火星诺亚高地的秘密英文原文
译:
Shea


    在3年半的轨道飞行中,火星全球勘探者的轨道照相机拍摄了许多激动人心的照片,其中最让人心动的是这张诺亚高地中央环形山的照片。

    这座环形山坐落在南纬47度,西经355度,看上去几乎已被完全填充满,并且由于尚不清楚的原因有些局部的凹陷处也受到了侵蚀。在这一地区我们看到了MOC调查的两项重要结果——由液体流动侵蚀而成沟渠,以及分层的岩石的序列证明火星过去存在的地质活动。


                

    照片A显示了其他两张照片的位置,这三张照片是这个环形山的一系列照片中的一部分。

               

    照片B展示了在凹墙处沟渠的样例。它们的形状证明了流动的液体在它们的形成过程中所起的作用;暗色的地表预示在最近他们仍很活跃(或者,就像它周围的斜坡以及火星上的大部分地区,可能是由尘土的堆积而形成的)。这些沟渠形成于凹墙的下方,那儿存在一个与众不同的富巨石层。

                 

    照片C由两张高分辨率的图像(M09-00539和M15-00964)拼接而成,它展示了一个略高于填充环形山的物质层的地区。岩层的次序清晰可见,那儿岩层既不包含漂石也没有被侵蚀而产生漂石。请特别注意靠近中心的垂直岩层——它们提供了这些物质强度的证据。而且,在这里,沟渠似乎发源自不同的岩层;然而,它们形成的时间可能和照片B中的不同,覆盖在它们之上的灰尘层相对较薄。环形山如何被包含漂石的岩层所填充仍是个谜。

 

   NASA/JPL/MSSS 提供照片 2001年2月6号

Secrets of the Martian Noachian Highlands
Chinese Version


  Among the most exciting places that the Mars Global Surveyor's Mars Orbiter Camera has photographed during its three and a half years in orbit has been this crater in central Noachis Terra. 

  Located at 47 deg S, 355 deg W, the crater appears to have been almost completely filled, and subsequently eroded in localized pits, by unknown processes. In this one place we see elements of the two most important results of the MOC investigation -- the discovery of young gullies formed by fluid erosion and the occurrence of thick sequences of layered rock attesting to a martian past of substantial geologic activity. 

  Picture A shows the location of the other two figures, which are sections of three of about a dozen images acquired of this crater. 

  Picture B shows examples of gullies on the pit walls. Their contributary pattern (including the angles at which they join) argues for fluid behavior during their creation; the dark floors suggest that they have been active recently (or else they, like the slopes around them and most of Mars, would be lighter-toned owing to the accumulation of dust). These gullies are formed well down on the pit wall, where a distinctive, boulder-rich layer is found. 

  Figure C, a mosaic of two high resolution images (M09-00539 and M15-00964), shows an area somewhat higher in the sequence of layered material that fills the crater. This sequence clearly alternates between layers that either contain or erode to form boulders and layers that do not have boulders. Note in particular the overhanging layers near the top center -- such overhangs are evidence of the strength of the material. Here, too, gullies appear to start at specific layers; these, however, may not be as young as those seen in (B), as they appear to have at least a thin covering of dust. How it is that this crater came to be filled with layers of material containing (or eroding to create) boulders is a mystery. 

  Malin Space Science Systems and the California Institute of Technology built the MOC using spare hardware from the Mars Observer mission. MSSS operates the camera from its facilities in San Diego, CA. The Jet Propulsion Laboratory's Mars Surveyor Operations Project operates the Mars Global Surveyor spacecraft with its industrial partner, Lockheed Martin Astronautics, from facilities in Pasadena, CA and Denver, CO. 

 

   NASA/JPL/MSSS PHOTO RELEASE February 6, 2001

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