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Welcome to Everything Science
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Super atoms turn the periodic table upside down |
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Everything Physical Science
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Written by Everything Science
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Researchers at Delft University of Technology (TU Delft) in The Netherlands have developed a technique for generating atom clusters made from silver and other metals. Surprisingly enough, these so-called super atoms (clusters of 13 silver atoms, for example) behave in the same way as individual atoms and have opened up a whole new branch of chemistry. A full account can be read in the new edition of TU Delft magazine Delft Outlook.
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| A small twisted wire, just like the filament in an incandescent bulb, but made of silver, forms the basis for the special silver particles. |
If a silver thread is heated to around 900 degrees Celsius, it will generate vapour made up of silver atoms. The floating atoms stick to each other in groups. Small lumps of silver comprising for example 9, 13 and 55 atoms appear to be energetically stable and are therefore present in the silver mist more frequently that one might assume. Prof. Andreas Schmidt-Ott and Dr. Christian Peineke of TU Delft managed to collect these super atoms and make them suitable for more detailed chemical experiments.
Science
The underlying mechanism governing this stability in super atoms was described in Science by scientists from Virginia Commonwealth University in 2005. They had discovered metal super atoms, but from aluminium. Their aluminium clusters of 13, 23 and 37 atoms reacted in the same way as individual atoms because they comprised electrons that revolved around the atom cluster as a whole. These so-called outer layers were strikingly similar to the outer layers of elements from the periodic table.
The super atoms gave the periodic table a third dimension as it were, according to Schmidt-Ott: ‘The chemical properties of the super atoms that have been identified up until now are very similar to those of elements in the periodic table, because their outer layers are much the same. However, we may yet discover super atoms with a different outer layer, giving us another set of completely new properties.’ (1) Comments posted about this in the forum |
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University of Kent conservationist to aid parrots in peril |
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Everything Biology
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Written by Everything Science
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A once critically endangered species of parrot now under threat from a highly contagious virus may be offered a renewed chance of survival by a conservationist at the University of Kent.
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| Mauritius parrot. Copyright: Gregory Guida 2007 |
Dr Jim Groombridge, Lecturer in Biodiversity Conservation at the University’s Durrell Institute of Conservation and Ecology (DICE), has been awarded £215,594 from the Leverhulme Trust to lead a three-year project that aims to determine what factors drive the Mauritius parakeet’s susceptibility to infection, and in particular the spread of the highly contagious (and often lethal) parrot-specific virus Psittacine Beak and Feather Disease (PBFD) that has recently infected this endangered parrot.
This project is all the more important given that the once widespread population of the Mauritius parakeet (Psittacula echo) fell to just 12 individuals by 1987, following a century of habitat loss and competition from the introduced ringneck parakeet. However, following a highly successful avian restoration programme, numbers of Mauritian parakeets eventually recovered to 350 birds (resulting in its downgrading from critically endangered to endangered) but in 2004 an outbreak of PBFD threatened this still recovering population.
Alongside its principal aim of providing important guidance for managing the disease-problems encountered by this endangered parrot, the project will also provide equally important guidance for managing infectious disease in species conservation programmes worldwide. In addition, it will provide a rare opportunity to study the epidemiology of infectious disease as extensive data is available from 20 years of careful monitoring of both the Mauritius parakeet and a closely related, introduced species of parakeet. (1) Comments posted about this in the forum |
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An extraterrestrial's view of the Earth |
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Everything Space
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Written by Everything Science
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Searchers for habitable planets in the Milky Way have found a new ally. According to research led by astronomers from the Instituto de Astrofisica de Canarias (IAC), clouds can provide enough information to determine the period of rotation of a planet and deduce the variability of its atmosphere. Owing to the role played by clouds, which are so commonplace on Earth but unique in the Solar System for their dynamism, it could suffice scientists to analyse the brightness of a planet to ascertain the length of its day and determine whether or not there is water on its surface.
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Photograph of the Earth in which agglomerations of clouds and the brightness reflected by the illuminated face of our planet can be seen. Terrestrial clouds can reflect up to 80% of the light they receive. Credit: Gabriel Pérez, IAC (Multimedia Service)
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Clouds are indicative of atmospheric pressure and existing temperature. Terrestrial cloud cover can be seen this three-dimensional representation, obtained from combined measurments from various meteorological satellites. The cloud distribution is represented during the phenomenon known as "El Niño" (1997-98) and shows anomalies in sea surface temperatures. Credit: NASA.
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From data obtained over two decades (1984-2005) by a network of meteorological satellites from all over the world, astronomers Enric Pallé, Pilar Monañés-Rodríguez and Manuel Vázquez from the IAC, together with Eric Ford from the University of Florida and Sara Seager of the Massachusetts Institute of Technology, have produced a computer-generated model of the Earth's brightness. Results have shown that, if observed as a point source, such as an extraterrestrial observer would view it, the Earth's cloud mass would follow a repetitive pattern with a certain frequency.
"The trick lies in interpreting the movement of the Earth's surface and the clouds as periodical signals, just as if we were to observe the spots on a spinning ball appearing and disappearing", explains Enric Pallé, first author of an article to be published next month in the American Astrophysical Journal.
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ALMA Antenna Transporter Presentation |
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Everything Space
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Written by Everything Science
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Today, the first of the two ALMA antenna transporters was given its name at a ceremony on the compounds of the manufacturer, the heavy-vehicle specialist Scheuerle Fahrzeugfabrik GmbH, in Baden-Württemberg. The colossus, 10 metres wide, 20 metres long and 6 metres high, will be shipped to Chile by the end of the month. The second one will follow in a few weeks.  | With a size of 10 metres wide, 20 metres long and 6 metres high, the ALMA antenna transporter is a real colossus. (c) ESO |
The transporter was named 'Otto' in honour of Otto Rettenmaier, the owner of the Scheuerle company. "The rather unusual move to name a vehicle is a recognition of the remarkable achievement these unique machines represent," said Hans Rykaczewski, the European ALMA Project Manager. "Their sizes alone would justify using superlatives to describe them. But they are also outstanding as they will operate at 5000 metres altitude, where the air is rare, and they have to be able to place 115-ton antennas with a precision of a few millimetres," he added.
"The ALMA antenna transporters are the proof of the excellence of our staff and of our ability to build heavy vehicles that are at the limits of the possible," said Otto Rettenmaier. "Never in the history of our company have we had to comply with such exceptional requirements on material and techniques as we had to do with these machines. We are proud as a company to have been able to contribute with such an exceptional piece of technology for astronomical research."
The ALMA Project, in which ESO leads the construction and the operations on behalf of Europe, is a giant, international observatory currently in construction on the high-altitude Chajnantor site in Chile, which will be composed initially of 66 high-precision telescopes, operating at wavelengths of 0.3 to 9.6 mm. The ALMA antennas will be electronically combined and provide astronomical observations which are equivalent to a single large telescope of tremendous size and resolution.
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