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发表于 2009-11-26 09:45 | 显示全部楼层 |阅读模式
本帖最后由 周文山 于 2009-11-27 09:39 编辑

火星曾三分之一覆盖海洋 生命存在可能性增加




图中标注的红色网状结构,科学家认为是由流向大海的河流侵蚀产生的溪谷。这个区域显然的结果比早期研究得出的结果大一倍。


蓝色区域或许是海洋曾经所在的地方。位于蓝色区域下方的黄色、红色和绿色地带,科学家认为是他们发现的溪谷。他们认为,这些溪谷是由河流从南向北流向海洋的过程中侵蚀而成的.


现在的火星:今年10月,美国宇航局的“勇气”号火星车拍摄到这张灰尘弥漫的火星表面图.
据《每日邮报》报道,北伊利诺斯大学和美国宇航局的科学家认为,火星曾有三分之一的表面被海洋覆盖。这种惊人的景象增加了这颗红色行星——我们的太阳系中第四大行星存在生命的可能性。

研究人员利用新软件对火星表面进行分析,进而得出了这一结论。他们找到了很多溪谷,绘制成迄今为止最为详细的火星溪谷图。1971年科学家首次在火星上发现溪谷,这些溪谷是由河流网造成的。通过这项研究发现,溪谷的覆盖范围比以前绘图得出的结果大1倍多。这些水道位于赤道和中南纬度之间的狭长地带。

这些专家认为,他们已经标出曾从这颗红色行星南部高地流向北部海洋的河流的路径。该迹象表明,数十亿年前,火星的大部分地区都是干旱的大陆性气候,跟地球上更加干旱的地方非常类似。这颗红色行星上经常下雨,雨水流入河流,最终汇入海洋。火星历史早期的这个潮湿阶段可能大大增加了它上面孕育生命的机会。

迄今为止,现有的唯一一张火星全球溪谷网络图尚未完成,而且是利用卫星图手工绘制。这张图显示,火星上的溪谷网比地球上的更加稀疏,因此研究人员怀疑它们是由河流的径流侵蚀形成的。因此他们提出另一种解释——“地下水基蚀”,根据这一理论,水从地面喷出或渗出,产生侵蚀,形成河谷。

这张新图是利用卫星数据进行电脑分析产生的,该图显示,火星一些地区的溪谷网的稠密度几乎跟地球上的一模一样。领导这项研究的北伊利诺斯大学的罗伟(Wei Luo)教授说:“现在还很难说径流侵蚀不是火星溪谷网形成的主要机制。”

科学家在《地球物理学研究杂志:行星》(Journal of Geophysical Research - Planets)中写道,带状溪谷网模式可以解释是否火星北部曾存在一个较大的海洋。火星表面的最大特征是:低地几乎都位于北半球,高地几乎都位于这颗红色行星的南半部分。科学家认为,火星北半球可能曾存在浩瀚的海洋,这里至今仍是低地。

据美国研究人员说,在这之前火星上的溪谷网覆盖范围一直被人们低估。罗伟说:“北半球存在一个单一海洋,可能解释了为什么南半球缺少溪谷网。”

他说:“火星最靠南的区域,也是距离北部水源最远的地方,可能没有降水,因此没有溪谷形成。这可能也解释了为什么从北向南溪谷变得越来越浅。”现在火星上非常寒冷干燥,它上面的河流和海洋早已消失。火星大气层非常稀薄,如果这颗红色行星上有微生物存在,它们一定艰难地生活在布满灰尘的火星地表下。
 楼主| 发表于 2009-11-26 09:55 | 显示全部楼层
English Version:

The Red Planet was once blue... Giant ocean once covered third of Mars

By Daily Mail Reporter
Last updated at 8:42 AM on 24th November 2009

[size=1.2em]A vast ocean once covered a third of Mars, scientists believe.

[size=1.2em]Such a stunning prospect greatly increases the chances of life having existed on the Red Planet, the fourth from the Sun in our solar system.

