Saturn
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Saturn has a mass of 5.7 x 10^26 kg and is less dense than water. It has a prominent ring system composed of icy particles ranging in size from dust grains to boulders. The rings have gaps and fine structure caused by orbital resonances with Saturn's many moons. Titan is Saturn's largest moon, with a thick nitrogen-rich atmosphere that obscures its surface from view.
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Saturn
Saturn is the 6th planet from the Sun and 2nd largest in the solar system. It is made up primarily of hydrogen and helium and has a dense atmosphere. Saturn is most notable for its extensive ring system composed of ice particles. The rings were first observed by Galileo in 1610 but their nature was not understood until the late 1600s. Modern space probes like Voyager and Cassini have revealed Saturn's atmospheric composition and weather patterns as well as details of its interior structure and ring system.
The Outer Planets
The outer planets are Jupiter, Saturn, Uranus, and Neptune. They are the largest planets in our solar system and are mainly composed of gases like hydrogen and helium, giving them low density. Most have a similar structure with an atmosphere of gases, a liquid hydrogen mantle, and a small molten rock core. Jupiter is the largest and has a prominent Great Red Spot storm and over 60 moons. Saturn is notable for its extensive ring system. Uranus and Neptune are both blue-green due to methane in their atmospheres.
Saturn presentation
Saturn is the 6th planet from the sun and is known for its prominent rings. It is the second largest planet in our solar system and has over 60 moons, some of which are Titan, Dione, Mimas, Enceladus, Rhea, and Thethys. Saturn has an icy surface with very cold weather, making it impossible for visitors due to the lack of oxygen in its gaseous atmosphere.
Solar system power point
The document summarizes key facts about the planets in our solar system. It explains that our solar system contains 8 planets that orbit the sun, along with over 170 moons, thousands of asteroids, and many dwarf planets. It provides details about each planet's composition, distance from the sun, atmospheric conditions, temperatures, and other distinguishing features. The sun is identified as the largest object that contains 99.8% of the mass in the solar system and provides light, heat, and energy to hold the system together.
uranus
Uranus is a gas giant planet with an atmosphere composed primarily of hydrogen and helium. Unlike the other planets in the solar system, Uranus spins on its side due to a large collision in the past. Uranus has 27 known moons named after characters from Shakespearean plays. The planet is extremely cold with an average temperature of -224 degrees Celsius due to its composition and distance from the Sun. It has a system of faint rings and weather characterized by powerful winds and storms.
Uranus
Uranus was the first planet discovered with a telescope by William Herschel in 1781, though he initially thought it was a comet. It orbits the sun every 84 Earth years at a distance of about 3 billion km. Uranus rotates on its side with an axial tilt of 98 degrees, and has 27 known moons as well as 13 known rings composed of small, dark particles. Uranus is composed of ice and rock, and has a blue-green color due to the scattering of light by methane ice crystals in its atmosphere.
Solar system
The document provides facts about objects in our solar system including the Sun, planets Mercury through Neptune, dwarf planets, asteroids, and the Kuiper Belt. It notes key details about each such as the Sun containing 99% of the solar system's mass, Venus rotating backwards compared to other planets, Jupiter having the largest moon Ganymede, Saturn being the ringed planet, and the Kuiper Belt potentially containing over a trillion comet nuclei. It aims to inform readers about characteristics of astronomical bodies in our neighborhood.
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Saturn
Saturn is the 6th planet from the Sun and 2nd largest in the solar system. It is made up primarily of hydrogen and helium and has a dense atmosphere. Saturn is most notable for its extensive ring system composed of ice particles. The rings were first observed by Galileo in 1610 but their nature was not understood until the late 1600s. Modern space probes like Voyager and Cassini have revealed Saturn's atmospheric composition and weather patterns as well as details of its interior structure and ring system.
The Outer Planets
The outer planets are Jupiter, Saturn, Uranus, and Neptune. They are the largest planets in our solar system and are mainly composed of gases like hydrogen and helium, giving them low density. Most have a similar structure with an atmosphere of gases, a liquid hydrogen mantle, and a small molten rock core. Jupiter is the largest and has a prominent Great Red Spot storm and over 60 moons. Saturn is notable for its extensive ring system. Uranus and Neptune are both blue-green due to methane in their atmospheres.
Saturn presentation
Saturn is the 6th planet from the sun and is known for its prominent rings. It is the second largest planet in our solar system and has over 60 moons, some of which are Titan, Dione, Mimas, Enceladus, Rhea, and Thethys. Saturn has an icy surface with very cold weather, making it impossible for visitors due to the lack of oxygen in its gaseous atmosphere.
Solar system power point
The document summarizes key facts about the planets in our solar system. It explains that our solar system contains 8 planets that orbit the sun, along with over 170 moons, thousands of asteroids, and many dwarf planets. It provides details about each planet's composition, distance from the sun, atmospheric conditions, temperatures, and other distinguishing features. The sun is identified as the largest object that contains 99.8% of the mass in the solar system and provides light, heat, and energy to hold the system together.
uranus
Uranus is a gas giant planet with an atmosphere composed primarily of hydrogen and helium. Unlike the other planets in the solar system, Uranus spins on its side due to a large collision in the past. Uranus has 27 known moons named after characters from Shakespearean plays. The planet is extremely cold with an average temperature of -224 degrees Celsius due to its composition and distance from the Sun. It has a system of faint rings and weather characterized by powerful winds and storms.
Uranus
Uranus was the first planet discovered with a telescope by William Herschel in 1781, though he initially thought it was a comet. It orbits the sun every 84 Earth years at a distance of about 3 billion km. Uranus rotates on its side with an axial tilt of 98 degrees, and has 27 known moons as well as 13 known rings composed of small, dark particles. Uranus is composed of ice and rock, and has a blue-green color due to the scattering of light by methane ice crystals in its atmosphere.
Solar system
The document provides facts about objects in our solar system including the Sun, planets Mercury through Neptune, dwarf planets, asteroids, and the Kuiper Belt. It notes key details about each such as the Sun containing 99% of the solar system's mass, Venus rotating backwards compared to other planets, Jupiter having the largest moon Ganymede, Saturn being the ringed planet, and the Kuiper Belt potentially containing over a trillion comet nuclei. It aims to inform readers about characteristics of astronomical bodies in our neighborhood.
