From candy floss to rock: study provides new evidence about beginnings of the Solar System

The earliest rocks in our Solar System were more like candy floss than the hard
The earliest rocks in our Solar System were more like candy floss than the hard rock that we know today
The earliest rocks in our Solar System were more like candy floss than the hard rock that we know today, according to research published Geoscience. The work, by researchers from Imperial College London and other international institutions, provides the first geological evidence to support previous theories, based on computer models and lab experiments, about how the earliest rocks were formed. The study adds weight to the idea that the first solid material in the Solar System was fragile and extremely porous - much like candy floss - and that it was compacted during periods of extreme turbulence into harder rock, forming the building blocks that paved the way for planets like Earth. Dr Phil Bland , lead author of the study from the Department of Earth Science and Engineering at Imperial College London, says: "Our study makes us even more convinced than before that the early carbonaceous chondrite rocks were shaped by the turbulent nebula through which they travelled billions of years ago, in much the same way that pebbles in a river are altered when subjected to high turbulence in the water. Our research suggests that the turbulence caused these early particles to compact and harden over time to form the first tiny rocks." The researchers reached their conclusions after carrying out an extremely detailed analysis of an asteroid fragment known as a carbonaceous chondrite meteorite, which came from the asteroid belt between Jupiter and Mars. It was originally formed in the early Solar System when microscopic dust particles collided with one another and stuck together, coalescing around larger grain particles called chondrules, which were around a millimetre in size.
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