Return to the Sea and Sky Home Page Return to Home Page Explore the Seas and Oceans Explore the Universe and Solar System Return to the Sky Menu
Return to the Sea and Sky Home Page
About Sea and Sky What's New at Sea and Sky Frequently Asked Questions
Sea and Sky Awards Sign Our Guest Book Search Sea and Sky Contact Sea and Sky Advertise on Sea and Sky
Return to the Sky Menu
Return to the Sea and Sky Home Page
Return to Tour of the Solar System  
 
 
The Sun
Mercury
Venus
Earth
Mars
Asteroids
Jupiter
Saturn
Uranus
Neptune
Pluto
Comets
Mars Symbol

Mars

Mars Global Surveyor photo of Mars Viking orbiter close-up of Olympus Mons on Mars Mars Reconaissance Orbiter view of Victoria Crater on Mars
Mars Global Surveyor photo
of the planet Mars
(NASA/JPL)
Viking orbiter close-up of the Olympus Mons vlocano on Mars
(NASA/JPL)
Mars Reconaissance Orbiter view of Victoria Crater on Mars
(NASA/JPL/University of Arizona)




God of War

With the Terran system well behind us, we next encounter a beautiful, bright red world. This is the planet Mars, and it is the fourth planet from the Sun. It was named after the Roman god of war because its color reminded observers of a bloody Roman battlefield. Early astronomers believed they could see faint, dark lines crossing the surface of the planet. Some believed these to be artificially built canals. This gave rise to some of the early speculation of intelligent life on Mars. These lines were later found to be an optical illusion. Later unmanned missions to the planet found no evidence of the so-called canals. Still, there is perhaps no other body in the Solar System that has intrigued us more than Mars. To this very day, it is still one of the most likely candidates for extraterrestrial life. In fact, meteorites recently discovered in Antarctica are believed to have originated from the red planet. These ancient Martian rocks may contain fossils of tiny bacteria. If this turns out to be true, it will be the first evidence that life evolved on other planets besides Earth.


Mars Pathfinder image of the rocky Martian surface Spirit rover image of a feature known as Husband Hill Opportunity rover image of Cape St. Vincent in Victoria Crater
Mars Pathfinder image of the rocky Martian surface
(NASA/JPL)
Spirit rover image of a feature known as "Husband Hill"
(NASA/JPL-Caltech/Cornell)
Opportunity rover image of Cape St. Vincent in Victoria Crater
(NASA/JPL/Cornell)


The Red Planet

The bright red color of Mars has earned it the name of red planet. This unique color is caused by the chemistry of its surface. Mars does have a thin atmosphere, which helps cause iron compounds to oxidize. It is this iron oxide in the rocks and sand that gives the planet it reddish-brown color. It could very appropriately be called the "rusty" planet. We have learned a great deal about Mars in the last few decades. Several unmanned space missions have been sent to explore the red planet. Several Mariner spacecraft orbited the planet in the mid and late 1960's. In 1975, two Viking spacecraft landed on the surface, sending back the first color pictures of this alien world. Recently, the Mars Pathfinder mission visited the planet. A small roving vehicle known as the Sojourner Rover explored the surface sending back the sharpest pictures to date. Scientists continue to be fascinated with Mars because of its similarities to Earth. Some have even suggested that we may be able to colonize the planet in the not too distant future. If the planet does turn out to be completely lifeless, it may be a candidate for a process known as terraforming. This process would involve using various chemical and biological means to make the planet warmer and the atmosphere more hospitable for human life.


Panoramic view of Victoria Crater taken by the Exploration Rover Opportunity
Panoramic view of Victoria Crater taken by the Exploration Rover Opportunity
(NASA/JPL)

Features of Mars

Mars is a small, rocky world about half the size of Earth. As small as it is, however, it is a planet of extremes. Mars is the home of the largest known volcano in the Solar System. Olympus Mons is an extinct volcanic crater that rises 15 miles above the Martian surface. That is over twice the height of the tallest mountain on Earth, Mt. Everest. It is a scar so large it can be seen from Earth. Another gigantic feature of the red planet is Valles Marinares. This is the Martian equivalent of the Grand Canyon. This one is much bigger, however. Valles Marinares stretches 3000 miles (4829 km) along the surface of Mars and is 435 miles (700 km) wide at its widest point. If this canyon existed on Earth, it would stretch across the continental United States from coast to coast! During the Martian winters, the poles of the planet are covered with large sheets of water ice. Several features that resemble riverbeds suggest that there may have been running water on Mars at one time. The thin atmosphere of Mars is composed mainly of carbon dioxide. Winds of up to 300 miles per hour whip up enormous dust storms that constantly erode and reshape the surface of the planet. With an average surface temperature of 60 degrees below zero, it may not seem very hospitable. But with its thin atmosphere and abundance of water, Mars remains the most likely candidate for life anywhere in the Solar System. A future manned mission to the planet is in the works. Only then will we be able to tell if the red planet is really a dead planet.

 

Statistics for Mars
Diameter ...... 4220 miles (6794 km)
Number of Natural Satellites ...... 2
Mean Distance from the Sun ...... 141,050,000 miles (227,940,000 km)
Rotational Period ...... 24.62 hours
Orbital Period ...... 687 days
Orbital Eccentricity ...... 0.093
Orbital Inclination ...... 1.85 degrees
Inclination of Axis ...... 23.98 degrees
Mean Surface Temperature ...... -81° F (-63° C)
Main Atmospheric Component ...... Carbon Dioxide
Atmospheric Pressure ...... 0.007 bars
Atmospheric Depth ...... 100 miles (161 km)
Apparent Magnitude ...... -2.01

 

The Moons of Mars
Name    Radius (km)    Distance (km) Year
   Discovered  
Phobos  13.5x10.8x9.4 9,380 1877
Deimos 7.5x6.1x5.5 23,460 1877
       

 

Return to the Martian System Continue to Phobos