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File:Mercury in color - Prockter07 centered.jpg

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466:"rays" by planetary scientists) emanating from them. Bright features such as these are caused by the presence of freshly crushed rock material that was excavated and deposited during the highly energetic collision of a meteoroid with Mercury to form an impact crater. The large circular light-colored area in the upper right of the image is the interior of the Caloris basin. Mariner 10 viewed only the eastern (right) portion of this enormous impact basin, under lighting conditions that emphasized shadows and elevation differences rather than brightness and color differences. MESSENGER has revealed that Caloris is filled with smooth plains that are brighter than the surrounding terrain, hinting at a compositional contrast between these geologic units. The interior of Caloris also harbors several unusual dark-rimmed craters, which are visible in this image. The MESSENGER science team is working with the 11-color images in order to gain a better understanding of what minerals are present in these rocks of Mercury's crust. 1278: 43: 462:
seen by spacecraft. The color image shown here was generated by combining the mosaics taken through the WAC filters that transmit light at wavelengths of 1000 nanometers (infrared), 700 nanometers (far red), and 430 nanometers (violet). These three images were placed in the red, green, and blue channels, respectively, to create the visualization presented here. The human eye is sensitive only across the wavelength range from about 400 to 700 nanometers. Creating a false-color image in this way accentuates color differences on Mercury's surface that cannot be seen in black-and-white (single-color) images.
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Color differences on Mercury are subtle, but they reveal important information about the nature of the planet's surface material. A number of bright spots with a bluish tinge are visible in this image. These are relatively recent impact craters. Some of the bright craters have bright streaks (called
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The diameter of Mercury is about 4880 kilometers (3030 miles). The image spatial resolution is about 2.5 kilometers per pixel (1.6 miles/pixel). The WAC departure mosaic sequence was executed by the spacecraft from approximately 19:45 to 19:56 UTC on January 14, 2008, when the spacecraft was moving
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MESSENGER's Wide Angle Camera (WAC), part of the Mercury Dual Imaging System (MDIS), is equipped with 11 narrow-band color filters. As the spacecraft receded from Mercury after making its closest approach on January 14, 2008, the WAC recorded a 3x3 mosaic covering part of the planet not previously
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Mercurio è il pianeta più interno del sistema solare e il più vicino al Sole. È il più piccolo e la sua orbita è anche la più eccentrica, ovvero la meno circolare, degli otto pianeti. @Alfio
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joint project implies that all materials created by its probe are copyrighted and require permission for commercial non-educational use.
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This file contains additional information, probably added from the digital camera or scanner used to create or digitize it.
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If the file has been modified from its original state, some details may not fully reflect the modified file.
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More than 100 pages use this file. The following list shows the first 100 pages that use this file only. A
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states that all of the images in the photo gallery are in the public domain "Unless otherwise noted."
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from a distance of roughly 12,800 to 16,700 km (7954 to 10377 miles) from the surface of Mercury.
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Merkurius, planet terkecil dan terdekat dengan matahari dalam sistem Tata Surya.
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data may be copyrighted if they are not explicitly produced by the
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Imagen a color de Mercurio tomada por el primer Messenger.
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This image is a derivative work of the following images:
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The NASA website hosts a large number of images from the
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Mercure vue par la sonde MESSENGER, le 14 janvier 2008.
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in the United States because it was solely created by
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licensed with PD-USGov-NASA, PD-USGov-NASA/copyright
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Commons is a freely licensed media file repository.
