Discussion of Some Real and/or Theoretical Effects of Captured Satellites on Both Terrestrial Planets and Gaseous PlanetsThe purpose of this chapter is to demonstrate pathways to make Mars more habitable. Mars as it exists today is not habitable but it probably had habitable conditions for a brief...
It is shown that the sidereal anisotropy (SiA) of cosmic rays (CRs) with energies smaller than 104GeV consists of three kinds: one (GA) is of galactic origin from the direction ΦG(αG= 0 hr;δG= −20°), and the other two (tail-in TA and nose-in HA) are of solar origin ...
The great dichotomy of the Solar System: Small terrestrial embryos and massive giant planet cores Mars in the inner disk and of a few multi-Earth-mass cores in the outer disk, within the lifetime of the gaseous component of the protoplanetary ... A Morbidelli,M Lambrechts,S Jacobson,......
It is shown that the sidereal anisotropy (SiA) of cosmic rays (CRs) with energies smaller than 104GeV consists of three kinds: one (GA) is of galactic origin from the direction ΦG(αG= 0 hr;δG= −20°), and the other two (tail-in TA and nose-in HA) are of solar origin ...
Terrestrial planet formation would not complete until after such an early giant planet instability12,13; the growing terrestrial planets may even have been sculpted by its perturbations, explaining the small mass of Mars relative to Earth14.
It has recently been shown that the terrestrial planets and asteroid belt can be reproduced if the giant planets underwent an inward-then-outward migration (the "Grand Tack"; Walsh et al 2011). Inward migration occurs when Jupiter opens a gap and type II migrates inward. The planets "tack"...
Processes by which terrestrial planets can form in the cores of giant gaseous protoplanets are discussed.doi:10.1016/0019-1035(82)90038-0A.G.W. CameronWilliam M. DecampliPeter BodenheimerElsevier Inc.IcarusCameron, A. G. W., Decampli, W. M., and Bodenheimer, P. (1982) Evolution of ...
There, emissions of light of up to 108 J, would create a Transient Luminous Event (TLE) analogous to a terrestrial " elve" .doi:10.1002/2014JA020457A. LuqueD. DubrovinF. J. Gordillo￢ázquezU. EbertC. PriceJohn Wiley & Sons, Inc.Journal of Geophysical Research: Space Physics...
- Inside this orbit, by contrast, the high density particles are preferentially selected by the vortices and assembled by local gravitational instabilities into planetesimals, massive enough to be released by the vortices and to grow later, in successive collisions, to form the terrestrial planets. ...
- Inside this orbit, by contrast, the high density particles are preferentially selected by the vortices and assembled by local gravitational instabilities into planetesimals, massive enough to be released by the vortices and to grow later, in successive collisions, to form the terrestrial planets.P...