Seasons
... Axis- imaginary line drawn from the north to the south pole. Rotation- the spinning of the earth on its axis. 1 rotation on its axis =24 hours ...
... Axis- imaginary line drawn from the north to the south pole. Rotation- the spinning of the earth on its axis. 1 rotation on its axis =24 hours ...
Exam 1 - UGA Physics
... 13. In Ptolemy's description of the solar system, the deferent is (b) a circular path (around Earth) along which the center of a planet's epicycle moves. 14. The early Copernican system for planetary motions is (c) Sun-centered, with planets moving in perfect circles around the Sun. 15. When Mercur ...
... 13. In Ptolemy's description of the solar system, the deferent is (b) a circular path (around Earth) along which the center of a planet's epicycle moves. 14. The early Copernican system for planetary motions is (c) Sun-centered, with planets moving in perfect circles around the Sun. 15. When Mercur ...
Rotation and Revolution
... Night and Day What causes night and day? The rotation of the Earth • The side of the Earth that is facing the sun has daylight, the side of the Earth away from the sun has night. • It takes 24 hours for the Earth to complete one rotation. • The Earth is tilted on it’s axis at a 23.5 degree angle. • ...
... Night and Day What causes night and day? The rotation of the Earth • The side of the Earth that is facing the sun has daylight, the side of the Earth away from the sun has night. • It takes 24 hours for the Earth to complete one rotation. • The Earth is tilted on it’s axis at a 23.5 degree angle. • ...
HELP
... 6 The Earth gets enough light from the Sun to keep the planet warm and for plants to photosynthesise. Can plants photosynthesise on Pluto? Give reasons for your answer. ...
... 6 The Earth gets enough light from the Sun to keep the planet warm and for plants to photosynthesise. Can plants photosynthesise on Pluto? Give reasons for your answer. ...
Sample Midterm
... A heliocentric model in which the Earth passed slower moving outer planets. A heliocentric model in which the planets executed looping orbits about the Sun. A geocentric model in which the planets passed the slower moving Earth. A geocentric model in which planets moved on epicycles about the Earth. ...
... A heliocentric model in which the Earth passed slower moving outer planets. A heliocentric model in which the planets executed looping orbits about the Sun. A geocentric model in which the planets passed the slower moving Earth. A geocentric model in which planets moved on epicycles about the Earth. ...
Section 26.3 - CPO Science
... 1. is in orbit around the Sun; 2. is nearly round in shape; and 3. has cleared its orbit of other objects. ...
... 1. is in orbit around the Sun; 2. is nearly round in shape; and 3. has cleared its orbit of other objects. ...
Rotation and Revolution
... Night and Day What causes night and day? The rotation of the Earth • The side of the Earth that is facing the sun has daylight, the side of the Earth away from the sun has night. • It takes 24 hours for the Earth to complete one rotation. • The Earth is tilted on it’s axis at a 23.5 degree angle. • ...
... Night and Day What causes night and day? The rotation of the Earth • The side of the Earth that is facing the sun has daylight, the side of the Earth away from the sun has night. • It takes 24 hours for the Earth to complete one rotation. • The Earth is tilted on it’s axis at a 23.5 degree angle. • ...
Rotation and Revolution
... Night and Day What causes night and day? The rotation of the Earth • The side of the Earth that is facing the sun has daylight, the side of the Earth away from the sun has night. • It takes 24 hours for the Earth to complete one rotation. • The Earth is tilted on it’s axis at a 23.5 degree angle. • ...
... Night and Day What causes night and day? The rotation of the Earth • The side of the Earth that is facing the sun has daylight, the side of the Earth away from the sun has night. • It takes 24 hours for the Earth to complete one rotation. • The Earth is tilted on it’s axis at a 23.5 degree angle. • ...
SNC 1D Astonomy
... • The time it takes for the Earth to make one revolution around the sun is 365.24 days. • It takes one day for Earth to make one rotation on its axis. • The first clocks were pillars and sticks in the ground and people used the shadows they made to tell the time. ...
... • The time it takes for the Earth to make one revolution around the sun is 365.24 days. • It takes one day for Earth to make one rotation on its axis. • The first clocks were pillars and sticks in the ground and people used the shadows they made to tell the time. ...
Overview - School District of La Crosse
... A. Astrophysics- the use of atomic physics to explain how various forms of radiation are created. 1. a stars radiation is the summation of all the radiation given off by the individual atoms of the star( quantum mechanics). a. the interaction of gravity holding the atoms together in the star and und ...
... A. Astrophysics- the use of atomic physics to explain how various forms of radiation are created. 1. a stars radiation is the summation of all the radiation given off by the individual atoms of the star( quantum mechanics). a. the interaction of gravity holding the atoms together in the star and und ...