ASTRONOMY
The document summarizes tides, including their causes due to the gravitational interaction between the Earth, Moon and Sun. It describes the stages of a tidal cycle from flood tide to low tide. It distinguishes between spring tides, which occur during full and new moons when gravitational forces align to produce stronger tides, and neap tides during quarter moons when forces are perpendicular and tides are weaker. Rare proxigean spring tides result from a close and aligned positioning of the Moon.
Neptune
Neptune is the 8th and farthest planet from the Sun. It is smaller than Uranus but more massive. Neptune was discovered in 1846 based on calculations by Urbain Le Verrier and independent predictions by John Couch Adams. Voyager 2 is the only spacecraft to have visited Neptune, discovering its rings and 6 of its 14 known moons during a flyby in 1989. Neptune has a rocky core and is composed primarily of ice giants with winds reaching over 1,500 mph.
Planets and Satellites
The document describes the inner and outer planets of the solar system, as well as their natural and artificial satellites. It provides details about the moons of each planet, including Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. It also discusses different types of artificial satellites such as communication, resource, navigation, military, scientific, and weather satellites and how they are used.
SATURN
Saturn is the sixth planet from the sun and orbits within 29 years. It rotates on its axis every 10.65 hours and is unique for being the largest planet with rings. Saturn's rotation is complex, with different rotational speeds depending on latitude - ranging from 10 hours and 14 minutes at the equator to 10 hours and 39 minutes above and below the equatorial belt. Ancient Babylonians first tracked Saturn as early as 1830 BC using just their naked eyes.
The sun
The sun is the largest object in the solar system, containing over 99% of its mass. It emits light and heat that support life on Earth and influence all solar system objects. The sun has various internal layers, including the core where energy is produced through nuclear fusion, and an outer atmosphere. Sunspots, solar flares, and other features periodically appear on its surface. In a few billion years, the sun will expand and grow hotter, eventually making Earth uninhabitable.
The solar system
The solar system consists of the Sun and everything bound to it by gravity, including 8 planets that orbit the Sun. The planets are Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. Other objects in the solar system include asteroids, comets, and meteors. Each planet has unique characteristics such as size, composition, temperature, and number of moons. Earth stands out as the only known planet capable of supporting life.
Uranus
Uranus is about four times the diameter of Earth and is the third largest planet. It orbits the Sun at a distance of approximately 1.8 billion miles. Uranus has 27 known moons, including its five largest - Miranda, Ariel, Umbriel, Titania, and Oberon. Uranus has a system of rings composed of ice particles. Although larger than Earth, Uranus' surface gravity is less due to its gaseous composition, which also gives it a blue appearance when viewed from Earth. Voyager 2 took almost nine and a half years to reach Uranus during its journey through the solar system.
Galaxies
There are several types of galaxies including spiral, elliptical, irregular, and barred galaxies. Spiral galaxies are the most common type and have tightly or loosely wound spiral arms. The Milky Way is a typical spiral galaxy located in the outer range of the galaxy. Other galaxy types include whirlpool galaxies like M51a, barred galaxies like NGC 1365, and elliptical galaxies which can be very large or small dwarf galaxies. Irregular galaxies have no distinct shape.
Solar system PPT
The document summarizes key facts about our solar system including:
- It contains 1 star, 8 planets, many moons, asteroids, comets and meteoroids.
- Terrestrial planets like Earth are rocky while Jovian planets like Jupiter are gaseous.
- Asteroids, meteoroids and comets originate from leftover material that did not form planets.
- The nebular hypothesis and condensation theory explain how the solar system formed from a large cloud or disk of dust and gas over billions of years.
Grade 7 SCIENCE
The Solar System is made up of the Sun and objects that orbit it. It formed 4.6 billion years ago from a giant cloud and is located in the Milky Way galaxy. The inner planets are terrestrial and composed of rock, while the outer planets are gas giants made of hydrogen and helium or ice giants. Smaller objects like asteroids, comets, and dwarf planets also orbit the Sun. The planets have varied features like atmospheres, rings, and moons. Life exists on Earth, the only known habitable world.
Saturn report
Saturn is the 6th planet from the Sun and 2nd largest planet in our Solar System. It is a gas giant made primarily of hydrogen and helium that spins very quickly, causing it to be flattened at the poles. Saturn is most notable for its intricate system of rings, comprised of ice particles and dust. Galileo first observed Saturn's rings in 1610, though he incorrectly thought they were moons on either side of the planet. Saturn has over 60 moons, many of which have been explored by space probes like Pioneer, Voyager, and Cassini-Huygens.
The Sun and Other Stars
Stars are balls of superheated gas, including our Sun which is at the center of our solar system. Stars appear as points of light in the sky because they are extremely far away, though most are similar in size to the Sun. All stars begin as clouds of dust and gas that condense to form stars, which will spend most of their life as average stars like the Sun before running out of fuel and expanding, collapsing, and potentially exploding as supernovae or becoming black holes.
Planet Uranus
Uranus has 27 known moons, with Oberon and Titania being the largest. The surfaces of the four largest moons are covered with craters formed by meteorites, and astronomers believe they are composed of ice and rock. Uranus has 13 dark, faint rings composed likely of ice and dust encircling its equator. Astronomers use telescopes to observe how Uranus orbits the sun in an oval path, taking 84 years to complete one revolution around a distance of approximately 3 billion kilometers from the sun. William Herschel first discovered Uranus in 1781 using a telescope.
The Planet Neptune
The document discusses the planet Neptune, including that it was discovered in 1846, has an average temperature of -360 degrees Fahrenheit, and is composed primarily of hydrogen, helium, and methane. It notes facts like Neptune's winds reaching speeds of 1,490 miles per hour and its orbital period being equivalent to 165 Earth years. The document also explains that while Neptune contains water, its atmosphere is not suitable for human life due to the lack of oxygen.
Neptune
Neptune is the eighth and farthest known planet from the Sun in our solar system. It is classified as an ice giant along with Uranus. Neptune was discovered in 1846 and is named after the Roman god of the sea. With winds up to 2,100 km/hr, Neptune has the fastest winds in the solar system. Voyager 2 is the only spacecraft to have visited Neptune, sending back data and images of the planet and its moons during its flyby in 1989.
The sun (more advanced)
Maybe too in-depth for most elementary students, but very good broad coverage for teacher background or more advanced students in elementary or middle school.
