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SOLAR SYSTEM 
By: María Martín, Leire Martín and Elisa Vicente.
Mercury, Venus, The Earth and Mars are very similar but they are not the same. 
These planets were formed in a warm region, this warm pushed away hydrogen 
and helium which are light gases. Teluric planets are mainly composed of heavy 
components like carbon, iron, silicon… and they are solid and rocky. 
As these plantes have been evolucionating, their atmospheres had been replaced 
by light gases from the interior and warm zones. Heavy elements were moved 
to their interior to form cores. 
Mercury: smallest planet near the Sun and without atmosphere is a desert of 
craters burnt by the Sun. Mercury rotates on its own axis in 58 days and a half. 
When it is facing the Sun it reaches 425º whereas the zones which are facing 
the shadow can reach 170º below 0. Both poles mantain very cold that is why 
scientists think there could be water. 
Venus: It had oceans but the Sun evaporate the water and escape through space. 
Actually, the atmosphere of this planet is very dense and is composed of 
anhidrid carbonic. Several layers of clouds of sulphuric acid impede rays of the 
son to reach its surface because of the green house effect which reaches a 
temperature of 500ºC. They had discovered plateaus, deep valleys and 
volcanos perhaps active.
The Earth: It is characterised by the huge amounts of water it 
has conserved thanks to the distance which separates the 
Earth from the Sun. Its atmosphere is composed of nitrogen, 
oxygen , small amount of anhidric carbonic and water 
vapour. 
Our planet is composed of a 70% of water. This make the 
Earth different from the other plants which rotate around the 
Sun. Thanks to this, we have three estates: gas, solid and 
liquid. 
The Earth is composed of a core which has 10 to 60 km deep 
a solid mantle of 2900 km dense, an external nucleus of 
2200 km and an interior solid nucleus of 1200 km of density.
The Scales of the Earth: 200 million years ago all continents 
were unified into one which was called pangea surrounded 
by one ocean. This mass started to fragment and continents 
started to separate. 
Magnetic Field: The magnetic field of the Earth is more 
important than Mercury. It is said that its origin comes from 
the existence of electric currents which flow in the nucleus of 
the liquid iron. This magnetic field, it doesn´t spread around 
the Earth. In Sun direction, it blocks the solar wind protecting 
it from some particles with a type of shield called 
magnetopause.
 Mars: it had an important atmosphere which 
provide beningn temperatures, rivers and oceans. 
But as the planet is small, and its mass is weak, 
most part of its atmosphere disolved in space. It 
only has a few of anhidrid carbonic. The water it 
contained froze in the subsoil and its interior also 
froze. Sometimes, windstorms takes place and 
they make huge amounts of dust which takes 
weeks to dissappear.
They are Jupiter, Saturn, Urane and 
Neptune. Outer planets are situated 
beyond the astoid belt. They are gigant in 
relation with the other planets of the Solar 
system. 
They are mainly composed of hydrogen 
and helium and they are surrounded by 
rings of satellites and by plenty of moons
 Jupiter is the fifth planet in 
relation to the sun. It is the 
biggest planet and the one 
which has more mass in the 
Solar System. It is the 
fastest revolving the sun. It 
has the biggest number of 
moons, it has 67 moons. 
 Jupiter has a diameter of 
142 984 km. It is 7778.3 
millions of km away from the 
sun. It lasts 11.9 years to 
orbit the sun. It rotates in its 
on axis in
 Regular Satellites 
 Galilean moons: They are the principal moons, which were discovered by Galileo Galilei in 1610. 
Their names comes from the lovers of Zeus: 
 Io: It is the most volcanic place in the earth and it has continuous eruptions which regenerates its 
surface. 
 Europe: this satellite has grooves and ridges that cross the surface covered with ice. 
 Ganymede: It is the biggest moon of the Solar system. Its crust is full of impact craters. 
 Callisto: It is the moon that is situated farthest away from Jupiter. The ice from its craters bright 
deeply. 
 Amaltean Group: They orbit very close to Jupiter. They are: 
 
 Metis 
 Adrastea 
 Amalthea 
 Thebis 
 
 Irregular Satellites: 
 They are group of satellites that rotate in orbit so far away from Jupiter that the gravitation from the 
Sun affects them and so they don´t orbit in a regular orbit.
 Jupiter has biggest atmosphere in all the Solar System. It is 
principally made up by Hydrogen and Helium, but it also 
contains Methane, water vapour and other substances. The 
Jupiter´s atmosphere contains a lot of atmospheric 
phenomenon. The most known are: 
The great Red Spot: It is a huge storm 
that could have existed for more than 300 
years. In this storm, there are winds up to 
400km/h. 
The Little Red Spot: it is a big storm was 
created in 2006.
 It is the sixth planet in relation to the Sun. It has the second 
greatest mass, after Jupiter. It has a volume of 740 times the 
Earth, but it just have a mass of 95 times the Earth. It is the 
only planet that has system of rings. Galileo was the first one 
that observed its rings, in 1610. 
•Saturn has a diameter 
of 120 536 km. the 
gravity is 10,44m/s2. Its 
atmosphere it is made 
up by hydrogen and 
helium. It has a radius 
of 60 300km.
