233:
tessera terrain. During the first phase, the thrust faults and fold belts started to develop parallel to the margins. At the beginning of the first phase, these faults and folds made an impact on the tessera terrain, but later on it made an impact on the intratessera volcanic plains. On second phase, all the thrust faults and fold belts experienced a perpendicular extension. Furthermore, the last phase occurred when the extensional events continuously carried out the deformed structures from the plateau and affecting the volcanic units.
164:
recognition from SAR images. The folds observed in this part of the Regio are concentric, associated with plunges, and share a common axis that is trending in an east–west fashion. Another feature that is observed in this part is ribbons structures. Ribbons can be described as structures that are steep with long depression of about 1–3 km in width and shallow depths of less than 500 m. In contrast to the folding structures, the ribbons in the western part are randomly distributed.
199:
127:
2183:
207:
2193:
24:
253:. However, this model needs a lot amount of time of crustal thickening (1–4 billion years). There are also a few constraints for this model. The first one is that this model provides no explanation for the contractional structures and the second one is that the timing of the extensional structures does not correlate well with the known cross-cutting relationships.
279:
because the mantle underneath the lava ponds are depleted with residual melts as compared to the neighboring undepleted mantle. However, there are a few issues accompanying this model. The first issue is that scientists are not confident that meteor impacts have the capabilities to melt a significant
265:
and volcanic activities associated with the thin lithosphere. Planetary scientists that support this model identify two categories of extensional structures: long-narrow graben, referred to as a ribbons, and more widely spaced graben. The sequence of formation for these structures is still debatable.
186:
In the eastern part of Ovda, the structural setting is defined mainly by wide folds and ribbons structures. The wide folds are observed to have amplitudes up to 25 km and several hundred km in length. While the ribbons structures generally hold a radial pattern. Some of the ribbons structures on
232:
There are generally two different phases of structural evolution that describe the Regio's crustal plateau margins. The initial phase preceded the first phase and the last phase concluded the second phase. The initial phase was when all the material being set in place, which would then construct the
163:
Folds and a distinct compositional layering generally characterize the western part of Ovda Regio. Compositional layering means that the structural layers differ from each other in terms of their chemical compositions. In particular, the layers are differentiated based on their tone and textural
113:
chasmata to the south. The crustal plateau serves as a place to hold the localized tessera terrains in the planet, which makes up roughly 8% of Venus' surface area. The kinematic evolution of crustal plateaus on Venus has been a debated topic in the planetary science community. Understanding its
219:
Regionally, there are two separate phases of tectonic evolution. Initially, the Regio was at a stable state where there are no stresses acting on the crustal plateaus. This state was then followed by the first phase in which the north–south-oriented compressional stresses acted on the Regio and
150:
to find insight into the Regio's deformation and formation mechanisms. The challenge in this process is to find the ideal temporal and spatial relationships, which hold a prominent role in comprehending the tectonic processes. In terms of structural setting, the Regio is characterized mainly by
280:
portion of the planet's lithosphere and generate enough magma that would cause isostasy. The second issue is the planet's large folds need a high amount of stresses to pass the thin brittle layer, but the underlying magma is not capable of transferring enough stresses through the layer.
177:
stack and duplex formation on the southern margin. A more detailed analysis was conducted in this part indicate that central Ovda hosts a strike-slip tectonic regime where the deformation is accompanied by three different structures: folds, normal faults, and strike-slip faults.
172:
Central Ovda is distinguishable by ridges exhibiting east–west orientations similar to those of western Ovda. These ridges are common on the northern margin and often share a common axis with the fold structures. Other structural features observed in this part of Ovda are
187:
this part of Ovda are quite difficult to interpret due to the SAR images' limited resolution. A good number of grabens are also present in this part, although the grabens are not highly distinguishable and are limited to fold crests.
