We are in a time of transition in our understanding of Mercury. Of particular interest here is the emerging picture of the planet as a system, with interactions between interior, surface, exosphere, and magnetosphere that have influenced and constrained the evolution of each part of the system. Previous books have emphasized the results of Mariner 10 and current ground-based measurements, with very little discussion of the nature and influence of the magnetosphere. This book will present the planet in the context of its surroundings, thus providing a foundation for the next major influx of information from Mercury and contributing to the planning for future missions.

Autorentext

Pamela Clark grew up in New England and, inspired by President John Kennedy, decided she wanted to explore outer space by the time she was thirteen years old. She was encouraged by several teachers, including her sixth grade teacher, Ed Vandall, and high school biology teacher, Robert Blake, as well as by Werner von Braun. She thought, "If they can put a man on the moon, they can put a woman (me) on Mars!" So, she left home to seek her fortune in the space program. She obtained her BA from St. Joseph College, a tiny Catholic women's college run by the Sisters of Mercy in West Hartford, Connecticut. There, she had many opportunities to participate in laboratory research with Sr. Chlorophyll (Dr. Claire Markham) and Sr. Moon Rock (Dr. Mary Ellen Murphy) and to coordinate an NSF inter-disciplinary undergraduate field research project. While obtaining her PhD in planetary geochemistry from the University of Maryland, she worked at GSFC/NASA outside of Washington DC and the Astrogeology Branch of the USGS in Flagstaff, Arizona, simulating, analyzing, correlating, and interpreting lunar X-ray spectra. She was a member of the group, led by Isidore Adler and Jack Trombka, that pioneered the use of orbital x-ray and gamma-ray spectrometers to determine the composition of planetary surfaces. She participated in the Flagstaff Lunar Data Consortium, the first attempt to create a common format for all remote sensing data for a planetary body. After completing her PhD, she joined the technical staff at NASA/JPL outside of Los Angeles for awhile, working with the Ray Jurgens of the Goldstone Solar System Radar group, and expanding her remote sensing background to include radar and thermal and near infrared studies of planetary surfaces with particular emphasis on the study of the physical nature of Mercury's surface. Dr. Clark helped to organize a consortium of scientists interested in Mercury and edits the Mercury Messenger newsletter. She eventually returned Goddard as amember of the XGRS team on the NEAR mission to asteroid Eros. Currently, as a member of the sciences and exploration division at GSFC, Dr. Clark is the science lead in a group initiated by Steve Curtis to develop new paradigms for the design of space missions and vehicles. She provides science support for the Magnetosphere Multi-Scale Mission, and continues to study the Moon, asteroids, and Mercury. Dr. Clark has done several stints in academic institutions, including Murray State University in Kentucky, Albright College in Reading, Pennsylvania, and Catholic University in Washington DC. She has developed courses in analytical and environmental chemistry, geochemistry, physical geology, mineralogy, optics, planetary astronomy, remote sensing, and physics. A space scientist by day, Dr. Clark is otherwise engaged in prison ministry, or in writing about or giving workshops in her wide-ranging fields of interest, including oral and local history, genealogy, Irish history, Celtic spirituality, herb gardening, and cooking. One of her major goals in life is to increase the awareness and the sense of wonder about the planet Mercury. Information about her work can be found at http://www.lpi.usra.edu/publications/newsletters/mercmessenger/ or http://ants.gsfc.nasa.gov

Zusammenfassung
UNDERSTANDING THE PLANET MERCURY Thirty years have elapsed since the one and only mission to Mercury, Mariner 10, performed three ?ybys of the planet, capturing moderate-reso- tion (100 m at best) images of one hemisphere (45% of the surface) and d- covering that Mercury could be the only other terrestrial planet to have a global magnetic ?eld and core dynamo analogous to the Earth's. At the time of this writing, the MESSENGER mission to Mercury has been launched. We are still a couple of years away from the ?rst of the next ?ybys of Mercury, by MESSENGER, on its way to insertion into a nearly polar, but highly ellip- cal, orbit, seven years from launch. In the interim, a plethora of ground-based observations has been providing information on hitherto unseen aspects of Mercury's surface and exosphere. Furthermore, Mariner 10 data have been analyzed and reanalyzed as the technology for modeling and image processing has improved, leading to important breakthroughs in our understanding of Mercury and its environment. Thus, we are writing this book with the realization that we are in a time of transition in our understanding of the planet Mercury. Of particular interest to us in this book is the emerging picture of Mercury as a very dynamic system, with interactions between interior, surface, exosphere, and magne- sphere that have in?uenced and constrained the evolution of each part of the system.

Inhalt
Mercury From a Systems Perspective.- Past and Planned Missions to Mercury.- Mercury's Interior.- Mercury's Surface.- Mercury' Exosphere.- Mercury's Magnetosphere.- The Future of Mercury Exploration.