BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CLEVER Planets - ECPv6.15.3//NONSGML v1.0//EN CALSCALE:GREGORIAN METHOD:PUBLISH X-ORIGINAL-URL:https://cleverplanets.org X-WR-CALDESC:Events for CLEVER Planets REFRESH-INTERVAL;VALUE=DURATION:PT1H X-Robots-Tag:noindex X-PUBLISHED-TTL:PT1H BEGIN:VTIMEZONE TZID:America/Chicago BEGIN:DAYLIGHT TZOFFSETFROM:-0600 TZOFFSETTO:-0500 TZNAME:CDT DTSTART:20190310T080000 END:DAYLIGHT BEGIN:STANDARD TZOFFSETFROM:-0500 TZOFFSETTO:-0600 TZNAME:CST DTSTART:20191103T070000 END:STANDARD BEGIN:DAYLIGHT TZOFFSETFROM:-0600 TZOFFSETTO:-0500 TZNAME:CDT DTSTART:20200308T080000 END:DAYLIGHT BEGIN:STANDARD TZOFFSETFROM:-0500 TZOFFSETTO:-0600 TZNAME:CST DTSTART:20201101T070000 END:STANDARD BEGIN:DAYLIGHT TZOFFSETFROM:-0600 TZOFFSETTO:-0500 TZNAME:CDT DTSTART:20210314T080000 END:DAYLIGHT BEGIN:STANDARD TZOFFSETFROM:-0500 TZOFFSETTO:-0600 TZNAME:CST DTSTART:20211107T070000 END:STANDARD END:VTIMEZONE BEGIN:VEVENT DTSTART;TZID=America/Chicago:20211019T120000 DTEND;TZID=America/Chicago:20211019T130000 DTSTAMP:20260423T161057 CREATED:20210905T202515Z LAST-MODIFIED:20211012T145141Z UID:2350-1634644800-1634648400@cleverplanets.org SUMMARY:Seminar - Laurette Piani DESCRIPTION:Speaker: LAURETTE PIANI\, CRPG Nancy \nTitle: Distribution of water in the inner Solar System and interest for the origin of water on Earth \nAbstract:Hydrogen is the most abundant element of the Solar System; nonetheless its distribution and evolution in the protoplanetary disk and planetary materials remain fairly unknown. As a striking example\, the origin of Earth’s hydrogen -and thus water- is one of the most puzzling issues. Chondrites are rocky fragments of asteroids that formed at different times and heliocentric distances in the protoplanetary disk. By studying hydrogen in chondrites from different classes and groups\, we can have a window on the water distribution at the time of the planet formation. In this talk\, I will present recent works on hydrogen in chondrites that allow us to discuss the origin of the hydrogen isotopic distribution in the Solar System and implications for the Earth’s water budget. \n\nZoom Meeting Details: \nRegister in advance for this webinar (registration is required for the first attendance only\, you will then be automatically registered for all the following seminars.:\nhttps://riceuniversity.zoom.us/webinar/register/WN_vECxt9E3S_K1QS8zejzl3w \n\n\n\nLink provided in the registration confirmation email\nPassword: CLEVER\n\n  URL:https://cleverplanets.org/event/seminar-laurette-piani/ END:VEVENT BEGIN:VEVENT DTSTART;TZID=America/Chicago:20211005T120000 DTEND;TZID=America/Chicago:20211005T130000 DTSTAMP:20260423T161057 CREATED:20210916T184950Z LAST-MODIFIED:20210928T044212Z UID:2353-1633435200-1633438800@cleverplanets.org SUMMARY:Seminar – Jennifer Bergner DESCRIPTION:Speaker: JENNIFER BERGNER\, UNIVERSITY OF CHICAGO \nTitle: Volatile chemistry in planet-forming disks \nAbstract:The viability of prebiotic chemistry on a nascent planet is dependent on the inventory of volatiles incorporated during the planet’s formation\, particularly carriers of the elements CHNOPS. This raises the questions: how did Earth obtain its prebiotic precursors\, and how commonly do other planets inherit the ingredients for prebiotic chemistry?  By studying the volatile chemistry at play in the evolutionary progenitors of planetary systems (protostars and protoplanetary disks)\, we gain valuable insight into these questions.  In this talk I will share recent progress in characterizing the chemistry of volatile species in planet-forming disks using ALMA\, which reveals how the changing physical environment alters the chemistry over the disk lifetime.  