BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Instituto de Astrofísica de Andalucía - ECPv6.16.1//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-ORIGINAL-URL:https://www.iaa.csic.es
X-WR-CALDESC:Eventos para Instituto de Astrofísica de Andalucía
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:Europe/Paris
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20230326T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20231029T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20240331T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20241027T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20250330T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20251026T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20240411T123000
DTEND;TZID=Europe/Paris:20240411T133000
DTSTAMP:20260523T033617
CREATED:20240408T094728Z
LAST-MODIFIED:20250125T201527Z
UID:21125-1712838600-1712842200@www.iaa.csic.es
SUMMARY:LP791-18d as a case study for outgassing rocky exoplanets
DESCRIPTION:Over the past three decades\, the discovery of over five thousand exoplanets has opened avenues for atmospheric characterization\, now feasible for a select subset through spectroscopic observations paired with Bayesian inference techniques. These exoplanetary atmospheres serve as crucial windows into planetary formation and evolutionary histories. Achieving accurate interpretations demands a comprehensive approach\, advancing theory and modeling to understand the continuous interplay between exoplanetary atmospheres and their surrounding environments—both lower and upper boundaries. This project focuses on rocky exoplanets situated near their host stars\, often exhibiting states of magma oceans or heightened volcanic activity due to proximity and tidal forces from neighboring planets. These unique candidates offer enhanced opportunities for observing the ongoing production of secondary atmospheres through outgassing processes. We present a holistic modeling framework for understanding interior-atmosphere interactions and predict the atmospheric footprint of the planet’s interior based on its oxidation state. Moreover\, we assess the detectability using the James Webb Space Telescope (JWST) and propose a spectral index capable of inferring the oxidation state of a planet’s interior. \nFecha: 11/04/2024 – 12:30Conferenciante: Dr. Leonardos GkouvelisFiliación: Ludwig-Maximilians-University of Munich\, Germany \n 
URL:https://www.iaa.csic.es/evento/lp791-18d-as-a-case-study-for-outgassing-rocky-exoplanets/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
END:VCALENDAR