SlideShare uma empresa Scribd logo
1 de 20
Solar System

Ismael Fernández Caballero
Nicolás García López Varela
Andrea Feito Bañón
4ºESO B
Introduction
• The Solar System comprises the Sun and its planetary
system of eight planets, as well as a number of dwarf
planets, moons, and other objects that orbit the Sun. It
formed 4.6 billion years ago from the gravitational
collapse of a giant molecular cloud. The vast majority of
the system's mass is in the Sun, with most of the
remaining mass contained in Jupiter.
• The four smaller inner planets, Mercury, Venus, Earth and
Mars, also called the terrestrial planets.
• The four outer planets, called the gas giants, are
substantially more massive than the terrestrials.
• The two largest, Jupiter and Saturn.
• The two outermost planets, Uranus and Neptune.
• All planets have almost circular orbits that lie within a
nearly flat disc called the ecliptic plane.
Mercury
• Diameter: 4880km
• Distance from the Sun: 57.91 million km
• Orbital period: 58.646 days
• Mercury is the closest planet to the sun, it has a rocky surface, full
with craters. It doesn’t have an atmosphere, so the temperature
can change between -183º and 467º.
• There have been two spatial missions, first in 1974 (Mariner 10) and
in 2004 (Messenger).
• Its name comes from the roman god of the messengers and the
thieves.
• Because of the Sun light it can only be seen during the twilight .
Venus
• Diameter:12104 km
• Distance from the Sun: 108.2 million km
• Orbital period: 224.7 days
• It has a similar size and composition as de Earth but its surface
is always covered by clouds. Because of this clouds
temperatures are extremely hot: from 120º to 470º.
• There have been 6 expeditions to Venus.
• Its name comes from the roman goddess of beauty and love.
THE EARTH.
•
•
•
•

It’s the 3rd planet from the Sun.
It’s called the ‘Blue Planet’
Earth formed approximately 4.54 billion years ago
Earth gravitationally interacts with other objects in space,
especially the Sun and the Moon
• Earth rotates about its own axis 366.26 times, creating
365.26 solar days
Earth’s composition.
• Earth is a terrestrial planet, meaning that it is a rocky
body, rather than a gas giant like Jupiter. It is the largest of
the four terrestrial planets in size and mass. Of these four
planets, Earth also has the highest density, the highest
surface gravity, the strongest magnetic field, and fastest
rotation, and is probably the only one with active plate
tectonics.
• The mass of the Earth is approximately 5.98×1024 kg.
• It is composed mostly of iron (32.1%), oxygen (30.1%), silicon
(15.1%), magnesium (13.9%), sulfur (2.9%), nickel
(1.8%), calcium (1.5%), and aluminium (1.4%); with the
remaining 1.2% consisting of trace amounts of other
elements.
•

