Stevenson D J
California Institute of Technology, 150-21, Pasadena, California 91125, USA.
Nature. 2001 Jul 12;412(6843):214-9. doi: 10.1038/35084155.
The detection of strongly magnetized ancient crust on Mars is one of the most surprising outcomes of recent Mars exploration, and provides important insight about the history and nature of the martian core. The iron-rich core probably formed during the hot accretion of Mars approximately 4.5 billion years ago and subsequently cooled at a rate dictated by the overlying mantle. A core dynamo operated much like Earth's current dynamo, but was probably limited in duration to several hundred million years. The early demise of the dynamo could have arisen through a change in the cooling rate of the mantle, or even a switch in convective style that led to mantle heating. Presently, Mars probably has a liquid, conductive outer core and might have a solid inner core like Earth.
在火星上探测到强磁化的古老地壳是近期火星探测最令人惊讶的成果之一,它为火星核心的历史和性质提供了重要见解。富含铁的核心可能在约45亿年前火星的热吸积过程中形成,随后以上覆地幔决定的速率冷却。一个核心发电机的运行方式很像地球目前的发电机,但持续时间可能限于几亿年。发电机的早期消亡可能是由于地幔冷却速率的变化,甚至是导致地幔加热的对流方式的转变。目前,火星可能有一个液态的、导电的外核,并且可能像地球一样有一个固态的内核。