scholarly journals The use of jet penetrators for movement in the lunar soil

2019 ◽  
Vol 11 (S) ◽  
pp. 221-230
Author(s):  
Vladimir A. ZAGOVORCHEV ◽  
Olga V. TUSHAVINA
Keyword(s):  
Penetration Depth ◽  
Lunar Soil ◽  
Sufficient Accuracy ◽  
The Moon ◽  
Depth Of Penetration ◽  
Soil Movement ◽  
Subsurface Layers ◽  
Zero Entry ◽  
Entry Speed ◽  
Static Resistance

The possibility of using penetrators for researching the subsurface layers of the moon is considered. Possible options for launching such penetrators are indicated, from the way the launch is carried out depends on the depth of penetration into the regolith. It was found that when the propulsion system has less traction than the static resistance of the lunar soil, movement does not occur if the launch of the penetrator is accomplished from the surface with zero entry speed. The dependences are given that permit calculating with sufficient accuracy the penetrator mass, penetration depth and the resulting overloads. The depth of penetration of the inertial penetrator depends on its mass-dimensional qualities and the speed of entry into the soil, which is limited by the level of permissible overloads. The use of a solid fuel engine on the penetrator facilitates increasing the allowable speed of the penetrator into the ground by reducing the overloads acting on it, and thereby increasing the penetration depth.

scholarly journals 2.2.4 Lunar Soil Movement Registered by the Apollo 17 Cosmic Dust Experiment

1976 ◽  
Vol 31 ◽  
pp. 233-237 ◽  
Author(s):  
Otto E. Berg ◽  
Henry Wolf ◽  
John Rhee
Keyword(s):  
Lunar Surface ◽  
Lunar Soil ◽  
Cosmic Dust ◽  
Dust Particles ◽  
The Moon ◽  
Normal Impact ◽  
Soil Movement ◽  
Impact Parameters

In December, 1973, a Lunar Ejecta and Meteorites (LEAM) experiment was placed in the Taurus-Littrow area of the moon by the Apollo 17 Astronauts. Objectives of the experiment were centered around measurements of impact parameters of cosmic dust on the lunar surface. During preliminary attempts to analyze the data it became evident that the events registered by the sensors could not be attributed to cosmic dust but could only be identified with the lunar surface and the local sun angle. The nature of these data coupled with post-flight studies of instrument characteristics, have led to a conclusion that the LEAM experiment is responding primarily to a flux of highly charged, slowly moving lunar surface fines. Undoubtedly concealed in these data is the normal impact activity from cosmic dust and probably lunar ejecta, as well. This paper is based on the recognition that the bulk of events registered by the LEAM experiment are not signatures of hypervelocity cosmic dust particles, as expected, but are induced signatures of electrostatically charged and transported lunar fines.

Thematic maps in the scientific studies of the moon

2019 ◽  
Vol 943 (1) ◽  
pp. 68-75
Author(s):  
S.G. Pugacheva ◽  
E.A. Feoktistova ◽  
V.V. Shevchenko
Keyword(s):  
Natural Resources ◽  
Thermal Inertia ◽  
High Growth ◽  
Lunar Soil ◽  
Nature Management ◽  
The Moon ◽  
Surface Cooling ◽  
Laser Altimeters ◽  
Space Infrastructure ◽  
The Impact

The article presents the results of astrophysical studies of the Moon’s reflected and intrinsic radiation. We studied the intensity of the Moon’s infrared radiation and, thus, carried out a detailed research of the brightness temperature of the Moon’s visible disc, estimated the thermal inertia of the coating substance by the rate of its surface cooling, and the degree of the lunar soil fragmentation. Polarimetric, colorimetric and spectrophotometric measurements of the reflected radiation intensity were carried out at different wavelengths. In the article, we present maps prepared based on our measurement results. We conducted theresearch of the unique South Pole – Aitken basin (SPA). The altitude profiles of the Apollo-11 and Zond-8 spacecrafts and the data of laser altimeters of the Apollo-16 and Apollo-15 spacecrafts were used as the main material. Basing upon this data we prepared a hypsometric map of SPA-basing global relief structure. A surface topography map of the Moon’s Southern Hemisphere is given in the article. The topography model of the SPA topography surface shows displacement centers of the altitude topographic rims from the central rim. Basing upon the detailed study of the basin’s topography as well as its “depth-diameter” ratio we suggest that the basin originated from the impact of a giant cometary body from the Orta Cloud. In our works, we consider the Moon as a part of the Earth’s space infrastructure. High growth rates of the Earth’s population, irrational nature management will cause deterioration of scarce natural resources in the near future. In our article, we present maps of the natural resources on the Moon pointing out the most promising regions of thorium, iron, and titanium. Probably in 20 or 40 years a critical mining level of gold, diamonds, zinc, platinum and other vital rocks and metals will be missing on the Earth.

