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Atmospheric escape from young exoplanets

Paper Authors:

J. Orell-Miquel,

F. Murgas,

E. Pallé,

M. Mallorquín,

M. López-Puertas,

M. Lampón,

J. Sanz-Forcada,

L. Nortmann,

S. Czesla,

E. Nagel,

I. Ribas,

M. Stangret,

J. Livingston,

E. Knudstrup,

S. H. Albrecht,

I. Carleo,

J. Caballero,

F. Dai,

E. Esparza-Borges,

A. Fukui,

K. Heng,

Th. Henning,

T. Kagetani,

F. Lesjak,

J. P. de Leon,

D. Montes,

G. Morello,

N. Narita,

A. Quirrenbach,

P. J. Amado,

A. Reiners,

A. Schweitzer,

J. I. Vico Linares

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Key Details

20 young exoplanets surveyed for atmospheric escape in helium and hydrogen alpha

New helium triplet detections for TOI-1268b and TOI-2018b

No evidence young planets show more frequent atmospheric escape

Escape signatures peak for 1-3 billion year old systems

Dimensionless ratio R_He/R_Hill may explain helium detections

Upper boundary found for helium detections in temperature-density space

AI generated summary

Atmospheric escape from young exoplanets

This paper presents a survey of 20 young exoplanets looking for atmospheric escape signals in the helium triplet and hydrogen alpha spectral lines. Two new helium detections were found for TOI-1268b and TOI-2018b. When combined with 50 other planets from the literature, the results show that young planets do not exhibit more frequent escape signatures compared to older planets. Instead, escape seems more common for 1-3 billion year old systems. The paper explores what factors best explain the observed helium absorption, like the ratio of the absorbing height to the Hill radius, and it identifies an upper boundary in planet temperature and density above which helium is unlikely to be detected.

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