About 70.8%of the surface is covered by water. The remaining 29.2%
(148.94 million km2) not covered by water consists of mountains, deserts,
plains, plateaus…
• The Earth provides liquid water, an environment where complex organic
molecules can assemble and interact, and sufficient energy to sustain
metabolism.
• So we can live in it.
Mars
• Diameter: 6794 km
• Distance from the Sun: 227.94 million km
• Orbital period: 686.93 days
• It is said that there was once life in Mars, when it had a very
similar atmosphere to the Earth and there was water.
• In Mars’ surface there are a lot of volcanoes and dry rivers.
Olympus volcano is one of the biggest volcanoes in all the
solar system. It has a height of 25 km and a diameter of 600
km.
• It has two satellites: Fobos and Deimos, they are asteroids
that are trapped in Mars gravitational field.
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 of 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.
Jupiter is primarily composed of hydrogen with a
quarter of its mass being helium, although helium
only comprises about a tenth of the number of
molecules. It may also have a rocky core of heavier
elements, but like the other gas giants, Jupiter
lacks a well-defined solid surface. Because of its
rapid rotation, the planet's shape is that of an
oblate spheroid.
• The outer atmosphere is
visibly segregated into
several bands at different
latitudes, resulting in
turbulence and storms along
their interacting boundaries
• Surrounding Jupiter is a
faint planetary ring system
and a powerful
magnetosphere. There are
also at least 67 moons,
including the four large
moons called the Galilean
moons that were first
discovered by Galileo in
1610. Ganymede, the largest
of these moons, has a
diameter greater than that
of the planet Mercury.
Saturn.
• Saturn is the sixth planet from the Sun and the second largest
planet in the Solar System.
• It’s a gas giant made up mostly of hydrogen and helium.
• It has the lowest density of all the planets, and is the only one
less dense than water.
• It spins faster than any other planet except Jupiter, completing
a rotation roughly every 10-and-a-half hours.
Composition and structure.
-96.3 percent molecular hydrogen, 3.25 percent helium, minor
amounts of methane, ammonia, hydrogen
deuteride, ethane, ammonia ice aerosols, water ice
aerosols, ammonia hydrosulfide aerosols.
Saturn seems to have a hot solid inner core of iron and rocky
material surrounded by an outer core probably composed of
ammonia, methane, and water.
Average distance from the sun: 885,904,700 miles
Saturn has at least 62 moons.
Saturn actually has many rings made of billions of particles of
ice and rock, ranging in size from a grain of sugar to the size of a
house.
• The first spacecraft to reach Saturn was
Pioneer 11 in 1979, flying within 13,700 miles
(22,000 km) of it, which discovered the
planet's two of its outer rings as well as the
presence of a strong magnetic field.
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 place them in a
category called "ice giants".
• It is the only planet whose name
is derived from a figure from
Greek mythology rather than
Roman mythology like the other
planets, from the Latinized
version of the Greek god of the
sky, Ouranos.
• Like the other giant planets,
Uranus has a ring system, a
magnetosphere, and numerous
moons.
• The Uranian system has a unique
configuration among those of
the planets because its axis of
rotation is tilted sideways,
nearly into the plane of its
revolution about the Sun.
• It is the coldest planetary
atmosphere in the Solar
System, with a minimum
temperature of 49 K
(−224.2 °C), and has a complex,
layered cloud structure, with
water thought to make up the
lowest clouds, and methane the
uppermost layer of clouds. In
contrast, the interior of Uranus
is mainly composed of ices and
rock.
• Uranus's atmosphere, apart of
containing hydrogen and helium,
contains more "ices" such as
water, ammonia, and methane,
along with traces of
hydrocarbons.
•
•
•
•
•
•
•
•

Neptune.
The planet Neptune was discovered on Sept. 23, 1846.
Neptune is the eighth and farthest planet from the Sun in the
Solar System.
Neptune goes around the sun once roughly every 165 Earth
years.
COMPOSITION:
Hydrogen - 80 percent; Helium - 19.0 percent; Methane - 1.5
percent
Neptune has 13 known moons.
Neptune's unusual rings are not uniform, but possess bright
thick clumps of dust called arcs.
NASA's Voyager 2 space satellite was the first and as yet only
spacecraft to visit Neptune on Aug. 25, 1989.

Mais conteúdo relacionado

Mais procurados

Kuiper Belt, Oort Cloud, Demotion of Pluto Astronomy Lesson PowerPoint
Kuiper Belt, Oort Cloud, Demotion of Pluto Astronomy Lesson PowerPointKuiper Belt, Oort Cloud, Demotion of Pluto Astronomy Lesson PowerPoint
Kuiper Belt, Oort Cloud, Demotion of Pluto Astronomy Lesson PowerPoint
www.sciencepowerpoint.com
 
What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: Structure
What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: StructureWhat is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: Structure
What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: Structure
Uday Kumar Shil
 
Es Ch. 23 Solar System
Es Ch. 23 Solar SystemEs Ch. 23 Solar System
Es Ch. 23 Solar System
Mr. Motuk
 
Kuiper belt & oort cloud 2
Kuiper belt & oort cloud 2Kuiper belt & oort cloud 2
Kuiper belt & oort cloud 2
molloylibrarian
 

Mais procurados (20)

Unit 1 the universe
Unit 1 the universeUnit 1 the universe
Unit 1 the universe
 
Kuiper Belt, Oort Cloud, Demotion of Pluto Astronomy Lesson PowerPoint
Kuiper Belt, Oort Cloud, Demotion of Pluto Astronomy Lesson PowerPointKuiper Belt, Oort Cloud, Demotion of Pluto Astronomy Lesson PowerPoint
Kuiper Belt, Oort Cloud, Demotion of Pluto Astronomy Lesson PowerPoint
 
