Friday, March 4, 2016

Formation of the Solar System

~ 4.6 billion years ago huge cloud of gas and dust started collapsing gravitationally

• As it collapsed it spun faster (conservation of angular momentum)

• No (or little) spin in the perpendicular plane

• Local clusters of dust and gas condensed - protosun formed first

• As material cooled, it condensed but never stopped rotating (rotates still since there’s nothing to stop it)

• Cores probably formed first, then attracted neighboring materials to form:  planetesimal, protoplanet

• Probably not a unique system - there is increasing evidence for the existence of many other planetary systems

• Still an evolving theory

• All planets revolve around the sun in the same direction, but 3 have different directions of rotation (relative to the rest and to the direction of solar system motion) - Uranus, Venus, (Pluto)


The Terrestrial Planets:  Mercury, Venus, Earth, and Mars

Relative Characteristics:

Planet         Distance        Period          Radius          Mass

Mercury      0.4               0.24             0.38             0.055
Venus         0.7               0.62             0.95             0.82
Earth          1                  1                 1                 1
Mars           1.5               1.88            0.53             0.11

The Jovian Planets (gas giants)

Jupiter        5.2               11.9            11.2            318
Saturn        9.5               29.5            9.3              95
Uranus       19                84               4.0             14.6
Neptune     30                165             3.9              17.2

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