Search Publications

Composition and structure of fresh ammonia clouds on Jupiter based on quantitative analysis of Galileo/NIMS and New Horizons/LEISA spectra
DOI: 10.1016/j.icarus.2017.10.037 Bibcode: 2018Icar..307..347S

Sromovsky, L. A.; Fry, P. M.

Ammonia gas has long been assumed to be the main source of condensables for the upper cloud layer on Jupiter, but distinctive spectral features associated with ammonia have been seen only rarely. Since both ammonia and NH4SH absorb in the 3 µm region, and widespread absorption in the 3 µm region was present (Sromovsky and Fr…

2018 Icarus
eHST 13
Stepped fans and facies-equivalent phyllosilicates in Coprates Catena, Mars
DOI: 10.1016/j.icarus.2017.10.030 Bibcode: 2018Icar..307..260G

Warner, N. H.; Gupta, S.; Grindrod, P. M. +2 more

Stepped fan deposits and phyllosilicate mineralogies are relatively common features on Mars but have not previously been found in association with each other. Both of these features are widely accepted to be the result of aqueous processes, but the assumed role and nature of any water varies. In this study we have investigated two stepped fan depo…

2018 Icarus
MEx 13
Constraining the parameter space of comet simulation experiments
DOI: 10.1016/j.icarus.2018.03.025 Bibcode: 2018Icar..311..105K

Hagermann, Axel; Kaufmann, Erika

Our interpretation of the data returned by Rosetta and other cometary missions is based on the predictions of theoretical models and the results of laboratory experiments. For example, Kossacki et al. (2015) showed that 67P's surface hardness reported by Spohn et al. (2015) can be explained by sintering. The present work supports Rosetta's observa…

2018 Icarus
Rosetta 13
The upcoming mutual event season for the Patroclus-Menoetius Trojan binary
DOI: 10.1016/j.icarus.2018.01.009 Bibcode: 2018Icar..305..198G

Buie, M. W.; Grundy, W. M.; Noll, K. S. +1 more

We present new Hubble Space Telescope and ground-based Keck observations and new Keplerian orbit solutions for the mutual orbit of binary Jupiter Trojan asteroid (617) Patroclus and Menoetius, targets of NASA's Lucy mission. We predict event times for the upcoming mutual event season, which is anticipated to run from late 2017 through mid 2019.

2018 Icarus
eHST 12
Regional stratigraphy of the south polar layered deposits (Promethei Lingula, Mars): "Discontinuity-bounded" units in images and radargrams
DOI: 10.1016/j.icarus.2017.08.030 Bibcode: 2018Icar..308...76G

Thomas, Nicolas; Forget, François; Rossi, Angelo Pio +5 more

The Mars South Polar Layered Deposits (SPLD) are the result of depositional and erosional events, which are marked by different stratigraphic sequences and erosional surfaces. To unambiguously define the stratigraphic units at regional scale, we mapped the SPLD on the basis of observed discontinuities (i.e., unconformities, correlative discontinui…

2018 Icarus
MEx 12
Compressive strength and elastic modulus at Agilkia on comet 67P/Churyumov-Gerasimenko derived from the SESAME/CASSE touchdown signals
DOI: 10.1016/j.icarus.2017.09.038 Bibcode: 2018Icar..303..251M

Flandes, Alberto; Krüger, Harald; Arnold, Walter +8 more

We report an analysis of the Comet Acoustic Surface Sounding Experiment (CASSE) acceleration signals at Philae's first touchdown site Agilkia on comet 67P/Churyumov-Gerasimenko. The signals yield the forces in the contact zone foot-sole and comet surface, and from these forces a compression strength of approximately 10 kPa can be derived. The sole…

2018 Icarus
Rosetta 12
Large catchment area recharges Titan's Ontario Lacus
DOI: 10.1016/j.icarus.2017.08.009 Bibcode: 2018Icar..299..331D

Barnes, Jason W.; Kirk, Randolph L.; Dhingra, Rajani D. +1 more

We seek to address the question of what processes are at work to fill Ontario Lacus while other, deeper south polar basins remain empty. Our hydrological analysis indicates that Ontario Lacus has a catchment area spanning 5.5% of Titan's surface and a large catchment area to lake surface area ratio. This large catchment area translates into large …

2018 Icarus
Cassini 11
Aerosol properties in the upper clouds of Venus from glory observations by the Venus Monitoring Camera (Venus Express mission)
DOI: 10.1016/j.icarus.2017.08.011 Bibcode: 2018Icar..299..272M

Markiewicz, Wojciech J.; Petrova, Elena V.; Shalygina, Oksana S.

From the angular positions of the glory features observed on the upper cloud deck of Venus in three VMC channels (at 0.365, 0.513, and 0.965 µm), the dominating sizes of cloud particles and their refractive indices have been retrieved, and their spatial and temporal variations have been analyzed. For this, the phase profiles of brightness we…

2018 Icarus
VenusExpress 11
Glory on Venus and selection among the unknown UV absorbers
DOI: 10.1016/j.icarus.2018.02.016 Bibcode: 2018Icar..306..163P

Petrova, Elena V.

The comparison of the phase profiles of glories observed on the cloud top of Venus by the Venus Monitoring Camera (Venus Express) and the light-scattering characteristics of sulfuric acid droplets, containing admixtures with a high refractive index, makes it easier to choose between some candidates for the so-called unknown UV absorber in the Venu…

2018 Icarus
VenusExpress 11
Mars radar clutter and surface roughness characteristics from MARSIS data
DOI: 10.1016/j.icarus.2017.07.011 Bibcode: 2018Icar..299...22C

Schroeder, Dustin M.; Whitten, Jennifer L.; Campbell, Bruce A.

Radar sounder studies of icy, sedimentary, and volcanic settings can be affected by reflections from surface topography surrounding the sensor nadir location. These off-nadir ;clutter; returns appear at similar time delays to subsurface echoes and complicate geologic interpretation. Additionally, broadening of the radar echo in delay by surface re…

2018 Icarus
MEx 10