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Asteroids: Difference between revisions
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[[File:Ceres and Vesta, Moon size comparison.jpg|thumb|Vesta (left) and Ceres, the two largest objects in the asteroid belt between Mars and Jupiter, shown to scale with the Moon]] | [[File:Ceres and Vesta, Moon size comparison.jpg|thumb|Vesta (left) and Ceres, the two largest objects in the asteroid belt between Mars and Jupiter, shown to scale with the Moon]] | ||
{{Solar system}} | |||
The asteroid belt between [[Mars]] and Jupiter is what remains today of the planet [[Maldek]], destroyed when its lifewaves waged a war ending in nuclear annihilation. | The asteroid belt between [[Mars]] and [[Jupiter]] is what remains today of the planet [[Maldek]], destroyed when its lifewaves waged a war ending in nuclear annihilation. | ||
The existence of a planet between Mars and Jupiter was predicted by Johann Titius and restated in 1772 by German astronomer Johann Bode based on the numerical progression of the distances of the then-known planets from the sun. Following the discovery in 1781 of [[Uranus]], whose location conformed to Bode’s law, astronomers began to search for the missing planet, finding instead the asteroid belt. About 95 of the thousands of asteroids, or minor planets as they are called, that have since been discovered in our solar system are part of this main asteroid belt between [[Mars]] and [[Jupiter]]. | The existence of a planet between Mars and Jupiter was predicted by Johann Titius and restated in 1772 by German astronomer Johann Bode based on the numerical progression of the distances of the then-known planets from the sun. Following the discovery in 1781 of [[Uranus]], whose location conformed to Bode’s law, astronomers began to search for the missing planet, finding instead the asteroid belt. About 95 of the thousands of asteroids, or minor planets as they are called, that have since been discovered in our solar system are part of this main asteroid belt between [[Mars]] and [[Jupiter]]. | ||