Results 21 to 30 of about 2,550 (207)
It is widely accepted that Titan and the mid-sized regular satellites around Saturn were formed in the circum-Saturn disk. Thus, if these mid-sized satellites were simply accreted by collisions of similar ice-rock satellitesimals in the disk, the ...
Agnor +56 more
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NEOWISE: Observations of the Irregular Satellites of Jupiter and Saturn [PDF]
We present thermal model fits for 11 Jovian and 3 Saturnian irregular satellites based on measurements from the WISE/NEOWISE dataset. Our fits confirm spacecraft-measured diameters for the objects with in situ observations (Himalia and Phoebe) and ...
Bauer, James M. +7 more
core +2 more sources
Spitzer IRS Observations of Titan as a Precursor to JWST MIRI Observations
In this work, we present for the first time infrared spectra of Titan from the Spitzer Space Telescope (2004–2009). The data are from both the short wavelength–low resolution (SL; 5.13–14.29 μ m, R ∼ 60–127) and short wavelength–high resolution (SH; 9.89–
Brandon Park Coy +6 more
doaj +1 more source
Shallow normal fault slopes on Saturnian icy satellites [PDF]
AbstractFault dips are a function of the coefficient of internal friction, μi, of the lithospheric material. Laboratory deformation experiments of H2O ice at conditions applicable to icy bodies yield 0 ≤ μi ≤ 0.55 such that normal faults dip between 45° and 59°.
Chloe B. Beddingfield +2 more
openaire +1 more source
IR SPECTRAL MAPPING OF THE MARTIAN SOUTH POLAR RESIDUAL CAP USING CRISM [PDF]
Polycyclic aromatic hydrocarbons (PAHs) are considered to be important in theories of abiogenesis (Allamandola, 2011) . There is evidence that PAHs have been detected on two icy Saturnian satellites using the Visual and Infrared Mapping Spectrometer ...
J. Campbell +3 more
doaj +1 more source
Last giant impact on the Neptunian system. Constraints on oligarchic masses in the trans-Saturnian region [PDF]
Stochastic impacts by large bodies are, at present, the usually accepted mechanisms able to account for the obliquity of the ice giants. We attempt to set constraints on giant impacts as the cause of Neptune's current obliquity in the framework of modern
Agnor +52 more
core +3 more sources
In the last few years Cassini-VIMS, the Visible and Infared Mapping Spectrometer, returned to us a comprehensive view of the Saturn's icy satellites and rings. After having analyzed the satellites' spectral properties (Filacchione et al.
B.J. Buratti +89 more
core +1 more source
Cassini ISS mutual event astrometry of the mid-sized Saturnian satellites 2005-2012 [PDF]
Reproduced with permission from Astronomy & Astrophysics ...
Acton +19 more
core +4 more sources
A Search for Water Masers in the Saturnian System
We searched for H2O 6(1,6)-5(2,3) maser emission at 22.235 GHz from several Saturnian satellites with the Nobeyama 45m radio telescope in May 2009. Observations were made for Titan, Hyperion, Enceladus and Atlas, for which Pogrebenko et al.
Deguchi, Shuji +4 more
core +1 more source
Four, and possibly as many as six, new satellites of Saturn have been found as a result of data from the Voyager 2 encounter with the planet in August 1981. The discoveries bring the number of Saturnian satellites to between 21 and 23. The two ‘possible’ satellites were seen in only one observation each, so their orbits are not yet confirmed.The ...
openaire +1 more source