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work of the federal government of the United States
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work of the federal government of the United States
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MESSENGER first photo of unseen side of mercury.jpg
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Johns Hopkins University Applied Physics Laboratory
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1902: 1897: 1892: 1887: 1885:Ibsen (crater) 1882: 1877: 1872: 1870:Homer (crater) 1867: 1862: 1857: 1852: 1847: 1842: 1837: 1832: 1827: 1822: 1817: 1812: 1807: 1805:Degas (crater) 1802: 1797: 1792: 1787: 1782: 1777: 1772: 1767: 1762: 1757: 1752: 1750:Bashō (crater) 1747: 1742: 1737: 1735:Atget (crater) 1732: 1727: 1725:Arecibo Catena 1722: 1717: 1712: 1707: 1702: 1697: 1692: 1685:is available. 1678: 1673: 1672: 1665: 1661: 1658: 1654:1,991 × 1,974 1652: 1647: 1642: 1638: 1637: 1634: 1631: 1628: 1625: 1622: 1614: 1599: 1596: 1594: 1593: 1592: 1590: 1589: 1585: 1580: 1578: 1577: 1576: 1575: 1573: 1561: 1558: 1556: 1555: 1554: 1552: 1551: 1547: 1542: 1540: 1539: 1538: 1537: 1535: 1523: 1518: 1516: 1515: 1514: 1512: 1511: 1507: 1502: 1500: 1499: 1498: 1497: 1495: 1491: 1466: 1465: 1451: 1450: 1449: 1448: 1447: 1443: 1438: 1436: 1435: 1434: 1432: 1431: 1427: 1422: 1420: 1419: 1418: 1417: 1415: 1411: 1407: 1403: 1399: 1395: 1383: 1378: 1376: 1375: 1374: 1372: 1355: 1354: 1340: 1339: 1338: 1337: 1336: 1332: 1327: 1325: 1324: 1323: 1321: 1320: 1316: 1311: 1309: 1306: 1305: 1304: 1303: 1301: 1297: 1293: 1289: 1285: 1281: 1267: 1259: 1251: 1243: 1235: 1227: 1219: 1211: 1203: 1195: 1194: 1191: 1188: 732: 731: 723: 720: 709:Uploaded with 706: 705: 704: 703: 693: 684: 663: 660: 657: 656: 654: 653: 638: 627: 618: 592: 577: 565: 557: 547: 546: 537: 506: 494: 493: 475: 472: 459: 458: 451: 450: 445: 444: 432: 416: 415:Other versions 412: 411: 389: 385: 384: 379: 375: 374: 369: 365: 364: 348: 331: 328: 326: 317: 315: 312: 309: 308: 299: 286: 285: 282: 281: 278: 277: 253: 252: 192: 191: 168: 167: 153: 151: 124: 123: 102: 92: 91: 45: 40: 39: 34: 29: 24: 19: 9: 6: 4: 3: 2: 2635: 2621: 2618: 2617: 2613: 2610: 2609: 2605: 2602: 2601: 2597: 2594: 2593: 2589: 2587: 2584: 2583: 2579: 2576: 2575: 2572: 2569: 2567:Software used 2566: 2565: 2561: 2558: 2557: 2553: 2550: 2549: 2545: 2542: 2541: 2538: 2535: 2527: 2525: 2516: 2513: 2512: 2510: 2506: 2503: 2501: 2498: 2497: 2495: 2491: 2488: 2487: 2485: 2481: 2478: 2477: 2475: 2471: 2468: 2466: 2463: 2461: 2458: 2457: 2455: 2451: 2448: 2446: 2443: 2441: 2438: 2436: 2433: 2432: 2430: 2426: 2423: 2422: 2420: 2416: 2413: 2411: 2408: 2406: 2403: 2401: 2398: 2396: 2393: 2391: 2388: 2386: 2383: 2381: 2378: 2376: 2375:استكشاف