Hamiltonian Formulation and Perturbations for Dust Motion Around Cometary Nuclei     

Yu Jiang  Juergen Schmidt  Hexi Baoyin  Hengnian Li  Junfeng Li 《Earth, Moon, and Planets》2017,120(3):147-168

In this paper we analyze the dynamical behavior of large dust grains in the vicinity of a cometary nucleus. To this end we consider the gravitational field of the irregularly shaped body, as well as its electric and magnetic fields. Without considering the effect of gas friction and solar radiation, we find that there exist grains which are static relative to the cometary nucleus; the positions of these grains are the stable equilibria. There also exist grains in the stable periodic orbits close to the cometary nucleus. The grains in the stable equilibria or the stable periodic orbits won’t escape or impact on the surface of the cometary nucleus. The results are applicable for large charge dusts with small area-mass ratio which are near the cometary nucleus and far from the Solar. It is found that the resonant periodic orbit can be stable, and there exist stable non-resonant periodic orbits, stable resonant periodic orbits and unstable resonant periodic orbits in the potential field of cometary nuclei. The comet gravity force, solar gravity force, electric force, magnetic force, solar radiation pressure, as well as the gas drag force are all considered to analyze the order of magnitude of these forces acting on the grains with different parameters. Let the distance of the dust grain relative to the mass centre of the cometary nucleus, the charge and the mass of the dust grain vary, respectively, fix other parameters, we calculated the strengths of different forces. The motion of the dust grain depends on the area-mass ratio, the charge, and the distance relative to the comet’s mass center. For a large dust grain (> 1 mm) close to the cometary nucleus which has a small value of area-mass ratio, the comet gravity is the largest force acting on the dust grain. For a small dust grain (< 1 mm) close to the cometary nucleus with large value of area-mass ratio, both the solar radiation pressure and the comet gravity are two major forces. If the a small dust grain which is close to the cometary nucleus have the large value of charge, the magnetic force, the solar radiation pressure, and the electric force are all major forces. When the large dust grain is far away from the cometary nucleus, the solar gravity and solar radiation pressure are both major forces.  相似文献   

我国海洋遥感应用的进展   总被引：1，自引：0，他引：1  

刘宝银 《地球信息科学学报》2000,2(4):67-70

本文就我国20余年的海洋遥感应用历程,以三个阶段,4种类型信息源的分析及其相关手段和理论基础,按时间前后,着重阐述了所取得的成果,并展示我国海洋遥感技术未来发展的机遇与挑战.  相似文献   

渤海湾西岸几种地球化学的环境指标   总被引：2，自引：1，他引：1  

岳军  Dong yue  张宝华  牟林  王国明  陈安蜀  袁宝印  刘景兰  魏俊浩 《地质学报》2011,85(7):1239-1250

为了探讨渤海湾西岸全新世地层的古环境,本文进行了多种地球化学环境指标的分析,在此,将指示不同环境的指标进行了分项(或归类)如:古气候、氧化-还原、海-陆相环境指标等;并将其分别进行R型聚类分析和散点分析(获得了元素指标的相关系数及聚散特征).具体分析结果为:①古气候指标:如图2所示,古温度值与Rb/Sr比值呈正相关关系...  相似文献   

Orbits and manifolds near the equilibrium points around a rotating asteroid   总被引：6，自引：0，他引：6  

Yu Jiang  Hexi Baoyin  Junfeng Li  Hengnian Li 《Astrophysics and Space Science》2014,349(1):83-106

We study the orbits and manifolds near the equilibrium points of a rotating asteroid. The linearised equations of motion relative to the equilibrium points in the gravitational field of a rotating asteroid, the characteristic equation and the stable conditions of the equilibrium points are derived and discussed. First, a new metric is presented to link the orbit and the geodesic of the smooth manifold. Then, using the eigenvalues of the characteristic equation, the equilibrium points are classified into 8 cases. A theorem is presented and proved to describe the structure of the submanifold as well as the stable and unstable behaviours of a massless test particle near the equilibrium points. The linearly stable, the non-resonant unstable, and the resonant equilibrium points are discussed. There are three families of periodic orbits and four families of quasi-periodic orbits near the linearly stable equilibrium point. For the non-resonant unstable equilibrium points, there are four relevant cases; for the periodic orbit and the quasi-periodic orbit, the structures of the submanifold and the subspace near the equilibrium points are studied for each case. For the resonant equilibrium points, the dimension of the resonant manifold is greater than 4, and we find at least one family of periodic orbits near the resonant equilibrium points. As an application of the theory developed here, we study relevant orbits for the asteroids 216 Kleopatra, 1620 Geographos, 4769 Castalia and 6489 Golevka.  相似文献   

Orbital Mechanics near a Rotating Asteroid   总被引：2，自引：0，他引：2  

Yu Jiang  Hexi Baoyin 《Journal of Astrophysics and Astronomy》2014,35(1):17-38

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The hierarchical stability of the seven known large size ratio triple asteroids using the empirical stability parameters     