[size=1.2em]Researchers have come to the conclusion after using new software to analyse images of the surface. As a result, they have managed to find dozens of valleys to build up the most detailed map to date.



The areas marked in red show where scientists believe valleys were caused by a network of rivers feeding into the ocean. This area is twice that mapped by earlier research, right


The area in blue shows where the ocean would have been. The yellow, red and green belt below it is where scientists found the valleys. They believe these were caused by water running from the south towards the ocean in the north



[size=1.2em]The valleys, first spotted in 1971, were caused by a network of rivers more than twice as extensive as previously mapped. The water channels were in a belt between the equator and mid-southern latitudes.
[size=1.2em]
[size=1.2em]The experts from Northern Illinois University and Nasa believe they mark the paths of rivers that once flowed from the planet's southern highlands into a huge ocean in the north.
More...

[size=1.2em]
[size=1.2em]The evidence suggests that billions of years ago much of Mars had an 'arid continental climate' similar to drier areas of the Earth.[size=1.2em]
[size=1.2em]Rain would have fallen regularly, swelling the rivers and topping up the ocean basin. Such a wet period early in the planet's history would have greatly increased the chances of life.[size=1.2em]
[size=1.2em]Until now the only global map of Martian valley networks that existed was incomplete and drawn by hand from satellite images.



Mars today: Nasa's Exploration Rover Spirit recorded this view of the Red Planet's dusty surface in October of this year

Writers and artists once thought Mars could be a lush planet with a population of Martians. The pictures beamed back from Viking 1 in 1976 quickly dispelled this view.

[size=1.2em]This indicated that valley networks are far more sparse on Mars than on Earth, raising doubts that they were created by the 'run-off erosion' of rivers.[size=1.2em]
[size=1.2em]An alternative explanation, known as 'groundwater sapping', was that water springing or seeping out of the ground eroded the channels.[size=1.2em]
[size=1.2em]The new map, created by a computerised analysis of satellite data, shows that some regions of Mars had valley networks almost as dense as those on Earth.[size=1.2em]
[size=1.2em]'It is now difficult to argue against run-off erosion as the major mechanism of Martian valley networks,' said research leader Professor Wei Luo, from Northern Illinois University.[size=1.2em]
[size=1.2em]The belt pattern of the valley network could best be explained if there was a large northern ocean, said the scientists writing in the Journal of Geophysical Research - Planets.[size=1.2em]
[size=1.2em]The Martian surface is characterised by lowlands located mostly in the northern hemisphere, and highlands mostly in the planet's southern half.[size=1.2em]
[size=1.2em]A planet-wide ocean may once have covered the northern regions where the lowlands exist today, the scientists believe.[size=1.2em]
[size=1.2em]The features resembling dry river valleys on Mars have been hotly debated by scientists since their discovery by the Mariner 9 spacecraft in 1971.[size=1.2em]
[size=1.2em]But, according to the US researchers, the extent of the valley networks has been greatly underestimated until now.[size=1.2em]
[size=1.2em]Professor Luo added: 'A single ocean in the northern hemisphere would explain why there is a southern limit to the presence of valley networks.[size=1.2em]
[size=1.2em]'The southernmost regions of Mars, located farthest from the water reservoir, would get little rainfall and would develop no valleys. This would also explain why the valleys become shallower as you go from north to south, which is the case.'[size=1.2em]
[size=1.2em]The Mars of today is a bitter cold place and bone dry, the rivers and seas are long gone. Its atmosphere is thin and wispy, and if microbes still exist, they're probably eking out a meagre existence somewhere beneath the planet's dusty soil.
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发表于 2009-11-26 11:02 | 显示全部楼层
★太湖大学生在外QQ群:76231925      Welcome all of you!
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发表于 2009-11-26 13:02 | 显示全部楼层
学习...............................
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 楼主| 发表于 2009-11-26 15:36 | 显示全部楼层
回复 4# 老鹰


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