Celestial Mechanics
... Celestial Mechanics The Heliocentric Model of Copernicus Sun at the center and planets (including Earth) orbiting along circles. inferior planets - planets closer to Sun than Earth - Mercury, Venus superior planets - planets farther from Sun than Earth - all other planets elongation - the angle seen ...
... Celestial Mechanics The Heliocentric Model of Copernicus Sun at the center and planets (including Earth) orbiting along circles. inferior planets - planets closer to Sun than Earth - Mercury, Venus superior planets - planets farther from Sun than Earth - all other planets elongation - the angle seen ...
Final Study Guide copy
... pole that are high enough above the horizon they don’t rise or set The Direction of Spin - Looking down on the north pole, the Earth spins counterclockwise. Looking straight on at the Earth, it spins in an Eastward direction. This means the celestial sphere overhead moves in a westward direction fro ...
... pole that are high enough above the horizon they don’t rise or set The Direction of Spin - Looking down on the north pole, the Earth spins counterclockwise. Looking straight on at the Earth, it spins in an Eastward direction. This means the celestial sphere overhead moves in a westward direction fro ...
Chapter 8 Powerpoint
... Understanding the Solar System • By definition, there are eight planets which consist of four terrestrial planets which are closer to the Sun and four gaseous giant planets which are further away. The terrestrial and gas planets are separated by a belt of rocky debris known as the ...
... Understanding the Solar System • By definition, there are eight planets which consist of four terrestrial planets which are closer to the Sun and four gaseous giant planets which are further away. The terrestrial and gas planets are separated by a belt of rocky debris known as the ...
The Solar System
... 6th in the Solar System Several rings Ball of gases and clouds Made of rock and ice 33 moons Rings size of a car ...
... 6th in the Solar System Several rings Ball of gases and clouds Made of rock and ice 33 moons Rings size of a car ...
The Doppler effect
... To track the actual motion of each celestial body we use the stars as the frame of reference instead of Earth. This is because we are looking for motions in the sky that are different from the big motion caused by Earth’s rotation. ...
... To track the actual motion of each celestial body we use the stars as the frame of reference instead of Earth. This is because we are looking for motions in the sky that are different from the big motion caused by Earth’s rotation. ...
University Mohamed Khider- Biskra Faculty of letters and
... b. Pluto c. Mars 3. What is the Latin name for the sun? a. Smilax b. Rubram c. Sol 4. The body that supplies heat and light to the small planet we call Earth is? a. Star b. Asteroid c. Moon 5. What objects gravitational pull is so great that nothing – not even light can escape from it? a. Black Hole ...
... b. Pluto c. Mars 3. What is the Latin name for the sun? a. Smilax b. Rubram c. Sol 4. The body that supplies heat and light to the small planet we call Earth is? a. Star b. Asteroid c. Moon 5. What objects gravitational pull is so great that nothing – not even light can escape from it? a. Black Hole ...
Solar System Review - answer key
... 5. Describe the shape of the orbit of the planets in our Solar System. The planets orbit around the sun in an elliptical, but nearly circular, pattern. 6. Why are dwarf planets and plutoids not considered planets? Planets must orbit around the sun, have enough gravity to pull themselves into a spher ...
... 5. Describe the shape of the orbit of the planets in our Solar System. The planets orbit around the sun in an elliptical, but nearly circular, pattern. 6. Why are dwarf planets and plutoids not considered planets? Planets must orbit around the sun, have enough gravity to pull themselves into a spher ...
Star
... -Some dwarf stars are as small as the Earth. -Our sun is a medium size star (1,390,000 km). -Some stars are 1,000 times larger than our sun. -Density affects mass…no relationship between size and mass. Example: a star can be smaller than our sun, but have a greater mass…meaning it is more dense! ...
... -Some dwarf stars are as small as the Earth. -Our sun is a medium size star (1,390,000 km). -Some stars are 1,000 times larger than our sun. -Density affects mass…no relationship between size and mass. Example: a star can be smaller than our sun, but have a greater mass…meaning it is more dense! ...
What makes day and night?
... moon takes twenty- four hours to spin around one time. The sun is four – five billion kms away. The sun is a ball of gas. By Josh Alesci- Bateman 1H The Earth and the sun make night and day. The Earth spins around to make night and day. Whilst one side is having morning the other side is having nigh ...
... moon takes twenty- four hours to spin around one time. The sun is four – five billion kms away. The sun is a ball of gas. By Josh Alesci- Bateman 1H The Earth and the sun make night and day. The Earth spins around to make night and day. Whilst one side is having morning the other side is having nigh ...
