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Probing the regoliths of the classical Uranian satellites: Are their surfaces mantled by a layer of tiny H2O ice grains?

  • Published:2020-03 Issue: Volume:338 Page:113513
  • ISSN:0019-1035
  • Container-title:Icarus
  • language:en
  • Short-container-title:Icarus

Author:

Cartwright Richard J.,Emery Joshua P.,Grundy William M.,Cruikshank Dale P.,Beddingfield Chloe B.,Pinilla-Alonso Noemi

Funder

NASA Earth and Space Science Fellowship

NASA ROSES Solar System Observations

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference93 articles.

1. Polarimetry of major Uranian moons at the 6-m telescope;Afanasiev;Astrophys. Bull.,2014

2. Discovery of two distinct polarimetric behaviours of trans-Neptunian objects;Bagnulo;Astronomy & Astrophysics,2008

3. Polarimetry of small bodies of the solar system with large telescopes;Bagnulo;J. Quant. Spectrosc. Radiat. Transf.,2011

4. The near infrared spectrum of Miranda: evidence of crystalline water ice;Bauer;Icarus,2002

5. Hidden Tectonism on Miranda’s Elsinore Corona Revealed by Polygonal Impact Craters;Beddingfield,2019

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