Evolution of the Solar System: Constraints from Meteorites
暫譯: 太陽系的演化:來自隕石的限制因素
Hezel, Dominik C., Palme, Herbert, Mezger, Klaus
- 出版商: Springer
- 出版日期: 2026-07-09
- 售價: $4,650
- 貴賓價: 9.5 折 $4,417
- 語言: 英文
- 頁數: 638
- 裝訂: Hardcover - also called cloth, retail trade, or trade
- ISBN: 9402423680
- ISBN-13: 9789402423686
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相關分類:
化學 Chemistry
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商品描述
This essential collection from leading experts in the field of early solar system sciences and astrophysics provides a comprehensive overview of our current understanding of how planetary systems form, and in particular how our solar system formed.
Our knowledge about solar system evolution is based on a broad foundation of chemical and isotope data from meteorites and their components such as Ca, Al-rich inclusions, chondrules, matrix, and presolar grains, as well as from astromaterials of sample return missions, and modelling accretion processes. The chapters in this volume present the latest data and modelling results from cosmochemistry and astrophysics, and discuss their implications for early solar system evolution from the earliest solids formed in the protoplanetary disk, all the way to accretion and differentiation of planetesimals and planet formation. The importance of past, current, and future space missions is highlighted in this context.
The volume is aimed at researchers and advanced students in the field of meteoritics, cosmochemistry, astrophysics, and planetary sciences. Often, the articles take controversial views into account, rather than promoting individual views.
Reprinted from Space Science Reviews, Topical Collection: Evolution of the Solar System: Constraints from Meteorites
商品描述(中文翻譯)
這本由領域內頂尖專家編輯的必備合集,提供了我們對行星系統形成的當前理解的全面概述,特別是我們的太陽系是如何形成的。
我們對太陽系演化的知識是基於來自隕石及其組成部分(如鈣、鋁豐富的包體、球粒、基質和前太陽顆粒)的廣泛化學和同位素數據,以及來自樣本回收任務的天體材料和模型化的聚集過程。本卷中的章節展示了來自宇宙化學和天體物理學的最新數據和模型結果,並討論了這些結果對早期太陽系演化的影響,從原行星盤中形成的最早固體,一直到小行星的聚集和分化以及行星的形成。在這個背景下,過去、現在和未來的太空任務的重要性得到了強調。
本書旨在針對隕石學、宇宙化學、天體物理學和行星科學領域的研究人員和高級學生。文章通常考慮到有爭議的觀點,而不是推廣個別觀點。
摘自《太空科學評論》,專題合集:太陽系的演化:來自隕石的約束。
作者簡介
Dominik Hezel is a cosmochemist and meteoriticist with an additional expertise in data science. His research focus is the origin, formation, and processing of the first solids in the early solar system, and the distribution of meteorite components in the protoplanetary disk. He develops data science and AI tools, and maintained MetBase for many years, before it merged with Astromaterials. Dominik studied at the Universität Heidelberg (Germany), received his doctoral degree from the Universität zu Köln (Germany), was a postdoctoral researcher at the Natural History Museum in London (UK), and is now a staff scientist at the Goethe Universität Frankfurt am Main (Germany).
Herbert Palme studied physics and mathematics at the University of Vienna. After his PhD at the Institut für Radiumforschung und Kernphysik with Prof. Berta Karlik, he moved to Mainz to take a post-doc position with Heinrich Wänke at the Cosmochemistry Department of the Max-Planck-Institut für Chemie. From 1976 to 1977 he spent a year with Ed Anders at the University of Chicago. In 1984 he did his habilitation for mineralogy at the University of Mainz. From 1994 to 2008 Herbert Palme was professor of mineralogy and geochemistry at the University of Cologne. After his retirement he became honorary collaborator at the Senckenberg Museum and Research Institution in Frankfurt.
Klaus Mezger is a petrologist and geochemist with particular expertise in isotope geo- and cosmochemistry. His research focus is on the chemical evolution of the Earth with a focus on the formation of ancient continental crust, and chemical processes in the early Solar system from the formation of the first solids to the accretion and differentiation of planetesimals and planets. He received his doctoral degree from Stony Brook University (USA), was a postdoctoral researcher at the University of Michigan (USA), staff scientist at the Max-Planck Institute for Chemistry (Germany) and professor at the University of Münster (Germany), before joining the faculty at the University of Bern (Switzerland) as professor of Isotope Geology.