Uranus presentation
This document provides information about Uranus in 3 paragraphs and a conclusion. It notes that Uranus was named after the god of the sky due to its color, and was the first planet spotted through a telescope. The document describes Uranus' surface as made of gases like hydrogen, methane and helium with winds up to 200 mph. It states Uranus has over 25 moons with Ariel being the best known and Mab the smallest. The concluding paragraph compares Uranus and Earth, noting Uranus is colder, has rings, different composition and no solid surface.
ASTRONOMY
Astronomy is the scientific study of celestial objects and phenomena that originate outside Earth's atmosphere. It includes studying stars, planets, moons, nebulae, galaxies, and other astronomical objects as well as their evolution, physics, chemistry, and interactions. Related fields include cosmology, which studies the universe as a whole, and astrophysics which applies physics to astronomical objects and phenomena. Astronomy uses various methods of observation across the electromagnetic spectrum from radio to gamma rays. Some important astronomers mentioned include Galileo, who made early observations with telescopes and contributed to the scientific revolution, Hipparchus who created one of the first star catalogs, Edwin Hubble who discovered galaxies outside the Milky Way, and Johannes Kepler who explained the motions of planets
Solar system - a powerpoint presentation by Tanisha Pahwa - 5th
This document provides a summary of the solar system and its exploration in the form of a slideshow presentation. It begins with an introduction to the solar system, then provides details about each planet from the Sun to Neptune in individual slides. Additional slides cover other heavenly bodies like dwarf planets, asteroids, meteors, comets and the Indian Space Research Organisation (ISRO). The presentation includes interesting facts, diagrams and numbers about each topic. It aims to educate students in class 4 about the amazing facts of space and the universe.
NEPTUNE
Neptune is the eighth and farthest planet from the Sun. It has 4 rings and 14 known moons, including its largest moon Triton. Triton is unique among large moons as it is one of the few moons in the solar system known to be geologically active today, with geysers of icy particles. Neptune was officially discovered in 1846 based on calculations by Adams and Le Verrier, though Galileo had observed it earlier without recognizing it as a planet.
Planet Saturn
Saturn is the sixth planet from the sun and named after the Roman god of agriculture. It is a gas giant with 18 known moons, the largest being Titan which is bigger than Mercury. Saturn's iconic rings are made of ice particles and span over 270,000 km wide, though they are only about 30 meters thick. The rings are composed of three main sections divided by darker gaps. Saturn orbits the sun every 29.5 years and spins rapidly on its axis, completing a day every 10 hours.
Saturn Powerpoint Project
Saturn is the sixth planet from the Sun and has a diameter of about 120,536 km. It has no solid surface and is composed primarily of hydrogen and helium. Saturn was first discovered in 1610 and has been explored by spacecraft, with its most notable features being its prominent ring system. It takes Saturn approximately 29.46 Earth years to complete one orbit around the Sun.
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ASTRONOMY
The document summarizes tides, including their causes due to the gravitational interaction between the Earth, Moon and Sun. It describes the stages of a tidal cycle from flood tide to low tide. It distinguishes between spring tides, which occur during full and new moons when gravitational forces align to produce stronger tides, and neap tides during quarter moons when forces are perpendicular and tides are weaker. Rare proxigean spring tides result from a close and aligned positioning of the Moon.
Neptune
Neptune is the 8th and farthest planet from the Sun. It is smaller than Uranus but more massive. Neptune was discovered in 1846 based on calculations by Urbain Le Verrier and independent predictions by John Couch Adams. Voyager 2 is the only spacecraft to have visited Neptune, discovering its rings and 6 of its 14 known moons during a flyby in 1989. Neptune has a rocky core and is composed primarily of ice giants with winds reaching over 1,500 mph.
Planets and Satellites
The document describes the inner and outer planets of the solar system, as well as their natural and artificial satellites. It provides details about the moons of each planet, including Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. It also discusses different types of artificial satellites such as communication, resource, navigation, military, scientific, and weather satellites and how they are used.
SATURN
Saturn is the sixth planet from the sun and orbits within 29 years. It rotates on its axis every 10.65 hours and is unique for being the largest planet with rings. Saturn's rotation is complex, with different rotational speeds depending on latitude - ranging from 10 hours and 14 minutes at the equator to 10 hours and 39 minutes above and below the equatorial belt. Ancient Babylonians first tracked Saturn as early as 1830 BC using just their naked eyes.
The sun
The sun is the largest object in the solar system, containing over 99% of its mass. It emits light and heat that support life on Earth and influence all solar system objects. The sun has various internal layers, including the core where energy is produced through nuclear fusion, and an outer atmosphere. Sunspots, solar flares, and other features periodically appear on its surface. In a few billion years, the sun will expand and grow hotter, eventually making Earth uninhabitable.
The solar system
The solar system consists of the Sun and everything bound to it by gravity, including 8 planets that orbit the Sun. The planets are Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. Other objects in the solar system include asteroids, comets, and meteors. Each planet has unique characteristics such as size, composition, temperature, and number of moons. Earth stands out as the only known planet capable of supporting life.
Uranus
Uranus is about four times the diameter of Earth and is the third largest planet. It orbits the Sun at a distance of approximately 1.8 billion miles. Uranus has 27 known moons, including its five largest - Miranda, Ariel, Umbriel, Titania, and Oberon. Uranus has a system of rings composed of ice particles. Although larger than Earth, Uranus' surface gravity is less due to its gaseous composition, which also gives it a blue appearance when viewed from Earth. Voyager 2 took almost nine and a half years to reach Uranus during its journey through the solar system.
Galaxies
There are several types of galaxies including spiral, elliptical, irregular, and barred galaxies. Spiral galaxies are the most common type and have tightly or loosely wound spiral arms. The Milky Way is a typical spiral galaxy located in the outer range of the galaxy. Other galaxy types include whirlpool galaxies like M51a, barred galaxies like NGC 1365, and elliptical galaxies which can be very large or small dwarf galaxies. Irregular galaxies have no distinct shape.
Solar system PPT
The document summarizes key facts about our solar system including:
- It contains 1 star, 8 planets, many moons, asteroids, comets and meteoroids.
- Terrestrial planets like Earth are rocky while Jovian planets like Jupiter are gaseous.
- Asteroids, meteoroids and comets originate from leftover material that did not form planets.
- The nebular hypothesis and condensation theory explain how the solar system formed from a large cloud or disk of dust and gas over billions of years.
