![Lecture 1](http://s1.studyres.com/store/data/008591908_1-ee76986a3843192fcdd7a9e7def5aa78-300x300.png)
Lecture 1
... particles of ice and ice-coated rock ranging in size from a few micrometers to about 10 m • Jupiter’s faint rings are composed of a relatively small amount of small, dark, rocky particles that reflect very little light ...
... particles of ice and ice-coated rock ranging in size from a few micrometers to about 10 m • Jupiter’s faint rings are composed of a relatively small amount of small, dark, rocky particles that reflect very little light ...
Jupiter Jupiter is the largest planet in the solar system. Its diameter is
... discovered a comet near Jupiter. The comet, later named Shoemaker-Levy 9, probably once orbited the sun independently, but had been pulled by Jupiter's gravity into an orbit around the planet. When the comet was discovered, it had broken into 21 pieces. The comet probably had broken apart when it pa ...
... discovered a comet near Jupiter. The comet, later named Shoemaker-Levy 9, probably once orbited the sun independently, but had been pulled by Jupiter's gravity into an orbit around the planet. When the comet was discovered, it had broken into 21 pieces. The comet probably had broken apart when it pa ...
The Revolution of the Moons of Jupiter
... Therefore, the perpendicular distance of the moon should be a sinusoidal curve if you plot it versus time (see Figure 2). By taking enough measurements of the position of a moon, you can fit a sine curve to the data and determine the radius of the orbit (the amplitude of the sine curve) and the peri ...
... Therefore, the perpendicular distance of the moon should be a sinusoidal curve if you plot it versus time (see Figure 2). By taking enough measurements of the position of a moon, you can fit a sine curve to the data and determine the radius of the orbit (the amplitude of the sine curve) and the peri ...
A Brief History of Planetary Science
... When Triton was first captured it was probably in a highly eccentric orbit which resulted in tidal heating ...
... When Triton was first captured it was probably in a highly eccentric orbit which resulted in tidal heating ...
The Moons of Jupiter
... Ejected particles that remain neutral co-orbit with Io Electrons easily stripped from the ejected sulfur, chlorine, and oxygen atoms by the intense magnetic field of Jupiter Resulting plasma remains in a torus around Jupiter and rotates with the magnetic field of Jupiter Rapidly rotating magnetic fi ...
... Ejected particles that remain neutral co-orbit with Io Electrons easily stripped from the ejected sulfur, chlorine, and oxygen atoms by the intense magnetic field of Jupiter Resulting plasma remains in a torus around Jupiter and rotates with the magnetic field of Jupiter Rapidly rotating magnetic fi ...
Astronomy for Kids - Jupiter
... in size and mass. Jupiter's diameter of over 85,000 miles is almost twelve times that of Earth and its mass is well over twice as much as all the rest of the planets put together. These facts make it appropriate that the planet is named after the king of all the other gods in ancient Roman mythology ...
... in size and mass. Jupiter's diameter of over 85,000 miles is almost twelve times that of Earth and its mass is well over twice as much as all the rest of the planets put together. These facts make it appropriate that the planet is named after the king of all the other gods in ancient Roman mythology ...
CI513 Instruction and Technology Lesson Planning Guide
... d. We can see comets because it does not encounter enough friction in space to cause it to heat up and burn. When the ice turns to vapor (from the Sun melting it), particles of dust trapped in the ice break free. Radiation streaming out from the Sun pushes this material away from the comet in a long ...
... d. We can see comets because it does not encounter enough friction in space to cause it to heat up and burn. When the ice turns to vapor (from the Sun melting it), particles of dust trapped in the ice break free. Radiation streaming out from the Sun pushes this material away from the comet in a long ...
Jupiter and Saturn
... Jupiter and Saturn? 3. What is going on in Jupiter’s Great Red Spot? 4. What is the nature of the multicolored clouds of Jupiter and Saturn? 5. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin? 6. How do astronomers know about the deep interiors of Jupiter a ...
... Jupiter and Saturn? 3. What is going on in Jupiter’s Great Red Spot? 4. What is the nature of the multicolored clouds of Jupiter and Saturn? 5. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin? 6. How do astronomers know about the deep interiors of Jupiter a ...
