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A dense ring of the trans-Neptunian object Quaoar outside its Roche limit
Des anneaux planétaires sont observés non seulement autour de planètes géantes1, mais aussi autour de petits corps tels que le Centaure Chariklo2 et la planète naine Haumea3. Jusqu'à présent, tous les anneaux denses connus étaient situés assez près de leurs corps parents, étant à l'intérieur de la limite de Roche, où les forces de marée empêchent les ...
René Duffard, Zouhair Benkhaldoun
exaly +10 more sources
On the Relation between Hot Jupiters and the Roche Limit [PDF]
Many of the known extrasolar planets are ``hot Jupiters,'' giant planets with orbital periods of just a few days. We use the observed distribution of hot Jupiters to constrain the location of the ``inner edge'' and planet migration theory. If we assume the location of the inner edge is proportional to the Roche limit, then we find that this edge is ...
Frederic A Rasio, Eric B. Ford
exaly +4 more sources
Roche's Limits for Satellites [PDF]
THE notice in NATURE (July 15, p. 89) respecting Dr. Fountain's work on Roche's limit for satellites brings to my recollection some estimates which I made many years ago with respect to the stability of satellites moving close to the surface of Mars (Trans. Roy. Dub. Soc., 1897, vol. vi.).
J Joly
exaly +3 more sources
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