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Raditladi (crater)

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350: 314: 184: 338: 326: 38: 2660: 2672: 286:. Both types of structures form when magma from a deep reservoir intrudes into the overlying rocks along conical or cylindrical fractures. The second hypothesis holds that the graben formed as a result of the floor uplift caused by the weight of the smooths plains outside the crater. Such plains are indeed present to the north and east of Raditladi, although their thickness and age are not known. 149:. The troughs may also have resulted from volcanic processes under the floor of Raditladi. The basin is relatively young, probably younger than one billion years, with only a few small impact craters on its floor and with well-preserved basin walls and peak-ring structure. It is one of 110 peak ring basins on Mercury. 294:
The relative age of any surface feature can be determined from the density of impact crater on it. The density of craters on the floor of Raditladi is about 10% of that on the plains west of Caloris. The crater density is the same on the ejecta covered plains outside the basin. The smooths plains and
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Baker, David M. H.; Head, James W.; Schon, Samuel C.; Ernst, Carolyn M.; Prockter, Louise M.; Murchie, Scott L.; Denevi, Brett W.; Solomon, Sean C.; Strom, Robert G. (2011). "The transition from complex crater to peak-ring basin on Mercury: New observations from MESSENGER flyby data and constraints
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of smooth plains. The hummocky plains are slightly bluer than smooth plains. The areas outside Raditladi are covered by the dark relatively blue impact ejecta. The peak ring massifs at some places expose a bright blue material identical to one on the floors of some bright Mercurian impact craters
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Understanding how these troughs formed in the young Raditladi basin could provide an important indicator of processes that acted relatively recently in Mercury's geologic history. There are two main theories of graben formation. The first is that they represent a surface manifestation of
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plains. The former partially embay the hummocky plains and are probably volcanic in origin. The latter are present mainly on a part of the floor between the peak ring and crater rim; they interpreted to be the original crater floor material not covered by the light colored
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hummocky plains also have the same crater density and therefore the same apparent age. The low crater density indicates that Raditladi is much younger than Caloris—it may have formed within the last billion years, whereas the age of Caloris is 3.5–3.9 billion years.
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Robinson, Mark S.; Murchie, Scott L.; Blewett, David T.; Domingue, DL; Hawkins Se, 3rd; Head, JW; Holsclaw, GM; McClintock, WE; et al. (2008). "Reflectance and Color Variations on Mercury: Regolith Processes and Compositional Heterogeneity".
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with a diameter of 125 km. The ring is slightly offset from the geometrical center of the basin in the north-west direction. The floor of Raditladi is covered by two types of terrain: light smooth plains and dark
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Chapman, C. R., Baker, D. M. H., Barnouin, O. S., Fassett, C. I., Marchie, S., Merline, W. J., Ostrach, L. R., Prockter, L. M., and Strom, R. G., 2018. Impact Cratering of Mercury. In
145:(graben), which are rare surface features on Mercury. The floor of Raditladi is partially covered by relatively light smooth plains, which are thought to be a product of the effusive 683: 574:
Head, James W.; Murchie, Scott L.; Prockter, Louise M.; Solomon, Sean C.; et al. (2009). "Evidence for intrusive activity on Mercury from the first MESSENGER flyby".
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Watters, Thomas R.; Solomon, Sean C.; Robinson, Mark S.; Head, James W.; et al. (2009). "The tectonics of Mercury: The view after MESSENGER's first flyby".
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Zhiyong Xiao, Robert G. Strom, David T. Blewett, Paul K. Byrne, Sean C. Solomon, Scott L. Murchie, Ann L. Sprague, Deborah L. Domingue, Jörn Helbert, 2013.
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Strom, G.; Chapman, Clark R.; Merline, William J.; Solomon, SC; et al. (2008). "Mercury Cratering Record Viewed from MESSENGER's First Flyby".
653: 555: 75: 313: 236:. The geometrical center of the system of graben coincides with the center of Raditladi and is offset from the center of the peak ring complex. 232:(pulling apart) of the surface. The troughs are arranged in a circular pattern approximately 70 km in diameter. They are thought to be 167:
basin on the part of Mercury's surface previously not seen by spacecraft. This crater (or basin) was subsequently (on 8 April 2008) named
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Prockter, Louise M.; Watters, Thomas R.; Chapman, Clark R.; Denevi, B. W.; et al. (2009). "The curious case of Raditladi basin".
