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Enceladus' Damascus Sulci

Dr Carly Howett

Associate Professor of Space Instrumentation

Research theme

  • Exoplanets and planetary physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Planetary surfaces
  • Solar system
  • Space instrumentation
carly.howett@physics.ox.ac.uk
Atmospheric Physics Clarendon Laboratory, room 314
  • About
  • Publications

The formation of Charon's red poles from seasonally cold-trapped volatiles

Nature 539:7627 (2016) 65-68

Authors:

WM Grundy, DP Cruikshank, GR Gladstone, CJA Howett, TR Lauer, JR Spencer, ME Summers, MW Buie, AM Earle, K Ennico, JW Parker, SB Porter, KN Singer, SA Stern, AJ Verbiscer, RA Beyer, RP Binzel, BJ Buratti, JC Cook, CM Dalle Ore, CB Olkin, AH Parker, S Protopapa, E Quirico, KD Retherford, SJ Robbins, B Schmitt, JA Stansberry, OM Umurhan, HA Weaver, LA Young, AM Zangari, VJ Bray, AF Cheng, WB McKinnon, RL McNutt, JM Moore, F Nimmo, DC Reuter, PM Schenk, F Bagenal, T Andert, O Barnouin, M Bird, M Brozović, HA Elliott, TK Greathouse, M Hahn, DP Hamilton, ME Hill, DP Hinson, J Hofgartner, M Horányi, AD Howard, DE Jennings, JA Kammer, P Kollmann, P Lavvas, IR Linscott, CM Lisse, AW Lunsford, DJ McComas, M Mutchler, JI Nunez, M Paetzold, S Philippe, M Piquette, HJ Reitsema, JH Roberts, K Runyon, E Schindhelm, MR Showalter, AJ Steffl, DF Strobel, T Stryk, JR Szalay, HB Throop, CCC Tsang, GL Tyler, MH Versteeg, GE Weigle, OL White, WW Woods, EF Young

Abstract:

© 2016 Macmillan Publishers Limited, part of Springer Nature. All rights reserved. A unique feature of Pluto's large satellite Charon is its dark red northern polar cap. Similar colours on Pluto's surface have been attributed to tholin-like organic macromolecules produced by energetic radiation processing of hydrocarbons. The polar location on Charon implicates the temperature extremes that result from Charon's high obliquity and long seasons in the production of this material. The escape of Pluto's atmosphere provides a potential feedstock for a complex chemistry. Gas from Pluto that is transiently cold-trapped and processed at Charon's winter pole was proposed as an explanation for the dark coloration on the basis of an image of Charon's northern hemisphere, but not modelled quantitatively. Here we report images of the southern hemisphere illuminated by Pluto-shine and also images taken during the approach phase that show the northern polar cap over a range of longitudes. We model the surface thermal environment on Charon and the supply and temporary cold-trapping of material escaping from Pluto, as well as the photolytic processing of this material into more complex and less volatile molecules while cold-trapped. The model results are consistent with the proposed mechanism for producing the observed colour pattern on Charon.
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Pluto's global surface composition through pixel-by-pixel Hapke modeling of New Horizons Ralph/LEISA data

(2016)

Authors:

S Protopapa, WM Grundy, DC Reuter, DP Hamilton, CM Dalle Ore, JC Cook, DP Cruikshank, B Schmitt, S Philippe, E Quirico, RP Binzel, AM Earle, K Ennico, CJA Howett, AW Lunsford, CB Olkin, A Parker, KN Singer, A Stern, AJ Verbiscer, HA Weaver, LA Young, the New Horizons Science Team
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Dual-telescope multi-channel thermal-infrared radiometer for outer planet fly-by missions

Acta Astronautica Elsevier 128 (2016) 628-639

Authors:

Shahid Aslam, Michael Amato, Neil Bowles, Simon Calcutt, Tilak Hewagama, Joseph Howard, Carly Howett, Wen-Ting Hsieh, Terry Hurford, Jane Hurley, Patrick Irwin, Donald E Jennings, Ernst Kessler, Brook Lakew, Mark Loeffler, Michael Mellon, Anthony Nicoletti, Conor A Nixon, Nathaniel Putzig, Gerard Quilligan, Julie Rathbun, Marcia Segura, John Spencer, Joseph Spitale, Garrett West

Abstract:

The design of a versatile dual-telescope thermal-infrared radiometer spanning the spectral wavelength range 8–200 µm, in five spectral pass bands, for outer planet fly-by missions is described. The dual-telescope design switches between a narrow-field-of-view and a wide-field-of-view to provide optimal spatial resolution images within a range of spacecraft encounters to the target. The switchable dual-field-of-view system uses an optical configuration based on the axial rotation of a source-select mirror along the optical axis. The optical design, spectral performance, radiometric accuracy, and retrieval estimates of the instrument are discussed. This is followed by an assessment of the surface coverage performance at various spatial resolutions by using the planned NASA Europa Mission 13-F7 fly-by trajectories as a case study.
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The Geology of Pluto and Charon Through the Eyes of New Horizons

(2016)

Authors:

Jeffrey M Moore, William B McKinnon, John R Spencer, Alan D Howard, Paul M Schenk, Ross A Beyer, Francis Nimmo, Kelsi N Singer, Orkan M Umurhan, Oliver L White, S Alan Stern, Kimberly Ennico, Cathy B Olkin, Harold A Weaver, Leslie A Young, Richard P Binzel, Marc W Buie, Bonnie J Buratti, Andrew F Cheng, Dale P Cruikshank, Will M Grundy, Ivan R Linscott, Harold J Reitsema, Dennis C Reuter, Mark R Showalter, Veronica J Bray, Carrie L Chavez, Carly JA Howett, Tod R Lauer, Carey M Lisse, Alex Harrison Parker, SB Porter, Simon J Robbins, Kirby Runyon, Ted Stryk, Henry B Throop, Constantine CC Tsang, Anne J Verbiscer, Amanda M Zangari, Andrew L Chaikin, Don E Wilhelms
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Surface Compositions Across Pluto and Charon

(2016)

Authors:

WM Grundy, RP Binzel, BJ Buratti, JC Cook, DP Cruikshank, CM Dalle Ore, AM Earle, K Ennico, CJA Howett, AW Lunsford, CB Olkin, AH Parker, S Philippe, S Protopapa, E Quirico, DC Reuter, B Schmitt, KN Singer, AJ Verbiscer, RA Beyer, MW Buie, AF Cheng, DE Jennings, IR Linscott, J Wm Parker, PM Schenk, JR Spencer, JA Stansberry, SA Stern, HB Throop, CCC Tsang, HA Weaver, GE Weigle, LA Young, the New Horizons Science Team
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