عطارد 2373: 2371: 2368: 2366: 2363: 2361: 2358: 2356: 2353: 2351: 2348: 2346: 2343: 2341: 2338: 2336: 2335:برنامج مارينر 2333: 2331: 2328: 2326: 2323: 2321: 2318: 2316: 2313: 2311: 2308: 2306: 2303: 2301: 2298: 2296: 2293: 2291: 2288: 2286: 2283: 2281: 2278: 2276: 2273: 2272: 2270: 2266: 2263: 2261: 2258: 2257: 2255: 2251: 2248: 2246: 2243: 2242: 2240: 2236: 2233: 2232: 2230: 2226: 2223: 2221: 2218: 2217: 2215: 2211: 2208: 2207: 2205: 2204: 2203: 2195: 2193: 2186: 2183: 2181: 2178: 2176: 2173: 2171: 2168: 2166: 2163: 2161: 2158: 2156: 2155:Zola (crater) 2153: 2151: 2148: 2146: 2143: 2141: 2138: 2136: 2133: 2131: 2128: 2126: 2123: 2121: 2118: 2116: 2113: 2111: 2108: 2106: 2103: 2101: 2098: 2096: 2093: 2091: 2088: 2086: 2083: 2081: 2080:Simeiz Vallis 2078: 2076: 2073: 2071: 2068: 2066: 2063: 2061: 2058: 2056: 2053: 2051: 2048: 2046: 2043: 2041: 2038: 2036: 2033: 2031: 2028: 2026: 2023: 2021: 2018: 2016: 2013: 2011: 2008: 2006: 2003: 2001: 1998: 1996: 1993: 1991: 1988: 1986: 1983: 1981: 1978: 1976: 1973: 1971: 1968: 1966: 1965:Odin Planitia 1963: 1961: 1958: 1956: 1953: 1951: 1948: 1946: 1943: 1941: 1938: 1936: 1933: 1931: 1928: 1926: 1923: 1921: 1918: 1916: 1913: 1911: 1908: 1906: 1903: 1901: 1898: 1896: 1893: 1891: 1888: 1886: 1883: 1881: 1878: 1876: 1873: 1871: 1868: 1866: 1863: 1861: 1858: 1856: 1853: 1851: 1848: 1846: 1843: 1841: 1838: 1836: 1833: 1831: 1828: 1826: 1823: 1821: 1818: 1816: 1813: 1811: 1808: 1806: 1803: 1801: 1798: 1796: 1793: 1791: 1788: 1786: 1783: 1781: 1778: 1776: 1773: 1771: 1768: 1766: 1763: 1761: 1758: 1756: 1753: 1751: 1748: 1746: 1745:Bach (crater) 1743: 1741: 1738: 1736: 1733: 1731: 1728: 1726: 1723: 1721: 1718: 1716: 1713: 1711: 1708: 1706: 1703: 1701: 1698: 1696: 1693: 1691: 1688: 1687: 1686: 1684: 1670: 1664: 1659: 1653: 1651: 1648: 1646: 1643: 1640: 1639: 1635: 1632: 1629: 1626: 1623: 1621: 1620: 1618: 1595: 1583: 1579: 1557: 1545: 1541: 1521: 1517: 1505: 1501: 1476: 1469: 1461: 1454: 1441: 1440:public domain 1437: 1425: 1421: 1398:public domain 1381: 1377: 1358: 1357:point in time 1350: 1343: 1342:captured with 1330: 1326: 1314: 1310: 1307: 1296:point in time 1288:captured with 1192: 1185: 1182: 1157: 1132: 1107: 1082: 1057: 1032: 1007: 982: 957: 932: 907: 882: 857: 832: 807: 782: 757: 730: 729: 724: 718: 717: 714: 713: 712: 702: 698: 694: 692: 689: 685: 683: 679: 675: 674: 672: 669: 668: 667: 651: 647: 643: 639: 637: 634: 633: 628: 626: 623: 619: 616: 614:{{Cc-Hubble}} 610: 608:{{PD-Hubble}} 604: 601: 597: 593: 590: 586: 582: 578: 575: 571: 567: 566: 564: 562: 558: 549: 548: 538: 536: 534: 530: 526: 522: 518: 514: 513: 512:public domain 507: 500: 499: 485:Public domain 482:Public domain 480: 479: 471: 467: 463: 456: 455: 449: 443: 441: 436: 433: 430: 425: 422: 421: 