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By how much does the backside of a reentry capsule heat up? 


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The backside of a reentry capsule can experience significant heating during entry and descent. Studies have shown that the backshell radiative heating on various configurations can reach peak heat flux values. For instance, a sphere-cone configuration observed a peak heat flux of about 3.5 W/cm² at the payload juncture during entry . Additionally, the ellipsled geometry experienced around 1.25 W/cm² on the backshell but up to 8 W/cm² on the base at very high angles of attack . Furthermore, in hypersonic flows, the heat flux on the afterbody of capsules can become significantly larger, emphasizing the importance of accurate heat transfer predictions for designing efficient thermal protection systems . These findings highlight the critical need for effective thermal shielding to manage the intense heating experienced by reentry capsules.

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The backside of a reentry capsule heats up to over 10,000 K due to strong shock waves, triggering endothermic chemical reactions that reduce the temperature field during Earth reentry.
The backside of a reentry capsule heats up less than estimated due to spending more time in a dilute atmosphere, as predicted by the fluctuation-dissipation theory from Boltzmann kinetic equation.
The heat flux on the afterbody of a reentry capsule increases significantly, as observed in the study, with values notably larger compared to the forebody.
The paper focuses on measuring heat transfer on the front side of a re-entry capsule, not the backside. Backside heat-up is not addressed in the paper.
The backshell of a reentry capsule can experience peak heat fluxes of about 3.5 W/cm² for a sphere-cone configuration and up to 8 W/cm² for an ellipsled at high angles of attack.

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