Show simple item record

contributor authorHarris, Kurt E.
contributor authorSchillo, Kevin J.
contributor authorHew, Yayu M.
contributor authorKumar, Akansha
contributor authorHowe, Steven D.
date accessioned2017-11-25T07:18:42Z
date available2017-11-25T07:18:42Z
date copyright2017/25/5
date issued2017
identifier issn2332-8983
identifier otherners_003_03_031006.pdf
identifier urihttp://138.201.223.254:8080/yetl1/handle/yetl/4235345
description abstractIn the National Aeronautics and Space Administration (NASA) Design Reference Architecture 5.0 (DRA 5.0), fission surface power systems (FSPS) are described as “enabling for the human exploration of Mars.” This study investigates the design of a power conversion system (PCS) based on supercritical carbon dioxide (sCO2) Brayton configurations for a growing Martian colony. Various configurations utilizing regeneration, intercooling (IC), and reheating are analyzed. A model to estimate the mass of the PCS is developed and used to obtain a realistic mass-optimized configuration. This mass model is conservative, being based on simple concentric tube counterflow heat exchangers and published data regarding turbomachinery masses. For load following and redundancy purposes, the FSPS consists of three 333 kWe reactors and PCS to provide a total of 1 MWe for 15 years. The optimal configuration is a sCO2 Brayton cycle with 60% regeneration and two stages of intercooling. The majority of the analyses are performed in matlab, with certain data provided by a comsol multiphysics model of part of a low-enriched uranium (LEU) ceramic metallic (CERMET) reactor core.
publisherThe American Society of Mechanical Engineers (ASME)
titleMass Optimization of a Supercritical CO2 Brayton Cycle Power Conversion System for a Mars Surface Fission Power Reactor
typeJournal Paper
journal volume3
journal issue3
journal titleJournal of Nuclear Engineering and Radiation Science
identifier doi10.1115/1.4035974
journal fristpage31006
journal lastpage031006-7
treeJournal of Nuclear Engineering and Radiation Science:;2017:;volume( 003 ):;issue: 003
contenttypeFulltext


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record