393:(â20°, 124°), partly exposed in the Michelangelo quadrangle, consists of one ring 660 km in diameter. The exact age of Beethoven is uncertain; the density of superposed primary impact craters suggests a post-Caloris, late c3 age, but it may be as old as early c2 age due to the large range of error in the crater age estimate. The ejecta from Beethoven are very extensive east and southeast of the basin rim and are mappable as far as 600 km downrange from the rim. However, ejecta appear to be almost absent on the west side of the basin. The reason for this asymmetry is unclear; possibly Beethoven is the result of an oblique impact that produced an asymmetric ejecta distribution (Gault and Wedekind, 1978), or possibly basin radial texture in the western rim area has been obliterated by ejecta from
39:
449:
craters within a morphologically defined sequence. Although these conditions hold generally, degradation may be accelerated locally by adjacent impact events and flooding by plains materials and, rarely, may be decelerated by structural rejuvenation of topographic elements of craters. Thus, the stratigraphic significance of crater morphology is only approximate. By analogy with lunar materials, all mapped crater materials are thought to be of impact origin. Only craters larger than 30 km in diameter are mapped.
27:
437:
are distributed regionally and have no obvious source for ballistic deposition; (2) large tracts are confined within basin depositional environments, analogous to the lunar maria; (3) indirect evidence elsewhere on
Mercury exists for volcanic modification of impact craters (Schultz, 1977); and (4) possible volcanic collapse craters are associated with plains-filled craters (â61°, 161° and â57°, 102°). Parts of smooth plains deposits may be a complex mix of overlapping crater ejecta.
2785:
2797:
483:
resemble lunar mare ridges and also are considered to be of tectonic origin. The mercurian ridges are probably related to minor compressive stresses that postdate smooth plains emplacement. Numerous lineaments are associated with basin rim material, but most of these lineaments are probably related to ejecta deposition. A few may be faults, particularly where they occur close to preexisting basin rings.
274:
craters and stratigraphic relations. These results are uncertain, as the crater density of heavily cratered terrain on
Mercury ranges from 11.2 to 17.4 Ă 10â5 km-2 for craters of diameters 20 km or greater (Guest and Gault, 1976). The results obtained are consistent with a qualitative assignment of relative age that is based on position and size of these ancient basins.
57:, where the imaged part is heavily cratered terrain that has been strongly influenced by the presence of multiring basins. At least four such basins, now nearly obliterated, have largely controlled the distribution of plains materials and structural trends in the map area. Many craters, interpreted to be of
453:
superposition relations do not exist. Results of these crater counts indicate that
Dostoevskij, presumed to be of c3 age (McCauley and others, 1981), is actually one of the oldest basins in the map area (early c1). Thus, strict morphological determination of stratigraphic age may be significantly in error.
503:
The
Caloris impact occurred during the time of formation of the intermediate plains material. In the map area, Caloris ejecta may be present at depth or may have been reworked locally by adjacent impacts. Two groups of Caloris secondary craters are evident. Shortly after the Caloris impact, extensive
436:
The origin of the younger plains materials is critical to mercurian geologic history. They are thought to be either volcanic or a facies of ballistic ejecta (Oberbeck and others, 1977). The interpretation favored here is that large parts of these smooth plains are of volcanic origin, because (1) they
356:
at â16°, 165° (Schaber and McCauley, 1980). It consists of three discontinuous rings; ejecta may be mapped as far as 350 km from the outermost ring. The density of superposed craters suggests an age older than the
Caloris Basin, either late c1 or early c2. A small unnamed basin at â48°, 136° may
515:
production continues to the present day on all units. If the geologic history of the Moon is a guide, most of the events discussed were essentially complete within the first 1.5 to 2.0 billion years of
Mercury's history (Murray and others, 1975). A summary of global mercurian geology may be found in
499:
rocks and possibly ancient volcanic flows. Deposition of the intercrater plains material was waning as the next oldest basins (Dostoevskij, Tolstoj) were formed. Partly overlapping their formation was the deposition of the intermediate plains material, probably emplaced partly as distal basin ejecta
456:
Throughout the map area are crater clusters and chains that are satellitic to both craters and basins, but the host crater may not be identifiable everywhere. This material is interpreted to be from secondary impact craters of a wide variety of ages. Many mercurian secondaries are well preserved and
319:
from adjacent large craters. In some areas, the intercrater plains material appears to embay c1 craters, and it is found in all of the degraded basins described above. The origin of mercurian intercrater plains material remains unknown. Both volcanic (Strom, 1977) and impact-debris models (Oberbeck
127:
Systematic mapping of the
Michelangelo quadrangle has revealed the presence of four nearly obliterated multiring basins. These basins are here named for unrelated superposed, named craters, as was done for highly degraded lunar basins (Wilhelms and El-Baz, 1977). From oldest to youngest, the basins
491:
The interpretable geologic history of the
Michelangelo quadrangle begins with the formation of the four ancient, multiring basins. From oldest to youngest, they are: Barma-Vincente, Bartok-Ives, Hawthorne-Riemenschneider, and Eitoku-Milton. These basins presumably formed during the period of heavy
477:
is an example. These lobate ridges appear to be of compressive tectonic origin and, although global in distribution, may be deflected locally by the presence of preexisting, basin-related structure. Additional effects of these ancient basin rings may be seen where the rim of
Dostoevskij intersects
805:
Prepared for the
National Aeronautics and Space Administration by the U.S. Department of the Interior, U.S. Geological Survey. Published in hardcopy as USGS Miscellaneous Investigations Series Map Iâ1659, as part of the Atlas of Mercury, 1:5,000,000 Geologic Series. Hardcopy is available for sale
482:
at â40°, 174°); parts of the Dostoevskij rim appear to have been structurally accented by this intersection. These relations are similar to those associated with highly degraded, ancient basins on Mars (Chicarro and others, 1983). The smooth plains material displays numerous ridges that generally
452:
The large basins of the Michelangelo quadrangle have been dated relatively by counting the cumulative density of superposed primary impact craters that have diameters greater than 20 km. This technique has proven to be of great value in dating lunar basins (Wilhelms, in press), where obvious
420:
The oldest of the three younger plains units is intermediate plains material. It forms planar to gently undulating surfaces and both embays tracts of cratered terrain and fills crater floors. Both upper and lower contacts with other plains units are gradational. These gradations suggest that the
273:
Because none of the four basins has ejecta deposits that are preserved, the basins are assumed to be the oldest features in the map area; moreover, they are embayed or buried by all other units. The figures for the relative ages of the basins are based on the density of superposed primary impact
76:
may correspond to similar materials at â30° to â40°, 90° to 100°. The color data (orange/ultraviolet) presented in Hapke and others (1980) likewise show no particular correlation with mapped terrain types. The "yellow" region (moderately high orange/ultraviolet) centered at â33°, 155° appears to
448:
Crater deposits are mapped stratigraphically according to a morphologic degradation sequence devised by N. J. Trask (McCauley and others, 1981). This method assumes that (1) all craters of a given size range initially resemble fresh craters and (2) degrees of impact erosion are constant for all
368:
on the map area are not immediately apparent. No Caloris ejecta are evident, and most structural trends appear to be unrelated to this impact. However, near the west border of the map are two groups of large, overlapping craters centered at â31°, 183° and â49°, 182°. These groups appear to have
277:
The basins have largely controlled subsequent geologic processes in the map area. Large concentrations of smooth plains deposits are found within the basin boundaries and at the intersections of rings of different basins. Moreover, the trends of scarp segments, interpreted by some workers to be
314:
The oldest recognizable plains unit in the map area is the intercrater plains material, originally described by Trask and Guest. This material is generally undulating to hummocky and appears to underlie tracts of cratered terrain, as evidenced by the superposition of many coalescing
492:
bombardment inferred from lunar history (Wilhelms, in press). Contemporaneous with their formation and shortly afterward, was the deposition of the intercrater plains material. This unit has a complex history of deposition; it was reworked in place and probably includes
504:
smooth plains material, probably of volcanic origin, was deposited. During this period of deposition occurred the impacts of the last of the major basins (Beethoven, Michelangelo, Valmiki, and Bach). Minor tectonic activity continued as scarps and lunar mare-type
908:
______The geologic history of the Moon: U.S Geological Survey Professional Paper 1348 (in press). Wilhelms, D. E., and El-Baz, Farouk, 1977, Geologic map of the east side of the Moon: U.S. Geological Survey Miscellaneous Investigations Series Map I-948, scale
849:
Murray, B. C., Belton, M. J. S., Danielson, G. E., Davies, M. E., Gault, D. E., Hapke, Bruce, O'Leary, Brian, Strom, R. G., Suomi, Verner, and Trask, N. J., 1974, Mercury's surface: Preliminary description and interpretation from Mariner 10 pictures:
424:
The smooth plains unit forms both widespread regional deposits and crater floor material. The regional deposits are significantly less cratered than those of other plains units, although they typically display crater densities comparable to older
61:, display a spectrum of modification styles and degradation states. The interaction between basins, craters, and plains in this quadrangle provides important clues to geologic processes that have formed the morphology of the mercurian surface.
