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arXiv · 1403.6849

Observing Planetary Rings with JWST: Science Justification and Observation Requirements

Matthew S. Tiscareno·Mark R. Showalter·Richard G. French·Joseph A. Burns·Jeffrey N. Cuzzi·Imke de Pater·Douglas P. Hamilton·Matthew M. Hedman·Philip D. Nicholson·Daniel Tamayo·Anne J. Verbiscer·Stefanie N. Milam·John A. Stansberry
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Abstract

The James Webb Space Telescope (JWST) will provide unprecedented opportunities to observe the rings and small satellites in our solar system, accomplishing three primary objectives: 1) discovering new rings and moons, 2) unprecedented spectroscopy, and 3) time-domain observations. We give details on these science objectives and describe requirements that JWST must fulfill in order to accomplish the science objectives

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Matthew S. Tiscareno, Mark R. Showalter, Richard G. French, Joseph A. Burns, Jeffrey N. Cuzzi, Imke de Pater, Douglas P. Hamilton, Matthew M. Hedman, Philip D. Nicholson, Daniel Tamayo, Anne J. Verbiscer, Stefanie N. Milam, John A. Stansberry. 2014-03-26. Observing Planetary Rings with JWST: Science Justification and Observation Requirements. https://arxiv.org/abs/1403.6849

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