scholarly journals Optimal rendezvous trajectory between Sample Return Orbiter and Orbiting Sample Container in a Mars Sample Return mission

2020 ◽  
Vol 171 ◽  
pp. 31-41 ◽  
Author(s):  
Alberto Fossà ◽  
Carlo Bettanini
2021 ◽  
Vol 11 (17) ◽  
pp. 8115
Author(s):  
Radu Mihalache ◽  
Dragos Mihai ◽  
Gheorghe Megherelu ◽  
Ionut Florian Popa ◽  
Ionut Sebastian Vintila ◽  
...  

The mission objective of the Phobos Sample Return is to collect and return 100 g of Phobos’ surface material to Earth inside a tight enclosure composed of a Vault, a Sample Container and sealing elements. One important aspect of the project was the development of a closing mechanism capable of ensuring a pushing force high enough compared to the available force of the robotic arm (40 N). The need for a higher pushing force derived from the design tests which were carried out to experimentally determine the necessary force to overcome the resistance of the sealing element when the vault is closed. Two types of sealing elements, custom made for this project, along with two SC with different geometrical shapes in the sealing area were tested. For better accuracy, the tests considered the imposed operational temperature domain for the vault, ECSS standards and the test rig set-up being performed at environmental temperature (+20 °C), −20 °C, −60 °C and +70 °C. The results of the tests highlighted that the negative temperature has a significant influence over the closing force, as this force is increasing once the operational temperature is decreasing. Based on the work performed, the most suitable type of sealing element was identified, in particular the piston geometry which allows a smaller force to close the vault.


2014 ◽  
Vol 66 (1) ◽  
Author(s):  
Takashi Mikouchi ◽  
Mutsumi Komatsu ◽  
Kenji Hagiya ◽  
Kazumasa Ohsumi ◽  
Michael E Zolensky ◽  
...  

2014 ◽  
Vol 53 (7) ◽  
pp. 1135-1142 ◽  
Author(s):  
Yoshinori Takano ◽  
Hajime Yano ◽  
Yasuhito Sekine ◽  
Ryu Funase ◽  
Ken Takai

2008 ◽  
Vol 23 (3) ◽  
pp. 809-847 ◽  
Author(s):  
Michael Küppers ◽  
H. U. Keller ◽  
E. Kührt ◽  
M. F. A’Hearn ◽  
K. Altwegg ◽  
...  

2009 ◽  
Vol 106 (17) ◽  
pp. 6904-6909 ◽  
Author(s):  
Matthieu Gounelle ◽  
Marc Chaussidon ◽  
Alessandro Morbidelli ◽  
Jean-Alix Barrat ◽  
Cécile Engrand ◽  
...  

Micrometeorites with diameter ≈100–200 μm dominate the flux of extraterrestrial matter on Earth. The vast majority of micrometeorites are chemically, mineralogically, and isotopically related to carbonaceous chondrites, which amount to only 2.5% of meteorite falls. Here, we report the discovery of the first basaltic micrometeorite (MM40). This micrometeorite is unlike any other basalt known in the solar system as revealed by isotopic data, mineral chemistry, and trace element abundances. The discovery of a new basaltic asteroidal surface expands the solar system inventory of planetary crusts and underlines the importance of micrometeorites for sampling the asteroids' surfaces in a way complementary to meteorites, mainly because they do not suffer dynamical biases as meteorites do. The parent asteroid of MM40 has undergone extensive metamorphism, which ended no earlier than 7.9 Myr after solar system formation. Numerical simulations of dust transport dynamics suggest that MM40 might originate from one of the recently discovered basaltic asteroids that are not members of the Vesta family. The ability to retrieve such a wealth of information from this tiny (a few micrograms) sample is auspicious some years before the launch of a Mars sample return mission.


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