There is widespread agreement among geologists that the Himalayas began forming roughly 50-70 million years ago when the northward-moving Indo-Australian tectonic plate began colliding with the relatively stationary Eurasian Plate. The boundary of the collision is called the Tibetan Plateau, which was shattered and pushed upward to form the great Himalyan peaks such as Mt Everest.
First to collide were the leading edges of the continental shelves, where massive amounts of seafloor ocean sediments and sedimentary rock were being tilted and thrust upward. Evidence of this exists on the top of Mt. Everest, the world's highest peak above sea level, where there are ancient marine fossils in abundance.
The Indo-Australian Plate continues to be driven northward, sliding under the Tibetan Plateau at the rate of about 6.7 cm (2.6 inches) per year and causes the Plateau to continue to be pushed upward. The Indo-Australian Plate has slowed to less than half of its original velocity, but it appears likely that it will continue moving northward for roughly another 10 million years, creating a Himalayan-like landscape as far north as 1500 km (930 miles) from the present range of mountains.
The Himalaya mountains were formed in a collision of the Indian Plate pushing into the Eurasian Plate, in a convergent boundary known as a continental collision.
Convergent boundary mountains are formed where two tectonic plates collide, causing one plate to be forced beneath the other in a process called subduction. This collision can lead to the formation of mountain ranges due to the intense pressure and folding of the Earth's crust. The Himalayas are a notable example of convergent boundary mountains, formed by the collision of the Indian Plate with the Eurasian Plate.
(A+LS) Convergent Boundary
The Himalayan Mountains are a result of the collision between the Indian Plate and the Eurasian Plate. This collision has led to the uplift of the mountains through convergent tectonic processes. The movement of the plates continues to push the mountains higher over time.
Although they aren't common, yes, transform faults can give rise to mountains. Most transform faults take place between oceanic crust, but an easy-to-see example is that of the San Andreas Fault giving rise to the San Gabriel Mountains.
The physical feature that formed the northeast boundary of Asoka's empire was the Himalayan mountain range.
Intercontinental convergent boundary.
convergent plate boundary
The collision boundary type modeled the formation of the Himalayan mountains, where the Indian tectonic plate collided with the Eurasian plate. This collision resulted in the uplift and formation of the massive mountain range.
The Himalayan mountain range is a specific geographic example of a feature formed at a convergent boundary between the Indian Plate and the Eurasian Plate. The collision of these two plates has led to the uplift and formation of one of the world's highest mountain ranges.
the himalaya mountains were formed in a collision at a convergent boundary
The type of boundary that the Andes mountains are, in South America, is a convergent plate boundary. This was formed from the collision of the South American plate boundary and the Nazca plate.
Mountains are formed at the boundary where tectonic plates collide or move apart.
The Himalaya mountains were formed in a collision of the Indian Plate pushing into the Eurasian Plate, in a convergent boundary known as a continental collision.
continental continental convergent boundary
Continental Collision Boundary
it contains mountains and volcanoes