Overview

The 4.5 billion-year-old Earth is the only known astronomical object to harbor life, giving rise to billions of species of stunning diversity, including ours, Homo sapiens. At 5.97 septillion kilograms and 40,000 kilometers in circumference, the third planet from the sun lies in the "Goldilocks zone," giving it the conditions needed to sustain liquid surface water.

1440 Findings

Hours of research by our editors, distilled into minutes of clarity.

  • Remnants of another planet that helped form the moon may be beneath Earth's surface

    Large mantle structures beneath Africa and the Pacific Ocean may be the buried remains of Thea, a large Mars-sized planet that collided with Earth. The theory is supported by isotopic evidence from volcanic and lunar rocks.

  • Humans have existed for just 0.004% of Earth’s history

    Born from the remains of the molecular cloud that birthed the sun, Earth experienced planetary-scale collisions, asteroid impacts, and lava seas. Life became possible after the planet cooled and formed a thin crust, atmosphere, and oceans.

  • Watch a visualization of the formation of the planets

    The nebular hypothesis proposes that a swirling cloud of gas and dust coalesced into a dense center, forming a star amid nuclear fusion. Lighter elements were blown far from the star while heavier elements remained nearby, serving as primary materials for terrestrial and jovian planets, respectively.

  • Scientists investigate Earth's interior by studying seismic waves

    Scientists investigate Earth's interior by studying seismic wavesBelow Earth's atmosphere lies the crust, which extends to the Mohorovičić discontinuity between five and 20 miles below Earth's surface. Below the crust lies the mantle, the liquid-metal outer core, and the solid inner core, which surpasses 5,200 degrees Celsius (9,392 degrees Fahrenheit).

  • The 'Goldilocks zone' is the region around a star where liquid water can exist

    Also referred to as the habitable zone, this region varies based on the properties of a planetary system's host star, including its size and luminosity, which measure the rate at which the star radiates energy per unit area.

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