Titan : Interior, Surface, Atmosphere, and Space Environment

Ingo Müller-Wodarg

ISBN 10: 0521199921 / ISBN 13: 9780521199926

Verlag: Cambridge University Press Feb 2014, 2014

Beschreibung

Neuware - Titan, the largest of Saturn's moons, shares remarkable similarities with Earth. Its thick atmosphere is composed primarily of nitrogen; it features the most complex organic chemistry known outside of Earth and, uniquely, hosts an analog to Earth's hydrological cycle, with methane forming clouds, rain and seas. Using the latest data from the ongoing Cassini-Huygens missions, laboratory measurements and numerical simulations, this comprehensive reference examines the physical processes that shape Titan's fascinating atmospheric structure and chemistry, weather, climate, circulation and surface geology. The text also surveys leading theories about Titan's origin and evolution, and assesses their implications for understanding the formation of other complex planetary bodies. Written by an international team of specialists, chapters offer detailed, comparative treatments of Titan's known properties and discuss the latest frontiers in the Cassini-Huygens mission, offering students and researchers of planetary science, geology, astronomy and space physics an insightful reference and guide.

Bestandsnummer des Verkäufers 9780521199926

Bibliografische Details

• Titel: Titan : Interior, Surface, Atmosphere, and Space Environment
• Verlag: Cambridge University Press Feb 2014
• Erscheinungsjahr: 2014
• Sprache: Englisch
• ISBN-10: 0521199921
• ISBN-13: 9780521199926
• Einband: Buch
• Zustand: Neu
• Abmessungen: 287B x 220 H x 30 T Millimeter Breite: 287 mm, Höhe: 220 mm, Tiefe: 30 mm
• Gewicht: 1611 Gramm

Über diesen Titel

Inhaltsangabe

"Although Titan is similar in terms of mass and size to Jupiter's moons, Ganymede and Callisto, it is the only one harboring a massive atmosphere. Moreover, unlike the Jovian system populated with four large moons, Titan is the only large moon around Saturn. The other Saturnian moons are much smaller and have an average density at least 25% less that Titan's uncompressed density and much below the density expected for a Solar composition (Johnson and Lunine, 2005), although with a large variation from satellite to satellite. Both Jupiter's and Saturn's moon systems are thought to have formed in a disk around the growing giant planet. However, the difference in architecture between the two systems probably reflects different disk characteristics and evolution (e.g. Sasaki et al., 2010), and in the case of Saturn, possibly the catastrophic loss of one or more Titan-sized moons (Canup, 2010). Moreover, the presence of a massive atmosphere on Titan as well as the emission of gases from Enceladus' active south polar region (Waite et al., 2009) suggest that the primordial building blocks that comprise the Saturnian system were probably more volatile-rich than Jupiter's"--

Über die Autorinnen und Autoren

Ingo Müller-Wodarg is Reader in Planetary Science at Imperial College London. A specialist in the atmospheres of planets, moons and smaller objects in our Solar System, he has authored or co-authored more than 50 peer-reviewed scientific papers, including 22 on Titan. He is a team member of the Cassini Ion Neutral Mass Spectrometer, Team Leader for the Venus Express Atmospheric Drag Experiment, and plays key roles in designing forthcoming space missions, including the Jupiter Icy Moon Explorer mission. In 2002, he was awarded a Royal Society University Research Fellowship.

Caitlin Griffith is Professor of Planetary Sciences at the University of Arizona, where she investigates the atmospheres of planets, moons and exoplanets. She has authored or co-authored 80 peer-reviewed scientific papers, many of which concern Titan. In 1995, she was awarded the National Science Foundation Young Investigator Award. More recently she has served on the NRC Decadal Study and NASA's Planetary Science Subcommittee, which sets scientific priorities for future American space missions. She is currently helping to design two spacecraft missions to study Titan's organic lakes and the atmospheres of exoplanets.

Emmanuel Lellouch is an astronomer at the Observatoire de Paris. He has authored or co-authored nearly 200 peer-reviewed scientific papers, including 25 on Titan. He has been a member of instrument teams on several space missions, including the Cassini Composite Infrared Spectrometer and the Huygens Descent Imager/Spectral Radiometer. In 1995, he was awarded the Urey Prize of the Division of Planetary Sciences by the American Astronomical Society.

Tom Cravens is Professor of Physics and Astronomy at the University of Kansas. With more than 200 published papers, he has investigated the sources of X-rays throughout the Solar System as well as the upper atmospheres and ionospheres of most Solar System planets and satellites, including Titan. A fellow of the American Geophysical Union, he is a team member of the Cassini Ion and Neutral Mass Spectrometer and author of the Cambridge University Press textbook Physics of Solar System Plasmas (1997).