Motion of the Earth and Moon – Part 2
... o Moon o Sun o Planets T: “You are right, there are stars, the moon, the sun and planets in the sky. We are first going to talk about the moon and how the moon moves. While the earth rotates on its axis every day, the moon rotates on its axis and ORBITS the earth every 28 days. Look at the globe and ...
... o Moon o Sun o Planets T: “You are right, there are stars, the moon, the sun and planets in the sky. We are first going to talk about the moon and how the moon moves. While the earth rotates on its axis every day, the moon rotates on its axis and ORBITS the earth every 28 days. Look at the globe and ...
The Solar System - Solon City Schools
... planets. Aristotle stated that the earth was in the center of the solar system. Ptolemy stated that the earth was in the center of the universe. He thought that the planets moved in small circles as they moved around the sun. ...
... planets. Aristotle stated that the earth was in the center of the solar system. Ptolemy stated that the earth was in the center of the universe. He thought that the planets moved in small circles as they moved around the sun. ...
Powerpoint - Sandhills Astronomical Society
... “Small Solar System Bodies.” These currently include most of the solar system asteroids, most Trans-Neptunian Objects (TNOs), comets, and other small bodies. ...
... “Small Solar System Bodies.” These currently include most of the solar system asteroids, most Trans-Neptunian Objects (TNOs), comets, and other small bodies. ...
Section 1 Earth`s Moon
... pull on Earth decreases with distance from the moon. • As a result, the ocean on Earth’s near side is pulled toward the moon with the greatest force. • The solid Earth experiences a lesser force. • These differences cause Earth’s tidal bulges. Because Earth rotates, tides occur in a regular rhythm a ...
... pull on Earth decreases with distance from the moon. • As a result, the ocean on Earth’s near side is pulled toward the moon with the greatest force. • The solid Earth experiences a lesser force. • These differences cause Earth’s tidal bulges. Because Earth rotates, tides occur in a regular rhythm a ...
Page 190 7.3 Orbit and Motions of the Moon By watching the
... Unlike almost all other large moons, our Moon has an orbit with a large tilt with respect to its planet's equator. In discussing eclipses in chapter 1, we noted that the Moon's orbit is tilted by a little more than 5° with respect to the Earth's orbit around the Sun. As a result, its orbit is tilte ...
... Unlike almost all other large moons, our Moon has an orbit with a large tilt with respect to its planet's equator. In discussing eclipses in chapter 1, we noted that the Moon's orbit is tilted by a little more than 5° with respect to the Earth's orbit around the Sun. As a result, its orbit is tilte ...
Jupiter: The Giant Planet
... Jupiter is the fifth planet from the Sun and is the largest one in the solar system. If Jupiter were hollow, more than one thousand Earths could fit inside. It also contains more matter than all of the other planets combined. There is a ring system, but it is very faint and is totally invisible from ...
... Jupiter is the fifth planet from the Sun and is the largest one in the solar system. If Jupiter were hollow, more than one thousand Earths could fit inside. It also contains more matter than all of the other planets combined. There is a ring system, but it is very faint and is totally invisible from ...
Earth, Sun, and Moon
... it from incoming meteoroids, most of which burn up in our atmosphere. The Moon has no such protection from collisions. • Temperature: The lack of an atmosphere causes the Moon to have extreme temperatures. An atmosphere acts like a blanket around a planet. At night, it holds in This footprint some ...
... it from incoming meteoroids, most of which burn up in our atmosphere. The Moon has no such protection from collisions. • Temperature: The lack of an atmosphere causes the Moon to have extreme temperatures. An atmosphere acts like a blanket around a planet. At night, it holds in This footprint some ...
Our Solar System copy
... atmosphere is one of the coldest places in the solar system, with temperatures at its cloud tops approaching -218 degrees. Temperatures at the planet's centre are approximately 5,000 degrees. Neptune takes around 165 years to orbit the sun! The atmosphere of Neptune is made up of methane, this is wh ...
