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YJC2013 H2 Phy Topic 7 Gravitational field
YJC2013 H2 Phy Topic 7 Gravitational field

... acting towards the centre of the Earth. Any circular orbit must have its centre at the centre of Earth. Therefore, if the satellite were to be in orbit other than that in the equatorial plane (as sketched), it will sometimes be over the northern hemisphere and sometimes over the southern hemisphere. ...
Space Rocks! - California Academy of Sciences
Space Rocks! - California Academy of Sciences

... The moon has a lot more visible impact craters because it doesn't have an atmosphere to burn up smaller incoming space rocks. The moon also does not have liquid water or an active crust (with volcanoes and other forces) to change the surface and remove evidence of past impacts. The Moon once had lar ...
Volcanism in our Solar System
Volcanism in our Solar System

... volcanically active, in the past, displays the most recent large amount of activity, and we know this because of the cratering present everywhere else on the planets surface. This evidence shows how the volcanoes on the Tharsis bulge had been resurfacing the region and erasing the traces of past im ...
Orbits Explorer
Orbits Explorer

... orbiting debris) in the ring, lifting this material into a more elliptical (oblong) orbit, vacating a zone. This process, resulting from a condition called RESONANCE, can occur only when the ORBITAL PERIOD (time to circle the planet once) of the larger moon and the smaller moon (or space debris) are ...
The sun, yellow dwarf star at the heart of the solar system
The sun, yellow dwarf star at the heart of the solar system

... magnetic field is called the heliosphere. The sun's magnetic field is carried out through the solar system by a stream of electrically charged gas. Known as the solar wind, this stream blows outward from the sun in all directions. Since the sun rotates, the magnetic field spins out into a large rotatin ...
Chapter 7
Chapter 7

... 4. In 1990, David Robilliard rode a bicycle on the back wheel for more than 5 h. If the wheel‘s initial angular speed was 8.0 rad/s and Robilliard tripled this speed in 25 s, what was the average angular acceleration? 5. Earth takes about 365 days to orbit once around the sun. Mercury, the innermos ...
DEEP IMPACT and ROSETTA
DEEP IMPACT and ROSETTA

... - Oort Cloud - Kuiper Belt (+Centaurs) with “graveyards” for - Jupiter family comets - dormant comets - main belt comets ? ...
Solar System History - Mr. Hill`s Science Website
Solar System History - Mr. Hill`s Science Website

... *Plutoid – a dwarf planet outside the orbit of Neptune. **Closest – closest approach to Sun; Farthest – farthest distance from Sun. ***Your weight times the number in the column. ...
Earth_Universe02
Earth_Universe02

... • Produces a glowing head called the coma • Some may develop a tail that points away from Sun due to • Radiation pressure and the • Solar wind ...
English - Tinybop
English - Tinybop

... 36 years for the NASA spacecraft Voyager to reach the edge of our solar system. Our solar system is just one of billions in the Milky Way galaxy. There is so much to explore, discover, and learn about what is out there! Astronomers, scientists who study space and all of the stars, planets, asteroids ...
YJC2013Yisun JC H2 Physics - Gravitational field Tutorial
YJC2013Yisun JC H2 Physics - Gravitational field Tutorial

... acting towards the centre of the Earth. Any circular orbit must have its centre at the centre of Earth. Therefore, if the satellite were to be in orbit other than that in the equatorial plane (as sketched), it will sometimes be over the northern hemisphere and sometimes over the southern hemisphere. ...
Conceptual Physics
Conceptual Physics

... The orbits of satellites about a central massive body can be described as either circular or elliptical. As mentioned earlier in the chapter, a satellite orbiting about the earth in circular motion is moving with a constant speed and remains at the same height above the surface of the earth. It acco ...
Huge Quantum Gravity Effects in the Solar System
Huge Quantum Gravity Effects in the Solar System

... seem to suggest that quantum effects are very small for the motion of planets in the Solar System. Nevertheless, there are other effects that can make quantum effects become enormous. In particular, classical chaos in the Solar System [1, 2, 3, 4, 5, 6, 7, 8, 9] can exponentially amplify quantum un ...
NATS 1311 From the Cosmos to Earth
NATS 1311 From the Cosmos to Earth

... visible light. Nonetheless, geological features stand out well. In (b), the data have been converted to a threedimensional perspective view; heights are magnified by a factor of more than 20, so the volcano is not actually as steep-sided as it appears. ...
Classroom activity
Classroom activity

... If the students are old enough and there is time, have them calculate the scaled distances from the Sun to each planet. You could also have them calculate the diameters of the Sun and planets on this scale. (They will be very small! Only the Sun would be wider than 1 cm in diameter. Jupiter, the la ...
Study Guide for Quiz #2
Study Guide for Quiz #2

... Describe diurnal and annual motion. How do the two compare? What is the relationship between how far the sky moves in an hour compared to a month? How would you describe the location of an object in the sky with respect to the zenith, horizon and cardinal points? What causes the Earth’s seasons? Wha ...
Jack - WhatsOutThere
Jack - WhatsOutThere

... The Sun is a second generation star, some of its material came from other stars. The Sun is approx 4.6 billion years old and has used up about half of the hydrogen in its core. It has enough fuel to go on for another 5 billion years. Scientists are not sure what will happen then. Some think that whe ...
The Solar System Powerpoint
The Solar System Powerpoint

... might think the minimum size requirement is arbitrary, but the size cutoff is actually based on other properties of the object and its history in the Solar System. Both planets and dwarf planets orbit the Sun, not other planets (in which case we call them moons). Both must be large enough that their ...
The Solar System - Thomas County Schools
The Solar System - Thomas County Schools

... around the Sun and controls the rest of the motion of the solar system. • The mass of an object and the distance between objects determine the force of gravity. Inertia and gravity work together. • The gravitational attractions of the planets, either individually or as a group are small because of t ...
Lecture18
Lecture18

... Because the gravitational force decreases with (distance)2, the attractive force experienced by one object (e.g., the Earth) due to the gravitational field of a second object (e.g., the Moon) varies with position (closest parts attracted most strongly). Tidal forces are difference forces. ...
Days and Years (Sessions I and II) Days and
Days and Years (Sessions I and II) Days and

... a street corner, they must continue to stay in straight lines as they make the turn. Ask, Which member of the line must move faster to keep the line even and straight, the innermost musician who is closest to the corner or outermost musician? (the outermost musician) How is this similar to the Solar ...
Solar System - Bellevue ISD
Solar System - Bellevue ISD

... might think the minimum size requirement is arbitrary, but the size cutoff is actually based on other properties of the object and its history in the Solar System. Both planets and dwarf planets orbit the Sun, not other planets (in which case we call them moons). Both must be large enough that their ...
Script Planets of our Solar System
Script Planets of our Solar System

... Mars is nicknamed “The Red Planet” because of the reddish appearance of its surface. The reddish appearance is caused by the metals in the rocks and soil. Over time, these metals have begun to rust, which now makes the planet look red. There are some features on Mars that can be also found on Earth. ...
Light: The Cosmic Messenger
Light: The Cosmic Messenger

... and then recycled through interstellar space. So you are made of the dust of exploded stars that lived and died before our solar system was formed. You are star stuff! ...
Newton`s Universal Law of Gravitation
Newton`s Universal Law of Gravitation

... back on Earth. On a somewhat negative note, spaceight is known to aect the human immune system, possibly making the crew members more vulnerable to infectious diseases. Experiments own in space also have shown that some bacteria grow faster in microgravity than they do on Earth. However, on a pos ...
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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.
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