Grade 7 SCIENCE
The Solar System is made up of the Sun and objects that orbit it. It formed 4.6 billion years ago from a giant cloud and is located in the Milky Way galaxy. The inner planets are terrestrial and composed of rock, while the outer planets are gas giants made of hydrogen and helium or ice giants. Smaller objects like asteroids, comets, and dwarf planets also orbit the Sun. The planets have varied features like atmospheres, rings, and moons. Life exists on Earth, the only known habitable world.
Saturn report
Saturn is the 6th planet from the Sun and 2nd largest planet in our Solar System. It is a gas giant made primarily of hydrogen and helium that spins very quickly, causing it to be flattened at the poles. Saturn is most notable for its intricate system of rings, comprised of ice particles and dust. Galileo first observed Saturn's rings in 1610, though he incorrectly thought they were moons on either side of the planet. Saturn has over 60 moons, many of which have been explored by space probes like Pioneer, Voyager, and Cassini-Huygens.
The Sun and Other Stars
Stars are balls of superheated gas, including our Sun which is at the center of our solar system. Stars appear as points of light in the sky because they are extremely far away, though most are similar in size to the Sun. All stars begin as clouds of dust and gas that condense to form stars, which will spend most of their life as average stars like the Sun before running out of fuel and expanding, collapsing, and potentially exploding as supernovae or becoming black holes.
Planet Uranus
Uranus has 27 known moons, with Oberon and Titania being the largest. The surfaces of the four largest moons are covered with craters formed by meteorites, and astronomers believe they are composed of ice and rock. Uranus has 13 dark, faint rings composed likely of ice and dust encircling its equator. Astronomers use telescopes to observe how Uranus orbits the sun in an oval path, taking 84 years to complete one revolution around a distance of approximately 3 billion kilometers from the sun. William Herschel first discovered Uranus in 1781 using a telescope.
The Planet Neptune
The document discusses the planet Neptune, including that it was discovered in 1846, has an average temperature of -360 degrees Fahrenheit, and is composed primarily of hydrogen, helium, and methane. It notes facts like Neptune's winds reaching speeds of 1,490 miles per hour and its orbital period being equivalent to 165 Earth years. The document also explains that while Neptune contains water, its atmosphere is not suitable for human life due to the lack of oxygen.
Neptune
Neptune is the eighth and farthest known planet from the Sun in our solar system. It is classified as an ice giant along with Uranus. Neptune was discovered in 1846 and is named after the Roman god of the sea. With winds up to 2,100 km/hr, Neptune has the fastest winds in the solar system. Voyager 2 is the only spacecraft to have visited Neptune, sending back data and images of the planet and its moons during its flyby in 1989.
The sun (more advanced)
Maybe too in-depth for most elementary students, but very good broad coverage for teacher background or more advanced students in elementary or middle school.
Uranus presentation
This document provides information about Uranus in 3 paragraphs and a conclusion. It notes that Uranus was named after the god of the sky due to its color, and was the first planet spotted through a telescope. The document describes Uranus' surface as made of gases like hydrogen, methane and helium with winds up to 200 mph. It states Uranus has over 25 moons with Ariel being the best known and Mab the smallest. The concluding paragraph compares Uranus and Earth, noting Uranus is colder, has rings, different composition and no solid surface.
ASTRONOMY
Astronomy is the scientific study of celestial objects and phenomena that originate outside Earth's atmosphere. It includes studying stars, planets, moons, nebulae, galaxies, and other astronomical objects as well as their evolution, physics, chemistry, and interactions. Related fields include cosmology, which studies the universe as a whole, and astrophysics which applies physics to astronomical objects and phenomena. Astronomy uses various methods of observation across the electromagnetic spectrum from radio to gamma rays. Some important astronomers mentioned include Galileo, who made early observations with telescopes and contributed to the scientific revolution, Hipparchus who created one of the first star catalogs, Edwin Hubble who discovered galaxies outside the Milky Way, and Johannes Kepler who explained the motions of planets
Solar system - a powerpoint presentation by Tanisha Pahwa - 5th
This document provides a summary of the solar system and its exploration in the form of a slideshow presentation. It begins with an introduction to the solar system, then provides details about each planet from the Sun to Neptune in individual slides. Additional slides cover other heavenly bodies like dwarf planets, asteroids, meteors, comets and the Indian Space Research Organisation (ISRO). The presentation includes interesting facts, diagrams and numbers about each topic. It aims to educate students in class 4 about the amazing facts of space and the universe.
NEPTUNE
Neptune is the eighth and farthest planet from the Sun. It has 4 rings and 14 known moons, including its largest moon Triton. Triton is unique among large moons as it is one of the few moons in the solar system known to be geologically active today, with geysers of icy particles. Neptune was officially discovered in 1846 based on calculations by Adams and Le Verrier, though Galileo had observed it earlier without recognizing it as a planet.
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Solar system - a powerpoint presentation by Tanisha Pahwa - 5th
Solar system - a powerpoint presentation by Tanisha Pahwa - 5th
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Planet Saturn
Saturn is the sixth planet from the sun and named after the Roman god of agriculture. It is a gas giant with 18 known moons, the largest being Titan which is bigger than Mercury. Saturn's iconic rings are made of ice particles and span over 270,000 km wide, though they are only about 30 meters thick. The rings are composed of three main sections divided by darker gaps. Saturn orbits the sun every 29.5 years and spins rapidly on its axis, completing a day every 10 hours.
Saturn Powerpoint Project
Saturn is the sixth planet from the Sun and has a diameter of about 120,536 km. It has no solid surface and is composed primarily of hydrogen and helium. Saturn was first discovered in 1610 and has been explored by spacecraft, with its most notable features being its prominent ring system. It takes Saturn approximately 29.46 Earth years to complete one orbit around the Sun.
Saturn Planet
Saturn is the sixth planet from the Sun and the second largest planet in the Solar System, after Jupiter. Saturn is named after the Roman god Saturn, equated to the Greek Cronus (the Titan father of Zeus), the Babylonian Ninurta and the Hindu Shani.
Saturn
Saturn is the sixth planet from the sun and the second largest planet in the solar system. It is made up of hydrogen gas, with a liquid hydrogen middle layer and a rocky core. Saturn has over 60 moons, including Titan, which is the second largest moon in the solar system. Saturn also has a prominent ring system made of ice particles and dust. The Cassini-Huygens mission orbited Saturn from 2004 to 2017 and made many discoveries about the planet and its moons.
Saturn
Saturn is the second largest planet in our solar system. It is famous for its beautiful ring system, which is made of billions of ice particles and chunks held in place by moons. Saturn has over 50 moons, including Titan, its largest moon, and Enceladus, which has shown signs of geological activity.