Our complementary simulations and lab experiments of astrophysical ices also allow us to probe the chemistry of the ice phase\, which is currently unobservable but represents the dominant volatile reservoir in disks.  Taken together\, we are assembling a more complete picture of the chemical environment which regulates the formation\, composition\, and potential habitability of planetesimals and planets. \n\nZoom Meeting Details: \nRegister in advance for this webinar (registration is required for the first attendance only\, you will then be automatically registered for all the following seminars.:\nhttps://riceuniversity.zoom.us/webinar/register/WN_vECxt9E3S_K1QS8zejzl3w \n\n\n\nLink provided in the registration confirmation email\nPassword: CLEVER URL:https://cleverplanets.org/event/seminar-jennifer-bergner/ END:VEVENT BEGIN:VEVENT DTSTART;TZID=America/Chicago:20210921T120000 DTEND;TZID=America/Chicago:20210921T130000 DTSTAMP:20260423T161057 CREATED:20210831T214033Z LAST-MODIFIED:20210905T152928Z UID:2330-1632225600-1632229200@cleverplanets.org SUMMARY:Seminar - Anders Johansen DESCRIPTION:Speaker: ANDERS JOHANSEN\, UNIVERSITY OF COPENHAGEN \nTitle: Formation of terrestrial planets by pebble accretion \nAbstract: \nThe formation of the terrestrial planets in the Solar System is normally considered to last several 10s of million years and to have proceeded by giant impacts within a population of Mars-sized protoplanets. Observations of protoplanetary discs around young stars reveal that such discs host several hundred Earth masses of mm-cm sized pebbles. This inspired the pebble accretion theory for planet formation where the cores of giant planets grow by rapid accretion of these pebbles. By extension\, pebble accretion should be an important process in terrestrial planet formation as well. I present a series of new papers where we show that Venus\, Earth and Mars likely formed within 3-5 Myr by rapid pebble accretion. Volatiles such as water\, nitrogen and carbon are delivered by small pebbles that are accreted at the earliest stages of planetary growth. Partition of these volatiles between core\, mantle and atmosphere combined with early atmospheric loss gives good matches to the modern atmospheres and water reservoirs of Venus\, Earth and Mars. Pebble accretion thus gives a quantitive prediction of volatile budgets and atmospheric compositions of terrestrial planets without invoking stochastic giant impacts as the delivery source.\n\n\n\nZoom Meeting Details: \n\nRegister in advance for this webinar (registration is required for the first attendance only\, you will then be automatically registered for all the following seminars.:\nhttps://riceuniversity.zoom.us/webinar/register/WN_vECxt9E3S_K1QS8zejzl3w\n\n\nLink provided in the registration confirmation email\nPassword: CLEVER URL:https://cleverplanets.org/event/clever-planets-seminar-series-2/ CATEGORIES:Lecture/Webinar END:VEVENT BEGIN:VEVENT DTSTART;TZID=America/Chicago:20210907T120000 DTEND;TZID=America/Chicago:20210907T130000 DTSTAMP:20260423T161057 CREATED:20210831T213052Z LAST-MODIFIED:20210905T152949Z UID:2327-1631016000-1631019600@cleverplanets.org SUMMARY:Seminar - Max Collinet DESCRIPTION:Speaker: MAX COLLINET\, GERMAN AEROSPACE CENTER (DLR)\, BERLIN \nTitle: Achondrites as witnesses of early melting processes in planetesimals and planetary embryos: experimental constraints and new meteorite discoveries \nAbstract:\nAchondrite meteorites are highly variable in composition: some are ultramafic (primitive achondrites) while others are basaltic (e.g. eucrites and angrites)\, to trachy-andesitic (e.g. GRA 06128 and Erg Chech 002). Those different groups correspond to the mantle and crust of planetary building blocks\, respectively. They represent a unique opportunity to constrain the early melting processes that affected planetesimals and could have influenced the final composition of planets. \nI will describe two sets of low pressure (20-120 bars) melting experiments on chondritic compositions\, simulating batch and fractional melting (0-30 wt.