344:
occur southeast of the rim. Although Dostoevskij was considered a type example of a c3 large crater (McCauley and others, 1981), crater counts indicate that it is much older. The Dostoevskij impact probably occurred in c1 time.
377:
secondaries (Schultz, 1976; Wilhelms, 1976b; Eggleton, 1981), these crater groups are interpreted to be Caloris Basin secondaries. Following the terminology developed by McCauley and others (1981) we have assigned them to the
457:
have sharp, unrounded rims. This morphology is probably a consequence of the stronger mercurian gravity, relative to the Moon, that produces higher impact velocities for crater ejecta on the mercurian surface (Scott, 1977).
820:
Dzurisin, Daniel, 1978, The tectonic and volcanic history of Mercury as inferred from studies of scarps, ridges, troughs, and other lineaments: Journal of Geophysical Research, v. 83, no. B10, p. 4883â4906.
282:
associated with global compression (Dzurisin, 1978), are deflected into basin-concentric patterns at their intersection with basin rings. These relations have also been noted for ancient basins on both the
816:
Chicarro, Augustin, Schultz, P. H., and Masson, Philippe, 1983, Basin control of ridge patterns on Mars: Abstracts of papers submitted to the Lunar and Planetary Science Conference, 14th, Houston, 1983,
298:, is also evident at â37°, 125°. It is unique among the two-ring basins in the map area because, although the inner ring is well preserved and similar in morphology to peak rings of fresh basins such as
823:
Eggleton, R. E., 1981, Map of the impact geology of the Imbrium basin of the Moon, in Geology of the Apollo 16 areaâCentral Lunar Highlands: U.S. Geological Survey Professional Paper 1048, pl. 12.
843:
Hapke, Bruce, Christman, Craig, Rava, Barry, and Mosher, Joel, 1980, A color-ratio map of Mercury: Lunar and Planetary Science Conference, 11th, Houston, 1980, Proceedings, v. 1, p. 817â821.
421:
assignment of age to plains deposits on Mercury is partly dependent on the relative abundance of superposed secondary craters, whose densities vary widely as a function of nearby source craters.
306:
and is suggestive of an extended period of structural rejuvenation along the margins of the inner ring. Crater density on this basin suggests that it is one of the oldest in the map area
213:
871:
Schaber, G. G., and McCauley, J.F., 1980, Geologic map of the Tolstoj quadrangle of Mercury: U.S. Geological Survey Miscellaneous Investigations Series Map I-1199, scale 1:5,000,000.
369:
formed simultaneously, as no specific stratigraphic sequence is evident. On the basis of crater clusters of similar appearance in the lunar highlands, which have been interpreted as
826:
Gault, D. E., and Wedekind, J. A., 1978, Experimental studies of oblique impact: Lunar and Planetary Science Conference, 9th, Houston, 1978, Proceedings, v. 3, p. 3843â 3875.
3981:
382:, Secondary-Crater Facies. These secondaries overlie Dostoevskij ejecta and thus confirm that basin as pre-Caloris. We determined a reference crater density for Caloris in the
846:
McCauley, J. F., Guest, J. E., Schaber, G. G., Trask, N. J., and Greeley, Ronald, 1981, Stratigraphy of the Caloris Basin, Mercury: Icarus, v. 47, no. 2, p. 184â202.
465:
The rings associated with the four ancient basins are the oldest structures within the mapped area and have to some degree controlled the structural trends of subsequent
440:
A very smooth plains unit occurs only as floor material in younger c4 and c5 craters. The material is interpreted to be crater impact melt and associated clastic debris.
320:
and others, 1977) have been proposed. The material is most likely polygenetic, including both crater and basin debris and possibly ancient volcanic flows. Physically and
332:
At least seven basins in or partly in the Michelangelo quadrangle postdate or are contemporaneous with the last stages of deposition of intercrater plains material.
164:
237:
91:) adjacent to the west is included in the map area because not enough Mariner 10 data were acquired of this quadrangle to justify the production of another map.
3421:
470:
189:
87:
cover scattered areas in the quadrangle; these photographs were used to supplement the geologic interpretation. About 10° of longitude of the H-13 quadrangle (
68:
features are evident in Earth-based views of the Michelangelo quadrangle, but these features do not appear to correlate directly with any mapped terrain unit.
500:
and partly as volcanic flows. Regional deformation of these plains units by compressive tectonics, forming scarps, was contemporaneous with their deposition.
3431:
2834:
4084:
394:
905:
Wilhelms, D. E., 1976b, Secondary impact craters of lunar basins: Lunar Science Conference, 7th, Houston, 1976, Proceedings, v. 3, p. 2883â2901.
864:
Oberbeck, V. R., Quaide, W. L., Arvidson, R. E., and Aggarwal, H. R., 1977, Comparative studies of lunar, martian, and mercurian craters and plains:
3867:
3720:
735:
Gault, D. E.; Guest, J. E.; Murray, J. B.; Dzurisin, D.; Malin, M. C. (1975). "Some comparisons of impact craters on Mercury and the Moon".
