A general theory of planet formation has been a topic of intense study over many years. The interest in such a theory emerges naturally from asking the question of where our planet came from. However, a general picture is also required which explains not only the planet Earth but the whole Solar System with its diverse planets. Moreover, after the first discovery of an exoplanet around a Sun-like star (Mayor and Queloz 1995) the exoplanet revolution added numerous additional constraints from thousands of systems of planets orbiting stars different than the Sun.The goal of planet formation as...
{"title":"Planet Formation—Observational Constraints, Physical Processes, and Compositional Patterns","authors":"Christoph Mordasini, Remo Burn","doi":"10.2138/rmg.2024.90.03","DOIUrl":"https://doi.org/10.2138/rmg.2024.90.03","url":null,"abstract":"A general theory of planet formation has been a topic of intense study over many years. The interest in such a theory emerges naturally from asking the question of where our planet came from. However, a general picture is also required which explains not only the planet Earth but the whole Solar System with its diverse planets. Moreover, after the first discovery of an exoplanet around a Sun-like star (Mayor and Queloz 1995) the exoplanet revolution added numerous additional constraints from thousands of systems of planets orbiting stars different than the Sun.The goal of planet formation as...","PeriodicalId":501196,"journal":{"name":"Reviews in Mineralogy and Geochemistry","volume":"27 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141868889","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Nearly 30 years after the discovery of the first exoplanet around a main sequence star, thousands of planets have now been confirmed. These discoveries have completely revolutionized our understanding of planetary systems, revealing types of planets that do not exist in our solar system but are common in extrasolar systems, and a wide range of system architectures. Our solar system is clearly not the default for planetary systems. The community is now moving beyond basic characterization of exoplanets (mass, radius, and orbits) towards a deeper characterization of their atmospheres and even surfaces. With improved observational capabilities there is potential to now probe the geology of rocky exoplanets; this raises the possibility of an analogous revolution in our understanding of rocky planet evolution. However, characterizing the geology or geological processes occurring on rocky exoplanets is a major challenge, even with next generation telescopes. This chapter reviews what we may be able to accomplish with these efforts in the near-term and long-term. In the near-term, the James Webb Space Telescope (JWST) is revealing which rocky planets lose versus retain their atmospheres. This chapter discusses the implications of such discoveries, including how even planets with no or minimal atmospheres can still provide constraints on surface geology and long-term geological evolution. Longer-term possibilities are then reviewed, including whether the hypothesis of climate stabilization by the carbonate–silicate cycle can be tested by next generation telescopes. New modeling strategies sweeping through ranges of possibly evolutionary scenarios will be needed to use the current and future observations to constrain rocky exoplanet geology and evolution.
{"title":"Exoplanet Geology: What Can We Learn from Current and Future Observations?","authors":"Bradford J. Foley","doi":"10.2138/rmg.2024.90.15","DOIUrl":"https://doi.org/10.2138/rmg.2024.90.15","url":null,"abstract":"<div>OVERVIEW</div>Nearly 30 years after the discovery of the first exoplanet around a main sequence star, thousands of planets have now been confirmed. These discoveries have completely revolutionized our understanding of planetary systems, revealing types of planets that do not exist in our solar system but are common in extrasolar systems, and a wide range of system architectures. Our solar system is clearly not the default for planetary systems. The community is now moving beyond basic characterization of exoplanets (mass, radius, and orbits) towards a deeper characterization of their atmospheres and even surfaces. With improved observational capabilities there is potential to now probe the geology of rocky exoplanets; this raises the possibility of an analogous revolution in our understanding of rocky planet evolution. However, characterizing the geology or geological processes occurring on rocky exoplanets is a major challenge, even with next generation telescopes. This chapter reviews what we may be able to accomplish with these efforts in the near-term and long-term. In the near-term, the James Webb Space Telescope (JWST) is revealing which rocky planets lose versus retain their atmospheres. This chapter discusses the implications of such discoveries, including how even planets with no or minimal atmospheres can still provide constraints on surface geology and long-term geological evolution. Longer-term possibilities are then reviewed, including whether the hypothesis of climate stabilization by the carbonate–silicate cycle can be tested by next generation telescopes. New modeling strategies sweeping through ranges of possibly evolutionary scenarios will be needed to use the current and future observations to constrain rocky exoplanet geology and evolution.","PeriodicalId":501196,"journal":{"name":"Reviews in Mineralogy and Geochemistry","volume":"2 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141868739","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Natalie R. Hinkel, Allison Youngblood, Melinda Soares-Furtado
Though distant and seemingly unreachable, planets outside the Solar System, or exoplanets, have captivated the imagination of scientists and stargazers alike. With more than 5,000 confirmed exoplanet detections to date, it has become apparent that the Solar System—with multiple small, rocky planets interior to the larger gaseous planets—is not the only possible architecture for planetary systems. For example, some systems have “hot-Jupiters” where Jupiter-sized planets orbit very close to their host star (at distances comparable to the Sun–Mercury separation, e.g., Dawson and Johnson 2018). There are also planets that orbit two stars at the same time—much like Luke Skywalker’s...
