Astronomical Optical Interferometry from the Lunar Surface
astro-ph.IM
/ Authors
Gerard van Belle, Tabetha Boyajian, Michelle Creech-Eakman, John Elliott, Kimberly Ennico-Smith, Dan Hillsberry, Kevin Hubbard, Takahiro Ito, Shri Kulkarni, Connor Langford
and 21 more authors
Laura Lee, David Leisawitz, Eric Mamajek, May Martin, Taro Matsuo, Dimitri Mawet, John Monnier, Jon Morse, Dave Mozurkewich, Paul Niles, Mark Panning, Lori Pigue, Aniket Sanghi, Gail Schaefer, Jeremy Scott, Stuart Shaklan, Locke Spencer, Aaron Tohuvavohu, Peter Tuthill, Karel Valenta, Jordan Wachs
/ Abstract
The lunar surface is a compelling location for large, distributed optical facilities, with significant advantages over orbital facilities for high spatial resolution astrophysics. The serious development of mission concepts is timely because of the confluence of multiple compelling factors. Lunar access technology is maturing rapidly, in the form of both US-based crewed and uncrewed landers, as well as international efforts. Associated with this has been a definitive maturation of astronomical optical interferometry technologies at Earth-based facilities over the past three decades, enabling exquisitely sharp views on the universe previously unattainable, though limited at present by the Earth's atmosphere. Importantly, the increasing knowledge and experience base about lunar surface operations indicates it is not just suitable, but highly attractive for lunar telescope arrays.