Nebular Hypothesis Overview
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Nebular Hypothesis Overview

Created by
@ResoundingHeptagon

Questions and Answers

The solar system evolved from a ______ that disintegrated due to the fall of its own gravity.

nebula

Matter began to move in a giant circular manner as the cloud continued to spin and contract, forming a disk with a ______ in the middle.

lump

The center contained high energy causing ______ reactions.

nuclear

The disk edge emerged much cooler than the center due to the great distance from the ______.

<p>sun</p> Signup and view all the answers

A ______ is a chunk of rock that orbits the sun.

<p>asteroid</p> Signup and view all the answers

A ______ is a cosmic snowball of rocks, dusts, and frozen gases that grows tails as it approaches the sun.

<p>comet</p> Signup and view all the answers

Similar to planet Uranus and Neptune, the ______ planet is known as a gaseous planet.

<p>ninth</p> Signup and view all the answers

Konstantin Batygin and Mike Brown are researchers of the ______.

<p>ninth planet</p> Signup and view all the answers

Study Notes

Nebular Hypothesis

  • Solar system formation traces back 4.5 billion years to a nebula disintegrating under its own gravity.
  • The initial cloud comprised light elements, with trace amounts of heavier ones.
  • Gravity-induced contraction led to denser atom formation through atomic clumping.
  • Matter circulated in a massive whirl, resulting in a flattened disk with a central lump as the cloud continued to spin.
  • Approximately 50 million years of high energy buildup in the center sparked nuclear reactions.
  • The Sun and disk cooled down within a few thousand years; outer disk temperatures were significantly lower due to distance.
  • Temperature variations led to the solidification of materials into various types: dust-like particles, rocky dust, and icy particles with water and frozen gases.
  • Planet formation took around 500 million years in total.

Definition of Terms (Space Objects)

  • Asteroid: A rocky fragment orbiting the sun.
  • Comet: A "cosmic snowball" made of rock, dust, and frozen gases; develops a tail when near the sun.
  • Meteor: Referred to as a "shooting star," this is a small debris piece entering a planet's atmosphere, leaving a bright tail.
  • Meteorites: Fragments of meteors that survive passage through the atmosphere and reach the ground.
  • Planet: A substantial celestial body that revolves around the Sun within the solar system.
  • Moon: Also called a satellite, it is a solid body, some possessing an atmosphere, formed from gas discs surrounding planets.

Ninth Planet

  • Known as "Planet Nine," it is akin to Uranus and Neptune, categorized as a gaseous planet.
  • Evidence for its existence comes from tracing its highly elongated orbit in the outer solar system.
  • Researchers Konstantin Batygin and Mike Brown are prominent figures in the search for Planet Nine.

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Description

This quiz explores the Nebular Hypothesis, explaining how our solar system evolved from a disintegrating nebula around 4.5 billion years ago. It discusses the process of cloud contraction due to gravity and the resulting formation of denser atoms. Dive into the fascinating journey of matter as it transitioned into a spinning disk that eventually formed our solar system.

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