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Neukum, G.; Oberst, J.; Hoffmann, H.; Wagner, R.; et al. (2001). "Geologic evolution and cratering history of Mercury".
210:(Bright Crater Floor Deposits—BCFD). BCFD in Raditladi are recognized more generally as a subset of a landform now called 2697: 852: 17: 302:
activity on Mercury lasted for much longer that had been thought, possibly extending to the last billion years.
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edited by Sean C. Solomon, Larry R. Nittler, and Brian J. Anderson. Cambridge Planetary Science. Chapter 9.
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is present outside the eastern peak ring of Raditladi. This dark spot is associated with the hollows.
2014: 2663: 1229: 795: 183: 1324: 175:(1910–1971), a Botswanan playwright and poet. Raditladi is one of the youngest features on Mercury. 2465: 2369: 687: 172: 118: 2389: 2619: 2109: 946: 1519: 228:
Visible on the floor of Raditladi inside the peak ring are concentric narrow troughs, formed by
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NASA Astronomy Picture of the Day: Unusual Hollows Discovered on Planet Mercury (27 March 2012)
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Extensional troughs on Mercury are quite rare, having been seen in only a few other locations:
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Dark spots on Mercury: A distinctive low-reflectance material and its relation to hollows
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spacecraft discovered a large impact crater approximately 2000 km west of the
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High-resolution mosaic of part of the central peak ring showing
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The central part of Raditladi is occupied by a large
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Central peak ring. Concentric troughs are visible.
246:, which is similar in many other ways to Raditladi 157:During its first flyby of Mercury in January 2008 2689: 457: 455: 453: 451: 449: 447: 445: 443: 803: 670:. Journal of Geophysical Research Planets. 141:there is a system of concentric extensional 652:: CS1 maint: numeric names: authors list ( 602: 554:: CS1 maint: numeric names: authors list ( 507: 505: 503: 501: 440: 137:with a diameter of 263 km. Inside its 810: 796: 708: 569: 567: 565: 298:The young age of Raditladi shows that the 36: 498: 404: 182: 562: 14: 2690: 384: 382: 223: 791: 684:"The Curious Case of Raditladi Basin" 676: 343:Exaggerated color image of Raditladi 756:Earth and Planetary Science Letters 576:Earth and Planetary Science Letters 379: 24: 747: 264:, a large basin discovered during 25: 2714: 2670: 2659: 2658: 348: 336: 324: 319:Position of Raditladi on Mercury 312: 660: 482: 13: 1: 1202:Skinakas (hypothetical basin) 737:10.1016/S0032-0633(01)00089-7 372: 152: 2491:Hypothetical moon of Mercury 693:. 2009-03-31. Archived from 412:on basin formation models". 7: 817: 717:Planetary and Space Science 464:Lunar and Planetary Science 414:Planetary and Space Science 360: 10: 2719: 2539:Mercury-crossing asteroids 776:10.1016/j.epsl.2009.01.025 691:Applied Physics Laboratory 672:doi.org/10.1002/jgre.20115 596:10.1016/j.epsl.2009.03.008 305: 178: 42:Mosaic of MESSENGER images 2698:Impact craters on Mercury 2653: 2632: 2612: 2595: 2560: 2551: 2529: 2506: 2499: 2483: 2453: 1210: 1172: 1114: 1066: 998: 980: 892: 876: 845: 838: 825: 490:Mercury: The View After 434:10.1016/j.pss.2011.05.010 253:and other troughs in the 114: 110:258 km (160 mi) 106: 69: 55: 47: 35: 688:Johns Hopkins University 173:Leetile Disang Raditladi 119:Leetile Disang Raditladi 2620:Colonization of Mercury 768:2009E&PSL.285..283W 729:2001P&SS...49.1507N 632:10.1126/science.1160080 588:2009E&PSL.285..251H 534:10.1126/science.1159317 426:2011P&SS...59.1932B 331:Topography of Raditladi 273:s second Mercury flyby. 