... atmosphere is one of the coldest places in the solar system, with temperatures at its cloud tops approaching -218 degrees. Temperatures at the planet's centre are approximately 5,000 degrees. Neptune takes around 165 years to orbit the sun! The atmosphere of Neptune is made up of methane, this is wh ...
Chapter 15 The Formation of Planetary Systems
... Kuiper-belt objects have been detected from Earth recently; a few are as large as, or larger than, Pluto, and their composition appears similar. About 1/3 of all Kuiper belt objects (including Pluto) have orbits that are in a 3:2 ...
... Kuiper-belt objects have been detected from Earth recently; a few are as large as, or larger than, Pluto, and their composition appears similar. About 1/3 of all Kuiper belt objects (including Pluto) have orbits that are in a 3:2 ...
Gravity - University of Colorado Boulder
... By 1650, the distance to the moon was well known: about 60 R e (60 earth radii). The moon’s period T was also well known: about 27 days. Newton could thus easily compute a(moon) = v(moon)^2 / R (using v = 2 Pi R/T) Put in the numbers, you’ll find a(moon) = 3E-3 m/s^2 = (1/3600)*g. Conclusions: the m ...
... By 1650, the distance to the moon was well known: about 60 R e (60 earth radii). The moon’s period T was also well known: about 27 days. Newton could thus easily compute a(moon) = v(moon)^2 / R (using v = 2 Pi R/T) Put in the numbers, you’ll find a(moon) = 3E-3 m/s^2 = (1/3600)*g. Conclusions: the m ...
Chapter 9 Planetary Geology
... History of Cratering • Most cratering happened in first billion years of solar system formation • A surface with many craters has not changed much in 3 billion years ...
... History of Cratering • Most cratering happened in first billion years of solar system formation • A surface with many craters has not changed much in 3 billion years ...
Astro Ch 19 planets
... Mercury vs. The Moon Take notes for each of the following categories. Be sure to include information on the Moon and Mercury for each one. ...
... Mercury vs. The Moon Take notes for each of the following categories. Be sure to include information on the Moon and Mercury for each one. ...
Earth - Fort Bend ISD
... There is NEVER a sunny day on Venus, the clouds are too thick! The clouds trap the heat near Venus’ surface –greenhouse effect The temperature is around 900 degrees F everyday! 20 spacecraft have visited Venus The surface is full of volcanoes with lava flow, craters, and strange domes not seen ...
... There is NEVER a sunny day on Venus, the clouds are too thick! The clouds trap the heat near Venus’ surface –greenhouse effect The temperature is around 900 degrees F everyday! 20 spacecraft have visited Venus The surface is full of volcanoes with lava flow, craters, and strange domes not seen ...
Newton`s 1st Law of Motion
... According to Aristotle, the Earth was too massive to be moved by an outside force. It was believed then that the planets and stars moved in perfect circles around the Earth. Copernicus interpreted astronomical observations in another way: Earth and the other planets moved around the sun. Copernicus ...
... According to Aristotle, the Earth was too massive to be moved by an outside force. It was believed then that the planets and stars moved in perfect circles around the Earth. Copernicus interpreted astronomical observations in another way: Earth and the other planets moved around the sun. Copernicus ...
Solar System - WordPress.com
... Distances and Diameters The first number is the number of miles. The second is the number of feet or inches in this exhibit. Distances from the center Sun – 0 – 0 Mercury – 36 million miles – 1.9’ Venus – 67 million miles – 3.5’ Earth – 93 million miles – 4.8’ Mars – 142 million miles – 7.4’ Ceres ...
... Distances and Diameters The first number is the number of miles. The second is the number of feet or inches in this exhibit. Distances from the center Sun – 0 – 0 Mercury – 36 million miles – 1.9’ Venus – 67 million miles – 3.5’ Earth – 93 million miles – 4.8’ Mars – 142 million miles – 7.4’ Ceres ...
by the earth
... forms into a sphere if you squeeze it with equal forces on all sides. • This effect is greatly reduced in celestial bodies of low mass, since the gravitational attraction is less, and these bodies tend not to be spherical. ...
