Kuiper Belt
... • Elongated orbits (far beyond Pluto) Space Debris Song – Orbital period of most hundreds of thousands of years – Some less than 200 years and encounter inner solar system ...
... • Elongated orbits (far beyond Pluto) Space Debris Song – Orbital period of most hundreds of thousands of years – Some less than 200 years and encounter inner solar system ...
Nine Planets and Counting - Adventure Science Center
... solar system objects and their features. It can be very interesting. 6. Have students investigate some of the many robotic spacecraft that have been launched to explore the planets and other objects in our Solar System. Mariner, Venera, Vikings 1 and 2, Voyagers 1 and 2, Mars Pathfinder and Sojourne ...
... solar system objects and their features. It can be very interesting. 6. Have students investigate some of the many robotic spacecraft that have been launched to explore the planets and other objects in our Solar System. Mariner, Venera, Vikings 1 and 2, Voyagers 1 and 2, Mars Pathfinder and Sojourne ...
Glossary from “The Wizard from Space”
... constellation. The most famous of these is the Big Dipper, which is made of stars borrowed from the Big Bear. Asteroid – An asteroid is a small piece of metal, or stone, that is believed to be all that is left of a planet that did not completely form. There are thousands of asteroids between Mars an ...
... constellation. The most famous of these is the Big Dipper, which is made of stars borrowed from the Big Bear. Asteroid – An asteroid is a small piece of metal, or stone, that is believed to be all that is left of a planet that did not completely form. There are thousands of asteroids between Mars an ...
File eschpt20 - My Teacher Pages
... Section 20-1 – Observing the Solar System • Geocentric System: Ptolemy developed the Geocentric Theory that the Earth is at the center of the revolving planets. • Heliocentric System: Later, during the 1500’s, Nicolaus Copernicus developed a new model, the Heliocentric System, which is the Earth an ...
... Section 20-1 – Observing the Solar System • Geocentric System: Ptolemy developed the Geocentric Theory that the Earth is at the center of the revolving planets. • Heliocentric System: Later, during the 1500’s, Nicolaus Copernicus developed a new model, the Heliocentric System, which is the Earth an ...
6th GradeSpace Systems NGSS
... 10. Students will graph the moon’s phases (tell them not to include the word “terminator” that is found in the suggested words to use). They may use classroom materials such as a compass for drawing the moons. (Page 6) 11. Writing activity: Students (with a partner) will come up with a description o ...
... 10. Students will graph the moon’s phases (tell them not to include the word “terminator” that is found in the suggested words to use). They may use classroom materials such as a compass for drawing the moons. (Page 6) 11. Writing activity: Students (with a partner) will come up with a description o ...
Newton and Kepler`s Third Law
... • If the moon is moving away, it must be gaining angular momentum: Angular momentum = mass x distance x speed • Angular momentum is conserved, so something must also be losing angular momentum. What? © 2014 Pearson Education, Inc. ...
... • If the moon is moving away, it must be gaining angular momentum: Angular momentum = mass x distance x speed • Angular momentum is conserved, so something must also be losing angular momentum. What? © 2014 Pearson Education, Inc. ...
Asteroids
... Why does our solar system have an Asteroid Belt? One theory that astronomers have is that 4.6 billion years ago, when our solar system was being formed, a tenth planet tried to form between Mars and Jupiter. However, Jupiter’s gravitational forces were too strong, so the material was unable to form ...
... Why does our solar system have an Asteroid Belt? One theory that astronomers have is that 4.6 billion years ago, when our solar system was being formed, a tenth planet tried to form between Mars and Jupiter. However, Jupiter’s gravitational forces were too strong, so the material was unable to form ...
Melbourne Solar System Trail.pub
... has about sixty moons. Titan, the largest, is the only moon in the Solar system with an atmosphere (Nitrogen). It also has lakes of liquid methane discovered by the Huygen’s probe which landed in 2005. < Jupiter 622 meters Uranus 1500 metres> ...
... has about sixty moons. Titan, the largest, is the only moon in the Solar system with an atmosphere (Nitrogen). It also has lakes of liquid methane discovered by the Huygen’s probe which landed in 2005. < Jupiter 622 meters Uranus 1500 metres> ...
