The Three-Body Problem: Finding Chaos in the Cosmos
... (n2+3n+2)/2 classical integrals of motion: n from the total momentum, n from the position of the center of mass, and n(n-1)/2 from the total angular momentum, and finally, 1 from the energy. Because 2nN-1 integrals of motion were necessary to integrate the N-body problem, there are in general not ...
... (n2+3n+2)/2 classical integrals of motion: n from the total momentum, n from the position of the center of mass, and n(n-1)/2 from the total angular momentum, and finally, 1 from the energy. Because 2nN-1 integrals of motion were necessary to integrate the N-body problem, there are in general not ...
Class 32
... bubble of plasma contained by a magnetic field generated in the interior of the planet. Jupiter’s magnetic field is 20,000 times stronger than the Earth’s and extends some 3 million km towards the Sun. ...
... bubble of plasma contained by a magnetic field generated in the interior of the planet. Jupiter’s magnetic field is 20,000 times stronger than the Earth’s and extends some 3 million km towards the Sun. ...
asteroids - WordPress.com
... In astronomy, a Trojan is a minor planet or natural satellite (moon) that shares an orbit with a planet or larger moon ...
... In astronomy, a Trojan is a minor planet or natural satellite (moon) that shares an orbit with a planet or larger moon ...
Science 8
... ______________________________________________________________________________________ ...
... ______________________________________________________________________________________ ...
Astronomy 1400 – 001: Solar System Astronomy
... a) Because the infrared sees through clouds on Io b) Because they are hot, they appear brighter in the infrared than the rest of Io ...
... a) Because the infrared sees through clouds on Io b) Because they are hot, they appear brighter in the infrared than the rest of Io ...
Jupiter
... describing how he had discovered Jupiter’s Moons some days before Galileo did • The names by which these satellites are known today (Io, Europa, Ganymede and Callisto) are those given them by Marius. • But untile the middle of the 20th century, these satellited were known as "Jupiter I," "Jupiter II ...
... describing how he had discovered Jupiter’s Moons some days before Galileo did • The names by which these satellites are known today (Io, Europa, Ganymede and Callisto) are those given them by Marius. • But untile the middle of the 20th century, these satellited were known as "Jupiter I," "Jupiter II ...
Distance from Sun - Barnhill-Memorial
... the size of a grain of sand to the size of a house. - Because Saturn is made of only gas and liquid, it is less dense than water. This means, if you had an ocean big enough to set Saturn in, it would float. ...
... the size of a grain of sand to the size of a house. - Because Saturn is made of only gas and liquid, it is less dense than water. This means, if you had an ocean big enough to set Saturn in, it would float. ...
Section 23.3 The Outer Planets
... Jupiter has a mass that is 2 1/2 times greater than the mass of all the other planets and moons combined. Structure of Jupiter Jupiter’s hydrogen-helium atmosphere also contains small amounts of methane, ammonia, water, and sulfur compounds. Jupiter and the Great Red Spot ...
... Jupiter has a mass that is 2 1/2 times greater than the mass of all the other planets and moons combined. Structure of Jupiter Jupiter’s hydrogen-helium atmosphere also contains small amounts of methane, ammonia, water, and sulfur compounds. Jupiter and the Great Red Spot ...
pptx format - Hildas and Trojans
... telescope, as opposed to photography or CCD imaging) than any other astronomer (And I assume he will hold this distinction forever as no one discovers asteroids visually now!) Hilda was named for daughter of another Austrian astronomer ...
... telescope, as opposed to photography or CCD imaging) than any other astronomer (And I assume he will hold this distinction forever as no one discovers asteroids visually now!) Hilda was named for daughter of another Austrian astronomer ...
(He) particles understand where we are traveling in space
... one system to another can help us understand more about the strength of each auroral source. Investigating scientific mysteries through an interdisciplinary lens helps us see science from a whole systems approach, which in turn gives us important information about our own Earth-based systems. On bot ...
... one system to another can help us understand more about the strength of each auroral source. Investigating scientific mysteries through an interdisciplinary lens helps us see science from a whole systems approach, which in turn gives us important information about our own Earth-based systems. On bot ...
Chapter 19: Robots
... • An array of robot probes, which have visited, or are due to visit the other planets of the Solar System. • Launch, on a Delta rocket, of Mars Surveyor Orbiter - shedding its nose cone and propulsion units, unfurling its solar array. • Slipping into an elliptical orbit, the spacecraft has to achiev ...
... • An array of robot probes, which have visited, or are due to visit the other planets of the Solar System. • Launch, on a Delta rocket, of Mars Surveyor Orbiter - shedding its nose cone and propulsion units, unfurling its solar array. • Slipping into an elliptical orbit, the spacecraft has to achiev ...
The Solar System
... than it receives from the sun. It’s HOT under that cold atmosphere • Why? Heat of formation takes a LONG time to dissipate, but mainly its because it is still slowly collapsing, converting gravitational potential energy into heat • You can see the hotter layers in infrared pictures… ...
... than it receives from the sun. It’s HOT under that cold atmosphere • Why? Heat of formation takes a LONG time to dissipate, but mainly its because it is still slowly collapsing, converting gravitational potential energy into heat • You can see the hotter layers in infrared pictures… ...