266:
that appear to protrude through superposed materials; (2) arcuate segments of ridges (rupes) aligned with massif material; and (3) arcuate
4008:
934:
3649:
857:
Murray, B. C., Strom, R. G., Trask, N. J., and Gault, D. E., 1975, Surface history of Mercury: Implications for terrestrial planets:
412:. All contain two rings and appear to be transitional between large craters and multiring basins. All postdate the Caloris event.
3888:
2827:
3827:
3074:
2663:
987:
4000:
3727:
3155:
592:
567:
3992:
2820:
977:
797:
541:
83:
data include complete photographic coverage of the quadrangle at a resolution of about 2 km. In addition, twelve
4021:
3775:
3642:
3628:
884:
Schultz, P. H, Schultz, R. A., and Rogers, John, 1982, The structure and evolution of ancient impact basins on Mars:
4074:
4027:
4013:
3700:
3612:
3591:
3012:
3677:
2900:
357:
also have formed in this time interval, but its age is uncertain due to its partial burial by ejecta from crater
3186:
2843:
2595:
2489:
1018:
1008:
927:
3670:
3663:
3577:
3507:
3235:
3220:
3193:
3095:
3024:
2962:
2888:
1326:
88:
3895:
3881:
3691:
3563:
3314:
2938:
2912:
2862:
2645:
2615:
2509:
2484:
1649:
1569:
3987:
3817:
3684:
2988:
2950:
2876:
1549:
992:
954:
3603:
2089:
3970:
3067:
3000:
2974:
2926:
2094:
1889:
1336:
2139:
336:(â44°, 176°) displays only one ring; presumably the inner peak ring is buried by plains material. The
302:, the outer ring is almost totally obliterated. This morphology is similar to that of the lunar basin
2788:
1354:
920:
1449:
3038:
2590:
2494:
2514:
3806:
3162:
2744:
2234:
3243:
1644:
3811:
3636:
3330:
3275:
3228:
2895:
2677:
2044:
1081:
383:
77:
correspond to a smooth plains deposit, but the region overlaps into adjacent cratered terrain.
20:
2149:
806:
from U.S. Geological Survey, Information Services, Box 25286, Federal Center, Denver, CO 80225
4079:
4040:
3944:
3924:
3874:
3500:
3475:
3389:
3148:
3060:
2419:
2244:
2239:
2174:
2034:
1829:
1634:
1579:
1409:
1389:
982:
469:. Several of the lobate ridges described by Strom follow arcuate patterns along rings of the
401:
2534:
3656:
3438:
3340:
3261:
3200:
3180:
3019:
2957:
2883:
2544:
2524:
2424:
2309:
1989:
1749:
1629:
1594:
1474:
1444:
1439:
1086:
1051:
1031:
709:
333:
111:
103:
2299:
1394:
1283:
1132:
829:
Guest, J. E., and Gault, D. E., 1976, Crater populations in the early history of Mercury:
8:
3919:
3459:
3452:
2933:
2907:
2857:
2800:
2632:
2504:
2404:
2399:
2279:
2249:
2204:
2084:
1784:
1684:
1554:
1469:
1429:
1359:
1096:
1056:
1036:
3796:
3514:
2269:
2069:
1624:
713:
405:
4032:
3791:
3771:
3570:
3445:
3396:
3320:
2983:
2945:
2871:
2764:
2640:
2585:
2559:
2479:
2444:
2414:
2409:
2159:
2129:
2029:
1944:
1934:
1919:
1914:
1824:
1724:
1714:
1664:
1619:
1544:
1514:
1504:
1379:
1374:
1349:
1321:
1091:
1061:
1041:
898:
Strom, R. G., 1977, Origin and relative age of lunar and mercurian intercrater plains:
613:
Strom, R. G.; Trask, N. J.; Guest, J. E. (1975). "Tectonism and volcanism on Mercury".
379:
358:
353:
107:
69:
3522:
1599:
1484:
874:
Schultz, P. H., 1976, Moon morphology: Austin, Tex., University of Texas Press, 626 p.
38:
3268:
2995:
2969:
2921:
2796:
2379:
2304:
2229:
2169:
2124:
2119:
2109:
2104:
2049:
1954:
1949:
1909:
1844:
1814:
1809:
1799:
1779:
1739:
1699:
1679:
1604:
1564:
1539:
1464:
1152:
1137:
1076:
1066:
1046:
891:
Scott, D. H., 1977, Moon-Mercury: Relative preservation states of secondary craters:
721:
686:
588:
563:
303:
99:
2209:
1494:
340:
from this basin may be mapped as far as 450 km from the rim; several secondary
3954:
3929:
3711:
3403:
3347:
2549:
2529:
2439:
2389:
2384:
2369:
2354:
2344:
2324:
2319:
2259:
2224:
2219:
2214:
2189:
2179:
2164:
2134:
2099:
2079:
2019:
2014:
1999:
1969:
1964:
1959:
1899:
1834:
1819:
1794:
1789:
1769:
1754:
1734:
1729:
1704:
1669:
1614:
1609:
1574:
1534:
1499:
1424:
1419:
1384:
1369:
1278:
1268:
1248:
1215:
1210:
1182:
1167:
1147:
943:
774:
744:
717:
682:
652:
622:
316:
295:
54:
643:
Trask, N. J.; Guest, J. E. (1975). "Preliminary geologic terrain map of Mercury".
3975:
3939:
3934:
3801:
3767:
3382:
3033:
2519:
2474:
2469:
2454:
2449:
2434:
2429:
2359:
2339:
2334:
2289:
2264:
2254:
2194:
2184:
2074:
2004:
1984:
1939:
1904:
1859:
1854:
1849:
1839:
1774:
1764:
1719:
1674:
1659:
1654:
1639:
1559:
1529:
1524:
1479:
1404:
1344:
1316:
1311:
1263:
1253:
1225:
1220:
1172:
1162:
1026:
700:
Trask, N. J.; Strom, R. G. (1976). "Additional evidence of mercurian volcanism".
479:
390:
374:
95:
73:
836:
Guest, J. E., and O'Donnell, W. P., 1977, Surface history of Mercury: A review:
511:
The cratering rate declined rapidly as the c3, c4 and c5 craters were produced.
3949:
3624:
3466:
3140:
2564:
2554:
2539:
2499:
2464:
2459:
2349:
2329:
2314:
2294:
2284:
2274:
2199:
2154:
2144:
2114:
2064:
2059:
2054:
2039:
2009:
1979:
1974:
1929:
1924:
1884:
1874:
1864:
1759:
1744:
1709:
1694:
1589:
1584:
1519:
1489:
1454:
1434:
1414:
1399:
1364:
1288:
1205:
1200:
1114:
321:
26:
4068:
3482:
3368:
2569:
2374:
2364:
2024:
1994:
1894:
1879:
1689:
1459:
1306:
1230:
1157:
1142:
505:
430:
409:
370:
365:
349:
299:
279:
58:
748:
656:
626:
72:
may correspond to a deposit of plains materials centered at â58°, 135°, and
3307:
3083:
2394:
1869:
1804:
1509:
1258:
1177:
341:
84:
429:(Murray and others, 1974). The unit characteristically contains mare-type
262:
The presence of these basins is indicated by three criteria: (1) isolated
3375:
3361:
3354:
3300:
2812:
2710:
426:
3584:
2695:
1273:
778:
474:
267:
80:
42:
3822:
2769:
2727:
2703:
466:
294:
In addition to the four multiring basins, an ancient two-ring basin,
31:
3902:
2655:
587:. National Aeronautics and Space Administration. pp. 114â115.
