Neptune Trojans: a Revisit and a New Membertwo     

Wu Rui-jun  Zhou Lei  Zhou Li-yong 《Chinese Astronomy and Astrophysics》2019,43(2):262-277

Up to now, 17 Neptune Trojan asteroids have been detected with their orbits being well determined by continuous observations. This paper analyzes systematically their orbital dynamics. Our results show that except for two temporary members with relatively short lifespans on Trojan orbits, the vast majority of Neptune Trojans located within their orbital uncertainties may survive in the solar system age. The escaping probability of Neptune Trojans, through slow diffusion in the orbital element space in 4.5 billion years, is estimated to be ～50%. The asteroid 2012 UW177 classified as a Centaur asteroid by the IAU Minor Planet Center currently is in fact a Neptune Trojan. Numerical simulations indicate that it is librating on the tadpole-shaped orbit around the Neptune's L₄ point. It was captured into the current orbit approximately 0.23 million years ago, and will stay there for at least another 1.3 million years in the future. Its high inclination of i ≈ 54^° not only makes it the most inclined Neptune Trojan, but also makes it exhibit the complicated and interesting co-orbital transitions between the leading and trailing Trojans via the quasi-satellite orbit phase.  相似文献   

Scaling-laws of Radio Spike Bursts and Their Constraints on New Solar Radio Telescopestwo     

Tan Bao-lin  Cheng Jun  Tan Cheng-ming  Kou Hong-xiang 《Chinese Astronomy and Astrophysics》2019,43(1):59-74

Radio observation is one of important methods in solar physics and space science. Sometimes, it is almost the sole approach to observe the physical processes such as the acceleration, emission, and propagation of non-thermal energetic particles, etc. So far, more than 100 solar radio telescopes have been built in the world, including solar radiometers, dynamic spectrometers, and radioheliographs. Some of them have been closed after the fulfillment of their primary scientific objectives, or for their malfunctions, and thus replaced by other advanced instruments. At the same time, based on some new technologies and scientific ideas, various kinds of new and much more complicated solar radio telescopes are being constructed by solar radio astronomers and space scientists, such as the American E-OVSA and the solar radio observing system under the framework of Chinese Meridian Project II, etc. When we plan to develop a new solar radio telescope, it is crucial to design the most suitable technical parameters, e.g., the observing frequency range and bandwidth, temporal resolution, frequency resolution, spatial resolution, polarization degree, and dynamic range. Then, how do we select a rational set of these parameters? The long-term observation and study revealed that a large strong solar radio burst is frequently composed of a series of small bursts with different time scales. Among them, the radio spike burst is the smallest one with the shortest lifetime, the narrowest bandwidth, and the smallest source region. Solar radio spikes are considered to be related to a single magnetic energy release process, and can be regarded as an elementary burst in solar flares. It is a basic requirement for the new solar radio telescope to observe and discriminate these solar radio spike bursts, even though the temporal and spatial scales of radio spike bursts actually vary with the observing frequency. This paper presents the scaling laws of the lifetime and bandwidth of solar radio spike bursts with respect to the observing frequency, which provide some constraints for the new solar radio telescopes, and help us to select the rational telescope parameters. Besides, we propose a spectrum-image combination mode as the best observation mode for the next-generation solar radio telescopes with high temporal, spectral, and spatial resolutions, which may have an important significance for revealing the physical essence of the various non-thermal processes in violent solar eruptions.  相似文献   

A Review for the Thermophysics and the Yarkovsky and YORP Effects of Asteroidstwo     

Jiang Hao-xuan  Ji Jiang-hui 《Chinese Astronomy and Astrophysics》2019,43(1):1-22

The thermophysics of asteroids has become an important frontier for the research of asteroids in recent years. In this paper, we have introduced the thermophysical models commonly used in this field, by using these thermophysical models and combining with the data observed by the space or ground-based IR telescopes, some thermophysical parameters of asteroids, such as the thermal inertia, geometric albedo, effective diameter, surface roughness, and surface temperature, etc., can be derived. We have mentioned also the shape model and IR observation of asteroids, as well as the obtained thermophysical parameters for a part of asteroids. These thermophysical parameters can be further applied to studying the asteroids’ Yarkovsky effect, YORP effect, and so on, even can provide the relevant information for the spacecraft landing on the asteroid surface and the return mission of a spacecraft after the asteroid sampling.  相似文献   