{"title":"Host Stars and How Their Compositions Influence Exoplanets","authors":"Natalie R. Hinkel, Allison Youngblood, Melinda Soares-Furtado","doi":"10.2138/rmg.2024.90.01","DOIUrl":"https://doi.org/10.2138/rmg.2024.90.01","url":null,"abstract":"Though distant and seemingly unreachable, planets outside the Solar System, or exoplanets, have captivated the imagination of scientists and stargazers alike. With more than 5,000 confirmed exoplanet detections to date, it has become apparent that the Solar System—with multiple small, rocky planets interior to the larger gaseous planets—is not the only possible architecture for planetary systems. For example, some systems have “hot-Jupiters” where Jupiter-sized planets orbit very close to their host star (at distances comparable to the Sun–Mercury separation, e.g., Dawson and Johnson 2018). There are also planets that orbit two stars at the same time—much like Luke Skywalker’s...","PeriodicalId":501196,"journal":{"name":"Reviews in Mineralogy and Geochemistry","volume":"57 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141868892","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Ian A. Crawford, Mahesh Anand, Simeon Barber, Aidan Cowley, Sarah Crites, Wenzhe Fa, Jessica Flahaut, Lisa R. Gaddis, Ben Greenhagen, Junichi Haruyama, Dana Hurley, Claire L. McLeod, Andrew Morse, Clive R. Neal, Hannah Sargeant, Elliot Sefton-Nash, Romain Tartèse
It has long been recognised (e.g., Ehricke 1985; Spudis 1996, 2016; Duke et al. 2006; Benaroya 2010; Kornuta et al. 2019) that the Moon has the potential to play a pivotal role in the development of a future space-faring civilisation. Indeed, as noted by Duke et al. (2006) in their chapter on the “Development of the Moon” in the first edition of this book (Jolliff et al. 2006a; hereinafter NVM I), the Moon can be viewed as a natural supply station in Earth orbit bearing raw materials that will assist in humanity’s...
