Chapter 25.1: Models of our Solar System
... 1. Models of the Solar System Ancient people thought … ...
... 1. Models of the Solar System Ancient people thought … ...
ppt file
... Copernicus (1473 - 1543): On the Revolution of Heavenly Spheres New Heliocentric Model ...
... Copernicus (1473 - 1543): On the Revolution of Heavenly Spheres New Heliocentric Model ...
wdtoc1
... Saturn's most distinctive feature is its ring system, which was first seen in 1610 by Italian scientist Galileo, using one of the first telescopes. He did not understand that the rings were separate from the body of the planet, so he described them as handles (ansae). The Dutch astronomer Christiaan ...
... Saturn's most distinctive feature is its ring system, which was first seen in 1610 by Italian scientist Galileo, using one of the first telescopes. He did not understand that the rings were separate from the body of the planet, so he described them as handles (ansae). The Dutch astronomer Christiaan ...
Chapter 25.1: Models of our Solar System
... 1. Models of the Solar System Ancient people thought … ...
... 1. Models of the Solar System Ancient people thought … ...
June 2012 - smile2340
... medium. Just like all fingerprints differ; no two substances have exactly the same index of refraction. A simple way to estimate n of water ( which is 1.333) is to place a quarter in a glass full of water and look through the water at the quarter from above and it will look closer. Next, mark where ...
... medium. Just like all fingerprints differ; no two substances have exactly the same index of refraction. A simple way to estimate n of water ( which is 1.333) is to place a quarter in a glass full of water and look through the water at the quarter from above and it will look closer. Next, mark where ...
Cosmic Distance Ladder Terrence Tao (UCLA)
... Once again, the ancient Greeks could answer this question! • Aristarchus already knew that the radius of the moon was about 1/180 of the distance to the moon. Since the Sun and Moon have about the same angular width (most dramatically seen during a solar eclipse), he concluded that the radius of th ...
... Once again, the ancient Greeks could answer this question! • Aristarchus already knew that the radius of the moon was about 1/180 of the distance to the moon. Since the Sun and Moon have about the same angular width (most dramatically seen during a solar eclipse), he concluded that the radius of th ...
The Sun and the Solar System
... A1: (a) use data of the diameter and average distance of the Sun and Moon, find the angular size (in units of arcsecond and in degree) of the Sun and the Moon viewed from the Earth. The Sun’s data are given at Table 16-1 (pp. 434), and the Moon’s data are given at Table 10-1 (pp. 257). (b) when the ...
... A1: (a) use data of the diameter and average distance of the Sun and Moon, find the angular size (in units of arcsecond and in degree) of the Sun and the Moon viewed from the Earth. The Sun’s data are given at Table 16-1 (pp. 434), and the Moon’s data are given at Table 10-1 (pp. 257). (b) when the ...
EARTH SCIENCE MIDTERM REVIEW SHEET
... Use the following review facts as a basis for studying. Use them when doing review assignments to look up helpful facts. Memorizing the facts is not as important as understanding what they mean and why. To help you be successful complete Castle Learning Midterm Pretest Introduction Indirect relation ...
... Use the following review facts as a basis for studying. Use them when doing review assignments to look up helpful facts. Memorizing the facts is not as important as understanding what they mean and why. To help you be successful complete Castle Learning Midterm Pretest Introduction Indirect relation ...
Why do we weigh more on Earth than on the moon?
... What makes one object have a stronger gravitational force than another? There are two factors that determine gravitational force. The first is an object’s mass. An object with a large amount of mass will exert more gravitational force than an object with a small amount of mass. Since Earth has more ...
... What makes one object have a stronger gravitational force than another? There are two factors that determine gravitational force. The first is an object’s mass. An object with a large amount of mass will exert more gravitational force than an object with a small amount of mass. Since Earth has more ...
Lecture 3 - Concord University
... orise & set of sun/moon/planets can be explained Q: how? owe don’t feel Earth is spinning would mean we move at 900 mph w.r.t. Earth center ...
... orise & set of sun/moon/planets can be explained Q: how? owe don’t feel Earth is spinning would mean we move at 900 mph w.r.t. Earth center ...
