Voyager 2/ISS images of Uranus and Neptune released shortly after the Voyager 2 flybys in 1986 and 1989, respectively, compared with a reprocessing of the individual filter images in this study to ...

In 1986 and 1989, Voyager 2 made the final two stops on its grand tour of the outer solar system when it swept by Uranus and Neptune, respectively. Now, nearly 40 years later, ...

The existence of these hidden oceans on Neptune and Uranus, as well as a lack of mixing within their interiors, a key feature in generating planetary magnetic fields, may hold the answer to why.

More information: Burkhard Militzer et al, Phase separation of planetary ices explains nondipolar magnetic fields of Uranus and Neptune, Proceedings of the National Academy of Sciences (2024). DOI ...

These NASA images of Uranus (left) and Neptune were taken by the Voyager 2 spacecraft, with models of the planets' interior structures seen in the inset.

Uranus and Neptune are not the colour we tend to think they are, scientist have said.. Generally, Neptune is depicted as a rich, deep blue. Uranus is usually seen as a pale green or cyan. In fact ...

Both of the ice giant planets, Uranus and Neptune, lacked what's known as a "dipole magnetic field." This was in stark contrast to our own rocky world, as well as the two gas giants Jupitar and ...

A 1986 image of Uranus and a 1989 image of Neptune released shortly after each Voyager 2 flyby, compared with the study’s reprocessed images of the planets that better approximate their true colors.

The hidden moons were discovered orbiting Uranus and Neptune, and the discovery brings the moon counts for these planets to 28 and 16, respectively. The discovery of these hidden moons is both ...