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
Artikel i vetenskaplig tidskrift, 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.

planets and satellites: gaseous planets

planets and satellites: atmospheres

satellites: physical evolution

planets

techniques: photometric

techniques: radial velocities

Författare

J. Orell-Miquel

Instituto de Astrofísica de Canarias

Universidad de la Laguna

F. Murgas

Instituto de Astrofísica de Canarias

Universidad de la Laguna

Enric Palle

Universidad de la Laguna

Instituto de Astrofísica de Canarias

M. Mallorquín

Instituto de Astrofísica de Canarias

Universidad de la Laguna

M. Lopez-Puertas

Instituto de Astrofisica de Andalucía (IAA)

M. Lampon

Instituto de Astrofisica de Andalucía (IAA)

J. Sanz-Forcada

Centro de Astrobiologia (CAB)

L. Nortmann

Georg-August-Universität Göttingen

S. Czesla

Thüringer Landessternwarte Tautenburg

E. Nagel

Georg-August-Universität Göttingen

I. Ribas

Institut de Ciències de l'Espai (ICE) - CSIC

Institut d'Estudis Espacials de Catalunya (IEEC)

M. Stangret

Istituto nazionale di astrofisica (INAF)

J.H. Livingston

National Astronomical Observatory of Japan

The Graduate University for Advanced Studies (SOKENDAI)

National Institutes of Natural Sciences

Emil Knudstrup

Aarhus Universitet

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

Simon Albrecht

Aarhus Universitet

Ilaria Carleo

Universidad de la Laguna

Instituto de Astrofísica de Canarias

J. A. Caballero

Centro de Astrobiologia (CAB)

Fei Dai

California Institute of Technology (Caltech)

E. Esparza-Borges

Universidad de la Laguna

Instituto de Astrofísica de Canarias

A. Fukui

Instituto de Astrofísica de Canarias

University of Tokyo

Kevin Heng

Ludwig-Maximilians-Universität München (LMU)

T. Henning

Max-Planck-Gesellschaft

T. Kagetani

University of Tokyo

F. Lesjak

Georg-August-Universität Göttingen

Jerome P. De Leon

University of Tokyo

D. Montes

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

Giuseppe Morello

Instituto de Astrofísica de Canarias

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

Norio Narita

University of Tokyo

National Institutes of Natural Sciences

Instituto de Astrofísica de Canarias

A. Quirrenbach

Landessternwarte Heidelberg-Königstuhl

P. J. Amado

Instituto de Astrofisica de Andalucía (IAA)

A. Reiners

Georg-August-Universität Göttingen

A. Schweitzer

Universität Hamburg

J. I. Vico Linares

Calar Alto Astronomical Observatory

Astronomy and Astrophysics

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

Vol. 689 A179

Ämneskategorier

Astronomi, astrofysik och kosmologi

DOI

10.1051/0004-6361/202449411

Mer information

Senast uppdaterat

2024-09-24