| LDR | | 01969nmm uu200445 4500 |
| 001 | | 000000332085 |
| 005 | | 20240805170007 |
| 008 | | 181129s2018 |||||||||||||||||c||eng d |
| 020 | |
▼a 9780438169715 |
| 035 | |
▼a (MiAaPQ)AAI10829577 |
| 035 | |
▼a (MiAaPQ)arizona:16433 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 248032 |
| 082 | 0 |
▼a 523 |
| 100 | 1 |
▼a Landis, Margaret E. |
| 245 | 10 |
▼a Icy Craters on Mars and Ceres. |
| 260 | |
▼a [S.l.] :
▼b The University of Arizona.,
▼c 2018 |
| 260 | 1 |
▼a Ann Arbor :
▼b ProQuest Dissertations & Theses,
▼c 2018 |
| 300 | |
▼a 133 p. |
| 500 | |
▼a Source: Dissertation Abstracts International, Volume: 79-12(E), Section: B. |
| 500 | |
▼a Adviser: Shane Byrne. |
| 502 | 1 |
▼a Thesis (Ph.D.)--The University of Arizona, 2018. |
| 520 | |
▼a The broad topic of my PhD dissertation is: Where and when do volatile compounds exist on the surface of planets? My two areas of focus are Mars and Ceres. |
| 520 | |
▼a For Mars, I study the Polar Layered Deposits (PLDs), which contain a stratigraphy that may contain a record of Mars climate history. In my thesis, I use crater statistics based on High Resolution Imaging Science Experiment (HiRISE) images to mea |
| 520 | |
▼a For Ceres, I model water ice sublimation as a source of the transient exosphere. The transient water vapor exosphere is not unexpected due to the high water content of Ceres determined from geophysical modeling, but the source is still unknown. |
| 590 | |
▼a School code: 0009. |
| 650 | 4 |
▼a Planetology. |
| 650 | 4 |
▼a Geomorphology. |
| 650 | 4 |
▼a Astrophysics. |
| 690 | |
▼a 0590 |
| 690 | |
▼a 0484 |
| 690 | |
▼a 0596 |
| 710 | 20 |
▼a The University of Arizona.
▼b Planetary Sciences. |
| 773 | 0 |
▼t Dissertation Abstracts International
▼g 79-12B(E). |
| 773 | |
▼t Dissertation Abstract International |
| 790 | |
▼a 0009 |
| 791 | |
▼a Ph.D. |
| 792 | |
▼a 2018 |
| 793 | |
▼a English |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14999323
▼n KERIS |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a 관리자 |