火星内部的岩水的地化学证据来自Shergotty石中的Pyroxenes
H Y McSween1, T L Grove, R C Lentz
1Department of Geological Sciences, University of Tennessee, Knoxville 37996, USA. mcsween@utk.edu
Nature
|February 24, 2001
概括
火山活动在火星上可能会给火星表面带来大量的水. 对谢尔戈蒂石的分析表明,早期的岩含有高达1.8%的水,这挑战了以前关于火星水的假设.
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
- 火山学 火山学是一门学科.
背景情况:
- 火星表面形态学表明,火星上存在着一个古老的海洋.
- 火山的排气被假设为水源,但推断的低磁性水含量与此相矛盾.
- 火星岩石上的火性石通常含水量较低.
研究的目的:
- 为了研究火山排气的潜力,为火星表面提供水.
- 为了协调有关火星排气历史的地质和地质数据.
- 为了确定火星上爆发前的岩水含量.
主要方法:
- 分析了谢尔戈蒂石的火素中的微量元素分布.
- 进行水性和无水性结晶实验.
- 比较内部核心和外部边缘构成的烯矿物质.
主要成果:
- 谢尔戈蒂石中的烟素内核与外边相比,富含可溶性微量元素.
- 这种丰富表明水存在于深处的岩中.
- 水在很大程度上在岩上升到表面的过程中丢失.
- 火星岩爆发前的含水量可能高达1.8%.
结论:
- 升起的岩石可能将大量的水送到火星表面.
- 这一发现使以前关于火星脱气的相互矛盾的约束相协调.
- 最近的火山活动可能在火星水的历史中发挥了重要作用.
相关概念视频
Conditions on Early Earth
Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
Minerals
Minerals are essential nutrients that the human body needs in small amounts to work properly. They play a vital role in many bodily functions, such as building strong bones and transmitting nerve impulses. Some minerals are needed for hormone production or to maintain a normal heartbeat. Major minerals include calcium, phosphorus, potassium, sulfur, sodium, chlorine, and magnesium, while trace minerals include iron, manganese, copper, iodine, zinc, cobalt, fluoride, and selenium.
Diversity of Archaea IV
Hyperthermophilic archaea are a group of extremophiles thriving at temperatures above 80°C, often in hydrothermal vents and volcanic soils where conditions surpass the boiling point of water. At such temperatures, proteins, membranes, and DNA in most organisms degrade, but hyperthermophiles have evolved remarkable adaptations to maintain stability and function.Unique Cellular FeaturesHyperthermophilic membranes are composed of a monolayer of biphytanyl tetraether lipids, which resist thermal...
Origin of Photosynthesis
Photosynthesis represents a fundamental biological process that transformed Earth's atmosphere and paved the way for complex life. Emerging roughly 3.4–3.8 billion years ago, the earliest photosynthetic organisms harnessed light energy to produce organic compounds. These anoxygenic phototrophs used electron donors like hydrogen sulfide (H₂S) or ferrous iron (Fe²⁺), rather than water, and did not release molecular oxygen (O₂) as a byproduct. Various groups, including green sulfur and purple...
Deep Sea Microbial Ecology
The deep ocean and its underlying sediments represent vast, largely unexplored microbial habitats that extend far beyond the sunlit photic zone. The photic (euphotic) zone typically spans the upper ~100–200 meters of pelagic waters in the open ocean, but its depth varies geographically and seasonally, where sufficient light supports photosynthetic life. Below this lies the deep sea, spanning roughly 1000–6000 meters (bathypelagic to abyssal zones), with deeper hadal trenches extending beyond...
Acid Mine Drainage
Mining activities that disturb sulfide-rich rocks, particularly those containing pyrite (FeS₂), initiate a cascade of geochemical and microbiological processes with serious environmental implications. When exposed to air and water, pyrite undergoes oxidation, releasing sulfate, ultimately forming sulfuric acid and mobilizing heavy metals into surrounding water systems. This phenomenon, known as acid mine drainage (AMD), results in low pH waters laden with toxic elements that threaten aquatic...


