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  • 1
    Publication Date: 1990-10-12
    Description: Europa and Ganymede may have undergone an episode of chaotic motion before the establishment of the current Laplace resonance involving the three inner Galilean satellites. During this episode, the orbital eccentricities of both satellites may have increased dramatically. As a result, the mechanical stresses due to tidal deformation of the satellites' icy lithospheres may have been large enough to result in extensive fracturing, and tidal heating may have melted water ice in the mantles of both satellites, triggering the geological activity that has modified their surfaces since the heavy cratering period. The tidal effects on Ganymede during this episode provide an explanation of the dichotomy between it and Callisto, which have similar bulk properties but very different geological histories.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Tittemore, W C -- New York, N.Y. -- Science. 1990 Oct 12;250(4978):263-7.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/17797308" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 1984-09-01
    Print ISSN: 0004-6256
    Electronic ISSN: 1538-3881
    Topics: Physics
    Published by Institute of Physics
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  • 3
    Publication Date: 2019-06-28
    Description: The results of a program to monitor the brightness of Io in the near infrared are reported. While Io's 2.2 micron flux can be explained very well by conventional albedo analysis, at 3.8 and 4.8 microns Io has large intrinsic variations presumably associated with volcanism. At the latter two wavelengths, Io appears brighter and more active on its trailing hemisphere. These wavelengths also have possibly significant terms at the Jupiter corotational periods of 13 and 6.5 hr. These are particularly significant for observations of the trailing hemisphere and have a marked peak when Io is in the active sector. The data also show that the variability occurs in outbursts. Eight of these were observed and four were studied, deriving color temperatures near 700 K which decayed to about 300 K after several hours. It is argued that the apparent peak and the significance of the corotational terms may be fortuitous.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Icarus (ISSN 0019-1035); 54; April 19
    Format: text
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  • 4
    Publication Date: 2019-06-28
    Description: L' (3.8 microns) and M (4.9 microns) photometry of 20 primary and 21 secondary standard stars that are sufficiently faint for large telescope observation is presented. The estimated uncertainties in the magnitudes of the primary standards are 0.01 at L', 0.02 at M, and 0.015 for the L'-M color. A color transformation between the present L' magnitudes and the L magnitudes of Elias et al. (1982) is obtained and found to be near agreement with that predicted for black-bodies.
    Keywords: ASTRONOMY
    Type: Astronomical Journal (ISSN 0004-6256); 89; 1366-137
    Format: text
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