| LDR | | 00000nmm u2200205 4500 |
| 001 | | 000000332284 |
| 005 | | 20241127172322 |
| 008 | | 181129s2018 ||| | | | eng d |
| 020 | |
▼a 9780438025943 |
| 035 | |
▼a (MiAaPQ)AAI10751743 |
| 035 | |
▼a (MiAaPQ)cornellgrad:10749 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 248032 |
| 049 | 1 |
▼f DP |
| 082 | 0 |
▼a 551.4 |
| 100 | 1 |
▼a Birch, Samuel Patrick Dennis.
▼0 (orcid)0000-0002-4578-1694 |
| 245 | 10 |
▼a Morphology and Landscape Evolution of Icy Worlds. |
| 260 | |
▼a [S.l.] :
▼b Cornell University.,
▼c 2018 |
| 260 | 1 |
▼a Ann Arbor :
▼b ProQuest Dissertations & Theses,
▼c 2018 |
| 300 | |
▼a 226 p. |
| 500 | |
▼a Source: Dissertation Abstracts International, Volume: 79-10(E), Section: B. |
| 500 | |
▼a Adviser: Alexander G. Hayes. |
| 502 | 1 |
▼a Thesis (Ph.D.)--Cornell University, 2018. |
| 520 | |
▼a The outer solar system contains dynamic worlds with active sedimentary cycles that govern their overall appearances. Two of these in particular, Titan and Comet 67P/Churyumov-Gerasimenko (67P), though vastly different in terms of size, thermal h |
| 520 | |
▼a 67P, though <4-km in size, is another geologically-active world where sublimation erosion drives a complex sedimentary cycle. After entering the inner solar system, where sublimation of water ice is possible, large gradients in thermal insolatio |
| 590 | |
▼a School code: 0058. |
| 650 | 4 |
▼a Geomorphology. |
| 650 | 4 |
▼a Astronomy. |
| 650 | 4 |
▼a Planetology. |
| 690 | |
▼a 0484 |
| 690 | |
▼a 0606 |
| 690 | |
▼a 0590 |
| 710 | 20 |
▼a Cornell University.
▼b Geological Sciences. |
| 773 | 0 |
▼t Dissertation Abstracts International
▼g 79-10B(E). |
| 773 | |
▼t Dissertation Abstract International |
| 790 | |
▼a 0058 |
| 791 | |
▼a Ph.D. |
| 792 | |
▼a 2018 |
| 793 | |
▼a English |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14997190
▼n KERIS |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a 관리자
▼b 관리자 |