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“旅行者2号”在天王星系统:成像科学成果。

Voyager 2 in the uranian system: imaging science results.

作者信息

Smith B A, Soderblom L A, Beebe R, Bliss D, Boyce J M, Brahic A, Briggs G A, Brown R H, Collins S A, Cook A F, Croft S K, Cuzzi J N, Danielson G E, Davies M E, Dowling T E, Godfrey D, Hansen C J, Harris C, Hunt G E, Ingersoll A P, Johnson T V, Krauss R J, Masursky H, Morrison D, Owen T, Plescia J B, Pollack J B, Porco C C, Rages K, Sagan C, Shoemaker E M, Sromovsky L A, Stoker C, Strom R G, Suomi V E, Synnott S P, Terrile R J, Thomas P, Thompson W R, Veverka J

出版信息

Science. 1986 Jul 4;233(4759):43-64. doi: 10.1126/science.233.4759.43.

Abstract

Voyager 2 images of the southern hemisphere of Uranus indicate that submicrometersize haze particles and particles of a methane condensation cloud produce faint patterns in the atmosphere. The alignment of the cloud bands is similar to that of bands on Jupiter and Saturn, but the zonal winds are nearly opposite. At mid-latitudes (-70 degrees to -27 degrees ), where winds were measured, the atmosphere rotates faster than the magnetic field; however, the rotation rate of the atmosphere decreases toward the equator, so that the two probably corotate at about -20 degrees . Voyager images confirm the extremely low albedo of the ring particles. High phase angle images reveal on the order of 10(2) new ringlike features of very low optical depth and relatively high dust abundance interspersed within the main rings, as well as a broad, diffuse, low optical depth ring just inside the main rings system. Nine of the newly discovered small satellites (40 to 165 kilometers in diameter) orbit between the rings and Miranda; the tenth is within the ring system. Two of these small objects may gravitationally confine the e ring. Oberon and Umbriel have heavily cratered surfaces resembling the ancient cratered highlands of Earth's moon, although Umbriel is almost completely covered with uniform dark material, which perhaps indicates some ongoing process. Titania and Ariel show crater populations different from those on Oberon and Umbriel; these were probably generated by collisions with debris confined to their orbits. Titania and Ariel also show many extensional fault systems; Ariel shows strong evidence for the presence of extrusive material. About halfof Miranda's surface is relatively bland, old, cratered terrain. The remainder comprises three large regions of younger terrain, each rectangular to ovoid in plan, that display complex sets of parallel and intersecting scarps and ridges as well as numerous outcrops of bright and dark materials, perhaps suggesting some exotic composition.

摘要

“旅行者2号”拍摄的天王星南半球图像显示,亚微米级的霾颗粒和甲烷冷凝云的颗粒在大气中形成了微弱的图案。云带的排列与木星和土星的云带相似,但纬向风几乎相反。在测量到风的中纬度地区(-70度至-27度),大气旋转速度比磁场快;然而,大气的旋转速度向赤道方向降低,因此两者可能在约-20度处共转。“旅行者号”的图像证实了环粒子的反照率极低。高相位角图像揭示了大约10²个新的环状特征,其光学深度极低,尘埃丰度相对较高,散布在主环内,以及主环系统内侧一个宽阔、弥散、光学深度低的环。新发现的九颗小卫星(直径40至165公里)在环和米兰达之间运行;第十颗在环系统内。其中两个小天体可能通过引力限制了E环。奥伯龙和天卫二表面布满了大量陨石坑,类似于地球月球古老的布满陨石坑的高地,尽管天卫二几乎完全被均匀的暗物质覆盖,这可能表明存在一些持续的过程。泰坦尼亚和天卫一显示出与奥伯龙和天卫二不同的陨石坑分布;这些陨石坑可能是由与局限于其轨道的碎片碰撞产生的。泰坦尼亚和天卫一还显示出许多张性断层系统;天卫一有强有力的证据表明存在喷出物质。米兰达表面大约一半是相对平坦、古老、布满陨石坑的地形。其余部分由三个较年轻地形的大区域组成,每个区域在平面上呈矩形到卵形,显示出复杂的平行和交叉的陡坡和山脊以及许多明暗物质的露头,这可能暗示了某种奇特的成分。

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