Planetary Sciences
... Planetary Sciences 1. show up to class … and be present 2. participate in class 3. get/borrow the book Planetary Sciences by de Pater and Lissauer 4. find course website: www.astro.gsu.edu/~thenry/PLANETS 5. find Icarus online (or in the library) 6. choose 3 planetary topic(s) you are most intereste ...
... Planetary Sciences 1. show up to class … and be present 2. participate in class 3. get/borrow the book Planetary Sciences by de Pater and Lissauer 4. find course website: www.astro.gsu.edu/~thenry/PLANETS 5. find Icarus online (or in the library) 6. choose 3 planetary topic(s) you are most intereste ...
Orbits of the Planets
... Because of misleading diagrams often seen in books other astronomy reference materials, most people believe that the orbits of the planets are highly elliptical – almost cigar shaped. In fact, the orbits of the planets are very nearly circular. The problem with this misconception about planetary orb ...
... Because of misleading diagrams often seen in books other astronomy reference materials, most people believe that the orbits of the planets are highly elliptical – almost cigar shaped. In fact, the orbits of the planets are very nearly circular. The problem with this misconception about planetary orb ...
Chapter01b
... ♦ III – evolution of the atmosphere due to the presence of life and human activity. The early atmosphere of the Earth is very different from the atmosphere today! We learn about the formation and the evolution of the Earth’s atmosphere from the Earth’s geological records and by studying other planet ...
... ♦ III – evolution of the atmosphere due to the presence of life and human activity. The early atmosphere of the Earth is very different from the atmosphere today! We learn about the formation and the evolution of the Earth’s atmosphere from the Earth’s geological records and by studying other planet ...
File
... planet within the Solar System. One of the storm is called the Great Red Spot Jupiter is classified as a gas giant along with Saturn, Uranus and Neptune but it is the biggest of the gas giant and Jupiter have stronger winds and storms than Earth . Together, these four planets are sometimes called as ...
... planet within the Solar System. One of the storm is called the Great Red Spot Jupiter is classified as a gas giant along with Saturn, Uranus and Neptune but it is the biggest of the gas giant and Jupiter have stronger winds and storms than Earth . Together, these four planets are sometimes called as ...
Solar System Notes
... Uranus has 10 narrow rings and a number of dusty bands Neptune has 8 satellites Neptune also has a series of rings ...
... Uranus has 10 narrow rings and a number of dusty bands Neptune has 8 satellites Neptune also has a series of rings ...
The Reason for the Seasons
... explain the seasons! So far we only know why the hottest part of each planet is around the middle…the sunlight hits that part most directly. If that was all that happened, though, we WOULDN’T have different seasons…just the same boring weather all year long. In Texas, it’d be about 90 degrees every ...
... explain the seasons! So far we only know why the hottest part of each planet is around the middle…the sunlight hits that part most directly. If that was all that happened, though, we WOULDN’T have different seasons…just the same boring weather all year long. In Texas, it’d be about 90 degrees every ...
ASTRONOMY EXAM IS _____Weds, 2/5
... 5. A chunk of ice and dust whose orbit is usually a long narrow ellipse is a(n) _______________. 6. If a meteoroid hits Earth’s surface, it is called a(n) _______________ . 7. An object that revolves around the sun, but is too small to be considered a planet, is a(n) _______________ . 8. A chunk of ...
... 5. A chunk of ice and dust whose orbit is usually a long narrow ellipse is a(n) _______________. 6. If a meteoroid hits Earth’s surface, it is called a(n) _______________ . 7. An object that revolves around the sun, but is too small to be considered a planet, is a(n) _______________ . 8. A chunk of ...
Chapter 7
... •Extreme axis tilt, 97 degrees — nearly tipped on its “side” — makes extreme seasons during its 84-year orbit. • The satellites and ring system also tipped in their orbits around 97 degrees • The extreme tilt probably caused by a collision with a large body ...
... •Extreme axis tilt, 97 degrees — nearly tipped on its “side” — makes extreme seasons during its 84-year orbit. • The satellites and ring system also tipped in their orbits around 97 degrees • The extreme tilt probably caused by a collision with a large body ...
Unit 7: Astronomy
... intensely on different parts of the Earth during the year. The difference in heating of the Earth’s surface produces the planet’s seasons and weather patterns. • The gravitational pull from the moon, and the spinning of the earth, causes ocean water to bulge, producing the tides. ...
