Quiz 2 Key - Oglethorpe University
... considered evidence for which model? A. The geocentric model B. The heliocentric model C. Neither model could explain this fact. 3.) In what way did Aristotle influence the acceptance of the heliocentric theory in 15th-century Europe? A. His philosophy assumed the geocentric theory and was adopted b ...
... considered evidence for which model? A. The geocentric model B. The heliocentric model C. Neither model could explain this fact. 3.) In what way did Aristotle influence the acceptance of the heliocentric theory in 15th-century Europe? A. His philosophy assumed the geocentric theory and was adopted b ...
Lecture 34 – Exobiology- Life Elsewhere in the Universe
... Contrary opinions about common life in the universe • “Rare Earth Hypothesis”, after book “Rare Earth” by Brownlee and Ward: Asserts that a large number of improbable events were necessary for the development of life on the Earth. These are unlikely to be duplicated elsewhere, so higher life is ext ...
... Contrary opinions about common life in the universe • “Rare Earth Hypothesis”, after book “Rare Earth” by Brownlee and Ward: Asserts that a large number of improbable events were necessary for the development of life on the Earth. These are unlikely to be duplicated elsewhere, so higher life is ext ...
Warm Up - Cloudfront.net
... to their masses and inversely proportional to the square of the distance between their centers of mass • The greater the mass of an object, the greater its gravitational force • Newton proved that the force of gravity, combined with the tendency of a planet to remain in straight-line motion, results ...
... to their masses and inversely proportional to the square of the distance between their centers of mass • The greater the mass of an object, the greater its gravitational force • Newton proved that the force of gravity, combined with the tendency of a planet to remain in straight-line motion, results ...
Eratosthenes of Cyrene (c.276-c.196 BC)
... Athens, who argued vehemently against the pluralistic teachings of atomism. "The world must be unique," he wrote. "There cannot be several worlds." He justified this stance on a number of grounds. For example, in his Metaphysics, he explains the motion of the planets and stars (around the Earth) as ...
... Athens, who argued vehemently against the pluralistic teachings of atomism. "The world must be unique," he wrote. "There cannot be several worlds." He justified this stance on a number of grounds. For example, in his Metaphysics, he explains the motion of the planets and stars (around the Earth) as ...
Inner Planets
... Earth (same as deep ocean) Has no moons. More than 20 space probes from USA & USSR The surface is rocky and very hot. .815 x size Earth Average temp of 462°C ...
... Earth (same as deep ocean) Has no moons. More than 20 space probes from USA & USSR The surface is rocky and very hot. .815 x size Earth Average temp of 462°C ...
The Sun
... Compared with everything else in the solar system, the sun is huge – I mean, really, really big. In fact, the Sun makes up 99% of the mass of the solar system. The sun produces energy through nuclear fusion – NOT fission. Memory trick: the sun has one s, and so does fusion. Fusion happens in the cor ...
... Compared with everything else in the solar system, the sun is huge – I mean, really, really big. In fact, the Sun makes up 99% of the mass of the solar system. The sun produces energy through nuclear fusion – NOT fission. Memory trick: the sun has one s, and so does fusion. Fusion happens in the cor ...
aka Nicholas Copernicus
... this was a work of fiction to placate the Church. The Church didn’t fall for it and forced him to recant. He spent the rest of his life in house arrest •Theory of Inertia= stated that things in motion remained in motion unless acted upon by another force– implied God is not necessary to move planets ...
... this was a work of fiction to placate the Church. The Church didn’t fall for it and forced him to recant. He spent the rest of his life in house arrest •Theory of Inertia= stated that things in motion remained in motion unless acted upon by another force– implied God is not necessary to move planets ...
Word - UW-Madison Astronomy
... a) What phase is the moon at a solar eclipse? A lunar eclipse? b) Briefly explain why solar and lunar eclipses do not occur every month. A sketch is worth a ...
... a) What phase is the moon at a solar eclipse? A lunar eclipse? b) Briefly explain why solar and lunar eclipses do not occur every month. A sketch is worth a ...
chapter4 - Empyrean Quest Publishers
... telescope was that Venus exhibits phases like Moon Galileo also noticed that the apparent size of Venus as seen through his telescope was related to the planet’s phase Venus appears small at gibbous phase, largest at crescent phase. She never gets full—sun washes out her light. ...
... telescope was that Venus exhibits phases like Moon Galileo also noticed that the apparent size of Venus as seen through his telescope was related to the planet’s phase Venus appears small at gibbous phase, largest at crescent phase. She never gets full—sun washes out her light. ...
Seasons
... b. The apparent center of the arcs is Polaris (north star) WHY? i. Since Polaris is located above the Earth’s axis of rotation, the stars and planets seem to rotate counterclockwise around Polaris at approximately 15o per hour. WHY 15o per hour? ii. The apparent daily motion of stars, moon, and pla ...
... b. The apparent center of the arcs is Polaris (north star) WHY? i. Since Polaris is located above the Earth’s axis of rotation, the stars and planets seem to rotate counterclockwise around Polaris at approximately 15o per hour. WHY 15o per hour? ii. The apparent daily motion of stars, moon, and pla ...
Sun Moon and Stars Study Guide
... It takes about as long as it takes the Moon to rotate once on its axis. About 28 days. ...
... It takes about as long as it takes the Moon to rotate once on its axis. About 28 days. ...
Astronomical history
... being the first star in our solar system and being the furthest away eluding to that the stars were placed outside of our solar system. (c) Ptolemy knew that Mars moved across the sky in a looping motion called retrograde motion. His model explained this motion using epicycles. Use the diagram below ...
