The Moon
... If orbit period faster than spin period, tidal bulge would have to move around surface of Moon, creating friction, which slows the Moon’s spin down until tidal bulge no longer migrates around. ...
... If orbit period faster than spin period, tidal bulge would have to move around surface of Moon, creating friction, which slows the Moon’s spin down until tidal bulge no longer migrates around. ...
Part 2, E
... The Earth’s solid surface and the oceans get deformed by the gravity of the moon and the sun. Geologists __have__ (1) long wondered whether this can _cause / trigger__ (2) earthquakes, and finally they have an answer. __Besides__ (3) causing ocean tides, the sun and the moon also pull at __the___ (4 ...
... The Earth’s solid surface and the oceans get deformed by the gravity of the moon and the sun. Geologists __have__ (1) long wondered whether this can _cause / trigger__ (2) earthquakes, and finally they have an answer. __Besides__ (3) causing ocean tides, the sun and the moon also pull at __the___ (4 ...
Earth Science Survey of Student Knowledge – Form B Set 1: Moon
... • The part of the lit side of the moon that is visible from Earth depends on the relative positions of the sun, Earth and moon. • For example, the moon appears fully lit when the sun and moon are located on opposite sides of the Earth (see 4). This phase, called the full moon, is only visible from E ...
... • The part of the lit side of the moon that is visible from Earth depends on the relative positions of the sun, Earth and moon. • For example, the moon appears fully lit when the sun and moon are located on opposite sides of the Earth (see 4). This phase, called the full moon, is only visible from E ...
Word
... The part of the lit side of the moon that is visible from Earth depends on the relative positions of the sun, Earth and moon. For example, the moon appears fully lit when the sun and moon are located on opposite sides of the Earth (see 4). This phase, called the full moon, is only visible from E ...
... The part of the lit side of the moon that is visible from Earth depends on the relative positions of the sun, Earth and moon. For example, the moon appears fully lit when the sun and moon are located on opposite sides of the Earth (see 4). This phase, called the full moon, is only visible from E ...
Earth`s Tilt
... The angle remains constant but the direction of the axis changes Would not affect Earth’s Seasons but would affect what stars are seen at night ...
... The angle remains constant but the direction of the axis changes Would not affect Earth’s Seasons but would affect what stars are seen at night ...
Meteorite - Otterbein University
... Formation of the Solar System • Condenses from a rotating cloud of gas and dust – Conservation of angular momentum flattens it ...
... Formation of the Solar System • Condenses from a rotating cloud of gas and dust – Conservation of angular momentum flattens it ...
Seasons/Sun Misconception #3
... Seasons / Sun Misconception #3 = The tilt always leans toward the Sun. It takes 365 days for Earth to rotate one time. So when we are on the side toward the Sun, it is summer. When we are on the side away from the Sun, it is winter. There are two problems here. First, the tilt always points toward t ...
... Seasons / Sun Misconception #3 = The tilt always leans toward the Sun. It takes 365 days for Earth to rotate one time. So when we are on the side toward the Sun, it is summer. When we are on the side away from the Sun, it is winter. There are two problems here. First, the tilt always points toward t ...
The path of the Moon in the sky
... these observed phenomena? It took the human race tens of thousands of years to reach the right answer ...
... these observed phenomena? It took the human race tens of thousands of years to reach the right answer ...
A power point by Claudia And Izzy!!!
... The sun is a big star The sun is like a big ball of fire. The sun is so bright it could blind you. The colour of the sun is orange. The distance to the sun is 92,960,000 kilometres. • You can not get to the sun. • This is a picture of the sun ...
... The sun is a big star The sun is like a big ball of fire. The sun is so bright it could blind you. The colour of the sun is orange. The distance to the sun is 92,960,000 kilometres. • You can not get to the sun. • This is a picture of the sun ...
Earth - altaastronomy
... – Magnetosphere – High above our atmosphere. – Troposphere – is where convection occurs due to surface heating, this gives us wind. – Ozone layer is between the stratosphere and the mesosphere – this protects us from much ultraviolet radiation. ...
