New Vision of the Saturnian System in the Context of a Highly Dissipative Saturn
暫譯: 在高度耗散的土星背景下的土星系新視野
Lainey, Valéry, Blanc, Michel, Crida, Aurélien
- 出版商: Springer
- 出版日期: 2026-07-21
- 售價: $2,540
- 貴賓價: 9.5 折 $2,413
- 語言: 英文
- 頁數: 463
- 裝訂: Hardcover - also called cloth, retail trade, or trade
- ISBN: 9402423869
- ISBN-13: 9789402423860
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相關分類:
物理學 Physics
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相關主題
商品描述
This book collects a set of contributions that reflect the profound transformation in our understanding of Saturn and its system of rings and moons. Once considered a relatively stable and slowly evolving system, it is now recognized as highly dynamic, shaped by unexpectedly strong tidal dissipation within the planet. This has major implications for the orbital evolution of its satellites, suggesting rapid outward migration and challenging long-standing views on the age and origin of both moons and rings. Central to these advances is the wealth of data returned by the Cassini mission, whose long-term observations, combined with significant progress in theoretical modeling, have reshaped our picture of the coupled evolution of Saturn, its interior, its rings, and its satellites.
Bringing together leading experts across planetary science, this volume presents a coherent and interdisciplinary synthesis of these developments. The contributions explore the dynamical history of the Saturnian system, the processes governing tidal dissipation, and the complex interactions between rings, moons, and planetary interiors.
By highlighting both recent breakthroughs and remaining open questions, the book offers a new vision of Saturn as a laboratory for understanding planetary systems. It provides essential insights not only into the evolution of giant planets and their satellites, but also into broader processes shaping planetary systems throughout the Solar System and beyond.
Reprinted from Space Science Reviews, New Vision of the Saturnian System in the Context of a Highly Dissipative Saturn, Vol. 219-222, 2023-2026.
商品描述(中文翻譯)
這本書收集了一系列貢獻,反映了我們對土星及其環和衛星系統理解的深刻變革。曾經被認為是一個相對穩定且緩慢演變的系統,現在卻被認識為高度動態,受到行星內部意外強烈的潮汐耗散影響。這對其衛星的軌道演變有重大影響,暗示著快速的外移,並挑戰了長期以來對衛星和環的年齡及起源的看法。這些進展的核心是卡西尼任務所返回的大量數據,其長期觀測結合理論建模的顯著進展,重新塑造了我們對土星、其內部、環和衛星之間耦合演變的認識。
本書匯集了行星科學領域的領先專家,呈現了這些發展的連貫且跨學科的綜合體。這些貢獻探討了土星系統的動力歷史、主導潮汐耗散的過程,以及環、衛星與行星內部之間的複雜互動。
通過突顯近期的突破和仍然存在的未解問題,本書提供了一個新的視角,將土星視為理解行星系統的實驗室。它不僅提供了對巨行星及其衛星演變的基本見解,還對塑造整個太陽系及更廣泛的行星系統的過程提供了重要的洞察。
重印自《太空科學評論》,《在高度耗散的土星背景下的土星系統新視野》,第219-222卷,2023-2026年。
作者簡介
Valéry Lainey is an astronomer specializing in astrometry, celestial mechanics, and the dynamical evolution of planetary systems. Based at the Observatoire de Paris, his research focuses on the orbital motion of natural satellites--especially those of the giant planets--and long-term tidal interactions. He combines astrometric observations with numerical modeling to study how satellite systems evolve.
Michel Blanc is a space plasma physicist and planetary scientist. He is Chair Professor at Shandong University and Emeritus Professor at the University of Toulouse. His research focuses on planetary magnetospheres and space environments, particularly those of Earth, Saturn, and Jupiter. He contributed to the Cassini-Huygens mission and is involved in NASA's Juno mission, while following ESA's JUICE and China's TianWen-4 missions.
Aurélien Crida is an astrophysicist and professor at Université Côte d'Azur, where he leads the Master of Astrophysics (MAUCA). His research focuses on planetary formation, especially planet-disc interactions driving migration, as well as satellite-ring interactions in systems like Saturn's. He uses analytical methods and numerical simulations to study the formation and evolution of planetary systems.
Jeff Cuzzi is a planetary scientist whose research focuses on planetary rings and early planet formation. He pioneered microwave observations and radiative transfer models of Saturn's rings and later joined the Voyager imaging team, studying the rings of Saturn, Uranus, and Neptune. He served as Interdisciplinary Scientist for Rings and Dust on the Cassini-Huygens mission. His work blends observational and theoretical approaches to understand ring evolution and planetesimal formation.