Saturn’s Moons
Saturn has over 60 moons that vary greatly in size, composition, and orbital periods. Titan is Saturn's largest moon and the only one with a significant atmosphere. Other notable moons include Enceladus, which has geysers at its south pole, and Mimas, which resembles the Death Star due to a large impact crater. The moons formed early in the solar system's history and theories suggest they may have originated from larger moons that broke apart.
Saturn
Saturn is named after the Roman god of agriculture. It is the second largest planet in our solar system and is made up of gas with no surface. Saturn has a diameter of 74,500 miles and is 885,500,000 miles from the sun. It has no signs of life but has 23 moons and millions of small rings composed together.
Saturn Gn
Saturn is known for its prominent ring system. Early astronomers like Galileo first observed the rings, though they were not well understood until Christiaan Huygens correctly interpreted them as a ring system in 1659. The Cassini mission has returned stunning images of Saturn and its moons like Titan, greatly increasing scientific understanding of the Saturnian system.
Jupiter
Jupiter is the largest planet in our solar system, with a mass more than twice that of all other planets combined. It is composed primarily of gas and liquid and rotates faster than any other planet. Jupiter has the strongest magnetic field of any planet and has over 60 moons, four of which are large moons called the Galilean satellites that were discovered by Galileo. Europa may have subsurface oceans that could potentially support life. Many missions have been sent to Jupiter to study its atmosphere, magnetosphere, rings and moons.
Solar system 2011
The document provides information about the planets in our solar system:
- Mercury is the closest planet to the sun and has no moons. It has large temperature variations.
- Venus is very hot and cloudy with sulfuric acid clouds. It rotates in the opposite direction of other planets.
- Jupiter is the largest planet and has 49 moons. It has a big red storm on its surface.
- Saturn has rings made of ice, dust and rocks. It is the second largest planet and has 18 moons.
Saturn powerpoint project final publish
Saturn is the second largest planet in our solar system. It orbits the Sun between approximately 840-941 million miles away, taking around 29.5 Earth years to complete a revolution. Voyager probes first explored Saturn in the 1970s and 1980s, finding it to be a giant ball of gas with no solid surface but possibly a rocky core. Its atmosphere consists mainly of hydrogen and helium.
Saturn and its Moons
The Cassini spacecraft has captured new images of Saturn and its moons over the past few months. It photographed plumes erupting from Enceladus, a glint of sunlight reflecting off a lake on Titan, and detailed views of the surfaces of moons like Mimas, Tethys, and Dione. Cassini's photos provide striking glimpses of the dynamic Saturn system and its icy, cratered moons over 1 billion kilometers from Earth.
Saturn
Saturn is the second largest planet in our solar system. It is famous for its beautiful rings, which are made of billions of ice particles held in place by moons. Saturn has over 50 moons, including Titan, its largest moon, and Enceladus, which has underground oceans.
Saturn
Saturn got its name from the Roman god Saturnus. It was discovered in 1610 by Galileo in Rome using just his telescope to look up at the sky. Saturn is the sixth planet from the sun, takes just over 29 Earth years to complete its orbit, and has a day that is approximately 10 hours and 39 minutes long.
Saturn and its Satellites
Learn about the Saturn and its Satellites through this slide. This presentation slide was built for the purpose of my research in my university.
Titan's moon
Saturn´s Moon Titan shows many incredible features as; only liquid bodies observed in the solar other than Earth, huge seas of hydrocarbons, only moon with a thick atmosphere and also are similar to Earth in that it is dominated by nitrogen, methane and argon. Surface features consistent with erosion and however, it seems highly doubtful it is a good candidate for life.
Planet Saturnus
Planet Saturnus adalah planet terbesar keenam di tata surya yang memiliki cincin yang sangat luas dan indah. Planet ini memiliki rotasi 10 jam 14 menit dan revolusi 29,46 tahun. Atmosfer Saturnus terdiri dari hidrogen, helium, metana dan amonia. Saturnus memiliki 56 bulan alami, termasuk Titan yang memiliki ukuran lebih besar dari planet Merkurius.
Cassini-Huygens Mission to Saturn Overview
The international Cassini-Huygens spacecraft was launched on October 15, 1997 and had a marathon 7-year 2-billion mile journey to the distant planet Saturn. The 23-foot tall, 14-foot wide, 6-ton spacecraft is the largest most sophisticated outer planet spacecraft ever built, and is in its third year of operation in orbit around the planet Saturn. Cassini-Huygens has been returning extraordinary data about the entire Saturn system: the spectacular rings; the numerous icy satellites with a variety of unique surface features; the giant planet itself; a huge magneto-sphere teeming with particles that interact with the rings and moons; and the intriguing moon Titan, which is slightly larger than the planet Mercury, and whose hazy atmosphere is denser than that of Earth. This talk will be an overview of the Cassini-Huygens mission to Saturn with a summary of the top science returns of its first three years in orbit.
The Minnesota Space Grant Consortium, run out of the Department of Aerospace Engineering and Mechanics at the University of Minnesota, hosts Trina Ray of NASA JPL on January 22, 2008.
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1. The document provides an overview of the solar system, describing the planets, their orbits, and key discoveries about their properties and formation.
2. It discusses that planets can be divided into terrestrial and gas giant planets. Terrestrial planets are rocky, while gas giants are much larger and composed primarily of hydrogen and helium.
3. The properties of each planet are then summarized, including their composition, atmospheres, moons, and how observations of the planets led to ideas like gravity and orbital mechanics.
Solar system pp
The document provides information about the solar system and beyond. It summarizes that the solar system consists of the Sun and objects that orbit it, including 8 planets. It is located within the Milky Way galaxy, which contains many stars, dust and gas. The document then provides details about the properties of objects in the solar system like planets, moons, asteroids and comets.
Ch08 solar system
The Solar System formed around 4.5 billion years ago from the collapse of a giant cloud of gas and dust. The inner planets are rocky while the outer planets are gaseous. Planets formed from the accretion of planetesimals, which collided and stuck together in the protoplanetary disk surrounding the young Sun. The temperature differences in the disk led to different compositions, with rocky planets in the hot inner region and icy planets in the cold outer region. Over time, planetesimals bombarded planetary surfaces and the planets differentiated into layers. Some planets may have migrated from their initial orbits due to interactions with the gas disk.