Grade 7 SCIENCE
Grade 7 SCIENCEGrade 7 SCIENCE
Grade 7 SCIENCE
 
What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: Structure
What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: StructureWhat is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: Structure
What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: Structure
 
venus and mars
venus and marsvenus and mars
venus and mars
 
11 lecture outline
11 lecture outline11 lecture outline
11 lecture outline
 
Solar system ms santos
Solar system ms santosSolar system ms santos
Solar system ms santos
 
The solar system
The solar systemThe solar system
The solar system
 
Geochemistry chapt 1
Geochemistry chapt 1Geochemistry chapt 1
Geochemistry chapt 1
 
Ppt for ma'am belmi
Ppt for ma'am belmiPpt for ma'am belmi
Ppt for ma'am belmi
 
Menace From Outer Space
Menace From Outer SpaceMenace From Outer Space
Menace From Outer Space
 
Es Ch. 23 Solar System
Es Ch. 23 Solar SystemEs Ch. 23 Solar System
Es Ch. 23 Solar System
 
Planets
PlanetsPlanets
Planets
 
Science and astronomy club (types of celestrial objects)
Science and astronomy club (types of celestrial objects)Science and astronomy club (types of celestrial objects)
Science and astronomy club (types of celestrial objects)
 
11 review clickers
11 review clickers11 review clickers
11 review clickers
 
Origin of the earth
Origin of the earthOrigin of the earth
Origin of the earth
 
Dwarf Planet PLUTO 2015
Dwarf Planet PLUTO 2015Dwarf Planet PLUTO 2015
Dwarf Planet PLUTO 2015
 
Geochemistry chapt 1
Geochemistry chapt 1Geochemistry chapt 1
Geochemistry chapt 1
 
Kuiper belt & oort cloud 2
Kuiper belt & oort cloud 2Kuiper belt & oort cloud 2
Kuiper belt & oort cloud 2
 
Astonishing Astronomy 101 – Chapters 9, 10 and 11
Astonishing Astronomy 101 – Chapters 9, 10 and 11Astonishing Astronomy 101 – Chapters 9, 10 and 11
Astonishing Astronomy 101 – Chapters 9, 10 and 11
 

Destaque (6)

Solar System
Solar SystemSolar System
Solar System
 
The Atlantic
The AtlanticThe Atlantic
The Atlantic
 
Facts About Mercury
Facts About MercuryFacts About Mercury
Facts About Mercury
 
Facts of 10 planets
Facts of 10 planetsFacts of 10 planets
Facts of 10 planets
 
Heat and temperature
Heat and temperatureHeat and temperature
Heat and temperature
 
32 Ways a Digital Marketing Consultant Can Help Grow Your Business
32 Ways a Digital Marketing Consultant Can Help Grow Your Business32 Ways a Digital Marketing Consultant Can Help Grow Your Business
32 Ways a Digital Marketing Consultant Can Help Grow Your Business
 

Semelhante a Solar system

Planets of the solar system kevin yu
Planets of the solar system kevin yuPlanets of the solar system kevin yu
Planets of the solar system kevin yu
assasinator911
 

Semelhante a Solar system (20)

The solar system
The solar system The solar system
The solar system
 
About our universe
About our universeAbout our universe
About our universe
 
SOLAR SYSTEM PPT CLASS 8
SOLAR SYSTEM  PPT CLASS 8 SOLAR SYSTEM  PPT CLASS 8
SOLAR SYSTEM PPT CLASS 8
 
Explain solar system 3 (2)
Explain solar system 3 (2)Explain solar system 3 (2)
Explain solar system 3 (2)
 
Space Facts for Kids Infographic
Space Facts for Kids InfographicSpace Facts for Kids Infographic
Space Facts for Kids Infographic
 
Solar system
Solar systemSolar system
Solar system
 
Solar system
Solar systemSolar system
Solar system
 
Solar system
Solar systemSolar system
Solar system
 
All Aboute milky gelaxy (solar system, sun to neptune).pdf
All  Aboute milky gelaxy  (solar system, sun to neptune).pdfAll  Aboute milky gelaxy  (solar system, sun to neptune).pdf
All Aboute milky gelaxy (solar system, sun to neptune).pdf
 
