Search Publications

Photochemistry of water in the martian thermosphere and its effect on hydrogen escape
DOI: 10.1016/j.icarus.2018.10.033 Bibcode: 2019Icar..321...62K

Krasnopolsky, Vladimir A.

Recent SPICAM IR solar occultations reveal significant abundances of water vapor up to ≈80 km near Mars perihelion. These abundances are stimulated by dust that heats the atmosphere and precludes condensation of water. This phenomenon correlates with detections of high escape of hydrogen near perihelion using the H Lyman-alpha in the SPICAM UV and…

2019 Icarus
MEx eHST 35
Latitudinal variation in the abundance of methane (CH4) above the clouds in Neptune's atmosphere from VLT/MUSE Narrow Field Mode Observations
DOI: 10.1016/j.icarus.2019.05.011 Bibcode: 2019Icar..331...69I

Bacon, Roland; Fletcher, Leigh N.; Irwin, Patrick G. J. +5 more

Observations of Neptune, made in 2018 using the new Narrow Field Adaptive Optics mode of the Multi Unit Spectroscopic Explorer (MUSE) instrument at the Very Large Telescope (VLT) from 0.48 to 0.93 µm, are analysed here to determine the latitudinal and vertical distribution of cloud opacity and methane abundance in Neptune's observable tropos…

2019 Icarus
eHST 33
The mutual orbit, mass, and density of transneptunian binary Gǃkúnǁ'hòmdímà (229762 2007 UK126)
DOI: 10.1016/j.icarus.2018.12.037 Bibcode: 2019Icar..334...30G

Buie, M. W.; Ragozzine, D.; Roe, H. G. +3 more

We present high spatial resolution images of the binary transneptunian object Gǃkúnǁ'hòmdímà (229762 2007 UK126) obtained with the Hubble Space Telescope and with the Keck observatory on Mauna Kea to determine the orbit of Gǃò'é ǃhúGǃò'é ǃhú, the much smaller and redder satellite. Gǃò'é ǃhú orbits in a prograde sense, on a circular or n…

2019 Icarus
eHST 30
Observational evidence for a dry dust-wind origin of Mars seasonal dark flows
DOI: 10.1016/j.icarus.2019.02.024 Bibcode: 2019Icar..325..115V

Vincendon, Mathieu; Carter, John; Stcherbinine, Aurélien +1 more

Seasonal flows on warm slopes, or recurring slope lineae ("RSL"), have been presented as strong evidence for currently flowing water on Mars. This assumption was supported by a correlation between activity and warm temperatures, and by the spectral identification of hydrated salts. Here we first demonstrate that salts spectral identification is no…

2019 Icarus
MEx 30
Analysis of Neptune's 2017 bright equatorial storm
DOI: 10.1016/j.icarus.2018.11.018 Bibcode: 2019Icar..321..324M

de Pater, Imke; Wong, Michael H.; Magnier, Eugene A. +22 more

We report the discovery of a large ( ∼ 8500 km diameter) infrared-bright storm at Neptune's equator in June 2017. We tracked the storm over a period of 7 months with high-cadence infrared snapshot imaging, carried out on 14 nights at the 10 m Keck II telescope and 17 nights at the Shane 120 inch reflector at Lick Observatory. The cloud feature was…

2019 Icarus
eHST 29
Hypotheses for the origin of the Hypanis fan-shaped deposit at the edge of the Chryse escarpment, Mars: Is it a delta?
DOI: 10.1016/j.icarus.2018.05.021 Bibcode: 2019Icar..319..885A

Sefton-Nash, Elliot; Bell, James F., III; Adler, Jacob B. +4 more

We investigated the origin of the fan-shaped deposit at the end of Hypanis Valles that has previously been proposed as an ExoMars, Mars 2020, and human mission candidate landing site, and found evidence that the landform is an ancient delta. Previous work suggests that the deposit originated from a time of fluvial activity both distinct from and p…

2019 Icarus
MEx 28
Observations of the chemical and thermal response of 'ring rain' on Saturn's ionosphere
DOI: 10.1016/j.icarus.2018.10.027 Bibcode: 2019Icar..322..251O

Baines, Kevin H.; O'Donoghue, James; Moore, Luke +4 more

In this study we performed a new analysis of ground-based observations that were taken on 17 April 2011 using the 10-metre Keck telescope on Mauna Kea, Hawaii. Emissions from H3+, a major ion in Saturn's ionosphere, were previously analyzed from these observations, indicating that peaks in emission at specific latitudes were …

2019 Icarus
Cassini 28
Kronoseismology III: Waves in Saturn's inner C ring
DOI: 10.1016/j.icarus.2018.10.013 Bibcode: 2019Icar..319..599F

Nicholson, Philip D.; French, Richard G.; McGhee-French, Colleen A. +1 more

We investigate waves driven in Saturn's rings by planetary normal modes, concentrating on the previously unexplored inner C ring. In this region, the known waves all have exceptionally short wavelengths, which has proven problematic for previous studies that depended on the accurate estimate of wave phases for wave identification. However, detaile…

2019 Icarus
Cassini 26
Cassini-VIMS observations of Saturn's main rings: II. A spectrophotometric study by means of Monte Carlo ray-tracing and Hapke's theory
DOI: 10.1016/j.icarus.2018.07.010 Bibcode: 2019Icar..317..242C

Clark, R. N.; Nicholson, P. D.; D'Aversa, E. +9 more

This work is the second in a series of manuscripts devoted to the investigation of the spectrophotometric properties of Saturn's rings from Cassini-VIMS (Visible and Infrared Mapping Spectrometer) observations. The dataset used for this analysis is represented by ten radial spectrograms of the rings which have been derived in Filacchione et al. (2…

2019 Icarus
Cassini 25
Effects of the solar wind and the solar EUV flux on O+ escape rates from Venus
DOI: 10.1016/j.icarus.2018.11.017 Bibcode: 2019Icar..321..379M

Fedorov, A.; Barabash, S.; Futaana, Y. +4 more

We investigate dependences of O+ escape rates from Venus both on the solar wind and the solar extreme ultraviolet (EUV) flux by using the 8.5-year dataset (May 2006 to December 2014) of the Ion Mass Analyzer and the magnetometer aboard Venus Express. We examine the O+ escape rates for 8 different conditions depending on the s…

2019 Icarus
VenusExpress 25