Maryame El Moutamid is a planetary scientist and celestial mechanician specializing in the dynamics of planetary rings, moons, and interiors. She is a Lead Scientist at the Southwest Research Institute and was previously at Cornell. She earned her Ph.D. from the Paris Observatory in 2013. Her work combines numerical simulations, spacecraft observations, and telescope data to study how gravitational interactions shape planetary systems over time.
Gianrico Filacchione is a planetary scientist and Director of Research specializing in the composition and evolution of Solar System bodies. He uses visible and infrared spectroscopy to study icy satellites, comets, asteroids, rings, and giant planets. He is Principal Investigator of the MIST-A instrument for the Emirates Mission to the Asteroid Belt and co-PI of the VIHI channel on ESA's BepiColombo mission. He has contributed to major missions including Cassini, Rosetta, Juno, and JUICE.
Carly Howett is a planetary scientist focusing on the surface properties of airless bodies. She combines spacecraft data analysis, mission operations, and instrument development to study temperature, composition, and surface processes. She is an Instrument Scientist on NASA's Lucy mission, a Co-Investigator on Europa Clipper, and Principal Investigator of the Ralph instrument on New Horizons, and previously contributed to Cassini.
Tilman Spohn is a planetary geophysicist specializing in the evolution of planets, satellites, and small bodies, and their potential habitability. He served as Executive Director of the International Space Science Institute (2019-2022) and previously directed the DLR Institute of Planetary Research. He has led key mission experiments, including MUPUS on Rosetta's Philae lander and HP3 on NASA's InSight mission, and is a Fellow of the American Geophysical Union.
作者簡介(中文翻譯)
瓦萊里·拉內(Valéry Lainey)是一位專門研究天體測量、天體力學及行星系統動力演化的天文學家。他在巴黎天文台工作,研究重點是自然衛星的軌道運動,特別是巨行星的衛星,以及長期的潮汐相互作用。他結合天體測量觀測與數值建模,研究衛星系統的演化。
米歇爾·布朗(Michel Blanc)是一位太空等離子體物理學家和行星科學家。他是山東大學的講座教授,並且是圖盧茲大學的名譽教授。他的研究重點是行星的磁層和太空環境,特別是地球、土星和木星的環境。他參與了卡西尼-惠更斯任務,並參與了NASA的朱諾任務,同時關注歐洲太空局的JUICE和中國的天問四號任務。
奧雷利安·克里達(Aurélien Crida)是一位天體物理學家,任教於藍色海岸大學(Université Côte d'Azur),並領導天體物理碩士課程(MAUCA)。他的研究重點是行星形成,特別是驅動遷移的行星-盤相互作用,以及像土星這樣的系統中的衛星-環相互作用。他使用分析方法和數值模擬來研究行星系統的形成和演化。
傑夫·庫茲(Jeff Cuzzi)是一位行星科學家,研究重點是行星環和早期行星形成。他開創了對土星環的微波觀測和輻射傳輸模型,並後來加入了旅行者成像團隊,研究土星、天王星和海王星的環。他在卡西尼-惠更斯任務中擔任環和塵埃的跨學科科學家。他的工作結合了觀測和理論方法,以理解環的演化和行星小體的形成。
瑪莉亞梅·艾爾·穆塔米德(Maryame El Moutamid)是一位行星科學家和天體力學家,專注於行星環、衛星和內部結構的動力學。她是西南研究所的首席科學家,之前在康奈爾大學工作。她於2013年在巴黎天文台獲得博士學位。她的工作結合數值模擬、太空船觀測和望遠鏡數據,研究重力相互作用如何隨時間塑造行星系統。
詹里科·菲拉基奧尼(Gianrico Filacchione)是一位行星科學家和研究主任,專門研究太陽系天體的組成和演化。他使用可見光和紅外光譜學來研究冰衛星、彗星、小行星、環和巨行星。他是阿聯酋小行星帶任務的MIST-A儀器的首席研究員,並且是歐洲太空局BepiColombo任務中VIHI通道的共同首席研究員。他參與了包括卡西尼、羅塞塔、朱諾和JUICE等重大任務。
卡莉·霍維特(Carly Howett)是一位行星科學家,專注於無大氣天體的表面特性。她結合太空船數據分析、任務操作和儀器開發,研究溫度、組成和表面過程。她是NASA的露西任務的儀器科學家,歐羅巴快船的共同研究員,以及新視野任務中拉爾夫儀器的首席研究員,並且之前參與了卡西尼任務。
蒂爾曼·斯波恩(Tilman Spohn)是一位行星地球物理學家,專門研究行星、衛星和小天體的演化及其潛在的宜居性。他曾擔任國際太空科學研究所的執行主任(2019-2022),並且之前是德國航空航天中心行星研究所的主任。他主導了多個關鍵任務實驗,包括羅塞塔的菲萊著陸器上的MUPUS和NASA的InSight任務上的HP3,並且是美國地球物理聯合會的會士。