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Chapter 3: The Origins and Evolution of Planetary Systems
AstrobiologyThe materials that form the diverse chemicals and structures on Earth—from mountains to oceans and biological organisms—all originated in a universe dominated by hydrogen and helium. Over billions of years, the composition and structure of the galaxies and stars evolved, and the elements of life, CHONPS, were formed through nucleosynthesis in stellar ...
Micah J, Schaible +5 more
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The dynamical evolution of stellar-planetary systems
Astronomy Reports, 2006We have carried out numerical simulations of the dynamical evolution of young stellar-planetary groups using various means to choose the initial conditions, which reflect the various assumptions about the physics of planetary formation: that planets form in circumstellar disks or simultaneously with stars as a result of the fragmentation of molecular ...
A. G. Mal’nev +2 more
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Planetary System Evolution and the Vega Stars: The Potential for Esa’s Infrared Space Observatory
, 1994R. Stencel, D. Backman
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Origin and early evolution of the planetary system
Earth, Moon, and Planets, 1985It is shown by linear stability analysis that a preplanetary (presatellite) disk of dust and gas with Keplerian velocity field can become unstable due to the collective self-gravity of the disk. The radial distribution of rings, which may result from this instability, is derived.
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Evolution History of Extrasolar Planetary Systems
2014In this chapter, we review the basics on the detection and characterization of exoplanetary systems. We first focus on the two leading techniques (the radial velocity and transit methods), deriving the basic quantities that can be extracted from observations with each technique.
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Resonant orbital evolution in the putative planetary system of PSR1257 + 12
Nature, 1992R. Malhotra +3 more
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