Aerodynamic and Aerothermodynamic Analysis of Space Mission by Antonio Viviani, Giuseppe Pezzella

By Antonio Viviani, Giuseppe Pezzella

Presenting an up to date view at the most crucial house car configurations, this publication comprises specified analyses for a number of various kind of house venture profiles whereas contemplating vital elements corresponding to aerodynamic a lot, aerodynamic heating, motor vehicle balance and touchdown features. With that during brain, the authors offer an in depth review on assorted state of the art issues of hypersonic aerodynamics and aerothermodynamics, and look at diversified area motor vehicle shapes beneficial for various house venture ambitions. those include:

· workforce go back motor vehicle (CRV)

· team Exploration motor vehicle (CEV)

· pattern go back motor vehicle (SRV)

· Flying attempt mattress (FTB).

Throughout Aerodynamic and Aerothermodynamic research of house challenge Vehicles many examples are given, with targeted computations and effects for the aerodynamics and aerothermodynamics of all such configurations. furthermore, a last bankruptcy on destiny launchers is equipped and an Appendix on a potential manned venture to Mars closes the booklet. This paintings can be utilized as a reference for modelling and layout recommendations, for college kids meaning to input aerospace commercial careers, and to help either teachers and engineers operating within the box of area automobile design.

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Extra resources for Aerodynamic and Aerothermodynamic Analysis of Space Mission Vehicles

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The approximation of air as a perfect gas, however, is no more valid when temperature overcomes a threshold. 2 when we introduced the high-temperature effects issue. So, let us consider the nose region of an Apollo-like vehicle traveling at M1 D 36, as sketched in Fig. 27 [3]. The bow shock wave is normal, or nearly normal, in the nose region. So that the gas temperature behind this strong bow shock wave reaches about 11,000 K. At such high temperature, flow dissociation and ionization occur by means of chemical reactions.

33 where ™ is the flow direction and ¤ is the Prandtl–Meyer function [Eq. 35)]. It is possible to discretize the problem and consider two neighboring points, labeled 1 and 2 in Fig. 26, on AB. The characteristic lines, approximated by straight line segments, emanating from these points intersect at point 3. Hence, point 3 is influenced by both 1 and 2. KC /3 , and we can calculate  3 and ¤3 . Proceeding in a like manner from the other points on AB and giving special treatment to the boundaries, the entire flowfield may be charted.

40 1 Basics of Hypersonic Aerodynamics and Aerothermodynamics Perfect air Vibrational energy excited I Il Ill 120 Typical flight corridoe of ASTV 90 Altitude, km 60 IV Ionization of atoms N N+ + O+ + O Shuttle ascent 30 Oxygen dissociates O2 20 0 Shuttle entry 3 C & ee- Ionization of molecules O2+ + eO+O N +N N2+ + eN +O NO++ e- B Nitrogen dissociates N2 2N 6 9 Velocity, km/sec Typical flight corridoe for NASP A 12 15 Fig. 5 cm radius sphere Note, however, that Fig. 5 cm radius sphere. Therefore, the boundaries of A, B, and C regions must be adjusted according to the particular re-entry trajectory in the light of the binary scaling principle [3].

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