POSSIBILITIES OF STUDYING THE LUNAR SOIL AND COMPARING THE COMPOSITIONS OF LUNAR AND TERRESTRIAL CLINOPYROXENES

2021 ◽  
Vol 27 (7) ◽  
pp. 6-17
Author(s):  
Z. Golitsyna ◽  
◽  
A. Kirdyashkin ◽  
Keyword(s):  
Lunar Surface ◽  
Experimental Studies ◽  
Compositional Analysis ◽  
Lunar Soil ◽  
The Moon ◽  
Initial Composition ◽  
Basic Model ◽  
Lunar Rocks ◽  
Celestial Bodies ◽  
Temperature And Pressure

The problem of compositional analysis of extraterrestrial crystalline rocks in the study of celestial bodies is considered. Since most of the bodies, terrestrial planets and their surrounding objects may contain clinopyroxenes, it is possible to study the temperature and pressure of rock formation in certain areas according to the state of these minerals, and the studies can be carried out identically to the geothermobarometry of Earth rocks. The paper presents the results of experimental studies of clinopyroxene compositions of the basic model system CaO-MgO-Al2O3-SiO2 in the pressure range of 12...30 kbar and temperatures of 1325...1650 °C, which can be assumed as conditions for the formation of lunar rocks. The development of the necessary experimental data obtained in terrestrial conditions will help in the future to conduct remote studies of the Moon and other celestial bodies without the need to deliver soil to Earth. The revealed clinopyroxenes can be analyzed with existing geothermometers and geobarometers obtained for different ranges of P-T conditions. The possibility of creating a new geothermobarometer based on the distribution of minals or cations in clinopyroxene specifically for lunar rocks is not excluded. The main features and possible instrumentation of the apparatus intended for the study of the lunar surface are described. The study of different areas of the lunar surface will determine where the country rocks are located most closely to the surface. Analysis of silicate components of the lunar rocks will make it possible to get closer to the solution to the problem of initial composition of the lunar mantle

Depth of penetration of lubricant fluids and water in Queenston shale of southern Ontario

2017 ◽  
Vol 54 (2) ◽  
pp. 248-257 ◽  
Author(s):  
Hayder Mohammed Salim Al-Maamori ◽  
M. Hesham El Naggar ◽  
Silvana Micic
Keyword(s):  
Polymer Solution ◽  
Penetration Depth ◽  
Deformation Behaviour ◽  
Test Procedure ◽  
Time Dependent ◽  
Efficient Technique ◽  
Depth Of Penetration ◽  
Water Penetration ◽  
Southern Ontario ◽  
Rock Formation

Queenston shale is a rock formation located in southern Ontario in Canada that exhibits time-dependent deformation behaviour induced by water penetration. Microtunnelling is an efficient technique that can be used to construct pipelines and tunnels in Queenston shale. In this technique, lubricant fluids, such as bentonite solution and polymer solution, are utilized, which can have a significant impact on the time-dependant deformation (i.e., swelling) of Queenston shale within their depth of influence. A test procedure was developed in this research to investigate the depth of penetration of lubricant fluids and water in Queenston shale. These fluids were applied under pressure, similar to that used in the microtunnelling process, on Queeenston shale specimens. The depth of penetration of these fluids into the test specimens was monitored with time. It was concluded that the penetration depth varied for the various fluids considered. Water had the deepest penetration into Queenston shale. Based on the observed results, an equation is developed to predict the depth of penetration of various fluids in the Queenston shale mass. Results of this research can assist in evaluating the depth of influence of various fluids in Queenston shale and the associated swelling zone can be predicted.

Research of Formed Lunar Regholit Analog AGK-2010 / Badania wytworzonego analogu gruntu księżycowego AGK-2010

2013 ◽  
Vol 58 (2) ◽  
pp. 551-556
Author(s):  
Stanisław Bednarz ◽  
Mirosław Rzyczniak ◽  
Andrzej Gonet ◽  
Karol Seweryn
Keyword(s):  
Grain Size ◽  
Shear Strength ◽  
Oil And Gas ◽  
Lunar Regolith ◽  
Lunar Soil ◽  
Research Centre ◽  
Mechanical Parameters ◽  
The Moon ◽  
The Cost ◽  
Academy Of Sciences

The results investigations of a soil having similar properties as lunar regolith performed at the Department of Drilling and Geoengineering, Faculty of Drilling, Oil and Gas, AGH University of Science and Technology in Kraków are presented in this paper. The research was carried out jointly with the Space Research Centre, Polish Academy of Sciences in Warsaw. The objective of the cooperation was to minimize the cost of tests of penetrator KRET, which will be used on the surface of the Moon. The American lunar regolith (e.g. CHENOBI) was used as reference soil. The most important properties were presented graphically in the form of figures and tables: grain size distribution, selected physical properties (bulk density, colour), selected mechanical parameters (shear strength, inner friction strength, cohesion). As a result the first Polish lunar soil analog AGK-2010 was produced.

