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Browsing by Author "Joy, Katherine H."

Browsing by Author "Joy, Katherine H."

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  • Foucher, F.; Hickman-Lewis, Keyron; Hutzler, Aurore; Joy, Katherine H.; Folco, L.; Bridges, John C.; Wozniakiewicz, P.; Martínez-Frías, Jesús; Debaille, V.; Zolensky, M. E. (Michael E.); Yano, H.; Bost, N.; Ferrière, Ludovic; Lee, M.; Michalski, J.; Schroeven-Deceuninck, H.; Kminek, G.; Viso, M.; Russell, Sara S. (Sara Samantha), 1966-; Smith, C.; Zipfel, J.; Westall, F.; https://orcid.org/0000-0003-4992-8750; https://orcid.org/0000-0002-2609-4485; https://orcid.org/0000-0002-3181-1303 (Elsevier, 2021-03-01)
    The practical limitations inherent to human and robotic planetary exploration necessitate the development of specific protocols and methods. This non-standard approach requires testing and validation phases in order to ...
  • Niihara, Takafumi; https://orcid.org/0000-0001-9535-6728; Joy, Katherine H.; https://orcid.org/0000-0003-4992-8750; Kring, David A. (David Allen); https://orcid.org/0000-0002-3440-6282 (Lunar and Planetary Institute, 2013-02-28)
    Joy et al. (2012) utilized a new element mapping routine that was developed to locate specific phases in complex crystalline or brecciated rocks. Several simple computer routines (macros) were developed to manage the data ...
  • Joy, Katherine H.; Crawford, Ian A.; Zolensky, M. E. (Michael E.); https://orcid.org/0000-0002-3181-1303; Fagan, Amy F.; Kring, David A. (David Allen); https://orcid.org/0000-0003-4992-8750; https://orcid.org/0000-0002-3440-6282 (Springer, 2016-10-19)
    In this review article, we discuss the evidence for populations of impactors delivered to the Moon at different times in the past. We also propose approaches to the identification and characterisation of meteoritic material ...
  • Joy, Katherine H.; https://orcid.org/0000-0003-4992-8750; Snape, J. F.; Nemchin, A. A.; Tartèse, Romain; Martin, D. M.; Whitehouse, M. J. (Martin J.); Vishnyakov, V.; Pernet-Fisher, J. F.; Kring, David A. (David Allen); https://orcid.org/0000-0002-3440-6282 (Royal Society, 2020)
    Apollo 16 soil-like regolith breccia 65745,7 contains two zircon-bearing clasts. One of these clasts is a thermally annealed silica-rich rock, which mineralogically has affinities with the High Alkali Suite (Clast 1), and ...

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