33
The Solar System By Matthew Schembri

The Solar System By Matthew Schembri. The Solar System Image

Embed Size (px)

Citation preview

Page 1: The Solar System By Matthew Schembri. The Solar System Image

The Solar SystemBy Matthew Schembri

Page 2: The Solar System By Matthew Schembri. The Solar System Image

The Solar System Image

Page 3: The Solar System By Matthew Schembri. The Solar System Image

Mercury

Page 4: The Solar System By Matthew Schembri. The Solar System Image

The Inside of Mercury

Page 5: The Solar System By Matthew Schembri. The Solar System Image

Information about Mercury

Mercury is the innermost planet in the Solar System. It is also the smallest, and its orbit is the most eccentric (that is, the least perfectly circular) of the eight planets. It orbits the Sun once in about 88 Earth days, completing three rotations about its axis for every two orbits.

Orbits means in physics, an orbit is the gravitationally curved path of an object around a point in space, for example the orbit of a planet around the center of a star system, such as the Solar System. Orbits of planets are typically elliptical.

Page 6: The Solar System By Matthew Schembri. The Solar System Image

Venus

Page 7: The Solar System By Matthew Schembri. The Solar System Image

The Inside in Venus

Page 8: The Solar System By Matthew Schembri. The Solar System Image

Information about Venus

Venus is the second planet from the Sun, orbiting it every 224.7 Earth days.[ The planet is named after the Roman goddess of love and beauty. After the Moon, it is the brightest natural object in the night sky, reaching an apparent magnitude of −4.6, bright enough to cast shadows

Page 9: The Solar System By Matthew Schembri. The Solar System Image

Earth

Page 10: The Solar System By Matthew Schembri. The Solar System Image

The Inside in Earth

Page 11: The Solar System By Matthew Schembri. The Solar System Image

Information about Earth

Earth is the third planet from the Sun, and the densest and fifth-largest of the eight planets in the Solar System. It is also the largest of the Solar System's four terrestrial planets. It is sometimes referred to as the world, the Blue Planet, or by its Latin name, Terra.

Earth formed approximately 4.54 billion years ago, and life appeared on its surface within one billion years. Earth's biosphere then significantly altered the atmospheric and other basic physical conditions, which enabled the proliferation of organisms as well as the formation of the ozone layer, which together with Earth's magnetic field blocked harmful solar radiation, and permitted formerly ocean-confined life to move safely to land.

Page 12: The Solar System By Matthew Schembri. The Solar System Image

Mars

Page 13: The Solar System By Matthew Schembri. The Solar System Image

The Inside in Mars

Page 14: The Solar System By Matthew Schembri. The Solar System Image

Information about Mars

Mars is the fourth planet from the Sun and the second smallest planet in the Solar System. Named after the Roman god of war, it is often described as the "Red Planet", as the iron oxide prevalent on its surface gives it a reddish appearance. Mars is a terrestrial planet with a thin atmosphere, having surface features reminiscent both of the impact craters of the Moon and the volcanoes, valleys, deserts, and polar ice caps of Earth. The rotational period and seasonal cycles of Mars are likewise similar to those of Earth, as is the tilt that produces the seasons. Mars is the site of Olympus Mons, the second highest known mountain within the Solar System (the tallest on a planet), and of Valles Marineris, one of the largest canyons. The smooth Borealis basin in the northern hemisphere covers 40% of the planet and may be a giant impact feature.

Page 15: The Solar System By Matthew Schembri. The Solar System Image

Jupiter

Page 16: The Solar System By Matthew Schembri. The Solar System Image

The Inside in Jupiter

Page 17: The Solar System By Matthew Schembri. The Solar System Image

Information about Jupiter

Jupiter is the fifth planet from the Sun and the largest planet in the Solar System. It is a gas giant with mass one-thousandth that of the Sun but is two and a half times the mass of all the other planets in the Solar System combined. Jupiter is classified as a gas giant along with Saturn, Uranus and Neptune. Together, these four planets are sometimes referred to as the Jovian or outer planets. The planet was known by astronomers of ancient times, and was associated with the mythology and religious beliefs of many cultures. The Romans named the planet after the Roman god Jupiter.[

Page 18: The Solar System By Matthew Schembri. The Solar System Image

Saturn

Page 19: The Solar System By Matthew Schembri. The Solar System Image

The Inside in Saturn

Page 20: The Solar System By Matthew Schembri. The Solar System Image

Information about Saturn

Saturn is the sixth planet from the Sun and the second largest planet in the Solar System, after Jupiter. Named after the Roman god Saturn, its astronomical symbol (♄) represents the god's sickle. Saturn is a gas giant with an average radius about nine times that of Earth. While only one-eighth the average density of Earth, with its larger volume Saturn is just over 95 times more massive than Earth.