Xiaodong Liu  Hexi Baoyin  Franck Marchis 《Astrophysics and Space Science》2014,349(2):677-680

In this study, the hierarchical stability of the seven known large size ratio triple asteroids is investigated. The effect of the solar gravity and primary’s J ₂ are considered. The force function is expanded in terms of mass ratios based on the Hill’s approximation and the large size ratio property. The empirical stability parameters are used to examine the hierarchical stability of the triple asteroids. It is found that the all the known large size ratio triple asteroid systems are hierarchically stable. This study provides useful information for future evolutions of the triple asteroids.  相似文献   

Extension of the critical inclination     

Xiaodong Liu  Hexi Baoyin  Xingrui Ma 《Astrophysics and Space Science》2011,334(1):115-124

The critical inclination is of special interest in artificial satellite theory. The critical inclination can maintain minimal deviations of eccentricity and argument of pericentre from the initial values, and orbits at this inclination have been applied to some space missions. Most previous researches about the critical inclination were made under the assumption that the oblateness term J ₂ is dominant among the harmonic coefficients. This paper investigates the extension of the critical inclination where the concept of the critical inclination is different from that of the traditional sense. First, the study takes the case of Venus for instance, and provides some preliminary results. Then for general cases, given the values of argument of pericentre and eccentricity, the relationship between the multiplicity of the solutions for the critical inclination and the values of J ₂ and J ₄ is analyzed. Besides, when given certain values of J ₂ and J ₄, the relationship between the multiplicity of the solutions for the critical inclination and the values of semimajor axis and eccentricity is studied. The results show that for some cases, the value of the critical inclination is far away from that of the traditional sense or even has multiple solutions. The analysis in this paper could be used as starters of correction methods in the full gravity field of celestial bodies.  相似文献   

洪湖人类活动的沉积物记录   总被引：4，自引：0，他引：4  

陈萍  何报寅  远藤邦彦  杜耘  李世杰 《湖泊科学》2004,16(3):233-237

对洪湖150cm长的沉积物样芯进行了TOC、TN、TP、Ca、硫化物测试和AMS定年,在此基础上对洪湖地区人类活动的湖泊沉积响应进行了讨论.TOC和TN的含量呈现相似的变化规律,它们在样芯顶部和底部都出现显著峰值,而中部变化平坦,表示1500年来洪湖环境变演的三个显著不同的阶段;TP从过去到现在总体呈上升的趋势,但上升的幅度不大,这与磷在沉积物中复杂的循环机制有关;Ca的剖面变化显示为底部含量高上部低,其变化情况较复杂;硫化物在顶部15cm的含量比背景值略高,可能指示了上个世纪人类对铁矿和矿物燃料开采强度的增大.  相似文献   

新疆巴里坤湖十五万年来古水文演化序列   总被引：14，自引：3，他引：11       下载免费PDF全文

袁宝印  魏兰英  王振海  顾兆炎  赵惠敏 《第四纪研究》1998,18(4):319-327

通过巴里坤湖钻孔岩芯沉积相分析、年代学测定、粒度分析、碳酸盐及其稳定同位素测定、孢粉分析等综合研究,建立了巴里坤湖沉积岩芯剖面十五万年来的时间序列、湖水位变化的古水文演化序列,分辨出十五万年来经历的高湖面阶段和低湖面阶段。低湖面阶段对应于冰期阶段,在冰期时,降水主要积累于山地,进入湖泊的水量较少,湖水位降低;高湖面阶段对应于间冰期的到来,山地冰川融化,湖水位迅速上升,但很快达到新的平衡,水位保持稳定。  相似文献   

末次间冰期以来新疆巴里坤湖蒸发盐的沉积环境记录   总被引：25，自引：9，他引：16       下载免费PDF全文

顾兆炎  赵惠敏  王振海  袁宝印 《第四纪研究》1998,18(4):328-334

沉积物岩芯的碳酸盐、石膏等蒸发盐含量和矿物组成的证据显示了新疆巴里坤湖末次间冰期以来一直是一个水位变化频繁的浅水盐湖,有时甚至为间歇式的湖泊,约在34000aB.P.前后巴里坤湖沉积相发生了显著的变化,34000aB.P.之前为泥坪-湖滨相沉积,34000aB．P．之后为成湖相沉积。尽管我们对巴里坤湖34000aB．P．前后的沉积相变难以理解,但是长期处于浅水状态的巴里坤湖沉积物中蒸发盐的含量和矿物组成仍然与气候变化密切相关。在泥坪-湖滨相形成的碳酸盐中白云石相对的增加是地表强烈蒸发的结果。以石膏为主的蒸发盐含量增加是温度和降水增加所致,而其含量减少则是冰川前进致使补给水矿化度降低造成的。这使我们获得了该区古气候变化并不服从于冰期与雨期同步模式的信息。  相似文献