CALCIUM CARBONATE




The early ocean known as Arabia (left, blue) would have looked like this when it formed 4 billion years ago on Mars, while the Deuteronilus ocean, about 3.6 billion years old, had a smaller shoreline. Both coexisted with the massive volcanic province Tharsis, located on the unseen side of the planet, which may have helped support the existence of liquid water. The water is now gone, perhaps frozen underground and partially lost to space, while the ancient seabed is known as the northern plains. Robert Citron images, UC Berkeley.
A new scenario seeking to explain how Mars’ putative oceans came and went over the last 4 billion years implies that the oceans formed several hundred million years earlier and were not as deep as once thought...
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NTU ground glass camera can take images in multispectrum, with potential uses in chemical sensing and food safety. Credit: Image courtesy of Nanyang Technological University
A new camera technology developed by scientists from NTU Singapore can take sharp, colour images without using a lens and colour filters. Using only a piece of ground glass and a monochrome sensor, the scientists created multi-coloured images by ‘reverse engineering’ the light that is scattered by the translucent matt surface of the ground glass, thus obtaining the original image that was projected on to it.
Since different wavelengths of light are scattered differently by the ground glass, the NTU scientists created an algorithm to reconstruct the image...
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The surface features of the northern and southern hemispheres of Mars are very different. In this topographic map, the northern hemisphere (shown in blue) is mostly smooth lowlands and has experienced extensive volcanism. The southern hemisphere (in orange) has an older, cratered highland surface. This dichotomy could have been caused by a giant impact. Credit: University of Arizona/LPL/SwRI
New research has revealed that a giant impact on Mars more than 4 billion years ago would explain the unusual amount of “iron loving” elements in the Red Planet. Planets form as small dust grains stick together and agglomerate with other grains, leading to bigger bodies termed “planetesimals...
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