512:
496:
583:
Davies, M. E.; Dwornik, S. E.; Gault, D. E.; Strom, R. G. (1978).
558:
Davies, M. E.; Dwornik, S. E.; Gault, D. E.; Strom, R. G. (1978).
877:
______1977, Endogenic modification of impact craters on Mercury:
493:
798:"Geologic Map Of The Michaelangelo (H-12) Quadrangle Of Mercury"
542:"Geologic Map Of The Michaelangelo (H-12) Quadrangle Of Mercury"
3982:
Lives of the Most Excellent Painters, Sculptors, and Architects
3052:
337:
263:
65:
765:
Strom, R. G. (1979). "Mercury: A post-Mariner 10 assessment".
433:, although no flow fronts have been observed in the map area.
386:
in order to correlate basin ages to that stratigraphic datum.
562:. National Aeronautics and Space Administration. p. 15.
288:
284:
912:
673:
Wilhelms, D. E. (1976). "Mercurian volcanism questioned".
734:
582:
557:
291:(Schultz and others, 1982; Chicarro and others, 1983).
795:
539:
98:
is south of Michelangelo quadrangle. To the west is
4066:
3868:Study of a Kneeling Nude Girl for The Entombment
3849:
612:
324:it resembles the lunar highlands megaregolith.
668:
666:
508:developed within the smooth plains materials.
3068:
2828:
928:
900:Physics of the Earth and Planetary Interiors
893:Physics of the Earth and Planetary Interiors
879:Physics of the Earth and Planetary Interiors
53:is in the southern hemisphere of the planet
760:
758:
663:
638:
636:
608:
606:
604:
478:the Barma-Vincente rings (for example, the
415:
4009:Restoration of the Sistine Chapel frescoes
3075:
3061:
2842:
2835:
2821:
935:
921:
796:Spudis, Paul D.; James G. Prosser (1984).
699:
642:
540:Spudis, Paul D.; James G. Prosser (1984).
327:
122:
4085:Surface features of Mercury by quadrangle
3650:The Creation of the Sun, Moon, and Plants
535:
533:
531:
529:
309:
30:Michelangelo quadrangle as mapped by the
755:
728:
693:
672:
633:
601:
37:
25:
400:The other basins in the quadrangle are
4067:
3828:Santa Maria degli Angeli e dei Martiri
526:
516:Guest and O'Donnell (1977) and Strom.
270:aligned with both massifs and ridges.
3848:
3749:
3544:
3115:
3056:
3017:
3005:
2993:
2981:
2955:
2943:
2931:
2905:
2893:
2881:
2869:
2816:
916:
764:
3432:Giuliano de' Medici, Duke of Nemours
854:, v. 185, no. 4146, p. 169â179.
902:, v. 15, nos. 2â3, p. 156â172.
895:, v. 15, nos. 2â3, p. 173â178.
888:, v. 87, no. 12, p. 9803â9820.
881:, v. 15, nos. 2â3, p. 202â219.
868:, v. 82, no. 11, p. 1681â1698.
861:, v. 80, no. 17, p. 2508â2514.
486:
443:
13:
14:
4096:
3643:Separation of Light from Darkness
4015:The Titan: Story of Michelangelo
3750:
3082:
2795:
2784:
2783:
886:Journal of Geophysical Research
866:Journal of Geophysical Research
859:Journal of Geophysical Research
833:, v. 3, no. 3, p. 121â123.
810:
737:Journal of Geophysical Research
645:Journal of Geophysical Research
615:Journal of Geophysical Research
117:
3721:The Crucifixion of Saint Peter
3116:
576:
551:
1:
3545:
3128:
1327:Skinakas (hypothetical basin)
597:. Special Publication SP-423.
572:. Special Publication SP-423.
519:
89:Solitudo Persephones Province
3882:Studies for the Libyan Sibyl
3850:Works on paper, milieu, etc.
3564:The Torment of Saint Anthony
2616:Hypothetical moon of Mercury
831:Geophysical Research Letters
722:10.1016/0019-1035(76)90129-9
687:10.1016/0019-1035(76)90128-7
460:
7:
3988:Michelangelo and the Medici
3818:San Giovanni dei Fiorentini
942:
10:
4101:
3971:Art patronage of Julius II
3896:PietĂ for Vittoria Colonna
2664:Mercury-crossing asteroids
789:
110:, and to the northeast is
18:
4023:The Agony and the Ecstasy
3963:
3912:
3859:
3855:
3844:
3784:
3760:
3756:
3745:
3710:
3623:
3602:
3555:
3551:
3540:
3492:
3422:Christ Carrying the Cross
3413:
3329:
3253:
3212:
3172:
3126:
3122:
3111:
3090:
3031:
2967:
2919:
2855:
2850:
2778:
2757:
2737:
2720:
2685:
2676:
2654:
2631:
2624:
2608:
2578:
1335:
1297:
1239:
1191:
1123:
1105:
1017:
1001:
970:
963:
950:
840:, v. 20, p. 273â300.
214:Hawthorne-Riemenschneider
141:
136:
133:
3889:The Punishment of Tityus
416:Younger plains materials
19:Not to be confused with
4075:Michelangelo quadrangle
4046:Michelangelo quadrangle
3776:Basilica of San Lorenzo
2745:Colonization of Mercury
749:10.1029/jb080i017p02444
657:10.1029/jb080i017p02461
627:10.1029/jb080i017p02478
328:Younger basin materials
123:Ancient basin materials
106:. To the northwest is
51:Michelangelo quadrangle
3797:Piazza del Campidoglio
3728:The Conversion of Saul
3604:Salone dei Cinquecento
3276:Piccolomini Altarpiece
3156:Battle of the Centaurs
2844:Quadrangles on Mercury
384:Shakespeare quadrangle
310:Older plains materials
46:
35:
21:Piazza del Campidoglio
4041:Michelangelo (crater)
3945:Sebastiano del Piombo
3925:Tommaso dei Cavalieri
3875:Male Back with a Flag
3390:The Genius of Victory
3149:Madonna of the Stairs
2090:Kuan Han-Chʻing
767:Space Science Reviews
102:, and to the east is
41:
29:
16:Quadrangle on Mercury
3807:St. Peter's Basilica
3657:The Creation of Adam
3181:Arca di San Domenico
2140:Li Chʻing-Chao
471:Barma-Vincente Basin
287:(Schultz, 1976) and
142:Ring diameters (km)
112:Beethoven quadrangle
104:Discovery quadrangle
3920:Cecchino dei Bracci
3414:Florence, 1516â1534
3254:Florence, 1501â1505
2596:Inter-crater plains
838:Vistas in Astronomy
714:1976Icar...28..559T
364:The effects of the
352:is centered in the
4034:A Season of Giants
4017:(1950 documentary)
3792:Capitoline Museums
3772:Laurentian Library
3571:Manchester Madonna
3321:Rothschild Bronzes
3173:Bologna, 1494â1495
779:10.1007/bf00221842
380:Van Eyck Formation
354:Tolstoj quadrangle
108:Tolstoj quadrangle
70:Solitudo Promethei
47:
36:
4062:
4061:
4058:
4057:
4054:
4053:
3840:
3839:
3836:
3835:
3741:
3740:
3737:
3736:
3701:The Last Judgment
3629:(ceiling gallery)
3613:Battle of Cascina
3592:Leda and the Swan
3536:
3535:
3532:
3531:
3331:Tomb of Julius II
3274:Additions to the
3269:Madonna of Bruges
3179:Additions to the
3050:
3049:
3045:
3044:
2810:
2809:
2753:
2752:
2672:
2671:
2604:
2603:
1650:ChĆng ChʼĆl
1645:Chiang Kʻui
1284:Santa MarĂa Rupes
1153:Mearcair Planitia
1138:Borealis Planitia
1133:ApÄrangi Planitia
743:(17): 2444â2460.
