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DTSTART;TZID=Europe/Rome:20180306T114500
DTEND;TZID=Europe/Rome:20180306T124500
DTSTAMP:20260430T171325
CREATED:20171016T082612Z
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UID:3643-1520336700-1520340300@www.oa-roma.inaf.it
SUMMARY:An experiment in Astrobiology: exploring the climate parameter space of rocky planets
DESCRIPTION:Astrobiology is a relatively new and fast-growing science\, whose main\ncharacteristic is to need expertises from different science fields.\nI’ll show how the climate of a planet influences its abitability.\nAstronomers from OATs\, climatologists from CNR and experts in\ndatabases from OATs joined their efforts to build a fast\, simplified\,\nyet effective climate model and database for extra-solar planets. I\nwill describe\nthe model\, its main feature\, its validation\, its application to a\nspecific exo-planet (Kepler 452b). I will then show how such a model\ncan be used to explore a huge parameter space and build a database\nthat can be used to characterize classes of habitable planets. I will\npoint out how this particular case is an good example of\nHigh-Throughput  Computing (HTC). Our database can also be used\, e.g.\,\nas a tool to get a first estimate of the habitability of a newly\ndiscovered rocky planet.\nThen I will describe possible future developements of such a research\nline\, including the study of the effect of the biosphere itself on the\nhabitability.
URL:https://www.oa-roma.inaf.it/event/seminar-by-giuseppe-murante/
LOCATION:Aula Gratton
CATEGORIES:Seminari
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DTSTART;TZID=Europe/Rome:20180306T114500
DTEND;TZID=Europe/Rome:20180306T124500
DTSTAMP:20260430T171325
CREATED:20171016T082612Z
LAST-MODIFIED:20171016T082612Z
UID:4735-1520336700-1520340300@www.oa-roma.inaf.it
SUMMARY:An experiment in Astrobiology: exploring the climate parameter space of rocky planets
DESCRIPTION:Astrobiology is a relatively new and fast-growing science\, whose main\ncharacteristic is to need expertises from different science fields.\nI’ll show how the climate of a planet influences its abitability.\nAstronomers from OATs\, climatologists from CNR and experts in\ndatabases from OATs joined their efforts to build a fast\, simplified\,\nyet effective climate model and database for extra-solar planets. I\nwill describe\nthe model\, its main feature\, its validation\, its application to a\nspecific exo-planet (Kepler 452b). I will then show how such a model\ncan be used to explore a huge parameter space and build a database\nthat can be used to characterize classes of habitable planets. I will\npoint out how this particular case is an good example of\nHigh-Throughput  Computing (HTC). Our database can also be used\, e.g.\,\nas a tool to get a first estimate of the habitability of a newly\ndiscovered rocky planet.\nThen I will describe possible future developements of such a research\nline\, including the study of the effect of the biosphere itself on the\nhabitability.
URL:https://www.oa-roma.inaf.it/event/seminar-by-giuseppe-murante-2/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
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