Scientific Library of Tomsk State University

   E-catalog        

Image from Google Jackets
Normal view MARC view

The Twin Sister Planets Venus and Earth electronic resource Why are they so different? / by Robert J. Malcuit.

By: Malcuit, Robert J [author.]Contributor(s): SpringerLink (Online service)Material type: TextTextPublication details: Cham : Springer International Publishing : Imprint: Springer, 2015Description: XIX, 401 p. 225 illus., 68 illus. in color. online resourceContent type: text Media type: computer Carrier type: online resourceISBN: 9783319113883Subject(s): earth sciences | geochemistry | Planetology | Geomorphology | Astrobiology | Geophysics | Earth Sciences | Planetology | Geochemistry | Astrobiology | Geomorphology | Geophysics and Environmental PhysicsDDC classification: 523.4 LOC classification: QB600-701Online resources: Click here to access online
Contents:
Introduction -- The Origin of the Sun and the Early Evolution of the Solar System -- Models for the Origin and Evolution of the Earth-Moon System -- A Prograde Gravitational Capture Model for the Origin and Evolution of the Earth-Moon System -- Some Critical Interpretations and Misinterpretations of Lunar Features -- Origin and Evolution of the Venus-Adonis System: A Retrograde Gravitational Capture Model -- A Retrograde Gravitational Capture Model for the Earth-Moon System -- Planet Orbit – Lunar Orbit Resonances and the History of the Earth-Moon System -- Discussion of the Probability of Finding Habitable Planets for Humans Orbiting Sun-Like Stars -- Summary and Conclusions -- Appendices -- Glossary -- Index.
In: Springer eBooksSummary: This book explains how it came to be that Venus and Earth, while very similar in chemical composition, zonation, size and heliocentric distance from the Sun, are very different in surface environmental conditions. It is argued here that these differences can be accounted for by planetoid capture processes and the subsequent evolution of the planet-satellite system. Venus captured a one-half moon-mass planetoid early in its history in the retrograde direction and underwent its “fatal attraction scenario” with its satellite (Adonis).  Earth, on the other hand, captured a moon-mass planetoid (Luna) early in its history in prograde orbit and underwent a benign estrangement scenario with its captured satellite.
Tags from this library: No tags from this library for this title. Log in to add tags.
No physical items for this record

Introduction -- The Origin of the Sun and the Early Evolution of the Solar System -- Models for the Origin and Evolution of the Earth-Moon System -- A Prograde Gravitational Capture Model for the Origin and Evolution of the Earth-Moon System -- Some Critical Interpretations and Misinterpretations of Lunar Features -- Origin and Evolution of the Venus-Adonis System: A Retrograde Gravitational Capture Model -- A Retrograde Gravitational Capture Model for the Earth-Moon System -- Planet Orbit – Lunar Orbit Resonances and the History of the Earth-Moon System -- Discussion of the Probability of Finding Habitable Planets for Humans Orbiting Sun-Like Stars -- Summary and Conclusions -- Appendices -- Glossary -- Index.

This book explains how it came to be that Venus and Earth, while very similar in chemical composition, zonation, size and heliocentric distance from the Sun, are very different in surface environmental conditions. It is argued here that these differences can be accounted for by planetoid capture processes and the subsequent evolution of the planet-satellite system. Venus captured a one-half moon-mass planetoid early in its history in the retrograde direction and underwent its “fatal attraction scenario” with its satellite (Adonis).  Earth, on the other hand, captured a moon-mass planetoid (Luna) early in its history in prograde orbit and underwent a benign estrangement scenario with its captured satellite.

There are no comments on this title.

to post a comment.