The formation of Mount Everest is a remarkable geological process driven by plate tectonics, spanning tens of millions of years.
The Indian Plate, moving northward at relatively high speed, collided with the relatively stationary Eurasian Plate. This massive collision caused the landmasses to buckle and fold, initiating the formation of the Himalayan mountain range, including what would become Mount Everest.
As the Indian Plate continued its northward movement, it began subducting beneath the Eurasian Plate. This subduction process caused rocks on the descending plate to melt, releasing magma and heat. The rising magma uplifted the overlying crust, while the compressional forces folded and stacked rock layers, dramatically increasing mountain heights.
Over millions of years, the Himalayas have been subjected to intense erosion from wind, rain, and glacial activity. Glaciers carved deep valleys and cirques into the range. However, the tectonic uplift rate has generally exceeded erosion, allowing peaks like Everest to reach their current extreme elevations.
The mountain-building process continues today. The Indian Plate still moves northward at approximately 5 cm per year, causing ongoing uplift of the Himalayas. This movement also makes the region seismically active, with frequent earthquakes. However, the uplift rate is gradually slowing over geological time.
Mount Everest's summit consists of marine limestone from the ancient Tethys Ocean floor, pushed upward by these colossal tectonic forces—a testament to the dynamic nature of our planet's crust.