Thermal Vacuum Testing of the Moon Mineralogy Mapper Instrument

2008 ◽  
Author(s):  
Jose I. Rodriguez ◽  
Howard Tseng ◽  
Burt Zhang ◽  
Arthur Na-Nakornpanom ◽  
Robert S. Leland
2000 ◽  
Author(s):  
M. Marchesi ◽  
R. Campaci ◽  
A. Nista ◽  
W. Prendin ◽  
S. Scarpa ◽  
...  

Author(s):  
Rachel L. Klima ◽  
Carle M. Pieters ◽  
Joseph W. Boardman ◽  
Robert O. Green ◽  
James W. Head ◽  
...  

Author(s):  
A. G. Vikulov

We implemented a systemic scientific approach to thermal vacuum development of spacecraft, which integrates the problems of thermal calculations, thermal vacuum tests and accuracy evaluation for mathematical models of heat transfer by means of solving identification problems. As a result, the following factors increase the efficiency of spacecraft ground testing: reducing the duration of thermal vacuum tests, making autonomous thermal vacuum testing of components possible, increasing the accuracy of thermal calculations


Author(s):  
Henry Quach ◽  
Marcos A. Esparza ◽  
Hyukmo Kang ◽  
Aman Chandra ◽  
Heejoo Choi ◽  
...  

2019 ◽  
Vol 11 (13) ◽  
pp. 1544
Author(s):  
Zhou ◽  
Zhang ◽  
Chen ◽  
Zhu

Olivine formation is directly related to Mg/Fe content. It is also significant in estimating the geological evolution of the moon. In this study, an estimation model of relative Mg number (Fo#) for lunar olivine was presented through multiple linear regression statistics. Sinus Iridum, the Copernicus Crater, and the pyroclastic deposit in the volcanic vents in the southeast of Orientale Basin were selected as the study areas. Olivine distribution was surveyed, and the relative Fo# calculation of olivine was implemented based on Moon Mineralogy Mapper (M3) data. Results demonstrated that olivine in the crater wall of Sinus Iridum and the Copernicus Crater had relatively high Fo#, which reflected the primitive melt. However, the difference in olivine spectral features between Sinus Iridum and the Copernicus Crater indicated different crystallization modes. The olivine in the pyroclastic deposit in the volcanic vents in the southwest of Orientale Basin also presented high Fo#, which indicated that the olivine was formed via rapid cooling crystallization and was accompanied by volcanic glass substances. As a result, the olivine relative Fo# calculated from the estimation model exhibited an important constraint implication for explanation of its causes.


Proceedings ◽  
2018 ◽  
Vol 2 (8) ◽  
pp. 534
Author(s):  
Jean-François Vandenrijt ◽  
Cédric Thizy ◽  
Fabian Languy ◽  
Marc Georges

Holographic interferometry at around 10 µm wavelengths has many advantages. It offers the possibility of large deformation measurement, while being much less sensitive to external perturbations. We present the state-of-the art of this technique applied to several industrial cases of the space industry. In particular, we demonstrate that the technique is well adapted to measurement of full-field deformation maps of space structures undergoing large temperature variations typical to what they experience in space conditions.


1995 ◽  
Author(s):  
Brian C. Baker ◽  
Fred E. Voss ◽  
George W. Wolfe

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