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Titlebook: Red Dwarfs; Their Geological, Ch David S. Stevenson Book 2019Latest edition Springer Nature Switzerland AG 2019 Habitable worlds.exoplaneta

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发表于 2025-3-21 16:34:09 | 显示全部楼层 |阅读模式
书目名称Red Dwarfs
副标题Their Geological, Ch
编辑David S. Stevenson
视频video
概述Combines knowledge from various fields in a cohesive multidisciplinary approach.Written in an accessible and reader-friendly style.Contains a plethora of chapter references and suggestions for further
图书封面Titlebook: Red Dwarfs; Their Geological, Ch David S. Stevenson Book 2019Latest edition Springer Nature Switzerland AG 2019 Habitable worlds.exoplaneta
描述.This thought-provoking book looks at the nature of red dwarf systems as potential homes for life. Realistically, what are the prospects for life on these distant worlds? Could life evolve and survive there? How do these planetary surfaces and geologies evolve? How would life on a planet orbiting a red dwarf differ from life on Earth? And what are the implications for finding further habitable worlds in our galaxy?.The author provides readers with insight into the habitability of planets and how this changes as time progresses and the central star evolves. Since the previous 2013 edition .Under a Crimson Sun., there has been a rise in newly discovered planets orbiting red dwarfs, accompanied by controversial areas of research that test what we think we know about these systems. This revised edition delves into the wealth of new material uncovered since that date. It explains the often conflicting results and analyses put forward and clarifies our understanding of these exciting new worlds. .The chapters explore the full width of relevant scientific discovery and speculation on the potential for red dwarf planets to host life. New content includes improved atmospheric models, new un
出版日期Book 2019Latest edition
关键词Habitable worlds; exoplanetary habitability; Life on exoplanets; Planetary evolution; Red dwarf stars; St
版次2
doihttps://doi.org/10.1007/978-3-030-25550-3
isbn_ebook978-3-030-25550-3
copyrightSpringer Nature Switzerland AG 2019
The information of publication is updating

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Exoplanetary Discovery, of 3605 planets had been confirmed, of which 1414 were Neptune-like; by the time this book goes to press that figure will, most likely, be out of date. Therefore, consider this chapter as an incomplete portrait that has many of its key features presented but not all of the hues and textures indicat
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Deep Cycles and Super-Terrans,n dioxide into the interior in the form of carbonate rock and returns this gas to the atmosphere, thereby modulating the planetary greenhouse effect. One of the more subtle and poorly understood processes is the modulation of surface water—and with it the abundance of many of the ions (both metal an
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Atmospheric Circulation and Climate,oing into understanding how planetary atmospheres may influence the same property. This chapter expands upon, improves the accuracy of, and produces viable models of atmospheres for planets with different orbital distances from red dwarf stars.
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The Niche, Its Hypervolume and the Entropy of Existence,n a few certainties, such as an energy and nutrient source, will life inevitably follow a path to complexity? Although Chaps. 8 and 9 deal with some specifics, this chapter will focus on developing some underlying ideas and principles that are likely to be applicable to all biological systems, no ma
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The Failure of Early Optimism,, Gliese 581 and Gliese 667C. Both systems hosted a number of super-terrans, whose numbers varied often by the month as radial velocity data was interpreted, reinterpreted, discarded, recovered—only for vexing to continue. Obviously, like many of the authors of the papers upon which the book was cen
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A New Hope, mass red dwarf and the closest star to our Sun, making it a particularly attractive target for further investigation. Meanwhile, the older TRAPPIST-1 system has seven planets, several of which could be habitable—at least in the crudest sense. Although each system has its detractors and flaws, both
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Book 2019Latest editionhese distant worlds? Could life evolve and survive there? How do these planetary surfaces and geologies evolve? How would life on a planet orbiting a red dwarf differ from life on Earth? And what are the implications for finding further habitable worlds in our galaxy?.The author provides readers wit
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