Saturn
The document discusses Saturn, including its composition, atmosphere, temperature, rings, orbit and rotation, natural satellites, mass and density, and important facts. Saturn is composed primarily of hydrogen and helium. Its upper atmosphere contains ammonia crystals and clouds of water or ammonium hydrosulfide lower down. It has a banded atmosphere with some of the fastest winds in the solar system. Saturn is known for its prominent ring system and numerous moons, including Titan.
Solar system
The document provides an overview of the solar system, including the 8 planets and 5 dwarf planets. It discusses key facts about each planet and dwarf planet such as their atmospheres, moons, and distinguishing characteristics. For example, it notes that Venus rotates backwards compared to other planets and has a dense carbon dioxide atmosphere causing a greenhouse effect. It also explains the requirements for something to be considered a planet versus a dwarf planet.
solar system lesson.ppt
This document provides a review of key concepts about objects in our solar system, including the planets, moons, asteroids, comets, and meteors. It begins with an overview of the planets, noting characteristics like their composition, atmospheres, and positions from the Sun. Specific details are then given about each planet. The document also describes asteroids, comets, and meteors - including what they are made of and their orbits. It concludes with an announcement of an upcoming review quiz.
Solar system
The document provides an overview of the solar system, including definitions of key terms like revolve, rotate, orbit, and differences between inner and outer planets. It describes each planet from Mercury to Neptune, as well as dwarf planets like Pluto, Ceres, and Eris. Key facts are mentioned for each celestial body, such as atmospheric compositions and notable moons or features. The solar system is depicted pictorially with an interactive journey highlighted.
solar .ppt
The document provides information about the Sun and eight planets in our solar system:
- The Sun is a huge ball of hydrogen and helium gases at the center of our solar system that is approximately 4.5 billion years old. It supports all life on Earth.
- Mercury is the closest planet to the Sun and has almost no atmosphere. Venus is covered by thick, toxic clouds and has a runaway greenhouse effect. Earth is the only known planet capable of sustaining life.
- Mars has the largest dust storms in the solar system. Jupiter is a gas giant with a strong magnetic field and over 67 moons. Saturn is known for its extensive ring system.
Solar System
The Solar System formed 4.6 billion years ago from the collapse of a giant molecular cloud. It consists of the Sun and objects bound to it by gravity, including eight planets whose orbits are nearly circular, as well as dwarf planets, asteroids, comets, and other small bodies. The four inner terrestrial planets are composed mainly of rock, while the four outer gas giants are much more massive and composed largely of hydrogen and helium. Exploration of the Solar System has increased understanding of its formation and components.
Solar Sytem.pptx
The document summarizes theories about the formation of the solar system and provides information about the planets, moons, asteroids, meteoroids, and comets within our solar system. It discusses how the Nebular Hypothesis proposes that the solar system formed from a rotating gas cloud that condensed to form the sun and planets. It then gives brief descriptions and key facts about each planet from Mercury to Pluto, as well as asteroids, meteoroids, and comets.
Solar system.pptx
The document summarizes key aspects of our solar system. It describes the components of the solar system including the sun, planets, asteroids, comets, and dwarf planets. It then provides details about the inner and outer planets, distinguishing their compositions. Specific information is given about Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune and some of their moons and characteristics.
What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: Structure
The document summarizes the structure and components of the solar system. It describes:
1. The solar system formed from a large rotating cloud of gas and dust called the solar nebula approximately 4.6 billion years ago. As it contracted, the nebula flattened into a disk and kilometer-sized protoplanets began to form.
2. The solar system consists of the Sun and celestial objects bound to it by gravity, including eight planets composed of rock/metal or gas/hydrogen that orbit in nearly circular paths within the ecliptic plane.
3. Most planets have their own moons, and the gas giants have rings composed of tiny particles orbiting them. The solar system can be divided into
Introduction to the Solar System
This is a presentation that I completed for EDU 290 in the Fall 2009. The intent of the assignment was to create a lesson that could be used by a student that missed the classroom instruction due to illness
Science Planets powerpoint
The document provides information about the planets and dwarf planets in our solar system. It describes the 8 major planets and 5 dwarf planets, and discusses their key characteristics such as composition, atmosphere, rotation, and moons. Examples include Mercury having no atmosphere and many impact craters, Venus rotating backwards and having extreme temperatures, and Pluto being the first and largest dwarf planet discovered.
Solar System
The Solar System consists of the Sun and objects that orbit it, including 8 planets, dwarf planets, asteroids, and comets. The inner Solar System contains terrestrial planets like Earth that are composed of rock and metals. The outer Solar System contains gas giants like Jupiter and Saturn that account for most of the mass. Objects follow elliptical orbits around the Sun, with closer objects moving faster according to Kepler's laws of planetary motion. The Solar System is believed to have formed 4.6 billion years ago from the gravitational collapse of a giant molecular cloud.
solar lesson.ppt
The document provides information about the planets in our solar system as well as other objects such as asteroids, comets, and meteors. It discusses key facts about each planet such as their position from the sun, composition, atmosphere, moons, and other distinguishing features. It also summarizes that asteroids are small rocky or metallic objects that orbit the sun within and outside of Mars' orbit, in a region called the asteroid belt. Comets are small icy objects that have elliptical orbits bringing them close to and far from the sun, developing tails as they near the sun. Meteoroids enter the earth's atmosphere as meteors and some survive impact as meteorites.
Solar system-yvonne
The document summarizes key facts about the planets in our solar system. It describes the inner planets Mercury, Venus, Earth, and Mars, as well as the outer planets Jupiter, Saturn, Uranus, and Neptune. It also discusses dwarf planets Pluto, Ceres, and Eris. The document outlines characteristics of each planet such as their atmospheres, moons, rotation, and features.
Chapter 2 Solar System
The document summarizes key concepts about Earth's place in the solar system, including its rotation, revolution, and tilted axis which causes seasons. It describes the inner and outer planets, noting Mercury and Venus are closest to the Sun while gas giants Jupiter, Saturn, Uranus and Neptune are farthest. Comets and meteorites are also briefly outlined. The document then discusses stars, their colors and lifecycles, as well as galaxies like the Milky Way and concepts like light years and the expanding universe.
Introduction of Solar System
The document provides details about the composition and formation of the solar system. It can be summarized as follows:
1) The solar system formed from the gravitational collapse of part of a large cloud of gas and dust known as the solar nebula. This led to the formation of the Sun and a protoplanetary disk surrounding it.
