Ariel: Enabling planetary science across light-years
Abstract
Ariel, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was adopted as the fourth medium-class mission in ESA's Cosmic Vision programme to be launched in 2029. During its 4-year mission, Ariel will study what exoplanets are made of, how they formed and how they evolve, by surveying a diverse sample of about 1000 extrasolar planets, simultaneously in visible and infrared wavelengths. It is the first mission dedicated to measuring the chemical composition and thermal structures of hundreds of transiting exoplanets, enabling planetary science far beyond the boundaries of the Solar System. The payload consists of an off-axis Cassegrain telescope (primary mirror 1100 mm x 730 mm ellipse) and two separate instruments (FGS and AIRS) covering simultaneously 0.5-7.8 micron spectral range. The satellite is best placed into an L2 orbit to maximise the thermal stability and the field of regard. The payload module is passively cooled via a series of V-Groove radiators; the detectors for the AIRS are the only items that require active cooling via an active Ne JT cooler. The Ariel payload is developed by a consortium of more than 50 institutes from 16 ESA countries, which include the UK, France, Italy, Belgium, Poland, Spain, Austria, Denmark, Ireland, Portugal, Czech Republic, Hungary, the Netherlands, Sweden, Norway, Estonia, and a NASA contribution.
Authors 97
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UCL
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Rutherford Appleton Laboratory
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RAL Space
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OU
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Commissariat à l'Énergie Atomique et aux Énergies Alternatives
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CEA
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U. de Bordeaux
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ESA
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M. Min Aachen
Space Research Organisation Netherlands
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SRON
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ESA
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ESA
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JPL
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ESO
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Institute for Space Astrophysics and Planetology · National Institute for Astrophysics
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INAF-IAPS
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KU Leuven
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National Agricultural Technology Institute
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INTA
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U. of Tartu
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IAP
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Technical University of Denmark
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DTU
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Czech Academy of Sciences, Heyrovsky Institute
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J. Heyrovský Institute
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U. of Cardiff
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U. of Vienna
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MPS
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IA
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Osservatorio di Astrofisica e Scienza dello Spazio · National Institute for Astrophysics
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INAF-OAS
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IAC
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CBK
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Consejo Superior de Investigaciones Científicas
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IEEC-CSIC
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Konkoly Obs
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Chalmers University of Technology
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Chalmers U
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U. of Oslo
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ESA
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ESA
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ESA
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ESA
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ESA
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ESA
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ESA
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ESA
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ESA
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ESA
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Rutherford Appleton Laboratory
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RAL Space
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IA
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Commissariat à l'Énergie Atomique et aux Énergies Alternatives
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CEA
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Commissariat à l'Énergie Atomique et aux Énergies Alternatives
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CEA
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Rutherford Appleton Laboratory
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RAL Space
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U. of Oxford
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IEEC-UB
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DIAS
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Consejo Superior de Investigaciones Científicas
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IEEC-CSIC
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RAL TD
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Rutherford Appleton Laboratory
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RAL Space
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IAC
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Rutherford Appleton Laboratory
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RAL Space
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National Institute for Astrophysics
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INAF-OAA
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Institut d'Estudis Espacials de Catalunya
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IEEC
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JPL
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Matthijs Krijger Aachen
Space Research Organisation Netherlands
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SRON
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Admatis
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MSSL
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ActiveSpace
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Osservatorio di Astrofisica e Scienza dello Spazio · National Institute for Astrophysics
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INAF-OAS
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IAS
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U. of Vienna
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U. di Firenze
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RUAG
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La Sapienza
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Rutherford Appleton Laboratory
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RAL Space
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Technical University of Denmark
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DTU
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JPL
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CSL
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UCL
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Rutherford Appleton Laboratory
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RAL Space
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Admatis
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Admatis
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Rutherford Appleton Laboratory
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RAL Space
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Institut d'Estudis Espacials de Catalunya
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IEEC
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OU
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U. of Padova
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U. of Leicester
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UCL
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Laboratoire d’études spatiales et d’instrumentation en astrophysique
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LESIA
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Czech Academy of Sciences, Heyrovsky Institute
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J. Heyrovský Institute
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Laboratoire d’études spatiales et d’instrumentation en astrophysique
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LESIA
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Laboratoire d’études spatiales et d’instrumentation en astrophysique
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LESIA
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McGill U
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IAA
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IA
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IAP
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UCL
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IA
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Laboratoire d’études spatiales et d’instrumentation en astrophysique
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LESIA
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Konkoly Obs
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CSED
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National Astronomical Observatory of Japan
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NAOJ
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Institut d'Estudis Espacials de Catalunya
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IEEC
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Technical University of Denmark
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DTU
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IAP
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La Sapienza
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