Published on:
25 April 2024
Primary Category:
Earth and Planetary Astrophysics
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
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
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.
Evolution of helium absorption in escaping atmospheres of gas giants orbiting K stars
Outflow of Helium from a Mature Mini-Neptune
How Atmospheric Escape Shapes Sub-Neptune Planet Populations
Helium absorption in young stars
Atmospheric dynamics and chemistry of ultra-hot Jupiter WASP-189 b
Atmospheric Clues Unlocked in Exoplanet WASP-4b
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