The Solar system

We live on the third planet from the Sun, in a system that contains a smallish star, a few small rocky planets, gas giant planets complete with their own systems of moons, and various smaller objects like minor planets, rocky asteroids, icy comets, meteors and even smaller bits of dust and gas.

 

We will begin this section of our study by taking stock of the general makeup and composition of our solar system. We will need to make sense of the stark  differences between terrestrial planets and gas giants, and their placement in our system.

 

We will use our observations of the solar system to build a model of how it must have evolved. Our model will eventually need to explain not only the characteristics of our own solar system, but also the characteristics of other systems of planets we have observed, orbiting distant stars. Some of these extrasolar systems exhibit traits very unlike our own, so our model will need to be very robust in explaining how these different types of systems could have formed.

Solar system

This artist's conception from NASA compares what a planetary system orbiting a brown dwarf might look like in comparison to our own solar system. Since a brown dwarf star is smaller than our Sun, the planets would orbit much closer to the star.

 

The image also shows the main layout of our solar system, with small terrestrial planets close to the Sun and gas giants farther out, in more widely-spaced orbits. The distances are not to scale.

relative sizes of the planets

The above image compares the relative sizes of the planets. Note the stark contrast of the gas giant planets, compared to the much smaller terrestrial planets.

relative sizes of planets and sun

This image shows the relative size of the Sun, compared to the planets. The sun contains some 99% of the mass of the solar system, even counting the asteroids and comets as well as the planets. Jupiter is the second largest body in our solar system, and it is tiny compared to the Sun.

This video gives a nice comparison of the sizes of the planets, and continues on to show how the Sun compares in size to some other stars.

Terrestrial vs. Jovian planets

Terrestrial planets are small, rocky planets. In our solar system, the terrestrial planets are Mercury, Venus, Earth and Mars. Gas giant planets are often called "Jovian" planets, after the largest gas giant planet in our solar system, Jupiter. The Jovian planets in our solar system are Jupiter, Uranus, Saturn and Neptune. Pluto was considered a planet until Aug. 4, 2006 when it was reclassified as a "dwarf planet."

Terrestrial

 

close to the sun

closely spaced orbits

small mass

small size

low escape speed

mostly rocky

high density

slow rotation

weak magnetic field

few moons

no rings

Gas giant

 

far from the sun

widely spaced orbits

large mass

large size

high escape speed

mostly gaseous

low density

fast rotation

strong magnetic field

many moons

rings

The planets lie close to the ecliptic, or the plane of Earth's orbit about the Sun. The planes of the other planets' orbits do not lie exactly in the same plane, but are within a few degrees, so the planets do not typically line up exactly.

 

Since Mercury and Venus are closer to the Sun than Earth is, they are always close to the horizon. Planets that are located farther away from the Sun than Earth can be found higher in the sky.

 

Once in awhile, the planets appear close together in the sky. In the above photo, five planets appear relatively close to each other. Of course, Saturn is really much farther away than Mars but here they lie in the same direction. An alignment of all eight planets and Pluto is very rare, happening only onec in about 500 years.