2) As the Sun formed and began generating heat, the protoplanetary disk flattened into a plane and began to condense, resulting in the formation of the planets, asteroids, comets and other bodies that make up the solar system.
3) Over time, scientific understanding of solar system formation has progressed from early hypotheses to the current nebular model, which views
Notes on our solar system
Our solar system contains 1 sun, 8 planets, 5 dwarf planets, and over 170 moons. The planets are divided into two groups - terrestrial planets which are small and rocky, and gas giants which are much larger and composed primarily of hydrogen and helium. Terrestrial planets include Mercury, Venus, Earth, and Mars. Gas giants include Jupiter, Saturn, Uranus, and Neptune. Dwarf planets such as Ceres and Pluto have not cleared their orbital path. Pluto was reclassified as a dwarf planet after astronomers discovered other similar objects in the Kuiper belt.
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What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: Structure
What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: Structure
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Energy work and power web
Energy exists in various forms and can be transferred from one form to another but not created or destroyed. Work is the transfer of energy due to a force acting on an object over a distance. Kinetic energy is the energy of motion while potential energy is stored energy due to an object's position or composition. Chemical energy powers living things through photosynthesis and can be stored for later use. Nuclear energy is released through fusion in stars and fission in bombs and reactors. According to Einstein's equation, matter and energy are directly related and matter can be converted to energy.
Mass and weight
Mass is a measure of the amount of matter in an object and does not change in different environments, while weight is the force of gravitational attraction on an object which does change depending on location. Weight is calculated as mass times the acceleration of gravity (w=mg), where mass is measured in kilograms and weight in newtons. On the moon, an object's mass would remain the same but its weight would be about 1/6 of what it is on Earth due to the moon's lower gravity.
Newtons laws of_motion
1. Newton's laws of motion describe the relationship between an object and the forces acting upon it. Newton's three laws are: (1) an object at rest stays at rest and an object in motion stays in motion unless acted upon by an unbalanced force, (2) the acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, and (3) for every action, there is an equal and opposite reaction.
2. Free-body diagrams are used to represent the forces acting on an object using vectors. They help visualize and solve problems related to Newton's laws of motion.
3. Newton's laws of motion and concepts like inertia, acceleration, and friction
Light
Light can be described as both a wave and a particle. As a wave, it travels at 300 million meters per second and is characterized by its wavelength and frequency. The different wavelengths of light make up the electromagnetic spectrum, from radio waves to gamma rays. As the frequency increases, so does the energy of the electromagnetic waves. Light also behaves as particles called photons, which are emitted or absorbed in specific wavelengths by electrons in atoms. This allows spectroscopy to be used to determine the composition of different objects by their emission or absorption spectra.
Copernican revolution modern
- Newton united physics and astronomy through his laws of motion and law of gravitation.
- Henrietta Swann Leavitt discovered the relationship between the variable period of stars and their absolute brightness, enabling the determination of distances in the universe.
- Edwin Hubble observed Cepheid variables in the Andromeda Nebula, proving that it was actually another galaxy, demonstrating that the universe is larger than previously believed.
Brahe and kepler
Tycho Brahe made extensive and accurate astronomical observations over many years, amassing a large collection of data on planetary positions and movements. Johannes Kepler used Brahe's data to formulate his Three Laws of Planetary Motion, providing the first mathematically-based model of the solar system. Galileo used the newly invented telescope to make observations of the moon, planets, and stars that supported Copernicus' heliocentric theory and contradicted Aristotle's geocentric model, leading to conflict with the Church. Isaac Newton subsequently developed his laws of motion and universal law of gravitation, providing a unified framework for understanding motion and gravity in the heavens and on Earth.
Modern view copernicus
Nicolaus Copernicus (1473-1543) published his heliocentric theory in 1543, just before his death. He realized that placing the Sun at the center of the universe with planets revolving around it made calculations and predictions much easier. This contradicted the geocentric Ptolemaic system that had been accepted for over 1400 years. Though his system was only slightly less complicated, it marked the beginning of replacing the Earth-centered view of the universe with one centered on the Sun. The Catholic Church initially ignored Copernicus' theory but eventually banned his book in 1616 as his ideas threatened established authority.
Phase diagram notes
A phase diagram shows the conditions needed for different phases of matter to exist in equilibrium. It indicates that applying enough pressure to ice will cause it to melt into liquid water, as seen by the red line. The triple point of a substance is the unique temperature and pressure where its solid, liquid, and gas phases coexist. For water, this is 0.01°C and 0.006 atm.
Work, force, and energy
1. The document discusses different forms of energy including mechanical, heat, chemical, radiant, electrical, sound, and nuclear energy.
2. It explains that energy from the sun is transferred through a food chain from plants to animals and is measured in calories. Stored energy from the sun can be found in fossil fuels.
3. Potential energy is stored energy due to position, while kinetic energy is the energy of motion. The law of conservation of energy states that energy cannot be created or destroyed, just converted from one form to another.
Gas laws
The document discusses the gas laws of Boyle's law, Charles' law, and Gay-Lussac's law. Boyle's law states that the pressure and volume of a gas are inversely proportional at constant temperature. Charles' law describes the direct proportionality of volume and temperature at constant pressure. Gay-Lussac's law found the direct relationship between pressure and temperature when volume is kept constant. The document also defines ideal gases as having no particle volume or intermolecular forces, while real gases do have particle volume and intermolecular attractive forces.
Kinetic theory
Kinetic Molecular Theory describes the behavior of gases in terms of particles in motion. It makes several assumptions about the size, motion, and energy of gas particles. Specifically, it assumes that gas particles are small, move randomly in straight lines until colliding elastically, and have a distribution of kinetic energies determined by their masses and velocities. This theory explains the low density, compressibility, and diffusion of gases as well as how temperature and pressure arise from the motion and collisions of gas particles.
Stars print
The document summarizes key information about stars and stellar evolution:
- Proxima Centauri is the nearest star to our sun at about 270 km away, while the next closest stars are much farther.
- A star's apparent brightness depends on both its luminosity and distance from Earth. Luminosity is measured by absolute brightness or total power radiated.
- The Hertzsprung-Russell diagram plots stars' temperatures and luminosities and helped show stages of stellar evolution.
- Stars evolve through stages as giants, dwarfs, white and brown dwarfs, neutron stars, pulsars, planetary and diffuse nebulae as their cores fuse hydrogen and heavier elements.
