Asteroids相关论文
In spite of the work available on periodic solutions to the planar or spatial CR3BP,the obtained results were usually co......
Shock features and noble gas signatures in ordinary chondrites (OCs) provide essential clues to decipher impact and ther......
回顾小行星热物理研究中两种热物理模型TPM（thermal physical model）和ATPM（advanced thermo physical model），讨论了其科学应用及适用......
A semi-analytic model for the study of 1/1 resonant dynamics of the planar elliptic restricted co-or
Mean motion resonances (MMRs) are widespread in our Solar System.Moreover,resonant dynamics has always been an essential......
从基本物理出发，详细地介绍在小行星热环境研究中常用的几个热模型，并结合观测论述其具体科学应用。一般来说，小行星热模型可以分为两......
使用Watec 902H视频CCD和IOTA时间同步装置及望远镜,观测了1436号小行星掩恒星WY Gem,分析了观测数据,得到了光变曲线,结果表明该......
地基雷达探测是研究太阳系中小行星的重要方法。雷达探测主要有两种方式：（1）连续波探测，可得到小行星表面的粗糙度等参数；（2）延迟多普勒探......
柯伊伯带是指位于海王星轨道外的小天体构成的盘状区域。一般认为柯伊伯带小天体是早期太阳系物质凝聚成各大行星后的残留物，因此这......
Bus-DeMeo光谱分类系统中有24种小行星光谱类型以及约27种陨石矿物学类型。小行星和陨石之间的光谱联系在质量和可靠性上差异很大......
Low-inclination near-earth asteroid （NEA） （297274） 1996 SK, which isalso classified as a potentially hazardous asteroid, has......
At present, optical autonomous navigation has become a key technologyin deep space exploration programs. Recent studies ......
基于Planetary Data System（PDS）公布的433 Eros多面体模型,使用多面体模型法计算了433 Eros的表面引力加速度分布情况,并研究了该方......
小行星自转参数的资料不仅可以为小行星碰撞演化提供数据,还可以为太阳系的演化研究提供依据.利用云南天文台1米望远镜对主带碳类......
Study of photometric phase curve with new brightness model： refining phase function system parameter
We characterize the morphology of the photometric phase curve model of an asteroid with a threeparameter magnitude phase......
We carried out new photometric observations of asteroid(106) Dione at three apparitions(2004, 2012 and 2015) to understa......
随着ＳＬ－９彗星撞击木星这一罕见天象得到观测证实，搜索近地小行星以及与之相当的彗星的任务日益受到重视。本文首先从冷暗天体的辐射趋向......
The problems of dynamics of celestial bodies are considered which in the literature are explained by instability and ran......
A 3-D shape model of the sixth largest of the main belt asteroids, (704) Interamnia, is presented. The model is reproduc......
A 3-D shape model of the sixth largest of the main belt asteroids, (704) Interamnia, is presented. The model is reproduc......