420: 417: 413: 409: 405: 401: 397: 393: 390: 386: 383: 380: 376: 366: 360: 356: 343: 339: 327: 320: 305: 300: 293: 292: 276: 275: 273: 269: 265: 262:, be sure to 261: 256: 251: 249: 245: 241: 232: 230: 226: 222: 213: 211: 207: 203: 194: 193: 188: 185: 184: 182: 178: 174: 170: 169: 166: 152: 150: 142: 139: 138: 135: 134: 120: 113: 112: 107: 103: 96: 95: 89: 80: 79:Original file 71: 67: 63: 59: 55: 49: 44: 38: 35: 33: 30: 28: 25: 23: 20: 18: 15: 2603:Image height 2536: 2533: 2521: 2400:حفرة فلايانو 2201: 2189: 2175:User:Aracowa 2115:Tir Planitia 1995:Poe (crater) 1680: 1616: 1613:File history 1180: 1155: 1130: 1105: 1080: 1055: 1030: 1005: 980: 955: 930: 905: 880: 855: 831:Hovnatanian 830: 806:Raden Saleh 805: 780: 755: 726: 711:derivativeFX 708: 707: 700: 691: 681: 665: 630: 588: 560: 521:unless noted 520: 510: 508: 468: 464: 460: 418: 257: 239: 220: 201: 172: 155: 144: 119:You can help 109: 77: 22:File history 2595:Image width 2586:Color space 2543:Orientation 2330:حوض كالوريس 2295:بيبيكولومبو 906:Cunningham 719:Annotations 697:Kwamikagami 688:Kwamikagami 574:14 CFR 1221 340:from first 322:Description 272:nominate it 2571:GIMP 2.4.4 2445:قالب:عطارد 2395:1981 ميداس 2360:عبور الشمس 2305:عبور عطارد 2300:قالب:عطارد 2192:more links 1855:Hero Rupes 1677:File usage 1630:Dimensions 1597:image/jpeg 1582:media type 1572:media type 1272:ကျောက်တုံး 1229:Indonesian 1081:Izquierdo 1006:Xiao Zhao 856:Raditladi 781:Qi Baishi 570:NASA logos 359:Мессенджер 190:Knowledge 171:This is a 85:image/jpeg 27:File usage 2290:مارينر 10 1683:full list 1656:(1.72 MB) 1627:Thumbnail 1624:Date/Time 1544:inception 1534:inception 1349:MESSENGER 1292:MESSENGER 1056:Kunisada 1031:Eminescu 721:InfoField 678:Superm401 605:See also 561:Warnings: 474:Licensing 342:MESSENGER 2606:2,025 px 2598:3,000 px 2530:Metadata 2505:बुध ग्रह 2490:Niskaduz 2245:बुध ग्रह 1224:Меркурий 1193:Captions 1106:Tolstoj 981:Enwonwu 881:Kertész 523:". (See 382:NASA/JPL 355:Меркурия 270:it, and 37:Metadata 2562:300 dpi 2554:300 dpi 1641:current 1636:Comment 1329:Mercury 1313:depicts 1284:Mercury 1280:depicts 1269:Burmese 1253:Italian 1240:ميركوري 1221:Russian 1213:Turkish 1205:Spanish 1197:English 1156:Neruda 756:Mozart 568:Use of 437::  426::  349:Русский 338:Mercury 332:English 314:Summary 81:‎ 2546:Normal 1380:planet 1300:planet 1261:German 1245:French 1237:Arabic 1216:mercur 1181:Basho 931:Atget 648:. 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File:Mercury in color - Prockter07 centered.jpg
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242 × 240 pixels
484 × 480 pixels
775 × 768 pixels
1,033 × 1,024 pixels
1,991 × 1,974 pixels
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Mercury

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