{"id":7,"date":"2014-12-19T14:42:40","date_gmt":"2014-12-19T14:42:40","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/exocartoinverse\/?page_id=2"},"modified":"2014-12-19T14:42:40","modified_gmt":"2014-12-19T14:42:40","slug":"sample-page","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/exocartoinverse\/","title":{"rendered":"Executive Summary"},"content":{"rendered":"<p>Although the faces of extrasolar planets will not be spatially-resolved in the foreseeable future, their rotational and orbital motions produce detectable changes in color and brightness. <a title=\"Characterization of extrasolar terrestrial planets from diurnal photometric variability\" href=\"http:\/\/adsabs.harvard.edu\/abs\/2001Natur.412..885F\">Ford, Seager &amp; Turner (2001)<\/a> used simulations of Earth to show that the changing colors of its disk-integrated reflected light encode information about continents, oceans, and clouds. The inverse problem&#8212;inferring the surface geography of a planet based on time-resolved photometry&#8212;is much more daunting than the forward problem and at first blush looked intractable. However, cracking the &#8220;exo-cartography&#8221; inverse problem is a worthy challenge because it offers important clues about planet formation, evolution, and climate&#8212;foremost areas of research in planetary science. This is also a timely problem, because reflected light from short-period planets can now be measured, and high-contrast imaging projects are poised to extend this approach to cooler planets.<\/p>\n<p>In recent years, progress in exo-cartography has been made by taking on small parts of the problem in isolation. Members of our team have demonstrated how disk-integrated reflected light curves can be analyzed to obtain a planet&#8217;s rotation rate, spin-orientation, surface geography, cloud distribution, and spectra of surfaces. These successes have led exo-cartography to be a primary science driver of next-generation direct-imaging missions <a title=\"Looking for a Mirror\" href=\"http:\/\/www.nytimes.com\/2014\/02\/17\/opinion\/looking-for-a-mirror.html\">(<em>NY Times<\/em>, 17\/02\/2014)<\/a>. But the full inverse problem is more challenging than the sum of its parts and that is what our ISSI International Team proposes to tackle.<\/p>\n<p>Our team will take a huge step forward by combining the major advances of the last decade. We will 1) construct a suite of full-physics simulated reflected lightcurves of exoplanets using the Virtual Planetary Laboratory&#8217;s Earth model, and 2) attempt to infer the planetary properties in a blind fashion by analyzing these lightcurves with a variety of inverse methods including a Markov Chain Monte Carlo. We will also set intermediate &#8220;data challenges&#8221; to better understand which assumptions are most critical to the retrieval exercise. The results of our collaboration will be published in one or more peer-reviewed papers, and our lightcurves and inverse models will be made publicly available to serve as a benchmark for future efforts.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Although the faces of extrasolar planets will not be spatially-resolved in the foreseeable future, their rotational and orbital motions produce detectable changes in color and brightness. Ford, Seager &amp; Turner (2001) used simulations of Earth to show that the changing &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/exocartoinverse\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-7","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/exocartoinverse\/wp-json\/wp\/v2\/pages\/7","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/exocartoinverse\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/exocartoinverse\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/exocartoinverse\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/exocartoinverse\/wp-json\/wp\/v2\/comments?post=7"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/exocartoinverse\/wp-json\/wp\/v2\/pages\/7\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/exocartoinverse\/wp-json\/wp\/v2\/media?parent=7"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}