Monday 6 May 2013
       Pygmy, in anthropology, member of any human group whose adult males grow to less than 59 inches (150 cm) in average height. A member of a slightly taller group is termed pygmoid.
The best-known Pygmy groups and those to whom the term is most commonly applied are the Pygmies of tropical Africa; elsewhere in Africa some of the San (Bushmen) of the Kalahari are of Pygmy size. There are also Pygmy groups, commonly known as Negritos, in Asia. Similarities in the physical features of the African and Asian groups are a result of their long period of adaptation to similar environments.

Virtually all Pygmy peoples are hunters and gatherers, practicing neither agriculture nor cattle raising. Most maintain close symbiotic relations with other groups in their region; consequently most have lost their indigenous languages and adopted that of their neighbours.

The famous Pygmy groups of the Ituri Forest in Congo (Kinshasa) present an example of a culture unchanging as a result of acculturation with neighbouring peoples. Known collectively as the Bambuti (Mbuti), they are probably the earliest inhabitants of the region.

Another well-known Pygmy group in equatorial Africa are the Twa (Batwa), who live in the high mountains and plains around Lake Kivu, in Congo,
                                           Researchers at The University of Auckland have proposed a new method for finding Earth-like planets and they anticipate that the number will be in the order of 100 billion.
The strategy uses a technique called gravitational microlensing, currently used by a Japan-New Zealand collaboration called MOA (Microlensing Observations in Astrophysics) at New Zealand’s Mt John Observatory.
Lead author Dr Phil Yock from the University of Auckland’s Department of Physics explains that the work will require a combination of data from microlensing and the NASA Kepler space telescope.
“Kepler finds Earth-sized planets that are quite close to parent stars, and it estimates that there are 17 billion such planets in the Milky Way. These planets are generally hotter than Earth, although some could be of a similar temperature (and therefore habitable) if they're orbiting a cool star called a red dwarf.”
“Our proposal is to measure the number of Earth-mass planets orbiting stars at distances typically twice the Sun-Earth distance. Our planets will therefore be cooler than the Earth. By interpolating between the Kepler and MOA results, we should get a good estimate of the number of Earth-like, habitable planets in the Galaxy. We anticipate a number in the order of 100 billion.”
“Of course, it will be a long way from measuring this number to actually finding inhabited planets, but it will be a step along the way.”

The first planet orbiting a Sun-like star was not found until 1995, despite strenuous efforts by astronomers. Dr Yock explains that this reflects the difficulty of detecting from a distance a tiny non-luminous object like Earth orbiting a bright object like the Sun. The planet is lost in the glare of the star, so indirect methods of detection must be used.
Whereas Kepler measures the loss of light from a star when a planet orbits between us and the star, microlensing measures the deflection of light from a distant star that passes through a planetary system en route to Earth – an effect predicted by Einstein in 1936.
In recent years, microlensing has been used to detect several planets as large as Neptune and Jupiter. Dr Yock and colleagues have proposed a new microlensing strategy for detecting the tiny deflection caused by an Earth-sized planet. Simulations carried out by Dr Yock and his colleagues – students and former students from The University of Auckland and France – showed that Earth-sized planets could be detected more easily if a worldwide network of moderate-sized, robotic telescopes was available to monitor them.
Coincidentally, just such a network of 1m and 2m telescopes is now being deployed by Las Cumbres Observatory Global Telescope Network (LCOGT) in collaboration with SUPA/St Andrews (Scottish Universities Physics Alliance),
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