made by vlad stegariu and stefan popovici national college, iasi, romania

12
ON TO MARS made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

Upload: sandra-barton

Post on 23-Dec-2015

218 views

Category:

Documents


2 download

TRANSCRIPT

Page 1: Made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

ON TO MARS

made by Vlad Stegariu and Stefan

Popovici

Page 2: Made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

National College, Iasi, Romania

Mars Features

Mars is the fourth planet from the Sun in the Solar System. The planet is named after the Roman god of war, Mars. It is often described as the "Red Planet", as the iron oxide prevalent on its surface gives it a reddish appearance.

Page 3: Made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

National College, Iasi, Romania

Mars’ satellites

Mars has two moons, Phobos and Deimos, which are small and irregularly shaped. These may be captured asteroids, similar to 5261 Eureka, a Martian Trojan asteroid.

Page 4: Made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

National College, Iasi, Romania

General informations

Surface area 144,798,500 km2

Volume 1.6318 × 1011 km3

Satellites 2

Mass 6.4185 × 1023 kg

Mean density 3.9335 ± 0.0004 g/cm³

Surface pressure 0.636 (0.4–0.87) kPa

Temperature min mean max−87 °C −63 °C 20 °C

Page 5: Made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

National College, Iasi, Romania

Volcanoes

Mars has the largest volcanoes in the solar system. The tallest one, Olympus Mons (Latin for Mount Olympus), rises 17 miles (27 kilometers) above the surrounding plains.

Page 6: Made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

National College, Iasi, Romania

Canyons

Along the equator lies one of the most striking features on the planet, a system of canyons known as the Valles Marineris. The name is Latin for Valleys of Mariner; a space probe called Mariner 9 discovered the canyons in 1971.

Page 7: Made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

National College, Iasi, Romania

Did you know?...

Until the first flyby of Mars occurred in 1965, by Mariner 4, many speculated about the presence of liquid water on the planet's surface.Press to to see a weird phenomena.

Page 8: Made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

National College, Iasi, Romania

Mars has approximately half the radius of Earth. It is less dense than Earth, having about 15% of Earth's volume and 11% of the mass. Its surface area is only slightly less than the total area of Earth's dry land.

Page 9: Made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

National College, Iasi, Romania

While Mars is larger and more massive than Mercury, Mercury has a higher density. This results in the two planets having a nearly identical gravitational pull at the surface—that of Mars is stronger by less than 1%.

Page 10: Made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

National College, Iasi, Romania

A sunset on Mars creates a glow due to the presence of tiny dust particles in the atmosphere. This photo is a combination of four images taken by Mars Pathfinder, which landed on Mars in 1997. For more informations click here.

Page 11: Made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

National College, Iasi, Romania

Polar deposits

The most interesting features in the polar regions of Mars are thick stacks of finely layered deposits of material. Scientists believe that the layers consist of mixtures of water ice and dust.

Page 12: Made by Vlad Stegariu and Stefan Popovici National College, Iasi, Romania

National College, Iasi, Romania

THE END