Interestingly, the layered interior structures of Uranus and Neptune may provide insight into some of the broad differences that really differentiate the solar system’s gas giants, Jupiter and Saturn, ...
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 ...
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 archive of data ...
When NASA's Voyager 2 spacecraft made its way to outer regions of the solar system in the late 80's, it noticed something odd. Both of the ice giant planets, Uranus and Neptune, lacked what's known as ...
Models for the interior structures of the ice-giant planets Uranus and Neptune have two distinct, intermediate layers: an upper, water-rich convecting layer where disorganized magnetic fields are ...
When Voyager 2 flew by Uranus and Neptune 40 years ago, astronomers were surprised that it detected no global dipole magnetic fields, like Earth's. The explanation: the ice giants are layered and ...
Ask anyone what their favorite planet in the solar system is besides Earth, and very few will say Uranus or Neptune. The ice giants in the outer solar system are rather dull-looking. Earlier this ...
If you buy through a BGR link, we may earn an affiliate commission, helping support our expert product labs. Uranus and Neptune may soon lose their reputation as the “boring” planets of the ...