標(biāo)題: Titlebook: Dynamics and Evolution of Minor Bodies with Galactic and Geological Implications; Proceedings of the C S. V. M. Clube,S. Yabushita,J. Henra [打印本頁(yè)] 作者: 爆裂 時(shí)間: 2025-3-21 16:20
書(shū)目名稱(chēng)Dynamics and Evolution of Minor Bodies with Galactic and Geological Implications影響因子(影響力)
書(shū)目名稱(chēng)Dynamics and Evolution of Minor Bodies with Galactic and Geological Implications影響因子(影響力)學(xué)科排名
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書(shū)目名稱(chēng)Dynamics and Evolution of Minor Bodies with Galactic and Geological Implications讀者反饋
書(shū)目名稱(chēng)Dynamics and Evolution of Minor Bodies with Galactic and Geological Implications讀者反饋學(xué)科排名
作者: BAIL 時(shí)間: 2025-3-21 21:24 作者: Cabg318 時(shí)間: 2025-3-22 03:16
Ancient woodland and traditional managementn to suspect that many other stars and their surrounding cometary systems would not make a similar contribution. Occasionally interstellar comets must pass through the inner solar system, but Whipple (1975) considers it unlikely that such a comet is among the known cases of apparently hyperbolic com作者: amygdala 時(shí)間: 2025-3-22 08:22
Observation and recording in woodlandstive advantages of a source region in an extended ‘inner core’ of the Oort cloud or a compact ‘comet belt‘ just beyond the planetary system are finely balanced, and it is premature to consider the problem solved. A complication is that some comets belonging to the Jupiter family may be part of a tim作者: 爭(zhēng)論 時(shí)間: 2025-3-22 09:04
Serum Bile Acids in Health and Disease,tate condition for maintaining this structure at its present size by captures from the classical Oort cloud is reviewed on the basis of recent results concerning the absolute number of Jupiter family comets as a function of perihelion distance as well as the coupled physical and dynamical evolutions作者: Spinal-Tap 時(shí)間: 2025-3-22 14:17
Serum Bile Acids in Health and Disease, asteroids both mean motion resonances and secular resonances not only structure the phase space of regular orbits but are mainly at the origin for the inherent chaos of planet crosser objects..For comets and their chaotic routes temporary trapping into orbital resonances is a well known phenomenon.作者: Spinal-Tap 時(shí)間: 2025-3-22 17:49 作者: left-ventricle 時(shí)間: 2025-3-22 21:23
The Role of Food Stamps in Welfare Reformsthat the planetary perturbations can greatly increase the streams thickness and each stream may produce several couples of meteor showers active in different seasons of the year. The theoretical and observed data are in a satisfactory accordance.作者: crease 時(shí)間: 2025-3-23 04:05 作者: Bridle 時(shí)間: 2025-3-23 08:16
David M. Betson,David H. Greenberga level, major evaporite (salt) deposits, continental flood-basalt eruptions, first-order discontinuities in sea-floor spreading, and major mountain building events, have been aggregated and analyzed with moving-window and spectral techniques that facilitate recognition of clustering and possible cy作者: 技術(shù) 時(shí)間: 2025-3-23 12:57 作者: Interregnum 時(shí)間: 2025-3-23 14:18 作者: 臭了生氣 時(shí)間: 2025-3-23 19:08 作者: Simulate 時(shí)間: 2025-3-24 01:51 作者: 旅行路線 時(shí)間: 2025-3-24 05:55 作者: Corporeal 時(shí)間: 2025-3-24 06:38 作者: Misnomer 時(shí)間: 2025-3-24 11:34
Selecting the Appropriate Assessment Methods and the magnetized ambient solar wind plasma on the evolution of their orbits are analysed. The orbital elements and the distribution in space of the charged dust particles undergo changes due to the effect of additional forces, especially the Lorentz force, acting on such particles, and, hence, t作者: HARP 時(shí)間: 2025-3-24 16:28
B. Hidayat,K. Supelli,K. A. van der Huchts, ropy glass and agglutinates. The agglutinates bonded by crystal and glassy materials contain hydrogen and helium from the solar wind components. Lunar shocked minerals of plagioclase and silica show anomalous compositions and densities. There are typical two formation processes on planetary mater作者: 山羊 時(shí)間: 2025-3-24 21:25 作者: Feigned 時(shí)間: 2025-3-25 02:32
https://doi.org/10.1007/978-94-009-7648-1ow close to the Sun dust grains survive. Dust grains close to the Sun are heated by solar radiation and are evaporated. Thus, a dust free zone is formed. There is a question as to how large this dust free zone may be.作者: 流浪 時(shí)間: 2025-3-25 04:20
Evolution Of Short-Period Meteoroid Streams,that the planetary perturbations can greatly increase the streams thickness and each stream may produce several couples of meteor showers active in different seasons of the year. The theoretical and observed data are in a satisfactory accordance.作者: 慢慢啃 時(shí)間: 2025-3-25 08:55 作者: capillaries 時(shí)間: 2025-3-25 12:17 作者: transient-pain 時(shí)間: 2025-3-25 19:08 作者: 虛弱的神經(jīng) 時(shí)間: 2025-3-25 23:28
http://image.papertrans.cn/e/image/283967.jpg作者: 英寸 時(shí)間: 2025-3-26 04:05 作者: idiopathic 時(shí)間: 2025-3-26 06:23 作者: 要塞 時(shí)間: 2025-3-26 09:10 作者: transdermal 時(shí)間: 2025-3-26 15:40