220:
produced an east–west folding pattern. This pattern provides the primary structural framework in Ovda Regio. Then, the second phase took place in which the compressional stresses intensified and developed significant mega
274:
Under the impact model, the crustal plateaus were formed by lava ponds from mantle melting due to meteor impacts to the planet's thin lithosphere. Based on this model, the crustal plateaus would be uplifted by
249:
This model describes that the mantle downwelling flow assisted the development of crustal thickening and shortening of the ductile crust because of compression and accretion of thin
574:"Tectonic and kinematic study of a strike-slip zone along the southern margin of Central Ovda Regio, Venus: Geodynamical implications for crustal plateaux formation and evolution"
266:
Some scientists believe that the ribbons were formed first, followed later on by the wide spaced graben. But there are other scientists who believe the reverse sequence.
142:(SAR) images from the NASA Magellan mission have been analyzed to recognize the distribution of its structural features. The distribution was then mapped to find its
358:
Kucinskas, Algis B.; Turcotte, Donald L.; Huang, Jie; Ford, Peter G. (25 August 1992). "Fractal
Analysis of Venus Topography in Tinatin Planitia and Ovda Regio".
313:
Ghent, Rebecca; Hansen, Vicki (6 January 1999). "Structural and
Kinematic Analysis of Eastern Ovda Regio, Venus: Implications for Crustal Plateau Formation".
537:
Hansen, Vicki L.; Willis, James J. (April 1998). "Ribbon
Terrain Formation, Southwestern Fortuna Tessera, Venus: Implications for Lithosphere Evolution".
2048:
710:
Bindschadler, Duane L.; Schubert, Gerald; Kaula, William M. (25 August 1992). "Coldspots and hotspots: Global tectonics and mantle dynamics of Venus".
97:, the regio covers an area of approximately 15,000,000 square kilometres (5,800,000 sq mi) and is bounded by regional plains to the north,
469:
Chetty, T.R.K.; Venkatrayudu, M.; Venkatasivappa, V. (24 May 2010). "Structural
Architecture and a New Tectonic Perspective of Ovda Regio, Venus".
110:
106:
1611:
430:
195:
There are a few ideas being continuously discussed in the planetary science community regarding the tectonic evolution of Ovda Regio:
640:
Romeo, I.; Capote, R. (13 June 2011). "Tectonic evolution of Ovda Regio: An example of highly deformed continental crust on Venus?".
2053:
2038:
130:
This 3D view depicts the border between the lowland plains on the right and the crustal plateau region of Ovda Regio on the left
1673:
573:
261:
This second model describes the upwelling of a mantle flow (plume) that accommodates the formation of crustal thickening by
1649:
1289:
1284:
1256:
1251:
972:
967:
241:
There are several models that have been debated to explain crustal plateau formation in Venus, particularly in Ovda Regio:
114:
complex evolution is expected to contribute to a better knowledge of the geodynamic history of Venus. It is named after a
2113:
2217:
914:
788:"Geologic constraints on crustal plateau surface theories, Venus: the lava pond and bolide impact hypothesis"
787:
210:
The tectonic evolution at the crustal plateau's margins of Ovda Regio. Modified from Romeo and Capote, 2010.
2108:
2086:
2168:
2163:
1536:
1465:
1430:
866:
335:
1891:
1337:
1241:
957:
400:
139:
2033:
1950:
1415:
1057:
1025:
675:
Kidder, J.G.; Phillips, R.J. (1996). "Convection-driven subsolidus crustal thickening on Venus".
2058:
2043:
1490:
1450:
861:
330:
745:
Hansen, Vicki L.; Phillips, Roger J.; Willis, James J.; Ghent, Rebecca R. (25 February 2000).