Microwave Thermal Radiation from the Moon

1949 ◽  
Vol 2 (1) ◽  
pp. 63 ◽  
Author(s):  
JH Piddington ◽  
HC Minnett
Keyword(s):  
Thermal Radiation ◽  
Phase Angle ◽  
Electromagnetic Waves ◽  
Lunar Phase ◽  
Phase Lag ◽  
The Moon ◽  
Average Temperature ◽  
Deep Interior ◽  
Subsurface Layers ◽  
New Moon

Measurements have been made of the thermal radiation from the moon in a 15 Mc/s. band, centred at 24,000 Mc/s. The radiation from the whole lunar disk has been measured during several phase cycles. Temperatures corresponding to this radiation have been deduced and curves of temperature against phase angle drawn. One of these corresponds to average temperature over the disk and the other to the temperature of a point on the lunar equator. They are found to be approximately sinusoidal, with amplitude � 40.3 �K, and � 52.0 �K. respectively and with a phase lag behind the lunar phase angle of about 45� in each case. These results conflict with previous measurements of temperature at long infra-red wavelengths in both amplitude and phase angle of the temperature curve. An explanation is given in terms of radiation from subsurface layers of the moon's crust, which are partially transparent to the electromagnetic waves with which we are dealing. The theory is developed quantitatively and it is found that the results are consistent with the existence of a thin layer of dust covering a solid lunar surface. Estimates are made of the temperatures of the disk of the new moon (156 �K.) and of the deep interior (241 �K.).

scholarly journals Penetration Depth of Closely Spaced Water-free Crevasses

1977 ◽  
Vol 18 (78) ◽  
pp. 37-46 ◽  
Author(s):  
J. Weertman
Keyword(s):  
Penetration Depth ◽  
Fracture Strength ◽  
Analytic Solution ◽  
Fluid Flows ◽  
Approximate Analytic Solution ◽  
Depth Of Penetration ◽  
Geothermal Heat ◽  
Cooling Fluid ◽  
Crack Problems ◽  
Secondary Cracking

AbstractAn approximate, analytic solution is found for the profile of a water-free crevasse in a field of closely spaced crevasses. The depth of penetration of the crevasses into the glacier is found. If the fracture strength of ice is taken to be zero, the penetration depth is equal to the value found by Nye and is independent of the crevasse spacing. This conclusion is in disagreement with results reported recently by R.A. Smith. If the fracture strength of ice is taken to be finite, the penetration depth is reduced if the spacing between crevasses is reduced.The results of the analysis can be applied to other crack problems. In particular, it can be applied to thermal, secondary cracking that it is hoped occurs when cooling fluid flows through the cracks created by hydraulic fracture for the purpose of extracting geothermal heat from hot, dry rock masses.

scholarly journals Influence of the Technology of Obtaining the Material of the Cathode of the Cu – Fe System at the Depth of Penetration of Ions into the Titanium Target

2022 ◽  
Author(s):  
V.V. Ovchinnikov
Keyword(s):  
Titanium Alloy ◽  
Powder Metallurgy ◽  
Penetration Depth ◽  
Depth Of Penetration ◽  
Titanium Target ◽  
Alloy Vt20

Abstract. The article presents the results of the influence of the technology of obtaining the material of the cathode of the implanter of the Cu – Fe system on the penetration depth of the titanium alloy VT20. It is shown that the use of 50% Cu – 50% Fe material as the material of the cathode of the implanter, obtained by alloying copper and iron, leads to a better increase in the thickness of the ion-doped layer than the use of the cathode obtained by powder metallurgy.

Quantitative Assessment of Penetration Depth in Clinical Ultrasound Systems

2007 ◽  
Author(s):  
Franco Marinozzi ◽  
Fabiano Bini ◽  
Federico Patane` ◽  
Daniele Piras
Keyword(s):  
Penetration Depth ◽  
Correlation Coefficient ◽  
Quantitative Assessment ◽  
Signal To Noise Ratio ◽  
Electronic Noise ◽  
Grey Level ◽  
Signal To Noise ◽  
Time And Space ◽  
Depth Of Penetration ◽  
Speckle Contrast

Most of the recent studies for image uniformity assessment involve signal to noise ratio (SNR) analysis computed over various combinations of mean grey level and variance [1–2] to quantify the speckle contrast and hence the depth of penetration (DOP). Speckle is auto correlated in time but not in space. Electronic noise always present at the bottom of the image, instead, is uncorrelated both in time and space. The extension of the area in which only the speckle is visible, gives an estimate of the penetration depth. The correlation coefficient of two subsequently acquired frames can be computed to quantify image uniformity where depth at which the correlation coefficient falls below a fixed threshold is defined as penetration depth.

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