Neptune, the outermost planet of the solar system, has only been visited by one spacecraft, Voyager 2, which zoomed past in 1989 and is now on its way to interstellar space. The Voyager 2 data set was incredibly rich but raised more questions than answers. One of the biggest puzzles is that Neptune’s rotation axis is tilted relative to the Sun, its magnetic axis is not at all aligned with its rotation, and its magnetic field environment has a lopsided shape.
“Imagine taking the Earth, tipping it over diagonally, and then moving its magnetic north pole to central Europe, and you start to get a sense of what Neptune is like,” said Adam Masters from Imperial College. “The planet’s unique magnetic field is still very poorly understood, and our new modeling represents a big leap forward.”
Understanding Neptune is important because it challenges our basic understanding of how the magnetic fields of planets and exoplanets can behave, and the lessons learned modeling Neptune also can be applied to understand how Earth’s magnetic field affects space weather.
Although new missions to Neptune have been proposed, none are likely to arrive for many decades. So for now, the only way to better understand how the planet works is through computer simulations. In a new example of interdisciplinary research at Imperial College London, the space and atmospheric physics group and the plasma physics group have been working together to address this challenge.
Jerry Chittenden of the plasma physics group worked with Jonathan Eastwood, a lecturer in the space and atmospheric physics group, and student Lars Mejnertsen. The scientists took simulations designed to understand plasma experiments in laboratories on Earth and applied them to space environments. Plasma, the gaseous “fourth state” of matter consisting of electrically charged particles, is commonly found in space, albeit in highly rarefied amounts, and this causes planetary magnetic fields to form structures in space known as magnetospheres.
Modeling an entire planet needs a vast simulation, so the team turned to the Science and Technology Facilities Council’s DiRAC supercomputer. DiRAC’s ability to use hundreds or even thousands of processors in parallel was crucial to vastly speeding up the calculations.
The results show that Neptune’s magnetic field is constantly rotating and changing and has revealed that the structure is quite different from the cartoons that were inferred from the original Voyager 2 measurements. “Magnetic fields are tricky to understand even when they are in simple systems,” said Masters. “But Neptune is particularly badly behaved. Its odd properties challenge our basic ideas on how magnetospheres work.”
“Modeling a whole planet is no easy task. But supercomputers now make it possible, and the new simulations explain a lot of what Voyager saw all those years ago. For example, we can now see how the solar wind — the stream of electrically charged particles from the Sun — enters and circulates around Neptune’s magnetic field. The combination of the dramatic planetary rotation and this circulation pattern is why Voyager 2 found a ‘lopsided’ magnetosphere.”
Understanding Neptune better also will help astronomers understand planets outside the solar system. A large number of those found to date are Neptune-sized, so studying the gas giant should give an insight into conditions on those other distant worlds.
And while Neptune is one of the most exotic planets in the solar system, this work also finds applications closer to home for models of the magnetic field of Earth. The Earth’s field plays a key role in controlling space weather, which can harm technology in space and on the ground. Basic research into the magnetic fields of other planets will help scientists improve our ability to forecast space weather events such as geomagnetic storms.
