Exploring potential candidates of alternative solid hydrocarbon propellants for cold-gas thrusters

dc.contributor.authorLee, Thimthanaen
dc.contributor.authorDavoodianidalik, Mahdien
dc.contributor.authorTsifakis, Dimitriosen
dc.contributor.authorBoswell, Roderick W.en
dc.contributor.authorCharles, Christineen
dc.date.accessioned2025-05-23T10:21:59Z
dc.date.available2025-05-23T10:21:59Z
dc.date.issued2025en
dc.description.abstractCold-gas thrusters play a vital role as a subsystem in satellite operations facilitating space maneuvers in numerous missions. Achieving optimal propulsion necessitates not only continuous development of thruster design but also an exploration of novel propellant options to enhance overall performance. While an ideal propellant remains elusive, many studies have identified alternative options to replace commonly used inert gases. Choosing a solid-state propellant offers benefits such as the absence of a pressurised tank and sloshing effect. Hydrocarbon propellants are advantageous due to their non-corrosiveness and abundance as organic compounds on Earth. The sublimation process for manipulating solid propellants typically requires only a few watts, making it suitable for low-power budget missions. This work presents five solid hydrocarbon propellants for cold-gas thrusters, three of which have not yet been experimentally explored. The comparison between various aspects, including mass flow rate, power consumption, and several key performance parameters, is discussed. The measured mass flow rate is a function of the species and temperature, following the trend of the vapour pressure. The power consumption for all propellants only depends on the required heating temperature as they share similar thermal properties. The thrust generated by each propellant is comparable and linearly proportional to the mass flow rate when the flow is choked. Specific impulse remains relatively constant across different mass flow rates due to the strong correlation between thrust and mass flow rate. The thrust-to-power ratio is generally comparable among the propellants, except hexamine, which demands more power at higher operating temperatures due to increased heat loss. Among these alternatives, camphor emerges as the most promising candidate due to its low power consumption, thrust generation, and mass efficiency. On the other hand, naphthalene offers the best in terms of its superior thrust-to-power ratio and cost-per-kilogram advantage.en
dc.description.sponsorshipThis research was funded by the SP3 laboratory .en
dc.description.statusPeer-revieweden
dc.format.extent12en
dc.identifier.issn0094-5765en
dc.identifier.otherORCID:/0000-0002-5430-8540/work/184098430en
dc.identifier.scopus85207942480en
dc.identifier.urihttp://www.scopus.com/inward/record.url?scp=85207942480&partnerID=8YFLogxKen
dc.identifier.urihttps://hdl.handle.net/1885/733752025
dc.language.isoenen
dc.provenanceThis is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).en
dc.rights© 2024 The Author(s)en
dc.sourceActa Astronauticaen
dc.subjectAdamantaneen
dc.subjectBorneolen
dc.subjectCamphoren
dc.subjectCold-gas thrustersen
dc.subjectHexamineen
dc.subjectNaphthaleneen
dc.titleExploring potential candidates of alternative solid hydrocarbon propellants for cold-gas thrustersen
dc.typeJournal articleen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage438en
local.bibliographicCitation.startpage427en
local.contributor.affiliationLee, Thimthana; Australian National Universityen
local.contributor.affiliationDavoodianidalik, Mahdi; Department of Nuclear Physics & Accelerator Applications, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationTsifakis, Dimitrios; Department of Nuclear Physics & Accelerator Applications, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationBoswell, Roderick W.; Centre for Plasma and Fluids, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationCharles, Christine; Department of Nuclear Physics & Accelerator Applications, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.identifier.citationvolume226en
local.identifier.doi10.1016/j.actaastro.2024.10.047en
local.identifier.pure211520d5-1fec-4a4b-8cfe-5fd00d25c4a2en
local.identifier.urlhttps://www.scopus.com/pages/publications/85207942480en
local.type.statusPublisheden

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