Acids bases and salts
This document provides an introduction to acids, bases and salts. It discusses key concepts including:
1) Acids have a sour taste and feel, bases have a bitter taste and slippery feel. Acids react vigorously with metals while bases don't.
2) When acids and bases are mixed, a neutralization reaction occurs producing water and a salt.
3) Arrhenius defined acids as substances that release H+ ions in water and bases as those that release OH- ions. Bronsted-Lowry expanded this to include acids as proton donors and bases as proton acceptors.
4) The pH scale is used to measure acidity/basicity, with acids having a pH <7 and bases
The sun
The document summarizes key information about the Sun, including its interior structure, energy production through nuclear fusion, and atmospheric layers. The Sun's core produces energy through proton-proton fusion, with a small amount of mass being converted to energy. Sunspots occur in 11-year cycles and are associated with magnetic fields, while solar flares and coronal mass ejections can emit large amounts of energy and eject plasma into space.
Asteroids and comets
This document discusses debris in our solar system and its importance in understanding the origin and evolution of the early solar system. It provides an overview of asteroids, meteorites, comets, and impact craters on Earth. Evidence suggests an asteroid or comet impact was responsible for the extinction of dinosaurs 65 million years ago. The study of solar system debris holds keys to deciphering the history of our solar system.
Solutions
A solution is a homogeneous mixture composed of a solute dissolved in a solvent. A solution is formed through solvation, where solvent particles surround solute particles and pull them away from each other. The solubility of a substance depends on factors like temperature, pressure, and the properties of the solute and solvent. Increasing temperature, pressure, surface area, or agitation can increase solubility and the rate of solvation. Concentration refers to the ratio of solute to solvent and affects properties like reaction rates.
Dwarf planets
This document discusses dwarf planets in the solar system. It defines dwarf planets as celestial bodies that orbit the sun, are massive enough to be rounded by their own gravity, but have not cleared their orbit of other objects. It provides details on the five officially recognized dwarf planets: Ceres, Pluto, Eris, Haumea, and Makemake. It describes their sizes, compositions, orbits, and discoveries.
Uranus and neptune
Uranus and Neptune are cold, gaseous planets discovered in the last 350 years using telescopes and mathematics. They have similar physical properties but Neptune shows more surface features. Uranus's unique tilted axis causes extreme seasons, while Neptune has unexplained internal heat. Both planets have moon systems, with Triton in a rare retrograde orbit around Neptune. Faint rings have also been detected circling Uranus and Neptune.
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Saturn
- 1. Saturn
- 2. Orbital and Physical Properties Mass: 5.7 × 10 26 kg (97 times Earth) Radius: 60,000 km (9.5 times Earth, .8 times Jupiter) Density: 700 kg/m 3 – less than water! Rotation: rapid and differential, enough to flatten Saturn considerably Rings: very prominent; wide but extremely thin
- 6. Saturn’s Atmosphere Wind patterns on Saturn are similar to those on Jupiter, with zonal flow :
- 7. Saturn’s Atmosphere Jupiter-style “ spots ” rare on Saturn; don’t form often and quickly dissipate if they do
- 8. A Storm on Saturn
- 10. Saturn’s Interior and Magnetosphere Interior structure similar to Jupiter’s:
- 12. Saturn’s Interior and Magnetosphere Saturn also has a strong magnetic field , but only 5% as strong as Jupiter’s Creates aurorae :
- 13. Saturn’s Spectacular Ring System Saturn has an extraordinarily large and complex ring system , which was visible even to the first telescopes
- 14. Saturn’s Spectacular Ring System Ring features visible from Earth:
- 15. Saturn’s rings are not in order
- 16. Saturn's rings change their appearance to terrestrial observers as the tilted ring plane orbits the Sun.
- 18. Roche Limit
- 19. Saturn’s Spectacular Ring System Closest distance that moon could survive is called Roche limit ; ring systems are all inside this limit
- 20. Saturn’s Spectacular Ring System Voyager probes showed Saturn’s rings to be much more complex than originally thought Earth is shown on the same scale as the rings
- 21. Saturn’s Spectacular Ring System Voyager also found radial “ spokes ” that formed and then dissipated; this probably happens frequently
- 22. Saturn’s Spectacular Ring System Cassini division turns out not to be completely empty: It is caused by an orbital resonance with other ring particles and Saturn’s innermost moon
- 23. Saturn’s Spectacular Ring System Strangest ring is outermost, F ring: It appears to have braids and kinks .
- 24. Saturn’s Spectacular Ring System F ring’s oddities probably caused by two shepherd moons , one of which can be seen here:
- 26. The Moons of Saturn Saturn’s many moons appear to be made of water ice Besides the small moons, Saturn has: Six medium-sized moons ( Mimas , Enceladus , Tethys , Dione , Rhea , and Iapetus ) One large moon ( Titan ) which is almost as large as Ganymede
- 28. The Moons of Saturn: Titan Titan has been known for many years to have an atmosphere thicker and denser than Earth’s; mostly nitrogen and argon Makes surface impossible to see; the picture at right was taken from only 4000 km away:
- 29. The Moons of Saturn: Titan Trace chemicals in Titan’s atmosphere make it chemically complex
- 30. The Moons of Saturn: Titan Due to difficulty of getting information, little is known about either the surface or the interior structure of Titan. This image, taken with an infrared telescope, shows some indication of surface features :
- 33. Huygens to Titan
- 34. The Moons of Saturn: The Medium-Sized Moons
- 36. The Moons of Saturn: The Medium-Sized Moons Rhea , the largest, has a highly reflective, heavily cratered surface: Wispy features are on trailing side but not leading; origin not yet understood:
- 37. The Moons of Saturn: The Medium-Sized Moons Dione and Tethys are similar, having icy, heavily cratered surfaces:
- 38. The Moons of Saturn: The Medium-Sized Moons Mimas is the closest moon to Saturn, and has a crater covering one-third of its surface, the result of an impact that must have almost destroyed the moon: That’s no moon! Oh, no. It totally is a moon.
- 39. The Moons of Saturn: The Medium-Sized Moons Enceladus orbits close to Mimas, but is very shiny , indicating a surface covered with ice crystals:
- 40. The Moons of Saturn: The Medium-Sized Moons Iapetus is two-faced: its leading side is very dark (reflects 3% of incoming light), while its trailing side is bright (reflects 50% of incoming light). Cause is unknown.
- 41. Iapetus
- 46. The Other Side of Saturn