Paper Title:
Outflowing 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
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
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.
Atmospheric escape from young exoplanets
How Atmospheric Escape Shapes Sub-Neptune Planet Populations
Evolution of helium absorption in escaping atmospheres of gas giants orbiting K stars
Atmospheric escape from the young Neptune AU Mic b
Atmospheric erosion of exoplanets
Helium absorption in young stars
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