% melting). They are the first experiments in which the alkali elements were retained successfully during melting at low pressure. By comparing the experimental results with the meteorite record\, I will argue that the melting processes\, and the efficiency of melt extraction\, varied greatly in achondrite parent bodies but that all planetesimals from the inner solar system (i.e. the non-carbonaceous reservoir) were initial rich in alkalis and other moderately volatile elements. The efficient extraction of silicate melts from the ureilite parent body suggest that highly volatile elements were also present during partial melting. \n\n\nZoom Meeting Details: \n\nRegister in advance for this webinar (registration is required for the first attendance only\, you will then be automatically registered for all the following seminars.:\nhttps://riceuniversity.zoom.us/webinar/register/WN_vECxt9E3S_K1QS8zejzl3w\n\n\nLink provided in the registration confirmation email\nPassword: CLEVER URL:https://cleverplanets.org/event/clever-planets-seminar-series/ CATEGORIES:Lecture/Webinar END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20210704 DTEND;VALUE=DATE:20210710 DTSTAMP:20260423T161057 CREATED:20210115T192911Z LAST-MODIFIED:20210115T192911Z UID:2229-1625356800-1625875199@cleverplanets.org SUMMARY:Goldschmidt 2021 DESCRIPTION: URL:https://cleverplanets.org/event/goldschmidt-2021/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20210315 DTEND;VALUE=DATE:20210320 DTSTAMP:20260423T161057 CREATED:20210115T192640Z LAST-MODIFIED:20210115T192640Z UID:2227-1615766400-1616198399@cleverplanets.org SUMMARY:LPSC 2021 DESCRIPTION: URL:https://cleverplanets.org/event/lpsc-2021/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20210222 DTEND;VALUE=DATE:20210227 DTSTAMP:20260423T161057 CREATED:20210115T192438Z LAST-MODIFIED:20210115T192438Z UID:2225-1613952000-1614383999@cleverplanets.org SUMMARY:Habitable Worlds 2021 Workshop DESCRIPTION: URL:https://cleverplanets.org/event/habitable-worlds-2021-workshop/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20201207 DTEND;VALUE=DATE:20201212 DTSTAMP:20260423T161057 CREATED:20200508T192641Z LAST-MODIFIED:20200508T192641Z UID:2176-1607299200-1607731199@cleverplanets.org SUMMARY:AGU 2020 DESCRIPTION:San Francisco URL:https://cleverplanets.org/event/agu-2020/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20200621 DTEND;VALUE=DATE:20200627 DTSTAMP:20260423T161057 CREATED:20200513T221538Z LAST-MODIFIED:20200513T221742Z UID:2193-1592697600-1593215999@cleverplanets.org SUMMARY:Goldschmidt 'Virtual' Conference 2020 DESCRIPTION:San Francisco URL:https://cleverplanets.org/event/goldschmidt-virtual-conference/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20200531 DTEND;VALUE=DATE:20200605 DTSTAMP:20260423T161057 CREATED:20200204T171644Z LAST-MODIFIED:20200204T171644Z UID:2147-1590883200-1591315199@cleverplanets.org SUMMARY:American Astronomical Society meeting DESCRIPTION:Madison\, Wisconsin URL:https://cleverplanets.org/event/american-astronomical-society-meeting/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20200316 DTEND;VALUE=DATE:20200321 DTSTAMP:20260423T161057 CREATED:20200204T171053Z LAST-MODIFIED:20200204T171245Z UID:2144-1584316800-1584748799@cleverplanets.org SUMMARY:Lunar and Planetary Science Conference DESCRIPTION:Held in The Woodlands\, Texas URL:https://cleverplanets.org/event/lunar-and-planetary-science-conference/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20200119 