Titlebook: Solar System Astrophysics; Planetary Atmosphere Eugene F. Milone,William J.F. Wilson Book 2014Latest edition Springer Science+Business Medi

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Comets and Meteors,he flash of light across the sky) and their cause in terms of the heating and ablation of meteoroids plummeting into the Earth’s atmosphere. The chapter concludes with a discussion of interplanetary dust and the effects on it of solar radiation.

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Meteorites, Asteroids and the Age and Origin of the Solar System,mber of small bodies being detected in both the inner and the outer solar system, so we will also describe what has been learned about these objects in recent years. Finally we consider the birth of the solar system in the context of what we know about proto-stellar disks.

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The Giant Planets,l properties of the giant planets are summarized in Table 12.1 excerpted from Cox (2000), the 2012 Astronomical Almanac, Tholen et al. (2000), and other sources, including the NASA-Goddard Space Flight Center website links at http://nssdc.gsfc.nasa.gov/planetary/factsheet/.

delta-waves

Extra-Solar Planetary Systems,rtant as well as some of the more interesting cases. We tackle the thorny question of how to define a planet (and a star, and of those intermediate objects, brown dwarfs). We reexamine the origin and stability of the solar system in this wider context, and conclude with a discussion of habitable zones, our own, in particular.

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Book 2014Latest editionetary atmospheres and of the bodies of the outer solar system and their analogs in other planetary systems. This volume begins with an expanded treatment of the physics, chemistry, and meteorology of the atmospheres of the Earth, Venus, and Mars, moving on to their magnetospheres and then to a full

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Planetary Atmospheres,and temperature variation with height in the atmosphere are derived, as are the centrifugal and Coriolis forces acting on a moving parcel of air. The effects that these and other factors have on global atmospheric structure and circulation are then discussed in detail. The chapter concludes with a d

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The Giant Planets,n system dwarfs the Sun in size. Jupiter, Saturn, and Neptune radiate considerably more energy than they receive from the Sun. The physical and orbital properties of the giant planets are summarized in Table 12.1 excerpted from Cox (2000), the 2012 Astronomical Almanac, Tholen et al. (2000), and oth