scholarly journals Experiments Indicate Regolith is Looser in the Lunar Polar Regions Than at the Lunar Landing Sites

Author(s):  
P. T. Metzger ◽  
S. Anderson ◽  
A. Colaprete
Icarus ◽  
2019 ◽  
Vol 333 ◽  
pp. 528-547
Author(s):  
W. Iqbal ◽  
H. Hiesinger ◽  
C.H. van der Bogert

2004 ◽  
Vol 3 (3) ◽  
pp. 273-273

In the paper Biological contamination studies of lunar landing sites by D.P. Glavin et al., published online 2004, there is an error on page 4 of the paper.On Page 4, line 5, column 1:∼3×105 should read ∼3×107


2014 ◽  
Vol 101 ◽  
pp. 149-161 ◽  
Author(s):  
Myriam Lemelin ◽  
David M. Blair ◽  
Carolyn E. Roberts ◽  
Kirby D. Runyon ◽  
Daniela Nowka ◽  
...  

2020 ◽  
Author(s):  
Igor Mitrofanov ◽  
Lev Zelenyi ◽  
Vladislav Tretyakov

<p>The most interesting sites for future lunar outposts are thought to be located closely to poles, and South one is found to be more preferable.  But before humans could land there, the sequence of robotic missions should be implemented to study the natural environment at the selected sites, to deliver some supporting systems for ensuring conditions of habitability and also to test the innovated technology for Earth-Moon-Earth round trip.</p><p>Therefore, the Russian Lunar Program will be ignited by four robotic missions, which Russian Academy of Science has selected for the initial stage of this Program. Their names Luna-25 -28 were selected taking into account the name of the last Soviet lander Luna-24 of 1976. The objectives of these missions are critically important for accomplishment of the future polar expeditions of humans. The missions will conduct orbital mapping of polar regions with fine spatial resolution, measurements of radiation environment at the selected landing sites, testing of water and space volatiles in the polar regolith, and, in particular – testing presence of complex molecules and pre-biotic molecular complexes, the lunar dust and exosphere, etc. Mobile elements of landing missions will investigate local areas around the landing sites to determine the best spots for the future habitation modules of human missions. In addition, the researches for the basic science will also be accomplished by these missions, such as the experiments for lunar-based astronomy at long wavelengths and at gamma-rays, the experiments for lunar seismology, for monitoring of interplanetary plasma and solar wind, etc.</p><p>The talk presents in details the concept of the key mission of the first stage of the Lunar Program, the Luna-28 mission for lunar polar sample return. The mission concept is based on the several basic requirements. The mission should have the return module for direct flight from Moon to Earth. The module should be able to deliver to the Earth a set of samples of polar regolith with the total mass of about 2 kilograms. They should be quarried from different depths of the shallow subsurface from several cm down to 1 meter. Samples should be delivered to the Earth with all volatiles, including water, in the frozen state. Small moonrover “Lunokhod” with mass below 100 kg should be delivered to the Moon by the lander. Before the launch of the return module, the rover could deliver remotely selected stones for return at the nearest vicinity of the lander, after the launch, the rover should conduct scientific studies of the area around the landing site.</p><p>The mission of Luna-28 will also be supported by the ground segment for proper curation of delivered samples and for their studies in the leading domestic and international research centers. The complex molecules and organic molecular complexes will be the main objects for these studies.   </p>


The Moon ◽  
1972 ◽  
Vol 5 (1-2) ◽  
pp. 52-89 ◽  
Author(s):  
Thomas B. McCord ◽  
Michael P. Charette ◽  
Torrence V. Johnson ◽  
Larry A. Lebofsky ◽  
Carle Pieters
Keyword(s):  

Icarus ◽  
2020 ◽  
Vol 352 ◽  
pp. 113991
Author(s):  
W. Iqbal ◽  
H. Hiesinger ◽  
C.H. van der Bogert

2020 ◽  
Vol 217 (1) ◽  
Author(s):  
Jianjun Liu ◽  
Xingguo Zeng ◽  
Chunlai Li ◽  
Xin Ren ◽  
Wei Yan ◽  
...  

AbstractLanding site selection is of fundamental importance for lunar landing mission and it is closely related to the scientific goals of the mission. According to the widely concerned lunar science goals and the landing site selection of the ongoing lunar missions; China has carried out the selection of landing site for a series of Chang’ E (CE) missions. Under this background, this paper firstly introduced the principles, process, method and result of landing site selection of China’s Lunar Exploration Program (CLEP), and then analyzed the support of the selected landing sites to the corresponding lunar research. This study also pointed out the outcomes that could possibly contribute to the key lunar questions on the basis of the selected landing sites of CE-4 and CE-5 such as deep material in South Pole-Aitken (SPA) basin, lunar chronology, volcanic thermodynamics and geological structure evolution history of the Moon. Finally, this approach analyzed the development trend of China’s follow-up lunar landing missions, and suggested that the South Pole Region of the Moon could be the landing site of high priority for the future CE missions.


Geophysics ◽  
1978 ◽  
Vol 43 (4) ◽  
pp. 819-822 ◽  
Author(s):  
Raymond D. Watts ◽  
William Isherwood

Prior to 1974, glaciologists used gravity surveys as a means of determining ice thickness, but the density variations in the underlying rocks were inherent sources of errors in their measurements. Because of these errors and because of the poor resolution of the gravity techniques, better geophysical tools for obtaining ice depths were sought. In polar regions, where the ice is below its melting temperature throughout most of the ice mass, radio echo sounders were used successfully starting about 1960. Until 1974, however, radio echo sounder experiments on temperate glaciers were unsuccessful. Temperate glaciers are found throughout the mountains of Washington, Western Canada, and Alaska. In many of these areas, terrain is so rugged that a helicopter‐borne gravity crew can find very few landing sites which are not on glaciers (Figure 1).


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