银河系铝元素丰度研究     

马文娟  李宏杰  张波 《天文学报》2019,60(5):15-21

恒星的Al元素丰度可以为探索星团和星系的化学演化提供重要线索.通过系统分析银河系薄盘、厚盘、核球、银晕以及M4、M5等球状星团中恒星的[Al/Fe]随恒星金属丰度[Fe/H]的变化趋势,得出银河系薄盘、厚盘和核球恒星的[Al/Fe]随着[Fe/H]的增加而缓慢下降,而球状星团M4和M5恒星的[Al/Fe]随[Fe/H]增加没有下降趋势,这暗示Ia超新星对M4和M5恒星元素丰度的贡献比较小.详细研究了银河系恒星[Al/Fe]与[Mg/Fe]、[Na/Fe]的相关性,结果表明银河系场星的[Al/Fe]与[Mg/Fe]正相关,但在球状星团M4和M5恒星中未见此相关性;银河系盘星及M4和M5等球状星团恒星的[Al/Fe]与[Na/Fe]都存在正相关.  相似文献   

宇宙线的超新星遗迹起源     

张轶然  刘四明 《天文学报》2019,60(5):63-84

宇宙线的起源是高能天体物理的核心问题之一.一直以来,超新星爆发被认为是能谱膝区以下宇宙线的主要来源.多波段观测表明,超新星遗迹有能力加速带电粒子至亚PeV (10~(15)eV)能量.扩散激波加速被认为是最有效的天体高能粒子加速机制之一,而超新星遗迹的大尺度激波正好为这一机制提供平台.近年来,一系列较高精度的地面和空间实验极大地推动了对宇宙线以及超新星遗迹的研究.新的观测事实挑战着传统的扩散激波加速模型以及其在银河系宇宙线超新星遗迹起源学说上的应用,深化了人们对宇宙高能现象的认识.结合超新星遗迹辐射能谱的时间演化特性,构建的时间依赖的超新星遗迹粒子加速模型,不仅能够解释200 GV附近宇宙线的能谱反常,还自然地形成能谱膝区,甚至可以将超新星遗迹粒子加速对宇宙线能谱的贡献延伸至踝区.该模型预期超新星遗迹中粒子的输运行为表现为湍流扩散,这需要未来的观测以及与粒子输运相关的等离子体数值模拟工作来进一步验证.  相似文献   

Flora小行星族自转特性研究     

王夷博  刘承志  范存波  许妍 《天文学报》2019,(1):1-12

小行星族作为灾变碰撞的残留物,其基础物理性质提供了其母体以及后续演化信息.其中轨道以及自转特性分别反映了Yarkovsky效应以及Yarkovsky-O’Keefe-Radzievskii-Paddack效应(YORP效应)对于小行星族演化的影响.基于小行星光变数据库(Asteroid Lightcurve Database),通过对Flora小行星族自转速率分布进行研究,发现随着直径减小,族成员自转速率倾向于主要集中在3–5 d^-1的范围内.同时,可以注意到Flora小行星族整体表现出更倾向于顺行自转状态的现象,但对于轨道半长轴小于2.2au的成员来说,其顺行自转与逆行自转状态成员数目比接近于近地小行星中顺逆行自转状态源1:3的比例;此外,对于轨道半长轴大于2.2 au且具有顺行自转状态的部分族成员,在轨道半长轴-绝对星等分布中表现出聚集现象,并在聚集区域中有9颗成员展现出类似Slivan状态特征.  相似文献   