DTEND;VALUE=DATE:20200125 DTSTAMP:20260423T161057 CREATED:20190208T155029Z LAST-MODIFIED:20190208T155029Z UID:1644-1579392000-1579910399@cleverplanets.org SUMMARY:2020 Gordon Research Conference - Origins of Life DESCRIPTION:Information available – April 1\, 2019 \nApplication deadline – December 22\, 2019 URL:https://cleverplanets.org/event/2020-gordon-origins-life/ CATEGORIES:Conference ATTACH;FMTTYPE=image/png:https://cleverplanets.org/wp-content/uploads/2019/02/grc_logo.png END:VEVENT BEGIN:VEVENT DTSTART;TZID=America/Chicago:20191213T112000 DTEND;TZID=America/Chicago:20191213T233500 DTSTAMP:20260423T161057 CREATED:20191209T131816Z LAST-MODIFIED:20191209T131835Z UID:2124-1576236000-1576280100@cleverplanets.org SUMMARY:Talk by Megan Duncan at AGU 2019 DESCRIPTION:San Francisco. \n“Variations in Moderately Volatile Elements in Planetary Bodies from Impact Vaporization” \nAbstract: \nPlanet-building processes have a strong effect on the distribution of the elements in the resulting bodies. In particular\, moderately volatile elements (MVEs) have distinct differences in depletion between the meteorite groups and the planets. Understanding the chemical effects of impacts and post-impact processes are necessary in order to place constraints on the bulk composition of the planet (pre-differentiation). Vaporizing collisions\, common in energetic periods of accretion such giant planet migration and the terrestrial giant impact stage\, can separate refractory and volatile components as the system re-equilibrates during vapor plume expansion and cooling. In order to understand the chemical changes caused by high velocity collisions\, we must know the liquid-vapor phase boundary of the dominant mineral(s) of the original bodies\, likely a silicate mineral such as olivine or pyroxene. To constrain the equations of state of these minerals\, we conducted shock-and-release experiments with the Sandia Z machine on single crystal forsterite\, olivine\, and bronzite to determine the pressure (P)\, temperature (T)\, entropy\, and density of the shocked and post-shocked states. \nUpon decompression from the shocked state\, the high pressure fluid intersects the phase boundary and separates into a two-phase mixture at high P and T (e.g.\, ~1–1000 bar and ~4000–6500 K)\, driving melt-vapor partitioning under near-equilibrium conditions with limited isotopic fractionation. As the system continues to cool\, the MVE concentrations evolve until the system reaches the triple point and the melt freezes. The remaining condensable vapor adsorbs onto the larger solid droplets or condenses as new dust. Thus\, the MVE concentrations in the post-impact system may have large variations that are correlated with particle size. We explore the hypothesis that impact vaporization leads to a net enrichment of MVEs in dust-sized particles. Nebular size-sorting processes may separate the larger\, MVE-poor solids and the MVE-rich dust\, creating zones of variable depletion. During accretion\, the MVE-enriched dust may be variably incorporated into planetesimals and contribute to the chemical diversity observed in meteorites and planets. \nSNL is managed by NTESS under DOE-NSSA contract DE-NA0003525. URL:https://cleverplanets.org/event/talk-by-megan-duncan-at-agu-2019/ CATEGORIES:Conference END:VEVENT BEGIN:VEVENT DTSTART;TZID=America/Chicago:20191212T134000 DTEND;TZID=America/Chicago:20191212T180000 DTSTAMP:20260423T161057 CREATED:20191209T131315Z LAST-MODIFIED:20191209T131315Z UID:2120-1576158000-1576173600@cleverplanets.org SUMMARY:Poster by Daman Grewal at AGU 2019 DESCRIPTION:San Francisco. \n“The core-mantle partitioning of carbon and nitrogen in carbon-undersaturated ultramafic systems” \nAbstract: \nIn addition to their highly volatile character\, segregation into the metallic core could have played an important role in explaining the depletion of carbon (C) and nitrogen (N) in the bulk silicate reservoirs of rocky bodies [e.g.