J.M. Trigo-Rodriguez – författare

Josep M. Trigo-Rodriguez Ae Frans J. M. Rietmeijer Ae Jordi Llorca Ae Diego Janches Originally published in the journal Earth, Moon, and Planets, Volume 102, Nos 1-4. DOI: 10. 1007/s11038-008-9228-0 Springer Science+Business Media B. V. 2008 This volume is a compilation of articles that summarize the most recent results in meteor, meteoroid and related ?elds presented at the Meteoroids 2007 conference held in the impressive CosmoCaixa Science Museum in Barcelona, Spain. The conference took place between 11 and 15 of June and was organized by the Institute of Space Sciences (Consejo Superior de Investigaciones Cient?'?cas, CSIC) and the Institut d'Estudis Espacials de Catalunya (IEEC). Researchers in meteor science and supporting ?elds representing more than 20 countries participated at this international conference where 126 presentations were delivered in oral and poster forms. The 69 papers included in this volume represent the work of 154 authors from about 70 different institutions across the globe. The Me- oroids conference is an international meeting that takes place every 3 years since the ?rst one held in Bratislava, Slovakia in 1994. The 2007 meeting was the ?rst one where samples of a comet, 81P/Wild 2, were available from the NASA Stardust mission, and results from laboratory characterizations were presented and discussed.Seemingly aware of the upcoming meeting a bolide was observed over La Mancha, Spain, on May 10.

Josep M. Trigo-Rodriguez Ae Frans J. M. Rietmeijer Ae Jordi Llorca Ae Diego Janches Originally published in the journal Earth, Moon, and Planets, Volume 102, Nos 1-4. DOI: 10. 1007/s11038-008-9228-0 Springer Science+Business Media B. V. 2008 This volume is a compilation of articles that summarize the most recent results in meteor, meteoroid and related ?elds presented at the Meteoroids 2007 conference held in the impressive CosmoCaixa Science Museum in Barcelona, Spain. The conference took place between 11 and 15 of June and was organized by the Institute of Space Sciences (Consejo Superior de Investigaciones Cient?'?cas, CSIC) and the Institut d'Estudis Espacials de Catalunya (IEEC). Researchers in meteor science and supporting ?elds representing more than 20 countries participated at this international conference where 126 presentations were delivered in oral and poster forms. The 69 papers included in this volume represent the work of 154 authors from about 70 different institutions across the globe. The Me- oroids conference is an international meeting that takes place every 3 years since the ?rst one held in Bratislava, Slovakia in 1994. The 2007 meeting was the ?rst one where samples of a comet, 81P/Wild 2, were available from the NASA Stardust mission, and results from laboratory characterizations were presented and discussed.Seemingly aware of the upcoming meeting a bolide was observed over La Mancha, Spain, on May 10.

“The Early Evolution of the Atmospheres of Terrestrial Planets” presents the main processes participating in the atmospheric evolution of terrestrial planets.

“The Early Evolution of the Atmospheres of Terrestrial Planets” presents the main processes participating in the atmospheric evolution of terrestrial planets. A group of experts in the different fields provide an update of our current knowledge on this topic. Several papers in this book discuss the key role of nitrogen in the atmospheric evolution of terrestrial planets. The earliest setting and evolution of planetary atmospheres of terrestrial planets is directly associated with accretion, chemical differentiation, outgassing, stochastic impacts, and extremely high energy fluxes from their host stars. This book provides an overview of the present knowledge of the initial atmospheric composition of the terrestrial planets. Additionally it includes some papers about the current exoplanet discoveries and provides additional clues to our understanding of Earth’s transition from a hot accretionary phase into a habitable world. All papers included were reviewed by experts in their respective fields.We are living in an epoch of important exoplanet discoveries, but current properties of these exoplanets do not match our scientific predictions using standard terrestrial planet models. This book deals with the main physio-chemical signatures and processes that could be useful to better understand the formation of rocky planets.