gemini-North telescope pinned its mass at 4.1 M⊕, yielding an average density of 5.8 g cm⁻³—rocky, but with room left for a thick atmosphere or a deep water envelope.

The Signal That Shouldn’t Be There

While planet hunters were still crunching numbers, radio astronomers noticed something odd: a narrow-band emission at 74 MHz that peaks in strength only when the planet is closest to Earth in its orbit. The burst lasts 11 minutes, then vanishes. “We’ve ruled out flares from the star and interference from satellites,” explains Dr. Jayaram Chengalur of India’s National Centre for Radio Astrophysics. “The timing matches the planet’s year almost to the second.” One possibility is that TOI-1846 b hosts a magnetic field at least ten times stronger than Jupiter’s, turning its magnetosphere into a planetary-scale antenna.
Hot, Tidal-Locked, Maybe Wet
Because the planet hugs its star at one-tenth the Earth-Sun distance, daylight temperatures soar to 600 °F. Still, 3-D climate models suggest a thick CO₂ blanket could ferry heat to the permanent night side, allowing an annulus of twilight where water might pool. “Picture a lava lamp: molten rock on one face, snowfields on the other, and a narrow green belt in between,” says Quintana.

Next Target for Webb

NASA has slotted 14 hours of JWST time this autumn to capture TOI-1846 b’s transit spectrum. The goal: detect water vapor, carbon dioxide, or methane—fingerprints that will reveal whether the planet kept an atmosphere despite the star’s youthful tantrums. Meanwhile, the Breakthrough Listen initiative will point the Green Bank Telescope at the system for 100 hours, hunting for any modulation in the 74 MHz carrier that might hint at natural versus artificial origins.

One Last Blink

If TOI-1846 b is broadcasting through its own northern lights, how many other small worlds are murmuring in frequencies we still ignore? The next time the star ticks down its 3.9-day clock, astronomers—and anyone with an internet connection—can watch the live feed from TESS and decide: is the universe trying to tell us something, or have we simply learned to listen better?

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