VISUAL ARCHIVE / IMAGE STORY
How Deep Do Jupiter’s Winds Go?
Juno traced jet streams far below the clouds; the visible flow lines are explanatory.
Jupiter’s visible bands belong to a much deeper system of winds. Juno data indicate flows reaching roughly 3,000 kilometers below the cloud tops and organized along the planet’s rotation axis. AI-generated conceptual illustration; The Last Transmission © 2026 DarkScienceDocs.com
THE OBSERVATION
What we can actually see.
Juno’s gravity data indicate that the familiar east-west belts and zones extend roughly 3,000 kilometers beneath Jupiter’s cloud tops. The result comes from interpreting a gravity field affected by moving mass, not from a camera following wind down into darkness.
THE ILLUSTRATION
What the artwork imagines.
The curved flow lines make an invisible three-dimensional circulation pattern legible. Their widths, colors, and exact paths are not a direct measurement of each parcel of gas.
FROM THE ILLUSTRATED ARTICLE
The story that inspired it.
The article uses deep winds as one reminder that interpreting gravity requires separating atmospheric motion from the mass distribution of the interior.
Read The Planet That Wouldn’t Keep Its CoreCHECK THE RECORD
The image interprets the research below. Follow the original work for the measurements and limits behind the scene.
NASA Juno mission scienceOTHER IMAGE STORIES
Jupiter’s Unseen Core
A Radio Signal Along Jupiter’s Edge
The Mark Shared by Titan and Pluto