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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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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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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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Calculations of the Evolution of Planetary Orbits
Mechanics of Solids, 2021N I Amel'Kin, Amel'Kin N I
exaly
Understanding the evolution of planetary systems with GAPS2
2023Benatti, S., Desidera, S.
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Orbital Dynamics and the Evolution of Planetary Habitability in the AU Mic System
Astronomical Journal, 2022Stephen R Kane +2 more
exaly
The formation and evolution of planetary systems
Geochimica et Cosmochimica Acta, 1990openaire +1 more source