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Thermal Properties and Behaviour of Am-Bearing Fuel in European Space Radioisotope Power Systems

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posted on 2022-12-22, 11:21 authored by Emily Jane Watkinson, Ramy Mesalam, Jean-François Vigier, Ondřej Beneš, Jean-Christophe Griveau, Eric Colineau, Mark Sierig, Daniel Freis, Richard M Ambrosi, Dragos Staicu, Rudy JM Konings
The European Space Agency is funding the research and development of 241Am-bearing oxide-fuelled radioisotope power systems (RPSs) including radioisotope thermoelectric generators (RTGs) and European Large Heat Sources (ELHSs). The RPSs’ requirements include that the fuel’s maximum temperature, Tmax, must remain below its melting temperature. The current prospected fuel is (Am0.80U0.12Np0.06Pu0.02)O1.8. The fuel’s experimental heat capacity, Cp, is determined between 20 K and 1786 K based on direct low temperature heat capacity measurements and high temperature drop calorimetry measurements. The recommended high temperature equation is Cp(T/K) = 55.1189 + 3.46216 × 102 T − 4.58312 × 105 T−2 (valid up to 1786 K). The RTG/ELHS Tmax is estimated as a function of the fuel thermal conductivity, k, and the clad’s inner surface temperature, Ti cl, using a new analytical thermal model. Estimated bounds, based on conduction-only and radiation-only conditions between the fuel and clad, are established. Estimates for k (80–100% T.D.) are made using Cp, and estimates of thermal diffusivity and thermal expansion estimates of americium/uranium oxides. The lowest melting temperature of americium/uranium oxides is assumed. The lowest k estimates are assumed (80% T.D.). The highest estimated Tmax for a ‘standard operating’ RTG is 1120 K. A hypothetical scenario is investigated: an ELHS Ti cl = 1973K-the RPSs’ requirements’ maximum permitted temperature. Fuel melting will not occur.

Funding

This research was funded by a number of entities. E. J. Watkinson wishes to acknowledge the Visiting Scientist agreement that has enabled the collaboration with EC JRC Karlsruhe. The University of Leicester acknowledges its significant in-kind contribution that paid for the time for E. J. Watkinson to work on this research, and the majority of travel and associated access costs for this collaboration. The University of Leicester also wishes to acknowledge the National Nuclear Laboratory for the provision of a contribution to the research travel and subsistence costs, as part of an ESA-funded programme. The University of Leicester acknowledges funding and support by the European Space Agency to pursue this research more widely, particularly of Keith Stephenson. ESA contract no.: 4000125885. Part of this research was funded by the H2020 EURATOM Research and Training Programme.

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Citation

Watkinson, E.J.; Mesalam, R.; Vigier, J.-F.; Beneš, O.; Griveau, J.-C.; Colineau, E.; Sierig, M.; Freis, D.; Ambrosi, R.M.; Staicu, D.; Konings, R.J.M. Thermal Properties and Behaviour of Am-Bearing Fuel in European Space Radioisotope Power Systems. Thermo 2021, 1, 297-331. https://doi.org/10.3390/thermo1030020

Author affiliation

School of Physics and Astronomy

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  • VoR (Version of Record)

Published in

Thermo

Volume

1

Issue

3

Pagination

297 - 331

Publisher

MDPI

eissn

2673-7264

Acceptance date

2021-10-08

Copyright date

2021

Available date

2021-10-15

Language

en

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