Search Publications

Low velocity collisions of porous planetesimals in the early solar system
DOI: 10.1016/j.icarus.2017.09.024 Bibcode: 2018Icar..301..196D

Kührt, E.; Davidsson, B.; Hviid, S. +1 more

The ESA Rosetta mission has shown that Comet 67P/Churuymov-Gerasimenko is bi-lobed, has a high average porosity of around 70%, does not have internal cavities on size scales larger than 10 m, the lobes could have individual sets of onion shell-like layering, and the nucleus surface contains 100 m-scale cylindrical pits. It is currently debated whe…

2018 Icarus
Rosetta 6
Ejecta deposits of Bakhuysen Crater, Mars
DOI: 10.1016/j.icarus.2018.06.001 Bibcode: 2018Icar..314..175C

Tornabene, L. L.; Osinski, G. R.; Caudill, C. M.

Bakhuysen Crater is a Late Noachian to Early Hesperian age ∼150 km-diameter impact structure located in the heavily cratered southern highlands of Mars. It is one of the largest craters on Mars with well-preserved ejecta deposits. Impact ejecta deposits allow an understanding of crustal composition, volatile content, and evolution of terrestrial p…

2018 Icarus
MEx 6
Retrieval of H2O abundance in Titan's stratosphere: A (re)analysis of CIRS/Cassini and PACS/Herschel observations
DOI: 10.1016/j.icarus.2018.04.003 Bibcode: 2018Icar..311..288B

Lellouch, E.; Irwin, P. G. J.; Teanby, N. A. +6 more

Since its first measurement 20 years ago by the Infrared Space Observatory (ISO), the water (H2O) mole fraction in Titan's stratosphere remains uncertain due to large differences between the determinations from available measurements. More particularly, the recent measurements made from the Herschel observatory (PACS and HIFI) estimated…

2018 Icarus
Cassini Herschel 6
Internal gravity, self-energy, and disruption of comets and asteroids
DOI: 10.1016/j.icarus.2017.09.030 Bibcode: 2018Icar..303..234D

Korycansky, D. G.; Dobrovolskis, Anthony R.

The internal gravity and self-gravitational energy of a comet, asteroid, or small moon have applications to their geophysics, including their formation, evolution, cratering, and disruption, the stresses and strains inside such objects, sample return, eventual asteroid mining, and planetary defense strategies for potentially hazardous objects. Thi…

2018 Icarus
Rosetta 6
The strength of ice-saturated extraterrestrial rock analogs
DOI: 10.1016/j.icarus.2018.06.016 Bibcode: 2018Icar..315...61A

Seager, Sara; Atkinson, Jared; Durham, William B.

In situ resource utilization (ISRU) activities have been identified by the National Research Council as one of the most important scientific endeavors of the coming decade. The failure of the MUPUS-PEN experiment on Rosetta's Philae lander to penetrate the surface of comet 67P demands knowledge of the mechanical properties of extraterrestrial mate…

2018 Icarus
Rosetta 6
Formation and degradation of chaotic terrain in the Galaxias regions of Mars: implications for near-surface storage of ice
DOI: 10.1016/j.icarus.2018.03.002 Bibcode: 2018Icar..309...69G

Conway, Susan J.; Gallagher, Colman; Balme, Matt +1 more

Galaxias Chaos is a region of low plateaus separated by narrow fractures - a chaotic terrain. Galaxias Mensae and Galaxias Colles are characterised by mesa and knobby terrains of individual landforms, or small assemblages, separated by plains. Galaxias Chaos has been attributed to ground disturbance due to sublimation in shallow subsurface ice-ric…

2018 Icarus
MEx 6
Enceladus' near-surface CO2 gas pockets and surface frost deposits
DOI: 10.1016/j.icarus.2017.10.025 Bibcode: 2018Icar..302...18M

McCord, Thomas B.; Radebaugh, Jani; Combe, Jean-Philippe +4 more

Solid CO2 surface deposits were reported in Enceladus' South Polar Region by Brown et al. (2006). They noted that such volatile deposits are temporary and posited ongoing replenishment. We present a model for this replenishment by expanding on the Matson et al. (2012) model of subsurface heat and chemical transport in Enceladus. Our mod…

2018 Icarus
Cassini 5
Energetic electron measurements near Enceladus by Cassini during 2005-2015
DOI: 10.1016/j.icarus.2017.10.022 Bibcode: 2018Icar..306..256K

Krupp, N.; Roussos, E.; Khurana, K. K. +9 more

Enceladus is the main source of neutral and charged particles in the Saturnian magnetosphere. The particles originate at more than 100 active geysers forming a plume above the south pole of the moon and are continuously released into Saturn's magnetosphere. Therefore the understanding of the interaction of those particles and the local magnetosphe…

2018 Icarus
Cassini 5
Collapse-driven formation of depressions on comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.icarus.2017.11.019 Bibcode: 2018Icar..302..266L

Leliwa-Kopystynski, J.

The extremely diverse surface of comet 67P/Churyumov-Gerasimenko contains a large number of depressions or craters of very different scales. Among the most prominent are two large roughly circular depressions, each with radii of several hundred meters. In this work a model for the formation of the depressions is proposed. It is based on the theory…

2018 Icarus
Rosetta 5
Energy deposition and ion production from thermal oxygen ion precipitation during Cassini's T57 flyby
DOI: 10.1016/j.icarus.2018.01.014 Bibcode: 2018Icar..305..186S

Smith, Michael; Snowden, Darci; Jimson, Theodore +1 more

Cassini's Radio Science Investigation (RSS) and Langmuir Probe observed abnormally high electron densities in Titan's ionosphere during Cassini's T57 flyby. We have developed a three-dimensional model to investigate how the precipitation of thermal magnetospheric O+ may have contributed to enhanced ion production in Titan's ionosphere. …

2018 Icarus
Cassini 5