2020
DOI: 10.1098/rsta.2020.0141
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A 20 m wide-field diffraction-limited telescope

Abstract: A 20 m space telescope is described with an unvignetted 1° field of view—a hundred times larger in area than fields of existing space telescopes. Its diffraction-limited images are a hundred times sharper than from wide-field ground-based telescopes and extend over much if not all the field, 40 arcmin diameter at 500 nm wavelength, for example. The optical system yielding a 1°, 1.36 m diameter image at f/3.9 has relatively small central obscuration, 9% by area on axis, and is fully baffled. Several carousel-mo… Show more

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Cited by 7 publications
(3 citation statements)
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“…There are many issues to be discussed [2178][2179][2180][2181][2182][2183][2184][2185][2186][2187][2188][2189][2190][2191][2192][2193], including how to discriminate the elusive science signals from pervasive low radio frequency and terahertz foregrounds, and handling the abrasive role of lunar dust. One can add imaging via mega-telescopes in dark and cold polar craters and making use of the seismic stability of the Moon for deployment of GW telescopes, using technology that dates back to, and goes far beyond, the Apollo-era era seismometers.…”
Section: Lunar Astronomymentioning
confidence: 99%
“…There are many issues to be discussed [2178][2179][2180][2181][2182][2183][2184][2185][2186][2187][2188][2189][2190][2191][2192][2193], including how to discriminate the elusive science signals from pervasive low radio frequency and terahertz foregrounds, and handling the abrasive role of lunar dust. One can add imaging via mega-telescopes in dark and cold polar craters and making use of the seismic stability of the Moon for deployment of GW telescopes, using technology that dates back to, and goes far beyond, the Apollo-era era seismometers.…”
Section: Lunar Astronomymentioning
confidence: 99%
“…I assume here an observatory design specially tailored for such a mission, however the goals of the DRAKE mission could equally be achieved as a specific component of a general purpose observatory project. Possible locations include deep space, such as the L2 Lagrange point or a location on the Moon, such as the Shackleton crater at the lunar South Pole (Schneider et al 2021;Eads & Angel 2021). Each location has advantages and disadvantages.…”
Section: Observatory Designmentioning
confidence: 99%
“…The possibilities for ultrahigh-resolution imaging of the nearest exoplanets with a lunar hyper-telescope array in the optical/IR are described by Antoine Labeyrie [8]. The case is made for constructing a large telescope observatory using lunar regolith (Nick Woolf and Roger Angel [9]), along with the design for a diffraction-limited 20 m lunar telescope (Ryker Eads and Roger Angel [10]).…”
mentioning
confidence: 99%