Astronomy
... C) Chemical reactions bind the atmosphere into the rocks on Mars, changing the pressure D) The amount of gas doesn’t change, but because the temperature does, the pressure does as well E) Mars’ rotation is so much faster than Earth’s, which causes it to have much more dramatic storms 20. The outer p ...
... C) Chemical reactions bind the atmosphere into the rocks on Mars, changing the pressure D) The amount of gas doesn’t change, but because the temperature does, the pressure does as well E) Mars’ rotation is so much faster than Earth’s, which causes it to have much more dramatic storms 20. The outer p ...
Outer Planets and Moons Notes
... Saturn has _____________ moons, and the largest is _________________. What characteristics of Titan are of particular interest to astronomers? Why? ...
... Saturn has _____________ moons, and the largest is _________________. What characteristics of Titan are of particular interest to astronomers? Why? ...
File
... The equatorial belts are bands of clouds moving with velocities up to 400 miles/hr. Wind direction alternates from one band to another. The light colored zones are regions of upward moving convective currents. The darker belts are made of downward sinking material. The two are therefore always fo ...
... The equatorial belts are bands of clouds moving with velocities up to 400 miles/hr. Wind direction alternates from one band to another. The light colored zones are regions of upward moving convective currents. The darker belts are made of downward sinking material. The two are therefore always fo ...
JUPITER AND URANUS
... rings and Uranus is known for its 11 rings. Both of their cores are mostly rocky. Also, they are both outer planets making ...
... rings and Uranus is known for its 11 rings. Both of their cores are mostly rocky. Also, they are both outer planets making ...
Jupiter=Zeus=Indra
... • Lava is enriched in magnesium and iron • Infrared photo of Jupiter & Io shows red spot in white & lava below volcanic plume ...
... • Lava is enriched in magnesium and iron • Infrared photo of Jupiter & Io shows red spot in white & lava below volcanic plume ...
Jupiter Reading Comprehension Worksheet
... the largest planet in our solar system and the fifth planet from the Sun. It is so large that all of the other planets in the solar system could fit inside of it. Jupiter has the most natural satellites or moons of any planet. The count is currently at 63, although not all of them have been named. I ...
... the largest planet in our solar system and the fifth planet from the Sun. It is so large that all of the other planets in the solar system could fit inside of it. Jupiter has the most natural satellites or moons of any planet. The count is currently at 63, although not all of them have been named. I ...
File - Homeschooling Mommie
... the largest planet in our solar system and the fifth planet from the Sun. It is so large that all of the other planets in the solar system could fit inside of it. Jupiter has the most natural satellites or moons of any planet. The count is currently at 63, although not all of them have been named. I ...
... the largest planet in our solar system and the fifth planet from the Sun. It is so large that all of the other planets in the solar system could fit inside of it. Jupiter has the most natural satellites or moons of any planet. The count is currently at 63, although not all of them have been named. I ...
ppt
... a large fraction of comets and planetesimals heading for the inner solar system This helps reduce the probability of an impact event that could wipe out life on Earth However, Jupiter cannot be too massive as some comets must reach the primordial Earth to supply it with water ...
... a large fraction of comets and planetesimals heading for the inner solar system This helps reduce the probability of an impact event that could wipe out life on Earth However, Jupiter cannot be too massive as some comets must reach the primordial Earth to supply it with water ...
Meet the Giants
... Wild Weather on Neptune The Sun at Neptune is 900 times dimmer than at Earth. Since heat from the Sun drives weather, the winds on Neptune should be relatively mild. Instead, they whip around at more than 2,000 km per hour. The weather is correspondingly wild, with enormous dark storms that come an ...
... Wild Weather on Neptune The Sun at Neptune is 900 times dimmer than at Earth. Since heat from the Sun drives weather, the winds on Neptune should be relatively mild. Instead, they whip around at more than 2,000 km per hour. The weather is correspondingly wild, with enormous dark storms that come an ...
Mars Jupiter and Saturn ppt
... • two moons- Phobos and Deimos • Moon actually asteroids that got caught in ...
... • two moons- Phobos and Deimos • Moon actually asteroids that got caught in ...
File - Miss Burnett`s 6th grade Classroom
... gas surface unlike the rocky surface of the inner planets, like Earth. ...
... gas surface unlike the rocky surface of the inner planets, like Earth. ...
What do you think about the origin of most of Jupiter`s moons?
... • Neptune moved rapidly outward. Its elliptical orbit settled down to circular by exchanging angular momentum with the Kuiper objects. ...
... • Neptune moved rapidly outward. Its elliptical orbit settled down to circular by exchanging angular momentum with the Kuiper objects. ...
Juno (spacecraft)
Juno is a NASA New Frontiers mission to the planet Jupiter. Juno was launched from Cape Canaveral Air Force Station on 5 August 2011 and will arrive on 4 July 2016. The spacecraft is to be placed in a polar orbit to study Jupiter's composition, gravity field, magnetic field, and polar magnetosphere. Juno will also search for clues about how the planet formed, including whether it has a rocky core, the amount of water present within the deep atmosphere, how its mass is distributed, and its deep winds, which can reach speeds of 618 kilometers per hour (384 mph).The spacecraft's name comes from Greco-Roman mythology. The god Jupiter drew a veil of clouds around himself to hide his mischief, but his wife, the goddess Juno, was able to peer through the clouds and see Jupiter's true nature.