b. 248 years
... 7. Does a waxing moon appear to be larger or smaller as each night goes by? a. Larger ...
... 7. Does a waxing moon appear to be larger or smaller as each night goes by? a. Larger ...
Jupiter`s Moons - cloudfront.net
... Jupiter has at least 61 moons. Most are very small. The first 4 moons of Jupiter were discovered by Galileo and are thus called the Galilean moons. They are large, about the size of the Earth’s Moon. These and four more smaller moons all orbit in the same direction as Jupiter spins. These 8 moons a ...
... Jupiter has at least 61 moons. Most are very small. The first 4 moons of Jupiter were discovered by Galileo and are thus called the Galilean moons. They are large, about the size of the Earth’s Moon. These and four more smaller moons all orbit in the same direction as Jupiter spins. These 8 moons a ...
Rings, Moons, etc
... Note: Meteor is only the name of the visible streak as the rock burns in atmosphere. ...
... Note: Meteor is only the name of the visible streak as the rock burns in atmosphere. ...
Comets and Asteroids
... irregularly shaped bodies composed of a mixture of non-volatile grains and frozen gases. They have highly elliptical orbits that bring them very close to the Sun and swing them deeply into space, often beyond the orbit of Pluto. As comets approach the Sun they develop enormous tails of luminous mate ...
... irregularly shaped bodies composed of a mixture of non-volatile grains and frozen gases. They have highly elliptical orbits that bring them very close to the Sun and swing them deeply into space, often beyond the orbit of Pluto. As comets approach the Sun they develop enormous tails of luminous mate ...
Comets - Cloudfront.net
... Comets that orbit with a period of less than 200 years are called short period comets. They originate from the Kuiper belt Each time a comet nears the Sun it loses mass. Gradually it evaporates leaving only dust and rock… a meteor shower ...
... Comets that orbit with a period of less than 200 years are called short period comets. They originate from the Kuiper belt Each time a comet nears the Sun it loses mass. Gradually it evaporates leaving only dust and rock… a meteor shower ...
PPT - University of Delaware
... – Students calculate distances and planet/moon sizes if the Earth were 1 cm, 1 inch or 1 foot in diameter. – Plot orbits on 40”x36” map of Wilmington. – Determine location of planets today and plot. – Compute and plot location of planets in one years time. ...
... – Students calculate distances and planet/moon sizes if the Earth were 1 cm, 1 inch or 1 foot in diameter. – Plot orbits on 40”x36” map of Wilmington. – Determine location of planets today and plot. – Compute and plot location of planets in one years time. ...
Outer Planets
... •Neptune’s magnetic field is tipped 47 degrees. •Its wind speeds up to 2200 kilometers per hour. •Neptune gives off 2.7 times more energy than it obtains from the sun. •Its temperature was once o measured at –214 C. ...
... •Neptune’s magnetic field is tipped 47 degrees. •Its wind speeds up to 2200 kilometers per hour. •Neptune gives off 2.7 times more energy than it obtains from the sun. •Its temperature was once o measured at –214 C. ...
the gas giants
... diameter is eleven times larger than Earth's. In fact, Jupiter is only ten times smaller than the sun. This giant planet makes up about 70 percent of all the planetary matter in our solar system. Jupiter's atmosphere is made of mostly helium and hydrogen. There are strong winds in its upper atmosphe ...
... diameter is eleven times larger than Earth's. In fact, Jupiter is only ten times smaller than the sun. This giant planet makes up about 70 percent of all the planetary matter in our solar system. Jupiter's atmosphere is made of mostly helium and hydrogen. There are strong winds in its upper atmosphe ...
Chapter 23: Touring Our Solar System
... a dwarf planet as a celestial body in direct orbit of the Sun[1] that is massive enough for its shape to be controlled by gravitation, but that unlike a planet has not cleared its orbital region of other ...
... a dwarf planet as a celestial body in direct orbit of the Sun[1] that is massive enough for its shape to be controlled by gravitation, but that unlike a planet has not cleared its orbital region of other ...
ppt
... • composed of 90% hydrogen and 10% helium, with small amounts of CH4, NH3, H2O vapor and other compounds • At great depths within Jupiter, the pressure is so great that the hydrogen atoms are broken up, freeing the electrons so that the resulting atoms consist of bare protons. This produces a state ...
... • composed of 90% hydrogen and 10% helium, with small amounts of CH4, NH3, H2O vapor and other compounds • At great depths within Jupiter, the pressure is so great that the hydrogen atoms are broken up, freeing the electrons so that the resulting atoms consist of bare protons. This produces a state ...
Section 23.3 The Outer Planets
... 12. Is the following sentence true or false? Uranus’s rings were discovered when Uranus passed in front of a distant star and blocked its view. 13. Uranus’s moon Miranda has a greater variety of than any solar system body yet examined. ...
... 12. Is the following sentence true or false? Uranus’s rings were discovered when Uranus passed in front of a distant star and blocked its view. 13. Uranus’s moon Miranda has a greater variety of than any solar system body yet examined. ...
Section 23.3 The Outer Planets
... 12. Is the following sentence true or false? Uranus’s rings were discovered when Uranus passed in front of a distant star and blocked its view. 13. Uranus’s moon Miranda has a greater variety of than any solar system body yet examined. ...