Solar system
Solar systemSolar system
Solar system
 
Planets of the solar system kevin yu
Planets of the solar system kevin yuPlanets of the solar system kevin yu
Planets of the solar system kevin yu
 
Planets of the solar system kevin yu
Planets of the solar system kevin yuPlanets of the solar system kevin yu
Planets of the solar system kevin yu
 
solar .ppt
solar .pptsolar .ppt
solar .ppt
 
Gagandeep
GagandeepGagandeep
Gagandeep
 
solar lesson.ppt
solar lesson.pptsolar lesson.ppt
solar lesson.ppt
 
Solar system.pptx
Solar system.pptx Solar system.pptx
Solar system.pptx
 
Facts of 10 planets
Facts of 10 planetsFacts of 10 planets
Facts of 10 planets
 
The Planets
The PlanetsThe Planets
The Planets
 
Solar System
Solar SystemSolar System
Solar System
 
Stars and solar system
Stars and solar systemStars and solar system
Stars and solar system
 

Último

Making and Justifying Mathematical Decisions.pdf
Making and Justifying Mathematical Decisions.pdfMaking and Justifying Mathematical Decisions.pdf
Making and Justifying Mathematical Decisions.pdf
Chris Hunter
 
Gardella_Mateo_IntellectualProperty.pdf.
Gardella_Mateo_IntellectualProperty.pdf.Gardella_Mateo_IntellectualProperty.pdf.
Gardella_Mateo_IntellectualProperty.pdf.
MateoGardella
 

Último (20)

Paris 2024 Olympic Geographies - an activity
Paris 2024 Olympic Geographies - an activityParis 2024 Olympic Geographies - an activity
Paris 2024 Olympic Geographies - an activity
 
Grant Readiness 101 TechSoup and Remy Consulting
Grant Readiness 101 TechSoup and Remy ConsultingGrant Readiness 101 TechSoup and Remy Consulting
Grant Readiness 101 TechSoup and Remy Consulting
 
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
 
Making and Justifying Mathematical Decisions.pdf
Making and Justifying Mathematical Decisions.pdfMaking and Justifying Mathematical Decisions.pdf
Making and Justifying Mathematical Decisions.pdf
 
Web & Social Media Analytics Previous Year Question Paper.pdf
Web & Social Media Analytics Previous Year Question Paper.pdfWeb & Social Media Analytics Previous Year Question Paper.pdf
Web & Social Media Analytics Previous Year Question Paper.pdf
 
Mehran University Newsletter Vol-X, Issue-I, 2024
Mehran University Newsletter Vol-X, Issue-I, 2024Mehran University Newsletter Vol-X, Issue-I, 2024
Mehran University Newsletter Vol-X, Issue-I, 2024
 
Código Creativo y Arte de Software | Unidad 1
Código Creativo y Arte de Software | Unidad 1Código Creativo y Arte de Software | Unidad 1
Código Creativo y Arte de Software | Unidad 1
 
APM Welcome, APM North West Network Conference, Synergies Across Sectors
APM Welcome, APM North West Network Conference, Synergies Across SectorsAPM Welcome, APM North West Network Conference, Synergies Across Sectors
APM Welcome, APM North West Network Conference, Synergies Across Sectors
 
Nutritional Needs Presentation - HLTH 104
Nutritional Needs Presentation - HLTH 104Nutritional Needs Presentation - HLTH 104
Nutritional Needs Presentation - HLTH 104
 
Key note speaker Neum_Admir Softic_ENG.pdf
Key note speaker Neum_Admir Softic_ENG.pdfKey note speaker Neum_Admir Softic_ENG.pdf
Key note speaker Neum_Admir Softic_ENG.pdf
 
Z Score,T Score, Percential Rank and Box Plot Graph
Z Score,T Score, Percential Rank and Box Plot GraphZ Score,T Score, Percential Rank and Box Plot Graph
Z Score,T Score, Percential Rank and Box Plot Graph
 
microwave assisted reaction. General introduction
microwave assisted reaction. General introductionmicrowave assisted reaction. General introduction
microwave assisted reaction. General introduction
 
Measures of Dispersion and Variability: Range, QD, AD and SD
Measures of Dispersion and Variability: Range, QD, AD and SDMeasures of Dispersion and Variability: Range, QD, AD and SD
Measures of Dispersion and Variability: Range, QD, AD and SD
 
