Role of Sample Return in Addressing Major Questions in Planetary Sciences

ISBN-13: 9789402420746 / Angielski / Twarda / 2020 / 503 str.

Mahesh Anand; Sara Russell; Yangting Lin

Spis treści

1. Preface (replaces Editorial)
2. Accretion of the Earth – Missing Components?
3. Oxygen Isotopes and Sampling of the Solar System
4. Revolutionizing our Understanding of the Solar System via Sample Return from Mercury
5. What is the oxygen isotope composition of Venus? The scientific case for sample return from Earth’s “sister” planet
6. Constraining the evolutionary history of the Moon and the inner Solar System: A case for new returned lunar samples
7. The non-carbonaceous–carbonaceous meteorite dichotomy
8. Exploring the bimodal Solar System via sample return from the main asteroid belt: The case for revisiting Ceres
9. Concepts of the small body sample return missions - The 1st 10 Ma year evolution of the solar system
10. Organic matter in the Solar System – implications for future on-site and sample return missions    
11. The Importance of Phobos Sample Return for Understanding the Mars-moon System
12. Exploring Mars with Returned Samples
13. Sample collection and return from Mars: Optimising sample collection based on the microbial ecology of terrestrial volcanic environments
14. Concerns of organic contamination for sample return space missions
15. Advanced Curation of Astromaterials for Planetary Science

O autorze

Mahesh Anand is a Professor of Planetary Science and Exploration at the Open University, UK. He received his PhD from the University of Cambridge, UK and subsequently worked as a researcher at the University of Tennessee, USA and at the Natural History Museum, in London, UK before joining the OU. His recent research has focused on understanding the origin and distribution of volatiles in the inner Solar System through laboratory investigations of extraterrestrial samples. He has authored >100 research papers in journals of high-scientific standing and currently chairs the UK-node of the NASA Solar System Exploration Research Virtual Institute (SSERVI).

Sara Russell is Merit Researcher in Cosmic Mineralogy at the Natural History Museum in London, UK, and Visiting Professor at the Open University, UK. She received her PhD from the Open University and worked as a Lindemann postdoctoral fellow at the California Institute of Technology, USA and NASA funded postdoc at the Smithsonian Institution, in Washington DC, USA, before taking up her position at the Museum. Sara analyses meteorites and material returned from space missions to answer fundamental questions about the formation of the Solar System and evolution of the Earth’s Moon. Sara is the proud namesake of Asteroid (5497) Sararussell.

Yangting Lin is a Professor and deputy director of the Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, CAS. He received his PhD from the Institute of Geochemistry, CAS, and worked as an Associate, and then a full Professor in Guangzhou Institute of Geochemistry, CAS, before joining IGGCAS. Since Chang’E-1, Yangting has been deeply involved in Chinese lunar and deep space exploration program. His team decoded the latest phase of volcanic history of the Imbrium basin and determined the lunar deep interior’s composition from the in situ exploration data acquired by the lunar rover Yutu-1 and 2. He has published about 130 peer-reviewed papers.

Meenakshi Wadhwa is a planetary scientist and educator. She received her doctorate from Washington University in St. Louis. She was a postdoctoral researcher at the University of California at San Diego and curator in the Department of Geology at the Field Museum in Chicago before moving to Arizona State University (ASU), where she is a Professor in the School of Earth and Space Exploration. At ASU, she served as director of the Center for Meteorite Studies for over 12 years and is currently director of the School of Earth and Space Exploration. She is a recipient of the Fulbright-Nehru Academic and Professional Excellence Award, the Guggenheim Fellowship and the Nier Prize of the Meteoritical Society. She was recently awarded an American Council on Education Fellowship and is a Fellow of the American Geophysical Union. Asteroid 8356 is named 8356 Wadhwa in her honor.

Kuljeet Kaur Marhas is a cosmochemist who has been involved in analyses of samples returned from NASA Stardust and JAXA Hayabusa-1 mission. She received her doctorate degree from Physical Research Laboratory, India and was a postdoc at Max Planck Institute fur Cosmochimie, Mainz Germany, followed by research associateship at McDonnell Centre for Space science, Washington University St Louis USA. Currently, she is an Associate Professor in Planetary Sciences Division at Physical Research Laboratory, Ahmedabad, India. She has received numerous awards and fellowships including ‘Indian National Science Academy young scientist’, ‘Women Excellence Award, SERB, India’, ‘Eminent Mass Spectrometerist’. She is a conferred fellow of American Geophysical Union for receiving D. Lal Medal.

Shogo Tachibana is a cosmochemist who is interested in what was responsible for making diverse Solar System planets, including the Earth. He received his doctorate from Osaka University, Japan. He has been involved in Hayabusa2 and OSIRIS-REx asteroids sample return missions. He has worked to set the scientific goal of Hayabusa2 and to develop the sample acquisition system. He is now a professor at UTokyo Organization for Planetary and Space Science, the University of Tokyo, and is also a specially appointed professor at Institute of Space and Astronautical Science, JAXA. He is a recipient of the Nier Prize of the Meteoritical Society and the Paul W. Gast Lectureship from the European Association of Geochemistry and the Geochemical Society.

Blurb

In the past 50 years, our understanding of the origin and evolution of the Solar System has grown exponentially, in large part due to the availability of meteorites and the success of sample return missions. This book contains fourteen papers, each led by a team of expert scientists, which review our present understanding of Solar System formation and evolution through sample analysis.

The chapters are structured around three main themes: (i) initial conditions and workings of the Solar System; (ii) planetary habitats; and (iii) sample curation. Through these themes, the volume presents the outstanding scientific questions to be addressed through future missions, identifies specific target bodies to be studied, and evaluates relevant sample curation facilities. In all, the book is intended to assist in formulating a viable strategy for planning future sample return missions.

Previously published in Space Science Reviews in the Topical Collection "Role of Sample Return in Addressing Major Questions in Planetary Sciences”