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.
Robert Malcuit Libros


Exploring theoretical planetology, this book presents five scenarios to evaluate Mars' potential for terraforming and its implications for the search for habitable exoplanets. Four scenarios focus on Martian satellite capture models, assessing gravitational influences and biological evolution pathways. The fifth examines Mars’ current lifeless state. Through ten chapters, readers will discover how a Mars-like planet can become habitable and the essential conditions for identifying life-supporting exoplanets. It caters to both planetologists and enthusiasts of planetary evolution.