EGU23-10186, updated on 26 Feb 2023
https://doi.org/10.5194/egusphere-egu23-10186
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

The First Observations of Deimos by the Emirates Mars Ultraviolet Spectrometer (EMUS)

Gregory Holsclaw1, Justin Deighan1, Michael Chaffin1, Hessa Al Matroushi2, Robert Lillis3, Matthew Fillingim3, Scott England4, Sonal Jain1, Fatma Lootah2, Hoor Al Mazmi5, Gabriel Bershenyi1, Emily Pilinski1, Thibaud Teil1, Jeff Parker6, and Omran Sharaf2
Gregory Holsclaw et al.
  • 1Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO, USA
  • 2Mohammed Bin Rashid Space Centre, Dubai, UAE
  • 3Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, UAE
  • 4Virginia Polytechnic Institute and State University, Aerospace and Ocean Engineering, Blacksburg, VA, USA
  • 5UAE Space Agency, Abu Dhabi, UAE
  • 6Advanced Space LLC, Westminster, CO, USA

The Emirates Mars Mission (EMM) Hope probe launched on 20 Jul 2020 and entered Mars orbit on 9 Feb 2021, carrying a payload of 3 complementary instruments to characterize the global atmosphere across the full range of altitudes (surface to exosphere) at diurnal and seasonal timescales.  The unique, high-altitude orbit of the Hope probe (19,970 km periapse, 42,650 km apoapse altitude, 25 deg inclination, 54.5-hour period) that enables its synoptic view of the red planet also brings the spacecraft across the orbit of Mars’ outermost moon, Deimos.  The Hope trajectory was slightly modified by two maneuvers in Aug 2022 and Jan 2023 that will allow the surface of Deimos to be observed in a series of flybys in Feb-Mar 2023.  Here we present preliminary results from the Emirates Mars Ultraviolet Spectrometer (EMUS), an imaging spectrograph with a wavelength range of 100-170 nm and a field of view of 10.75 x 0.18 deg (using the high-resolution slit position).  We will derive the absolute reflectance of the surface, search for any compositionally distinct spectral features (e.g. carbon, polycyclic aromatic hydrocarbons, water ice), and examine any spatial heterogeneity across the surface.

How to cite: Holsclaw, G., Deighan, J., Chaffin, M., Al Matroushi, H., Lillis, R., Fillingim, M., England, S., Jain, S., Lootah, F., Al Mazmi, H., Bershenyi, G., Pilinski, E., Teil, T., Parker, J., and Sharaf, O.: The First Observations of Deimos by the Emirates Mars Ultraviolet Spectrometer (EMUS), EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-10186, https://doi.org/10.5194/egusphere-egu23-10186, 2023.