Extrasolar Planets and Astrobiology"This book: Provides extensive grounding in key issues of astrophysics, chemistry, biology and geophysics; over 150 images and illustrations; exercises for each chapter, ranging from straightforward calculation problems to more far-ranging research-oriented exercises; an online component for users that includes new exercises and a continually updated blog of late-breaking scientific news items, fully cross referenced with the book; and extensive bibliographies for each chapter."--BOOK JACKET. |
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LibraryThing Review
User Review - AlanWPowers - LibraryThingScharf provides a clear and stunning immersion into the world of--well, really, literally, the WORLDS of--exoplanets and exosuns. (I haven't seen this one used, but why not--we have "exomoons.") So ... Read full review
Contents
Introduction Background | 1 |
Introduction Background and Preview 1 | 20 |
Problems | 28 |
References and Suggested Reading | 73 |
Planet Formation | 77 |
Extrasolar Planets | 129 |
References | 190 |
a Brief History and its Boundaries | 196 |
References | 296 |
Cosmochemistry Dust and Prebiotic Molecules | 300 |
Comets Meteorites and Protoplanetary Disk | 333 |
References | 360 |
Habitable Zones | 365 |
References | 419 |
Alternate Habitable Zones and Beyond | 424 |
453 | |
Common terms and phrases
actually albedo appears approximately assume atmosphere atoms bodies carbon cell Chapter characteristics chemical chemistry chondrites cloud collapse comets complex composition consider core cosmic rays curve daisies density described detailed detected discuss disk distance dust Earth effect elements embryo energy environment Equation estimate example exist fact Figure formation function further giant planets given grain gravitational growth habitable heating illustration impact increase indicate initial interstellar Jupiter known larger less light lower major mass material mean measurements mechanisms million molecular molecules momentum Moon nature objects observed occur oceans orbital organisms origin particles period phase photons physical planet planetary planetesimals population possible potential present pressure processes produce proto-planetary radiation radius range region relative result seen shown simple solar system solid species star stellar structure surface temperature terrestrial transit typical University worlds zone