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NEAT: a space born astrometric mission for the detection and characterization of nearby habitable planetary systems

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arxiv 1207.6511 v1 pith:UOMJMMQP submitted 2012-07-27 astro-ph.IM astro-ph.SR

Fabien Malbet , Renaud Goullioud , Pierre-Olivier Lagage , Alain Léger , Mike Shao , Antoine Crouzier , the NEAT Consortium This is my paper · ORCID
classification astro-ph.IMastro-ph.SR
keywords missionneatplanetarynearbyastrometriccharacterizationdownearth
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The NEAT (Nearby Earth Astrometric Telescope) mission is a proposal submitted to ESA for its 2010 call for M-size mission within the Cosmic Vision 2015-2025 plan. The main scientific goal of the NEAT mission is to detect and characterize planetary systems in an exhaustive way down to 1 Earth mass in the habitable zone and further away, around nearby stars for F, G, and K spectral types. This survey would provide the actual planetary masses, the full characterization of the orbits including their inclination, for all the components of the planetary system down to that mass limit. NEAT will continue the work performed by Hipparcos and Gaia by reaching a precision that is improved by two orders of magnitude on pointed targets.

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  1. Effects of planetary mass uncertainties on the interpretation of the reflectance spectra of Earth-like exoplanets

    astro-ph.EP 2025-02 conditional novelty 6.0 of 10

    Reflected-light retrievals of cloudy Earth-like exoplanets misidentify the background gas unless the planet's mass is known to roughly 10% precision.

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