Titlebook: Impact of Modern Dynamics in Astronomy; Proceedings of the I J. Henrard,S. Ferraz-Mello Conference proceedings 1999 Springer Science+Busine

STRI

書目名稱Impact of Modern Dynamics in Astronomy影響因子(影響力)




書目名稱Impact of Modern Dynamics in Astronomy影響因子(影響力)學(xué)科排名




書目名稱Impact of Modern Dynamics in Astronomy網(wǎng)絡(luò)公開度




書目名稱Impact of Modern Dynamics in Astronomy網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Impact of Modern Dynamics in Astronomy被引頻次




書目名稱Impact of Modern Dynamics in Astronomy被引頻次學(xué)科排名




書目名稱Impact of Modern Dynamics in Astronomy年度引用




書目名稱Impact of Modern Dynamics in Astronomy年度引用學(xué)科排名




書目名稱Impact of Modern Dynamics in Astronomy讀者反饋




書目名稱Impact of Modern Dynamics in Astronomy讀者反饋學(xué)科排名

fastness

minion

https://doi.org/10.1007/978-94-011-4527-5astronomy; chaos; cosmology; planet; solar system; star

VERT

Entirety

The Use of Geocentric Variables to Search for Meteoroid Streams and Their ParentsA set of geocentric variables suitable for the identification of meteoroid streams has been recently proposed and successfully applied to photographic meteor orbits. We describe these variables and the secular invariance of some of them, and discuss their use to improve the search for meteoroid stream parents.

Anticlimax

吹牛大王

Periodic Orbits Around a Massive Straight SegmentIn this paper, we consider the motion of a particle under the gravitational field of a massive straight segment This model is used as an approximation to the gravitational field of irregular shaped bodies, such as asteroids, comet nuclei and planets’s moons. For this potential, we find several families of periodic orbits and bifurcations.

搜尋

Bianchi Cosmologies as Dynamical Systemsianchi class A cosmological models. We introduce new variables in which the Hamiltonian constraint for all the class A models is solved algebraically. We present results of dimension reduction of the investigated models.

PTCA635

制定法律

Trojans in Stable Chaotic Motionper elements. For each time interval we compared the root mean squares of the orbital elements (a, e and i) with the corresponding proper element It turned out that the variations of the proper elements .. in the different time intervals are correlated with the corresponding r.m.s.(e); this is not the case for sin .. with r.m.s.(i).