word
... Claims that the Solar System has a tenth planet are bolstered by the finding by a group lead by Bonn astrophysicists that this putative planet, announced last summer and tentatively named 2003 UB313, is bigger than Pluto. By measuring its thermal emission, the scientists were able to determine a dia ...
... Claims that the Solar System has a tenth planet are bolstered by the finding by a group lead by Bonn astrophysicists that this putative planet, announced last summer and tentatively named 2003 UB313, is bigger than Pluto. By measuring its thermal emission, the scientists were able to determine a dia ...
New "planet" is larger than Pluto
... Claims that the Solar System has a tenth planet are bolstered by the finding by a group lead by Bonn astrophysicists that this putative planet, announced last summer and tentatively named 2003 UB313, is bigger than Pluto. By measuring its thermal emission, the scientists were able to determine a dia ...
... Claims that the Solar System has a tenth planet are bolstered by the finding by a group lead by Bonn astrophysicists that this putative planet, announced last summer and tentatively named 2003 UB313, is bigger than Pluto. By measuring its thermal emission, the scientists were able to determine a dia ...
All About Saturn
... with the wide, flat rings is the sixth planet from the sun and sits between Jupiter and Uranus. Recent exploratory missions to the planet have revealed many interesting features that will be of interest to scientists for years to come. Saturn is the second largest planet behind Jupiter with a fast r ...
... with the wide, flat rings is the sixth planet from the sun and sits between Jupiter and Uranus. Recent exploratory missions to the planet have revealed many interesting features that will be of interest to scientists for years to come. Saturn is the second largest planet behind Jupiter with a fast r ...
Asteroids and Meteorites
... • Meteorites let us sample the primiFve and processed material elsewhere in the solar system • Most originate in the asteroid belt • Most are idenFfiable with an asteroid family • Large rocks will hit ...
... • Meteorites let us sample the primiFve and processed material elsewhere in the solar system • Most originate in the asteroid belt • Most are idenFfiable with an asteroid family • Large rocks will hit ...
Survey of Solar Systems
... Although we have only walked on the Earth and the Moon, we have detailed pictures sent to us from spacecraft of most of the planets and their satellites. Some are baren balls of rock; others are mostly ice. Some have thin, frigid atmospheres so cold that ordinary gases crystallize as snow on their c ...
... Although we have only walked on the Earth and the Moon, we have detailed pictures sent to us from spacecraft of most of the planets and their satellites. Some are baren balls of rock; others are mostly ice. Some have thin, frigid atmospheres so cold that ordinary gases crystallize as snow on their c ...
Chapter 11 Jovian Planet Systems Are jovian
... •! How do other jovian ring systems compare to Saturn’s? •! Jovian planets all have rings because they possess many small moons close-in •! Impacts on these moons are random •! Saturn’s incredible rings may be an “accident” of our time ...
... •! How do other jovian ring systems compare to Saturn’s? •! Jovian planets all have rings because they possess many small moons close-in •! Impacts on these moons are random •! Saturn’s incredible rings may be an “accident” of our time ...
Dating the Universe
... ! Jupiter's gravity influences nearby planetesimals ! Nearby planetesimal orbits made more eccentric – Higher eccentricity means higher impact velocities – Higher impact velocities mean less "sticking" – Planetesimals cannot accrete and grow very well Astro 202 ...
... ! Jupiter's gravity influences nearby planetesimals ! Nearby planetesimal orbits made more eccentric – Higher eccentricity means higher impact velocities – Higher impact velocities mean less "sticking" – Planetesimals cannot accrete and grow very well Astro 202 ...
11_LectureOutlines
... because the particles are too small to have survived this long. • There must be a continuous replacement of tiny particles. • The most likely source is impacts with the jovian moons. ...
... because the particles are too small to have survived this long. • There must be a continuous replacement of tiny particles. • The most likely source is impacts with the jovian moons. ...
Formation of the Solar System
... 1. Examine Figure 1, which shows the orbits of the inner planets. In general, what shape are the inner ...
... 1. Examine Figure 1, which shows the orbits of the inner planets. In general, what shape are the inner ...
What is a Planet?
... A similar challenge accompanied the recognition of the asteroid belt. When Piazzi discovered Ceres in 1801, astronomers welcomed it as the missing planet that filled the gap between the orbits of Mars and Jupiter, according to Bode’s Law (later shown to be specious). But in 1802 Olbers discovered Pa ...
... A similar challenge accompanied the recognition of the asteroid belt. When Piazzi discovered Ceres in 1801, astronomers welcomed it as the missing planet that filled the gap between the orbits of Mars and Jupiter, according to Bode’s Law (later shown to be specious). But in 1802 Olbers discovered Pa ...
Juno_NASA
... water-ice. These icy planetesimals could have carried in the other, more volatile, elements trapped within the ice. Colder ice would carry more volatiles, so Jupiter’s water content will tell us whether or not Jupiter formed farther from the Sun and drifted in to it’s current location. If Juno does ...
... water-ice. These icy planetesimals could have carried in the other, more volatile, elements trapped within the ice. Colder ice would carry more volatiles, so Jupiter’s water content will tell us whether or not Jupiter formed farther from the Sun and drifted in to it’s current location. If Juno does ...
