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arXiv · 2312.02381

WASP-69b's Escaping Envelope is Confined to a Tail Extending at Least Seven Planet Radii

Dakotah Tyler·Erik A. Petigura·Antonija Oklopčić·Trevor J. David
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Abstract

Studying the escaping atmospheres of highly-irradiated exoplanets is critical for understanding the physical mechanisms that shape the demographics of close-in planets. A number of planetary outflows have been observed as excess H/He absorption during/after transit. Such an outflow has been observed for WASP-69b by multiple groups that disagree on the geometry and velocity structure of the outflow. Here, we report the detection of this planet's outflow using Keck/NIRSPEC for the first time. We observed the outflow 1.28 hours after egress until the target set, demonstrating the outflow extends at least $5.8 \times 10^5$ km or 7.5 planet radii. This detection is significantly longer than previous observations which report an outflow extending $\sim$2.2 planet radii just one year prior. The outflow is blue-shifted by $-$23 km s$^{-1}$ in the planetary rest frame. We estimate a current mass loss rate of 1 $M_{\oplus}$ Gyr$^{-1}$. Our observations are most consistent with an outflow that is strongly sculpted by ram pressure from the stellar wind. However, potential variability in the outflow could be due to time-varying interactions with the stellar wind or differences in instrumental precision.

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Dakotah Tyler, Erik A. Petigura, Antonija Oklopčić, Trevor J. David. 2023-12-04. WASP-69b's Escaping Envelope is Confined to a Tail Extending at Least Seven Planet Radii. https://arxiv.org/abs/2312.02381

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