651:(17): 2461â2477.
621:(17): 2478â2507.
594:978-1-114-27448-8
569:978-1-114-27448-8
260:
259:
100:Neruda quadrangle
4092:
4001:Replicas of the
3955:Luigi del Riccio
3930:Vittoria Colonna
3857:
3856:
3846:
3845:
3758:
3757:
3747:
3746:
3678:Prophet Jeremiah
3553:
3552:
3542:
3541:
3515:Palestrina PietĂ
3508:Florentine PietĂ
3348:Rebellious Slave
3133:
3132: 1488â1492
3130:
3124:
3123:
3113:
3112:
3077:
3070:
3063:
3054:
3053:
2853:
2852:
2837:
2830:
2823:
2814:
2813:
2799:
2787:
2786:
2683:
2682:
2629:
2628:
2150:Liang Kʻai
1355:Africanus Horton
1279:Resolution Rupes
1269:Enterprise Rupes
1249:Antoniadi Dorsum
1216:Goldstone Vallis
1211:Goldstone Catena
1183:Utaridi Planitia
1168:Stilbon Planitia
1148:Caloris Planitia
968:
967:
937:
930:
923:
914:
913:
817:p. 105â106.
804:
802:
783:
782:
762:
753:
752:
732:
726:
725:
697:
691:
690:
670:
661:
660:
640:
631:
630:
610:
599:
598:
585:Atlas of Mercury
580:
574:
573:
560:Atlas of Mercury
555:
549:
548:
546:
537:
487:Geologic history
444:Crater materials
131:
130:
4100:
4099:
4095:
4094:
4093:
4091:
4090:
4089:
4065:
4064:
4063:
4050:
3976:Casa Buonarroti
3959:
3940:Gherardo Perini
3935:Ascanio Condivi
3908:
3851:
3832:
3812:Tor San Michele
3802:Palazzo Farnese
3780:
3752:
3733:
3706:
3627:
3619:
3598:
3556:Panel paintings
3547:
3528:
3523:Rondanini PietĂ
3493:Rome, 1534â1564
3488:
3409:
3383:Awakening Slave
3325:
3249:
3213:Rome, 1496â1500
3208:
3187:Saint Petronius
3168:
3131:
3118:
3107:
3086:
3081:
3051:
3046:
3036:
3022:
3010:
2998:
2986:
2972:
2960:
2948:
2936:
2924:
2910:
2898:
2886:
2874:
2860:
2846:
2841:
2811:
2806:
2774:
2749:
2733:
2716:
2687:
2668:
2650:
2620:
2600:
2574:
2495:Sholem Aleichem
1331:
1322:Rembrandt Basin
1317:Raditladi Basin
1312:Pantheon Fossae
1299:
1293:
1264:Discovery Rupes
1254:Adventure Rupes
1241:
1235:
1226:Haystack Vallis
1221:Haystack Catena
1193:
1187:
1173:Suisei Planitia
1163:Sobkou Planitia
1125:
1119:
1107:
1101:
1013:
997:
978:Albedo features
959:
946:
941:
813:
800:
792:
787:
786:
763:
756:
733:
729:
698:
694:
671:
664:
641:
634:
611:
602:
595:
581:
577:
570:
556:
552:
544:
538:
527:
522:
489:
463:
446:
418:
391:Beethoven Basin
375:Orientale basin
330:
312:
278:expressions of
138:
125:
120:
96:Bach quadrangle
74:Solitudo Martis
24:
17:
12:
11:
5:
4098:
4088:
4087:
4082:
4077:
4060:
4059:
4056:
4055:
4052:
4051:
4049:
4048:
4043:
4038:
4036:(1990 TV film)
4030:
4019:
4011:
4006:
3998:
3990:
3985:
3978:
3973:
3967:
3965:
3961:
3960:
3958:
3957:
3952:
3950:Febo di Poggio
3947:
3942:
3937:
3932:
3927:
3922:
3916:
3914:
3910:
3909:
3907:
3906:
3899:
3892:
3885:
3878:
3871:
3863:
3861:
3860:Works on paper
3853:
3852:
3842:
3841:
3838:
3837:
3834:
3833:
3831:
3830:
3825:
3820:
3815:
3809:
3804:
3799:
3794:
3788:
3786:
3782:
3781:
3779:
3778:
3764:
3762:
3754:
3753:
3743:
3742:
3739:
3738:
3735:
3734:
3732:
3731:
3724:
3716:
3714:
3712:Pauline Chapel
3708:
3707:
3705:
3704:
3697:
3696:
3695:
3688:
3681:
3674:
3671:Prophet Isaiah
3667:
3664:Prophet Daniel
3660:
3653:
3646:
3633:
3631:
3625:Sistine Chapel
3621:
3620:
3618:
3617:
3608:
3606:
3600:
3599:
3597:
3596:
3588:
3581:
3578:The Entombment
3574:
3567:
3559:
3557:
3549:
3548:
3538:
3537:
3534:
3533:
3530:
3529:
3527:
3526:
3519:
3511:
3504:
3496:
3494:
3490:
3489:
3487:
3486:
3479:
3472:
3471:
3470:
3467:Medici Madonna
3463:
3456:
3449:
3442:
3435:
3427:Medici Chapel
3425:
3417:
3415:
3411:
3410:
3408:
3407:
3400:
3393:
3386:
3379:
3372:
3365:
3358:
3351:
3344:
3336:
3334:
3327:
3326:
3324:
3323:
3318:
3311:
3304:
3297:
3296:
3295:
3272:
3265:
