Mars Facts

The red planet is dusty, cold world with a thin atmosphere and is home to four NASA robots.

Mars is the fourth planet from the Sun and the seventh largest:

Planet Profile

orbit: 227,940,000 km (1.52 AU) from Sun
diameter: 6,794 km
mass: 6.4219e23 kg

History of Mars

Mars (Greek: Ares) is the god of War. The planet probably got this name due to its red color; Mars is sometimes referred to as the Red Planet. (An interesting side note: the Roman god Mars was a god of agriculture before becoming associated with the Greek Ares; those in favor of colonizing and terraforming Mars may prefer this symbolism.) The name of the month March derives from Mars.

Mars has been known since prehistoric times. Of course, it has been extensively studied with ground-based observatories. But even very large telescopes find Mars a difficult target, it’s just too small. It is still a favorite of science fiction writers as the most favorable place in the Solar System (other than Earth!) for human habitation. But the famous “canals” “seen” by Lowell and others were, unfortunately, just as imaginary as Barsoomian princesses.

The first spacecraft to visit Mars was Mariner 4 in 1965. Several others followed including Mars 2, the first spacecraft to land on Mars and the two Viking landers in 1976. Ending a long 20 year hiatus, Mars Pathfinder landed successfully on Mars on 1997 July 4. In 2004 the Mars Expedition Rovers “Spirit” and “Opportunity” landed on Mars sending back geologic data and many pictures; they are still operating after more than three years on Mars. In 2008, Phoenix landed in the northern plains to search for water. Three Mars orbiters (Mars Reconnaissance OrbiterMars Odyssey, and Mars Express) are also currently in operation.

Mars’ orbit is significantly elliptical. One result of this is a temperature variation of about 30 C at the subsolar point between aphelion and perihelion. This has a major influence on Mars’ climate. While the average temperature on Mars is about 218 K (-55 C, -67 F), Martian surface temperatures range widely from as little as 140 K (-133 C, -207 F) at the winter pole to almost 300 K (27 C, 80 F) on the day side during summer.

Though Mars is much smaller than Earth, its surface area is about the same as the land surface area of Earth.

Mars has some of the most highly varied and interesting terrain of any of the terrestrial planets, some of it quite spectacular:

  • Olympus Mons: the largest mountain in the Solar System rising 24 km (78,000 ft.) above the surrounding plain. Its base is more than 500 km in diameter and is rimmed by a cliff 6 km (20,000 ft) high.
  • Tharsis: a huge bulge on the Martian surface that is about 4000 km across and 10 km high.
  • Valles Marineris: a system of canyons 4000 km long and from 2 to 7 km deep (top of page);
  • Hellas Planitia: an impact crater in the southern hemisphere over 6 km deep and 2000 km in diameter.

Much of the Martian surface is very old and cratered, but there are also much younger rift valleys, ridges, hills and plains. (None of this is visible in any detail with a telescope, even the Hubble Space Telescope; all this information comes from the spacecraft that we’ve sent to Mars.)

The southern hemisphere of Mars is predominantly ancient cratered highlands somewhat similar to the Moon. In contrast, most of the northern hemisphere consists of plains which are much younger, lower in elevation and have a much more complex history. An abrupt elevation change of several kilometers seems to occur at the boundary. The reasons for this global dichotomy and abrupt boundary are unknown (some speculate that they are due to a very large impact shortly after Mars’ accretion). Mars Global Surveyor has produced a nice 3D map of Mars that clearly shows these features.

The interior of Mars is known only by inference from data about the surface and the bulk statistics of the planet. The most likely scenario is a dense core about 1700 km in radius, a molten rocky mantle somewhat denser than the Earth’s and a thin crust. Data from Mars Global Surveyor indicates that Mars’ crust is about 80 km thick in the southern hemisphere but only about 35 km thick in the north. Mars’ relatively low density compared to the other terrestrial planets indicates that its core probably contains a relatively large fraction of sulfur in addition to iron (iron and iron sulfide).

Like Mercury and the Moon, Mars appears to lack active plate tectonics at present; there is no evidence of recent horizontal motion of the surface such as the folded mountains so common on Earth. With no lateral plate motion, hot-spots under the crust stay in a fixed position relative to the surface. This, along with the lower surface gravity, may account for the Tharis bulge and its enormous volcanoes. There is no evidence of current volcanic activity. However, data from Mars Global Surveyor indicates that Mars very likely did have tectonic activity sometime in the past.

There is very clear evidence of erosion in many places on Mars including large floods and small river systems. At some time in the past there was clearly some sort of fluid on the surface. Liquid water is the obvious fluid but other possibilities exist. There may have been large lakes or even oceans; the evidence for which was strenghtened by some very nice images of layered terrain taken by Mars Global Surveyor and the mineralology results from MER Opportunity. Most of these point to wet episodes that occurred only briefly and very long ago; the age of the erosion channels is estimated at about nearly 4 billion years. However, images from Mars Express released in early 2005 show what appears to be a frozen sea that was liquid very recently (maybe 5 million years ago). Confirmation of this interpretation would be a very big deal indeed! (Valles Marineris was NOT created by running water. It was formed by the stretching and cracking of the crust associated with the creation of the Tharsis bulge.)