{"title":"Lunar Resources","authors":"Ian A. Crawford, Mahesh Anand, Simeon Barber, Aidan Cowley, Sarah Crites, Wenzhe Fa, Jessica Flahaut, Lisa R. Gaddis, Ben Greenhagen, Junichi Haruyama, Dana Hurley, Claire L. McLeod, Andrew Morse, Clive R. Neal, Hannah Sargeant, Elliot Sefton-Nash, Romain Tartèse","doi":"10.2138/rmg.2023.89.19","DOIUrl":"https://doi.org/10.2138/rmg.2023.89.19","url":null,"abstract":"It has long been recognised (e.g., Ehricke 1985; Spudis 1996, 2016; Duke et al. 2006; Benaroya 2010; Kornuta et al. 2019) that the Moon has the potential to play a pivotal role in the development of a future space-faring civilisation. Indeed, as noted by Duke et al. (2006) in their chapter on the “Development of the Moon” in the first edition of this book (Jolliff et al. 2006a; hereinafter NVM I), the Moon can be viewed as a natural supply station in Earth orbit bearing raw materials that will assist in humanity’s...","PeriodicalId":501196,"journal":{"name":"Reviews in Mineralogy and Geochemistry","volume":"94 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138548096","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2023-12-01DOI: 10.2138/rmg.2023.89erratumtable9
Lisa R. Gaddis, Katherine H. Joy, Ben J. Bussey, James D. Carpenter, Ian A. Crawford, R. Elphic, Jasper S. Halekas, Samuel J. Lawrence, Long Xiao
{"title":"ERRATUM: Recent Exploration of the Moon: Science from Lunar Missions Since 2006","authors":"Lisa R. Gaddis, Katherine H. Joy, Ben J. Bussey, James D. Carpenter, Ian A. Crawford, R. Elphic, Jasper S. Halekas, Samuel J. Lawrence, Long Xiao","doi":"10.2138/rmg.2023.89erratumtable9","DOIUrl":"https://doi.org/10.2138/rmg.2023.89erratumtable9","url":null,"abstract":"","PeriodicalId":501196,"journal":{"name":"Reviews in Mineralogy and Geochemistry","volume":"43 ","pages":""},"PeriodicalIF":0.0,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138988546","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Barbara A. Cohen, Carolyn H. van der Bogert, William F. Bottke, Natalie M. Curran, Caleb I. Fassett, Harald Hiesinger, Katherine H. Joy, Sara Mazrouei, Alexander Nemchin, Gregory A. Neumann, Marc V. Norman, Nicolle E. B. Zellner
Establishing an absolute lunar impact chronology has important ramifications for understanding the early structure of the Solar System, to understand the evolution of both the dynamics and composition of the bodies. Our existing understanding of inner Solar System chronology is anchored to the crater density and analogy with impact flux rates on the Moon. The topic of lunar impact history has been the subject of numerous reviews (e.g., Hartmann et al. 2000; Ryder et al. 2000; Stöffler et al. 2006; Chapman et al. 2007; Fassett and Minton 2013; Bottke and Norman 2017; Zellner 2017...
{"title":"Impact History of the Moon","authors":"Barbara A. Cohen, Carolyn H. van der Bogert, William F. Bottke, Natalie M. Curran, Caleb I. Fassett, Harald Hiesinger, Katherine H. Joy, Sara Mazrouei, Alexander Nemchin, Gregory A. Neumann, Marc V. Norman, Nicolle E. B. Zellner","doi":"10.2138/rmg.2023.89.09","DOIUrl":"https://doi.org/10.2138/rmg.2023.89.09","url":null,"abstract":"Establishing an absolute lunar impact chronology has important ramifications for understanding the early structure of the Solar System, to understand the evolution of both the dynamics and composition of the bodies. Our existing understanding of inner Solar System chronology is anchored to the crater density and analogy with impact flux rates on the Moon. The topic of lunar impact history has been the subject of numerous reviews (e.g., Hartmann et al. 2000; Ryder et al. 2000; Stöffler et al. 2006; Chapman et al. 2007; Fassett and Minton 2013; Bottke and Norman 2017; Zellner 2017...","PeriodicalId":501196,"journal":{"name":"Reviews in Mineralogy and Geochemistry","volume":"52 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138547851","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
William M. Farrell, Jasper S. Halekas, Mihaly Horányi, Rosemary M. Killen, Cesare Grava, Jamey R. Szalay, Mehdi Benna, Pamela E. Clark, Michael R. Collier, Anthony Colaprete, Jan Deca, Richard C. Elphic, Shahab Fatemi, Yoshifumi Futaana, Mats Holmström, Dana M. Hurley, Georgiana Y. Kramer, Paul R. Mahaffy, Masaki N. Nishino, Sarah K. Noble, Yoshifumi Saito, Andrew R. Poppe, Kurt D. Retherford, Xu Wang, Shoichiro Yokota
The topics of lofted dust, ejected atomic and molecular species, and plasma interactions at the Moon have made revolutionary strides since the last ‘New Views of the Moon’ review in 2006 (Jolliff et al. 2006). Specifically, in the last 13 years, there have been over a half-dozen spacecraft that are dedicated, wholly or in part, to the study of this neutral, ionized, and particulate atmosphere at the Moon. A key finding is that all three of these phenomena are inter-connected, and suggest the term ‘exosphere’ can be extended to particulates and surface-emitted plasma like reflected protons and exo-ions...
