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91̽»¨
Juno Jupiter image

Dr. Katherine Shirley (she/her)

Postdoctoral Research Assistant

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Planetary surfaces
  • Solar system
  • Space instrumentation
katherine.shirley@physics.ox.ac.uk
Atmospheric Physics Clarendon Laboratory, room 315
  • About
  • Publications

Returning to Mars with BEBOP (Broadband Exploration with Bolometric Optics)

Copernicus Publications (2024)

Authors:

Kevin S Olsen, Rory Evans, Henry Eshbaugh, Tristram J Warren, Katherine A Shirley, Keith Nowicki, Neil E Bowles

Extended Silicic Volcanism in the Gruithuisen Region—Revisiting the Composition and Thermophysical Properties of Gruithuisen Domes on the Moon

The Planetary Science Journal IOP Publishing 5:6 (2024) 132

Authors:

Nandita Kumari, Timothy D Glotch, Jean-Pierre Williams, Mark T Sullivan, Shuai Li, Benjamin T Greenhagen, Dany Waller, Tyler Powell, Catherine M Elder, Benjamin D Byron, Katherine A Shirley

Abstract:

The formation mechanisms, extent, and compositions of red spots on the lunar surface have intrigued the lunar community for decades. By identifying a new dome and another silicic crater in the highlands nearby, we find that the silicic volcanism in the Gruithuisen region extends beyond the three major domes. Our observations indicate that the Gruithuisen domes have low iron and titanium contents. They are enveloped by ejecta from surrounding regions and host silica-rich material excavated by the young craters consistent with previous work. Our boulder maps of the Gamma dome display a high boulder count and indicate that the Diviner rock abundance maps are only sensitive to boulders larger than ∼2 m. The H-parameter values are sensitive to presence of rocks and may be a better indicator of rocks at submeter scales. The Delta dome has gentle slopes, lower rock abundance, and one young crater, and it could serve as a safe and scientifically valuable site for landing and exploration of the domes and nearby region. The dome also displays anomalously high H-parameter in the same region as the crater, indicating the potential presence of pyroclastic materials. We observe up to 200 ppm of OH/H2O on the domes and nearby mare despite the presence of a weak magnetic field to the south of Delta dome, further 91̽»¨ing the potential presence of pyroclastics in the region. This study could potentially aid in logistical and scientific decisions of the future NASA missions in the region.

Destination: Space! A Virtual Flash Talk Series

Copernicus Publications (2024)

Authors:

Katherine Shirley, Helena Cotterill, Tristram Warren, Helena Bates, Robert Spry, Sian Tedaldi, Neil Bowles

The bulk mineralogy, elemental composition, and water content of the Winchcombe CM chondrite fall

Meteoritics and Planetary Science Wiley 59:5 (2024) 1006-1028

Authors:

HC Bates, AJ King, KS Shirley, E Bonsall, C Schröder, F Wombacher, T Fockenberg, RJ Curtis, NE Bowles

Effects of space weathering on the Christiansen feature position of lunar surface materials

Icarus Elsevier 412 (2024) 115976

Authors:

Nandita Kumari, Timothy D Glotch, Katherine A Shirley, Benjamin T Greenhagen, Benjamin D Byron

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