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Solar Wind Compression of Jupiter's Magnetosphere Reveals Planetary Vulnerabilities

New research documents how a 2017 solar wind event altered Jupiter's atmosphere, offering insights into planetary responses to solar activity and advancing space weather forecasting.

An image of Jupiter's hot region. Image: O'Donoghue et al., Geophysical Research Letters 2025
Jupiter in stunning 3D
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Overview

  • A 2017 solar wind event compressed Jupiter's magnetosphere, heating its atmosphere by 300°F (150°C) and creating a hot region spanning half the planet's circumference.
  • The event triggered intense auroral activity, causing Jupiter's upper atmosphere to expand and redirect hot gas toward the equator, challenging prior assumptions about auroral heating being confined to polar regions.
  • Researchers used data from the Keck telescope and NASA's Juno spacecraft to observe the phenomenon, marking the first documented instance of such an event on Jupiter.
  • The study found that solar wind compressions occur on Jupiter 2–3 times per month, depending on solar activity, and demonstrated the accuracy of solar wind models in predicting these disturbances.
  • These findings highlight the susceptibility of planetary atmospheres to solar influences and provide valuable insights for improving space weather forecasting to protect Earth's infrastructure.