The Observations of Deimos from the Emirates Mars Infrared Spectrometer (EMIRS)
- 1Northern Arizona University, Department of Astronomy and Planetary Science, Flagstaff, United States of America (nathan.smith@nau.edu)
- 2Space Science Institute, Boulder, CO, USA
- 3Mars Space Flight Facility, Arizona State University, Tempe, AZ, USA
- 4Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO, USA
- 5Mohammed Bin Rashid Space Centre, Dubai, UAE
- 6Advanced Space, Westminster, CO, USA
We present the initial views of the surface of Mars’ outer moon Deimos as observed by the Emirates Mars InfraRed Spectrometer (EMIRS), a Fourier transform infrared spectrometer observing from 6-50 µm with a spectral sampling of up to 5 cm-1. The primary science goal of the Emirates Mars Mission (EMM) is to study the variability in Mars’ atmosphere. As part of a coordinated campaign, the EMM spacecraft has adjusted its orbit into a resonance with Deimos, where it will periodically fly by the moon. Beginning the spring of 2023, EMIRS will collect numerous thermal infrared spectra of Deimos’ surface with a spatial resolution ranging from ~1-10 km. These observations will be the best-resolved infrared views of Deimos to date. Our planned observations achieve nearly complete global coverage of the surface, and span a range of local solar times, enabling investigations of both compositional and thermophysical properties. We will discuss these observations and initial findings.
How to cite: Smith, N., Edwards, C., Osterloo, M., Christensen, P., Anwar, S., Pilinski, E., Wren, P., Noss, D., Rios, K., Dickenshied, S., Al Matroushi, H., Deighan, J., Parker, J., and Sharaf, O.: The Observations of Deimos from the Emirates Mars Infrared Spectrometer (EMIRS), EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-10291, https://doi.org/10.5194/egusphere-egu23-10291, 2023.