... planet embedded in a planetesimal disk [33]. In this report we will restrict ourselves to the interaction of a forming planet with its gaseous protoplanetary disk. Here, the embedded planet disturbs the surrounding disk due to its ...
... earth wall ( MSE ) with embedded bridge - supporting piles Qingming Wang & Chao Xu Department of Geotechnical Engineering , Tongji University , Shanghai , China * Panpan Shen_ Shanghai Investigation , Design & Research Institute Co ...
... planet embedded in a circumstellar disk was investigated by Kley (2000). This author studied the evolution of the embedded planet through hydrodynamical simulations (see also the review article by Kley and Burkert 2000). and found that ...
The book covers the topic of Embedded Computers for Spacecraft.
... planet embedded at r = 1 and j = 0 [(a) and (b) adapted from Baruteau et al., 2011a)] and (c) in an equivalent two-dimensional laminar disk with an azimuthal magnetic field (adapted from Guilet et al., 2013). In the turbulent simulation ...
... planet and averaged in time after steady-state conditions are achieved (after 1000 orbits); modified from Fung and Chiang (2016). (b) Nebular surface density with an embedded Jupiter and Saturn near but outside their 3:2 mean-motion ...
... planet embedded in a disk of material surrounding its star. occurs for interaction with an object orbiting beyond the planet: The planet's tug causes the object to speed up, which means the planet has transferred energy away from itself ...
... planet = new Planet(); Optional<Planet> p2 = planetRepository.find(eq("idplanet",""earth"); if (!p2.isPresent()) { planet = p2.get(); } Searching embedded documents Usually, you will have embedded documents, so looking inside them is a ...
... planet embedded in a circumstellar disk show prograde circulation of material within the planet's Roche lobe that is reminiscent of a circumplanetary disk ( Lubow et al . , 1999 , Kley , 1999 ) . These simulations show that gas can flow ...
... planet–disk interactions. Embedded satellites that are not massive enough to open a gap in the disk's density profile undergo what is called type-I migration (Goldreich and Tremaine, 1978a, 1980; Ward, 1997). The density waves launched ...