3.5+ Years of Characterising Exoplanetary Systems with CHEOPS

Characterizing Exoplanets Satellite (CHEOPS) is the first ESA space mission dedicated to the study of known exoplanets. The satellite, carrying a 30cm photometric telescope, carried out its 3.5-year nominal mission between December 2019 and September 2023 is currently in it’s first extended mission. CHEOPS is performing ultra-high precision photometry of exoplanetary systems with a sensitivity allowing to characterise small planets transiting Solar-type stars. CHEOPS is improving density measurements of low-mass planets, detecting and confirming small planets orbiting bright host stars and resolving the architectures of key exoplanet systems, including PLATO-like systems with long-period small planets. CHEOPS also probes planetary atmospheres through measurements of secondary eclipses and phase-curve observations. I will report on highlights of over 4 years worth of CHEOPS science and discuss how the mission is orienting itself in its first extension lasting until December 2026.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2024-10-28
DOI
https://doi.org/10.5281/zenodo.13999844
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
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article

3.5+ Years of Characterising Exoplanetary Systems with CHEOPS

Zenodo (CERN European Organization for Nuclear Research)
Stellar, planetary, and galactic studies
article

3.5+ Years of Characterising Exoplanetary Systems with CHEOPS

article en

Abstract

Characterizing Exoplanets Satellite (CHEOPS) is the first ESA space mission dedicated to the study of known exoplanets. The satellite, carrying a 30cm photometric telescope, carried out its 3.5-year nominal mission between December 2019 and September 2023 is currently in it’s first extended mission. CHEOPS is performing ultra-high precision photometry of exoplanetary systems with a sensitivity allowing to characterise small planets transiting Solar-type stars. CHEOPS is improving density measurements of low-mass planets, detecting and confirming small planets orbiting bright host stars and resolving the architectures of key exoplanet systems, including PLATO-like systems with long-period small planets. CHEOPS also probes planetary atmospheres through measurements of secondary eclipses and phase-curve observations. I will report on highlights of over 4 years worth of CHEOPS science and discuss how the mission is orienting itself in its first extension lasting until December 2026.

Zenodo (CERN European Organization for Nuclear Research)
University of Geneva (CH)
Openalex Percentile: Top 74%
Stellar, planetary, and galactic studies
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