LPI Announces Publication of Space Science Series Volume

CCTPThe Lunar and Planetary Institute (LPI) is pleased to announce the release of Comparative Climatology of Terrestrial Planets, the latest volume in the prestigious Space Science Series, published by The University of Arizona Press. Volumes in the Series are produced under a unique collaborative agreement between the Press and the LPI. The LPI provides pre-press production services, including copyediting and formatting, and the Press provides traditional publishing services, including printing, marketing, and distribution. This unique collaboration enables the Press to offer the books in this series at a price that is affordable to a much wider segment of the community, including graduate students.

The early development of life, a fundamental question for humankind, requires the presence of a suitable planetary climate. Our understanding of how habitable planets come to be begins with the worlds closest to home. Venus, Earth, and Mars differ only modestly in their mass and distance from the Sun, yet their current climates could scarcely be more divergent. Only Earth has abundant liquid water, Venus has a runaway greenhouse, and evidence for life-supporting conditions on Mars points to a bygone era.  In addition, an Earth-like hydrologic cycle has been revealed in a surprising place: Saturn’s cloud-covered satellite Titan has liquid hydrocarbon rain, lakes, and river networks.

Deducing the initial conditions for these diverse worlds and unraveling how and why they diverged to their current climates is a challenge at the forefront of planetary science. Comparative Climatology of the Terrestrial Planets, edited by Stephen J. Mackwell, Amy A. Simon-Miller, Jerald W. Harder, and Mark A. Bullock, with 69 contributing authors, sets forth the foundations for this emerging new science and brings the reader to the forefront of our current understanding of atmospheric formation and climate evolution. Particular emphasis is given to surface-atmosphere interactions, evolving stellar flux, mantle processes, photochemistry, and interactions with the interplanetary environment, all of which influence the climatology of terrestrial planets. From this cornerstone, both current professionals and most especially new students are brought to the threshold, enabling the next generation of new advances in our own solar system and beyond.

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