2092:
2081:
1973:
1917:
1885:
1880:
1631:
1626:
1621:
1616:
1606:
1601:
1206:
1176:
262:
653:
482:
93:
that stretches from 10°N to 15°S and 50°E to 110°E. Known as the largest crustal plateau in
2007:
1924:
1526:
1510:
853:
802:
758:
719:
684:
649:
588:
546:
478:
438:
367:
322:
838:
8:
2196:
1931:
1470:
1405:
962:
907:
394:
857:
806:
762:
723:
688:
592:
550:
371:
326:
1475:
1420:
1410:
1390:
1264:
1156:
1063:
508:
135:
28:
The red rectangle shows the approximate location of Ovda Regio on the western part of
2192:
2158:
2017:
1721:
1716:
1711:
1688:
1505:
1495:
1440:
1435:
1400:
2143:
2138:
1693:
1593:
1573:
1531:
1370:
1365:
1191:
977:
934:
871:
810:
766:
727:
692:
657:
604:
596:
554:
486:
375:
340:
147:
1091:
1833:
1731:
1583:
1455:
1445:
1425:
1395:
1380:
1360:
1355:
1350:
1345:
1033:
600:
202:
The regional tectonic evolution at Ovda Regio. Modified from Chetty et al., 2010.
90:
29:
2186:
1578:
1500:
1485:
1375:
1302:
1297:
1274:
1269:
1211:
1171:
1151:
1101:
1086:
900:
206:
661:
490:
2211:
2153:
1956:
1659:
1460:
1385:
1317:
1307:
1161:
1141:
1121:
1005:
198:
98:
2063:
1899:
1868:
1654:
1327:
1322:
1196:
1181:
1111:
1096:
1038:
839:"Impacts do not initiate volcanic eruptions: Eruptions close to the crater"
558:
344:
102:
1980:
1312:
1236:
1186:
1136:
1126:
1076:
1071:
1000:
815:
771:
746:
250:
115:
65:
126:
1860:
1786:
1761:
1546:
1541:
1231:
1226:
1221:
1201:
1131:
1081:
1043:
1010:
221:
731:
696:
572:
Romeo, Ignacio; Capote, Ramon; Anguita, Francisco (10 February 2005).
379:
2133:
1943:
1853:
1846:
1839:
1826:
1821:
1816:
1811:
1806:
1801:
1796:
1751:
1736:
1726:
1166:
1146:
1116:
1106:
875:
174:
2148:
2012:
2002:
1791:
1781:
1776:
1771:
1766:
1756:
1746:
1741:
1706:
1641:
1216:
276:
1997:
1480:
86:
82:
468:
1937:
1909:
1904:
1873:
1700:
152:
509:"Structural Analysis of Central and Eastern Ovda Regio, Venus"
923:
94:
78:
23:
143:
747:"Structures in tessera terrain, Venus: Issues and answers"
357:
744:
709:
892:
118:
forest spirit that can appear as both male and female.
134:
Extensive research has been conducted to describe the
571:
2209:
227:
214:
674:
908:
536:
639:
312:
915:
901:
836:
22:
865:
814:
770:
334:
712:Journal of Geophysical Research: Planets
635:
633:
631:
629:
627:
625:
502:
500:
464:
462:
460:
458:
456:
392:
205:
197:
125:
738:
506:
413:
308:
306:
304:
302:
2210:
830:
785:
779:
668:
565:
530:
236:
190:
896:
786:Hansen, Vicki L. (22 November 2006).
703:
622:
497:
453:
121:
422:
299:
244:
518:. Lunar and Planetary Science XXVII
428:
351:
13:
256:
89:in the western highland region of
14:
2229:
837:Ivanov, M.A.; Head, H.J. (2003).
151:ribbons, folds, and a complex of
2191:
2182:
2181:
795:Journal of Geophysical Research
751:Journal of Geophysical Research
677:Journal of Geophysical Research
396:Mythology of All Races Volume 4
360:Journal of Geophysical Research
269:
181:
167:
158:
407:
386:
290:
49:10°N to 15°S and 50°E to 110°E
1:
516:Lunar and Planetary Institute
296:Dimensions are 6000 × 2500 km
283:
601:10.1016/j.icarus.2004.11.007
228:Marginal kinematic evolution
215:Regional kinematic evolution
57:15,000,000 square kilometres
7:
2114:Artificial objects on Venus
2109:Geological mapping of Venus
642:Planetary and Space Science
471:Planetary and Space Science
10:
2234:
507:Ghent, R.R.; Hansen, V.L.
