English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/8218
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL
Exportar a otros formatos:


Stardust's Hydrazine (N2H4) Fuel: A Potential Contaminant for the Formation of Titanium Nitride (Osbornite)

AuthorsMartínez-Frías, J. ; Nna Mvondo, Delphine ; Rodríguez-Losada, José A.
KeywordsHydrazine (N2H4) monopropellant
Stardust space mission
Comet dust
Titanium nitride
Sample contamination
Nitridation processes
Issue Date14-Mar-2007
PublisherAmerican Chemical Society
CitationEnergy & Fuels 21(3): 1822-1823 (2007)
AbstractHundreds of space probes, satellites, and shuttles use ultrapure hydrazine monopropellant for guidance once in orbit. Stardust is the first U.S. mission devoted to exploring a comet and is the first U.S. mission designed to capture samples robotically from a comet and return them to Earth. The spacecraft is equipped with two sets of thrusters that use ultrapure hydrazine as a monopropellant.2,3 One of the biggest scientific surprises of this mission was the detection of tiny (sub-100-nm-size) grains of vanadium-bearing titanium nitride (osbornite).4,5 The use of hydrazine is one of the best significant methods of nitridation, which, precisely, has been used for the specific formation of titanium nitride. Stardust's hydrazine could have acted as a potential contaminant, coreacting with Ti compounds (either from the comet or the spacecraft), for the formation of the titanium nitride (osbornite) particles.
Description2 pages.
Publisher version (URL)http://dx.doi.org/10.1021/ef070014r
Appears in Collections:(CAB) Artículos
Files in This Item:
There are no files associated with this item.
Show full item record
Review this work

WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.