The Ariel payload design post-PDR

dc.contributor.author
Gómez Cama, José María
dc.contributor.author
Serre, Christophe
dc.contributor.author
et al.
dc.contributor.author
Andrew Caldwell, Georgia Bishop
dc.date.issued
2025-04-24T16:52:17Z
dc.date.issued
2025-04-24T16:52:17Z
dc.date.issued
2024-08-23
dc.date.issued
2025-04-24T16:52:17Z
dc.identifier
0277-786X
dc.identifier
https://hdl.handle.net/2445/220587
dc.identifier
750057
dc.description.abstract
The Ariel space mission will characterize spectroscopically the atmospheres of a large and diverse sample of hundreds of exoplanets. Through the study of targets with a wide range of planetary parameters (mass, density, equilibrium temperature) and host star types the origin for the diversity observed in known exoplanets will be better understood. Ariel is an ESA Medium class science mission (M4) with a spacecraft bus developed by industry under contract to ESA, and a Payload provided by a consortium of national funding agencies in ESA member states, plus contributions from NASA, the CSA and JAXA. The payload is based on a 1-meter class telescope operated at below 60K, built all in Aluminium, which feeds two science instruments. A multi-channel photometer and low-resolution spectrometer instrument (the FGS, Fine Guidance System instrument) operating from 0.5 – 1.95 microns in wavelength provides both guidance information for stabilizing the spacecraft pointing as well as vital scientific information from spectroscopy in the near-infrared and photometry in the visible channels. The Ariel InfraRed Spectrometer (AIRS) instrument provides medium resolution spectroscopy from 1.95 – 7.8 microns wavelength coverage over two instrument channels. Supporting subsystems provide the necessary mechanical, thermal and electronics support to the cryogenic payload. This paper presents the overall picture of the payload for the Ariel mission. The payload tightly integrates the design and analysis of the various payload elements (including for example the integrated STOP analysis of the Telescope and Common Optics) in order to allow the exacting photometric stability requirements for the mission to be met. The Ariel payload has passed through the Preliminary Design Review (completed in Q2 2023) and is now developing and building prototype models of the Telescope, Instruments and Subsystems (details of which will be provided in other contributions to this conference). This paper will present the current status of the development work and outline the future plans to complete the build and verification of the integrated payload.
dc.format
1 p.
dc.format
application/pdf
dc.format
application/pdf
dc.language
eng
dc.publisher
Society of Photo-Optical Instrumentation Engineers (SPIE)
dc.relation
Reproducció del document publicat a: https://doi.org/https://doi.org/10.1117/12.3019713
dc.relation
Proceedings of SPIE, 2024, vol. 13092
dc.relation
https://doi.org/https://doi.org/10.1117/12.3019713
dc.rights
(c) Society of Photo-Optical Instrumentation Engineers (SPIE), 2024
dc.rights
info:eu-repo/semantics/openAccess
dc.source
Articles publicats en revistes (Enginyeria Electrònica i Biomèdica)
dc.subject
Atmosfera
dc.subject
Telescopis
dc.subject
Astronomia
dc.subject
Atmosphere
dc.subject
Telescopes
dc.subject
Astronomy
dc.title
The Ariel payload design post-PDR
dc.type
info:eu-repo/semantics/article
dc.type
info:eu-repo/semantics/publishedVersion


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