191:. MESSENGER NAC mosaic. 289: 192: 51:Peak-ring impact basin 1965:Kuan Han-Chʻing 186: 2015:Li Chʻing-Chao 390:"Mercury: Raditladi" 60:Raditladi quadrangle 2471:Inter-crater plains 624:2008Sci...321...66R 526:2008Sci...321...79S 476:2009LPI....40.1758P 224:Extensional troughs 87: /  32: 723:(14–15): 1507–21. 367:Geology of Mercury 193: 30: 2685: 2684: 2628: 2627: 2547: 2546: 2479: 2478: 1525:Chŏng Chʼŏl 1520:Chiang Kʻui 1159:Santa María Rupes 1028:Mearcair Planitia 1013:Borealis Planitia 1008:Apārangi Planitia 420:(15): 1932–1948. 300:effusive volcanic 124: 123: 27:Crater on Mercury 16:(Redirected from 2710: 2674: 2662: 2661: 2558: 2557: 2504: 2503: 2025:Liang Kʻai 1230:Africanus Horton 1154:Resolution Rupes 1144:Enterprise Rupes 1124:Antoniadi Dorsum 1091:Goldstone Vallis 1086:Goldstone Catena 1058:Utaridi Planitia 1043:Stilbon Planitia 1023:Caloris Planitia 843: 842: 812: 805: 798: 789: 788: 779: 762:(3–4): 283–286. 741: 740: 712: 706: 705: 703: 702: 680: 674: 664: 658: 657: 651: 643: 606: 600: 599: 571: 560: 559: 553: 545: 509: 496: 486: 480: 479: 459: 438: 437: 408: 402: 401: 399: 397: 386: 352: 340: 328: 316: 272: 260:on the floor of 102: 101: 99: 98: 97: 92: 91:27.15°N 240.94°W 88: 85: 84: 83: 80: 40: 33: 29: 21: 2718: 2717: 2713: 2712: 2711: 2709: 2708: 2707: 2688: 2687: 2686: 2681: 2649: 2624: 2608: 2591: 2562: 2543: 2525: 2495: 2475: 2449: 2370:Sholem Aleichem 1206: 1197:Rembrandt Basin 1192:Raditladi Basin 1187:Pantheon Fossae 1174: 1168: 1139:Discovery Rupes 1129:Adventure Rupes 1116: 1110: 1101:Haystack Vallis 1096:Haystack Catena 1068: 1062: 1048:Suisei Planitia 1038:Sobkou Planitia 1000: 994: 982: 976: 888: 872: 853:Albedo features 834: 821: 816: 750: 748:Further reading 745: 744: 713: 709: 700: 698: 682: 681: 677: 665: 661: 645: 644: 618:(5885): 66–69. 607: 603: 572: 563: 547: 546: 520:(5885): 79–81. 510: 499: 487: 483: 460: 441: 409: 405: 395: 393: 388: 387: 380: 375: 363: 356: 353: 344: 341: 332: 329: 320: 317: 308: 292: 270: 251:Pantheon Fossae 226: 216:. A confirmed 181: 155: 95: 93: 89: 86: 81: 78: 76: 74: 73: 43: 28: 23: 22: 18:Raditladi Basin 15: 12: 11: 5: 2716: 2706: 2705: 2700: 2683: 2682: 2680: 2679: 2667: 2654: 2651: 2650: 2648: 2647: 2642: 2636: 2634: 2630: 2629: 2626: 2625: 2623: 2622: 2616: 2614: 2610: 2609: 2607: 2606: 2599: 2597: 2593: 2592: 2590: 2589: 2588:(2018–present) 2583: 2575: 2566: 2564: 2555: 2549: 2548: 2545: 2544: 2542: 2541: 2535: 2533: 2527: 2526: 2524: 2523: 2518: 2512: 2510: 2501: 2497: 2496: 2494: 2493: 2487: 2485: 2481: 2480: 2477: 2476: 2474: 2473: 2468: 2463: 2457: 2455: 2451: 2450: 2448: 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: 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Index

Raditladi Basin
}
Raditladi quadrangle
Mercury
27°09′N 240°56′W / 27.15°N 240.94°W / 27.15; -240.94
Leetile Disang Raditladi
impact crater
Mercury
peak ring
troughs
volcanism
MESSENGER
Caloris
Leetile Disang Raditladi

hollows
peak ring
hummocky
lavas
hollows
extension
graben
Rachmaninoff
Pantheon Fossae
Caloris
Rembrandt
MESSENGER
ring dikes
cone sheets
effusive volcanic

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