Image Credentials: Image Title: Earth’s Weather Satellites Secretly Spied on Venus for a Decade — The Surprising Discoveries Source: (sora.chatgpt) Date: June 2025 Attribution: Created by AI-generated imagery (sora.chatgpt), it does not depict a real-world scene.
July 2, 2025 | University of Tokyo
For the past decade, Japan’s Himawari-8 and -9 weather satellites—designed to monitor Earth’s atmosphere—have quietly been snapping infrared images of Venus, capturing unprecedented details of its swirling cloud tops. By stitching together 437 images taken between 2015 and 2025, scientists have now uncovered hidden thermal patterns, planetary waves, and even calibration errors in past Venus mission data.
The study, led by the University of Tokyo, demonstrates how Earth-orbiting weather satellites can double as planetary observatories, filling critical gaps in long-term planetary monitoring. The findings, published in Nature Astronomy, reveal decadal-scale atmospheric changes on Venus that were previously impossible to track.
Why Venus Is So Hard to Study
Venus’s thick, sulfuric acid-laden clouds obscure its surface, but its upper atmosphere exhibits dynamic weather patterns, including:
✔ Super-rotating winds (60x faster than the planet’s rotation)
✔ Thermal tides (temperature fluctuations driven by solar heating)
✔ Planetary-scale waves (massive atmospheric disturbances)
However, studying these phenomena long-term has been challenging because:
🔹 Planetary missions (like ESA’s Venus Express or JAXA’s Akatsuki) last only a few years.
🔹 Ground telescopes are limited by Earth’s atmosphere and daylight.
“No Venus mission has observed continuously for 10 years—until now,” says Gaku Nishiyama, lead researcher and visiting scientist at the University of Tokyo.
Himawari’s Unexpected Venus Mission
Launched in 2014 (Himawari-8) and 2016 (Himawari-9), these geostationary weather satellites were equipped with Advanced Himawari Imagers (AHI), designed to monitor Earth in 16 infrared and visible bands.
But because Venus occasionally appears near Earth’s limb in AHI images, Nishiyama’s team realized they could repurpose the data for planetary science.
Key Discoveries
🔎 Thermal Tides & Planetary Waves – The team detected day-to-year variations in Venus’s cloud-top temperatures, revealing shifting wave patterns.
🔎 Decadal Atmospheric Changes – Some thermal tide fluctuations may be linked to long-term climate cycles.
🔎 Calibration Errors in Past Missions – The data helped identify inconsistencies in older Venus spacecraft measurements.
“This method gives us precious data until the next Venus missions arrive in the 2030s,” says Nishiyama.
Why This Matters
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Cost-Effective Planetary Science – Weather satellites, already in orbit, can supplement dedicated planetary missions.
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Future Missions – The findings will help plan observations for upcoming probes like NASA’s VERITAS and ESA’s EnVision.
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Beyond Venus – The technique could monitor the Moon, Mercury, and other solar system bodies in infrared.
“We’ve opened a new way to study planetary atmospheres without expensive new missions,” Nishiyama adds.
What’s Next?
The Himawari satellites will continue operating until 2029, providing even more Venus data. Meanwhile, scientists are exploring how other Earth-observing satellites—like NOAA’s GOES-R—could contribute to planetary science.
Story Source:
Materials provided by University of Tokyo. Note: Content may be edited for style and length.
Journal Reference:
- Gaku Nishiyama, Yudai Yudai, Shinsuke Uno, Shohei Aoki, Tatsuro Iwanaka, Takeshi Imamura, Yuka Fujii, Thomas G. Müller, Makoto Taguchi, Toru Kouyama, Océane Barraud, Mario D’Amore, Jörn Helbert, Solmaz Adeli, Harald Hiesinger. Temporal variation in the cloud-top temperature of Venus revealed by meteorological satellites. Earth, Planets and Space, 2025; 77 (1) DOI: 10.1186/s40623-025-02223-8