Alessandro Morbidelli received the Master in Physics at the University of Milan (Italy) in 1988, and the Ph.D. in Mathematics at the University of Namur (Belgium) in 1991. In 1993 he obtained a CNRS permanent position at the observatoire de la Côte d'Azur in Nice and in 2023 he was elected Professor at Collège de France in Paris. He is an expert of the formation and dynamical evolution of our Solar system. including giant planet formation and orbital migration, the effect of giant planets on the circulation of dust in the disk, planetesimal formation, terrestrial planet formation etc.Morbidelli has been the recipient of the Urey prize of the Division for Planetary Science of the American Astronomical Society in 2000 and the bronze and silver medal of CNRS in 1995 and 2019.
Jutta Zipfel is a petrologist and cosmochemist with broad expertise in meteorites. Her research focus is on the formation conditions of primitive materials in the early solar system and on processes related to accretion and differentiation of asteroidal bodies. She received her doctoral degree from Johannes Gutenberg University in Mainz (Germany), was a postdoctoral researcher at the University of California, San Diego (USA), staff scientist at the Max Planck Institute for Chemistry (Germany) before becoming section leader and curator of the meteorite collection at Senckenberg - Leibniz Institution for Biodiversity and Earth System Research (Germany). Since 2023 she is serving as secretary of the Meteoritical Society.
作者簡介(中文翻譯)
Dominik Hezel 是一位宇宙化學家和隕石學家,並擁有數據科學的專業知識。他的研究重點是早期太陽系中第一批固體的起源、形成和處理,以及隕石成分在原行星盤中的分佈。他開發數據科學和人工智慧工具,並在 MetBase 維護多年,直到其與 Astromaterials 合併。Dominik 在德國海德堡大學學習,並在德國科隆大學獲得博士學位,曾在英國倫敦自然歷史博物館擔任博士後研究員,現在是德國法蘭克福歌德大學的研究科學家。
Herbert Palme 在維也納大學學習物理和數學。在與 Berta Karlik 教授於放射性研究與核物理研究所獲得博士學位後,他移居美因茨,與 Heinrich Wänke 在馬克斯·普朗克化學研究所的宇宙化學部門擔任博士後研究員。1976年至1977年間,他在芝加哥大學與 Ed Anders 共度了一年。1984年,他在美因茨大學獲得礦物學的資格認證。1994年至2008年,Herbert Palme 擔任科隆大學的礦物學和地球化學教授。退休後,他成為法蘭克福森肯貝格博物館和研究機構的榮譽合作者。
Klaus Mezger 是一位岩石學家和地球化學家,特別擅長同位素地球化學和宇宙化學。他的研究重點是地球的化學演化,專注於古老大陸地殼的形成,以及早期太陽系中的化學過程,從第一批固體的形成到小行星和行星的聚集與分化。他在美國石溪大學獲得博士學位,曾在美國密西根大學擔任博士後研究員,並在德國馬克斯·普朗克化學研究所擔任研究科學家,之後在德國明斯特大學擔任教授,最終加入瑞士伯爾尼大學擔任同位素地質學教授。
Alessandro Morbidelli 於1988年在意大利米蘭大學獲得物理碩士學位,並於1991年在比利時納穆爾大學獲得數學博士學位。1993年,他在法國尼斯的藍色海岸天文台獲得法國國家科學研究中心的永久職位,並於2023年當選為法國巴黎高等學院的教授。他是我們太陽系形成和動力演化的專家,包括巨行星的形成和軌道遷移、巨行星對塵埃在盤中循環的影響、小行星的形成、地球行星的形成等。Morbidelli 在2000年獲得美國天文學會行星科學部的烏雷獎,並於1995年和2019年獲得法國國家科學研究中心的銅獎和銀獎。
Jutta Zipfel 是一位岩石學家和宇宙化學家,對隕石有廣泛的專業知識。她的研究重點是早期太陽系中原始材料的形成條件,以及與小行星體的聚集和分化相關的過程。她在德國美因茨的約翰·古騰堡大學獲得博士學位,曾在美國加州大學聖地亞哥分校擔任博士後研究員,並在德國馬克斯·普朗克化學研究所擔任研究科學家,之後成為德國森肯貝格-萊布尼茨生物多樣性與地球系統研究機構的隕石收藏部門負責人和策展人。自2023年以來,她擔任隕石學會的秘書。