UP8.LP2.OtherCelestialBodies
... Titan is the second largest moon in the entire solar system – it orbits Saturn. Composed primarily of ice and rocky material. The only moon known to have a dense atmosphere. ...
... Titan is the second largest moon in the entire solar system – it orbits Saturn. Composed primarily of ice and rocky material. The only moon known to have a dense atmosphere. ...
This Month`s Celestial Events - Fort Worth Astronomical Society
... Shoemaker by Levy: The Man Who Made an Impact by David H. Levy Eugene “Gene” Shoemaker was a geologist who helped pioneer the field of planetary science. He helped train the Apollo astronauts in lunar geology during the 1960s. He also was a major part of the investigating science teams for lunar and ...
... Shoemaker by Levy: The Man Who Made an Impact by David H. Levy Eugene “Gene” Shoemaker was a geologist who helped pioneer the field of planetary science. He helped train the Apollo astronauts in lunar geology during the 1960s. He also was a major part of the investigating science teams for lunar and ...
Kristen Turiano
... The Oort cloud is a nearly spherical collection of icy bodies about 1,000 times farther away from the sun than Pluto's orbit Gravitational interactions with passing stars can cause icy bodies in the Oort cloud to enter the inner solar system and become active comets. Comets lose ice and dust each ti ...
... The Oort cloud is a nearly spherical collection of icy bodies about 1,000 times farther away from the sun than Pluto's orbit Gravitational interactions with passing stars can cause icy bodies in the Oort cloud to enter the inner solar system and become active comets. Comets lose ice and dust each ti ...
Handout
... cause of tides and their variations the precession of the earth’s axis the perturbation of the motion of the moon by gravity of the sun ...
... cause of tides and their variations the precession of the earth’s axis the perturbation of the motion of the moon by gravity of the sun ...
Gravity
... What is the weight of a 70 kg astronaut in a satellite with an orbital radius of 1.3 x 107 m? Weight = GMm/r2 Using: G = 6.67 x 10-11 N-m2/kg2 and M = 5.98 x 1024 kg Weight = 165 N What is the astronaut’s apparent weight? The astronaut is in uniform circular motion about Earth. The net force on the ...
... What is the weight of a 70 kg astronaut in a satellite with an orbital radius of 1.3 x 107 m? Weight = GMm/r2 Using: G = 6.67 x 10-11 N-m2/kg2 and M = 5.98 x 1024 kg Weight = 165 N What is the astronaut’s apparent weight? The astronaut is in uniform circular motion about Earth. The net force on the ...
universalgravitation
... What is the weight of a 70 kg astronaut in a satellite with an orbital radius of 1.3 x 107 m? Weight = GMm/r2 Using: G = 6.67 x 10-11 N-m2/kg2 and M = 5.98 x 1024 kg Weight = 165 N What is the astronaut’s apparent weight? The astronaut is in uniform circular motion about Earth. The net force on the ...
... What is the weight of a 70 kg astronaut in a satellite with an orbital radius of 1.3 x 107 m? Weight = GMm/r2 Using: G = 6.67 x 10-11 N-m2/kg2 and M = 5.98 x 1024 kg Weight = 165 N What is the astronaut’s apparent weight? The astronaut is in uniform circular motion about Earth. The net force on the ...
Planets - people.vcu.edu
... same rate as the planet Mars) e) its surface temperature considering its location and placement ...
... same rate as the planet Mars) e) its surface temperature considering its location and placement ...
Jupiter and Saturn: Lords of the Planets Chapter Fourteen
... 2. Why are there important differences between the atmospheres of Jupiter and Saturn? 3. What is going on in Jupiter’s Great Red Spot? 4. What is the nature of the multicolored clouds of Jupiter and Saturn? 5. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin ...
... 2. Why are there important differences between the atmospheres of Jupiter and Saturn? 3. What is going on in Jupiter’s Great Red Spot? 4. What is the nature of the multicolored clouds of Jupiter and Saturn? 5. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin ...