Northern Hemisphere – December 2012
... Jupiter rises at sunset at the beginning of the month and is visible throughout the night as it reaches opposition (opposite the Sun in the sky) during December. Shining at magnitude -2.8, it reaches 60 degrees' elevation in Taurus in the south, helping us to see it with little atmospheric interfere ...
... Jupiter rises at sunset at the beginning of the month and is visible throughout the night as it reaches opposition (opposite the Sun in the sky) during December. Shining at magnitude -2.8, it reaches 60 degrees' elevation in Taurus in the south, helping us to see it with little atmospheric interfere ...
PDF file
... • Realized that the orbits cannot be perfect circles. The orbits were elliptical. • Discovered 3 mathematical laws of planetary motion. ...
... • Realized that the orbits cannot be perfect circles. The orbits were elliptical. • Discovered 3 mathematical laws of planetary motion. ...
NATS1311_090908_bw
... determine local solar time is 3:00 PM. If time at Greenwich is 1:00 PM, you are two hours east of Greenwich and your longitude is 15º X 2 = 30º East Longitude. Accurate determination of longitude required invention of clock that could remain accurate on a rocking ship. By early 1700s, considered so ...
... determine local solar time is 3:00 PM. If time at Greenwich is 1:00 PM, you are two hours east of Greenwich and your longitude is 15º X 2 = 30º East Longitude. Accurate determination of longitude required invention of clock that could remain accurate on a rocking ship. By early 1700s, considered so ...
Our Space Journey
... because the surface is not solid enough. All of the things you see have a gravitational field. The larger the object the more force of gravity. Normally every thing gets pulled to the surface but things like balloons don't get any gravity because of the helium. Every planet has gravity but not as mu ...
... because the surface is not solid enough. All of the things you see have a gravitational field. The larger the object the more force of gravity. Normally every thing gets pulled to the surface but things like balloons don't get any gravity because of the helium. Every planet has gravity but not as mu ...
Geological Processes, Moon, and Mercury
... of the planet, its distance from the star, and its rotation rate. You don't expect much erosion on planets that are too small, too close to or too far from the star, or that don't spin enough to keep winds moving. A source of erosion you might not normally consider comes from micrometeorite impacts. ...
... of the planet, its distance from the star, and its rotation rate. You don't expect much erosion on planets that are too small, too close to or too far from the star, or that don't spin enough to keep winds moving. A source of erosion you might not normally consider comes from micrometeorite impacts. ...
Newton`s Second Law of Motion
... 1 Newton (force) will accelerate a 1 kg object (mass) at 1 (m/s)/s (acceleration). • Notice that a newton is equal to a kilogram times a meter per second per second (kg(m/s)/s). ...
... 1 Newton (force) will accelerate a 1 kg object (mass) at 1 (m/s)/s (acceleration). • Notice that a newton is equal to a kilogram times a meter per second per second (kg(m/s)/s). ...
astro 001 - courses.psu.edu
... In the figure above, we observe the Sun from State College, PA, at three possible rising locations (1, 2 and 3) along the eastern horizon. Due east is marked with a vertical bar and labeled EAST. Please refer to this diagram when responding to Questions 1 - 3. 1. Which position is closest to the ris ...
... In the figure above, we observe the Sun from State College, PA, at three possible rising locations (1, 2 and 3) along the eastern horizon. Due east is marked with a vertical bar and labeled EAST. Please refer to this diagram when responding to Questions 1 - 3. 1. Which position is closest to the ris ...
Name
... B) the varying speed of the Earth in its orbit about the Sun. C) the precession of the Earth's rotation axis. D) the tilt of the Earth's rotation axis relative to the ecliptic. E) the tilt of the Moon's orbital plane relative to the ecliptic. 36) Which object is not considered a star? A) The Sun B) ...
... B) the varying speed of the Earth in its orbit about the Sun. C) the precession of the Earth's rotation axis. D) the tilt of the Earth's rotation axis relative to the ecliptic. E) the tilt of the Moon's orbital plane relative to the ecliptic. 36) Which object is not considered a star? A) The Sun B) ...