... – Magnetosphere – High above our atmosphere. – Troposphere – is where convection occurs due to surface heating, this gives us wind. – Ozone layer is between the stratosphere and the mesosphere – this protects us from much ultraviolet radiation. ...
Chapter 1 Notes for Earth Science
... -Earth revolves, or travels around, the sun. -It takes on year to revolve once around the sun. -The path Earth takes around the sun is its orbit. -Inner planets are Mercury, Venus, Earth, and Mars. -Outer planets are Jupiter, Saturn, Uranus, and Neptune. -Inner planets are smaller and made of rock. ...
... -Earth revolves, or travels around, the sun. -It takes on year to revolve once around the sun. -The path Earth takes around the sun is its orbit. -Inner planets are Mercury, Venus, Earth, and Mars. -Outer planets are Jupiter, Saturn, Uranus, and Neptune. -Inner planets are smaller and made of rock. ...
ppt
... Earth was spinning too fast and part of it was torn off to form the Moon. BUT, spin axes are not aligned, no water on the Moon. ...
... Earth was spinning too fast and part of it was torn off to form the Moon. BUT, spin axes are not aligned, no water on the Moon. ...
Earth Science - Atlanta Public Schools
... 23. In the blank space after each of the layers listed above state the composition and weather it is molten or solid. 24. How do temperature, density, and pressure change with depth? ...
... 23. In the blank space after each of the layers listed above state the composition and weather it is molten or solid. 24. How do temperature, density, and pressure change with depth? ...
Chapter 6 - USD Home Pages
... the point that Earth’s tidal stresses would tear it up, leaving a very nice ring system. 45. What IF? Earth were now in synchronous rotation with the Moon? That is, that the Earth rotated at the same rate as the Moon orbits it. What would be different about Earth and life on it? In the first place, ...
... the point that Earth’s tidal stresses would tear it up, leaving a very nice ring system. 45. What IF? Earth were now in synchronous rotation with the Moon? That is, that the Earth rotated at the same rate as the Moon orbits it. What would be different about Earth and life on it? In the first place, ...
Name 2 movements of the Earth:
... Why does Earth have season’s? • Because the Earth is tilted, its surface gets different amounts of sunlight at different times in the year. ...
... Why does Earth have season’s? • Because the Earth is tilted, its surface gets different amounts of sunlight at different times in the year. ...
TAKS Review - Greenslime
... • Neap Tides = lower high tides & higher low tides than average 8.7C ...
... • Neap Tides = lower high tides & higher low tides than average 8.7C ...
Revolution VS Rotation
... • Rotation - The Earth spinning on its own axis • Rotation speed- 24,855 miles/24hr or 1,038 miles/hr ...
... • Rotation - The Earth spinning on its own axis • Rotation speed- 24,855 miles/24hr or 1,038 miles/hr ...
FYS4160 Problem Sheet 1
... b) A tidal force pendulum consists of two equally massive points that are connected through a stiff, massless rod. The length of the rod is 2l. The pendulum oscillates with respect to the center of the rod which again is fixed in a constant distance from the center of the Earth. The oscillations tak ...
... b) A tidal force pendulum consists of two equally massive points that are connected through a stiff, massless rod. The length of the rod is 2l. The pendulum oscillates with respect to the center of the rod which again is fixed in a constant distance from the center of the Earth. The oscillations tak ...
Tidal acceleration
Tidal acceleration is an effect of the tidal forces between an orbiting natural satellite (e.g. the Moon), and the primary planet that it orbits (e.g. Earth). The acceleration causes a gradual recession of a satellite in a prograde orbit away from the primary, and a corresponding slowdown of the primary's rotation. The process eventually leads to tidal locking of the smaller first, and later the larger body. The Earth–Moon system is the best studied case.The similar process of tidal deceleration occurs for satellites that have an orbital period that is shorter than the primary's rotational period, or that orbit in a retrograde direction.The naming is somewhat confusing, because the speed of the satellite relative to the body it orbits is decreased as a result of tidal acceleration, and increased as a result of tidal deceleration.