... being the first star in our solar system and being the furthest away eluding to that the stars were placed outside of our solar system. (c) Ptolemy knew that Mars moved across the sky in a looping motion called retrograde motion. His model explained this motion using epicycles. Use the diagram below ...
Intro L4 IQ
... Diurnal changes, for example, the transit of stars during the course of the night (or the sun during the day) are caused by the Earth’s rotation. Diurnal changes are far more obvious than annual changes ...
... Diurnal changes, for example, the transit of stars during the course of the night (or the sun during the day) are caused by the Earth’s rotation. Diurnal changes are far more obvious than annual changes ...
Early Astronomy
... These world models attempted to explain phenomena visible to everyone: The daily and annual motions of the Sun across the sky The motion and phases of the Moon The daily and annual motions of the stars (i.e., the celestial sphere) The odd motions of the 5 known planets, or “wanderers” Sola ...
... These world models attempted to explain phenomena visible to everyone: The daily and annual motions of the Sun across the sky The motion and phases of the Moon The daily and annual motions of the stars (i.e., the celestial sphere) The odd motions of the 5 known planets, or “wanderers” Sola ...
2. Kepler a. They observed the sun, moon, and stars move across
... Name the person being described in each clue. Copernicus Galileo Kepler Ptolemy This scientist proved that the heliocentric model of the solar system was 1. Galileo correct with observations from his telescope. This scientist determined that planetary orbits were ellipses, or oval in 2. Kepler shape ...
... Name the person being described in each clue. Copernicus Galileo Kepler Ptolemy This scientist proved that the heliocentric model of the solar system was 1. Galileo correct with observations from his telescope. This scientist determined that planetary orbits were ellipses, or oval in 2. Kepler shape ...
CRCT Review 1
... 17. If you were to watch the stars all night, they would seem to A. stay in exactly the same place in the sky. B. move across the sky at night, as the Sun does during the day. C. go in circles around the point straight up from where you are. D. move across the sky at night, in the opposite directio ...
... 17. If you were to watch the stars all night, they would seem to A. stay in exactly the same place in the sky. B. move across the sky at night, as the Sun does during the day. C. go in circles around the point straight up from where you are. D. move across the sky at night, in the opposite directio ...
Earth Science, 10th edition Chapter 20: Origin of Modern Astronomy
... 2. Constructed a model of the solar system that put the Sun at the center, but he used circular orbits for the planets 3. Ushered out old astronomy b. Tycho Brahe (1546-1601) 1. Precise observer 2. Tried to find stellar parallax – the apparent shift in a star's position due to the revolution of Eart ...
... 2. Constructed a model of the solar system that put the Sun at the center, but he used circular orbits for the planets 3. Ushered out old astronomy b. Tycho Brahe (1546-1601) 1. Precise observer 2. Tried to find stellar parallax – the apparent shift in a star's position due to the revolution of Eart ...
PPT: The Scientific Revolution
... Skepticism and Independent Reasoning: For example, Descartes reached the extreme of skepticism by doubting his own existence. Then, he realized that his own act of thinking proved his own existence (I think, therefore, I am.) Challenges to Religion: The idea that the universe worked like a machine a ...
... Skepticism and Independent Reasoning: For example, Descartes reached the extreme of skepticism by doubting his own existence. Then, he realized that his own act of thinking proved his own existence (I think, therefore, I am.) Challenges to Religion: The idea that the universe worked like a machine a ...
Document
... sun. • THE climate is very active with large storms whirling through the atmosphere. • Their can be high-speed winds that reach 1,342miles per hour. ...
... sun. • THE climate is very active with large storms whirling through the atmosphere. • Their can be high-speed winds that reach 1,342miles per hour. ...
History of Astronomy Scavenger Hunt
... Directions: Using the internet, search for the person and date for each discovery. 1. I was the first person to use a telescope to look at the heavens. Who am I? Galileo 2. We discovered the relationship between a star’s temperature and it’s brightness. Who are we? Ejnar Hertzsprung and Henry Norris ...
... Directions: Using the internet, search for the person and date for each discovery. 1. I was the first person to use a telescope to look at the heavens. Who am I? Galileo 2. We discovered the relationship between a star’s temperature and it’s brightness. Who are we? Ejnar Hertzsprung and Henry Norris ...
Module 7 Developmental task - Number
... Eight planets rotate the Sun in our solar system – our Earth being the third planet from the Sun. The planets vary in size – the smallest, Mercury, has a radius of only 2 439 km, whereas the largest planet, Jupiter, has a radius more than 70 000 km at its equator. ...
... Eight planets rotate the Sun in our solar system – our Earth being the third planet from the Sun. The planets vary in size – the smallest, Mercury, has a radius of only 2 439 km, whereas the largest planet, Jupiter, has a radius more than 70 000 km at its equator. ...
Dialogue Concerning the Two Chief World Systems
The Dialogue Concerning the Two Chief World Systems (Dialogo sopra i due massimi sistemi del mondo) was a 1632 Italian-language book by Galileo Galilei comparing the Copernican system with the traditional Ptolemaic system. It was translated into Latin as Systema cosmicum (English: Cosmic System) in 1635 by Matthias Bernegger. The book was dedicated to Galileo's patron, Ferdinando II de' Medici, Grand Duke of Tuscany, who received the first printed copy on February 22, 1632.In the Copernican system the Earth and other planets orbit the Sun, while in the Ptolemaic system everything in the Universe circles around the Earth. The Dialogue was published in Florence under a formal license from the Inquisition. In 1633, Galileo was found to be ""vehemently suspect of heresy"" based on the book, which was then placed on the Index of Forbidden Books, from which it was not removed until 1835 (after the theories it discussed had been permitted in print in 1822). In an action that was not announced at the time, the publication of anything else he had written or ever might write was also banned.