Design of the VenSpec-H instrument on ESA’s EnVision mission: development of critical elements, highlighting the wavefront corrector and grating

• Published in: Journal of applied remote sensing Vol. 19; no. 1; p. 014523
• Main Authors: De Cock, Roderick, Robert, Séverine, Neefs, Eddy, Erwin, Justin, Vervaeke, Michael, Thienpont, Hugo, Renotte, Etienne, Klinkenberg, Philippe, Borguet, Benoit, Thomas, Solal, Moelans, Wouter, Algoedt, Aaron, De Vos, Lieve, Sørensen, Ramatha, Blau, Moshe, Carine Vandaele, Ann, Thomas, Ian R., Berkenbosch, Sophie, Jacobs, Lars, Bogaert, Pieter, Beeckman, Bram, Brassine, Ansje, Messios, Neophytos, De Donder, Erwin, Bolsée, David, Pereira, Nuno, Ristic, Bojan, Tackley, Paul J., Gerya, Taras, Kögl, Stefan, Kögl, Paola, Gröbelbauer, Hans-Peter, Wirz, Florian, Székely, Gerhard Stefan, Eaton, Nick, Roibás-Millán, Elena, Torralbo, Ignacio, Rubio-Arnaldo, Higinio, Álvarez, José Miguel, Ortega, Daniel Navajas, Stam, Daphne, Castro-Marin, Jose M., Ortega, Jaime Jiménez, Lara, Luisa, Helbert, Jörn, Alemanno, Giulia, Marcq, Emmanuel
• Format: Journal Article
• Language: English
• Published: Society of Photo-Optical Instrumentation Engineers 01.01.2025; Bellingham, WA : SPIE
• Subjects: Sciences of the Universe; infrared spectrometer; grating; EnVision; freeform corrector; space instrumentation
• ISSN: 1931-3195; 1931-3195
• DOI: 10.1117/1.JRS.19.014523

EnVision is the European Space Agency’s upcoming mission to Venus with a launch scheduled in 2031. One of the payloads on board is the Venus Spectrometers (VenSpec) suite, containing three spectrometer channels, one of which is Venus Spectrometer with high resolution (VenSpec-H). VenSpec-H performs absorption measurements in the atmosphere of Venus in four near-infrared spectral bands. VenSpec-H is developed under Belgian management and builds on heritage from instruments on Venus Express and Trace Gas Orbiter. The operating wavelength range (1.15 to 2.5  μm) imposes stringent temperature requirements on the instrument to make nightside measurements below the Venus clouds possible. Most importantly, the spectrometer’s optical components are held in a separate cold section inside the instrument, cooled down to −45°C, to remove the thermal background from the signal. Some passive optical elements in the cold spectrometer had low technological readiness at the start of the project. One of them is a wavefront corrector: the freeform corrector plate, used to compensate for aberrations introduced in the system by a parabolic mirror. This device is developed by the Brussels Photonics lab of Vrije Universiteit Brussel using a supply chain with shape-adaptive corrective polishing and dedicated metrology. Another is the echelle grating, used to disperse the incoming light into its spectral components, which is built by Advanced Mechanical and Optical Systems. We highlight the manufacturing and metrology processes of both devices. Besides that, some mechanisms, placed in the warmer part of the instrument, had to be developed: a turn window unit to protect the interior of the instrument during the aerobraking phase of the mission, a filter wheel mechanism to select the spectral bands of interest, and an integrated detector cooler assembly to register the spectra.