What Will Earth Look Like in 500 Million Years?

The deep future of Earth, viewed across geological time, reveals a planet in a state of continuous, slow-motion transformation. Over the next 500 million years, the forces that shape our world—plate tectonics and stellar evolution—will drive changes that fundamentally alter the planet’s surface and habitability. These processes will ultimately result in an environment unrecognizable from the one we inhabit today. Five hundred million years is a vast expanse of time, nearly equivalent to the entire history of complex animal life on Earth, and it will witness the planet’s final transformation before the Sun enters its more destructive phases.

The Next Supercontinent

Earth’s continents are constantly shifting across the mantle in a pattern known as the supercontinent cycle. This cycle, also referred to as the Wilson Cycle, sees the dispersal and reassembly of all major landmasses roughly every 300 to 500 million years. By the 500-million-year mark, the current continental arrangement will be re-forged into a new, single landmass, often referred to as Pangaea Ultima.

The formation of this massive continent is predicted to involve the closure of the Atlantic and Indian Oceans. North and South America will eventually collide with Africa and Eurasia, stitching the current continents back together into one colossal landform. This tectonic convergence will be marked by intense mountain-building events, creating vast, high ranges where today’s ocean basins lie.

This single landmass will profoundly change global geography and the planet’s weather systems. The vast, unbroken continental interior will lead to extreme aridity and temperature swings far from coastal areas. Shallow inland seas, which are biologically productive and regulate global climate, will largely disappear as the continental shelves are uplifted and fused.

Solar Evolution and Increased Heat

The Sun is the primary external driver of the planet’s long-term environmental change. As a main-sequence star, the Sun steadily converts hydrogen into helium in its core, a process that increases its energy output over cosmic timescales. The accumulation of denser helium “ash” causes the core to contract, raising the temperature and pressure in the surrounding layer where hydrogen fusion occurs.

This increased rate of fusion means the Sun is getting brighter and hotter with age. Within the next 500 to 600 million years, the Sun’s luminosity is projected to increase by approximately 5% to 6% compared to its current output. This increase in stellar radiation will have catastrophic consequences for Earth’s surface temperature.

The additional solar energy reaching the planet will initiate global warming that is not reversible by natural planetary feedback mechanisms. This steady rise in heat marks the beginning of the end of Earth’s era as a habitable world. The increased solar flux triggers the subsequent atmospheric and hydrological collapse.

Atmospheric and Ocean Collapse

The combined effects of the supercontinent formation and increased solar heat will trigger catastrophic environmental feedback loops. A significant consequence will be the disruption of the carbonate-silicate weathering cycle, which acts as Earth’s long-term thermostat by regulating atmospheric carbon dioxide. Silicate weathering occurs when atmospheric carbon dioxide dissolves in rainwater to form carbonic acid, which reacts with silicate rocks to lock the carbon away as carbonate minerals.

The formation of Pangaea Ultima will dramatically reduce active continental margins and diminish global volcanism, which recycles carbon dioxide back into the atmosphere. Simultaneously, rising global temperature will accelerate the weathering process, stripping the atmosphere of carbon dioxide at an unsustainable rate. This will cause atmospheric carbon dioxide levels to fall below the threshold required for C3 photosynthesis, leading to the global extinction of most trees and plant life.

As the temperature rises, the oceans will begin to evaporate on a massive scale. The increased heat will drive a “moist greenhouse” effect, where large amounts of water vapor rise into the upper atmosphere. There, solar ultraviolet radiation will break down the water molecules into hydrogen and oxygen. The light hydrogen atoms will then escape into space, permanently removing water from the planet.

This runaway evaporation will lead to the complete loss of liquid surface water, leaving behind a superheated, dense atmosphere rich in water vapor but with no surface ocean. Without liquid water, the process of plate tectonics will likely cease entirely, as water is required to lubricate the subduction zones. The planet will become a dry, scorched world with a thick, Venus-like atmosphere, from which recovery is impossible.

The Final State of Life

The loss of atmospheric carbon dioxide and global superheating will precipitate a mass extinction event far surpassing any in Earth’s history. The failure of C3 photosynthesis will cause the collapse of nearly all terrestrial ecosystems, leading to the rapid extinction of most plant and all animal life that depends on them. Land animals, including all mammals, will be unable to survive the prolonged, extreme temperatures and the disappearance of their food sources.

Even the oceans, initially a refuge, will succumb to the rising heat and eventual evaporation. Complex marine life will face thermal stress and anoxia before the water disappears entirely, leaving only the most resilient organisms. The only life forms predicted to persist in this desolate future are specialized extremophiles.

These hardy microorganisms, such as hyperthermophiles, may find sanctuary deep within the planet’s crust, utilizing chemosynthesis near geothermal vents, or surviving in rare pockets of liquid water underground. The surface of Earth will be sterilized, transformed into a barren, orange-red desert exposed to intense heat and radiation. By 500 million years, the planet will be largely devoid of any complex, multicellular life.