Click on an object to jump to it: The Solar System

Our Sun Mercury Venus Earth The Moon Mars Jupiter Saturn Uranus Neptune The Solar System

Click to play sound

There are two basic types of planets, Earth-like (Terrestrial) planets and Jupiter-like (Jovian) planets. The Terrestrial planets are small, dense, rocky worlds. They are located in the inner part of the Solar System, they have solid surfaces, just a couple moons at most, rotate slowly, and have no rings around them.

The Jovian planets are large planets located in the outer part of the Solar System. The Jovian planets are gas giants, large objects made mostly of hydrogen and helium. They are much larger than terrestrial planets and are rapidly rotating objects. They all have rings, and extensive families of moons and no solid surface on which to stand on. The apparent visible surfaces are just the top layers of clouds in their atmospheres.

Our Sun

Our Sun

Click to play sound

The Sun is the center star of our Solar System. All of the planets, asteroids and comets revolve around the Sun. The Sun’s role as the center of the system comes from its high mass. It has 99.8% of the mass in the Solar System. The sun is a star, a hot ball of glowing gases. Without the sun’s intense energy and heat, there would be no life on Earth. And though it is special to us, there are billions of stars like our sun scattered across the Milky Way galaxy.

Quick Facts

Type Star G2V
Luminosity 3.83 x 1033 ergs/sec  
Visual Brightness (V) -26.74  
Absolute Magnitude 4.83  
Composition 92.1% Hydrogen, 7.8% Helium  
Temperature 5,504 °C 5777 K
Mass 1.989 x 1030 kg 333,060.402 x Earth
Equatorial Radius 695,508 km 109.2 x Earth
Gravity 274.0 m/s2  
Mean Rotation Period 25.38 Earth Days 609.12 Hours
Age 4.6 Billion Years  

Terrestrial Planets:

Mercury

Mercury

Click to play sound

Mercury is the closest planet to the Sun and smallest of the terrestrial planets. It has a very thin atmosphere, which is only a little more substantial than a vacuum.

Quick Facts

Type Terrestrial  
Mass 3.3010 x 1023 kg 0.055 x Earth
Diamiter 4,879 km  
Gravity 3.7 m/s2  
Surface Temperature -173 to + 427 °C 100 to 700 K
Rotation Period 58.646 Earth Days 1407.5 Hours
Atmosphere vacuum  
Ring System? No  
Global Magnetic Field? Yes  
No. of Moons 0  
Mean Distance from Sun 57,909,227 km 0.38709927 AU
Mean Orbit Velocity 170,503 km/h 4.7362 x 104 m/s
Orbit Period 88 Earth Days  

Venus

Venus

Click to play sound

Venus has a very thick atmosphere mostly composed of carbon dioxide gas. The thick carbon dioxide atmosphere traps heat from the Sun during the day and does not let the surface cool at night. The high temperature and unbreathable thick atmosphere would make the planet very inhospitable to human visitors.

Quick Facts

Type Terrestrial  
Mass 4.8673 x 1024 kg  
Diamiter 12,104 km  
Gravity 8.87 m/s2  
Surface Temperature 462 °C 735 K
Rotation Period -243.018 Earth Days -5832.4 Hours
Atmosphere Carbon Dioxide, Nitrogen CO2, N2
Ring System? No  
Global Magnetic Field? No  
No. of Moons 0  
Mean Distance from Sun 108,209,475 km 0.72333566 AU
Mean Orbit Velocity 126,074 km/h 3.5020 x 104 m/s
Orbit Period 224.7 Earth Days  

Earth

Earth

Click to play sound

Earth is our home planet. Most of its surface (over 70%) is covered with oceans, with the remainder featuring a wide variety of land forms, from mountains and valleys to plains and beaches. Earth has a thick atmosphere, which is mostly nitrogen (78%) and oxygen (21%). The region on and below the surface of Earth is filled with life which makes this planet unique.

Quick Facts

Type Terrestrial  
Mass 5.9722 x 1024 kg  
Diamiter 12,756 km  
Gravity 9.80665 m/s2  
Surface Temperature -88 to + 58 °C 185 to 331 K
Rotation Period 0.99726968 Earth Days 23.934 Hours
Atmosphere Nitrogen, Oxygen N2, O2
Ring System? No  
Global Magnetic Field? Yes  
No. of Moons 1  
Mean Distance from Sun 149,598,262 km 1 AU
Mean Orbit Velocity 107,218 km/h 2.9783 x 104 m/s
Orbit Period 1 Earth Years 365.2 Earth Days

The Moon

Earth's Moon

Click to play sound

The moon revolves around Earth and determines Earth’s tides. The Moon is our natural satellite. So far is the only object in space humans have travelled to. Neil Armstrong is the first human to step on the moon on 20th of July 1969: Neil Armstrong on the Moon

Quick Facts

Mass 7.3477 x 1022 kg  
Diamiter 3,475 km  
Gravity 1.624 m/s2 0.166 x Earth
Surface Temperature -233 to +123 °C 40 to 396 K
Rotation Period 27.322 Earth Days 655.73 Hours
Mean Distance from Earth 384,400 km 0.00257 AU
Mean Orbit Velocity 3,680.5 km/h 1,022 m/s
Orbit Period 0.074803559 Earth Years 27.322 Earth Days

Mars

Mars

Click to play sound

Mars is about half the size of Earth in diameter. Mars has a carbon dioxide atmosphere, but it is extremely thin. The thin air does not retain heat well. Mars has polar ice caps, made of water ice and carbon dioxide ice. The Martian surface has features that look like dry stream-beds, leading many researchers to suspect that at some time in the distant past, Mars may have had liquid water flowing on its surface.

