A hard drive from space: Hidden magnetic messages uncovered

Death of a dynamo: A hard drive from space
An image of the Esquel meteorite, which consists of gem-quality cystals embedded in metal. The magnetism of this metal has been used to investigate the development of planetary bodies 4.6 billions of years ago in the early solar system. Credit: Natural History Museum, London

The dying moments of an asteroid's magnetic field have been successfully captured by researchers, in a study that offers a tantalising glimpse of what may happen to the Earth's magnetic core billions of years from now.

Using a detailed imaging technique, the research team were able to read the contained in ancient meteorites, formed in the early solar system over 4.5 billion years ago. The readings taken from these tiny 'space magnets' may give a sneak preview of the fate of the Earth's magnetic core as it continues to freeze. The findings are published today (22 January) in the journal Nature.

Using an intense beam of x-rays to image the nanoscale magnetisation of the meteoritic metal, researchers led by the University of Cambridge were able to capture the precise moment when the core of the meteorite's parent asteroid froze, killing its magnetic field. These 'nano-paleomagnetic' measurements, the highest-resolution paleomagnetic measurements ever made, were performed at the BESSY II synchrotron in Berlin.

The researchers found that the magnetic fields generated by asteroids were much longer-lived than previously thought, lasting for as long as several hundred million years after the asteroid formed, and were created by a similar mechanism to the one that generates the Earth's own magnetic field. The results help to answer many of the questions surrounding the longevity and stability of magnetic activity on small bodies, such as asteroids and moons.

"Observing magnetic fields is one of the few ways we can peek inside a planet," said Dr Richard Harrison of Cambridge's Department of Earth Sciences, who led the research. "It's long been assumed that metal-rich meteorites have poor magnetic memories, since they are primarily composed of iron, which has a terrible memory - you wouldn't ever make a hard drive out of iron, for instance. It was thought that the magnetic signals carried by metal-rich meteorites would have been written and rewritten many times during their lifetime, so no-one has ever bothered to study their magnetic properties in any detail."

The particular meteorites used for this study are known as pallasites, which are primarily composed of iron and nickel, studded with gem-quality silicate crystals. Contained within these unassuming chunks of iron however, are tiny particles just 100 nanometres across - about one thousandth the width of a human hair - of a unique magnetic mineral called tetrataenite, which is magnetically much more stable than the rest of the , and holds within it a magnetic memory going back billions of years.

"We're taking ancient magnetic field measurements in nanoscale materials to the highest ever resolution in order to piece together the magnetic history of asteroids - it's like a cosmic archaeological mission," said PhD student James Bryson, the paper's lead author.

Death of a dynamo: A hard drive from space
Magnetic microscopy image of the meteoritic metal in the Brenham meteorite. Red and Blue signals correspond to oppositely magnetised regions of the metal, and these signals have allowed scientists to reconstruct the field generated billions of years ago by the asteroid from which this meteorite originated. Credit: James Bryson

The researchers' magnetic measurements, supported by computer simulations, demonstrate that the magnetic fields of these asteroids were created by compositional, rather than thermal, convection - meaning that the field was long-lasting, intense and widespread. The results change our perspective on the way magnetic fields were generated during the early life of the solar system.

These meteorites came from asteroids formed in the first few million years after the formation of the Solar System. At that time, planetary bodies were heated by radioactive decay to temperatures hot enough to cause them to melt and segregate into a liquid metal core surrounded by a rocky mantle. As their cores cooled and began to freeze, the swirling motions of liquid metal, driven by the expulsion of sulphur from the growing inner core, generated a magnetic field, just as the Earth does today.

"It's funny that we study other bodies in order to learn more about the Earth," said Bryson. "Since asteroids are much smaller than the Earth, they cooled much more quickly, so these processes occur on shorter timescales, enabling us to study the whole process of core solidification."

Scientists now think that the Earth's core only began to freeze relatively recently in geological terms, maybe less than a billion years ago. How this freezing has affected the Earth's magnetic field is not known. "In our meteorites we've been able to capture both the beginning and the end of core freezing, which will help us understand how these processes affected the Earth in the past and provide a possible glimpse of what might happen in the future," said Harrison.

However, the Earth's core is freezing rather slowly. The solid inner core is getting bigger, and eventually the liquid outer core will disappear, killing the Earth's , which protects us from the Sun's radiation. "There's no need to panic just yet, however," said Harrison. "The won't completely freeze for billions of years, and chances are, the Sun will get us first."


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More information: "Long-lived magnetism from solidification-driven convection on the pallasite parent body" Nature. DOI: 10.1038/nature14114
Journal information: Nature

Citation: A hard drive from space: Hidden magnetic messages uncovered (2015, January 21) retrieved 12 November 2019 from https://phys.org/news/2015-01-death-dynamo-hard-space.html
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