Estimate of the environment impact of the ELT instrument MOSAIC

MOSAIC is an instrument for the Extremely Large Telescope (ELT). The instrument has started phase B, and apart from technical and financial requirements, MOSAIC has the additional requirement to investigate and minimise its environmental impact. The first step is to estimate the carbon footprint (and other effects) in a ‘Life Cycle Analysis’, for the instrument development up to Provisional Acceptance in Chile. This paper presents a preliminary analysis, aimed at identifying potential contributors to environmental impact. Investigated contributors are: materials, Full-Time-Equivalents, travel, and transport of the instrument. Not yet investigated (due to lack of information or certainty) are: electronics, test facilities and prototyping. Uncertainty in input data and conversion factors leads to error bars of a factor 2 or larger. Therefore, the outcome of the analysis can be used for internal comparison of contributors only, and it should not be used for comparison to other instruments or disciplines.

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Published
2024-08-23
DOI
https://doi.org/10.1117/12.3018865
Primary Topic
Astronomical Observations and Instrumentation
Type
article
Field-Weighted Citation Impact
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article

Estimate of the environment impact of the ELT instrument MOSAIC

A. Janssen, M. Puech, F. Wildi, M. Rodrigues et al.
Astronomical Observations and Instrumentation
article

Estimate of the environment impact of the ELT instrument MOSAIC

A. Janssen, M. Puech, F. Wildi, M. Rodrigues, Franck Ducret, Gavin Dalton, Éric Prieto, Nazim A. Bharmal, Cyril Pannetier, Rubén Sánchez-Janssen, R. Pelló, Kacem El Hadi, Jeff Lynn, Marisa Garcia Vargas
article en

Abstract

MOSAIC is an instrument for the Extremely Large Telescope (ELT). The instrument has started phase B, and apart from technical and financial requirements, MOSAIC has the additional requirement to investigate and minimise its environmental impact. The first step is to estimate the carbon footprint (and other effects) in a ‘Life Cycle Analysis’, for the instrument development up to Provisional Acceptance in Chile. This paper presents a preliminary analysis, aimed at identifying potential contributors to environmental impact. Investigated contributors are: materials, Full-Time-Equivalents, travel, and transport of the instrument. Not yet investigated (due to lack of information or certainty) are: electronics, test facilities and prototyping. Uncertainty in input data and conversion factors leads to error bars of a factor 2 or larger. Therefore, the outcome of the analysis can be used for internal comparison of contributors only, and it should not be used for comparison to other instruments or disciplines.

Durham University (GB), Observatoire de Paris (FR), University of Oxford (GB), Laboratoire d’Astrophysique de Marseille (FR), UK Astronomy Technology Centre (GB), Netherlands Institute for Radio Astronomy (NL)
Agence Nationale de la Recherche, Science and Technology Facilities Council
Openalex Percentile: Top 86%
Astronomical Observations and Instrumentation
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