 There is not an exact number of satellites, but 
the most important are: 
 Titan: it is the biggest one 
 Mimas: it could have water. 
 Enceladus 
 Tethys 
 Dione 
 Rhea 
 Hyperion 
 Iapetus 
 Phoebe
 The system of rings of Saturn 
consists in countless small 
particles made up by ice water and 
some rocks that go from 
millimetres to metres. These rocks 
are made up by silicates and 
tholins. There are a lot of gaps 
between the rings but there are 
very few between the fragments. 
This system consists of 7 rings. 
 This ring makes that the brightness 
of Saturn increase, but we cannot 
see them without a telescope. 
 The densest rings are A and B, 
they are separated by the division 
of Cassini. We also have the C, D, 
E and F rings.
 The astronomers of the Antiquity didn´t 
named as a planet because of 
darkness and of the slow speed of its 
orbit. It was discovered as a planet in 
1781 by William Herschel. It was the 
first planet discovered by a telescope. 
 It is made up by frozen water, methane 
and ammoniac. It also contains 
hydrocarbons. 
 It has a very inclined axis (of 97.7º). So 
it has the north and south poles were 
other planets have the equator. Uranus 
also has system of rings; seen from the 
Earth seams that ring are like a 
dartboard. 
 It lasts 84 Earth´s years to do one lap 
around the Sun. It is 3 000 millions of 
km away from the Sun. it turns around 
itself in 17 hours and 14 minutes.
 It has a very cold climate. It radiates even less 
energy than Neptune. It has a very uniform 
atmosphere in relation with the other outer planets. 
When the ´Voyager2´ flew near Uranus in 1986, it 
was discovered that there was ten different levels 
of clouds in its atmosphere. 
 It has the coldest atmosphere of the Solar System; 
temperatures can reach -224ºC. 
 It has a system of rings, as all the giant planets. 
The fragments of their rings go from micrometer to 
one meter. There are 13 known planets.
 It is the first planet that was discovered by mathematic predictions. It 
has a mass of 17 times the Earth and a volume of 57 times. It has 
some phenomena similar to the ones of Jupiter, as the Great Dark 
Spot, which had a similar size to the one of the Earth. 
•It has a nucleus composed 
of rocks and a frozen crust. 
The atmosphere it is very 
dense and it is composed of 
hydrogen, helium, water and 
methane. Although it has a 
very cold climate, 
temperatures in the centre of 
the planet can reach 4 700 
ºC.
 Neptune has fourteen satellites. 
• Triton: it is the biggest one. It is the only satellite of Neptune 
with an spherical shape. The others are irregular. It is 
considered to be a fragment of the Kuiper´s belt. It was 
discovered by William Lassell in 1846. 
• Nereid 
• Naiad 
• Thalassa 
• Despina 
• Galatea 
• Larissa 
• Proteus

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Solar system

  • 1. SOLAR SYSTEM By: María Martín, Leire Martín and Elisa Vicente.
  • 2. Mercury, Venus, The Earth and Mars are very similar but they are not the same. These planets were formed in a warm region, this warm pushed away hydrogen and helium which are light gases. Teluric planets are mainly composed of heavy components like carbon, iron, silicon… and they are solid and rocky. As these plantes have been evolucionating, their atmospheres had been replaced by light gases from the interior and warm zones. Heavy elements were moved to their interior to form cores. Mercury: smallest planet near the Sun and without atmosphere is a desert of craters burnt by the Sun. Mercury rotates on its own axis in 58 days and a half. When it is facing the Sun it reaches 425º whereas the zones which are facing the shadow can reach 170º below 0. Both poles mantain very cold that is why scientists think there could be water. Venus: It had oceans but the Sun evaporate the water and escape through space. Actually, the atmosphere of this planet is very dense and is composed of anhidrid carbonic. Several layers of clouds of sulphuric acid impede rays of the son to reach its surface because of the green house effect which reaches a temperature of 500ºC. They had discovered plateaus, deep valleys and volcanos perhaps active.
  • 3. The Earth: It is characterised by the huge amounts of water it has conserved thanks to the distance which separates the Earth from the Sun. Its atmosphere is composed of nitrogen, oxygen , small amount of anhidric carbonic and water vapour. Our planet is composed of a 70% of water. This make the Earth different from the other plants which rotate around the Sun. Thanks to this, we have three estates: gas, solid and liquid. The Earth is composed of a core which has 10 to 60 km deep a solid mantle of 2900 km dense, an external nucleus of 2200 km and an interior solid nucleus of 1200 km of density.
  • 4. The Scales of the Earth: 200 million years ago all continents were unified into one which was called pangea surrounded by one ocean. This mass started to fragment and continents started to separate. Magnetic Field: The magnetic field of the Earth is more important than Mercury. It is said that its origin comes from the existence of electric currents which flow in the nucleus of the liquid iron. This magnetic field, it doesn´t spread around the Earth. In Sun direction, it blocks the solar wind protecting it from some particles with a type of shield called magnetopause.
