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 dataset 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.

 

Team member Dr Adam Masters, a planetary scientist at Imperial, commented: “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. The planet’s unique magnetic field is still very poorly understood, and our new modelling 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 modelling Neptune can also be applied to understand how the 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.

 

Prof Jerry Chittenden of the plasma physics group worked with Dr Jonathan Eastwood, a lecturer in the space and atmospheric physics group, and PhD 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.

 

Modelling 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 to the cartoons that were inferred from the original Voyager 2 measurements. Dr Masters commented: “Magnetic fields are tricky to understand, even when they are in simple systems. But Neptune is particularly badly behaved. Its odd properties challenge our basic ideas on how magnetospheres work.”

A snapshot of Neptune’s magnetic field from the movie. Credit: Lars Mejnertsen, Imperial College London.

Quelle: The Royal Astronomical Society (RAS)