000762688 000__ 03106cam\a2200481Ii\4500
000762688 001__ 762688
000762688 005__ 20230306142234.0
000762688 006__ m\\\\\o\\d\\\\\\\\
000762688 007__ cr\cn\nnnunnun
000762688 008__ 150304s2015\\\\nyua\\\\ob\\\\000\0\eng\d
000762688 019__ $$a906182926
000762688 020__ $$a9781493922444$$q(electronic book)
000762688 020__ $$a1493922440$$q(electronic book)
000762688 020__ $$z9781493922437
000762688 0247_ $$a10.1007/978-1-4939-2244-4$$2doi
000762688 035__ $$aSP(OCoLC)ocn904338863
000762688 035__ $$aSP(OCoLC)904338863$$z(OCoLC)906182926
000762688 040__ $$aN$T$$beng$$erda$$epn$$cN$T$$dGW5XE$$dN$T$$dIDEBK$$dCDX$$dUPM$$dCOO$$dE7B$$dEBLCP$$dYDXCP$$dS3O$$dOCLCF$$dOCLCQ$$dIAO$$dIAS$$dJBG$$dIAD
000762688 043__ $$azme----
000762688 049__ $$aISEA
000762688 050_4 $$aQB611
000762688 08204 $$a523.41$$223
000762688 1001_ $$aClark, Pamela Elizabeth,$$eauthor.
000762688 24510 $$aMercury's interior, surface, and surrounding environment :$$blatest discoveries /$$cPamela Elizabeth Clark.
000762688 264_1 $$aNew York, NY :$$bSpringer,$$c2015.
000762688 300__ $$a1 online resource (viii, 97 pages) :$$billustrations.
000762688 336__ $$atext$$btxt$$2rdacontent
000762688 337__ $$acomputer$$bc$$2rdamedia
000762688 338__ $$aonline resource$$bcr$$2rdacarrier
000762688 4901_ $$aSpringerBriefs in astronomy,$$x2191-9100
000762688 504__ $$aIncludes bibliographical references.
000762688 5050_ $$aMessenger Mission -- Planetary Formation -- Terrestrial Planet Surface Processes -- Exosphere Dynamic -- Magnetosphere Dynamics -- Data Release Schedule Index.
000762688 506__ $$aAccess limited to authorized users.
000762688 520__ $$aThis SpringerBrief details the MESSENGER Mission, the findings of which present challenges to widely held conventional views and remaining mysteries surrounding the planet. The work answers the question of why Mercury is so dense, and the implications from geochemical data on its planetary formation. It summarizes imaging and compositional data from the terrestrial planet surface processes and explains the geologic history of Mercury. It also discusses the lack of southern hemisphere coverage. Our understanding of the planet Mercury has been in a transitional phase over the decades since Mariner 10. The influx of new data from the NASA MESSENGER Mission since it was inserted into the orbit of Mercury in March of 2011 has greatly accelerated that shift. The combined compositional data of relatively high volatiles (S, K), relatively low refractories (Al, Ca), and low crustal iron, combined with an active, partially molten iron rich core, has major implications for Mercury and Solar System formation. From a scientist at NASA Goddard Space Flight Center, this presents a comprehensive overview of the discoveries from the ten-year MESSENGER mission.
000762688 588__ $$aOnline resource; title from PDF title page (SpringerLink, viewed March 11, 2015).
000762688 651_0 $$aMercury (Planet)$$xGeology.
000762688 651_0 $$aMercury (Planet)$$xSurface.
000762688 77608 $$iPrint version:$$z9781493922437
000762688 830_0 $$aSpringerBriefs in astronomy.
000762688 852__ $$bebk
000762688 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-1-4939-2244-4$$zOnline Access$$91397441.1
000762688 909CO $$ooai:library.usi.edu:762688$$pGLOBAL_SET
000762688 980__ $$aEBOOK
000762688 980__ $$aBIB
000762688 982__ $$aEbook
000762688 983__ $$aOnline
000762688 994__ $$a92$$bISE