Early in its history, Mars was much more like Earth. As with Earth almost all of its carbon dioxide was used up to form carbonate rocks. But lacking the Earth’s plate tectonics, Mars is unable to recycle any of this carbon dioxide back into its atmosphere and so cannot sustain a significant greenhouse effect. The surface of Mars is therefore much colder than the Earth would be at that distance from the Sun.

Mars has a very thin atmosphere composed mostly of the tiny amount of remaining carbon dioxide (95.3%) plus nitrogen (2.7%), argon (1.6%) and traces of oxygen (0.15%) and water (0.03%). The average pressure on the surface of Mars is only about 7 millibars (less than 1% of Earth’s), but it varies greatly with altitude from almost 9 millibars in the deepest basins to about 1 millibar at the top of Olympus Mons. But it is thick enough to support very strong winds and vast dust storms that on occasion engulf the entire planet for months. Mars’ thin atmosphere produces a greenhouse effect but it is only enough to raise the surface temperature by 5 degrees (K); much less than what we see on Venus and Earth.

Early telescopic observations revealed that Mars has permanent ice caps at both poles; they’re visible even with a small telescope. We now know that they’re composed of water ice and solid carbon dioxide (“dry ice”). The ice caps exhibit a layered structure with alternating layers of ice with varying concentrations of dark dust. In the northern summer the carbon dioxide completely sublimes, leaving a residual layer of water ice. ESA’s Mars Express has shown that a similar layer of water ice exists below the southern cap as well. The mechanism responsible for the layering is unknown but may be due to climatic changes related to long-term changes in the inclination of Mars’ equator to the plane of its orbit. There may also be water ice hidden below the surface at lower latitudes. The seasonal changes in the extent of the polar caps changes the global atmospheric pressure by about 25% (as measured at the Viking lander sites).

Recent observations with the Hubble Space Telescope have revealed that the conditions during the Viking missions may not have been typical. Mars’ atmosphere now seems to be both colder and dryer than measured by the Viking landers (more details from STScI).

The Viking landers performed experiments to determine the existence of life on Mars. The results were somewhat ambiguous but most scientists now believe that they show no evidence for life on Mars (there is still some controversy, however). Optimists point out that only two tiny samples were measured and not from the most favorable locations. More experiments will be done by future missions to Mars.

A small number of meteorites (the SNC meteorites) are believed to have originated on Mars.

On 1996 Aug 6, David McKay et al announced what they thought might be evidence of ancient Martian microorganisms in the meteorite ALH84001. Though there is still some controversy, the majority of the scientific community has not accepted this conclusion. If there is or was life on Mars, we still haven’t found it.

Large, but not global, weak magnetic fields exist in various regions of Mars. This unexpected finding was made by Mars Global Surveyor just days after it entered Mars orbit. They are probably remnants of an earlier global field that has since disappeared. This may have important implications for the structure of Mars’ interior and for the past history of its atmosphere and hence for the possibility of ancient life.

When it is in the night time sky, Mars is easily visible with the unaided eye. Mars is a difficult but rewarding target for an amateur telescope though only for the three or four months each martian year when it is closest to Earth. Its apparent size and brightness varies greatly according to its relative position to the Earth. There are several Web sites that show the current position of Mars (and the other planets) in the sky. More detailed and customized charts can be created with a planetarium program.

Mars’ Satellites

Mars has two tiny satellites which orbit very close to the martian surface:

Satellite(000 km)(km)(kg)DiscovererDate

(“Distance” is measured from the center of Mars).

