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Life near the Roche limit: Behavior of ejecta from satellites close to planets
Icarus, 1980A study of the dynamics of nearby debris from impact craters was made to explain the distinctive features seen on Phobos, Deimis, and Amalthea. The planetary tides and satellite rotation were considered, and the usual pseudo-energy (Jacobi) integral was numerically calculated in the framework of a restricted body problem where satellites are modelled ...
A.R. Dobrovolskis, Joseph A. Burns
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Centaurus X-3 and Roche Limits of Close Binary Systems
Publications of the Astronomical Society of Japan, 1969Abstract The maximum durations of eclipses have been calculated for X-ray eclipsing binaries as a function of mass ratios under the assumption that the X-ray component is a point and the occulting star is confined within the critical Roche lobe of the close binary system.
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A Simplified Theoretical Treatment and Simulated Experimental Calculation of the Roche Limit
The Physics Teacher, 2006First calculated theoretically in 1850 by French mathematician Eduardo Roche, the Roche limit is the approximate distance from a Jovian planet beyond which moons are found. Within this distance, tidal forces (differential gravitational forces) are stronger than the gravitational binding forces between particles so moons cannot form and instead rings ...
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American Journal of Clinical Pathology
Abstract Objectives The aims of this study were to (1) establish the maximum allowable interference limits for hemolysis, lipemia, and icterus for chemistry analytes tested in body fluid samples and (2) assess the effectiveness of serial dilution to mitigate spectral interferences.
Darci R Block +3 more
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Abstract Objectives The aims of this study were to (1) establish the maximum allowable interference limits for hemolysis, lipemia, and icterus for chemistry analytes tested in body fluid samples and (2) assess the effectiveness of serial dilution to mitigate spectral interferences.
Darci R Block +3 more
openaire +2 more sources