1. Главная
  2. Ресурсы
  3. Библиотечный поиск
A chemical survey ofexoplanets with ARIEL G. TinettiP. DrossartPaul Eccleston2018 год

A chemical survey of exoplanets with ARIEL
статья из журнала

Полный текстСтраница публикацииПубликация в OpenAlex
Аннотация: Thousands of exoplanets have now been discovered with a huge range of masses, sizes and orbits: from rocky Earth-like planets to large gas giants grazing the surface of their host star. However, the essential nature of these exoplanets remains largely mysterious: there is no known, discernible pattern linking the presence, size, or orbital parameters of a planet to the nature of its parent star. We have little idea whether the chemistry of a planet is linked to its formation environment, or whether the type of host star drives the physics and chemistry of the planet's birth, and evolution. ARIEL was conceived to observe a large number (~1000) of transiting planets for statistical understanding, including gas giants, Neptunes, super-Earths and Earth-size planets around a range of host star types using transit spectroscopy in the 1.25–7.8 μm spectral range and multiple narrow-band photometry in the optical. ARIEL will focus on warm and hot planets to take advantage of their well-mixed atmospheres which should show minimal condensation and sequestration of high-Z materials compared to their colder Solar System siblings. Said warm and hot atmospheres are expected to be more representative of the planetary bulk composition. Observations of these warm/hot exoplanets, and in particular of their elemental composition (especially C, O, N, S, Si), will allow the understanding of the early stages of planetary and atmospheric formation during the nebular phase and the following few million years. ARIEL will thus provide a representative picture of the chemical nature of the exoplanets and relate this directly to the type and chemical environment of the host star. ARIEL is designed as a dedicated survey mission for combined-light spectroscopy, capable of observing a large and well-defined planet sample within its 4-year mission lifetime. Transit, eclipse and phase-curve spectroscopy methods, whereby the signal from the star and planet are differentiated using knowledge of the planetary ephemerides, allow us to measure atmospheric signals from the planet at levels of 10–100 part per million (ppm) relative to the star and, given the bright nature of targets, also allows more sophisticated techniques, such as eclipse mapping, to give a deeper insight into the nature of the atmosphere. These types of observations require a stable payload and satellite platform with broad, instantaneous wavelength coverage to detect many molecular species, probe the thermal structure, identify clouds and monitor the stellar activity. The wavelength range proposed covers all the expected major atmospheric gases from e.g. H2O, CO2, CH4 NH3, HCN, H2S through to the more exotic metallic compounds, such as TiO, VO, and condensed species. Simulations of ARIEL performance in conducting exoplanet surveys have been performed – using conservative estimates of mission performance and a full model of all significant noise sources in the measurement – using a list of potential ARIEL targets that incorporates the latest available exoplanet statistics. The conclusion at the end of the Phase A study, is that ARIEL – in line with the stated mission objectives – will be able to observe about 1000 exoplanets depending on the details of the adopted survey strategy, thus confirming the feasibility of the main science objectives.
Год издания: 2018
Авторы: G. Tinetti, P. Drossart, Paul Eccleston, P. Hartogh, A. Heske, Jérémy Leconte, G. Micela, Marc Ollivier, G. L. Pilbratt, Ludovic Puig, D. Turrini, B. Vandenbussche, P. Wolkenberg, Jean‐Philippe Beaulieu, Lars A. Buchave, Martin Ferus, Matt Griffin, M. Guêdel, K. Justtanont, Pierre-Olivier Lagage, Pedro Machado, G. Malaguti, M. Min, H. U. Nørgaard-Nielsen, M. Rataj, T. P. Ray, I. Ribas, Mark G. Swain, R. Szabó, Stephanie Werner, J. K. Barstow, M. R. Burleigh, James Cho, Vincent Coudé du Foresto, A. Coustenis, L. Decin, Therese Encrenaz, M. Galand, M. Gillon, Ravit Helled, J. C. Morales, A. García Muñoz, A. Moneti, I. Pagano, E. Pascale, G. Piccioni, D. J. Pinfield, Subhajit Sarkar, Franck Selsis, Jonathan Tennyson, A. H. M. J. Triaud, Olivia Vénot, I. Waldmann, David Waltham, Gillian Wright, J. Amiaux, Jean-Louis Auguères, Michel Berthé, Naidu Bezawada, Georgia Bishop, Neil E. Bowles, Deirdre Coffey, J. Colomé, Martin Crook, P.