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Gaspra

加斯帕

Gaspra is one of the larger asteroids and gained publicity in 1991 when the spacecraft Galileo swung by it on October 29 in a slingshop maneuver to gain energy as a part of its planned Jupiter mission. Referred to as 951 Gaspra, this asteroid is an irregular body with dimensins about 19x12x11 kilometers (12x7.5x7 miles).

Gaspra 是一颗较大的小行星,1991年因航天器伽利略号在10月29日经过它时,利用‘弹弓’机动为其木星任务获取能量而受到关注。被称为951 Gaspra,这颗小行星形状不规则,尺寸约为19×12×11公里(12×7.5×7英里)。
NASA Image

This picture of 951 Gaspra is an enhanced image based on data from the Galileo spacecraft as it approached on October 29, 1991. The base image is a black and white image upon which are superimposed subtle color variations constructed from violet, green, and near-infrared(1000nm) images taken in an earlier sequence. The subtle color variations have been artificially exaggerated; the surface looked fairly homogeneous. However, the subtle changes were there and were correlated with significant surface features. The bluish areas represent regions of slightly higher albedo, which also absorb somewhat more strongly in the 1000 nm band, probably due to the mineral olivine. These bluish areas tend to be associated with some of the crisper craters and ridges. The slightly reddish areas, apparently concentrated in topographic lows, represent regions of somewhat lower albedo and weaker absorption near 1000 nm. In general, such patterns can be explained in terms of greater exposure of fresher rock in the brighter bluish areas and the accumulation of some regolith materials in the darker reddish areas.

这张951 Gaspra的图片是根据1991年10月29日伽利略探测器接近时传回的数据增强而成的。原始图像是一张黑白图像,其上叠加了由紫色、绿色和近红外(1000nm)图像构建的细微颜色变化,这些图像是在先前序列中拍摄的。这些细微的颜色变化被人为放大了;表面看起来相当均匀。然而,这些细微的变化确实存在,并且与显著的表面特征相关联。蓝色区域代表略高反照率的区域,这些区域在1000nm波段吸收更强,可能由于橄榄石矿物所致。这些蓝色区域往往与一些陨石坑和山脊更为清晰地关联。略带红色的区域,似乎集中在地形低处,代表反照率较低的区域,在1000nm附近吸收较弱。总体而言,这种模式可以解释为较新的岩石在较亮的蓝色区域更暴露,而较暗的红色区域则积累了部分月壤物质。
NASA 图像
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