Jupiter
... With its powerful gravity, Jupiter sucked up many of them and also kicked lots of them out of the Solar System that could have hit Earth. Because of this, Jupiter is sometimes called the Solar System’s vacuum cleaner. Although things have calmed down, impacts do still happen from time to time, as d ...
... With its powerful gravity, Jupiter sucked up many of them and also kicked lots of them out of the Solar System that could have hit Earth. Because of this, Jupiter is sometimes called the Solar System’s vacuum cleaner. Although things have calmed down, impacts do still happen from time to time, as d ...
3.4, 3.5, 3.6 Notes
... What are the terrestrial planets? • The terrestrial planets are the four small, dense, rocky planets that orbit closest to the sun. In order by distance from the sun, these planets are Mercury, Venus, Earth, and Mars. The terrestrial planets have similar compositions and consist of an outer crust ...
... What are the terrestrial planets? • The terrestrial planets are the four small, dense, rocky planets that orbit closest to the sun. In order by distance from the sun, these planets are Mercury, Venus, Earth, and Mars. The terrestrial planets have similar compositions and consist of an outer crust ...
Voyager Thorugh Space - Open Court Resources.com
... • The gravitational attraction between two very large distant objects can be strong enough to pull them toward each other. • word structure; apposition; context clues • Def. n. a force that pulls two free bodies or objects toward each other (pg.171) November 2008 ...
... • The gravitational attraction between two very large distant objects can be strong enough to pull them toward each other. • word structure; apposition; context clues • Def. n. a force that pulls two free bodies or objects toward each other (pg.171) November 2008 ...
PHAS 2B17 Physics of the Solar System
... most of the light scattered from a comet at optical wavelengths is scattered by daughters. For this reason, the daughters have received a lot of observational attention and many are well understood. What we would prefer to understand is the origin and abundance of the parent molecules, but the paren ...
... most of the light scattered from a comet at optical wavelengths is scattered by daughters. For this reason, the daughters have received a lot of observational attention and many are well understood. What we would prefer to understand is the origin and abundance of the parent molecules, but the paren ...
The Dwarf Planets
... to become round comes from looking at icy satellites of the giant planets. The smallest body that is generally round is Saturn's satellite Mimas, which has a diameter of about 400 km. Several satellites which have diameters around 200 km are not round. So somewhere between 200 and 400 km an icy body ...
... to become round comes from looking at icy satellites of the giant planets. The smallest body that is generally round is Saturn's satellite Mimas, which has a diameter of about 400 km. Several satellites which have diameters around 200 km are not round. So somewhere between 200 and 400 km an icy body ...
chapter11JovianPlane..
... because the particles are too small to have survived this long. • There must be a continuous replacement of tiny particles. • The most likely source is impacts with the jovian moons. ...
... because the particles are too small to have survived this long. • There must be a continuous replacement of tiny particles. • The most likely source is impacts with the jovian moons. ...
19uranusneptune5s
... Uranus was discovered in 1781 by William Herschel while surveying the sky Herschel had built a very high quality telescope and was systematically observing the brighter stars when he found Uranus ...
... Uranus was discovered in 1781 by William Herschel while surveying the sky Herschel had built a very high quality telescope and was systematically observing the brighter stars when he found Uranus ...
Powerpoint Presentation (large file)
... 1. How did Uranus and Neptune come to be discovered? 2. What gives Uranus its distinctive greenish-blue color? 3. Why are the clouds on Neptune so much more visible than those on Uranus? 4. Are Uranus and Neptune merely smaller versions of Jupiter and Saturn? 5. What is so unusual about the magnetic ...
... 1. How did Uranus and Neptune come to be discovered? 2. What gives Uranus its distinctive greenish-blue color? 3. Why are the clouds on Neptune so much more visible than those on Uranus? 4. Are Uranus and Neptune merely smaller versions of Jupiter and Saturn? 5. What is so unusual about the magnetic ...
Prelab 2: The “Planet Walk” Lab
... 1. (4 points) Determine the scale factor of the model: The easiest way to do this is to determine the diameter of the model sun or a model planet, and then compare this to the actual diameter listed in your textbook (or other resource). The ratio of the actual size to this measured scale-model size ...
... 1. (4 points) Determine the scale factor of the model: The easiest way to do this is to determine the diameter of the model sun or a model planet, and then compare this to the actual diameter listed in your textbook (or other resource). The ratio of the actual size to this measured scale-model size ...
Habitability potential of icy moons around giant planets and the
... Hydrodynamic coupling Gravita;onal coupling Electromagne;c coupling ...
... Hydrodynamic coupling Gravita;onal coupling Electromagne;c coupling ...
a Kuiper Belt object?
... comets still reside in the region beyond Neptune in which they formed during the birth of the solar system. The Oort cloud comets are thought to have formed in the region of the jovian planets, and were kicked out to the great distance of the Oort cloud by gravitational encounters with the planets. ...
... comets still reside in the region beyond Neptune in which they formed during the birth of the solar system. The Oort cloud comets are thought to have formed in the region of the jovian planets, and were kicked out to the great distance of the Oort cloud by gravitational encounters with the planets. ...