2218:Surface features of Venus
2177:
2164:Neith (hypothetical moon)
2126:
2101:
2072:
2026:
1990:
1965:
1681:
1672:
1640:
1592:
1566:
1559:
1519:
1336:
1283:
1250:
1056:
1024:
993:
986:
950:
943:
930:
922:
662:10.1016/j.pss.2011.05.013
491:10.1016/j.pss.2010.05.010
414:McLeish, Kenneth (1996).
61:
53:
45:
37:
21:
1892:Pioneer Venus Multiprobe
1242:List of coronae on Venus
140:Synthetic aperture radar
2034:European Venus Explorer
1650:Venus-crosser asteroids
718:(E8): 13, 495–13, 532.
654:2011P&SS...59.1428R
483:2010P&SS...58.1286C
1894: / Pioneer 13
1888: / Pioneer 12
559:10.1006/icar.1998.5897
393:Holmberg, Uno (1927).
345:10.1006/icar.1999.6085
211:
203:
131:
1886:Pioneer Venus Orbiter
1207:Scalloped margin dome
1177:Quetzalpetlatl Corona
263:magmatic underplating
209:
201:
129:
816:10.1029/2006je002714
772:10.1029/1999JE001137
683:(E10): 23181–23294.
858:2003Geo....31..869I
807:2006JGRE..11111010H
763:2000JGR...105.4135H
724:1992JGR....9713495B
689:1996JGR...10123181K
593:2005Icar..175..320R
551:1998Icar..132..321H
372:1992JGR....9713635K
366:(E8): 13635–13641.
327:1999Icar..139..116G
237:Dynamic development
191:Kinematic evolution
18:
1265:Guinevere Planitia
1157:Nightingale Corona
435:Trinity University
429:Kroeger, Glenn C.
416:Dictionary of Myth
212:
204:
136:structural geology
132:
122:Structural geology
16:
2205:
2204:
2122:
2121:
2018:Venus Life Finder
1689:Sputnik programme
1668:
1667:
1555:
1554:
1052:
1051:
757:(E2): 4135–4152.
732:10.1029/92JE01165
697:10.1029/96JE02530
648:(13): 1428–1445.
477:(10): 1286–1297.
441:on 8 October 2015
431:"Exploring Earth"
380:10.1029/92JE01132
245:Downwelling model
105:to the east, and
85:located near the
72:
71:
2225:
2195:
2185:
2184:
2087:Inspiration Mars
1679:
1678:
1564:
1563:
1537:Surface features
1192:Sacajawea Patera
991:
990:
978:Mapping of Venus
948:
947:
935:Outline of Venus
917:
910:
903:
894:
893:
887:
886:
884:
882:
876:10.1130/g19669.1
869:
843:
834:
828:
827:
825:
823:
818:
792:
783:
777:
776:
774:
742:
736:
735:
707:
701:
700:
672:
666:
665:
637:
620:
619:
617:
615:
610:on 27 April 2015
609:
603:. Archived from
578:
569:
563:
562:
534:
528:
527:
525:
523:
513:
504:
495:
494:
466:
451:
450:
448:
446:
437:. Archived from
426:
420:
419:
411:
405:
404:
390:
384:
383:
355:
349:
348:
338:
310:
297:
294:
148:spatial relation
26:
19:
15:
2233:
2232:
2228:
2227:
2226:
2224:
2223:
2222:
2208:
2207:
2206:
2201:
2173:
2118:
2097:
2074:
2068:
2022:
1986:
1961:
1932:Cassini–Huygens
1834:Mariner program
1664:
1636:
1588:
1551:
1515:
1332:
1288:
1279:
1255:
1246:
1062:
1060:
1048:
1034:Aphrodite Terra
1020:
982:
939:
926:
921:
891:
890:
880:
878:
867:10.1.1.142.1430
852:(10): 869–872.