3257:
3255:
3251:
3250:
3248:
3247:
3240:
3236:Standing Cupid
3232:
3225:
3221:Sleeping Cupid
3216:
3214:
3210:
3209:
3207:
3206:
3205:
3204:
3197:
3194:Saint Proculus
3190:
3176:
3174:
3170:
3169:
3167:
3166:
3159:
3152:
3145:
3141:Head of a Faun
3136:
3134:
3120:
3119:
3109:
3108:
3106:
3105:
3102:
3099:
3091:
3088:
3087:
3080:
3079:
3072:
3065:
3057:
3048:
3047:
3043:
3042:
3029:
3028:
3016:
3004:
2992:
2979:
2978:
2966:
2954:
2942:
2930:
2917:
2916:
2904:
2892:
2880:
2867:
2866:
2851:
2848:
2847:
2840:
2839:
2832:
2825:
2817:
2808:
2807:
2805:
2804:
2792:
2779:
2776:
2775:
2773:
2772:
2767:
2761:
2759:
2755:
2754:
2751:
2750:
2748:
2747:
2741:
2739:
2735:
2734:
2732:
2731:
2724:
2722:
2718:
2717:
2715:
2714:
2713:(2018âpresent)
2708:
2700:
2691:
2689:
2680:
2674:
2673:
2670:
2669:
2667:
2666:
2660:
2658:
2652:
2651:
2649:
2648:
2643:
2637:
2635:
2626:
2622:
2621:
2619:
2618:
2612:
2610:
2606:
2605:
2602:
2601:
2599:
2598:
2593:
2588:
2582:
2580:
2576:
2575:
2573:
2572:
2567:
2562:
2557:
2552:
2547:
2542:
2537:
2532:
2527:
2522:
2517:
2512:
2507:
2502:
2497:
2492:
2487:
2482:
2477:
2472:
2467:
2462:
2457:
2452:
2447:
2442:
2437:
2432:
2427:
2422:
2417:
2412:
2407:
2402:
2397:
2392:
2387:
2382:
2377:
2372:
2367:
2362:
2357:
2352:
2347:
2342:
2337:
2332:
2327:
2322:
2317:
2312:
2307:
2302:
2297:
2292:
2287:
2282:
2277:
2272:
2267:
2262:
2257:
2252:
2247:
2242:
2237:
2232:
2227:
2222:
2217:
2212:
2207:
2202:
2197:
2192:
2187:
2182:
2177:
2172:
2167:
2162:
2157:
2152:
2147:
2142:
2137:
2132:
2127:
2122:
2117:
2112:
2107:
2102:
2097:
2092:
2087:
2082:
2077:
2072:
2067:
2062:
2057:
2052:
2047:
2042:
2037:
2032:
2027:
2022:
2017:
2012:
2007:
2002:
1997:
1992:
1987:
1982:
1977:
1972:
1967:
1962:
1957:
1952:
1947:
1942:
1937:
1932:
1927:
1922:
1917:
1912:
1907:
1902:
1897:
1892:
1890:Guido d'Arezzo
1887:
1882:
1877:
1872:
1867:
1862:
1857:
1852:
1847:
1842:
1837:
1832:
1827:
1822:
1817:
1812:
1807:
1802:
1797:
1792:
1787:
1782:
1777:
1772:
1767:
1762:
1757:
1752:
1747:
1742:
1737:
1732:
1727:
1722:
1717:
1712:
1707:
1702:
1697:
1692:
1687:
1682:
1677:
1672:
1667:
1662:
1657:
1652:
1647:
1642:
1637:
1632:
1627:
1622:
1617:
1612:
1607:
1602:
1597:
1592:
1587:
1582:
1577:
1572:
1567:
1562:
1557:
1552:
1547:
1542:
1537:
1532:
1527:
1522:
1517:
1512:
1507:
1502:
1497:
1492:
1487:
1482:
1477:
1472:
1467:
1462:
1457:
1452:
1447:
1442:
1437:
1432:
1427:
1422:
1417:
1412:
1407:
1402:
1397:
1392:
1387:
1382:
1377:
1372:
1367:
1362:
1357:
1352:
1347:
1341:
1339:
1333:
1332:
1330:
1329:
1324:
1319:
1314:
1309:
1303:
1301:
1295:
1294:
1292:
1291:
1289:Victoria Rupes
1286:
1281:
1276:
1271:
1266:
1261:
1256:
1251:
1245:
1243:
1237:
1236:
1234:
1233:
1228:
1223:
1218:
1213:
1208:
1206:Arecibo Vallis
1203:
1201:Arecibo Catena
1197:
1195:
1189:
1188:
1186:
1185:
1180:
1175:
1170:
1165:
1160:
1155:
1150:
1145:
1140:
1135:
1129:
1127:
1121:
1120:
1118:
1117:
1115:Caloris Montes
1111:
1109:
1103:
1102:
1100:
1099:
1094:
1089:
1084:
1079:
1074:
1069:
1064:
1059:
1054:
1049:
1044:
1039:
1034:
1029:
1023:
1021:
1015:
1014:
1012:
1011:
1005:
1003:
999:
998:
996:
995:
993:Magnetic field
990:
985:
980:
974:
972:
965:
961:
960:
958:
957:
951:
948:
947:
940:
939:
932:
925:
917:
911:
910:
906:
903:
896:
889:
882:
875:
872:
869:
862:
855:
847:
844:
841:
834:
827:
824:
821:
818:
812:
809:
808:
807:
791:
788:
785:
784:
754:
727:
708:(4): 559â563.
692:
681:(4): 551â558.
662:
632:
600:
593:
575:
568:
550:
524:
523:
521:
518:
506:wrinkle ridges
488:
485:
462:
459:
445:
442:
417:
414:
366:Caloris impact
361:(â44°, 129°).