Page 21: The Solar System By Matthew Schembri. The Solar System Image

Uranus

Page 22: The Solar System By Matthew Schembri. The Solar System Image

The Inside in Uranus

Page 23: The Solar System By Matthew Schembri. The Solar System Image

Information about Uranus

Uranus is the seventh planet from the Sun. It has the third-largest planetary radius and fourth-largest planetary mass in the Solar System. Uranus is similar in composition to Neptune, and both are of different chemical composition than the larger gas giants Jupiter and Saturn. For this reason, astronomers sometimes place them in a separate category called "ice giants". Uranus's atmosphere, while similar to Jupiter's and Saturn's in its primary composition of hydrogen and helium, contains more "ices" such as water, ammonia, and methane, along with traces of hydrocarbons.

Page 24: The Solar System By Matthew Schembri. The Solar System Image

Neptune

Page 25: The Solar System By Matthew Schembri. The Solar System Image

The Inside in Neptune

Page 26: The Solar System By Matthew Schembri. The Solar System Image

Neptune

Neptune is the eighth and farthest planet from the Sun in the Solar System. It is the fourth-largest planet by diameter and the third-largest by mass. Neptune is 17 times the mass of Earth and is somewhat more massive than its near-twin Uranus, which is 15 times the mass of Earth but not as dense. On average, Neptune orbits the Sun at a distance of 30.1 AU, approximately 30 times the Earth–Sun distance.

Page 27: The Solar System By Matthew Schembri. The Solar System Image

The Sun

Page 28: The Solar System By Matthew Schembri. The Solar System Image

The Inside in The Sun

Page 29: The Solar System By Matthew Schembri. The Solar System Image

Information about the sun

The Sun is the star at the center of the Solar System. It is almost perfectly spherical and consists of hot plasma interwoven with magnetic fields. It has a diameter of about 1,392,684 km, about 109 times that of Earth, and its mass (about 2×1030 kilograms, 330,000 times that of Earth) accounts for about 99.86% of the total mass of the Solar System.

Page 30: The Solar System By Matthew Schembri. The Solar System Image

The Ozone Layer

Page 31: The Solar System By Matthew Schembri. The Solar System Image

Information about the ozone layer

The ozone layer is a layer in Earth's atmosphere containing relatively high concentrations of ozone (O3). However, "relatively high," in the case of ozone, is still very small with regard to ordinary oxygen, and is less than ten parts per million, with the average ozone concentration in Earth's atmosphere being only about 0.6 parts per million. The ozone layer is mainly found in the lower portion of the stratosphere from approximately 20 to 30 kilometres (12 to 19 mi) above Earth, though the thickness varies seasonally and geographically.

The ozone layer absorbs 97–99% of the Sun's medium-frequency ultraviolet light (from about 200 nm to 315 nm wavelength), which potentially damages exposed life forms on Earth.

Page 32: The Solar System By Matthew Schembri. The Solar System Image

References http://en.wikipedia.org/wiki/Earth

http://en.wikipedia.org/wiki/File:Orbital_motion.gif

http://en.wikipedia.org/wiki/File:Planets2013.jpg

http://en.wikipedia.org/wiki/Jupiter

http://en.wikipedia.org/wiki/Mars

http://en.wikipedia.org/wiki/Mercury_(planet)

http://en.wikipedia.org/wiki/Neptune

http://en.wikipedia.org/wiki/Orbits

http://en.wikipedia.org/wiki/Saturn

http://en.wikipedia.org/wiki/Solar_System

http://en.wikipedia.org/wiki/Sun

http://en.wikipedia.org/wiki/Uranus

http://en.wikipedia.org/wiki/Venus

http://en.wikipedia.org/wiki/Ozone_layer

Page 33: The Solar System By Matthew Schembri. The Solar System Image

The End