841:
835:
831:
821:
819:
801:(E11): E11010.
790:
784:
780:
743:
739:
708:
704:
673:
669:
638:
623:
613:
611:
607:
576:
570:
566:
535:
531:
521:
519:
511:
505:
498:
467:
454:
444:
442:
427:
423:
412:
408:
391:
387:
356:
352:
336:10.1.1.124.2964
311:
300:
295:
291:
286:
272:
259:
257:Upwelling model
247:
239:
230:
217:
193:
184:
170:
161:
138:of Ovda Regio.
124:
91:Aphrodite Terra
33:
30:Aphrodite Terra
12:
11:
5:
2231:
2221:
2220:
2203:
2202:
2200:
2199:
2189:
2178:
2175:
2174:
2172:
2171:
2166:
2161:
2156:
2151:
2146:
2141:
2136:
2130:
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2028:
2024:
2023:
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2015:
2010:
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1994:
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1468:
1463:
1458:
1453:
1448:
1443:
1438:
1433:
1428:
1423:
1418:
1416:Goeppert-Mayer
1413:
1408:
1403:
1398:
1393:
1388:
1383:
1378:
1373:
1368:
1363:
1358:
1353:
1348:
1342:
1340:
1334:
1333:
1331:
1330:
1325:
1320:
1315:
1310:
1305:
1303:Artemis Chasma
1300:
1298:Aikhulu Chasma
1294:
1292:
1281:
1280:
1278:
1277:
1275:Sedna Planitia
1272:
1270:Lakshmi Planum
1267:
1261:
1259:
1248:
1247:
1245:
1244:
1239:
1234:
1229:
1224:
1219:
1214:
1212:Siddons Patera
1209:
1204:
1199:
1194:
1189:
1184:
1179:
1174:
1172:Pavlova Corona
1169:
1164:
1159:
1154:
1152:Maxwell Montes
1149:
1144:
1139:
1134:
1129:
1124:
1119:
1114:
1109:
1104:
1102:Ciuacoatl Mons
1099:
1094:
1089:
1087:Artemis Corona
1084:
1079:
1074:
1068:
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1054:
1053:
1050:
1049:
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1036:
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1021:
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920:
919:
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905:
897:
889:
888:
829:
778:
737:
702:
667:
621:
587:(2): 320–334.
564:
545:(2): 321–343.
529:
496:
452:
421:
406:
385:
350:
321:(1): 116–136.
298:
288:
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34:
27:
9:
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3:
2:
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2110:
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2100:
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2019:
2016:
2014:
2011:
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2001:
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1996:
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1989:
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1957:Venus Express
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1881:Pioneer Venus
1879:
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1656:
1655:Venus trojans
1653:
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1451:Maria Celeste
1449:
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1329:
1326:
1324:
1321:
1319:
1318:Devana Chasma
1316:
1314:
1311:
1309:
1308:Baltis Vallis
1306:
1304:
1301:
1299:
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1162:Onatah Corona
1160:
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1143:
1142:Jaszai Patera
1140:
1138:
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1130:
1128:
1125:
1123:
1122:Heng-o Corona
1120:
1118:
1115:
1113:
1110:
1108:
1105:
1103:
1100:
1098:
1095:
1093:
1092:Baʽhet Corona
1090:
1088:
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1080:
1078:
1075:
1073:
1070:
1069:
1067:
1065:
1059:
1055:
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1037:
1035:
1032:
1031:
1029:
1027:
1023:
1017:
1014:
1012:
1009:
1007:
1006:Asteria Regio
1004:
1002:
999:
998:
996:
992:
989:
985:
979:
976:
974:
971:
969:
966:
964:
961:
959:
956:
955:
953:
949:
946:
942:
936:
933:
932:
929:
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918:
913:
911:
906:
904:
899:
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868:
863:
859:
855:
851:
847:
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833:
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812:
808:
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800:
796:
789:
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773:
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764:
760:
756:
752:
748:
741:
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721:
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713:
706:
698:
694:
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671:
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560:
556:
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548:
544:
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533:
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492:
488:
484:
480:
476:
472:
465:
463:
461:
459:
457:
440:
436:
432:
425:
418:. Bloomsbury.
