Search Publications

Late origin of the Saturn system
DOI: 10.1016/j.icarus.2012.12.009 Bibcode: 2013Icar..223..544A

Asphaug, Erik; Reufer, Andreas

Saturn is orbited by a half dozen ice rich middle-sized moons (MSMs) of diverse geology and composition. These comprise ∼4.4% of Saturn’s satellite mass; the rest is Titan, more massive per planet than Jupiter’s satellites combined. Jupiter has no MSMs. Disk-based models to explain these differences exist, but have various challenges and assumptio…

2013 Icarus
Cassini 63
Photometric properties of the nucleus of Comet 103P/Hartley 2
DOI: 10.1016/j.icarus.2012.11.001 Bibcode: 2013Icar..222..559L

A'Hearn, Michael F.; Thomas, Peter C.; Bodewits, Dennis +8 more

We have studied the photometric properties of the nucleus of a hyperactive comet, 103P/Hartley 2, at visible wavelengths using the DIXI flyby images with both disk-integrated and disk-resolved analyses. The disk-integrated phase function of the nucleus has a linear slope of 0.046 ± 0.002 mag/deg and an absolute magnitude of 18.4 ± 0.1 at V-band. T…

2013 Icarus
eHST 63
A complete climatology of the aerosol vertical distribution on Mars from MEx/SPICAM UV solar occultations
DOI: 10.1016/j.icarus.2012.12.001 Bibcode: 2013Icar..223..892M

Montmessin, Franck; Bertaux, Jean-Loup; Maltagliati, Luca +4 more

We present the first results on solar occultations performed with the UV channel of SPICAM, on board Mars Express. From the dataset of over 900 occultations (performed between April 2004 and October 2011), about 640 atmospheric profiles of the martian atmosphere were derived. This dataset, spanning four martian years, allows characterization of th…

2013 Icarus
MEx 63
Survey of cometary CO2, CO, and particulate emissions using the Spitzer Space Telescope
DOI: 10.1016/j.icarus.2013.06.011 Bibcode: 2013Icar..226..777R

Reach, William T.; Kelley, Michael S.; Vaubaillon, Jeremie

We surveyed 23 comets using the Infrared Array Camera on the Spitzer Space Telescope in wide filters centered at 3.6 and 4.5 µm. Emission in the 3.6 µm filter arises from sunlight scattered by dust grains; the 3.6 µm images generally have a coma near the nucleus and a tail in the antisolar direction due to dust grains swept back …

2013 Icarus
ISO 62
CoRoT: Harvest of the exoplanet program
DOI: 10.1016/j.icarus.2013.03.022 Bibcode: 2013Icar..226.1625M

Guillot, Tristan; Cabrera, Juan; Deeg, Hans J. +6 more

One of the objectives of the CoRoT mission is the search for transiting extrasolar planets using high-precision photometry, and the accurate characterization of their fundamental parameters. The CoRoT satellite consecutively observes crowded stellar fields since February 2007, in high-cadence precise photometry; periodic eclipses are detected and …

2013 Icarus
CoRoT 58
Titan's atmosphere and surface liquid: New calculation using Statistical Associating Fluid Theory
DOI: 10.1016/j.icarus.2012.10.032 Bibcode: 2013Icar..222...53T

Kargel, Jeffrey S.; Tan, Sugata P.; Marion, Giles M.

The application of PC-SAFT equation of state (EOS) in analyzing the in situ measurement of atmospheric data by Huygens probe reveals new insights into Titan's atmosphere and surface liquids. The EOS offers the most reliable and accurate calculations in fluid phase equilibria at the cryogenic conditions encountered in Titan and other extra-terrestr…

2013 Icarus
Huygens 56
Sizes of main-belt asteroids by combining shape models and Keck adaptive optics observations
DOI: 10.1016/j.icarus.2013.07.023 Bibcode: 2013Icar..226.1045H

Hanuš, J.; Marchis, F.; Ďurech, J.

We select 50 main-belt asteroids with a diameter between 20 and 400 km for which we have (i) shape models derived by the lightcurve inversion method and (ii) resolved observations of good quality collected with the Keck II adaptive optics (AO) system in the near-infrared. We derive the size of these asteroids by minimizing the difference between t…

2013 Icarus
AKARI 55
NeMars: An empirical model of the martian dayside ionosphere based on Mars Express MARSIS data
DOI: 10.1016/j.icarus.2013.03.021 Bibcode: 2013Icar..225..236S

Sánchez-Cano, B.; Witasse, O.; Radicella, S. M. +2 more

Several models of the martian ionosphere have been developed in the last years. In this paper, a new empirical model for the dayside electron density of the martian ionosphere (primary and secondary layer), called NeMars, is described. The model is mainly based on MARSIS AIS data (Active Ionospheric Sounding from the Mars Advanced Radar and Ionosp…

2013 Icarus
MEx 51
Morphology of fluvial networks on Titan: Evidence for structural control
DOI: 10.1016/j.icarus.2013.06.016 Bibcode: 2013Icar..226..742B

Black, Benjamin A.; Perron, J. Taylor; Burr, Devon M. +2 more

Although Titan’s surface shows clear evidence of erosional modification, such as fluvial incision, evidence for tectonism has been less apparent. On Earth, fluvial networks with strongly preferred orientations are often associated with structural features, such as faults or joints, that influence flow or erodibility. We delineated and classified t…

2013 Icarus
Cassini 51
Mars ionosphere total electron content analysis from MARSIS subsurface data
DOI: 10.1016/j.icarus.2012.12.011 Bibcode: 2013Icar..223..423C

Amata, E.; Orosei, R.; Picardi, G. +6 more

We describe a method to estimate the total electron content (TEC) of the Mars ionosphere from the output parameters of an algorithm, called the Contrast Method (Picardi, G., Sorge, S. [2000]. Proc. SPIE. Eighth International Conference on Ground Penetrating Radar, vol. 4084, pp. 624-629; Ilyushin, Ya.A., Kunitsyn, V.E. [2004]. J. Commun. Technol. …

2013 Icarus
MEx 51