The oldest rocks from space are dated back to about 4.5 billion years ago, so this is around when our planet would have formed. The entire Solar System (which includes the Earth) arose when a giant cloud of gas and dust called a nebula began to collapse under its own gravity. This probably happened when, about five billion years ago, a nearby star exploded in a supernova, releasing a shockwave that caused the cloud to contract. Most of the gas gathered in the center to form the Sun, while the rest flattened out into a spinning disk.
The heavier, metallic elements existed closer to the Sun and would form the terrestrial planets. Through gravity, dust particles within the protoplanetary disk began to stick together, growing into pebbles, then boulders, then planetesimals. These chunks of rock collided with one another and clumped together to form larger and larger bodies. This is called accretion: when an object grows in size and mass by gravitationally collecting the material around it. Slowly, over millions of years, Earth formed by this process.
Our planet started out as a hot mass of scorched rock. Volcanic outgassing created the early atmosphere, but it contained almost no oxygen and would have been toxic to humans and most modern life. Much of the Earth was still molten because of extreme volcanism and frequent collisions with other bodies. One very big collision is thought to have been responsible for creating the Moon and tilting the Earth at an angle. Over time, such cosmic bombardments ceased, allowing our planet to cool and form a solid crust. Water that was brought here by comets and asteroids condensed into clouds and the oceans took shape. Earth was finally hospitable to life, and the earliest forms that arose enriched the atmosphere with oxygen.
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Earth was formed by collisions within the giant disc-shaped cloud of material. Gravity gathered the dust and gas together into clumps.
To determine if an Earth-like planet is geologically alive or dead, observations of tectonic activity, such as volcanic eruptions, earthquakes, and mountain building, are needed. Detecting the presence of a magnetic field can also indicate a planet's geologic activity, as it is generated by a molten outer core. Additionally, analyzing surface features like rift valleys, plate boundaries, and uplifted mountain ranges can provide clues to the planet's geological history and current activity.
in aprox 2.5 billion years due to the solidification of earth molten core, unlike mars who's core has already solidifyed resulting in the dead planet we see today
Er ... which planet exactly do you think that we come from? As far as science can discover, Earth IS the only planet with life on it, so you're asking how far Earth is from Earth.
mars
Mars is no longer geologically active because it has a smaller core compared to Earth, leading to a diminished internal heat source. This lack of heat prevents the movement of molten rock within the planet, inhibiting the formation of geological features like volcanoes or tectonic activity. Without these processes, Mars remains geologically inactive.
The Earth is geologically active due to the convection of heat from the planet's interior.
It describes the ongoing changes to the surfaces of terrestrial worlds. This is because terrestrial surfaces change over time. The moon and mercury are considered geologically dead because their surfaces have remained the same for billions of years.
No. Smaller planets become geologically dead sooner. A larger planet has a larger volume and thus a larger heat reservoir than a smaller planet and so can remain geologically active for longer.
Earth is the only geologically active planet among the terrestrial planets. There are some geologically active moons in orbit around the gas giants. Enceladus is quite an interesting moon of Saturn.
The Moon is not a planet, it, as the name suggest, is a moon.It is not geologically active anymore.
An adverb form of the noun "geology" would be "geologically," as in, 'The San Andreas Fault is a geologically active region.'
Mercury has no atmosphere, and its surface is heavily cratered much like Earth's moon. It is estimated that the planet has been geologically dormant for a few billion years.
To determine if an Earth-like planet is geologically alive or dead, observations of tectonic activity, such as volcanic eruptions, earthquakes, and mountain building, are needed. Detecting the presence of a magnetic field can also indicate a planet's geologic activity, as it is generated by a molten outer core. Additionally, analyzing surface features like rift valleys, plate boundaries, and uplifted mountain ranges can provide clues to the planet's geological history and current activity.
It is the only planet that has life form on it.
in aprox 2.5 billion years due to the solidification of earth molten core, unlike mars who's core has already solidifyed resulting in the dead planet we see today
Er ... which planet exactly do you think that we come from? As far as science can discover, Earth IS the only planet with life on it, so you're asking how far Earth is from Earth.
mars