... 12. Is the following sentence true or false? Uranus’s rings were discovered when Uranus passed in front of a distant star and blocked its view. 13. Uranus’s moon Miranda has a greater variety of than any solar system body yet examined. ...
Asteroids, Comets, and Meteorites, Oh My! - Willoughby
... Coma – large halo of gas and dust that forms around the nucleus of a comet when it gets close to the sun. It actually loses mass as it gets close to the sun. ...
... Coma – large halo of gas and dust that forms around the nucleus of a comet when it gets close to the sun. It actually loses mass as it gets close to the sun. ...
Jupiter - barransclass
... Jupiter has a mass 318 times greater than the Earth’s and a diameter that is 11 times larger. The mass of Jupiter is 70% of the total mass of all the other planets in our Solar System Jupiter’s volume is large enough to contain 1,300 planets the size of Earth. Jupiter rotates faster than any planet ...
... Jupiter has a mass 318 times greater than the Earth’s and a diameter that is 11 times larger. The mass of Jupiter is 70% of the total mass of all the other planets in our Solar System Jupiter’s volume is large enough to contain 1,300 planets the size of Earth. Jupiter rotates faster than any planet ...
Week Two
... In the yellow and gray regions, a haze or cloud layer is reflecting sunlight away. Orange and red colors indicate very high clouds, like cirrus clouds on Earth. These ...
... In the yellow and gray regions, a haze or cloud layer is reflecting sunlight away. Orange and red colors indicate very high clouds, like cirrus clouds on Earth. These ...
Jupiter Versus the Earth: Composition & Structure
... Inside Earth The major regions in the Earth are the crust, mantle, outer core, and inner core: • The outer crust is relatively thin (~30 km thick in the continents and ~5 km thick in the oceans) • The mantle is ~3000 km thick (almost halfway to the center of the Earth) and is made of a dense rock c ...
... Inside Earth The major regions in the Earth are the crust, mantle, outer core, and inner core: • The outer crust is relatively thin (~30 km thick in the continents and ~5 km thick in the oceans) • The mantle is ~3000 km thick (almost halfway to the center of the Earth) and is made of a dense rock c ...
Homework, August 29, 2002 AST110-6
... and the planet today wasn’t spinning. How else would the jovian system be different? Think of as many effects as you can, and explain each in a sentence. 4. Chapter 8, Problem 23. Minor Ingredients Matter. Suppose the jovian planet atmospheres were composed only of hydrogen and helium, with no hydro ...
... and the planet today wasn’t spinning. How else would the jovian system be different? Think of as many effects as you can, and explain each in a sentence. 4. Chapter 8, Problem 23. Minor Ingredients Matter. Suppose the jovian planet atmospheres were composed only of hydrogen and helium, with no hydro ...
ppt
... • Has at least 30 known satellites. Its largest moon, Titan, is unique among moons for it has its own atmosphere. • Voyager 2 flyby in 1981 gave us close-up of rings and 1990 Hubble Telescope recorded enormous storms. ...
... • Has at least 30 known satellites. Its largest moon, Titan, is unique among moons for it has its own atmosphere. • Voyager 2 flyby in 1981 gave us close-up of rings and 1990 Hubble Telescope recorded enormous storms. ...
Moons Jupiter was known to have at least 16 moons at the time this
... There are four Galilean moons which are about the size of Earth’s moon. From closest to the planet to farthest they are: Io, Europa, Ganymede, and Callisto. ...
... There are four Galilean moons which are about the size of Earth’s moon. From closest to the planet to farthest they are: Io, Europa, Ganymede, and Callisto. ...
To Jupiter … and Beyond! - Five Star Publications, Inc.
... of Jupiter. Moving at more than 100,000 miles per hour, it was crushed, disintegrated and lost forever. But that little spacecraft taught us much about Jupiter. Never fear, your spaceship will not have the same fate. When you get to Jupiter, you will find it to be a massive planet. It is the largest ...
... of Jupiter. Moving at more than 100,000 miles per hour, it was crushed, disintegrated and lost forever. But that little spacecraft taught us much about Jupiter. Never fear, your spaceship will not have the same fate. When you get to Jupiter, you will find it to be a massive planet. It is the largest ...
Moons of the planets
... learned from studies of the Earth’s moon (the Moon). It is the key to understanding the solar system How much can we learn from the moons (or satellites) of the other planets? Of the three solar system objects most interesting from the viewpoint of exobiology (existence of life in outer space), two ...
... learned from studies of the Earth’s moon (the Moon). It is the key to understanding the solar system How much can we learn from the moons (or satellites) of the other planets? Of the three solar system objects most interesting from the viewpoint of exobiology (existence of life in outer space), two ...
Final exam
... Big, eccentric orbits : some get inside Earth's orbit (with aphelion at or outside Jupiter, some got out as far as 50,000 AU "Dirty snowballs" mostly ice and some rock ...
... Big, eccentric orbits : some get inside Earth's orbit (with aphelion at or outside Jupiter, some got out as far as 50,000 AU "Dirty snowballs" mostly ice and some rock ...
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.