Jupiter, Saturn, Uranus, and Neptune
... similar densities indicating that they were not heated by Saturn as they formed • Saturn’s moons have a smaller density than those of Jupiter indicating interiors must be mostly ice • Most moons are inundated with craters, many of which are surrounded by white markings of shattered ice • The moons a ...
... similar densities indicating that they were not heated by Saturn as they formed • Saturn’s moons have a smaller density than those of Jupiter indicating interiors must be mostly ice • Most moons are inundated with craters, many of which are surrounded by white markings of shattered ice • The moons a ...
the outer planets, their satellites and the plutoids
... 2. A planet must also have enough mass to become nearly spherical. 3. And a planet must be able to sweep other small astronomical objects out of its orbital path. 4. The object must have a maximum magnitude larger than 1+. Such objects will be called Plutoids or trans-Neptunian Objects. Satellite ...
... 2. A planet must also have enough mass to become nearly spherical. 3. And a planet must be able to sweep other small astronomical objects out of its orbital path. 4. The object must have a maximum magnitude larger than 1+. Such objects will be called Plutoids or trans-Neptunian Objects. Satellite ...
Smaller Bodies of the Solar System
... proposed as source for long-period comets and a replenisher of the Oort Cloud. beyond Neptune (extending from 30 AU out to around 100 AU). occasionally disturbed by gravitational interactions these objects are sent hurtling into the inner solar system to become short-period comets ...
... proposed as source for long-period comets and a replenisher of the Oort Cloud. beyond Neptune (extending from 30 AU out to around 100 AU). occasionally disturbed by gravitational interactions these objects are sent hurtling into the inner solar system to become short-period comets ...
Jupiter`s ring
... object (e.g. a moon) can exist, as a body held together by its selfgravity, as it orbits a more massive body (e.g. its parent planet); closer in, and the smaller body is ripped to pieces by the tidal forces on it. Read more: http://www.universetoday.com/56538/rochelimit/#ixzz2DXWFSN5Q ...
... object (e.g. a moon) can exist, as a body held together by its selfgravity, as it orbits a more massive body (e.g. its parent planet); closer in, and the smaller body is ripped to pieces by the tidal forces on it. Read more: http://www.universetoday.com/56538/rochelimit/#ixzz2DXWFSN5Q ...
Universe Now - Course Pages of Physics Department
... colour), and nitrogen present. – Highly inclined orbit (29 degrees). ...
... colour), and nitrogen present. – Highly inclined orbit (29 degrees). ...
Ch10_Lecture
... densities indicating that they were not heated by Saturn as they formed • Saturn’s moons have a smaller density than those of Jupiter indicating interiors must be mostly ice • Most moons are inundated with craters, many of which are surrounded by white markings of shattered ice • The moons also have ...
... densities indicating that they were not heated by Saturn as they formed • Saturn’s moons have a smaller density than those of Jupiter indicating interiors must be mostly ice • Most moons are inundated with craters, many of which are surrounded by white markings of shattered ice • The moons also have ...
Chapter 10 The Outer Worlds… Jupiter Jupiter Jupiter`s Interior
... objects • These objects are very dark, implying they are rich in carbon particles or organic-like materials • The extremely narrow rings may be held in place by shepherding satellites ...
... objects • These objects are very dark, implying they are rich in carbon particles or organic-like materials • The extremely narrow rings may be held in place by shepherding satellites ...
11/11/08 Chapter 9 The Outer Worlds… Jupiter Jupiter Jupiter`s
... • Beyond the orbit of Mars, the low temperatures of the solar nebula allowed condensing bodies there to capture hydrogen and hydrogen-rich gases • This, together with the vast amount of material in the outer Solar System, lead to the creation of the four large Jovian planets – Jupiter, Saturn, Uranu ...
... • Beyond the orbit of Mars, the low temperatures of the solar nebula allowed condensing bodies there to capture hydrogen and hydrogen-rich gases • This, together with the vast amount of material in the outer Solar System, lead to the creation of the four large Jovian planets – Jupiter, Saturn, Uranu ...
Solar System 2
... • Jupiter, the largest planet in the solar system, is about 11 times Earth’s diameter and 318 times Earth’s mass. • Jupiter is similar to the Sun in composition, consisting mostly of hydrogen and helium with only about 2% heavier elements. • The clouds in Jupiter’s atmosphere consist of frozen ammon ...
... • Jupiter, the largest planet in the solar system, is about 11 times Earth’s diameter and 318 times Earth’s mass. • Jupiter is similar to the Sun in composition, consisting mostly of hydrogen and helium with only about 2% heavier elements. • The clouds in Jupiter’s atmosphere consist of frozen ammon ...
