首页> 外文学位 >Paleolakes and the crustal dichotomy boundary on Mars.
【24h】

Paleolakes and the crustal dichotomy boundary on Mars.

机译:火星上的古湖和地壳二分法边界。

获取原文
获取原文并翻译 | 示例

摘要

Because of its implications for habitability, understanding the longevity and role of standing water in Martian geomorphology is the primary focus of the U.S. and European Mars exploration programs. This dissertation addresses four related issues: (1) the relevance of particular landform assemblages to the occurrence of Martian paleolakes; the age, longevity, and maturity of these landforms; and their implications for paleoclimate; (2) the development of a large mid-latitude paleolake in the southern highlands, which appears to have overflowed catastrophically to carve Ma'adim Vallis; (3) the origin and development of fretted terrain along the highland/lowland boundary, which some investigators have suggested may include shorelines; and (4) the hydrology of Martian watersheds that supplied the enclosed basins. Most known putative deltas record a relatively brief period of aggradation without subsequent erosion controlled by a lower base level. Most of these deposits occur at the ends of V-shaped, entrenched lower reaches of valley networks, and some late-stage basin overflows are evident. These observations suggest a late episode of valley network incision that was intense but short-lived relative to the more general Noachian landscape degradation. Ma'adim Vallis, one of the largest valleys in the Martian highlands, appears to have originated somewhat earlier by catastrophic overflow of a large paleolake located south of the valley heads. Support for the paleolake overflow hypothesis comes from the morphology and morphometry of the valley, its tributaries, and the contributing Eridania basin to the south. At Aeolis Mensae along the dichotomy boundary, we show that fretted terrain formed exclusively in a >2 km thick, late Noachian (∼3.7 Ga) sedimentary deposit that overlies the base of an older cratered slope. New orbital imaging reveals 21 late-stage channels within valley networks, which we use to estimate formative discharges and to evaluate water supply mechanisms. We find that channel width and associated formative discharge are comparable to terrestrial valley networks of similar area and relief. In four large valleys with few tributaries, wider channels may represent large subsurface outflows or paleolake overflows, as these four channels originate at breached basin divides and/or near source regions for the catastrophic outflow channels.
机译:由于其对可居住性的影响,因此了解死水的寿命和在火星地貌中的作用是美国和欧洲火星勘探计划的主要重点。本文研究了四个相关问题:(1)特定地貌组合与火星古湖发生的相关性;这些地貌的年龄,寿命和成熟度;及其对古气候的影响; (2)在南部高地发展了一个大型的中纬度古湖,似乎已经灾难性地淹没了Ma'adim Vallis; (3)沿高地/低地边界的微动地形的起源和发展,一些调查人员认为这可能包括海岸线; (4)为封闭盆地提供火星流域的水文。最著名的推定三角洲记录了相对短暂的凝结期,而随后的侵蚀却没有受到较低的碱水平的控制。这些沉积物大多数发生在V型,根深蒂固的山谷网络的末端,并且明显存在后期盆地溢流。这些观察结果表明,与较一般的Noachian景观退化相比,山谷网络切口的后期事件强度大但寿命短。马阿迪姆·瓦利斯(Ma'adim Vallis)是火星高原上最大的山谷之一,似乎早些时候起源于位于山谷首部以南的大型古冰川的灾难性溢出。对古湖溢流假说的支持来自于山谷,其支流和南部贡献的伊里达尼亚盆地的形态和形态。在沿二分法边界的风神Mensae处,我们发现,碎裂的地形仅在厚度大于2 km的晚Noachian(约3.7 Ga)沉积沉积物上形成,该沉积物覆盖了较老的火山口斜坡的底部。新的轨道成像揭示了山谷网络内的21个后期通道,我们用它们来估算形成性流量并评估供水机制。我们发现,河道宽度和相关的形成放电可与具有相似面积和起伏的陆地谷底网络相媲美。在四个支流很少的大山谷中,较宽的河道可能代表着较大的地下流出物或古湖溢流,因为这四个河道起源于破坏性的盆地分界和/或灾难性流出道的源区附近。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号