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Variations in the Ionospheric Peak Altitude at Mars in Response to Dust Storms: 13 Years of Observations From the Mars Express Radar Sounder
DOI: 10.1029/2019JE006092 Bibcode: 2020JGRE..12506092G

Gurnett, D. A.; Němec, F.; Morgan, D. D. +7 more

Previous observations have shown that, during Martian dust storms, the peak of the ionosphere rises in altitude. Observational studies of this type, however, have been extremely limited. Using 13 years of ionospheric peak altitude data from the Mars Advanced Radar for Subsurface and Ionosphere Sounding instrument on Mars Express, we study how the …

2020 Journal of Geophysical Research (Planets)
MEx 25
Aram Dorsum: An Extensive Mid-Noachian Age Fluvial Depositional System in Arabia Terra, Mars
DOI: 10.1029/2019JE006244 Bibcode: 2020JGRE..12506244B

Sefton-Nash, Elliot; Williams, Rebecca M. E.; Fawdon, Peter +5 more

A major debate in Mars science is the nature of the early Mars climate, and the availability of precipitation and runoff. Observations of relict erosional valley networks have been proposed as evidence for extensive surface runoff around the Noachian-Hesperian boundary. However, these valley networks only provide a time-integrated record of landsc…

2020 Journal of Geophysical Research (Planets)
MEx 20
Magnetic Properties of Asteroid (162173) Ryugu
DOI: 10.1029/2019JE006035 Bibcode: 2020JGRE..12506035H

Motschmann, Uwe; Fujimoto, Masaki; Richter, Ingo +22 more

Observations of the magnetization state of asteroids indicate diverse properties. Values between 1.9 × 10-6 Am2/kg (Eros) and 10-2 Am2/kg (Braille) have been reported. A more detailed understanding of asteroidal magnetic properties allows far-reaching conclusions of the magnetization mechanism as well as…

2020 Journal of Geophysical Research (Planets)
Rosetta 17
The Bathymetry of Moray Sinus at Titan's Kraken Mare
DOI: 10.1029/2020JE006558 Bibcode: 2020JGRE..12506558P

Lunine, J. I.; Hayes, A. G.; Le Gall, A. +4 more

Moray Sinus is an estuary located at the northern end of Titan's Kraken Mare. The Cassini RADAR altimeter acquired three segments over this mare during the T104 flyby of Titan, on August 21, 2014. Herein, we present a detailed analysis of the received echoes. Some of these waveforms exhibit a reflection from the seafloor, from up to 85-18+28 m of …

2020 Journal of Geophysical Research (Planets)
Cassini 16
Polyphase Mid-Latitude Glaciation on Mars: Chronology of the Formation of Superposed Glacier-Like Forms from Crater-Count Dating
DOI: 10.1029/2019JE006102 Bibcode: 2020JGRE..12506102H

Hepburn, A. J.; Hubbard, B.; Ng, F. S. L. +2 more

Reconstructing Mars's glacial history informs understanding of its physical environment and past climate. The known distribution of viscous flow features (VFFs) containing water ice suggests that its mid-latitudes were glaciated during the Late Amazonian period (the last several hundred million years). The identification of a subgroup of VFFs—call…

2020 Journal of Geophysical Research (Planets)
MEx 16
Ganymede's Far-Ultraviolet Reflectance: Constraining Impurities in the Surface Ice
DOI: 10.1029/2020JE006476 Bibcode: 2020JGRE..12506476M

Nichols, J. D.; Raut, U.; Retherford, K. D. +2 more

We present reflectance spectra of Ganymede's leading and trailing hemispheres in the wavelength range 138-215 nm, obtained by the Hubble Space Telescope Cosmic Origins Spectrograph (HST/COS) in 2014. The most notable feature of both spectra is the absence of a sharp water absorption edge at ~165 nm, seen in laboratory measurements of ice reflectiv…

2020 Journal of Geophysical Research (Planets)
eHST 15
Paleolakes in the Northwest Hellas Region, Mars: Implications for the Regional Geologic History and Paleoclimate
DOI: 10.1029/2019JE006196 Bibcode: 2020JGRE..12506196Z

Xiao, Long; Glotch, Timothy D.; Zhao, Jiannan

Hellas basin is one of the largest and oldest impact basins on the Martian surface. Its surrounding highland regions have undergone complicated geologic processes after the formation of Hellas basin. However, the geologic and climatic histories of the highlands surrounding Hellas are still unclear. Paleolakes provide us clues to answer these quest…

2020 Journal of Geophysical Research (Planets)
MEx 15
Small Impact Crater Populations on Saturn's Moon Tethys and Implications for Source Impactors in the System
DOI: 10.1029/2020JE006400 Bibcode: 2020JGRE..12506400F

Ferguson, S. N.; Rhoden, A. R.; Kirchoff, M. R.

Current estimates place the ages of the inner Saturnian satellites (Mimas, Enceladus, Tethys, Dione, and Rhea) between 4.5 Gyr and 100 Myr. These estimates are based on impact crater measurements and dynamical simulations, both of which have uncertainties. Models of satellite evolution are inherently simplified and rely on uncertain or unknown par…

2020 Journal of Geophysical Research (Planets)
Cassini 15
A Survey of Small-Scale Waves and Wave-Like Phenomena in Jupiter's Atmosphere Detected by JunoCam
DOI: 10.1029/2019JE006369 Bibcode: 2020JGRE..12506369O

Wong, Michael H.; Fletcher, Leigh N.; Ingersoll, Andrew P. +17 more

In the first 20 orbits of the Juno spacecraft around Jupiter, we have identified a variety of wave-like features in images made by its public-outreach camera, JunoCam. Because of Juno's unprecedented and repeated proximity to Jupiter's cloud tops during its close approaches, JunoCam has detected more wave structures than any previous surveys. Most…

2020 Journal of Geophysical Research (Planets)
eHST 14
Studies of the 2018/Mars Year 34 Planet-Encircling Dust Storm
DOI: 10.1029/2020JE006700 Bibcode: 2020JGRE..12506700G

Guzewich, S. D.; Fedorova, A. A.; Kahre, M. A. +1 more

Mars' planet-encircling or global dust storms (GDSs) are an iconic and enigmatic feature of the Red Planet. Occurring every few Mars Years (MYs), on average, they are a stochastic process in the otherwise largely repeatable annual cycle of martian weather. In 2018 (MY 34 in the calendar of Clancy et al. [2000],

ExoMars-16 12