{"title":"The Dust, Atmosphere, and Plasma at the Moon","authors":"William M. Farrell, Jasper S. Halekas, Mihaly Horányi, Rosemary M. Killen, Cesare Grava, Jamey R. Szalay, Mehdi Benna, Pamela E. Clark, Michael R. Collier, Anthony Colaprete, Jan Deca, Richard C. Elphic, Shahab Fatemi, Yoshifumi Futaana, Mats Holmström, Dana M. Hurley, Georgiana Y. Kramer, Paul R. Mahaffy, Masaki N. Nishino, Sarah K. Noble, Yoshifumi Saito, Andrew R. Poppe, Kurt D. Retherford, Xu Wang, Shoichiro Yokota","doi":"10.2138/rmg.2023.89.13","DOIUrl":"https://doi.org/10.2138/rmg.2023.89.13","url":null,"abstract":"The topics of lofted dust, ejected atomic and molecular species, and plasma interactions at the Moon have made revolutionary strides since the last ‘New Views of the Moon’ review in 2006 (Jolliff et al. 2006). Specifically, in the last 13 years, there have been over a half-dozen spacecraft that are dedicated, wholly or in part, to the study of this neutral, ionized, and particulate atmosphere at the Moon. A key finding is that all three of these phenomena are inter-connected, and suggest the term ‘exosphere’ can be extended to particulates and surface-emitted plasma like reflected protons and exo-ions...","PeriodicalId":501196,"journal":{"name":"Reviews in Mineralogy and Geochemistry","volume":"7 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138548404","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Francis M. McCubbin, Jessica J. Barnes, Peng Ni, Hejiu Hui, Rachel L. Klima, David Burney, James M. D. Day, Tomáš Magna, Jeremy W. Boyce, Romain Tartèse, Kathleen E. Vander Kaaden, Edgar Steenstra, Stephen M. Elardo, Ryan A. Zeigler, Mahesh Anand, Yang Liu
The intrinsic properties of the elements and their resulting behavior in natural systems represent the underpinnings of geochemistry as a scientific discipline (Goldschmidt 1937). One of the most valuable intrinsic properties of an element is its volatility. The volatility of an element is most commonly expressed as a 50% condensation temperature, which corresponds to the temperature at which 50% of an element would have condensed from a gas of solar composition at nebular total pressure of 10–4 bars (e.g., Lodders 2003). Refractory elements are characterized by high condensation temperatures with the inverse being true for more...
{"title":"Endogenous Lunar Volatiles","authors":"Francis M. McCubbin, Jessica J. Barnes, Peng Ni, Hejiu Hui, Rachel L. Klima, David Burney, James M. D. Day, Tomáš Magna, Jeremy W. Boyce, Romain Tartèse, Kathleen E. Vander Kaaden, Edgar Steenstra, Stephen M. Elardo, Ryan A. Zeigler, Mahesh Anand, Yang Liu","doi":"10.2138/rmg.2023.89.17","DOIUrl":"https://doi.org/10.2138/rmg.2023.89.17","url":null,"abstract":"The intrinsic properties of the elements and their resulting behavior in natural systems represent the underpinnings of geochemistry as a scientific discipline (Goldschmidt 1937). One of the most valuable intrinsic properties of an element is its volatility. The volatility of an element is most commonly expressed as a 50% condensation temperature, which corresponds to the temperature at which 50% of an element would have condensed from a gas of solar composition at nebular total pressure of 10–4 bars (e.g., Lodders 2003). Refractory elements are characterized by high condensation temperatures with the inverse being true for more...","PeriodicalId":501196,"journal":{"name":"Reviews in Mineralogy and Geochemistry","volume":"1 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138547903","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Robin M. Canup, Kevin Righter, Nicolas Dauphas, Kaveh Pahlevan, Matija Ćuk, Simon J. Lock, Sarah T. Stewart, Julien Salmon, Raluca Rufu, Miki Nakajima, Tomáš Magna
The Earth–Moon system is unusual in several respects. The Moon is roughly ¼ the radius of the Earth—a larger satellite-to-planet size ratio than all known satellites other than Pluto’s Charon. The Moon has a tiny core, perhaps with only ~1% of its mass, in contrast to Earth whose core contains nearly 30% of its mass. The Earth–Moon system has a high total angular momentum, implying a rapidly spinning Earth when the Moon formed. In addition, the early Moon was hot and at least partially molten with a deep magma ocean. Identification of a model for lunar origin that can satisfactorily...
