With the newest radio
telescope ALMA, the researchers propose to open a whole new era in decode the
chemical universe. Research group that works with the radio telescope has
already established incredible ability ALMA during the study of the interstellar
gas, which is in the constellation of Orion.
Molecule, while in
space, vibrate and rotate, with each of them has its own unique
"signature." Each time a molecule changes its state, by absorption or
excretion huge amounts of energy, which can "see" in the form of
electromagnetic radiation.
Due to its special
features, the radio telescope ALMA gives scientists previously unavailable to
them enough speed to study large areas of the sky, while defining the chemical
composition of even the most remote corners of the cosmos. Precisely because of
this, became available for research that was previously simply not possible
from due to its complexity.
For instance, the
example of studies of gas-dust clouds. Which is located in the constellation of
Orion, the scientists were able to accurately analyze the region of star
formation, where the stars are actively forming of the available gas and dust,
while creating entire star system. The goal of the first test the capabilities
of the telescope ALMA, was taken to the search space of traces of ethyl
cyanide, the formula of which is CH3CH2CN. This material has been repeatedly
found, and it is an ideal test sample for what would analyze the quality and
speed of this new astronomical tool. Spectral lines, which have been given a
telescope ALMA, fully confirmed the presence of the desired substance in a
given region of space, in particular the specific molecules corresponding ethyl
cyanide. Thus, scientists have confirmed the suitability of this telescope as a
new and very powerful astronomical telescope, which is able to carry out
chemical spectral analysis of the most remote regions of space.
Himself being completed
ALMA telescope in the Atacama Desert, which is located in northern Chile, is he
will be at an altitude of 5000 meters above sea level. Once in 2013, will be
completed 66 high-precision antennas, advanced capabilities of this telescope
will be able to open to scientists for more than impressive prospects for the
study of the universe, using the range of the infrared and very long waves.
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