Mixin Classes in Odoo 17 How to Extend Models Using Mixin Classes
Mixin Classes in Odoo 17  How to Extend Models Using Mixin ClassesMixin Classes in Odoo 17  How to Extend Models Using Mixin Classes
Mixin Classes in Odoo 17 How to Extend Models Using Mixin Classes
 
Basic Civil Engineering first year Notes- Chapter 4 Building.pptx
Basic Civil Engineering first year Notes- Chapter 4 Building.pptxBasic Civil Engineering first year Notes- Chapter 4 Building.pptx
Basic Civil Engineering first year Notes- Chapter 4 Building.pptx
 
Class 11th Physics NEET formula sheet pdf
Class 11th Physics NEET formula sheet pdfClass 11th Physics NEET formula sheet pdf
Class 11th Physics NEET formula sheet pdf
 
SECOND SEMESTER TOPIC COVERAGE SY 2023-2024 Trends, Networks, and Critical Th...
SECOND SEMESTER TOPIC COVERAGE SY 2023-2024 Trends, Networks, and Critical Th...SECOND SEMESTER TOPIC COVERAGE SY 2023-2024 Trends, Networks, and Critical Th...
SECOND SEMESTER TOPIC COVERAGE SY 2023-2024 Trends, Networks, and Critical Th...
 
Gardella_Mateo_IntellectualProperty.pdf.
Gardella_Mateo_IntellectualProperty.pdf.Gardella_Mateo_IntellectualProperty.pdf.
Gardella_Mateo_IntellectualProperty.pdf.
 
How to Give a Domain for a Field in Odoo 17
How to Give a Domain for a Field in Odoo 17How to Give a Domain for a Field in Odoo 17
How to Give a Domain for a Field in Odoo 17
 
Accessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impactAccessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impact
 

