SOLAR SYSTEM OVERVIEW - Ms. Ferebee`s Webpage
... was the center of the solar system. Copernicus believed that the Sun is the center of the solar system. He found that Earth rotates once in 24 hours, causing day and night. Galileo (1564- 1642) Galileo was an Italian scholar who made great contributions to what we know about the solar system. Using ...
... was the center of the solar system. Copernicus believed that the Sun is the center of the solar system. He found that Earth rotates once in 24 hours, causing day and night. Galileo (1564- 1642) Galileo was an Italian scholar who made great contributions to what we know about the solar system. Using ...
8 Grade/Comp.Sci.III adv Course Code: 2002110
... Gravity and the Solar System Gravity Overview 1. Define gravity The Laws of Planetary Motion 1. State Kepler’s first, second, and third laws of planetary motion. Page 2 of 4 ...
... Gravity and the Solar System Gravity Overview 1. Define gravity The Laws of Planetary Motion 1. State Kepler’s first, second, and third laws of planetary motion. Page 2 of 4 ...
Celestial Equator
... • The stars appear to move from east to west as follows: i. vertically downwards at the equator (if facing West); ii. downwards and to the right in the USA (if facing West); iii. from left to right at the north Pole; iv. from right to left at the South Pole. ...
... • The stars appear to move from east to west as follows: i. vertically downwards at the equator (if facing West); ii. downwards and to the right in the USA (if facing West); iii. from left to right at the north Pole; iv. from right to left at the South Pole. ...
Working with the Illinois Learning Standards: A Constructivist
... flat earth (no such thing as a spherical picture) and photos can be faked (you see Star Trek on TV, do you believe that this is real?) • centripetal force demonstration (ball on a string) • put students on an elevator and measure their weights as they accelerate upward and downward; they weigh less ...
... flat earth (no such thing as a spherical picture) and photos can be faked (you see Star Trek on TV, do you believe that this is real?) • centripetal force demonstration (ball on a string) • put students on an elevator and measure their weights as they accelerate upward and downward; they weigh less ...
LECTURE 1
... are. Take a look at all the things that you see around you every day. For example, the pencil in your hand, where does the lead in the pencil come from? The room you are probably in is made up of bricks, metal and glass; all of these things come from the Earth. Just about everything around you that ...
... are. Take a look at all the things that you see around you every day. For example, the pencil in your hand, where does the lead in the pencil come from? The room you are probably in is made up of bricks, metal and glass; all of these things come from the Earth. Just about everything around you that ...
Mercury_Orbit_Lab_1_(better_than_2)
... it is surprisingly easy to derive an orbit from basic observations. In this exercise you will use a set of simple observations, which you could have made yourself, to discover the size and shape of the orbit of Mercury. You will be repeating work that Johannes Kepler did to formulate his laws of pla ...
... it is surprisingly easy to derive an orbit from basic observations. In this exercise you will use a set of simple observations, which you could have made yourself, to discover the size and shape of the orbit of Mercury. You will be repeating work that Johannes Kepler did to formulate his laws of pla ...
explaining the seasons and locating the north and south celestial
... not perpendicular to the ecliptic plane formed by the earth’s trajectory about the sun. Likewise many have learned in elementary school how to locate the north-star (Polaris) using the Big Dipper as a guide, but are clueless when one mentions the Celestial Sphere of infinite radius which is intersec ...
... not perpendicular to the ecliptic plane formed by the earth’s trajectory about the sun. Likewise many have learned in elementary school how to locate the north-star (Polaris) using the Big Dipper as a guide, but are clueless when one mentions the Celestial Sphere of infinite radius which is intersec ...
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 ...
Sun - Cobb Learning
... once every 26,000 years. It will be closest to Polaris ~ A.D. 2100. There is nothing peculiar about Polaris at all (neither particularly bright nor nearby etc.) ...
... once every 26,000 years. It will be closest to Polaris ~ A.D. 2100. There is nothing peculiar about Polaris at all (neither particularly bright nor nearby etc.) ...
History of Astronomy
... been diminishing slowly since prehistoric times; and this fact has been confirmed by Egyptian and Chinese observations on the length of the shadow of a vertical pillar, made thousands of years before the Christian era, in summer and winter. There are other reasons why we must be tolerant of the crud ...
... been diminishing slowly since prehistoric times; and this fact has been confirmed by Egyptian and Chinese observations on the length of the shadow of a vertical pillar, made thousands of years before the Christian era, in summer and winter. There are other reasons why we must be tolerant of the crud ...
Game Guide / Chronopticon
... • Like the sun, any given star or constellation seems to move in an arc across the sky over the course of hours • Different constellations are visible during different times of year (or different seasons) • You can calculate elapsed time (hours) based on the apparent motion of constellations during ...
... • Like the sun, any given star or constellation seems to move in an arc across the sky over the course of hours • Different constellations are visible during different times of year (or different seasons) • You can calculate elapsed time (hours) based on the apparent motion of constellations during ...
Teacher: Mrs. Zimmerman Astronomy Part 2 Practice Test 1. In the
... As the planet makes one complete revolution around the star, starting at the position shown, the gravitational attraction between the star and the planet will 1. decrease, then increase 2. increase, then decrease ...
... As the planet makes one complete revolution around the star, starting at the position shown, the gravitational attraction between the star and the planet will 1. decrease, then increase 2. increase, then decrease ...
Earth In Space - Hicksville Public Schools / Homepage
... a star that remains stationary in the night sky found directly above the north pole axis. ...
... a star that remains stationary in the night sky found directly above the north pole axis. ...
