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At least 145 records · Page 8Linked to original sources
USGS1972

Geologic map of the Fracastorius Quadrangle of the Moon

The multi-ringed Nectaris basin ( Hartmann and Kuiper, 1962) dominates the Fracastorius quadrangle. The basin is 840 km across as measured from the outermost ring and lies athwart four quadrangles. Frac astorius , the southeastern quadrangle , straddles the three rings of the basin (fig. 1 ). In this quadrangle most pre- Imbri an structures and many depositions were formed by the Nectaris impact. Furthermore, the emplacement of many younger deposi ts was controlled by basin structures and locally by probable multi-ring structures related to the Fecunditatis basin center ed northeast of the quadrangle. Other geologic features in the area include diverse mantling deposits and both primary impact craters and secondary impact craters produced by ejecta from distant impacts .

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USGS1972

Geologic map of the Taruntius Quadrangle of the Moon

The distribution of major physiographic provinces and geologic units of the Tarant ius quadrangle is determined by the five intersecting circular multi-ringed mare basin s. Three basins, i n probable order of decreasing age, are Tran quill itatis , Fecun ditatis , Serenitatis, Nectaris , and Crisiu m . The uplifted ring structures of the basin form terra mountains, peninsulas , and islands, and the depressions between the uplifts are the major deposition sites of post -basin terra and mare material.

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USGS1973

Geologic map of the Langrenus Quadrangle of the Moon

The Langrenus quadrangle is on the east limb of the lunar nearside, at the southeast margin of Mare Fecunditatis . The crater Lan grenus , about 140 km in diameter, is the most prominent feature. Rugged terra materials, scattered by craters of various sizes and ages, occupy much of the east half of the map area, and smooth mare materials in the Fecunditatis basin dominate the west. Mare Spumans and other irregular maria in the northeast are part of a belt of such maria concentric with Mare Crisium , which is centered approximately 500 km north of the quadrangle.

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USGS1973

Geologic map of the Grimaldi quadrangle of the Moon

The Grimaldi quadrangle lies at the southwest margin of Oceanus Procellarum about 1,000 km east of Orientale, the youngest o f the lunar multi-ringed basins. The distal ends of the ejecta blanket surrounding the Orient al e basin partly covers the western third of the quadrangle. The relatively small, two-ring Grimaldi basin is in the northwest corner of the quadrangle, and the Humorum basin l ies about 750 km to the southeast. A vestigial multi-ring basin mostly engulfed by mare appears to control the distribution of terra and mare along the southwest margin of Oceanus Procellarum ; the craters Hansteen and Billy are on a northwe s t-trending topographic high which represents part of the ring system of this basin. Terra materials of distinctive texture, apparently unrelated to multi-ring basins and probably of volcanic origin, occupy the central parts of the quadrangle.

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USGS1973

Geologic map of the Petavius quadrangle of the Moon

The large crater Petavius , about 180 km in diameter, is the dominant geologic feature within this quadrangle at the southeast border of Mare Fecunditatis on the east limb of the near side. Four categories of materials have been distinguished herein : (1) terrae, with r u gged to gently rolling topography and moderate albedo; (2) plains, of low relief and moderate albedo; (3) craters, with low to rugged relief and low to high albedo; (4) maria, with essentially no reli e f and very low to moderately low albedo. Materials are places in chronologic sequence according to stratigraphic position and(or) physical characteristics believed indicative of relative age. Development of the lunar time-stratigraphic nomenclature has been summarized by Wilhelms (1970).

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