Darwin$18907$ - ορισμός. Τι είναι το Darwin$18907$
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Τι (ποιος) είναι Darwin$18907$ - ορισμός

SUGGESTED ESA CORNERSTONE MISSION
Darwin interferometer; Darwin (ESA); Darwin mission; Darwin Spacecraft; Darwin Mission; Darwin (space telescope); Darwin telescope

Darwin, Tasmania         
FORMER TOWN IN TASMANIA, AUSTRALIA
Darwin Townsite, Tasmania
*See also the Australian federal electoral Division of Darwin (1903–1955) for the electoral division now known as Division of Braddon
Henry Darwin         
BRITISH LAWYER AND DIPLOMAT (1929-1992)
Henry Galton Darwin; Darwin, Henry
Henry Galton Darwin (6 November 1929 – 17 September 1992) was a British lawyer and diplomat specialising in international law.
Robin Darwin         
BRITISH ARTIST AND RECTOR OF THE ROYAL COLLEGE OF ART (1910-1974)
Robert Vere Darwin; Sir Robert Darwin; Sir Robin Darwin
Sir Robert Vere "Robin" Darwin KCB CBE RA RSA PRWA NEAC (7 May 1910 – 30 January 1974) was a British artist and Rector of the Royal College of Art.

Βικιπαίδεια

Darwin (spacecraft)

Darwin was a suggested ESA Cornerstone mission which would have involved a constellation of four to nine spacecraft designed to directly detect Earth-like planets orbiting nearby stars and search for evidence of life on these planets. The most recent design envisaged three free-flying space telescopes, each three to four metres in diameter, flying in formation as an astronomical interferometer. These telescopes were to redirect light from distant stars and planets to a fourth spacecraft, which would have contained the beam combiner, spectrometers, and cameras for the interferometer array, and which would have also acted as a communications hub. There was also an earlier design, called the "Robin Laurance configuration," which included six 1.5 metre telescopes, a beam combiner spacecraft, and a separate power and communications spacecraft.

The study of this proposed mission ended in 2007 with no further activities planned. To produce an image, the telescopes would have had to operate in formation with distances between the telescopes controlled to within a few micrometres, and the distance between the telescopes and receiver controlled to within about one nanometre. Several more detailed studies would have been needed to determine whether technology capable of such precision is actually feasible.