Name: Sect:______ Date
... 2. What do you call the sum of all of the forces acting on an object? The net force. 3. Describe the difference between a balanced and unbalance force. Balanced forces are equal but in opposite directions so there is no motion as a result, while unbalanced forces are unequal which cause an object to ...
... 2. What do you call the sum of all of the forces acting on an object? The net force. 3. Describe the difference between a balanced and unbalance force. Balanced forces are equal but in opposite directions so there is no motion as a result, while unbalanced forces are unequal which cause an object to ...
HW2_Answers
... 3. Kepler found that the farther a planet was from the Sun, the slower it moved in its orbit. Use what you have learned about an orbit and the Newton’s law of Gravity to explain why Jupiter cannot orbit the Sun as fast as the Earth. Jupiter is farther from the Sun than the Earth. Because of this, th ...
... 3. Kepler found that the farther a planet was from the Sun, the slower it moved in its orbit. Use what you have learned about an orbit and the Newton’s law of Gravity to explain why Jupiter cannot orbit the Sun as fast as the Earth. Jupiter is farther from the Sun than the Earth. Because of this, th ...
Class 6 Orbits and Tides I : Orbital energy
... Unlike parabolic case, particle has non-zero velocity even when it is far from the gravitating mass (i.e. “at infinity”) This is an unbound orbit ...
... Unlike parabolic case, particle has non-zero velocity even when it is far from the gravitating mass (i.e. “at infinity”) This is an unbound orbit ...
–1– AST104 Sp06: Welcome to EXAM 2 Multiple Choice Questions
... d. Because liquid water on the surface is impossible without a liquid core. a. Jupiter, Mercury, Venus, Mars e. By putting one’s ear to the ground in a quiet location, one can hear the liquid core sloshing around. 30. Which is the LEAST helpful in distinguishing the Large-Impact model of the moon’s ...
... d. Because liquid water on the surface is impossible without a liquid core. a. Jupiter, Mercury, Venus, Mars e. By putting one’s ear to the ground in a quiet location, one can hear the liquid core sloshing around. 30. Which is the LEAST helpful in distinguishing the Large-Impact model of the moon’s ...
Name - MIT
... 32) The planets, the Earth, and the Sun all tend to fall in the same plane called … A) perihelion. B) aphelion. C) the ecliptic. D) retrograde motion. E) the umbra. 33) Precession causes … A) the Moon to orbit the Earth at a faster rate B) the position of the North Celestial Pole in the sky to vary ...
... 32) The planets, the Earth, and the Sun all tend to fall in the same plane called … A) perihelion. B) aphelion. C) the ecliptic. D) retrograde motion. E) the umbra. 33) Precession causes … A) the Moon to orbit the Earth at a faster rate B) the position of the North Celestial Pole in the sky to vary ...
Name
... B) He wanted the Moon to be at the center. C) He did not think Mars was a planet. D) He did not think Jupiter was a planet. E) He wanted all the orbits of the planets to be perfectly circular. 27) Which of these planets travels the slowest around the Sun? A) Venus B) Jupiter. C) Saturn D) Mercury E) ...
... B) He wanted the Moon to be at the center. C) He did not think Mars was a planet. D) He did not think Jupiter was a planet. E) He wanted all the orbits of the planets to be perfectly circular. 27) Which of these planets travels the slowest around the Sun? A) Venus B) Jupiter. C) Saturn D) Mercury E) ...
Study Guide: Use your notes and handouts to answer the following
... 35. When it is a full moon, what is the alignment of Earth, Sun, and Moon? Earth is in the middle of the Sun and Moon 36. When it is a new moon, what is the alignment of Earth, Sun, and Moon? The moon is in the middle of the Sun and Earth 37. What is an eclipse? Same as for question #23 38. How is a ...
... 35. When it is a full moon, what is the alignment of Earth, Sun, and Moon? Earth is in the middle of the Sun and Moon 36. When it is a new moon, what is the alignment of Earth, Sun, and Moon? The moon is in the middle of the Sun and Earth 37. What is an eclipse? Same as for question #23 38. How is a ...