{"id":29,"date":"2019-01-24T11:52:20","date_gmt":"2019-01-24T10:52:20","guid":{"rendered":"https:\/\/www.oa-roma.inaf.it\/nest\/?page_id=29"},"modified":"2019-04-18T12:10:27","modified_gmt":"2019-04-18T10:10:27","slug":"nest-science-goals","status":"publish","type":"page","link":"https:\/\/www.oa-roma.inaf.it\/nest\/nest-science-goals\/","title":{"rendered":"NEST Science Goals"},"content":{"rendered":"\n<p style=\"text-align:center\" class=\"has-medium-font-size\">Science goals and objectives of the NEST mission<\/p>\n\n\n\n<p class=\"has-medium-font-size\">The NEST mission will explore the near-Earth space and rendez-vous with <strong>several Near-Earth Asteroids<\/strong>, including the <strong>Potentially Hazardous Asteroid Apophis<\/strong>.<\/p>\n\n\n\n<p><\/p>\n\n\n\n<p>NEST is a mature, flexible, modular mission concept, being designed for a launch with ESA ARIEL Spacecraft in 2028, and a delivery in the Sun-Earth Lagrance Point L2, from which it will start its journet in the near-Earth environment. NEST aims at rendez-vous with multiple near-Earth asteroids, presenting a variety of physical properties. In the baseline scenario, we consider 2 NEAs to be visited with mission duration of less than 5 years.<\/p>\n\n\n\n<p>Our first target will be the 370-m Potential Hazardous Asteroid (99942) Apophis, which will have in 2029 a very close approach with the Earth (&lt; 40000 km). Multiple impact solution exist durig the course of the next century. Obtaining a detailed, in-situ physical characterisation of this body is of paramount importance fro being able to make precise predictions of future trajectory of Apophis.<\/p>\n\n\n\n<p>For the second mission target, presently we identified 36 promising NEA small (&lt; 100 m) targets and hundreds of preliminary 2- (or 3-, for a possible extened mission) asteroid sequences for the time window 2028-2032. We can easily adapt our mission scenario to varying constraints in terms of, e.g., launch date, propulsion specifics, mission architecture and duration.<\/p>\n\n\n\n<p>Our mission can be broken down into several complementary modules:<\/p>\n\n\n\n<p>i) <strong>Radar investigation of asteroid interiors<\/strong>; for the first time ever, the radar technique will be used to <em>in-situ<\/em> characterise asteroid interiors, in different size regimes. Information on composition, porosity, and their spatial variation will be obtained.<\/p>\n\n\n\n<p>ii) <strong>Complementary in-situ scientific investigation, using also a smallsat for Apophis investigation<\/strong>; a mothercraft\/daughtercraft mission architecture will allow to perform both remote and in-situ investigation with a number of scientific instruments. The mothercraft will release a smallsat (daughtercraft) at Apophis, and will operate in proximity of each target for few months, allowing a complete characterisation of surface, subsurface and interior properties of Apophis and of the selected target(s).<\/p>\n\n\n\n<p>NEST mission architecture relies on significant payload heritage and high-TRL available technology, based on our established Italian-German-French-Swiss consortium, with important contribution from Poland. However, we will consider possible complementary contributions from further ESA member states and partners willingly.<br><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Science goals and objectives of the NEST mission The NEST mission will explore the near-Earth space and rendez-vous with several Near-Earth Asteroids, including the Potentially Hazardous Asteroid Apophis. NEST is a mature, flexible, modular mission concept, being designed for a &hellip; <a href=\"https:\/\/www.oa-roma.inaf.it\/nest\/nest-science-goals\/\">Continua a leggere<span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":147,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_acf_changed":false,"footnotes":""},"class_list":["post-29","page","type-page","status-publish","hentry"],"acf":[],"_links":{"self":[{"href":"https:\/\/www.oa-roma.inaf.it\/nest\/wp-json\/wp\/v2\/pages\/29","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.oa-roma.inaf.it\/nest\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.oa-roma.inaf.it\/nest\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.oa-roma.inaf.it\/nest\/wp-json\/wp\/v2\/users\/147"}],"replies":[{"embeddable":true,"href":"https:\/\/www.oa-roma.inaf.it\/nest\/wp-json\/wp\/v2\/comments?post=29"}],"version-history":[{"count":8,"href":"https:\/\/www.oa-roma.inaf.it\/nest\/wp-json\/wp\/v2\/pages\/29\/revisions"}],"predecessor-version":[{"id":95,"href":"https:\/\/www.oa-roma.inaf.it\/nest\/wp-json\/wp\/v2\/pages\/29\/revisions\/95"}],"wp:attachment":[{"href":"https:\/\/www.oa-roma.inaf.it\/nest\/wp-json\/wp\/v2\/media?parent=29"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}