Interesting Facts about Mars

  • Mars is 141 million miles (227,940,000) kilometres from the Sun. This makes it the fourth planet from the Sun behind MercuryVenus and Earth.
  • Mars has a red/brown colour. This is because of iron oxide which is a mineral found in the soil on the planet’s surface. This creates a powder of rust which floats in the atmosphere of Mars and covers much of the landscape.
  • The planet was named Mars after the Roman god of war. This is thought to be because of the blood red colour of the planet. The Roman god Mars was supposedly pulled on a chariot by his two horses named Phobos and Deimos. These are the names of the two moons of Mars.
  • The moons of Mars were written about in the book ‘Gulliver’s Travels’ by author Jonathan Swift. The interesting thing is that he wrote the book 151 years before the moons were even discovered!
  • A year on Mars is 687 days. This is the time the planet takes to orbit the Sun.
  • A day on Mars is 24 hours and 39 minutes long. Very close to the 24-hour length of a day on Earth.
  • The tilt on the axis of Mars is 25 degrees. This means the planet experiences seasons much like we do on Earth as parts of the planet move closer to and further away from the Sun throughout its orbit.
  • Seasons vary in length and are not even like on Earth. Spring is 7 months, and summer is 6 months, autumn is 5.4 months and Winter just over 4 months. This all adds up to a year on Mars.
  • Summer is not like what you would expect to have on Earth! Temperatures generally reach a maximum of 20 degrees Celcius (70 degrees Fahrenheit) and drop down to around -73 degrees Celcius (-100 degrees Fahrenheit) These can then drop as low as – 153 degrees Celcius (-243 degrees Fahrenheit) in the Winter at the poles. Mars has a very thin atmosphere like venus meaning it cannot hold onto its heat.
  • Mars has the second least circular orbit of all the planets. Only Mercurys orbit is more eccentric. This means it does not go around the Sun in a perfect circle but instead makes more of an oval, moving further away from the Sun on one side of the orbit than the other.
  • Mars does not have much of a magnetic field. Slight magnetic fields have been found in certain areas of Mars, but these have been very weak. Scientists believe that these are leftover from a time billions of years ago when Mars did have a magnetic field. The latest theory is that a huge asteroid destroyed the previous magnetic field but this has not been proven, and it is possible that is just withered away.
  • Mars has polar ice caps. It is the only planet apart from Earth to have them. The north polar cap is called the Planum Boreum, and the South cap is called the Planum Australe.
  • Mars has a very thin atmosphere. The atmosphere contains 95.9% carbon dioxide and 2.7% nitrogen with traces of a mixture of other gases. This is a similar atmosphere to the one found on Venus.
  • Mars has 37% of the gravity on Earth. This means you could jump three times higher on Mars than you can on Earth!
  • Mars has a similar amount of land to Earth. Even though Mars is much smaller than Earth, it has roughly the same amount of land. This is because of the large amounts of water on Earth.
  • For much of the nineteenth-century people believed in Martians – Aliens who live on Mars. This was due to the work of an astronomer Giovani Schiaparelli who in 1877, saw what he thought were straight lines on the surface of Mars. He believed these to be the work of Martians. This and people’s imagination fuelled the idea of life on Mars. As technology developed and more powerful telescopes were available, the surface of Mars could be viewed more clearly, and the lines were discovered to be an optical illusion.
  • There is no evidence that there has ever been life on Mars. However, apart from Earth, it is the planet with the best conditions to support life.
  • Scientists believe there is potential for life under the surface of Mars. There are several space mission planned to investigate these theories.
  • The tallest volcano in the entire Solar System is on Mars. This volcano is called Olympus Mons and is 13 miles (21 kilometres) high. The highest volcano on Earth is Hawaii’s Mauna Loa which is 6.3miles (10 kilometres) and less than half the size of Olympus Mons. The volume contained inside Olympus Mons is also roughly 100 times more than that inside Mauna Loa.
  • Mars experiences some massive dust storms. These can cover the entire planet, and the dust can travel up to 66 miles per hour!
  • There are currently two NASA rovers on Mars collecting data from the planet. These are called Curiosity and Opportunity, and they are constantly providing new information about Mars.
  • There have been a total of 13 robot’s active on Mars. It is the only planet that is solely inhabited by robots!
  • 39 different missions have been launched to Mars. Only 16 of these were successful and included rovers, landers and orbiters.

More about Mars, Deimos, and Phobos

  • “The Face” on Mars”:
  • Mars in the Arts:
    • Mars in the Mind of Earth; links to Mars related fiction
    • Mars Bibliography, science fiction about Mars
    • Edgar Rice Burroughs’ A Princess of Mars
    • Edgar Rice Burroughs’ The Gods of Mars
    • Edgar Rice Burroughs’ The Warlord of Mars
    • Edgar Rice Burroughs’ Thuvia, Maid of Mars
    • H.G. Wells’ The War of the Worlds
    • Study guide to Ray Bradbury’s The Martian Chronicles
    • C. K. Anderson’s A Step Beyond
    • more references
    • Mars in Popular Culture
  • Mars FAQ for amateur astronomers (what to expect to see with a small telescope)
  • lots more Mars links

Open Issues

  • Why are the northern and southern hemispheres of Mars so different? Why are the northern and southern polar caps different?
  • What is the structure of Mars’s interior? What is it composed of, and which parts are molten or solid? Is there still active volcanism on Mars?
  • What exactly caused the erosion patterns that look so much like stream beds on Earth? How old are they?
  • How much subterranean (“sub-martian”?) water is/was there on Mars? There’s growing evidence, (eg, here: APOD) but it’s not yet definitive; much more work is needed.
  • Mars remains at the top of the list of possible life-bearing planets. The Viking probes found little evidence of life on Mars. But they sampled only two isolated locations. Is there life elsewhere or was there life at some time in the past on Mars? The recent meteoric evidence needs to be confirmed. Ultimately, a sample return mission will be necessary.
  • The future of Mars exploration is more hopeful than for the other planets. Three orbiters and three landers are now in operation at Mars. Several more robotic missions are planned by NASA and others. But no one seems willing to put any real money toward a manned expedition.