... intensely on different parts of the Earth during the year. The difference in heating of the Earth’s surface produces the planet’s seasons and weather patterns. • The gravitational pull from the moon, and the spinning of the earth, causes ocean water to bulge, producing the tides. ...
ssp1_6
... The orbital periods of Io, Europa and Ganymede are almost exactly in the ratio 1:2:4. This leads to resonant effects : The orbit of Io is perturbed by Europa and Callisto, because the moons regularly line up on one side of Jupiter. The gravitational pull of the outer moons is enough to produce a sm ...
... The orbital periods of Io, Europa and Ganymede are almost exactly in the ratio 1:2:4. This leads to resonant effects : The orbit of Io is perturbed by Europa and Callisto, because the moons regularly line up on one side of Jupiter. The gravitational pull of the outer moons is enough to produce a sm ...
POWERPOINT with Facts - Mrs. Brown`s Third Grade Class
... – The path an object takes as it moves around another object in space. ...
... – The path an object takes as it moves around another object in space. ...
Microgravity demonstration
... Depending on your diving skills you might even be able to do somersaults mid-air, just like an astronaut in space. The difference is that your fall will end with a splash when you hit the water, while an astronaut can savour the experience because they never reach ‘the bottom’. The astronaut will co ...
... Depending on your diving skills you might even be able to do somersaults mid-air, just like an astronaut in space. The difference is that your fall will end with a splash when you hit the water, while an astronaut can savour the experience because they never reach ‘the bottom’. The astronaut will co ...
What else is in our solar system, besides the sun, the planets, and
... colored orange. The four outer planets are blue. Neptune's few known Trojan asteroids are yellow, while Jupiter's are pink. The scattered objects between the Sun and the Kuiper belt are known as centaurs. The scale is in astronomical units. The pronounced gap at the bottom is due to obscuration by t ...
... colored orange. The four outer planets are blue. Neptune's few known Trojan asteroids are yellow, while Jupiter's are pink. The scattered objects between the Sun and the Kuiper belt are known as centaurs. The scale is in astronomical units. The pronounced gap at the bottom is due to obscuration by t ...
Mercury, Mars, Venus and the Earth : when worlds collide !
... Observatory, from the Institute of Earth Physics of Paris, and from the EGEE node of the Laboratory of the Linear Accelerator. Finally, it is the installation of the new JADE supercomputer at the National Computing Center CINES that allowed to find the 7 million hours of CPU time required to conclud ...
... Observatory, from the Institute of Earth Physics of Paris, and from the EGEE node of the Laboratory of the Linear Accelerator. Finally, it is the installation of the new JADE supercomputer at the National Computing Center CINES that allowed to find the 7 million hours of CPU time required to conclud ...
![Forces and the Universe Unit Review: Weight [N] = 4.44 x Weight](http://s1.studyres.com/store/data/004111559_1-4b4665791c2c3caffe7377372b89110f-300x300.png)
Forces and the Universe Unit Review: Weight [N] = 4.44 x Weight
... Explain why the Earth has seasons? The Earth has seasons because the it is tilted. When the northern hemisphere is tilted towards the sun it is summer in the northern hemisphere and winter in the southern hemisphere. When the northern hemisphere is tilted away from the sun it is winter in the northe ...
... Explain why the Earth has seasons? The Earth has seasons because the it is tilted. When the northern hemisphere is tilted towards the sun it is summer in the northern hemisphere and winter in the southern hemisphere. When the northern hemisphere is tilted away from the sun it is winter in the northe ...
Earth's rotation
Earth's rotation is the rotation of the planet Earth around its own axis. The Earth rotates from the west towards east. As viewed from North Star or polestar Polaris, the Earth turns counter-clockwise.The North Pole, also known as the Geographic North Pole or Terrestrial North Pole, is the point in the Northern Hemisphere where the Earth's axis of rotation meets its surface. This point is distinct from the Earth's North Magnetic Pole. The South Pole is the other point where the Earth's axis of rotation intersects its surface, in Antarctica.The Earth rotates once in about 24 hours with respect to the sun and once every 23 hours 56 minutes and 4 seconds with respect to the stars (see below). Earth's rotation is slowing slightly with time; thus, a day was shorter in the past. This is due to the tidal effects the Moon has on Earth's rotation. Atomic clocks show that a modern-day is longer by about 1.7 milliseconds than a century ago, slowly increasing the rate at which UTC is adjusted by leap seconds.