The Asteroid Belt - peterboroughastronomy.com
... The first thing we should establish is the difference between an asteroid and a comet. In the very simplest terms an asteroid is a chunk of rock that orbits the Sun and is within our solar system. A comet is a giant dirty snowball that is pulled in from a very distant area called the Oort Cloud. Thi ...
... The first thing we should establish is the difference between an asteroid and a comet. In the very simplest terms an asteroid is a chunk of rock that orbits the Sun and is within our solar system. A comet is a giant dirty snowball that is pulled in from a very distant area called the Oort Cloud. Thi ...
Is Pluto a planet or a Kuiper Belt comet?
... planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the • How are meteorites related to asteroid belt today. Most asteroids? asteroids in other regions of the inner solar system accreted into • Most meteorites are pieces of asteroids. Pri ...
... planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the • How are meteorites related to asteroid belt today. Most asteroids? asteroids in other regions of the inner solar system accreted into • Most meteorites are pieces of asteroids. Pri ...
Chapter 9
... densities indicating that they were not heated by Saturn as they formed • Saturn’s moons have a smaller density than those of Jupiter indicating interiors must be mostly ice • Most moons are inundated with craters, many of which are surrounded by white markings of shattered ice • The moons also have ...
... densities indicating that they were not heated by Saturn as they formed • Saturn’s moons have a smaller density than those of Jupiter indicating interiors must be mostly ice • Most moons are inundated with craters, many of which are surrounded by white markings of shattered ice • The moons also have ...
Life on Jovian Moons
... • The ice grains contained H, so a large amount of mass came together • When large enough, gravity took over from collisions in building a bigger body (‘direct gravitational accumulation’) • 4 large moons, the ‘Galilean Moons’ ...
... • The ice grains contained H, so a large amount of mass came together • When large enough, gravity took over from collisions in building a bigger body (‘direct gravitational accumulation’) • 4 large moons, the ‘Galilean Moons’ ...
MINOR Members of the Solar System
... 1. interplanetary debris that was not gravitationally swept up by the planets during the formation of the solar system, 2. material from the asteroid belt, or 3. the solid remains of comets that once traveled near Earth’s orbit A few meteoroids are believed to be fragments of the moon, or possibly M ...
... 1. interplanetary debris that was not gravitationally swept up by the planets during the formation of the solar system, 2. material from the asteroid belt, or 3. the solid remains of comets that once traveled near Earth’s orbit A few meteoroids are believed to be fragments of the moon, or possibly M ...
CH28 Solar System - Van Buren Public Schools
... would evolved into a small star. Despite its great size, however, it is only 1/800 as massive as the sun. Jupiter revolves around the Sun once every 12 Earthyears, and rotates more rapidly than any other planet, completing one rotation in slightly less than 10 hours. ...
... would evolved into a small star. Despite its great size, however, it is only 1/800 as massive as the sun. Jupiter revolves around the Sun once every 12 Earthyears, and rotates more rapidly than any other planet, completing one rotation in slightly less than 10 hours. ...
2/1/2012- Outer Planets Notes
... • Continuous storms of swirling, high-pressure gas have been observed on Jupiter. • The Great Red Spot is the most spectacular of these storms. ...
... • Continuous storms of swirling, high-pressure gas have been observed on Jupiter. • The Great Red Spot is the most spectacular of these storms. ...
Asteroids,Comets, Meteor ppt.
... planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the • How are meteorites related to asteroid belt today. Most asteroids? asteroids in other regions of the inner solar system accreted into • Most meteorites are pieces of asteroids. Pri ...
... planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the • How are meteorites related to asteroid belt today. Most asteroids? asteroids in other regions of the inner solar system accreted into • Most meteorites are pieces of asteroids. Pri ...
Asteroids,Comets, Meteor ppt.
... planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the • How are meteorites related to asteroid belt today. Most asteroids? asteroids in other regions of the inner solar system accreted into • Most meteorites are pieces of asteroids. Pri ...
... planetesimals, preventing them from accreting into a planet. Those that were not ejected from this region make up the • How are meteorites related to asteroid belt today. Most asteroids? asteroids in other regions of the inner solar system accreted into • Most meteorites are pieces of asteroids. Pri ...
Chapter 9
... system, but unlike Jupiter, Saturn’s moons are of similar densities indicating that they were not heated by Saturn as they formed • Saturn’s moons have a smaller density than those of Jupiter indicating interiors must be mostly ice • Most moons are inundated with craters, many of which are surrounde ...
... system, but unlike Jupiter, Saturn’s moons are of similar densities indicating that they were not heated by Saturn as they formed • Saturn’s moons have a smaller density than those of Jupiter indicating interiors must be mostly ice • Most moons are inundated with craters, many of which are surrounde ...
