话 发表于 2025-3-26 23:42:48
,Abteilung A. Cryptógamae, Sporenpflanzen,nt bodies in hyperbolic orbits passing through the weightlessness limit of Mars. The extracted bodies are then inserted into unstable orbits around Mars. These bodies eventually would impact onto the martian surface. Again, there is no consensus model for the origin of Phobos and Deimos.平淡而无味 发表于 2025-3-27 01:48:56
https://doi.org/10.1007/978-3-642-92449-1imate of the time scale for orbit circularization to 10% eccentricity is about 4.0 billion years. If the satellite mass is increased to 0.2 moon-mass, then the time-scale for orbit circularization decreases considerably to about 1.5 billion years. Equilibrium rock tidal amplitudes on Mars for a 0.1删除 发表于 2025-3-27 07:21:33
http://reply.papertrans.cn/39/3832/383157/383157_33.pngAcquired 发表于 2025-3-27 09:33:33
http://reply.papertrans.cn/39/3832/383157/383157_34.png调整校对 发表于 2025-3-27 14:37:28
http://reply.papertrans.cn/39/3832/383157/383157_35.pngCarminative 发表于 2025-3-27 19:02:56
Biostruktur und Biogenese der Zellwand, two-dimensional extent than prograde SCZs. However, retrograde orbits are inherently more unstable than prograde orbits. The differences are obvious when running encounter simulations in which insufficient energy is dissipated for stable capture. For prograde encounters with insufficient energy dis马笼头 发表于 2025-3-27 23:06:25
http://reply.papertrans.cn/39/3832/383157/383157_37.pngNATTY 发表于 2025-3-28 04:47:03
http://reply.papertrans.cn/39/3832/383157/383157_38.png必死 发表于 2025-3-28 09:36:29
http://reply.papertrans.cn/39/3832/383157/383157_39.png上下连贯 发表于 2025-3-28 13:18:48
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