BEGIN:VCALENDAR VERSION:2.0 METHOD:PUBLISH PRODID:-//Missouri State University/Calendar of Events//EN CALSCALE:GREGORIAN X-WR-TIMEZONE:America/Chicago BEGIN:VTIMEZONE TZID:America/Chicago BEGIN:DAYLIGHT TZOFFSETFROM:-0600 TZOFFSETTO:-0500 DTSTART:20070311T020000 RRULE:FREQ=YEARLY;BYMONTH=3;BYDAY=2SU TZNAME:CDT END:DAYLIGHT BEGIN:STANDARD TZOFFSETFROM:-0500 TZOFFSETTO:-0600 DTSTART:20071104T020000 RRULE:FREQ=YEARLY;BYMONTH=11;BYDAY=1SU TZNAME:CST END:STANDARD END:VTIMEZONE BEGIN:VEVENT UID:7f9a4e3c-95fc-4367-b412-124571ccc391.215853@calendar.missouristate.edu CREATED:20210329T134958Z LAST-MODIFIED:20210329T134958Z LOCATION: SUMMARY:PAMS Seminar: "Using ro-vibrational Emission from Protoplanetary D isks in Order to Observe Accretion and Planet Formation in Action" by Jos hua Kern DESCRIPTION:Joshua Kern is an alumnus from MSU\, graduating in 2015 with a BS in Physics and in 2017 with an MNAS degree. He is currently a PhD stu dent at Clemson University\, Department of Physics & Astronomy.\n\n\nAbst ract:Stars and planets form from collapsing clouds of gas. The detailed s tory of how that material moves from the gas cloud and eventually onto th e star or forming planets is intimately tied to the physics of protoplane tary disks. In the past 30 years\, advances in ground-based radio and inf rared telescope facilities (as well as theoretical models) have allowed a stronomers to probe the chemistry and dynamics of these disks on scales t hat are important for observing accretion and planet formation in action.   This talk will highlight aspects of protoplanetary disk physics\, their connection with observations\, and some exciting preliminary results fro m the spectroscopic analysis of ro-vibrational emission observed using iS HELL at the NASA Infrared Telescope Facility in Mauna Kea\, Hawaii.\n\n\n This seminar will be held exclusively on Zoom (955 5209 1021). Please vis it the Physics Seminars page for a link. X-ALT-DESC;FMTTYPE=text/html:<html><head><title></title></head><body><p><s trong>Joshua Kern&nbsp\;is an alumnus from MSU\, graduating in 2015 with a BS in Physics and in 2017 with an MNAS degree. He is currently a PhD st udent at Clemson&nbsp\;</strong><b>University\, Department of Physics &am p\; Astronomy.</b></p>\n<p>Abstract:<br>Stars and planets form from colla psing clouds of gas. The detailed story of how that material moves from t he gas cloud and eventually onto the star or forming planets is intimatel y tied to the physics of protoplanetary disks. In the past 30 years\, adv ances in ground-based radio and infrared telescope facilities (as well as theoretical models) have allowed astronomers to probe the chemistry and dynamics of these disks on scales that are important for observing accret ion and planet formation in action.&nbsp\; This talk will highlight aspec ts of protoplanetary disk physics\, their connection with observations\, and some exciting preliminary results from the spectroscopic analysis of ro-vibrational emission observed using iSHELL at the NASA Infrared Telesc ope Facility in Mauna Kea\, Hawaii.</p>\n<p>This seminar will be held exc lusively on Zoom (955 5209 1021). Please visit the&nbsp\;<a href="https:/ /physics.missouristate.edu/seminars.htm">Physics Seminars page</a> for a link.</p></body></html> DTSTART;TZID=America/Chicago:20210429T160000 DTEND;TZID=America/Chicago:20210429T170000 SEQUENCE:1 URL:https://physics.missouristate.edu/seminars.htm CATEGORIES:Public,Alumni,Current Students,Faculty,Future Students,Staff END:VEVENT END:VCALENDAR