-E. Crouzet, Vania Da Peppo, I. Escudero Sanz, Mauro Focardi, Martin Frericks, Tom Hunt, Ralf Kohley, Kevin Middleton, G. Morgante, R. Ottensamer, E. Pace, Chris Pearson, R. Stamper, Kate Symonds, M. Rengel, Étienne Renotte, P. A. R. Ade, L. Affer, Christophe Alard, N. F. Allard, F. Altieri, Yves André, Claudio Arena, Ioannis Argyriou, A. D. Aylward, Cristian Baccani, G. Á. Bakos, M. Banaszkiewicz, M. J. Barlow, V. Batista, G. Bellucci, S. Benatti, Pernelle Bernardi, Bruno Bézard, M. I. Błęcka, Émeline Bolmont, Bertrand Bonfond, R. Bonito, A. S. Bonomo, J. R. Brucato, A. S. Brun, Ian Bryson, Waldemar Bujwan, S. L. Casewell, B. Charnay, C. Cecchi‐Pestellini, G. Chen, A. Ciaravella, R. Claudi, R. Clédassou, M. Damasso, Mario Damiano, Camilla Danielski, Pieter Deroo, Anna Maria Di Giorgio, C. Dominik, V. Doublier, S. Doyle, René Doyon, Benjamin Drummond, Bastien Duong, Stephen Eales, Billy Edwards, M. Farina, E. Flaccomio, Leigh N. Fletcher, François Forget, Steve Fossey, M. Fränz, Yuka Fujii, Á. García-Piquer, W. K. Gear, Hervé Geoffray, Jean‐Claude Gérard, Lluís Gesa, H. L. Gomez, Rafał Graczyk, C. A. Griffith, Denis Grodent, M. G. Guarcello, Jacques Gustin, Keiko Hamano, Peter Hargrave, Yann Hello, Kevin Heng, E. Herrero, A. Hornstrup, Benoît Hubert, Shigeru Ida, Masahiro Ikoma, Nicolas Iro, P. G. J. Irwin, C. Jarchow, Jean Jaubert, H. R. A. Jones, Queyrel Julien, Shingo Kameda, F. Kerschbaum, P. Kervella, Tommi Koskinen, Matthijs Krijger, N. Krupp, M. Lafarga, Federico Landini, E. Lellouch, G. Leto, A. Luntzer, Theresa Rank-Lüftinger, A. Maggio, J. Maldonado, Jean-Pierre Maillard, U. Mall, J. B. Marquette, S. Mathis, Pierre Maxted, Taro Matsuo, Alexander S. Medvedev, Yamila Miguel, Vincent Minier, Giuseppe Morello, A. Mura, Norio Narita, V. Nascimbeni, N. Nguyen Tong, Vladimiro Noce, Fabrizio Oliva, Ε. Πάλλη, Paul I. Palmer, M. Pancrazzi, Ανδρέας Παπαγεωργίου, Vivien Parmentier, M. Perger, A. Petralia, S. Pezzuto, Raymond T. Pierrehumbert, I. Pillitteri, G. Piotto, G. Pisano, L. Prisinzano, Aikaterini Radioti, Jean-Michel Réess, L. Rezac, M. Rocchetto, A. Rosich, N. Sanna, A. Santerne, G. Savini, G. Scandariato, B. Sicardy, Carles Sierra, G. Sindoni, Konrad Skup, I. A. G. Snellen, Mateusz Sobiecki, Lauriane Soret, A. Sozzetti, A. Stiepen, Antoine Strugarek, Jake Taylor, W. D. Taylor, L. Terenzi, Marcell Tessenyi, Angelos Tsiaras, C. Tucker, Diana Valencia, Gautam Vasisht, Allona Vazan, F. Vilardell, Sandrine Vinatier, S. Viti, Rens Waters, Piotr Wawer, Anna Wawrzaszek, A. P. Whitworth, Yuk L. Yung, S. N. Yurchenko, M. R. Zapatero Osorio, Robert T. Zellem, T. Zingales, Frans Zwart
Издательство: Springer Science+Business Media
Источник: Experimental Astronomy
Ключевые слова: Stellar, planetary, and galactic studies, Astro and Planetary Science, High-pressure geophysics and materials
Другие ссылки: Experimental Astronomy (PDF)
Experimental Astronomy (HTML)
HAL (Le Centre pour la Communication Scientifique Directe) (PDF)
HAL (Le Centre pour la Communication Scientifique Directe) (HTML)
Edinburgh Research Explorer (University of Edinburgh) (PDF)
Edinburgh Research Explorer (University of Edinburgh) (HTML)
Research Repository at University College Dublin (University College Dublin) (PDF)
Research Repository at University College Dublin (University College Dublin) (HTML)
Leicester Research Archive (University of Leicester) (PDF)
Leicester Research Archive (University of Leicester) (HTML)
Zurich Open Repository and Archive (University of Zurich) (HTML)
Spiral (Imperial College London) (PDF)
Spiral (Imperial College London) (HTML)
BORIS (University Library Bern) (PDF)
BORIS (University Library Bern) (HTML)
Data Archiving and Networked Services (DANS) (PDF)
Data Archiving and Networked Services (DANS) (HTML)
HAL (Le Centre pour la Communication Scientifique Directe) (HTML)
HAL (Le Centre pour la Communication Scientifique Directe) (HTML)
HAL (Le Centre pour la Communication Scientifique Directe) (HTML)
IRIS Research product catalog (Sapienza University of Rome) (PDF)
IRIS Research product catalog (Sapienza University of Rome) (HTML)
Data Archiving and Networked Services (DANS) (PDF)
Data Archiving and Networked Services (DANS) (HTML)
University of Hertfordshire Research Archive (University of Hertfordshire) (PDF)
University of Hertfordshire Research Archive (University of Hertfordshire) (HTML)
Technical University of Denmark, DTU Orbit (Technical University of Denmark, DTU) (HTML)
Technical University of Denmark, DTU Orbit (Technical University of Denmark, DTU) (HTML)
Lirias (KU Leuven) (PDF)
Lirias (KU Leuven) (HTML)
Open Repository and Bibliography (University of Liège) (PDF)
Open Repository and Bibliography (University of Liège) (HTML)
Technical University of Denmark, DTU Orbit (Technical University of Denmark, DTU) (PDF)
Technical University of Denmark, DTU Orbit (Technical University of Denmark, DTU) (HTML)
Chalmers Research (Chalmers University of Technology) (PDF)
Chalmers Research (Chalmers University of Technology) (HTML)
Edinburgh Research Explorer (University of Edinburgh) (HTML)
Keele Research Repository (Keele University) (HTML)
ORCA Online Research @Cardiff (Cardiff University) (HTML)