Book Title: Ashtapad Maha Tirth 02
Author(s): Rajnikant Shah, Others
Publisher: USA Jain Center America NY

View full book text
Previous | Next

Page 246
________________ 16 Central Himalayan Geological Observations Augusto Gansser Summarized by Mayur Desai and Ajit Shah The following document presents excerpts from publication by A. Gansser, titled "Geology of Himalayas", published by Inter-science Publications, 1964. The selected excerpts related to geology of Mt. Kailash region are presented in here. Regional Setting The regional settings of the Himalayas have some striking particularities, such as their outstanding height, the thrusts, rock composition and their isolated position. The Himalayas have no direct continuation either towards the west or to the east. The singular syntaxial bends on both extremes preclude a straight forward continuation of the Himalayan elements. In the west, the Sulaiman Range is not a direct continuation of the Lower Himalayas, but is a fold system of younger sediments (Mesozoic and younger) which develops out of the Hazara Ranges in the west. Westwards, the Sulaiman belt is sharply limited by an ophiolitic tectonic line from the Flysch-type Baluchistan and Afghan sediments. This suture line may be a continuation, or most likely a branch, of the Indus suture line. The other branch seems to form the southern border of the Hindu-Kush Range, the western equivalent of the Karakorum. It is much more difficult to follow the eastern continuation of the Himalayas due to lack of geological information. The little we know indicates that here too there is no direct continuation of the range. The southeastern Assam foothills (Naga Hills) differ from the corresponding Himalayan foothills. The crystalline rocks of the Mishmi Hills seem to belong to the Higher Himalayas, though some indications of inverted metamorphism do exist. The backbone of the western Burmese ranges, the peculiar Arakan Yoma, has no affinities with the Lower or Higher Himalayas. The Flysch type sediments, mostly of Cretaceous age, expose some ultra basic rocks aligned along the eastern border which is faulted and partly thrusted. Acertain similarity with the Indus Flysch belt seems evident, but no direct connection with this important north Himalayan element is known. We have noted that the latter disappears east of the Manasarovar Lake in the northern Kumaon Himalayas. The Arakan Yoma Ranges certainly is on eastern equivalent of the Sulaiman Range. Within the mountain ranges of Asia, the Himalayas display thrusting of such a magnitude that a crustal shortening of about 400 km is suggested. This is not the figure assumed by some authors for the crustal shortening in the Alps. This amount, Copyright Acknowledgement - Inter Science Publishers. Original Source Central Himalaya: Geological observations of the Swiss Expedition, 1936 Ref. Vol. XII Ch. 86 F Pg. 5534-5555 Central Himalayan Geological Observations 190

Loading...

Page Navigation
1 ... 244 245 246 247 248 249 250 251 252 253 254 255 256 257 258 259 260 261 262 263 264 265 266 267 268 269 270 271 272 273 274 275 276 277 278 279 280 281 282 283 284 285 286 287 288 289 290 291 292 293 294 295 296 297 298 299 300 301 302 303 304 305 306 307 308 309 310 311 312 313 314 315 316 317 318 319 320 321 322 323 324 325 326 327 328 329 330 331 332 333 334 335 336 337 338 339 340 341 342 343 344 345 346 347 348 349 350 351 352 353 354 355 356 357 358 359 360 361 362 363 364 365 366 367 368 369 370 371 372 373 374 375 376 377 378 379 380 381 382 383 384 385 386 387 388 389 390 391 392 393 394 395 396 397 398 399 400 401 402 403 404 405 406 407 408 409 410 411 412 413 414 415 416 417 418 419 420 421 422 423 424 425 426 427 428 429 430 431 432 433 434 435 436 437 438 439 440 441 442 443 444 445 446 447 448 449 450 451 452 453 454 455 456 457 458 459 460 461 462 463 464 465 466 467 468 469 470 471 472 473 474 475 476 477 478 479 480 481 482 483 484 485 486 487 488 489 490 491 492 493 494 495 496 497 498 499 500 501 502 503 504 505 506 507 508 509 510 511 512 513 514 515 516 517 518 519 520 521 522 523 524 525 526 527 528 529 530 531 532