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BEGIN:VEVENT
SUMMARY:Colloquium: Konstantin Herbst
DTSTART:20230406T123000Z
DTEND:20230406T133000Z
DTSTAMP:20260926T073630Z
UID:www.aip.de-1682
CATEGORIES:Scientific
CATEGORIES:Generic Event
CATEGORIES:Public
CONTACT:Julián Alvarado-Gómez <julian.alvarado-gomez@aip.de>
DESCRIPTION:Title: Uncovering the Cosmic Threat: Exploring the Impact of C
 osmic Rays on Exoplanetary Habitability\nExoplanets are as diverse as they
  are fascinating. They vary from ultrahot Jupiter-like low-density planets
  to presumed gas-ice-rock mixture worlds that feature twice the Earth&#x27
 \;s bulk density. But much remains to be explored regarding the great dive
 rsity of exoplanetary atmospheres. With the James Webb Space Telescope (JW
 ST) observing the first potential Earth-like exoplanetary atmospheres\, we
  are now on the verge of entering a new era of exoplanetary science in whi
 ch potential atmospheric biosignatures (such as ozone\, nitrous oxide\, an
 d methane) are interpreted with increasing sophistication in terms of the 
 evolution of the planet-star system\, to assess and discount so-called fal
 se positives. However\, to interpret the upcoming observations\, model stu
 dies of planetary atmospheres that account for various processes — like 
 an atmospheric escape\, outgassing\, climate\, photochemistry\, the physic
 s of air showers\, and the transport of cosmic rays through astrosphers\, 
 planetary magnetic fields\, and planetary atmospheres — are necessary. H
 ere\, as an introduction to the field\, the impact of cosmic rays (CRs) on
  the atmospheric ionization and radiation exposure of the solar system pla
 nets Earth\, Mars\, and Venus will be discussed. Further\, utilizing the u
 nique model suite INCREASE\, the potential impact of cosmic rays on atmosp
 heric biosignatures of exoplanets and its consequences for observations wi
 th\, e.g\, JWST is being discussed.\n
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