Conference proceedings 1992ic of periodic phenomena in the Solar System as signified bygeological records, together with several associated developments incelestial dynamics. All these problems are interwoven. This book makesa contribution towards unravelling the nature of the interactionsbetween the Earth and its celestial environment. .作者: UNT 時(shí)間: 2025-3-26 19:01
Serum Bile Acids in Health and Disease, that evidently occur. Like in most earlier investigations, a clear shortage is found in the classical Oort cloud source. The shortage seems, however, less extreme than sometimes assumed. Monte Carlo simulations are envisaged as a way to shed further light on the fate of Jupiter family comets.作者: BOAST 時(shí)間: 2025-3-26 22:17 作者: echnic 時(shí)間: 2025-3-27 02:28 作者: 共棲 時(shí)間: 2025-3-27 06:29
J. Fred Giertz,Dennis H. Sullivane are also investigated..Correlations between the meteor numbers and the apparitions of naked-eye comet likely to be found, and seasonal variations in the meteor flux recorded during nineteen centuries show two maxima in July-August and October-November, the latter may be related to the Taurid complex.作者: Fortuitous 時(shí)間: 2025-3-27 11:47 作者: 束以馬具 時(shí)間: 2025-3-27 15:46
Observation and recording in woodlandsts, the cratering record on the terrestrial planets and satellites of the outer planets, and the environmental impact posed by massive bodies and their decay products in the Earth’s near-space environment.作者: 背帶 時(shí)間: 2025-3-27 21:07 作者: intercede 時(shí)間: 2025-3-28 01:38
Structure And Evolution Of The Jupiter Family, that evidently occur. Like in most earlier investigations, a clear shortage is found in the classical Oort cloud source. The shortage seems, however, less extreme than sometimes assumed. Monte Carlo simulations are envisaged as a way to shed further light on the fate of Jupiter family comets.作者: organic-matrix 時(shí)間: 2025-3-28 03:34 作者: 一再遛 時(shí)間: 2025-3-28 09:53 作者: confide 時(shí)間: 2025-3-28 11:21 作者: 柔聲地說(shuō) 時(shí)間: 2025-3-28 17:42 作者: outrage 時(shí)間: 2025-3-28 20:07 作者: DOLT 時(shí)間: 2025-3-29 02:18
Progress In The Elliptic Restricted 3-Body Problem: Asteroids In The 2/1, 3/1 And 1/1 Resonance,ose approach with a major planet can throw out the hody from the main belt or can cause a collision! We also prescnt new results of the largeness of stable zones around the Lagrangean equilibrium points L. and L. and compare them with existing ones.作者: nerve-sparing 時(shí)間: 2025-3-29 06:09 作者: 演繹 時(shí)間: 2025-3-29 10:59 作者: Indebted 時(shí)間: 2025-3-29 13:43
Short-Period Comets And Apollo-Amor-Aten Type Asteroids In View Of Tisserand Invariant,作者: Blasphemy 時(shí)間: 2025-3-29 19:35 作者: disparage 時(shí)間: 2025-3-29 22:30 作者: Emmenagogue 時(shí)間: 2025-3-30 03:54 作者: Tdd526 時(shí)間: 2025-3-30 08:04 作者: GIBE 時(shí)間: 2025-3-30 08:18 作者: cruise 時(shí)間: 2025-3-30 15:54 作者: ALLAY 時(shí)間: 2025-3-30 19:55 作者: 鐵砧 時(shí)間: 2025-3-31 00:04 作者: encomiast 時(shí)間: 2025-3-31 04:46 作者: NOT 時(shí)間: 2025-3-31 08:29 作者: 龍卷風(fēng) 時(shí)間: 2025-3-31 11:11 作者: ambivalence 時(shí)間: 2025-3-31 14:05
A Model Of The Galactic Tidal Interaction With The Oort Comet Cloud, was inside 15 AU we assume that planetary perturbations would have removed the comet from the . energy distribution accessible by the galactic tide. Comets which had their perihelia changed from beyond 15 AU to within 5 AU in a single orbit are taken to be observable. We are able to track the evolu作者: 廢止 時(shí)間: 2025-3-31 21:02
Origin Of Oort Cloud Comets In The Interstellar Space,ditional Oort Cloud (Oort, 1950) could be captured from the interstellar medium. However, we note that the so called Kuiper belt (Kuiper, 1951) of comets cannot arise through this process. Therefore we have to ask how necessary the concept of the yet unobserved Kuiper belt is for the theory of short作者: Mindfulness 時(shí)間: 2025-4-1 01:06
Collective Resonant Phenomena On Small Bodies In The Solar System,tion. Numerical results obtained in an other context show that the competition between the Poynting-Robertson drag and the gravitational interaction of grains near the 2/1 resonance might be very important in the long run for the structure of meteor streams.作者: 過(guò)度 時(shí)間: 2025-4-1 02:18
Dynamics Of Periodic Comets And Meteor Streams,merical study of cometary dynamics using mappings is carried out. A distribution like the Oort cloud is a typical stage of the evolution of comets in nearly-parabolic orbits under planetary perturbations..A change of the partial density of meteor streams is studied. For the case of librations the di作者: Magisterial 時(shí)間: 2025-4-1 07:45
Episodes Of Terrestrial Geologic Activity During The Past 260 Million Years: A Quantitative Approacnificant underlying periodicity of 26.6 Myr for the Mesozoic and Cenozoic (the exact period differs with minor changes in geologic dating). Phase information suggests that the most recent maximum of the cycle occurred within the last 9 Myr, and may be close to the present time. The quasi-regular pul作者: assail 時(shí)間: 2025-4-1 11:25 作者: Meander 時(shí)間: 2025-4-1 15:44
