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Titlebook: Astronautics; The Physics of Space Ulrich Walter Textbook 20183rd edition Springer Nature Switzerland AG 2018 Orbit mechanics.Orbit perturb

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21#
發(fā)表于 2025-3-25 03:56:48 | 只看該作者
https://doi.org/10.1007/978-3-642-92094-3In Chap.?., we have looked at two point masses that were moving under their mutual gravitational influence. Formally speaking we were dealing with two bodies each with six degrees of freedom (three position vector components and three velocity vector components).
22#
發(fā)表于 2025-3-25 07:52:11 | 只看該作者
23#
發(fā)表于 2025-3-25 12:32:36 | 只看該作者
Asynchronmaschinen im Gleichlauf,In this section we derive some useful formulas for the design of satellite missions.
24#
發(fā)表于 2025-3-25 16:30:13 | 只看該作者
25#
發(fā)表于 2025-3-25 20:30:55 | 只看該作者
26#
發(fā)表于 2025-3-26 02:28:50 | 只看該作者
Orbital Maneuvering,The most important maneuver in space is the one to change the orbit of a space vehicle. Because the initial and final orbits are subject to a central gravitational potential such a S/C will transit between two Keplerian orbits. This is true not only for planetary orbits but also for interplanetary flights with the Sun as the central body.
27#
發(fā)表于 2025-3-26 06:01:12 | 只看該作者
Planetary Entry,After a spaceflight, the planetary entry (a.k.a. reentry for entry into Earth’s atmosphere) of a spacecraft is subject to the same aerodynamic and physical laws and equations (see Eqs.?(6.3.6) and (6.3.7)) as ascent. One might therefore infer that the circumstances of both situations are the same.
28#
發(fā)表于 2025-3-26 09:57:32 | 只看該作者
Three-Body Problem,In Chap.?., we have looked at two point masses that were moving under their mutual gravitational influence. Formally speaking we were dealing with two bodies each with six degrees of freedom (three position vector components and three velocity vector components).
29#
發(fā)表于 2025-3-26 12:39:42 | 只看該作者
30#
發(fā)表于 2025-3-26 18:20:13 | 只看該作者
Orbit Geometry and Determination,In this section we derive some useful formulas for the design of satellite missions.
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