\, 1\,2]. As the core-mantle partitioning character of C and N strongly depends on fO2\, they can act as a powerful tracers to understand the fO2-dependent volatile accretion history of terrestrial bodies. Previous high P-T experimental studies have shown that the highly siderophile character of C increases with decrease in fO2\, but can get suppressed in systems with high fH2\, while N acts as a siderophile element at >IW–2.5 and is lithophile at 4 GPa) remain stable in equilibrium with an H2O-rich fluid. Above the solidus (between 800-850 °C from 3-7 GPa)\, carbonates remain stable along with silicate minerals (cpx\, olivine\, garnet) and a CO2-rich melt phase over a restricted temperature interval until carbonates are completely melted out at T > 1000 °C at 3-5 GPa and > 1100 °C at 7 GPa. \nDue to the breakdown of chlorite at conditions above 3 GPa and 800 °C our experiments suggest that ophicarbonates will be nearly completely dehydrated at subarc depths\, delivering H2O to arc magma source regions. The stability of carbonates in our experiments suggest that even for the hottest subduction zones\, ophicarbonates in the mantle lithosphere (below slab MOHO) can retain C in the form of crystalline carbonates past subarc depths and deliver C deeper into the mantle. If ophicarbonates formed in the mantle wedge become mechanically coupled with the subducting slab\, then C can be completely released in the hottest subduction zones in the form of CO2-rich melts\, while ophicarbonates in cooler subduction zones may retain some C. In agreement with previous modeling studies3\, the present experimental study suggests that ophicarbonates dehydrate and deliver H2O to arc magma source regions and retain some amount of C in all but the hottest subduction zones\, highlighting the importance of these lithologies in delivering C past subarc depths deep into the mantle. \n1Alt\, J. C. et al. Lithos (2013) \n2Sieber\, M. J. et al. EPSL (201) \n3Kerrick\, D. M.\, & Connolly\, J. A. D. Geology (1998) URL:https://cleverplanets.org/event/talk-by-james-eguchi-at-agu-fall-meeting/ CATEGORIES:Conference END:VEVENT BEGIN:VEVENT DTSTART;TZID=America/Chicago:20191209T114500 DTEND;TZID=America/Chicago:20191209T235000 DTSTAMP:20260423T161057 CREATED:20191209T130358Z LAST-MODIFIED:20191209T130358Z UID:2115-1575891900-1575935400@cleverplanets.org SUMMARY:Talk by Rajdeep Dasgupta at AGU Fall Meeting DESCRIPTION:In San Francisco. \nAbstract: \nLife-essential volatile elements such as carbon (C)\, hydrogen (H)\, and nitrogen (N) are all quite depleted in the inner Solar System rocky bodies such as Earth. Yet these ingredients are sufficiently abundant on the Earth’s surface that life could be sustained for billions of years in our planet. Is there anything unique about of Earth’s formation and early differentiation that led to acquisition of the life-essential volatile elements? The budgets of these major volatile elements are poorly known for other rocky planets; however\, do we expect the absolute and relative abundances of these ingredients for life to be similar across all Solar System planets? Here we will discuss some of the processes of planet formation and differentiation such as core formation\, magma ocean-atmosphere interaction that can fractionate the life-essential volatiles differently depending on the styles and timescales of planetary accretion and differentiation. We will emphasize how understanding the formation of habitable