HO-04 5a Astro Unit Content
... Much of the above information could usefully be represented in a Venn diagram. Students will be able to make, record, and then clearly share accurate results from “naked-eye” observations of objects in the sky (e.g., clouds, planes, sun, moon, stars). They will use their recorded observations to fin ...
... Much of the above information could usefully be represented in a Venn diagram. Students will be able to make, record, and then clearly share accurate results from “naked-eye” observations of objects in the sky (e.g., clouds, planes, sun, moon, stars). They will use their recorded observations to fin ...
Astronomy - Educator Pages
... There are three important areas of the solar system to know about. -The Asteroid Belt – the area between Mars and Jupiter where most of the solar systems asteroids and meteoroids orbit the sun. The Kuiper Belt- area outside the planet Neptune, containing several dwarf planets as well as smaller obj ...
... There are three important areas of the solar system to know about. -The Asteroid Belt – the area between Mars and Jupiter where most of the solar systems asteroids and meteoroids orbit the sun. The Kuiper Belt- area outside the planet Neptune, containing several dwarf planets as well as smaller obj ...
celestial equator
... equator. It is a projection of the Earth's equator out to the celestial sphere. The number of degrees that a celestial object is north or south of the celestial equator is called the declination (DEC) It is the analogue of latitude on the sky. The analogue of longitude is called right ascension (RA) ...
... equator. It is a projection of the Earth's equator out to the celestial sphere. The number of degrees that a celestial object is north or south of the celestial equator is called the declination (DEC) It is the analogue of latitude on the sky. The analogue of longitude is called right ascension (RA) ...
The Project Gutenberg EBook of History of Astronomy, by George
... An attempt has been made in these pages to trace the evolution of intellectual thought in the progress of astronomical discovery, and, by recognising the different points of view of the different ages, to give due credit even to the ancients. No one can expect, in a history of astronomy of limited s ...
... An attempt has been made in these pages to trace the evolution of intellectual thought in the progress of astronomical discovery, and, by recognising the different points of view of the different ages, to give due credit even to the ancients. No one can expect, in a history of astronomy of limited s ...
Study Guide for the Comprehensive Final Exam
... 20. Describe the location of sunrise and sunset along the horizon for any given day of the year. 21. Describe how the maximum altitude of the Sun depends on day of the year. 22. Explain why the solar day is different from the sidereal day. 23. Describe how day length varies depending on whether the ...
... 20. Describe the location of sunrise and sunset along the horizon for any given day of the year. 21. Describe how the maximum altitude of the Sun depends on day of the year. 22. Explain why the solar day is different from the sidereal day. 23. Describe how day length varies depending on whether the ...
AST 101 Final Exam DO NOT open the exam until
... b.) The Greeks made so many advancements in science and astronomy that it was assumed that all of their models were correct, including Ptolmey’s. c.) The successful naked eye observation of stellar parallax confirmed that the planets must orbit in circles within circles. d.) The model’s predictions ...
... b.) The Greeks made so many advancements in science and astronomy that it was assumed that all of their models were correct, including Ptolmey’s. c.) The successful naked eye observation of stellar parallax confirmed that the planets must orbit in circles within circles. d.) The model’s predictions ...
03jan13.ppt - Institute for Astronomy
... Axis tilt changes directness of sunlight during the year. ...
... Axis tilt changes directness of sunlight during the year. ...
Lesson Plan - California Academy of Sciences
... Dark room with minimal light pollution 1 copy per student of the assessment probe (optional) Glow-In-The-Dark Ball (optional) ...
... Dark room with minimal light pollution 1 copy per student of the assessment probe (optional) Glow-In-The-Dark Ball (optional) ...
Learning About Stars
... sky for thousands of years. When ancient people looked up, the stars looked almost identical to what we see today. Stars do change, but they change VERY slowly. We will probably not notice changes to the stars in our lifetime. ...
... sky for thousands of years. When ancient people looked up, the stars looked almost identical to what we see today. Stars do change, but they change VERY slowly. We will probably not notice changes to the stars in our lifetime. ...
Copernican heliocentrism
Copernican heliocentrism is the name given to the astronomical model developed by Nicolaus Copernicus and published in 1543. It positioned the Sun near the center of the Universe, motionless, with Earth and the other planets rotating around it in circular paths modified by epicycles and at uniform speeds. The Copernican model departed from the Ptolemaic system that prevailed in Western culture for centuries, placing Earth at the center of the Universe, and is often regarded as the launching point to modern astronomy and the Scientific Revolution.Copernicus was aware that the ancient Greek Aristarchus had already proposed a heliocentric theory, and cited him as a proponent of it in a reference that was deleted before publication, but there is no evidence that Copernicus had knowledge of, or access to, the specific details of Aristarchus' theory. Although he had circulated an outline of his own heliocentric theory to colleagues sometime before 1514, he did not decide to publish it until he was urged to do so late in his life by his pupil Rheticus. Copernicus's challenge was to present a practical alternative to the Ptolemaic model by more elegantly and accurately determining the length of a solar year while preserving the metaphysical implications of a mathematically ordered cosmos. Thus his heliocentric model retained several of the Ptolemaic elements causing the inaccuracies, such as the planets' circular orbits, epicycles, and uniform speeds, while at the same time re-introducing such innovations as,Earth is one of several planets revolving around a stationary Sun in a determined orderEarth has three motions: daily rotation, annual revolution, and annual tilting of its axisRetrograde motion of the planets is explained by Earth's motionDistance from Earth to the Sun is small compared to the distance to the stars.↑ 1.0 1.1 ↑