OWL-Moon: Very high resolution spectropolarimetric interferometry and imaging from the Moon: exoplanets to cosmology
Instrumentation and Methods for Astrophysics2022-08-23v1Cosmology and Nongalactic AstrophysicsEarth and Planetary AstrophysicsAstrophysics of GalaxiesSolar and Stellar Astrophysics
We outline a concept for OWL-Moon, a 50-100m aperture telescope located on the surface of the Moon, to address three major areas in astronomy, namely the detection of biosignatures on habitable exoplanets, the geophysics of exoplanets, and cosmology. Such a large lunar telescope, when coupled with large Earth-based telescopes, would allow Intensity Interferometric measurements, leading to pico-arcsecond angular resolution. This would have applications in many areas of astronomy and is timely in light of the renewed interest of space agencies in returning to the Moon.
@article{arxiv.2208.05971,
title = {OWL-Moon: Very high resolution spectropolarimetric interferometry and imaging from the Moon: exoplanets to cosmology},
author = {Jean Schneider and Joseph Silk and Farrokh Vakili},
journal= {arXiv preprint arXiv:2208.05971},
year = {2022}
}
Comments
Accepted in Experimental Astronomy. arXiv admin note: substantial text overlap with arXiv:1908.02080