Time-resolved image polarimetry of Trappist-1 during planetary transits

Abstract

We obtained linear polarization photometry ($J$-band) and low-resolution spectroscopy ($ZJ$-bands) of Trappist-1, which is a planetary system formed by an M8-type low-mass star and seven temperate, Earth-sized planets. The photopolarimetric monitoring campaign covered 6.5 h of continuous observations including one full transit of planet Trappist-1d and partial transits of Trappist-1b and e. The spectrophotometric data and the photometric light curve obtained over epochs with no planetary transits indicate that the low-mass star has very low level of linear polarization compatible with a null value. However, the "in transit" observations reveal an enhanced linear polarization signal with peak values of $p^{\ast }=0.1\%$ with a confidence level of 3 $\sigma$, particularly for the full transit of Trappist-1d, thus confirming that the atmosphere of the M8-type star is very likely dusty. Additional observations probing different atmospheric states of Trappist-1 are needed to confirm our findings, as the polarimetric signals involved are low. If confirmed, polarization observations of transiting planetary systems with central ultra-cool dwarfs can become a powerful tool for the characterization of the atmospheres of the host dwarfs and the validation of transiting planet candidates that cannot be corroborated by any other method.

arXiv commentAccepted for publication in MNRAS Letters

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Cited by in corpus (6)

• GJ357: A low-mass planetary system uncovered by precision radial-velocities and dynamical simulations
• Ground-based follow-up observations of TRAPPIST-1 transits in the near-infrared
• Generic Models for Disk-Resolved and Disk-Integrated Phase Dependent Linear Polarization of Light Reflected from Exoplanets
• Polarization of Rotationally Oblate Self-Luminous Exoplanets with Anisotropic Atmospheres
• Time-resolved Optical Polarization Monitoring of the Most Variable Brown Dwarf
• Evolution of spheroidal dust in electrically active sub-stellar atmospheres