Our solar system has at its center, an average star we call the Sun. In orbit
around the Sun are the nine planets: Mercury, Venus,
Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto .
There are also many
comets, asteroids, satellites of the planets, and background dust in the
solar system.
The Sun contains 99.85% of all the matter in the Solar System. The planets, which
condensed out of the same disk of material that formed the Sun, contain only 0.135% of
the mass of the solar system. Jupiter contains more than twice the matter of all the other
planets combined. Satellites of the planets, comets, asteroids, meteoroids, and the
interplanetary medium constitute the remaining 0.015%.
Below is an image containing pictures (from spacecraft missions) of the nine planets (drawn to scale, that is, the relative sizes of one planet to another planet are correct).
The terrestrial planets are the four innermost planets in the solar
system, Mercury, Venus,
Earth and Mars. They are called terrestrial because they have a compact, rocky surface
like the Earth's. The planets, Venus, Earth, and Mars have significant atmospheres while
Mercury has almost none. Below is a close-up picture of the four terrestrial
planets
Jupiter, Saturn, Uranus, and Neptune are known as the Jovian (Jupiter-like) planets ,
because they are all gigantic compared with Earth, and they have a gaseous nature like
Jupiter's. The Jovian planets are also referred to as the gas giants, although some or all of
them might have small solid cores.
| Orbital Distance (10^6 km) | Radius (km) | Mass (10^24 kg) |
Rotation Period (hours) | # Moons | Orbital Period (days) | Density (g/cm3) | |
| Mercury | 57.9 | 2439 | .3302 | 1407.6 | 0 | 88. | 5.43 |
|---|---|---|---|---|---|---|---|
| Venus | 108.2 | 6052 | 4.869 | 5832.5 | 0 | 224.7 | 5.25 |
| Earth | 149.6 | 6378 | 5.975 | 23.93 | 1 | 365.2 | 5.52 |
| Mars | 227.9 | 3393 | 0.6419 | 24.62 | 2 | 687. | 3.95 |
| Jupiter | 778.3 | 71492 | 1898.6 | 9.92 | 16 | 4330.6 | 1.33 |
| Saturn | 1427 | 60268 | 568.5 | 10.5 | 18 | 10747. | 0.69 |
| Uranus | 2869.6 | 25559 | 86.83 | 17.24 | 15 | 30588. | 1.29 |
| Neptune | 4496.6 | 24766 | 102.43 | 16.11 | 8 | 59800. | 1.64 |
| Pluto | 5913.5 | 1137 | 0.0125 | 153.1 | 1 | 90591. | 2.03 |
ACTIVITIES:
Using the information from the above table (and images), please answer the following questions:
A: Looking at the Radius column of the table, and the picture of the terrestrial planets, the answer is Venus .
A: Mars . The period of rotation is the time it takes for the planet to spin 360 degrees on its axis--- in other words, it's the length of our day. A day on Mars would be just about as long as it is on the Earth.
A: Jupiter .
A: Jupiter's radius is 71492 km and the Earth's is 6378 km, making Jupiter more than 11 times larger than the Earth.
The following diagram shows the approximate distance of the terrestrial planets to the Sun.
The following diagram shows the approximate
distance of the Jovian planets to the Sun.
ACTIVITIES:
Using the Orbital Distance column in the table, make two graphs similar to the plots shown above:
HINT: As in the example below, plot Orbital Distance in units of
10^6 km (that is, millions of kilometers).
Sample Plot:
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Galileo Solid State Imaging Team Leader: Dr. Michael J. S. Belton
The SSI Education and Public Outreach webpages were originally created and managed by Matthew Fishburn and Elizabeth Alvarez with significant assistance from Kelly Bender, Ross Beyer, Detrick Branston, Stephanie Lyons, Eileen Ryan, and Nalin Samarasinha.
Last updated: September 17, 1999, by Matthew Fishburn
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