Imran Mehdi,1 Paul von Allmen,1 Jacob Kooi,1 Mathieu Choukroun,1 Paul F. Goldsmith,1 Darren Hayton,1 Bruce Bumble,1 Pierre Echternach,1 Sabrina Feldman1
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Remote submm-wave spectrometers have the capability of providing statistically significant numbers of isotopic composition measurements within the budget constraints of available planetary missions. This talk will present a mission and instrument concept that would enable an accurate measurement of the D/H ratio on not one but several dozens of comets in a four-year mission lifetime. The instrument would utilize advanced cryogenic detectors that would allow us to measure the abundance of the para and ortho spin states of water and its isotopologues. State of the art superconducting heterodyne receivers have been developed that provide detection sensitivities approaching the quantum limit in the 500 GHz frequency range enabling the measurement of D/H ratio on around 50 comets from an observatory stationed for example at the thermally benign Lagrange point L2
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Imran Mehdi, Paul von Allmen, Jacob Kooi, Mathieu Choukroun, Paul F. Goldsmith, Darren Hayton, Bruce Bumble, Pierre Echternach, Sabrina Feldman, "A submm-wave comet explorer for water isotopic composition measurements," Proc. SPIE 10698, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave, 106980F (24 July 2018); https://doi.org/10.1117/12.2313041