Darwin (spacecraft)

Darwin
Mission typeInterferometric observatory
OperatorESA
Websitewww.esa.int/science/darwin
Orbital parameters
Reference systemSun–Earth L2
RegimeHalo orbit
Epochplanned

Darwin was a suggested ESA Cornerstone mission which would have involved a constellation of four to nine[2] 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.[3]

The study of this proposed mission ended in 2007 with no further activities planned.[1] 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.[4] Several more detailed studies would have been needed to determine whether technology capable of such precision is actually feasible.[2]

  1. ^ a b "Darwin factsheet: Finding Earth-like planets". European Space Agency. 2009-10-23. Archived from the original on 2008-05-13. Retrieved 2009-10-27.
  2. ^ a b c "Darwin: study ended, no further activities planned". European Space Agency. 2009-10-23. Retrieved 2009-10-27.
  3. ^ Cite error: The named reference Bulletin103-2000 was invoked but never defined (see the help page).
  4. ^ Penny, Alan J (1999-07-27). "A concept for the 'Free-Flyer' version". Rutherford Appleton Laboratory. Archived from the original on 2005-10-28. Retrieved 2009-10-30.