Introduction to Earth and Planetary System Science

Author(s):  
Naotatsu Shikazono
Author(s):  
Falko Kuester ◽  
Gloria Brown-Simmons ◽  
Christopher Knox ◽  
So Yamaoka

Author(s):  
Gloria J. Brown-Simmons ◽  
Falko Kuester ◽  
Christopher J. H. Knox ◽  
So Yamaoka

Author(s):  
Gloria Brown-Simmons ◽  
Falko Kuester ◽  
Christopher Knox ◽  
So Yamaoka

1986 ◽  
Author(s):  
Harold Masursky ◽  
Kaare Aksnes ◽  
G.E. Hunt ◽  
M.Y. Marov ◽  
P.M. Millman ◽  
...  

Author(s):  
Karel Schrijver

This chapter describes how the first found exoplanets presented puzzles: they orbited where they should not have formed or where they could not have survived the death of their stars. The Solar System had its own puzzles to add: Mars is smaller than expected, while Venus, Earth, and Mars had more water—at least at one time—than could be understood. This chapter shows how astronomers worked through the combination of these puzzles: now we appreciate that planets can change their orbits, scatter water-bearing asteroids about, steal material from growing planets, or team up with other planets to stabilize their future. The special history of Jupiter and Saturn as a pair bringing both destruction and water to Earth emerged from the study of seventeenth-century resonant clocks, from the water contents of asteroids, and from experiments with supercomputers imposing the laws of physics on virtual worlds.


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