329:
326:
322:lithologically
311:
308:
258:
257:
255:
252:
249:
246:
243:
240:
234:
233:
231:
228:
225:
222:
219:
216:
210:
209:
207:
204:
201:
198:
195:
192:
186:
185:
182:
179:
176:
173:
170:
167:
165:Barma-Vincente
161:
160:
157:
154:
151:
148:
144:
143:
140:
135:
124:
121:
119:
116:
15:
9:
6:
4:
3:
2:
4097:
4086:
4083:
4081:
4078:
4076:
4073:
4072:
4070:
4047:
4044:
4042:
4039:
4037:
4035:
4031:
4029:
4026:
4024:
4020:
4018:
4016:
4012:
4010:
4007:
4005:
4004:
3999:
3997:
3996:
3991:
3989:
3986:
3984:
3983:
3979:
3977:
3974:
3972:
3969:
3968:
3966:
3962:
3956:
3953:
3951:
3948:
3946:
3943:
3941:
3938:
3936:
3933:
3931:
3928:
3926:
3923:
3921:
3918:
3917:
3915:
3911:
3905:
3904:
3900:
3898:
3897:
3893:
3891:
3890:
3886:
3884:
3883:
3879:
3877:
3876:
3872:
3870:
3869:
3865:
3864:
3862:
3858:
3854:
3847:
3843:
3829:
3826:
3824:
3821:
3819:
3816:
3813:
3810:
3808:
3805:
3803:
3800:
3798:
3795:
3793:
3790:
3789:
3787:
3783:
3777:
3773:
3769:
3766:
3765:
3763:
3759:
3755:
3748:
3744:
3730:
3729:
3725:
3723:
3722:
3718:
3717:
3715:
3713:
3709:
3703:
3702:
3698:
3694:
3693:
3692:Prophet Jonah
3689:
3687:
3686:
3682:
3680:
3679:
3675:
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3483:Crouching Boy
3480:
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3369:Bearded Slave
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3315:Saint Matthew
3312:
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3098:
3097:
3096:List of works
3093:
3092:
3089:
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3073:
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2597:
2594:
2592:
2591:Ghost craters
2589:
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2048:
2046:
2045:Judah Ha-Levi
2043:
2041:
2038:
2036:
2033:
2031:
2028:
2026:
2023:
2021:
2018:
2016:
2013:
2011:
2008:
2006:
2003:
2001:
1998:
1996:
1993:
1991:
1988:
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1983:
1981:
1978:
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1973:
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1968:
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1328:
1325:
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1307:Caloris Basin
1305:
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1282:
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1231:Simeiz Vallis
1229:
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1214:
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1199:
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1184:
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1159:
1158:Odin Planitia
1156:
1154:
1151:
1149:
1146:
1144:
1143:Budh Planitia
1141:
1139:
1136:
1134:
1131:
1130:
1128:
1122:
1116:
1113:
1112:
1110:
1106:Mountains and
1104:
1098:
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1088:
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989:
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746:
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696:
688:
684:
680:
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669:
667:
658:
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650:
646:
639:
637:
628:
624:
620:
616:
609:
607:
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596:
590:
586:
579:
571:
565:
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536:
534:
532:
530:
525:
517:
514:
509:
507:
501:
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484:
481:
476:
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468:
458:
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450:
441:
438:
434:
432:
428:
422:
413:
411:
407:
403:
398:
396:
392:
387:
385:
381:
376:
372:
367:
362:
360:
355:
351:
350:Tolstoj Basin
346:
343:
342:crater chains
339:
335:
325:
323:
318:
307:
305:
301:
297:
292:
290:
286:
281:
280:thrust faults
275:
271:
269:
265:
256:
253:
250:
247:
244:
241:
239:
238:Eitoku-Milton
236:
235:
232:
229:
226:
223:
220:
217:
215:
212:
211:
208:
205:
202:
199:
196:
193:
191:
188:
187:
183:
180:
177:
174:
171:
168:
166:
163:
162:
158:
155:
152:
149:
146:
145:
132:
129:
115:
113:
109:
105:
101:
97:
92:
90:
86:
82:
78:
75:
71:
67:
62:
60:
59:impact origin
56:
52:
44:
40:
33:
28:
22:
4080:Michelangelo
4045:
4033:
4025:(1961 novel,
4022:
4014:
4002:
3994:
3993:Replicas of
3980:
3901:
3894:
3887:
3880:
3873:
3866:
3768:New Sacristy
3751:Architecture
3726:
3719:
3699:
3690:
3685:Prophet Joel
3683:
3676:
3669:
3662:
3655:
3648:
3641:
3611:
3590:
3583:
3576:
3569:
3562:
3521:
3513:
3506:
3499:
3481:
3474:
3465:
3458:
3451:
3444:
3437:
3430:
3420:
3402:
3395:
3388:
3381:
3374:
3367:
3360:
3353:
3346:
3339:
3313:
3308:Taddei Tondo
3306:
3299:
3292:
3288:
3284:
3281:Saints Peter
3280:
3267:
3260:
3242:
3234:
3227:
3219:
3199:
3192:
3185:
3161:
3154:
3147:
3139:
3101:â» attributed
3094:
3084:Michelangelo
3008:Michelangelo
3007:
2794:
2782:
2702:
2694:
2515:SveinsdĂłttir
2420:Rachmaninoff
2245:Michelangelo
2240:Mendes Pinto
2175:Ma Chih-Yuan
1830:Gainsborough
1635:Chao Meng-Fu
1580:Brunelleschi
1410:Amru Al-Qays
1390:Al-Hamadhani
1259:Beagle Rupes
1178:Tir Planitia
1072:Michelangelo
1071:
899:
892:
885:
878:
865:
858:
851:
837:
830:
811:Bibliography
770:
766:
740:
736:
730:
705:
701:
695:
678:
674:
648:
644:
618:
614:
584:
578:
559:
553:
510:
502:
490:
464:
455:
451:
447:
439:
435:
423:
419:
402:Michelangelo
399:
388:
363:
347:
331:
313:
293:
276:
272:
261:
139:(lat, long)
126:
118:Stratigraphy
93:
79:
64:Several low-
63:
50:
48:
3376:Atlas Slave
3362:Young Slave
3355:Dying Slave
3333:, 1505â1545
3301:Pitti Tondo
2896:Shakespeare
2711:BepiColombo
2707:(2004â2015)
2699:(1973â1975)
2678:Exploration
2545:Villa-Lobos
2525:To Ngoc Van
2490:Shakespeare
2425:Raden Saleh
2310:Mussorgskij
1990:Hovnatanian
1750:Dostoevskij
1630:Chaikovskij
1595:Callicrates
1475:Baranauskas
1445:Aristoxenes
1440:Apollodorus
1192:Canyons and
1082:Shakespeare
1019:Quadrangles
1009:Quadrangles
909:1:5,000,000
773:(1): 3â70.