Quick Facts

Type Terrestrial  
Mass 6.4169 x 1023 kg  
Diamiter 6,792 km  
Gravity 3.71 m/s2  
Surface Temperature -153 to +20 °C 120 to 293 K
Rotation Period 1.026 Earth Days 24.623 Hours
Atmosphere Carbon Dioxide, Nitrogen, Argon CO2, N2, Ar
Ring System? No  
Global Magnetic Field? No  
No. of Moons 2  
Mean Distance from Sun 227,943,824 km 1.523662 AU
Mean Orbit Velocity 86,677 km/h 2.4077 x 104 m/s
Orbit Period 687 Earth Days  

Jovian Planets:

Jupiter

Jupiter

Click to play sound

Jupiter is the largest planet in the Solar System. It is about 318 times as massive as Earth, and over 1,300 Earths could fit inside of it. Like all Jovian planets, Jupiter’s surface shows complicated wind patterns. Perhaps the most recognizable feature on Jupiter’s surface is the Great Red Spot, a huge storm, twice the diameter of Earth, which has been going on for at least 300 years.

Quick Facts

Type Jovian  
Mass 1.8981 x 1027 kg  
Diamiter 142,984 km  
Gravity 24.79 m/s2  
Temperature -148 °C 125 K
Rotation Period 0.41354 Earth Days 9.92496 Hours
Atmosphere Hydrogen, Helium H2, He
Ring System? Yes  
Global Magnetic Field? Yes  
No. of Moons 67  
Mean Distance from Sun 778,340,821 km 5.2028870 AU
Mean Orbit Velocity 47,002 km/h 1.3056 x 104 m/s
Orbit Period 4,331 Earth Days  

Saturn

Saturn

Click to play sound

Saturn is just a little smaller than Jupiter (its diameter is about 85% of Jupiter’s) but a lot lighter (its mass is about a third of Jupiter’s). This means that it has a very low density. In fact, its density is the lowest of all the planets and less than the density of water. In composition and internal structure, the planet is thought to be fairly similar to its larger sibling, Jupiter.

All Jovian planets are surrounded by a complex ring system made of icy particles. Saturn’s ring system is, by far, the most spectacular. The rings of the other Jovian planets are much thinner and fainter.

Quick Facts

Type Jovian  
Mass 5.6832 x 1026 kg  
Diamiter 120,536 km  
Gravity *10.4 m/s2  
Temperature -178 °C 95 K
Rotation Period 0.444 Earth Days 10.656 Hours
Atmosphere Hydrogen, Helium H2, He
Ring System? Yes  
Global Magnetic Field? Yes  
No. of Moons 62  
Mean Distance from Sun 1,426,666,422 km 9.53667594 AU
Mean Orbit Velocity 34,701 km/h 9.6391 x 103 m/s
Orbit Period 10,747 Earth Days  

* Derived from a 1 bar radius of 60,268 km.

Uranus

Uranus

Click to play sound

Uranus’s unique feature is that it appears to have been knocked over sometime in the past. Spinning perpendicular to it’s orbit. Most planets orbit around the Sun spinning upright. The cause of this is not yet certain, but it has been suggested that it was caused by an impact of a large object, such as a large asteroid or moon. Giant impacts like this were common during the early history of the Solar System; a similar impact is thought to have created the Earth’s Moon.

Quick Facts

Type Jovian  
Mass 8.6810 x 1025 kg  
Diamiter 51,118 km  
Gravity 8.87 m/s2  
Temperature -216 °C 57 K
Rotation Period -0.718 Earth Days -17.23992 Hours
Atmosphere Hydrogen, Helium, Methane H2, He, CH4
Ring System? Yes  
Global Magnetic Field? Yes  
No. of Moons 27  
Mean Distance from Sun 2,870,658,186 km 19.189165 AU
Mean Orbit Velocity 24,477 km/h 6.7991 x 103 m/s
Orbit Period 30,589 Earth Days  

Neptune

Neptune

Click to play sound

Neptune is similar in size to Uranus. Giant storm centers can be seen on its visible surface, similar to those on the other Jovian planets. The atmosphere features great wind patterns; its winds are the fastest in the Solar System, reaching speeds of 2,000 km/hour (or 1,200 miles/hour).

Quick Facts

Type Jovian  
Mass 1.0241 x 1026 kg  
Diamiter 49,528 km  
Gravity 11.15 m/s2  
Temperature -214 °C 59 K
Rotation Period 0.671 Earth Days 16.11000 Hours
Atmosphere Hydrogen, Helium, Methane H2, He, CH4
Ring System? Yes  
Global Magnetic Field? Yes  
No. of Moons 14  
Mean Distance from Sun 4,498,396,441 km 30.069923 AU
Mean Orbit Velocity 19,566 km/h 5.4349 x 103 m/s
Orbit Period 59,800 Earth Days  

Additional Resources

Earth at night as seen from ISS

Solar Flares

Earth 360 degrees

Jupiter

stars.chromeexperiments.com

joshworth.com/dev/pixelspace/pixelspace_solarsystem.html

NASA Eyes simulation

Test Yourself

Match the names with the images.

Sun
Mercury
Venus
Earth
Mars
Jupiter
Saturn
Uranus
Neptune
Our Sun
Mercury
Venus
Earth
Mars
Jupiter
Saturn
Uranus
Neptune