worlds would require bringing together constraints from many disciplines such as observational astronomy\, astrophysics\, geo- and cosmochemistry\, Earth history\, and geophysics. URL:https://cleverplanets.org/event/talk-by-rajdeep-dasgupta-at-agu-fall-meeting/ END:VEVENT BEGIN:VEVENT DTSTART;TZID=America/Chicago:20191209T082500 DTEND;TZID=America/Chicago:20191209T083000 DTSTAMP:20260423T161057 CREATED:20191209T131559Z LAST-MODIFIED:20191209T132313Z UID:2122-1575879900-1575880200@cleverplanets.org SUMMARY:Talk by Sarah Stewart at AGU 2019 DESCRIPTION:San Francisco. \n“Expect more surprises during planet formation” \nAbstract: \nPlanet assembly drives materials into pressure-temperature regimes far beyond the current states of planetary objects in our solar system. As a result\, planet formation produces unfamiliar phenomena\, such impact-generated vapor bubbles in the solar nebula and fast-spinning synestias. These newly recognized phenomena lead to fresh views on how to use geochemical observations to reconstruct planet formation. URL:https://cleverplanets.org/event/talk-by-sarah-stewart-at-agu-2019/ CATEGORIES:Conference END:VEVENT BEGIN:VEVENT DTSTART;TZID=America/Chicago:20191209T080000 DTEND;TZID=America/Chicago:20191213T170000 DTSTAMP:20260423T161057 CREATED:20190911T182018Z LAST-MODIFIED:20190911T182043Z UID:2050-1575878400-1576256400@cleverplanets.org SUMMARY:2019 AGU Fall Meeting DESCRIPTION:San Francisco\, CA URL:https://cleverplanets.org/event/agu-fall-meeting/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20190818 DTEND;VALUE=DATE:20190824 DTSTAMP:20260423T161057 CREATED:20190619T220421Z LAST-MODIFIED:20190619T220421Z UID:1934-1566086400-1566604799@cleverplanets.org SUMMARY:Rajdeep Dasgupta and students presenting at Goldschmidt Conference DESCRIPTION:Conference held in Barcelona\, Spain. \nAbstracts: \nAssociation of Large Oxidation Events and Carbon Isotope Excursions – Increased CO2 Drawdown and Deep Recycling of Organic Carbon\n– Eguchi J\, Seales J & Rajdeep D (2019) Goldschmidt Abstracts\, 2019 \nControl of Accretion and Early Differentiation Process on the Diversity of Volatile Inventory of Rocky Solar System Objects\n– Dasgupta R\, Grewal DS & Tsuno K (2019) Goldschmidt Abstracts\, 2019 \nThe Core-Mantle Partitioning of Nitrogen in Carbon-Undersaturated Ultramafic Systems\n– Grewal D\, Hough T\, Tsuno K & Dasgupta R (2019) Goldschmidt Abstracts\, 2019 URL:https://cleverplanets.org/event/rajdeep-dasgupta-and-students-presenting-at-goldschmidt-conference/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20190715 DTEND;VALUE=DATE:20190720 DTSTAMP:20260423T161057 CREATED:20190208T154256Z LAST-MODIFIED:20190208T154438Z UID:1637-1563148800-1563580799@cleverplanets.org SUMMARY:2019 Sagan Exoplanet Summer Workshop - Astrobiology for Astronomers DESCRIPTION:2019 Sagan Exoplanet Summer Workshop – Astrobiology for Astronomers\nHOSTED BY THE NASA EXOPLANET SCIENCE INSTITUTE\, HAMEETMAN AUDITORIUM\, CAHILL BUILDING\, CALIFORNIA INSTITUTE OF TECHNOLOGY\, PASADENA\, CA\nSubmit talks/posters – May 9- June 28\nFREE to register – deadline May 16 URL:https://cleverplanets.org/event/2019-sagan-exoplanet-workshop/ CATEGORIES:Conference ATTACH;FMTTYPE=image/jpeg:https://cleverplanets.org/wp-content/uploads/2019/02/exo.jpg END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20190624 DTEND;VALUE=DATE:20190629 DTSTAMP:20260423T161057 CREATED:20190619T215752Z LAST-MODIFIED:20190619T215752Z UID:1932-1561334400-1561766399@cleverplanets.org SUMMARY:Rajdeep Dasgupta and students presenting at the Astrobiology Science Conference DESCRIPTION:Conference held in Seattle\, Washington. URL:https://cleverplanets.org/event/rajdeep-dasgupta-and-students-presenting-at-the-astrobiology-science-conference/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20190623 