The science enabled by a dedicated solar system space telescope
The National Academy Committee on Astrobiology and Planetary Science (CAPS) made a recommendation to study a large/medium-class dedicated space telescope for planetary science, going beyond the Discovery-class dedicated planetary space telescope endorsed in Visions and Voyages. Such a telescope woul...
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Zusammenfassung: | The National Academy Committee on Astrobiology and Planetary Science (CAPS)
made a recommendation to study a large/medium-class dedicated space telescope
for planetary science, going beyond the Discovery-class dedicated planetary
space telescope endorsed in Visions and Voyages. Such a telescope would observe
targets across the entire solar system, engaging a broad spectrum of the
science community. It would ensure that the high-resolution, high-sensitivity
observations of the solar system in visible and UV wavelengths revolutionized
by the Hubble Space Telescope (HST) could be extended. A dedicated telescope
for solar system science would: (a) transform our understanding of
time-dependent phenomena in our solar system that cannot be studied currently
under programs to observe and visit new targets and (b) enable a comprehensive
survey and spectral characterization of minor bodies across the solar system,
which requires a large time allocation not supported by existing facilities.
The time-domain phenomena to be explored are critically reliant on high spatial
resolution UV-visible observations. This paper presents science themes and key
questions that require a long-lasting space telescope dedicated to planetary
science that can capture high-quality, consistent data at the required cadences
that are free from effects of the terrestrial atmosphere and differences across
observing facilities. Such a telescope would have excellent synergy with
astrophysical facilities by placing planetary discoveries made by astrophysics
assets in temporal context, as well as triggering detailed follow-up
observations using larger telescopes. The telescope would support future
missions to the Ice Giants, Ocean Worlds, and minor bodies across the solar
system by placing the results of such targeted missions in the context of
longer records of temporal activities and larger sample populations. |
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DOI: | 10.48550/arxiv.2008.08069 |