Concise pioneers of astronomy
... most celebrated as the first to propose a sun-centered universe. He is also famed for his pioneering attempt to determine the sizes and distances of the sun and moon. According to his contemporary, Archimedes, Aristarchus was the first to propose not only a heliocentric universe, but also one larger ...
... most celebrated as the first to propose a sun-centered universe. He is also famed for his pioneering attempt to determine the sizes and distances of the sun and moon. According to his contemporary, Archimedes, Aristarchus was the first to propose not only a heliocentric universe, but also one larger ...
Our Space Journey
... sun as well. Moon orbit takes 27 1/2 days but ... Because earth keeps on moving it takes two extra days, 29 1/2 to come back in to the same place. It takes the earth one year / 365 days 1/4 days to completely orbit the sun. The parts of the sun rotate at different speeds . The sun is star made up of ...
... sun as well. Moon orbit takes 27 1/2 days but ... Because earth keeps on moving it takes two extra days, 29 1/2 to come back in to the same place. It takes the earth one year / 365 days 1/4 days to completely orbit the sun. The parts of the sun rotate at different speeds . The sun is star made up of ...
Movement of the Planets Shape of the Earth
... • What observations do you have? • Are you able to explain these? • Could you predict behavior not observed? • Are you able to validate your predictions? ...
... • What observations do you have? • Are you able to explain these? • Could you predict behavior not observed? • Are you able to validate your predictions? ...
Lecture 4 - Orbits of the planets
... move together with the epicycle of Venus centered on a line between the Earth and the Sun • Then, Venus can never be the opposite side of the Sun from the Earth, so it can never have gibbous phases – no “full Venus”. ...
... move together with the epicycle of Venus centered on a line between the Earth and the Sun • Then, Venus can never be the opposite side of the Sun from the Earth, so it can never have gibbous phases – no “full Venus”. ...
Dynamics of the Earth
... Historically, a day is a time interval between successive upper transits of a given celestial reference point. upper transit – the passage of a body across the celestial meridian moving westward hour angle – the westward angular distance of an object from the meridian; negative if object is east of ...
... Historically, a day is a time interval between successive upper transits of a given celestial reference point. upper transit – the passage of a body across the celestial meridian moving westward hour angle – the westward angular distance of an object from the meridian; negative if object is east of ...
Grade 9 Science – Unit 4 Space Quiz
... b. Galaxies are moving away from Earth in all directions at a constant rate c. Remnant heat from the original very hot expansion has been measured d. All of the above 18. What type of star forms after a Supernova explosion? In this star, the centre collapses so that protons and electrons combine to ...
... b. Galaxies are moving away from Earth in all directions at a constant rate c. Remnant heat from the original very hot expansion has been measured d. All of the above 18. What type of star forms after a Supernova explosion? In this star, the centre collapses so that protons and electrons combine to ...
Geocentric model
In astronomy, the geocentric model (also known as geocentrism, or the Ptolemaic system) is a description of the cosmos where Earth is at the orbital center of all celestial bodies. This model served as the predominant cosmological system in many ancient civilizations such as ancient Greece including the noteworthy systems of Aristotle (see Aristotelian physics) and Ptolemy. As such, they believed that the Sun, Moon, stars, and naked eye planets circled Earth.Two commonly made observations supported the idea that Earth was the center of the Universe. The stars, the sun, and planets appear to revolve around Earth each day, making Earth the center of that system. The stars were thought to be on a celestial sphere, with the earth at its center, that rotated each day, using a line through the north and south pole as an axis. The stars closest to the equator appeared to rise and fall the greatest distance, but each star circled back to its rising point each day. The second observation supporting the geocentric model was that the Earth does not seem to move from the perspective of an Earth-bound observer, and that it is solid, stable, and unmoving.Ancient Roman and medieval philosophers usually combined the geocentric model with a spherical Earth. It is not the same as the older flat Earth model implied in some mythology, as was the case with the biblical and postbiblical Latin cosmology. The ancient Jewish Babylonian uranography pictured a flat Earth with a dome-shaped rigid canopy named firmament placed over it. (רקיע- rāqîa').However, the ancient Greeks believed that the motions of the planets were circular and not elliptical, a view that was not challenged in Western culture until the 17th century through the synthesis of theories by Copernicus and Kepler.The astronomical predictions of Ptolemy's geocentric model were used to prepare astrological and astronomical charts for over 1500 years. The geocentric model held sway into the early modern age, but from the late 16th century onward was gradually superseded by the heliocentric model of Copernicus, Galileo and Kepler. There was much resistance to the transition between these two theories. Christian theologians were reluctant to reject a theory that agreed with Bible passages (e.g. ""Sun, stand you still upon Gibeon"", Joshua 10:12 – King James 2000 Bible). Others felt a new, unknown theory could not subvert an accepted consensus for geocentrism.