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“旅行者2号”对天王星系统的射电科学观测:大气层、环和卫星

Voyager 2 radio science observations of the uranian system: atmosphere, rings, and satellites.

作者信息

Tyler G L, Sweetnam D N, Anderson J D, Campbell J K, Eshleman V R, Hinson D P, Levy G S, Lindal G F, Marouf E A, Simpson R A

出版信息

Science. 1986 Jul 4;233(4759):79-84. doi: 10.1126/science.233.4759.79.

Abstract

Voyager 2 radio occultation measurements of the Uranian atmosphere were obtained between 2 and 7 degrees south latitude. Initial atmospheric temperature profiles extend from pressures of 10 to 900 millibars over a height range of about 100 kilometers. Comparison of radio and infrared results yields mole fractions near the tropopause of 0.85 and 0.15 +/- 0.05 for molecular hydrogen and helium, respectively, if no other components are present; for this composition the tropopause is at about 52 kelvins and 110 millibars. Distinctive features in the signal intensity measurements for pressures above 900 millibars strongly favor model atmospheres that include a cloud deck of methane ice. Modeling of the intensity measurements for the cloud region and below indicates that the cloud base is near 1,300 millibars and 81 kelvins and yields an initial methane mole fraction of about 0.02 for the deep atmosphere. Scintillations in signal intensity indicate small-scale stucture throughout the stratosphere and upper troposphere. As judged from data obtained during occultation ingress, the ionosphere consists of a multilayer structure that includes two distinct layers at 2,000 and 3,500 kilometers above the 100-millibar level and an extended topside that may reach altitudes of 10,000 kilometers or more. Occultation measurements of the nine previously known rings at wavelengths of 3.6 and 13 centimeters show characteristic values of optical depth between about 0.8 and 8; the maxim value occurs in the outer region of the in ring, near its periapsis. Forward-scattered signals from this ring have properties that differ from those of any of Saturn's rings, and they are inconsistent with a discrete scattering object or local (three-dimensional) assemblies of orbiting objects. These signals suggest a new kdnd of planetary ring feature characterized by highly ordered cylindrical substructures of radial scale on the order of meters and azimuthal scale of kilometers or more. From radio data alone the mass of the Uranian system is GM(sys) = 5,794,547- 60 cubic kilometers per square second; from a combination of radio and optical navigation data the mass of Uranus alone is GM(u) = 5,793,939+/- 60 cubic kilometers per square second. From all available Voyager data, induding imaging radii, the mean uncompressed density of the five major satellites is 1.40+/- 0.07 grams per cubic centimeter; this value is consistent with a solar mix of material and apparently rules out a cometary origin of the satellites.

摘要

“旅行者2号”在南纬2度至7度之间对天王星大气层进行了无线电掩星测量。初始大气温度剖面在约100千米的高度范围内,压力从10毫巴延伸至900毫巴。如果不存在其他成分,将无线电和红外测量结果进行比较,得出对流层顶附近分子氢和氦的摩尔分数分别为0.85和0.15±0.05;对于这种成分,对流层顶温度约为52开尔文,压力为110毫巴。在压力高于900毫巴时信号强度测量中的显著特征强烈支持包含甲烷冰云层的大气模型。对云层区域及以下的强度测量进行建模表明,云底接近1300毫巴和81开尔文,并且得出深层大气中甲烷的初始摩尔分数约为0.02。信号强度的闪烁表明平流层和对流层上部存在小尺度结构。根据掩星进入期间获得的数据判断,电离层由多层结构组成,包括在100毫巴高度以上2000千米和3500千米处的两个不同层以及可能延伸至10000千米或更高高度的顶部延伸层。对9个先前已知环在3.6厘米和13厘米波长处的掩星测量显示,光学深度的特征值在约0.8至8之间;最大值出现在内环的外部区域,靠近其近心点。来自该环的前向散射信号具有与土星任何环都不同的特性,并且与离散散射物体或轨道物体的局部(三维)集合不一致。这些信号表明一种新型的行星环特征,其特点是具有高度有序的圆柱形子结构,径向尺度约为米级,方位尺度为千米或更大。仅根据无线电数据,天王星系统的质量为GM(sys)=5794547 - 60立方千米每秒平方;结合无线电和光学导航数据得出,仅天王星的质量为GM(u)=5793939±60立方千米每秒平方。根据“旅行者号”所有可用数据,包括成像半径,五大卫星的平均未压缩密度为1.40±0.07克每立方厘米;该值与太阳物质混合情况一致,显然排除了卫星的彗星起源。

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