BEGIN:VCALENDAR VERSION:2.0 PRODID:-//SACCRED - ECPv6.2.9//NONSGML v1.0//EN CALSCALE:GREGORIAN METHOD:PUBLISH X-ORIGINAL-URL:https://saccred.eu X-WR-CALDESC:Events for SACCRED REFRESH-INTERVAL;VALUE=DURATION:PT1H X-Robots-Tag:noindex X-PUBLISHED-TTL:PT1H BEGIN:VTIMEZONE TZID:Europe/Budapest BEGIN:DAYLIGHT TZOFFSETFROM:+0100 TZOFFSETTO:+0200 TZNAME:CEST DTSTART:20200329T010000 END:DAYLIGHT BEGIN:STANDARD TZOFFSETFROM:+0200 TZOFFSETTO:+0100 TZNAME:CET DTSTART:20201025T010000 END:STANDARD END:VTIMEZONE BEGIN:VEVENT DTSTART;TZID=Europe/Budapest:20200630T090000 DTEND;TZID=Europe/Budapest:20200701T180000 DTSTAMP:20240122T015814 CREATED:20200123T102209Z LAST-MODIFIED:20230515T172727Z UID:173-1593507600-1593626400@saccred.eu SUMMARY:Planet formation enters the observational era - an EAS 2020 SYMPOSIUM DESCRIPTION:Aims and scope \n\n\n\nTraditionally\, planet formation was mostly a theoretical field\, with rather loose observational constraints coming from proto-planetary disc observations and the Solar System. The field is now rapidly transforming thanks to ALMA and extreme adaptive optic systems\, which recently made it possible to detect for the first time forming planets in proto-planetary discs and study in detail the structure and chemical composition of the planet building-blocks. Some of these ingredients\, such as planetesimals\, persist across the main sequence as debris discs\, allowing us to study the architectures of (proto)planetary systems across both space and time as they evolve. In this way\, planet formation is now transforming into an observational field.The time is therefore ripe to discuss the status of the field and recent advancements. Many of those have been led by\, or held major contributions from\, European researchers\, making the session especially topical for EAS 2020: for example\, the discovery of embedded\, nascent protoplanets around PDS 70 through direct imaging and in two other systems through the study of disc kinematics\, the in-depth study of selected systems by the ALMA DSHARP Large Programme\, and debris disc surveys such as REASONS. The session will be comprehensive\, spanning planet(esimal) formation and evolution from the pre-main sequence to the Solar system\, and will also include the first results from the ALMA Disc Chemistry Large Programme. \n\n\n\nFor more information\, visit the event’s web page at https://eas.unige.ch/EAS2020/session.jsp?id=S1 \n\n\n\nScientific organisers \n\n\n\n\nGiovanni Rosotti (Leiden; chair)\n\n\n\nAlex Cridland (Leiden; co-chair)\n\n\n\nStefano Facchini (ESO; co-chair)\n\n\n\nSascha Zeegers (Academia Sinica; co-chair)\n\n\n\nElodie Choquet (Marseille)\n\n\n\nCathie Clarke (Cambridge)\n\n\n\nCornelis Dullemond (Heidelberg)\n\n\n\nAgnes Kospal (Budapest)\n\n\n\nJes Jorgensen (Copenhagen)\n\n\n\nGiuseppe Lodato (Milan)\n\n\n\nJonathan Marshall (Academia Sinica)\n\n\n\nLuca Matra (CfA)\n\n\n\nFarzana Meru (Warwick)\n\n\n\nJulien Milli (Grenoble)\n\n\n\nAlessandro Morbidelli (Nice)\n\n\n\nChristoph Mordasini (Bern)\n\n\n\nNicole Pawellek (Cambridge)\n\n\n\nLinda Podio (Arcetri) URL:/event/planet-formation-enters-the-observational-era-an-eas-2020-symposium/ END:VEVENT END:VCALENDAR