Unified model explains extreme jet streams on all giant planets

One of the most notable properties of the giant planets in our solar system—Jupiter, Saturn, Uranus and Neptune—are the extreme winds observed around their equators. While some of these planets have eastward equatorial winds, others have a westward jet stream. For the first time, an international team of scientists led by Leiden Observatory and SRON, can explain the winds on all the giant planets using one model.