By Frederick I. Ordway
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Extra resources for Advances in space science and technology. Volume 3
According to Nichols  pressure ridges are long sharp welts, many of which are broken by a central fissure. Pressure ridges of New Mexico are considered to have been caused by the collapse of a lava flow that was initially domical in cross section. The shortest ridge is 130 ft (40 meters) long but some pressure ridges are more than 1200 ft (366 meters) long. They are 10 to 25 ft (3 to 8 meters) high and as much as 100 ft (30 meters) wide. A pressure ridge south of Amboy crater area, California, appears to have been caused by tensional forces peculiar to the flow THE ROLE OF GEOLOGY IN LUNAR EXPLORATION 29 FIG.
According to information released 52 JACK GREEN AND JACK R. VAN LOPIK by the United States Geological Survey, coesite, the high pressure modification of quartz, was found by x-ray diffractometry in the strongly sheared Coconino sandstone from drillings in the floor of Meteor Crater. Coesite is extremely refractory and has been suggested as a suitable nosecone material. 3. WATER CONTENT OF POSSIBLE LUNAR SURFACE MATERIALS In the search for critical raw materials on the Moon, no single substance is as important as water.
The unit flow thickness in the Columbia Plateau of the northwestern United States is probably less than 50 ft (15 meters) ; in India, the average thickness of a basaltic flow is less than 60 ft (18 meters) ; in Iceland, the average flow is 13 to 30 ft (4 to 9 meters) thick. The area may be a few acres or many 40 JACK GREEN AND JACK R. VAN LOPIK square miles. In Iceland, single flows covering over 100 sq mile (259 sq km) are known, and one flow is said to cover 400 sq mile (1040 sq km). One of the paradoxes of volcanic phenomena is the diversity of products resulting from the consolidation of a megascopically uniform lava.
Advances in space science and technology. Volume 3 by Frederick I. Ordway