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Πέμπτη 25 Φεβρουαρίου 2016

Exoplanets spectroscopy with diffraction primary objective telescopes -T...

                  



Exoplanets spectroscopy with diffraction primary objective telescopes -T...

Δημοσιεύτηκε στις 22 Φεβ 2016
When
diffraction is employed as the primary collector modality of a
telescope instead of reflection or refraction, a new set of performance
capabilities emerges. A diffraction-based telescope forms a spectrogram
first and an image as secondary data. The results are startling. In
multiple object capability, the diffraction telescope on earth can
capture 2 million spectra to R bigger than 100,000 in a single night,
better for a census of exoplanets by radial velocity than any prior art.
In a space telescope in a direct observation mode, this type
diffraction primary objective could reveal spectral analyses of
individual exoplanets. We introduce three embodiments: THE MOST, HOMES
and ADEDPT.

Tom Ditto has served as a Fellow of NASA Advanced
Innovative Concepts and a P.I. in the National Science Foundation SBIR
program working in holographic optics. He is also a Fellow of the
Guggenheim Foundation, National Endowment for the Arts, and the American
Film Institute. He promises a rousing media presentation.
ANAΡΤΗΣΗ ΑΠΟ ΤΟ YOUTUBE 26/2/2016

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