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Searching for evidence of hydrothermal activity at Apollinaris Mons, Mars
DOI: 10.1016/j.icarus.2011.10.022 Bibcode: 2012Icar..217..297E

Markiewicz, Wojciech J.; Heggy, Essam; Marzo, Giuseppe A. +5 more

A multidisciplinary approach involving various remote sensing instruments is used to investigate Apollinaris Mons, a prominent volcano on Mars, as well as the surrounding plains for signs of prolonged hydrologic and volcanic, and possibly hydrothermal activity. The main findings include (1) evidence from laser altimetry indicating the large thickn…

2012 Icarus
MEx 17
Direct wind measurements from November 2007 in Venus' upper atmosphere using ground-based heterodyne spectroscopy of CO 2 at 10 µm wavelength
DOI: 10.1016/j.icarus.2011.03.019 Bibcode: 2012Icar..217..863S

Sornig, M.; Sonnabend, G.; Kroetz, P. +2 more

Between November 23 and 28, 2007, the Cologne Tuneable Heterodyne Infrared Spectrometer THIS was installed at the McMath-Pierce Solar Telescope (Kitt Peak, Arizona, USA) to determine zonal wind velocities and to estimate the subsolar-to-antisolar flow. We investigate dynamics in the upper atmosphere of Venus by measuring the Doppler shift of fully…

2012 Icarus
VenusExpress 17
Mimas' far-UV albedo: Spatial variations
DOI: 10.1016/j.icarus.2012.06.012 Bibcode: 2012Icar..220..922H

Johnson, Robert E.; Buratti, Bonnie J.; Hendrix, Amanda R. +7 more

We present Cassini Ultraviolet Imaging Spectrograph (UVIS) observations of Mimas at far-ultraviolet wavelengths (170-190 nm) which show an interesting albedo gradient across the anti-saturnian hemisphere. We discuss the photometric behavior of Mimas in the far-UV and review the important exogenic processes and their expected effects, relevant over…

2012 Icarus
Cassini 16
Venusian middle-atmospheric dynamics in the presence of a strong planetary-scale 5.5-day wave
DOI: 10.1016/j.icarus.2011.06.017 Bibcode: 2012Icar..217..702Y

Yamamoto, Masaru; Takahashi, Masaaki

The middle atmospheric dynamics on Venus are investigated using a middle atmosphere general circulation model. The magnitude of the superrotation is sensitive to the amplitude of the planetary-scale waves. In particular, the critical level absorptions of the forced planetary-scale waves might contribute to the maintenance of the superrotation near…

2012 Icarus
VenusExpress 16
The brightening of Saturn's F ring
DOI: 10.1016/j.icarus.2012.02.020 Bibcode: 2012Icar..219..181F

Nicholson, Philip D.; Hedman, Matthew M.; Showalter, Mark R. +5 more

Image photometry reveals that the F ring is approximately twice as bright during the Cassini tour as it was during the Voyager flybys of 1980 and 1981. It is also three times as wide and has a higher integrated optical depth. We have performed photometric measurements of more than 4800 images of Saturn's F ring taken over a 5-year period with Cass…

2012 Icarus
Cassini 16
Habitable periglacial landscapes in martian mid-latitudes
DOI: 10.1016/j.icarus.2012.03.019 Bibcode: 2012Icar..219..345U

Hauber, E.; Ulrich, M.; Schirrmeister, L. +2 more

Subsurface permafrost environments on Mars are considered to be zones where extant life could have survived. For the identification of possible habitats it is important to understand periglacial landscape evolution and related subsurface and environmental conditions. Many landforms that are interpreted to be related to ground ice are located in th…

2012 Icarus
MEx 15
Quantification of middle and lower cloud variability and mesoscale dynamics from Venus Express/VIRTIS observations at 1.74 µm
DOI: 10.1016/j.icarus.2011.07.009 Bibcode: 2012Icar..217..615M

Baines, Kevin H.; Grinspoon, David H.; Momary, Thomas W. +1 more

We present an analysis of VIRTIS-M-IR observations of 1.74 µm emission from the nightside of Venus. The 1.74 µm window in the near infrared spectrum of Venus is an ideal proxy for investigating the evolution of middle and lower cloud deck opacity of Venus because it exhibits good signal to noise due to its brightness, good contrast bet…

2012 Icarus
VenusExpress 15
Cloud structure of Saturn's 2010 storm from ground-based visual imaging
DOI: 10.1016/j.icarus.2012.02.023 Bibcode: 2012Icar..219..142S

Sánchez-Lavega, A.; Pérez-Hoyos, S.; Colas, F. +5 more

We present a study of the vertical cloud structure for the initial stage of the Great White Spot (GWS), a giant storm that developed in Saturn in December 2010, using ground-based visual images. We focus in the characterization of the undisturbed atmosphere preceding the storm and the disturbed region in the wake of the GWS. The observations were …

2012 Icarus
Cassini 15
Structural asymmetry in martian impact craters as an indicator for an impact trajectory
DOI: 10.1016/j.icarus.2012.04.025 Bibcode: 2012Icar..220..194W

Kenkmann, T.; Wulf, G.; Poelchau, M. H.

Impact crater formation is a highly dynamic and complex geological phenomenon. Methods of structural geology are capable of giving insights into deformation processes that occur during cratering. While most deformation observed in craters exhibits a generally radial symmetry, recent discoveries of non-radial structural elements in the central upli…

2012 Icarus
MEx 14
Late-stage impacts and the orbital and thermal evolution of Tethys
DOI: 10.1016/j.icarus.2011.12.013 Bibcode: 2012Icar..218..348Z

Zhang, Ke; Nimmo, Francis

An inferred ancient episode of heating and deformation on Tethys has been attributed to its passage through a 3:2 resonance with Dione (Chen, E.M.A., Nimmo, F. [2008]. Geophys. Res. Lett. 35, 19203). The satellites encounter, and are trapped into, the e-Dione resonance before reaching the e-Tethys resonance, limiting the degree to which Tethys is …

2012 Icarus
Cassini 14