427:lunar maria
334:Dostoevskij
317:secondaries
242:â23°, 170°
218:â56°, 105°
194:â33°, 115°
190:Bartok-Ives
169:â52°, 162°
85:stereopairs
45:photomosaic
4069:Categories
4028:1965 film)
3585:Doni Tondo
3127:Florence,
3117:Sculptures
2696:Mariner 10
2505:Stravinsky
2405:Praxiteles
2400:Polygnotus
2280:Monteverdi
2250:Mickiewicz
2205:Mark Twain
1785:Enheduanna
1685:Cunningham
1555:Botticelli
1470:Balanchine
1430:Anguissola
1360:Ahmad Baba
1298:Basins and
1274:Hero Rupes
1240:Ridges and
1124:Plains and
983:Atmosphere
520:References
494:brecciated
475:Hero Rupes
81:Mariner 10
43:Mariner 10
34:spacecraft
3823:Porta Pia
3546:Paintings
3020:Discovery
2958:Beethoven
2884:Raditladi
2770:Sub-Earth
2728:Mercury-P
2704:MESSENGER
2656:Asteroids
2625:Astronomy
2560:Xiao Zhao
2535:VelĂĄzquez
2480:Scarlatti
2445:Rembrandt
2430:Raditladi
2415:Qi Baishi
2410:Prokofiev
2160:Lovecraft
2130:Lermontov
2030:Izquierdo
1945:Hiroshige
1935:Hemingway
1920:Hawthorne
1915:Hauptmann
1825:Futabatei
1725:Derzhavin
1715:Delacroix
1665:Coleridge
1620:Cervantes
1545:Boccaccio
1515:Belinskij
1505:Beethoven
1450:AĆvaghoáčŁa
1380:Al-Akhtal
1375:Akutagawa
1350:Abu Nuwas
1108:volcanoes
1087:Raditladi
1052:Discovery
1032:Beethoven
964:Geography
467:tectonism
461:Structure
359:Delacroix
32:MESSENGER
3903:Epifania
3761:Florence
3163:Crucifix
3039:features
3025:features
3013:features
3001:features
2989:features
2975:features
2963:features
2951:features
2939:features
2934:Eminescu
2927:features
2913:features
2908:Victoria
2901:features
2889:features
2877:features
2863:features
2858:Borealis
2789:Category
2738:See also
2721:Proposed
2688:and past
2633:Transits
2510:Sullivan
2485:Schubert
2380:Petrarch
2305:Murasaki
2300:MunkĂĄcsy
2230:Melville
2170:Lysippus
2125:Leopardi
2120:Larrocha
2110:Kurosawa
2105:Kunisada
2050:Kalidasa
1955:Hodgkins
1950:Hitomaro
1910:Harunobu
1845:Ghiberti
1815:Flaubert
1810:Firdousi
1800:Faulkner
1780:Eminescu
1740:Dominici
1700:De Graft
1680:Couperin
1605:Carducci
1565:Bramante
1550:Boethius
1540:Bjornson
1465:Balagtas
1395:Al-JÄhiz
1126:plateaus
1097:Victoria
1057:Eminescu
1037:Borealis
988:Features
513:Regolith
497:plutonic
304:Grimaldi
3964:Related
3774:in the
3637:Ceiling
3293:Gregory
3229:Bacchus
2984:Debussy
2946:Tolstoj
2872:Hokusai
2765:Fiction
2758:Related
2730:(~2031)
2686:Current
2586:Geology
2550:Vivaldi
2530:Tolstoj
2440:Raphael
2390:Picasso
2385:Phidias
2370:Oskison
2355:Neumann
2345:Nureyev
2325:Nampeyo
2320:Nabokov
2270:MoliĂšre
2260:Mistral
2225:Matisse
2220:Matabei
2215:Martial
2190:Mansart
2180:Machaut
2165:Lu Hsun
2135:Lessing
2100:Kulthum
2080:Kipling
2070:Kertész
2035:JanĂĄÄek
2020:Imhotep
2015:Ictinus
2000:Hun Kal
1970:Holberg
1965:Holbein
1960:Hokusai
1900:Han Kan
1835:Gauguin
1820:Flaiano
1795:Equiano
1790:Enwonwu
1770:Eastman
1755:Dowland
1735:Dickens
1730:Desprez
1705:Debussy
1670:Copland
1625:CĂ©zanne
1615:Calvino
1610:Carolan
1575:Bruegel
1535:Bernini
1500:Beckett
1425:Angelou
1420:Aneirin
1385:Alencar
1370:Aksakov
1337:Craters
1194:valleys
1092:Tolstoj
1062:Hokusai
1042:Debussy
1002:Regions
971:General
955:Outline
944:Mercury
852:Science
790:Sources
710:Bibcode
406:Valmiki
395:Valmiki
371:Imbrium
296:Surikov
264:massifs
156:Fourth
150:Second
55:Mercury
3913:Milieu
3501:Brutus
3476:Apollo
3397:Rachel
2996:Neruda
2970:Kuiper
2922:Derain
2801:Portal
2520:Titian
2475:Sander
2470:Rudaki
2455:Rivera
2450:Renoir
2435:Rameau
2360:Nizami
2340:Neruda
2335:Nawahi
2290:Mozart
2265:Mofolo
2255:Milton
2195:Mansur
2185:Mahler
2095:Kuiper
2075:Khansa
2005:Hurley
1985:Horace
1940:Hesiod
1905:Handel
1870:Goethe
1860:Glinka
1855:Giotto
1850:Gibran
1840:Geddes
1775:Eitoku
1765:Dvorak
1720:Derain
1675:Copley
1660:Chu Ta
1655:Chopin
1640:Chekov
1600:CamÔes
1570:Brontë
1560:Brahms
1530:Berkel
1525:Benoit
1485:BartĂłk
1480:Balzac
1405:Amaral
1345:Abedin
1300:fossae
1077:Neruda
1067:Kuiper
1047:Derain
702:Icarus
675:Icarus
591:
566:
431:ridges
408:, and
338:ejecta
268:scarps
159:Fifth
153:Third
147:Inner
137:Center
66:albedo
4003:PietĂ
3995:David
3439:Night
3341:Moses
3262:David
3244:PietĂ
3201:Angel
3104:â lost
3032:H-15
3018:H-11
3006:H-12
2994:H-13
2982:H-14
2920:H-10
2641:Earth
2609:Moons
2579:Other
2565:Yeats
2555:Vyasa
2540:Verdi
2500:Sinan
2465:Rodin
2460:Rizal
2350:Nervo
2330:Navoi
2315:Myron
2295:Munch
2285:Moody
2275:Monet
2210:MartĂ
2200:March
2155:Liszt
2145:Li Po
2115:Lange
2085:KĆshĆ
2065:Kenko
2060:Keats
2055:Karsh
2040:Jokai
2010:Ibsen
1980:Homer
1975:Holst
1930:Heine
1925:Haydn
1885:Grieg
1875:Gogol
1865:Gluck
1760:Durer
1745:Donne
1710:Degas
1695:Dario
1590:Byron
1585:Burns
1520:Bello
1495:BashĆ
1490:Barma
1455:Atget
1435:Anyte
1415:Andal
1400:Alver
1365:Ailey
1242:rupes
801:(PDF)
545:(PDF)
480:horst
254:1180
230:1050
206:1500
203:1175
184:1700
181:1250
134:Name
128:are:
3785:Rome
3770:and
3460:Dawn
3453:Dusk
3404:Leah
3291:and
3289:Pius
3285:Paul
3034:Bach
2968:H-6
2956:H-7
2944:H-8
2932:H-9
2906:H-2
2894:H-3
2882:H-4
2870:H-5
2856:H-1
2646:Mars
2570:Zola
2375:Ovid
2365:Okyo
2235:Mena
2025:Ives
1995:Hugo
1895:Hals
1880:Goya
1690:Dali
1460:Bach
1027:Bach
589:ISBN
564:ISBN
410:Bach
389:The
373:and
348:The
300:Bach
289:Mars
285:Moon
251:850
248:590
245:280
227:780
224:500
221:270
200:790
197:480
178:950
175:725
172:360
94:The
49:The
3446:Day
2395:Poe
1805:Fet
1510:Bek
775:doi
745:doi
718:doi
683:doi
653:doi
623:doi
4071::
3287:,
3283:,
3129:c.
3041:)
3027:)
3015:)
3003:)
2991:)
2977:)
2965:)
2953:)
2941:)
2929:)
2915:)
2903:)
2891:)
2879:)
2865:)
771:24
769:.
757:^
741:80
739:.
716:.
706:28
704:.
679:28
677:.
665:^
649:80
647:.
635:^
619:80
617:.
603:^
528:^
473:;
404:,
397:.
114:.
3814:â»
3616:â
3595:â
3518:â»
3239:â
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781:.
777::
751:.
747::
724:.
720::
712::
689:.
685::
659:.
655::
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625::
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23:.
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