DTEND;VALUE=DATE:20190629 DTSTAMP:20260423T161057 CREATED:20190208T154733Z LAST-MODIFIED:20190208T154812Z UID:1640-1561248000-1561766399@cleverplanets.org SUMMARY:2019 Gordon Research Conference - Origins of Solar Systems DESCRIPTION:Meteoritical\, Spacecraft and Astrophysical Perspectives on the Assembly and Composition of Planets\nHosted at Mount Holyoke College\, 50 College Street\, South Hadley\, MA\, US \nThe Gordon Research Conference on Origins of Solar Systems brings together a diverse group of scientists to discuss research at the frontier of understanding how planets and planetary systems form. Invited speakers from the fields of astronomy\, astrophysics\, cosmochemistry\, and planetary science will present their latest findings. A particular focus at this meeting will be the latest results from the Hayabusa2\, Osiris-Rex\, and New Horizons missions to primitive solar system bodies\, exoplanet results from the TESS space telescope\, and results from ground-based astronomical facilities like the Atacama Large Millimeter Array.\nApplication deadline – May 26\, 2019 URL:https://cleverplanets.org/event/2019-gordon-origins-solar-systems/ CATEGORIES:Conference ATTACH;FMTTYPE=image/png:https://cleverplanets.org/wp-content/uploads/2019/02/grc_logo.png END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20190611 DTEND;VALUE=DATE:20190612 DTSTAMP:20260423T161057 CREATED:20190611T172222Z LAST-MODIFIED:20190611T172335Z UID:1885-1560211200-1560297599@cleverplanets.org SUMMARY:Christopher Johns-Krull presenting talk at the American Astronomical Society DESCRIPTION:Conference held in St. Louis\, Missouri. \nPresentation citation: \nJohns-Krull\, C.M.\, Flagg\, L.\, Nofi\, L.\, Llama\, J.\, Prato\, L.\, Sullivan\, K.\, Jaffe\, D.T.\, & Mace\, G. 2019 “Direct Detection of CO in CI Tau b: Support for Hot Start Formation”. URL:https://cleverplanets.org/event/christopher-johns-krull-presenting-talk-at-the-american-astronomical-society/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20190610 DTEND;VALUE=DATE:20190615 DTSTAMP:20260423T161057 CREATED:20190614T160439Z LAST-MODIFIED:20190614T160551Z UID:1900-1560124800-1560556799@cleverplanets.org SUMMARY:Christopher Johns-Krull & students attending the American Astronomical Society conference DESCRIPTION:This is the 234th meeting of the conference. They are meeting in St. Louis. \nJohns-Krull and his students are presenting the following posters and talks: \nPoster 105.04\nTitle: Direct Detection of CO in CI Tau b: Support for Hot Start Formation\nAuthors: Christopher M. Johns-Krull; Laura Flagg; Larissa Nofi; Joe\nLlama; Lisa A. Prato; Kendall Sullivan; Daniel T. Jaffe; Gregory N. Mace \nPoster 201.06\nTitle: Radial Velocity Monitoring of the Young Star Hubble 4\nAuthors: Adolfo Carvalho; Christopher M. Johns-Krull; Lisa A. Prato \nTalk 221.04\nTitle: Direct Detection of CO in CI Tau b: Support for Hot Start Formation\nAuthors: Christopher M. Johns-Krull; Laura Flagg; Larissa Nofi; Joe\nLlama; Lisa A. Prato; Kendall Sullivan; Daniel T. Jaffe; Gregory N. Mace URL:https://cleverplanets.org/event/christopher-johns-krull-students-attending-the-american-astronomical-society/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20190610 DTEND;VALUE=DATE:20190611 DTSTAMP:20260423T161057 CREATED:20190611T172529Z LAST-MODIFIED:20190611T172529Z UID:1887-1560124800-1560211199@cleverplanets.org SUMMARY:Christopher Johns-Krull presenting poster at American Astronomical Society DESCRIPTION:Conference held in St. Louis\, Missouri. \nPresentation citation: \nCarvalho\, A.\, Johns-Krull\, C.M.