417:
410:
402:
398:
397:
389:
381:
377:
373:
369:
365:
361:
354:
346:
342:
337:
332:
328:
324:
320:
316:
309:
307:
305:
303:
293:
289:
281:
278:
267:
264:
254:
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242:
234:
225:
223:
208:
200:
196:
188:
179:
176:
165:
156:
154:
149:
145:
141:
137:
128:
119:
117:
112:
108:
104:
101:to the west,
100:
99:Salus Tessera
96:
92:
88:
84:
80:
76:
68:forest spirit
67:
64:
60:
56:
52:
48:
44:
40:
36:
31:
25:
20:
2093:Terraforming
2082:Colonization
2064:Shukrayaan-1
1979:
1972:
1949:
1942:
1930:
1923:
1916:
1900:Vega program
1869:Zond program
1859:
1852:
1845:
1838:
1732:Venera 1964A
1328:Ganis Chasma
1323:Diana Chasma
1197:Sachs Patera
1182:Pancake dome
1112:Fotla Corona
1097:Boala Corona
1039:Ishtar Terra
1015:
879:. Retrieved
849:
845:
832:
820:. Retrieved
798:
794:
781:
754:
750:
740:
715:
711:
705:
680:
676:
670:
645:
641:
612:. Retrieved
605:the original
584:
580:
567:
542:
538:
532:
520:. Retrieved
515:
474:
470:
443:. Retrieved
439:the original
434:
424:
415:
409:
395:
388:
363:
359:
353:
318:
314:
292:
273:
270:Impact model
260:
248:
240:
231:
218:
194:
185:
182:Eastern Ovda
171:
168:Central Ovda
162:
159:Western Ovda
133:
103:Thetis Regio
74:
73:
54:Surface area
38:Feature type
1981:BepiColombo
1674:Exploration
1527:Geodynamics
1511:Yablochkina
1313:Dali Chasma
1237:Zisa Corona
1187:Renpet Mons
1137:Irnini Mons
1127:Iaso Tholus
1077:Akna Montes
1072:Abeona Mons
1001:Alpha Regio
968:Dune fields
614:13 February
522:13 February
399:. pp.
251:lithosphere
222:shear zones
109:as well as
46:Coordinates
2169:Phosphorus
2144:In fiction
2139:In culture
1861:Mariner 10
1787:Kosmos 482
1762:Kosmos 167
1722:Sputnik 21
1717:Sputnik 20
1712:Sputnik 19
1547:Venusquake
1542:Venus snow
1471:Merit Ptah
1406:De Lalande
1232:Ushas Mons
1227:Theia Mons
1222:Skadi Mons
1202:Sapas Mons
1132:Idunn Mons
1082:Anala Mons
1044:Lada Terra
1016:Ovda Regio
1011:Beta Regio
963:Atmosphere
284:References
75:Ovda Regio
17:Ovda Regio
2159:Mythology
2134:Cytherean
1944:MESSENGER
1854:Mariner 5
1847:Mariner 2
1840:Mariner 1
1827:Venera 16
1822:Venera 15
1817:Venera 14
1812:Venera 13
1807:Venera 12
1802:Venera 11
1797:Venera 10
1752:Kosmos 96
1737:Kosmos 27
1727:Kosmos 21
1694:Sputnik 7
1642:Asteroids
1560:Astronomy
1476:Mona Lisa
1421:Golubkina
1411:Dickinson
1391:Cleopatra
1167:Ozza Mons
1147:Maat Mons
1117:Gula Mons
1107:Fand Mons
1064:volcanoes
1058:Mountains
958:Arachnoid