DMSP/OLS夜间灯光数据的四川省GDP空间化分析   总被引：1，自引：0，他引：1  

王俊华  张廷斌  易桂花  别小娟  刘栋  张甜甜 《测绘科学》2019,44(8):50-60

针对DMSP/OLS夜间灯光数据模拟省级格网GDP问题,该文选取2000、2006以及2010年DMSP/OLS稳定夜间灯光数据、辐射定标夜间灯光数据和四川省第二、三产业社会经济GDP数据,运用相关性分析、对比分析以及回归分析的方法,模拟出四川省GDP空间化密度图并分析与高程之间的关系。结果表明:在省级范围内,GDP与辐射定标灯光数据的相关性明显高于与稳定灯光数据的相关性,且前者的灯光指数CNLI与GDP相关性最高;运用3年的辐射定标灯光数据模拟得到四川省GDP密度图与GDP统计数据的拟合精度均达到0.99以上;2000-2010年四川省GDP呈现由成都市向四周不断扩张的趋势并随高程变化显著,四川省GDP高值区主要集中在高程1 000m以下的成都平原及周边区域,西部高原和山地地区GDP值较低。  相似文献   

鲁东南新石器遗址时空格局与自然环境的关系   总被引：1，自引：0，他引：1  

孔琪  刘冰  刘欢 《测绘科学》2019,44(7):88-95,104

针对史前文化遗址的时空间分布进行研究以进一步分析环境变化对人类聚居地带来的影响,对发现和保护历史文化遗址具有重要的意义。该文运用GIS空间分析方法对鲁东南地区史前遗址的时空分布特征进行分析,并结合区域地形地貌等条件分析遗址与自然环境条件的关系。结果表明:遗址点主要分布在高程50~200m、坡度0~6°、坡向朝南且距离河流200~2100m的范围内;且遗址点的分布呈现一定的聚集性,不同时期人类活动聚集中心存在迁移现象。由此得出古代人类倾向于选择海拔高度低,坡度小,向阳且靠近水源的地方聚居,且不同时期农业经济类型和社会的发展程度一定程度的影响了人类活动中心的位置分布。探究了鲁东南地区3个时期遗址时空分布和自然环境之间的关系,分析了不同时期人类活动中心的聚散特征。  相似文献   

滕州荆泉水源地岩溶塌陷特征与成因分析          下载免费PDF全文

贾继成  孟宪洲  白平 《山东国土资源》2018,34(6)

自2015年6月以来,在山东滕州荆泉水源地范围内连续发生多起岩溶塌陷。通过研究区域地质条件,在已有认识的基础上分析得出发育的浅层开口岩溶洞隙的存在,一定厚度的松散覆盖层及地下水位大幅下降是该区产生岩溶塌陷的基本条件。阐述了岩溶塌陷形成发育过程及影响因素,得出长期过量抽采岩溶水是区内岩溶塌陷的主要因素,合理减少地下水开采量是预防岩溶塌陷最有效的方法。  相似文献   

山东蓬莱地区侯格庄金矿床流体包裹体特征          下载免费PDF全文

王勇军  沈立军  朱裕振  黄鑫  徐昌  田明禛 《山东国土资源》2018,34(3)

侯格庄金矿床位于胶东栖(霞)-蓬(莱)金成矿带大柳行金矿田东南部。该文采用包裹体显微测温方法对金矿石中石英矿物内残留的流体包裹体进行研究,总结了金矿石石英矿物中的流体包裹体特征,并对该矿床成矿流体来源、矿床成因进行了研究。研究表明,该矿床石英矿物中流体包裹体以纯液包裹体为主,次为H_2O-CO_2气液两相包裹体及H_2O-CO_2三相包裹体,未见含子矿物包裹体。均一温度在109~396℃,盐度在2.9~22.44wt%NaCl,密度在0.64~1.06g/cm~3之间,估算成矿压力为128~340MPa,成矿深度约4.4~11.6km。该矿床至少经历了2个矿化期次,成矿流体为中低温、低盐度、低密度流体,流体来源于天水与岩浆水的混合产物,属中低温、中浅成热液矿床。  相似文献