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ASTR 1010 – Spring 2016 – Study Notes Dr. Magnani
ASTR 1010 – Spring 2016 – Study Notes Dr. Magnani

... people  and  so  the  idea  that  the  Universe  was  geocentric  became  entrenched.    In  the   second  century  AD,  the  Greek-­‐Egyptian  astronomer  Ptolemy  (a  Roman  citizen)   refined  the  geocentric  model  in  several  sophi ...
Lecture 2
Lecture 2

... – Created first scientific model ...
Lecture 2 - University of Chicago, Astronomy
Lecture 2 - University of Chicago, Astronomy

... errors. He believed that Tycho calculated his errors correctly, so he embarked on developing a world model that was in agreement with observations. And then he had an inspiration!.. Not a circle but an ellipse. A single ellipse with the Sun in its focus was able to fit all the data, instead of equan ...
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2. Kepler a. They observed the sun, moon, and stars move across

... 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. ...
Astronomy 1020 Exam 1 Review Questions
Astronomy 1020 Exam 1 Review Questions

... 19. Whose observations did Kepler use to formulate his 3 laws of planetary motion? Of what planet were these observations made? Why was Kepler so interested in geometric solids? 20. Who is considered the father of experimental physics? Who was the first person to use a telescope to study the cosmos? ...
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1 - Northwest ISD Moodle

... shows how the Earth’s gravitational field could influence the Sun’s motion. When the Earth is closest to the Sun in its orbit (a point called Perihelion), as small as we are, we do influence the Sun slightly, pulling it ...
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... Kepler’s laws of heliocentric planetary motions consistent will all of Tycho Brahe’s data but obtained very strong support only after vindication by accurate + unprecedented observations taken by Galileo Galilei with the recently invented telescope ...
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Geocentric vs. Heliocentric Models of the Solar System
Geocentric vs. Heliocentric Models of the Solar System

... If it fails even once must be reformulated or rejected! ...
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I. Early History of Astronomy

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... Universe: 15 billion years Milky Way Galaxy: 14 billion years Solar System: 4.6 Billion years Unicellular life: 3.4 billion years (oldest fossils) Cambrian era: 600 million years (fossils of complex, hard-bodied animals) Dinosaurs: 65-250 million years Homo sapiens: about a million years If 15 billi ...
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... distance light travels in one year (about 10 trillion km). Light from the Sun reaches Earth in a little more than 8 minutes. Light from the North Star (Polaris), reaches earth in about 700 years. Astronomers can use parallax to find out distances to the closer stars. Parallax is the apparent change ...
8th Grade - Astronomy
8th Grade - Astronomy

... not time. Example: Our next nearest star neighbor is Proxima Centauri which is 4.2 light-years from Earth. (p. 602) The apparent change in position of an object when seen from different places Astronomers use parallax to measure distances to nearby stars by measuring the Parallax apparent movement o ...
The History of Astronomy
The History of Astronomy

... “the simplest explanation is usually best.” ...
Solar System Vocabulary
Solar System Vocabulary

... Why do stars that are larger and brighter than the sun not appear this way from Earth? ...
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Foundations of Astronomy Presentation

... perfect sphere with Earth at the Center. Objects in space also move in perfect circles. ...
Geocentric vs. Heliocentric
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... A protoplanetary disk, such as those observed around some stars in the Orion nebula. Any planet of greater mass than Jupiter. A planet orbiting a star beyond the Sun; for example, the planet orbiting the star 51 Pegasi. D) A primitive organism thought to exist on Jupiter's moon, Europa. ...
The Heliocentric Model of the Solar System
The Heliocentric Model of the Solar System

... It is the actual sky image, more or less what the naked eye would see in a clear night far from city lights. The relative position of the stars, for example the 3 stars on a line at the center of the picture, seems to be ‘fixed’ relative to each other, i.e. they do not change relative positions in t ...
Word Pro - Smvocab
Word Pro - Smvocab

... Vocabulary List Angular Diameter - the apparent size of celestial objects measured by angle in degrees. Apogee - that point in the orbit of the moon or a planet which is most distant from the earth. Aristotle - one of the world's greatest thinkers and scientific investigators from ancient Greece. As ...
Astronomy Review (Cope) 64KB Jun 09 2013 08:13:01 PM
Astronomy Review (Cope) 64KB Jun 09 2013 08:13:01 PM

... 18. Starting with the speed of light being 3.00 x 10 meters per second (or 300,000 km per second), calculate how far light will travel in one (365 day) year. Stars ...
The Solar System
The Solar System

... People used to think that the Earth was at the centre of the universe, with everything going around it. We now know that this is not correct. The idea that fits scientific observations and allows us to predict the movement of the planets is called the heliocentric model. This just means that the Sun ...
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History of astronomy



Astronomy is the oldest of the natural sciences, dating back to antiquity, with its origins in the religious, mythological, cosmological, calendrical, and astrological beliefs and practices of pre-history: vestiges of these are still found in astrology, a discipline long interwoven with public and governmental astronomy, and not completely disentangled from it until a few centuries ago in the Western World (see astrology and astronomy). In some cultures, astronomical data was used for astrological prognostication.Ancient astronomers were able to differentiate between stars and planets, as stars remain relatively fixed over the centuries while planets will move an appreciable amount during a comparatively short time.
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