LEADER 03292nam 2200613Ia 450 001 9910820545703321 005 20240516150112.0 010 $a1-283-85708-1 010 $a3-11-028640-8 024 7 $a10.1515/9783110286403 035 $a(CKB)2670000000309331 035 $a(EBL)893725 035 $a(OCoLC)821198762 035 $a(SSID)ssj0000783913 035 $a(PQKBManifestationID)11437543 035 $a(PQKBTitleCode)TC0000783913 035 $a(PQKBWorkID)10761767 035 $a(PQKB)11288869 035 $a(MiAaPQ)EBC893725 035 $a(DE-B1597)176508 035 $a(OCoLC)828060178 035 $a(DE-B1597)9783110286403 035 $a(Au-PeEL)EBL893725 035 $a(CaPaEBR)ebr10634481 035 $a(CaONFJC)MIL416958 035 $a(EXLCZ)992670000000309331 100 $a20120615d2012 uy 0 101 0 $aeng 135 $aur|nu---|u||u 181 $ctxt 182 $cc 183 $acr 200 10$aOrigin of the moon $enew concept, geochemistry, and dynamics /$fby Erik M. Galimov and Anton M. Krivtsov 205 $a1st ed. 210 $aBerlin ;$aBoston $cDe Gruyter$dc2012 215 $a1 online resource (180 p.) 300 $aDescription based upon print version of record. 311 $a3-11-028628-9 320 $aIncludes bibliographical references (p. [145]-162) and index. 327 $tFront matter --$tContents --$tIntroduction --$tPart I. Geochemistry --$tChapter 1. The Moon as a celestial body --$tChapter 2. The history of the study of the Moon --$tChapter 3. The Moon as a geological body --$tChapter 4. Similarity and difference in composition of Earth and Moon --$tChapter 5. Hypotheses on the origin of the Moon --$tChapter 6. The model of evaporative accretion --$tChapter 7. Geochemical constraints and how the giant impact and evaporative accretion concepts satisfy them --$tPart II. Dynamics --$tChapter 8. Dynamical modeling of fragmentation of the gas-dust cloud --$tChapter 9. Dynamic modeling of accretion --$tConclusions --$tReferences --$tIndex 330 $aThe origin of the Moon remains an unsolved problem of the planetary science. Researchers engaged in celestial dynamics, geophysics, and geochemistry are still discussing various models of creation of our closest cosmic neighbour. The most popular scenario, the impact hypothesis involving a collision early in the Earth's history, has been substantially challenged by the new data. The birth and development of a planet-moon system always plays a role in the formation of an entire planetary system around our Sun or around another star. This way, the story of our Moon acquires broader ramifications for one of the hottest topics of the modern scholarship. All this has motivated the authors of this book to consider a new concept and to compare the currently discussed theories, analyzing their advantages and shortcomings in explaining the experimental data. 606 $aLunar geology 607 $aMoon$xOrigin 615 0$aLunar geology. 676 $a523.3 700 $aGalimov$b Erik M$01617845 701 $aKrivtsov$b Anton M$01617846 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910820545703321 996 $aOrigin of the moon$93949228 997 $aUNINA