Sub-field of view surface thermal modeling of Cassini CIRS observations of Rhea during south polar winter

Icarus Elsevier 377 (2022) 114910

Authors:

Georgina Miles, Carly JA Howett, John Spencer, Paul Schenk

Extreme exospheric dynamics at Charon: Implications for the red spot

Geophysical Research Letters Wiley 49:8 (2022) e2021GL097580

Authors:

B Teolis, U Raut, Ja Kammer, Cj Gimar, Cja Howett, Gr Gladstone, Kd Retherford

Abstract:

Charon's exosphere may exhibit extreme seasonal dynamics, with centuries of quiescence punctuated by short lived (∼4 earth years) exospheric surges near the equinoxes, as spring sunrise bi-annually drives frozen methane off the polar night zones. Charon's pole-centric red spot has been proposed to be the product of Ly-α photolysis of frozen methane into refractory hydrocarbon “tholins”, but the role of exospheric dynamics in the red material's formation has not been investigated. We show with exospheric modeling that methane “polar-swap”, in which exospheric CH4 sublimated from the spring polar zone is rapidly re-frozen onto the autumn hemisphere, deposits ∼30 μm polar frosts too thick for Ly-α light to penetrate. Ethane, the primary methane photoproduct under these conditions, may unlike methane remain frozen decades after polar sunrise under solar wind exposure. Solar wind radiolysis of polar ethane frost synthesizes higher-order refractories that may contribute to the coloration of Charon's polar zones.

Hypotheses for Triton's plumes: New analyses and future remote sensing tests

Icarus 375 (2022)

Authors:

JD Hofgartner, SPD Birch, J Castillo, WM Grundy, CJ Hansen, AG Hayes, CJA Howett, TA Hurford, ES Martin, KL Mitchell, TA Nordheim, MJ Poston, LM Prockter, LC Quick, P Schenk, RN Schindhelm, OM Umurhan

Abstract:

At least two active plumes were observed on Neptune's moon Triton during the Voyager 2 flyby in 1989. Models for Triton's plumes have previously been grouped into five hypotheses, two of which are primarily atmospheric phenomena and are generally considered unlikely, and three of which include eruptive processes and are plausible. These hypotheses are compared, including new arguments, such as comparisons based on current understanding of Mars, Enceladus, and Pluto. An eruption model based on a solar-powered, solid-state greenhouse effect was previously considered the leading hypothesis for Triton's plumes, in part due to the proximity of the plumes to the subsolar latitude during the Voyager 2 flyby and the distribution of Triton's fans that are putatively deposits from former plumes. The other two eruption hypotheses are powered by internal heat, not solar insolation. Based on new analyses of the ostensible relation between the latitude of the subsolar point on Triton and the geographic locations of the plumes and fans, we argue that neither the locations of the plumes nor fans are strong evidence in favor of the solar-powered hypothesis. We conclude that all three eruption hypotheses should be considered further. Five tests are presented that could be implemented with remote sensing observations from future spacecraft to confidently distinguish among the eruption hypotheses for Triton's plumes. The five tests are based on the: (1) composition and thickness of Triton's southern hemisphere terrains, (2) composition of fan deposits, (3) distribution of active plumes, (4) distribution of fans, and (5) surface temperature at the locations of plumes and/or fans. The tests are independent, but complementary, and implementable with a single flyby mission such as the Trident mission concept. We note that, in the case of the solar-driven hypothesis, the 2030s and 2040s may be the last chance for approximately a century to observe actively erupting plumes on Triton.

Exploring the Clouds of Venus: Science Driven Aerobot Missions to our Sister Planet

Institute of Electrical and Electronics Engineers (IEEE) 00 (2022) 1-20

Authors:

James Cutts, Kevin Baines, Leonard Dorsky, William Frazier, Jacob Izraelevitz, Siddharth Krishnamoorthy, Michael Pauken, Mark S Wallace, Paul Byrne, Sara Seager, Colin Wilson, Joseph O'Rourke

NASA's Lunar Trailblazer Mission: A Pioneering Small Satellite for Lunar Water and Lunar Geology

IEEE Aerospace Conference Proceedings 2022-March (2022)

Authors:

BL Ehlmann, RL Klima, CC Seybold, AT Klesh, MH Au, HA Bender, CL Bennett, DL Blaney, N Bowles, S Calcutt, D Copley-Woods, JL Dickson, K Djotni, KD Hanna, CS Edwards, R Evans, E Felder, R Fogg, RO Green, G Hawkins, M House, S Islas, G Lantoine, S Linch, T McCaa, I McKinley, TF Merkley, JK Miura, CM Pieters, W Santiago, E Scire, R Sherwood, K Shirley, C Smith, M Sondheim, P Sullivan, J Temples, DR Thompson, KI Waldorff, WR Williamson, TJ Warren, JL Wood, S Zareh

Abstract:

Selected in 2019 as a NASA SIMPLEx mission, Lunar Trailblazer is in implementation for flight system delivery at the end of 2022. The mission's goal is to understand the form, abundance, and distribution of water on the Moon and the lunar water cycle. Lunar Trailblazer also collects data of candidate landing sites to inform planning for future human and robotic exploration of the Moon and evaluate the potential for in situ resource utilization. Lunar Trailblazer's two science instruments, the High-resolution Volatiles and Minerals Moon Mapper (HVM3) and the Lunar Thermal Mapper (LTM) provide simultaneous high-resolution spectral imaging data to map OH/water, crustal composition, and thermophysical properties from a 100pm 30 km lunar polar orbit. The ∼210-kg flight system deploys from an ESPA Grande and utilizes a ∼1000 m/s Deltamathrm{V} hydrazine chemical propulsion system, similar to that employed by GRAIL. Trailblazing elements include the novel state-of-the-art dataset collected at substantially reduced price point, fully geographically co-registered data products delivered to the Planetary Data System, planetary mission team demographics, Caltech campus mission operations, and student staffing of select mission ops roles. Lunar Trailblazer's pioneering development is providing key lessons learned for future planetary small spacecraft.