卡西尼号最新图片(2004年06月10日)
Countdown to Phoebe
As Cassini sails toward its rendezvous with Phoebe, details on the small, dark moon are coming into view at a dizzying pace. The images shown here were taken only 13 hours apart on June 10, 2004, just one day prior to closest approach, and show a dramatic increase in detail between these two views. On Phoebe, the spin axis points up and approximately 13 degrees to the left of the boundary between day and night. Phoebe completes one rotation about its spin axis in 9 hours and 16 minutes. We are looking at opposite hemispheres in these two views.
A large crater, roughly 50 km (31 miles) across, is visible in the image on the left. The image on the right shows a body heavily pitted with craters of varying sizes, including very large ones, and displaying a substantial amount of variation in surface brightness. Features that appear to be cliffs may in fact be the boundaries between large craters. Despite its exaggerated topography, Phoebe is more round than irregular in shape.
Left to right, the two views were obtained at a phase, or Sun-Phoebe-spacecraft, angle of 87 degrees, and from distances ranging from 956,000 kilometers (594,000 miles) to 658,000 kilometers (409,000 miles). The image scale ranges from 5.7 to 3.9 kilometers (3.5 to 2.4 miles) per pixel. To aid visibility, the images were magnified three times via linear interpolation; no contrast enhancement was performed.
Phoebe is approximately 220 kilometers (137 miles) wide. Its many secrets await as Cassini draws close to its only flyby with this mysterious outer moon of Saturn at 1:56 pm PDT on June 11, 2004.
The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The imaging team is based at the Space Science Institute, Boulder, Colorado.
For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org.
Credit: NASA/JPL/Space Science Institute
Released: Jun 10, 2004 (PIA 06063)
据《洛杉矶时报》报道,美国国家航空航天局(NASA)专家最近又成功获取了一批土星最神秘的卫星土卫九的新照片,这是土星探测器“卡西尼”号在410万至250万千米远的距离上拍摄的。今天(6月11日)“卡西尼”号还将继续接近土卫九并在2000千米的距离上为这颗卫星拍摄最完美的写真集。
科学家们上一次拍摄土卫九是在1981年,那次使用的是安装在“旅行者”号探测器上的照相机。“卡西尼”号最近拍摄的土卫九照片比23年前“旅行者”号拍摄的照片质量提高了一倍多。这些新照片第一次让科学家们看清了土卫九的地貌状况,通过这些照片科学家们几乎可以分辨出土卫九表面的火山口和山峰。
土卫九最初被发现是在1898年,与土星的其它卫星相比从体积上来说它并算不上是老大,但是它却是土星最神秘的一颗卫星:在土星目前已探明的31颗卫星中,唯有它一个是逆向绕土星旋转的,它自转一周需要9小时16分钟。科学家们推测,土卫九这样独特的个性说明它最初可能不是太阳系的一分子,而是其它天外来客闯入太阳系后被土星重力场捕获并将其纳入了自己的卫星序列。
除此而外,土卫九还有另一个神秘之处:它的表面异常黑暗,但是却存在着水。这又不得不令科学家们相信它是构成土星的“建筑材料”的一部分。美国国家航空航天局的专家们期待着,本次对土卫九的近距离研究能够让他们获取更多有关太阳系形成的信息。
在与土卫九“亲密”接触后,“卡西尼”号还将继续进行它漫长的土星之旅。根据计划,“卡西尼”号将在土星轨道上工作四年。此外,它还将把一个小型探测器“惠更斯”号发送到土星最大的卫星土卫六上面以对这颗最令科研人员感兴趣的卫星展开研究。(编译/久亮)
来源: 新华网 2004-06-11 17:30 |
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