Chondrules and the Protoplanetary DiskCambridge University Press, 20/06/1996 - 346 من الصفحات This book is the first comprehensive review of chondrules and their origins since a consensus developed that they were made in the disk of gas and solids that formed the Sun and planets 4.5 billion years ago. Fifty scientists from assorted disciplines have collaborated to review how chondrules could have formed in the protoplanetary disk. When and where in the disk did they form? What were they made from and how fast were they heated and cooled? What provided the energy to melt chondrules--nebular shock waves, lightning discharges, protostellar jets? Following an exciting international conference in Albuquerque, New Mexico, the latest answers to these questions are presented in thirty-four articles, which will appeal to researchers in planetary science and meteoritics. |
المحتوى
MULTIPLE MELTING | 6 |
The role of chemical processes | 13 |
P Cassen | 95 |
4 | 101 |
35 | 103 |
5 | 138 |
R H Jones | 179 |
and chondrites | 315 |
Glossary | 335 |
J A Wood | 341 |
343 | |
طبعات أخرى - عرض جميع المقتطفات
عبارات ومصطلحات مألوفة
abundances accretion disk Acta aggregates Allende Arizona Press Astrophys barred olivine carbonaceous chondrites Chainpur chemical chon chondrule formation chondrule melts chondrule precursors chondrule rims Clayton clumps CM chondrites collisions components compound chondrules condensation Connolly constraints cooling rates Cosmochim crystals density drites droplets drules dust Early Solar System Earth Planet energy enstatite evaporation experimental FeO-poor FeO-rich fine-grained rims formation of chondrules formed forsterite FU Orionis Geochim Grossman heating events Hewins Icarus inclusions incomplete melting infalling isotopic composition Jones Keil Kerridge Lett liquidus Lofgren Lunar Planet MacPherson mass matrix metal meteorites Metzler microchondrules midplane minerals Nagahara nucleation observed olivine olivine chondrules ordinary chondrites oxygen isotopic parent body particles phase planetesimals porphyritic processes produced Protoplanetary Disk Protostars pyroxene ratio refractory relict grains Semarkona shock silicate solar nebula solid suggest Tauri stars thermal Thiemens tion turbulence University of Arizona velocity volatile elements Wasson J. T.