Mars is the
fourth planet from the Sun. Named after the Roman god of war, and often
described as the “Red Planet” due to its reddish appearance. Mars is a terrestrial
planet with a thin atmosphere composed primarily of carbon dioxide.
Mars Contents:
Facts – Missions – Moons – Pictures
Mars Features:
Olympus Mons (Volcano) – Valles Marineris – Noctis Labyrinthus – Polar Ice Caps
Mars
Characteristics: Size – Mass & Gravity – Rotation & Tilt – Orbit –
Atmosphere – Interior
Mars Planet Profile
- Mass: 641,693,000,000,000 billion kg (0.107 x Earth)
- Equatorial Diameter: 6,805
- Polar Diameter: 6,755
- Equatorial Circumference: 21,297 km
- Known Moons: 2
- Notable Moons: Phobos & Deimos
- Orbit Distance: 227,943,824 km (1.38 AU)
- Orbit Period: 686.98 Earth days (1.88 Earth years)
- Surface Temperature: -87 to -5 °C
- First Record: 2nd millennium BC
- Recorded By: Egyptian astronomers
- Size of Mars compared to the Earth
Size of Mars
Facts about Mars
Mars and Earth have approximately the same landmass:
Even though Mars
has only 15% of the Earth’s volume and just over 10% of the Earth’s mass,
around two thirds of the Earth’s surface is covered in water. Martian surface gravity
is only 37% of the Earth’s (meaning you could leap nearly three times higher on
Mars).
Mars is home to
the tallest mountain in the solar system.
Olympus Mons, a
shield volcano, is 21km high and 600km in diameter. Despite having formed over
billions of years, evidence from volcanic lava flows is so recent many
scientists believe it could still be active.
Only 18 missions
to Mars have been successful
As of September
2014 there have been 40 missions to Mars, including orbiters, landers and
rovers but not counting flybys. The most recent arrivals include the Mars
Curiosity mission in 2012, the MAVEN mission, which arrived on September 22,
2014, followed by the Indian Space Research Organization’s MOM Mangalyaan
orbiter, which arrived on September 24, 2014. The next missions to arrive will
be the European Space Agency’s ExoMars mission, comprising an orbiter, lander,
and a rover, followed by NASA’s InSight robotic lander mission, slated for
launch in March 2016 and a planned arrival in September, 2016.”
Mars has the
largest dust storms in the solar system:
They can last for
months and cover the entire planet. The seasons are extreme because its
elliptical (oval-shaped) orbital path around the Sun is more elongated than
most other planets in the solar system.
On Mars the Sun
appears about half the size as it does on Earth:
At the closest
point to the Sun, the Martian southern hemisphere leans towards the Sun,
causing a short, intensely hot summer, while the northern hemisphere endures a
brief, cold winter: at its farthest point from the Sun, the Martian northern
hemisphere leans towards the Sun, causing a long, mild summer, while the
southern hemisphere endures a lengthy, cold winter.
Pieces of Mars
have fallen to Earth:
Scientists have
found tiny traces of Martian atmosphere within meteorites violently ejected
from Mars, then orbiting the solar system amongst galactic debris for millions
of years, before crash landing on Earth. This allowed scientists to begin
studying Mars prior to launching space missions.
Mars takes its
name from the Roman god of war:
The ancient
Greeks called the planet Ares, after their god of war; the Romans then did
likewise, associating the planet’s blood-red colour with Mars, their own god of
war. Interestingly, other ancient cultures also focused on colour – to China’s
astronomers it was ‘the fire star’, whilst Egyptian priests called on ‘Her
Desher’, or ‘the red one’. The red colour Mars is known for is due to the rock
and dust covering its surface being rich in iron.
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