Solar system

  • 1. Solar System Ismael Fernández Caballero Nicolás García López Varela Andrea Feito Bañón 4ºESO B
  • 2. Introduction • The Solar System comprises the Sun and its planetary system of eight planets, as well as a number of dwarf planets, moons, and other objects that orbit the Sun. It formed 4.6 billion years ago from the gravitational collapse of a giant molecular cloud. The vast majority of the system's mass is in the Sun, with most of the remaining mass contained in Jupiter. • The four smaller inner planets, Mercury, Venus, Earth and Mars, also called the terrestrial planets. • The four outer planets, called the gas giants, are substantially more massive than the terrestrials. • The two largest, Jupiter and Saturn. • The two outermost planets, Uranus and Neptune. • All planets have almost circular orbits that lie within a nearly flat disc called the ecliptic plane.
  • 3. Mercury • Diameter: 4880km • Distance from the Sun: 57.91 million km • Orbital period: 58.646 days • Mercury is the closest planet to the sun, it has a rocky surface, full with craters. It doesn’t have an atmosphere, so the temperature can change between -183º and 467º. • There have been two spatial missions, first in 1974 (Mariner 10) and in 2004 (Messenger). • Its name comes from the roman god of the messengers and the thieves. • Because of the Sun light it can only be seen during the twilight .
  • 4.
  • 5. Venus • Diameter:12104 km • Distance from the Sun: 108.2 million km • Orbital period: 224.7 days • It has a similar size and composition as de Earth but its surface is always covered by clouds. Because of this clouds temperatures are extremely hot: from 120º to 470º. • There have been 6 expeditions to Venus. • Its name comes from the roman goddess of beauty and love.
  • 6.
  • 7. THE EARTH. • • • • It’s the 3rd planet from the Sun. It’s called the ‘Blue Planet’ Earth formed approximately 4.54 billion years ago Earth gravitationally interacts with other objects in space, especially the Sun and the Moon • Earth rotates about its own axis 366.26 times, creating 365.26 solar days
  • 8. Earth’s composition. • Earth is a terrestrial planet, meaning that it is a rocky body, rather than a gas giant like Jupiter. It is the largest of the four terrestrial planets in size and mass. Of these four planets, Earth also has the highest density, the highest surface gravity, the strongest magnetic field, and fastest rotation, and is probably the only one with active plate tectonics. • The mass of the Earth is approximately 5.98×1024 kg. • It is composed mostly of iron (32.1%), oxygen (30.1%), silicon (15.1%), magnesium (13.9%), sulfur (2.9%), nickel (1.8%), calcium (1.5%), and aluminium (1.4%); with the remaining 1.2% consisting of trace amounts of other elements.
  • 9. • About 70.8%of the surface is covered by water. The remaining 29.2% (148.94 million km2) not covered by water consists of mountains, deserts, plains, plateaus… • The Earth provides liquid water, an environment where complex organic molecules can assemble and interact, and sufficient energy to sustain metabolism. • So we can live in it.
  • 10. Mars • Diameter: 6794 km • Distance from the Sun: 227.94 million km • Orbital period: 686.93 days • It is said that there was once life in Mars, when it had a very similar atmosphere to the Earth and there was water. • In Mars’ surface there are a lot of volcanoes and dry rivers. Olympus volcano is one of the biggest volcanoes in all the solar system. It has a height of 25 km and a diameter of 600 km. • It has two satellites: Fobos and Deimos, they are asteroids that are trapped in Mars gravitational field.
  • 11.
  • 12. 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 of 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. Jupiter is primarily composed of hydrogen with a quarter of its mass being helium, although helium only comprises about a tenth of the number of molecules. It may also have a rocky core of heavier elements, but like the other gas giants, Jupiter lacks a well-defined solid surface. Because of its rapid rotation, the planet's shape is that of an oblate spheroid.
  • 13. • The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries • Surrounding Jupiter is a faint planetary ring system and a powerful magnetosphere. There are also at least 67 moons, including the four large moons called the Galilean moons that were first discovered by Galileo in 1610. Ganymede, the largest of these moons, has a diameter greater than that of the planet Mercury.
  • 14. Saturn. • Saturn is the sixth planet from the Sun and the second largest planet in the Solar System. • It’s a gas giant made up mostly of hydrogen and helium. • It has the lowest density of all the planets, and is the only one less dense than water. • It spins faster than any other planet except Jupiter, completing a rotation roughly every 10-and-a-half hours.
  • 15. Composition and structure. -96.3 percent molecular hydrogen, 3.25 percent helium, minor amounts of methane, ammonia, hydrogen deuteride, ethane, ammonia ice aerosols, water ice aerosols, ammonia hydrosulfide aerosols. Saturn seems to have a hot solid inner core of iron and rocky material surrounded by an outer core probably composed of ammonia, methane, and water. Average distance from the sun: 885,904,700 miles Saturn has at least 62 moons. Saturn actually has many rings made of billions of particles of ice and rock, ranging in size from a grain of sugar to the size of a house.
  • 16. • The first spacecraft to reach Saturn was Pioneer 11 in 1979, flying within 13,700 miles (22,000 km) of it, which discovered the planet's two of its outer rings as well as the presence of a strong magnetic field.
  • 17. 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 place them in a category called "ice giants".
  • 18. • It is the only planet whose name is derived from a figure from Greek mythology rather than Roman mythology like the other planets, from the Latinized version of the Greek god of the sky, Ouranos. • Like the other giant planets, Uranus has a ring system, a magnetosphere, and numerous moons. • The Uranian system has a unique configuration among those of the planets because its axis of rotation is tilted sideways, nearly into the plane of its revolution about the Sun.
  • 19. • It is the coldest planetary atmosphere in the Solar System, with a minimum temperature of 49 K (−224.2 °C), and has a complex, layered cloud structure, with water thought to make up the lowest clouds, and methane the uppermost layer of clouds. In contrast, the interior of Uranus is mainly composed of ices and rock. • Uranus's atmosphere, apart of containing hydrogen and helium, contains more "ices" such as water, ammonia, and methane, along with traces of hydrocarbons.
  • 20. • • • • • • • • Neptune. The planet Neptune was discovered on Sept. 23, 1846. Neptune is the eighth and farthest planet from the Sun in the Solar System. Neptune goes around the sun once roughly every 165 Earth years. COMPOSITION: Hydrogen - 80 percent; Helium - 19.0 percent; Methane - 1.5 percent Neptune has 13 known moons. Neptune's unusual rings are not uniform, but possess bright thick clumps of dust called arcs. NASA's Voyager 2 space satellite was the first and as yet only spacecraft to visit Neptune on Aug. 25, 1989.