Juno
... spacecraft's pointing extremely stable and easy to control. Just after launch, and before its solar arrays are deployed, Juno will be spun-up by rocket motors on its still attached second-stage rocket booster. While in orbit at Jupiter, the spinning spacecraft sweeps the fields of view of its instru ...
... spacecraft's pointing extremely stable and easy to control. Just after launch, and before its solar arrays are deployed, Juno will be spun-up by rocket motors on its still attached second-stage rocket booster. While in orbit at Jupiter, the spinning spacecraft sweeps the fields of view of its instru ...
what is a comet? - Fireballs in the sky
... that occurs in mid-October from the debris of Halley’s Comet. During the Orionids it is possible to see up to 70 meteors an hour. These meteors appear to radiate from between the constellations of Gemini and Orion, which is why they are named the Orionids. Outer Solar System: The region of the solar ...
... that occurs in mid-October from the debris of Halley’s Comet. During the Orionids it is possible to see up to 70 meteors an hour. These meteors appear to radiate from between the constellations of Gemini and Orion, which is why they are named the Orionids. Outer Solar System: The region of the solar ...
Impact Earth
... • Its orbit did not bring it close enough for the Earth’s gravity to pull it down. • Friction with the atmosphere would have caused it to burn up before it reached the ground. Small asteroids come as close as this every year or two. The unusual thing about the fly-past of 2004 FH was that astronomer ...
... • Its orbit did not bring it close enough for the Earth’s gravity to pull it down. • Friction with the atmosphere would have caused it to burn up before it reached the ground. Small asteroids come as close as this every year or two. The unusual thing about the fly-past of 2004 FH was that astronomer ...
WHAT ELSE IS OUT THERE BESIDES THE PLANETS
... planet that was destroyed in a massive collision long ago. The second theory is that asteroids are material that never formed a planet. In fact, if the estimated total mass of all asteroids was gathered into a single object, the object would be less than 932 miles across -- less than half the diamet ...
... planet that was destroyed in a massive collision long ago. The second theory is that asteroids are material that never formed a planet. In fact, if the estimated total mass of all asteroids was gathered into a single object, the object would be less than 932 miles across -- less than half the diamet ...
space-rocks - WLWV Staff Blogs
... orbit the sun in a belt between Mars and Jupiter. Scientists think there are probably millions of asteroids, ranging widely in size from hundreds of kilometers wide. Occasionally, asteroids’ orbital paths are influenced by the gravitational tug of planets, which cause their paths to alter. Scientist ...
... orbit the sun in a belt between Mars and Jupiter. Scientists think there are probably millions of asteroids, ranging widely in size from hundreds of kilometers wide. Occasionally, asteroids’ orbital paths are influenced by the gravitational tug of planets, which cause their paths to alter. Scientist ...
Comets - Images
... made of ice. When they approach the Sun the ice starts to evaporate forming the coma, a halo around the nucleus of dust and gas. Radiation pressure from the Sun pushes some of this dust and gas outwards (away from the Sun) to form two tails - one straight and blue (gas and ions), the other curved an ...
... made of ice. When they approach the Sun the ice starts to evaporate forming the coma, a halo around the nucleus of dust and gas. Radiation pressure from the Sun pushes some of this dust and gas outwards (away from the Sun) to form two tails - one straight and blue (gas and ions), the other curved an ...
Comet Shoemaker–Levy 9
Comet Shoemaker–Levy 9 (formally designated D/1993 F2) was a comet that broke apart and collided with Jupiter in July 1994, providing the first direct observation of an extraterrestrial collision of Solar System objects. This generated a large amount of coverage in the popular media, and the comet was closely observed by astronomers worldwide. The collision provided new information about Jupiter and highlighted its role in reducing space debris in the inner Solar System.The comet was discovered by astronomers Carolyn and Eugene M. Shoemaker and David Levy. Shoemaker–Levy 9, at the time captured by and orbiting Jupiter, was located on the night of March 24, 1993, in a photograph taken with the 40 cm (16 in) Schmidt telescope at the Palomar Observatory in California. It was the first comet observed to be orbiting a planet, and had probably been captured by the planet around 20 – 30 years earlier.Calculations showed that its unusual fragmented form was due to a previous closer approach to Jupiter in July 1992. At that time, the orbit of Shoemaker–Levy 9 passed within Jupiter's Roche limit, and Jupiter's tidal forces had acted to pull apart the comet. The comet was later observed as a series of fragments ranging up to 2 km (1.2 mi) in diameter. These fragments collided with Jupiter's southern hemisphere between July 16 and July 22, 1994, at a speed of approximately 60 km/s (37 mi/s) or 216,000 km/h (134,000 mph). The prominent scars from the impacts were more easily visible than the Great Red Spot and persisted for many months.