\, & Prato\, L. 2019 “Radial Velocity Monitoring of the Young Star Hubble 4”. URL:https://cleverplanets.org/event/christopher-johns-krull-presenting-poster-at-american-astronomical-society/ END:VEVENT BEGIN:VEVENT DTSTART;TZID=America/Chicago:20190513T080000 DTEND;TZID=America/Chicago:20190517T170000 DTSTAMP:20260423T161057 CREATED:20190611T171858Z LAST-MODIFIED:20190611T171944Z UID:1882-1557734400-1558112400@cleverplanets.org SUMMARY:Grad student Erik Weaver presented a poster at the "New Horizons in Planetary Systems" conference DESCRIPTION:This conference took place in Victoria\, British Columbia\, Canada. \nLink to conference site. URL:https://cleverplanets.org/event/grad-student-erik-weaver-presented-a-poster-at-the-new-horizons-in-planetary-systems-conference/ END:VEVENT BEGIN:VEVENT DTSTART;TZID=America/Chicago:20190322T080000 DTEND;TZID=America/Chicago:20190322T170000 DTSTAMP:20260423T161057 CREATED:20190611T171606Z LAST-MODIFIED:20190611T171606Z UID:1880-1553241600-1553274000@cleverplanets.org SUMMARY:Isella presented a talk at the 50th Lunar and Planetary Science Conference DESCRIPTION:This conference was held in Woodlands\, Texas. URL:https://cleverplanets.org/event/isella-presented-a-talk-at-the-50th-lunar-and-planetary-science-conference/ END:VEVENT BEGIN:VEVENT DTSTART;VALUE=DATE:20190318 DTEND;VALUE=DATE:20190323 DTSTAMP:20260423T161057 CREATED:20180824T145209Z LAST-MODIFIED:20190129T145259Z UID:999-1552867200-1553299199@cleverplanets.org SUMMARY:LPSC DESCRIPTION:50th annual Lunar and Planetary Science Conference\, bringing together “international specialists in petrology\, geochemistry\, geophysics\, geology\, and astronomy to present the latest results of research in planetary science\,” Houston\, TX \nAbstract deadline – January 9\, 2019\nProgram available – February 1\, 2019 \n  URL:https://cleverplanets.org/event/lpsc/ CATEGORIES:Conference ATTACH;FMTTYPE=image/png:https://cleverplanets.org/wp-content/uploads/2018/08/LPSC2019home-graphic.png END:VEVENT BEGIN:VEVENT DTSTART;TZID=America/Chicago:20190123T080000 DTEND;TZID=America/Chicago:20190125T170000 DTSTAMP:20260423T161057 CREATED:20181206T162051Z LAST-MODIFIED:20181206T174642Z UID:1548-1548230400-1548435600@cleverplanets.org SUMMARY:Math + X Symposium DESCRIPTION:Math + X Symposium on Inverse Problems and Deep Learning in Space Exploration\, “funded by the Simons Foundation under the MATH + X program and will bring together planetary scientists\, astrophysicists\, cosmologists\, mathematicians\, computer scientists and statisticians to present the state of the art on the one hand and emerging cross disciplinary directions of research on the other hand\, while enabling new collaborations\,” Rice University Biomedical Research Collaborative Building\, Houston\, TX \nRegistration is free. \nProgram: Program for Math+XSymposium URL:https://cleverplanets.org/event/math-x-symposium/ ATTACH;FMTTYPE=image/jpeg:https://cleverplanets.org/wp-content/uploads/2018/12/mathxsymposium_rice.jpg END:VEVENT BEGIN:VEVENT DTSTART;TZID=America/Chicago:20190115T080000 DTEND;TZID=America/Chicago:20190116T120000 DTSTAMP:20260423T161057 CREATED:20190112T000832Z LAST-MODIFIED:20190112T001721Z UID:1572-1547539200-1547640000@cleverplanets.org SUMMARY:Kick-Off Meeting DESCRIPTION:The first meeting of CLEVER Planets attendees is happening January 14-15th\, 2019\, at Rice University in Houston\, TX. At this Kick-Off Meeting\, co-investigators\, collaborators and their postdoctoral scholars and students will convene to share their research and discuss goals and collaborations for the project over the next few years. \nSee the itinerary and list of attendees here:\nCLEVERPlanets_Kick-OffMeeting_Schedule URL:https://cleverplanets.org/event/kick-off-meeting/ CATEGORIES:CLEVERPlanet Event,Conference,Meeting END:VEVENT END:VCALENDAR