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Outflow of Helium from a Mature Mini-Neptune

Published on:

3 August 2023

Primary Category:

Earth and Planetary Astrophysics

Paper Authors:

Michael Zhang,

Fei Dai,

Jacob L. Bean,

Heather A. Knutson,

Federica Rescigno

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Key Details

TOI 2134b is the first old mini-Neptune with detected helium loss

It has the weakest helium signal and lowest XUV flux of any detection

The helium absorption points to a Parker wind-like outflow

A strong correlation emerges between expected and observed mass loss

TOI 2134b anchors the low end of planet mass loss observations

AI generated summary

Outflow of Helium from a Mature Mini-Neptune

This paper reports the detection of a tenuous helium outflow from TOI 2134b, the first mature mini-Neptune found to be losing its atmosphere. The planet's advanced age of a few billion years, low XUV irradiation, and weak helium signal provide new insights. When plotted against other helium detections, a strong correlation emerges between the planets' energy-limited mass loss rates and their observed absorption. This anchors theoretical models. More observations are needed to fill in gaps and refine predictions.

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