Asteroid Basics

Asteroid Basics - Introduction

21396 views December 26, 2015 asteroidday 197

The following information was kindly provided to us by our partner, NEOShield-2.

For billions of years before Hollywood made the blockbuster movie Deep Impact, Near-Earth Objects (NEOs) have bombarded the Earth. According to the popular “giant impact theory,” our young Earth (around 50 million years old) was hit by another planet estimated to be about the size of Mars, creating our Moon. Since then, Earth has witnessed the impact of millions of NEOs of varying sizes and frequency. While astronomers and astrobiologists are divided on the details, it is generally believed that water and hydrocarbons brought to the Earth by NEOs played a significant role in the origins of life.

Our planet orbits the Sun among a swarm of asteroids whose orbits cross (or nearly cross) Earth’s orbit. These are not the asteroids that make up the asteroid belt between Mars and Jupiter, but rather the near-Earth asteroids whose orbits take them much closer to the Sun, and who regularly approach the orbit of Earth.  These asteroids are remnants of the formation of our solar system, and range in size from pebbles to many miles across.

NEOs can also be Comets. Composed mostly of water ice with embedded dust particles, comets originally formed in the cold outer planetary system while most of the rocky asteroids formed in the warmer inner solar system between the orbits of Mars and Jupiter.