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Department of Physics
Credit: Jack Hobhouse

Dr Tristram Warren

Head of Infrared Multilayer Laboratory

Sub department

  • Professional and support services

Research groups

  • Planetary surfaces
  • Solar system
  • Space instrumentation
Tristram.Warren@physics.ox.ac.uk
Telephone: 01865 (2)82436
Atmospheric Physics Clarendon Laboratory, room 304
  • About
  • Publications

LIRIS: demonstrating how small satellites can revolutionise lunar science data sets

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 13546 (2025) 135460d-135460d-9

Authors:

A Harvey, L Middlemass, J Friend, N Bowles, T Warren, S Eckersley, S Knox, B Hooper, A da Silva Curiel, K Nowicki, K Shirley
More details from the publisher

The Peregrine Ion Trap Mass Spectrometer (PITMS): Results from a CLPS-delivered Mass Spectrometer

The Planetary Science Journal American Astronomical Society 6:1 (2025) 14

Authors:

Barbara A Cohen, Simeon J Barber, Aleksandra J Gawronska, Feargus AJ Abernethy, Natalie M Curran, Phillip A Driggers, William M Farrell, David J Heather, Christopher Howe, Peter F Landsberg, Veneranda López-Días, Andrew D Morse, Thomas Morse, Michael J Poston, Parvathy Prem, Roland Trautner, Orenthal J Tucker, Tristram J Warren, Stefano Boccelli
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Bidirectional reflectance distribution function measurements of characterized Apollo regolith samples using the visible oxford space environment goniometer

Meteoritics and Planetary Science Wiley 59:11 (2024) 3111-3123

Authors:

RJ Curtis, TJ Warren, KA Shirley, DA Paige, NE Bowles
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Characterization of sites of scientific interest for ESA's PROSPECT instrument

Icarus Elsevier 421 (2024) 116240

Authors:

Sj Boazman, D Heather, M Hutton, M Schwinning, A Frigeri, N Schmitz, S Besse, M Formisano, C De Sanctis, C Gscheidle, C Orgel, P Reiss, E Sefton-Nash, T Warren

Abstract:

Many upcoming lunar missions and payloads are targeting the south pole of the Moon, due to the volatiles potentially harboured in this region including ESA's PROSPECT instrument. PROSPECT is designed to sample the lunar regolith within the first meter of the surface and to analyse any volatiles found. Remote sensing methods and a range of datasets including thermal models, illumination models, LRO NAC images, LOLA DEMs and LRO NAC DEMs generated with shape-from-shading, were used to identify suitable areas for PROSPECT science within the south polar region (84–90°S). Sites identified were down selected using a science matrix and scoring sites of interest based on if and how well the point of interest met the science requirements of PROSPECT. The highest scoring sites are presented and proposed to be ideal candidate landing sites for missions targeting the lunar south polar region, especially for missions that are interested in sampling volatiles, micro cold traps and Permanently Shaded Regions (PSRs). Understanding and sampling these colder areas within the south polar region will advance the understanding of volatiles within the lunar surface and volatile transfer.
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Details from ORA

Morphological analysis of polar landing regions for a solar powered ice drilling mission

Icarus Elsevier 411 (2024) 115927

Authors:

R Tomka, V Steinmann, T Warren, A Kereszturi
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