  • 5.  Mars: it had an important atmosphere which provide beningn temperatures, rivers and oceans. But as the planet is small, and its mass is weak, most part of its atmosphere disolved in space. It only has a few of anhidrid carbonic. The water it contained froze in the subsoil and its interior also froze. Sometimes, windstorms takes place and they make huge amounts of dust which takes weeks to dissappear.
  • 6. They are Jupiter, Saturn, Urane and Neptune. Outer planets are situated beyond the astoid belt. They are gigant in relation with the other planets of the Solar system. They are mainly composed of hydrogen and helium and they are surrounded by rings of satellites and by plenty of moons
  • 7.  Jupiter is the fifth planet in relation to the sun. It is the biggest planet and the one which has more mass in the Solar System. It is the fastest revolving the sun. It has the biggest number of moons, it has 67 moons.  Jupiter has a diameter of 142 984 km. It is 7778.3 millions of km away from the sun. It lasts 11.9 years to orbit the sun. It rotates in its on axis in
  • 8.  Regular Satellites  Galilean moons: They are the principal moons, which were discovered by Galileo Galilei in 1610. Their names comes from the lovers of Zeus:  Io: It is the most volcanic place in the earth and it has continuous eruptions which regenerates its surface.  Europe: this satellite has grooves and ridges that cross the surface covered with ice.  Ganymede: It is the biggest moon of the Solar system. Its crust is full of impact craters.  Callisto: It is the moon that is situated farthest away from Jupiter. The ice from its craters bright deeply.  Amaltean Group: They orbit very close to Jupiter. They are:   Metis  Adrastea  Amalthea  Thebis   Irregular Satellites:  They are group of satellites that rotate in orbit so far away from Jupiter that the gravitation from the Sun affects them and so they don´t orbit in a regular orbit.
  • 9.  Jupiter has biggest atmosphere in all the Solar System. It is principally made up by Hydrogen and Helium, but it also contains Methane, water vapour and other substances. The Jupiter´s atmosphere contains a lot of atmospheric phenomenon. The most known are: The great Red Spot: It is a huge storm that could have existed for more than 300 years. In this storm, there are winds up to 400km/h. The Little Red Spot: it is a big storm was created in 2006.
  • 10.  It is the sixth planet in relation to the Sun. It has the second greatest mass, after Jupiter. It has a volume of 740 times the Earth, but it just have a mass of 95 times the Earth. It is the only planet that has system of rings. Galileo was the first one that observed its rings, in 1610. •Saturn has a diameter of 120 536 km. the gravity is 10,44m/s2. Its atmosphere it is made up by hydrogen and helium. It has a radius of 60 300km.
  • 11.  There is not an exact number of satellites, but the most important are:  Titan: it is the biggest one  Mimas: it could have water.  Enceladus  Tethys  Dione  Rhea  Hyperion  Iapetus  Phoebe
  • 12.  The system of rings of Saturn consists in countless small particles made up by ice water and some rocks that go from millimetres to metres. These rocks are made up by silicates and tholins. There are a lot of gaps between the rings but there are very few between the fragments. This system consists of 7 rings.  This ring makes that the brightness of Saturn increase, but we cannot see them without a telescope.  The densest rings are A and B, they are separated by the division of Cassini. We also have the C, D, E and F rings.
  • 13.  The astronomers of the Antiquity didn´t named as a planet because of darkness and of the slow speed of its orbit. It was discovered as a planet in 1781 by William Herschel. It was the first planet discovered by a telescope.  It is made up by frozen water, methane and ammoniac. It also contains hydrocarbons.  It has a very inclined axis (of 97.7º). So it has the north and south poles were other planets have the equator. Uranus also has system of rings; seen from the Earth seams that ring are like a dartboard.  It lasts 84 Earth´s years to do one lap around the Sun. It is 3 000 millions of km away from the Sun. it turns around itself in 17 hours and 14 minutes.
  • 14.  It has a very cold climate. It radiates even less energy than Neptune. It has a very uniform atmosphere in relation with the other outer planets. When the ´Voyager2´ flew near Uranus in 1986, it was discovered that there was ten different levels of clouds in its atmosphere.  It has the coldest atmosphere of the Solar System; temperatures can reach -224ºC.  It has a system of rings, as all the giant planets. The fragments of their rings go from micrometer to one meter. There are 13 known planets.
  • 15.  It is the first planet that was discovered by mathematic predictions. It has a mass of 17 times the Earth and a volume of 57 times. It has some phenomena similar to the ones of Jupiter, as the Great Dark Spot, which had a similar size to the one of the Earth. •It has a nucleus composed of rocks and a frozen crust. The atmosphere it is very dense and it is composed of hydrogen, helium, water and methane. Although it has a very cold climate, temperatures in the centre of the planet can reach 4 700 ºC.
  • 16.  Neptune has fourteen satellites. • Triton: it is the biggest one. It is the only satellite of Neptune with an spherical shape. The others are irregular. It is considered to be a fragment of the Kuiper´s belt. It was discovered by William Lassell in 1846. • Nereid • Naiad • Thalassa • Despina • Galatea • Larissa • Proteus