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Enceladus's measured physical libration requires a global subsurface ocean
DOI: 10.1016/j.icarus.2015.08.037 Bibcode: 2016Icar..264...37T

Burns, J. A.; Porco, C.; Tajeddine, R. +5 more

Several planetary satellites apparently have subsurface seas that are of great interest for, among other reasons, their possible habitability. The geologically diverse saturnian satellite Enceladus vigorously vents liquid water and vapor from fractures within a south polar depression and thus must have a liquid reservoir or active melting. However…

2016 Icarus
Cassini 297
The global shape, density and rotation of Comet 67P/Churyumov-Gerasimenko from preperihelion Rosetta/OSIRIS observations
DOI: 10.1016/j.icarus.2016.05.002 Bibcode: 2016Icar..277..257J

Jorda, L.; Lara, L. M.; Lamy, P. +45 more

The Rosetta spacecraft reached Comet 67P/Churyumov-Gerasimenko (hereafter 67P/C-G) in August 2014 at an heliocentric distance of 3.6 a.u. and was then put in orbit around its nucleus to perform detailed observations. Among the collected data are the images acquired by the OSIRIS instrument up to the perihelion passage of the comet in August 2015, …

2016 Icarus
Rosetta 269
Refractory and semi-volatile organics at the surface of comet 67P/Churyumov-Gerasimenko: Insights from the VIRTIS/Rosetta imaging spectrometer
DOI: 10.1016/j.icarus.2016.02.028 Bibcode: 2016Icar..272...32Q

Fornasier, S.; Erard, S.; Drossart, P. +34 more

The VIRTIS (Visible, Infrared and Thermal Imaging Spectrometer) instrument aboard the Rosetta spacecraft has performed extensive spectral mapping of the surface of comet 67P/Churyumov-Gerasimenko in the range 0.3-5 µm. The reflectance spectra collected across the surface display a low reflectance factor over the whole spectral range, two spe…

2016 Icarus
Rosetta 157
Planetary surface dating from crater size-frequency distribution measurements: Poisson timing analysis
DOI: 10.1016/j.icarus.2016.05.019 Bibcode: 2016Icar..277..279M

Michael, G. G.; Kneissl, T.; Neesemann, A.

The predictions of crater chronology models have customarily been evaluated by dividing a crater population into discrete diameter intervals, plotting the crater density for each, and finding a best-fit model isochron, with the uncertainty in the procedure being assessed using 1/√n estimates, where n is the number of craters in an interval. This a…

2016 Icarus
MEx 131
Emerging trends and a comet taxonomy based on the volatile chemistry measured in thirty comets with high-resolution infrared spectroscopy between 1997 and 2013
DOI: 10.1016/j.icarus.2016.05.039 Bibcode: 2016Icar..278..301D

Weaver, Harold A.; Vervack, Ronald J.; Kawakita, Hideyo +1 more

A systematic analysis of the mixing ratios with respect to H2O for eight species (CH3OH, HCN, NH3, H2CO, C2H2, C2H6, CH4, and CO) measured with high-resolution infrared spectroscopy in thirty comets between 1997 and 2013 is presented. Some trends are…

2016 Icarus
eHST 129
Typology of dust particles collected by the COSIMA mass spectrometer in the inner coma of 67P/Churyumov Gerasimenko
DOI: 10.1016/j.icarus.2016.01.027 Bibcode: 2016Icar..271...76L

Langevin, Y.; Schulz, R.; Hilchenbach, M. +7 more

The COSIMA mass spectrometer on board the ROSETTA orbiter has collected dust in the near coma of comet 67P/Churyumov-Gerasimenko since August 11, 2014. The collected dust particles are identified by taking images with a microscope (COSISCOPE) under grazing incidence illumination before and after exposure of the target to cometary dust. More than 1…

2016 Icarus
Rosetta 123
Wave analysis in the atmosphere of Venus below 100-km altitude, simulated by the LMD Venus GCM
DOI: 10.1016/j.icarus.2016.06.004 Bibcode: 2016Icar..278...38L

Lebonnois, Sébastien; Sugimoto, Norihiko; Gilli, Gabriella

A new simulation of Venus atmospheric circulation obtained with the LMD Venus GCM is described and the simulated wave activity is analyzed. Agreement with observed features of the temperature structure, static stability and zonal wind field is good, such as the presence of a cold polar collar, diurnal and semi-diurnal tides. At the resolution used…

2016 Icarus
VenusExpress 86
The global surface composition of 67P/CG nucleus by Rosetta/VIRTIS. (I) Prelanding mission phase
DOI: 10.1016/j.icarus.2016.02.055 Bibcode: 2016Icar..274..334F

Longobardo, Andrea; Palomba, Ernesto; Piccioni, Giuseppe +27 more

From August to November 2014 the Rosetta orbiter has performed an extensive observation campaign aimed at the characterization of 67P/CG nucleus properties and to the selection of the Philae landing site. The campaign led to the production of a global map of the illuminated portion of 67P/CG nucleus. During this prelanding phase the comet's helioc…

2016 Icarus
Rosetta 79
Observations of an aeolian landscape: From surface to orbit in Gale Crater
DOI: 10.1016/j.icarus.2015.09.042 Bibcode: 2016Icar..280...37D

Day, Mackenzie; Kocurek, Gary

Landscapes derived solely from aeolian processes are rare on Earth because of the dominance of subaqueous processes. In contrast, aeolian-derived landscapes should typify Mars because of the absence of liquid water, the long exposure times of surfaces, and the presence of wind as the default geomorphic agent. Using the full range of available orbi…

2016 Icarus
MEx 79
Titan's surface at 2.18-cm wavelength imaged by the Cassini RADAR radiometer: Results and interpretations through the first ten years of observation
DOI: 10.1016/j.icarus.2015.09.027 Bibcode: 2016Icar..270..443J

Lorenz, R. D.; Janssen, M. A.; Hayes, A. G. +12 more

A comprehensive calibration and mapping of the thermal microwave emission from Titan's surface is reported based on radiometric data obtained at 2.18-cm wavelength by the passive radiometer included in the Cassini RADAR instrument. Compared to previous work, the present results incorporate the much larger data set obtained in the approximately ten…

2016 Icarus
Cassini 77