{"title":"Origin of the Moon","authors":"Robin M. Canup, Kevin Righter, Nicolas Dauphas, Kaveh Pahlevan, Matija Ćuk, Simon J. Lock, Sarah T. Stewart, Julien Salmon, Raluca Rufu, Miki Nakajima, Tomáš Magna","doi":"10.2138/rmg.2023.89.02","DOIUrl":"https://doi.org/10.2138/rmg.2023.89.02","url":null,"abstract":"The Earth–Moon system is unusual in several respects. The Moon is roughly ¼ the radius of the Earth—a larger satellite-to-planet size ratio than all known satellites other than Pluto’s Charon. The Moon has a tiny core, perhaps with only ~1% of its mass, in contrast to Earth whose core contains nearly 30% of its mass. The Earth–Moon system has a high total angular momentum, implying a rapidly spinning Earth when the Moon formed. In addition, the early Moon was hot and at least partially molten with a deep magma ocean. Identification of a model for lunar origin that can satisfactorily...","PeriodicalId":501196,"journal":{"name":"Reviews in Mineralogy and Geochemistry","volume":"9 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138548100","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Amy M. Gaffney, Juliane Gross, Lars E. Borg, Kerri L. Donaldson Hanna, David S. Draper, Nick Dygert, Lindy T. Elkins-Tanton, Kelsey B. Prissel, Tabb C. Prissel, Edgar S. Steenstra, Wim van Westrenen
In this chapter, we present and discuss in detail current and novel advances in our understanding of the processes that drove primordial differentiation of the Moon. This chapter focuses on four avenues of study: 1) data and observations generated from remote sensing missions, 2) experimental investigations of magma ocean crystallization processes, 3) physiochemical modeling of magma ocean processes, and 4) chronological constraints on lunar differentiation. Investigations completed over the past decade and a half provide results that allow for continued testing of the lunar magma ocean (LMO) hypothesis. Although much of the recent work provides constraints on the processes that...
{"title":"Magmatic Evolution I: Initial Differentiation of the Moon","authors":"Amy M. Gaffney, Juliane Gross, Lars E. Borg, Kerri L. Donaldson Hanna, David S. Draper, Nick Dygert, Lindy T. Elkins-Tanton, Kelsey B. Prissel, Tabb C. Prissel, Edgar S. Steenstra, Wim van Westrenen","doi":"10.2138/rmg.2023.89.03","DOIUrl":"https://doi.org/10.2138/rmg.2023.89.03","url":null,"abstract":"In this chapter, we present and discuss in detail current and novel advances in our understanding of the processes that drove primordial differentiation of the Moon. This chapter focuses on four avenues of study: 1) data and observations generated from remote sensing missions, 2) experimental investigations of magma ocean crystallization processes, 3) physiochemical modeling of magma ocean processes, and 4) chronological constraints on lunar differentiation. Investigations completed over the past decade and a half provide results that allow for continued testing of the lunar magma ocean (LMO) hypothesis. Although much of the recent work provides constraints on the processes that...","PeriodicalId":501196,"journal":{"name":"Reviews in Mineralogy and Geochemistry","volume":"109 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138547848","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
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