944:Geography
862:CiteSeerX
331:CiteSeerX
175:imbricate
2212:Category
2187:Category
2149:Hesperus
2073:Proposed
2027:Proposed
2013:Venera-D
2003:EnVision
1974:Akatsuki
1918:Magellan
1792:Venera 9
1782:Venera 8
1777:Venera 7
1772:Venera 6
1767:Venera 5
1757:Venera 4
1747:Venera 3
1742:Venera 2
1707:Venera 1
1703:program
1594:Transits
1506:Wheatley
1496:Stefania
1441:Isabella
1436:Guilbert
1401:Danilova
1257:plateaus
1217:Sif Mons
973:Features
822:29 March
277:isostasy
144:temporal
116:Marijian
81:crustal
79:Venusian
66:Marijian
2127:Related
2089:(flyby)
2008:VERITAS
1998:DAVINCI
1991:Planned
1966:Current
1951:Shin'en
1925:Galileo
1574:Aspects
1567:General
1532:Geology
1481:Nanichi
1466:Meitner
1431:Gregory
1371:Aurelia
1366:Ariadne
1338:Craters
1290:valleys
1285:Canyons
987:Regions
951:General
881:1 March
854:Bibcode
846:Geology
803:Bibcode
759:Bibcode
720:Bibcode
685:Bibcode
650:Bibcode
589:Bibcode
547:Bibcode
479:Bibcode
445:1 March
368:Bibcode
323:Bibcode
111:Ix Chel
87:equator
83:plateau
2197:Portal
2075:crewed
2049:VISAGE
1938:IKAROS
1910:Vega 2
1905:Vega 1
1874:Zond 1
1701:Venera
1660:Zoozve
1584:Phases
1456:Mariko
1446:Jeanne
1426:Grimke
1396:Cunitz
1381:Barton
1361:Alcott
1356:Agnesi
1351:Adivar
1346:Addams
1252:Plains
1026:Terrae
864:
581:Icarus
539:Icarus
333:
315:Icarus
153:graben
107:Kuanja
62:Eponym
2102:Other
1579:Orbit
1520:Other
1501:Wanda
1486:Riley
1376:Balch
994:Regio
924:Venus
842:(PDF)
791:(PDF)
608:(PDF)
577:(PDF)
512:(PDF)
95:Venus
77:is a
41:Regio
2154:Life
2054:VICI
2044:VISE
2039:VAMP
1682:Past
1632:2012
1627:2004
1622:1882
1617:1874
1612:1769
1607:1761
1602:1639
1491:Ruth
1461:Mead
1386:Buck
883:2015
824:2015
616:2015
524:2015
447:2015
146:and
2059:VOX
1287:and
1254:and
1061:and
872:doi
811:doi
799:111
767:doi
755:105
728:doi
693:doi
681:101
658:doi
597:doi
585:175
555:doi
543:132
487:doi
401:183
376:doi
341:doi
319:139
2214::
870:.
860:.
850:31
848:.
844:.
809:.
797:.
793:.
765:.
753:.
749:.
726:.
716:97
714:.
691:.
679:.
656:.
646:59
644:.
624:^
595:.
583:.
579:.
553:.
541:.
514:.
499:^
485:.
475:58
473:.
455:^
433:.
374:.
364:97
362:.
339:.
329:.
317:.
301:^
224:.
155:.
916:e
909:t
902:v
885:.
874::
856::
826:.
813::
805::
775:.
769::
761::
734:.
730::
722::
699:.
695::
687::
664:.
660::
652::
618:.
599::
591::
561:.
557::
549::
526:.
493:.
489::
481::
449:.
403:.
382:.
378::
370::
347:.
343::
325::
32:.
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
