Share Email Print

Proceedings Paper

Advantages of placing an array of telescopes on the Moon to detect extrasolar planets
Author(s): Marija Strojnik ; Gonzalo Paez
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

We define the simplest signal-to-noise ratio to determine the optimal wavelength interval for extra-solar planet detection. For a solar system similar to our own, we find it to be one hundred times smaller than that considered earlier. We propose the planet detection in a spectral interval around 0.3mm (900 GHz) where high-altitude observatories report atmospheric transmission of about 0.4.

Paper Details

Date Published: 19 September 2013
PDF: 10 pages
Proc. SPIE 8867, Infrared Remote Sensing and Instrumentation XXI, 886712 (19 September 2013); doi: 10.1117/12.2022350
Show Author Affiliations
Marija Strojnik , Ctr. de Investigaciones en Óptica, A.C. (Mexico)
Gonzalo Paez, Ctr. de Investigaciones en Óptica, A.C. (Mexico)

Published in SPIE Proceedings Vol. 8867:
Infrared Remote Sensing and Instrumentation XXI
Marija Strojnik Scholl; Gonzalo Páez, Editor(s)

© SPIE. Terms of Use
Back to Top
Sign in to read the full article
Create a free SPIE account to get access to
premium articles and original research
Forgot your username?