The MOPYS project: A survey of 70 planets in search of extended He I and H atmospheres No evidence of enhanced evaporation in young planets
Journal article, 2024

During the first billion years of their life, exoplanet atmospheres are modified by different atmospheric escape phenomena that can strongly affect the shape and morphology of the exoplanet itself. These processes can be studied with Lyα, Hα, and/or He I triplet observations. We present high-resolution spectroscopy observations from CARMENES and GIARPS checking for He I and Hα signals in 20 exoplanetary atmospheres: V1298 Tau c, K2-100 b, HD 63433 b, HD 63433 c, HD 73583 b, HD 73583 c, K2-77 b, TOI-2076 b, TOI-2048 b, HD 235088 b, TOI-1807 b, TOI-1136 d, TOI-1268 b, TOI-1683 b, TOI-2018 b, MASCARA-2 b, WASP-189 b, TOI-2046 b, TOI-1431 b, and HAT-P-57 b. We report two new high-resolution spectroscopy He I detections for TOI-1268 b and TOI-2018 b, and a Hα detection for TOI-1136 d. Furthermore, we detect hints of He I for HD 63433 b, and Hα for HD 73583 b and c, which need to be confirmed. The aim of the Measuring Out-flows in Planets orbiting Young Stars (MOPYS) project is to understand the evaporating phenomena and test their predictions from the current observations. We compiled a list of 70 exoplanets with He I and/or Hα observations, from this work and the literature, and we considered the He I and Hα results as proxy for atmospheric escape. Our principal results are that 0.1–1 Gyr planets do not exhibit more He I or Hα detections than older planets, and evaporation signals are more frequent for planets orbiting ∼1–3 Gyr stars. We provide new constraints to the cosmic shoreline, the empirical division between rocky planets and planets with atmosphere, by using the evaporation detections and we explore the capabilities of a new dimensionless parameter, RHe/RHill, to explain the He I triplet detections. Furthermore, we present a statistically significant upper boundary for the He I triplet detections in the Teq versus ρp parameter space. Planets located above that boundary are unlikely to show He I absorption signals.

techniques: photometric

planets

satellites: physical evolution

planets and satellites: atmospheres

techniques: radial velocities

planets and satellites: gaseous planets

Author

J. Orell-Miquel

University of La Laguna

Instituto de Astrofísica de Canarias

F. Murgas

University of La Laguna

Instituto de Astrofísica de Canarias

Enric Palle

University of La Laguna

Instituto de Astrofísica de Canarias

M. Mallorquín

University of La Laguna

Instituto de Astrofísica de Canarias

M. Lopez-Puertas

Spanish National Research Council (CSIC)

M. Lampon

Spanish National Research Council (CSIC)

J. Sanz-Forcada

Centro de Astrobiologia (CAB)

L. Nortmann

University of Göttingen

S. Czesla

Thüringer Landessternwarte Tautenburg

E. Nagel

University of Göttingen

I. Ribas

Centre Tecnològic de Telecomunicacions de Catalunya (CTTC)

Spanish National Research Council (CSIC)

M. Stangret

Istituto nazionale di astrofisica (INAF)

J.H. Livingston

The Graduate University for Advanced Studies (SOKENDAI)

National Astronomical Observatory of Japan

National Institutes of Natural Sciences

Emil Knudstrup

Aarhus University

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Simon Albrecht

Aarhus University

Ilaria Carleo

Instituto de Astrofísica de Canarias

University of La Laguna

J. A. Caballero

Centro de Astrobiologia (CAB)

Fei Dai

California Institute of Technology (Caltech)

E. Esparza-Borges

Instituto de Astrofísica de Canarias

University of La Laguna

A. Fukui

University of Tokyo

Instituto de Astrofísica de Canarias

Kevin Heng

Ludwig Maximilian University of Munich (LMU)

T. Henning

Max Planck Society

T. Kagetani

University of Tokyo

F. Lesjak

University of Göttingen

Jerome P. De Leon

University of Tokyo

D. Montes

IPARCOS-UCM (Instituto de Física de Partículas y del Cosmos)

Giuseppe Morello

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Instituto de Astrofísica de Canarias

Norio Narita

National Institutes of Natural Sciences

University of Tokyo

Instituto de Astrofísica de Canarias

A. Quirrenbach

Heidelberg-Königstuhl State Observatory

P. J. Amado

Spanish National Research Council (CSIC)

A. Reiners

University of Göttingen

A. Schweitzer

University of Hamburg

J. I. Vico Linares

Calar Alto Astronomical Observatory

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 689 A179

Subject Categories (SSIF 2011)

Astronomy, Astrophysics and Cosmology

DOI

10.1051/0004-6361/202449411

More information

Latest update

3/9/2025 1