Powerpoint Presentation (large file)
... 2. Why are there important differences between the atmospheres of Jupiter and Saturn? 3. What is going on in Jupiter’s Great Red Spot? 4. What is the nature of the multicolored clouds of Jupiter and Saturn? 5. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin ...
... 2. Why are there important differences between the atmospheres of Jupiter and Saturn? 3. What is going on in Jupiter’s Great Red Spot? 4. What is the nature of the multicolored clouds of Jupiter and Saturn? 5. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin ...
Mars By Sharon Fabian
... are lucky enough to get a look through a more powerful telescope, say 100x to 200x, you will get a really magnificent view. The three rings that were first discovered around Saturn, rings A, B, and C, can be seen at this magnification. It is even possible to see Saturn's own shadow falling across it ...
... are lucky enough to get a look through a more powerful telescope, say 100x to 200x, you will get a really magnificent view. The three rings that were first discovered around Saturn, rings A, B, and C, can be seen at this magnification. It is even possible to see Saturn's own shadow falling across it ...
Constructing the Solar System: A Smashing Success!
... planet building and are still in orbit around the Sun today. Most asteroids are found in orbits between Mars and Jupiter (although some are on Earth-crossing orbits, and some follow similar orbits to Jupiter—the Trojans). Asteroids are smaller than planets, and typically range from meters up to a fe ...
... planet building and are still in orbit around the Sun today. Most asteroids are found in orbits between Mars and Jupiter (although some are on Earth-crossing orbits, and some follow similar orbits to Jupiter—the Trojans). Asteroids are smaller than planets, and typically range from meters up to a fe ...
AST1001.ch8
... • TIMING: The planet that forms earliest captures the most hydrogen and helium gas. Capture ceases after the first solar wind blew the leftover gas away. • LOCATION: The planet that forms in a denser part of the nebula forms its core first. ...
... • TIMING: The planet that forms earliest captures the most hydrogen and helium gas. Capture ceases after the first solar wind blew the leftover gas away. • LOCATION: The planet that forms in a denser part of the nebula forms its core first. ...
Questions about Comets: Created by Laura Vican, 2014 Q: What are
... material went into the forming Sun. Some of the rocks and gas accreted (stuck together) to form planets. The leftover material is what makes up comets and asteroids. This process of planet formation happened 4.6 billion years ago! Q: How fast do comets go? A: The average comet speeds through the sol ...
... material went into the forming Sun. Some of the rocks and gas accreted (stuck together) to form planets. The leftover material is what makes up comets and asteroids. This process of planet formation happened 4.6 billion years ago! Q: How fast do comets go? A: The average comet speeds through the sol ...
Dynamics of Centaurs
... • ~ One-third have a > 30 AU • Dynamical lifetimes 1-100 Myr population should be 1/2000 of scattered disk (Jupiter-Saturn region) to 1/20 of scattered disk (q = 25-30 AU) • Size distribution of Centaurs may be shallower than that of KBOs • Observed orbital distribution of Centaurs consistent with ...
... • ~ One-third have a > 30 AU • Dynamical lifetimes 1-100 Myr population should be 1/2000 of scattered disk (Jupiter-Saturn region) to 1/20 of scattered disk (q = 25-30 AU) • Size distribution of Centaurs may be shallower than that of KBOs • Observed orbital distribution of Centaurs consistent with ...
THE COMPLETE COSMOS Chapter 10: Realm of the Comets
... in the Solar System where a moon is massive enough - compared to its planet - to swing its parent body around a point outside the planet. Pluto itself is tiny - one twenty-fifth the size of Mercury. Even when combined with its moon Charon, their joint mass is so small that they could not perturb the ...
... in the Solar System where a moon is massive enough - compared to its planet - to swing its parent body around a point outside the planet. Pluto itself is tiny - one twenty-fifth the size of Mercury. Even when combined with its moon Charon, their joint mass is so small that they could not perturb the ...
Comet Shoemaker–Levy 9
![](https://commons.wikimedia.org/wiki/Special:FilePath/Shoemaker-Levy_9_on_1994-05-17.png?width=300)
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.