Journal article
Oxidation response of transpiration-cooled ZrB2 on a hypersonic stagnation point
- Abstract:
- This work presents the oxidation response of a transpiration-cooled hypersonic stagnation point made of porous ZrB2. Low-order models are used to calculate the surface temperature and oxygen concentration for a given flight condition. An analytical material oxidation model computes the surface recession and oxide layer thickness. A 500 s steady-state trajectory at 44 km altitude and 3.6 km/s velocity is found to lead to 2.2 mm recession of the 3 mm nose radius. A constant mass injection at a blowing parameter of 0.6 reduces the recession to just 0.21 mm. The displacement of freestream oxygen by transpiration cooling has a significant effect on oxidation. Not accounting for the displacement of oxygen at the surface would increase the recession by up to 197%. The recession along the transient trajectory of an envisioned hypersonic vehicle with a 3 mm nose radius is found to exceed 0.94 mm with no mass injection. It is shown that nitrogen and helium injection at a blowing parameter of 0.6 can reduce the recession to 0.13 and 0.075 mm, respectively.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
-
-
(Preview, Accepted manuscript, pdf, 1.8MB, Terms of use)
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- Publisher copy:
- 10.2514/1.A35309
Authors
- Publisher:
- American Institute of Aeronautics and Astronautics
- Journal:
- Journal of Spacecraft and Rockets More from this journal
- Volume:
- 59
- Issue:
- 5
- Pages:
- 1486-1495
- Publication date:
- 2022-05-15
- Acceptance date:
- 2022-04-10
- DOI:
- EISSN:
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1533-6794
- ISSN:
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0022-4650
- Language:
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English
- Keywords:
- Pubs id:
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1261861
- Local pid:
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pubs:1261861
- Deposit date:
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2022-08-11
- ARK identifier:
Terms of use
- Copyright holder:
- The American Institute of Aeronautics and Astronautics, Inc.
- Copyright date:
- 2022
- Rights statement:
- Copyright © 2022 by the American Institute of Aeronautics and Astronautics, Inc. All rights reserved.
- Notes:
-
This is the accepted manuscript version of the article. The final version is available from American Institute of Aeronautics and Astronautics at https://doi.org/10.2514/1.A35309
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