... forms into a sphere if you squeeze it with equal forces on all sides. • This effect is greatly reduced in celestial bodies of low mass, since the gravitational attraction is less, and these bodies tend not to be spherical. ...
Solar System WebQuest Worksheet
... The Sun is the ______________________ of our solar system. The Sun is a ______________________. It is a ball of gas. The two gases that make up the Sun are _________________ and __________________. The temperature at the Sun’s core is _________________________ degrees Celsius. You could fit more tha ...
... The Sun is the ______________________ of our solar system. The Sun is a ______________________. It is a ball of gas. The two gases that make up the Sun are _________________ and __________________. The temperature at the Sun’s core is _________________________ degrees Celsius. You could fit more tha ...
Unit 3, Chapter 2 Quiz
... 21. The Sun accounts for approximately _______ of the mass in the Solar System. a) 99% b) 25% c) 50% d) 75% ...
... 21. The Sun accounts for approximately _______ of the mass in the Solar System. a) 99% b) 25% c) 50% d) 75% ...
File
... of Mars. The two planets shared an orbit for several million years until they collided (crash). Earth absorbed Theia, and the remaining debris eventually coagulated into Earth’s moon. The mass donated/given by Theia gave Earth the gravity Before, people believed that Earth is the center of the Solar ...
... of Mars. The two planets shared an orbit for several million years until they collided (crash). Earth absorbed Theia, and the remaining debris eventually coagulated into Earth’s moon. The mass donated/given by Theia gave Earth the gravity Before, people believed that Earth is the center of the Solar ...
How Big Is the Solar System
... large cloud of gas and dust called a nebula. Over many millions of years, the immense gravity of this large cloud caused the dust and gas to slowly fall inward towards its center. As matter in the cloud fell towards the center it began to spin. This spinning was caused by the basic laws of motion. O ...
... large cloud of gas and dust called a nebula. Over many millions of years, the immense gravity of this large cloud caused the dust and gas to slowly fall inward towards its center. As matter in the cloud fell towards the center it began to spin. This spinning was caused by the basic laws of motion. O ...
Structure of the Solar System
... 1.This gas giant has faint gray rings and 17 moons. Scientists think the rings might be made of graphite, the material used in pencils. ...
... 1.This gas giant has faint gray rings and 17 moons. Scientists think the rings might be made of graphite, the material used in pencils. ...
Planet Longitudes - ScholarWorks@UMass Amherst
... Stars are so far from Earth and so far apart that, even though they actually are moving, their arrangements in constellations do not appear to change from one night to the next. However, ancient astronomers noticed bright objects in the night sky that seemed to be "wandering stars". They appeared to ...
... Stars are so far from Earth and so far apart that, even though they actually are moving, their arrangements in constellations do not appear to change from one night to the next. However, ancient astronomers noticed bright objects in the night sky that seemed to be "wandering stars". They appeared to ...
Earth, Sun, and Moon - Uplift North Hills Prep
... it from incoming meteoroids, most of which burn up in our atmosphere. The Moon has no such protection from collisions. • Temperature: The lack of an atmosphere causes the Moon to have extreme temperatures. An atmosphere acts like a blanket around a planet. At night, it holds in some of the heat. On ...
... it from incoming meteoroids, most of which burn up in our atmosphere. The Moon has no such protection from collisions. • Temperature: The lack of an atmosphere causes the Moon to have extreme temperatures. An atmosphere acts like a blanket around a planet. At night, it holds in some of the heat. On ...
Formation of solar system HW
... No! Although our Solar System formed nearly 5 billion years ago, we can see stars forming elsewhere in the galaxy, such as in the Large Magellanic cloud 160,000 light years away. Although we can't know for sure, astronomers think that our early solar system looked very much like this. ...
... No! Although our Solar System formed nearly 5 billion years ago, we can see stars forming elsewhere in the galaxy, such as in the Large Magellanic cloud 160,000 light years away. Although we can't know for sure, astronomers think that our early solar system looked very much like this. ...
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.