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Why Star Positions?
Why Star Positions?

... from their positions given by Ptolemy in his great mathematical and astronomical treatise, the Almagest. Sirius, for example, Earth in orbit around Sun had moved nearly half a degree southwards, about the diameter of the Moon, over the intervening two thousand years9 . Proper motion as the angular A ...
Astronomy 101 Course Review and Summary
Astronomy 101 Course Review and Summary

... Aristotle (4th cent BC) showed that the Earth is round. Greek astronomers developed a geocentric model for the universe. Ptolemy (2nd cent) used epicycles to explain retrograde motion of planers. Copernicus (16th cent) proposed a heliocentric model for the universe. In the model of Copernicus, retro ...
Answers to Coursebook questions – Chapter E3
Answers to Coursebook questions – Chapter E3

Stars
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Ethan - St. Brigid
Ethan - St. Brigid

... Takes six years to get to in a spaceship. It might have a liquid interior small core. It is 890 million miles from the sun. It could float if you could find an ocean big enough. ...
Chapter 4
Chapter 4

... • Galileo showed stars must be much farther than Tycho thought — used his telescope to show that the Milky Way is countless individual stars. ...
Glossary of terms - Universal Workshop
Glossary of terms - Universal Workshop

... the “main belt” between the orbits of Mars and Jupiter, but some are farther out and some come in nearer than the Earth. astrology should not be confused with astronomy, though they had a common origin. It is a body of traditions about how the relative positions of the Sun, Moon, and planets may aff ...
Universe and Solar System
Universe and Solar System

... Role: You are a member of your 6th grade class, which is helping your school compete for a hosting the President for a nationally televised address on space. Audience: The selection team for the President’s visit to a middle school, including educators and NASA scientists. Situation: The first space ...
Earth in the Universe Grade One
Earth in the Universe Grade One

... What are the predictable patterns caused by Earth’s movement in the solar system? The solar system consists of the sun and a collection of objects of varying sizes and conditions—including planets and their moons—that are held in orbit around the sun by its gravitational pull on them. This system ap ...
The Prague Astronomical Clock
The Prague Astronomical Clock

... The length of such a solar day varies slightly from day to day but its average (mean) value is 24 hours. Star (Sidereal) Time The length of a star day is the time between two consecutive meridian transits of a star. A sidereal day is a little shorter than a solar day and equal to 23h 56m 04s. This i ...
Rotary Homework #1
Rotary Homework #1

... 2. The spacecraft is three times as far from the Earth’s center as when at the surface of the Earth. Therefore, since the force as gravity decreases as the square of the distance, the force of gravity on the spacecraft will be one-ninth of its weight at the Earth’s surface. 1350 kg  9.80 m s 2 ...
Part 2 - Hewlett
Part 2 - Hewlett

... One time each day (every 24 hours) 3. How often does Earth rotate once? _________________________________________________ 4. The diagrams below represent two pieces of evidence that Earth rotates. Identify the evidence represented by each diagram. ...
Lecture 2a
Lecture 2a

... •  Tycho Brahe’s - Earth at center but other planets orbit the Sun (effectively the same as Copernican) •  Kepler’s - Sun at center with planets orbitting the Sun in elliptical paths CORRECT •  Differentiate models by comparing predictions with observations SCIENTIFIC METHOD need best observations a ...
Lecture - Faculty
Lecture - Faculty

... Share Question If an interstellar cloud contracts to become a star, it does so because of what force? a) electromagnetic b) nuclear c) gravitational d) centrifugal ...
PowerPoint Presentation - Small Bodies in the Solar System
PowerPoint Presentation - Small Bodies in the Solar System

...  Hundreds of millions of years ago, collisions with asteroids more often.  Over time, the # of asteroids in the path of the Earth decreased and collisions become less frequent. ...
Stellar mass Black Holes
Stellar mass Black Holes

... v =GM ( − ) r a ...
StarFlight - Center for the Presentation of Science
StarFlight - Center for the Presentation of Science

... narration, guided tours and a simple user interface, to create an application suitable for nonguided use in a museum by non-scientists. The script was written to guide the viewer through the visual journey, highlight any relevant astronomical principles, and inform on the mythological basis of the c ...
Proof of Earth`s Shape and Size
Proof of Earth`s Shape and Size

... equation that determined the circumference of the earth. ...
Student Text, pp. 278-284
Student Text, pp. 278-284

... Periodically we hear of “space junk” that falls through Earth’s atmosphere, leaving streaks of light as friction causes it to vaporize. This “junk” falls toward Earth when its orbit becomes unstable, yet when it was in proper working order, it remained in a stable orbit around Earth (Figure 1). To m ...
The Solar System
The Solar System

... Uranus is the ancient Greek deity of the Heavens, the earliest supreme god. Uranus was the son and mate of Gaia the father of Cronus (Saturn) and of the Cyclopes and Titans (predecessors of the Olympian ...
Kepler`s Laws Powerpoint
Kepler`s Laws Powerpoint

... planet revolve around the Sun one time) of a planet is directly proportional to the cube of the planet’s average distance from the Sun, R. What this means for us : The planets farther from the Sun take longer to orbit the Sun. (Much weaker than the above statement) ...
Some 250 years ago, the philosopher Immanuel Universal
Some 250 years ago, the philosopher Immanuel Universal

... special either. Except that some exoplanets are special. It is tempting to describe the many planetary systems that have been discovered so far as weird. Rather than the ‘inevitable’ orderly arrangement of our own Solar System — with small planets close, large planets far, and everything going aroun ...
Class 6 Orbits and Tides I : Orbital energy
Class 6 Orbits and Tides I : Orbital energy

... Escape velocity is very important concept… ...
sc_examII_fall_2002 - University of Maryland
sc_examII_fall_2002 - University of Maryland

... Choose the BEST answer to each of the following questions using what you have learned in ASTR 101. Indicate your choice on the scantron. (2 pts. each) 1. In the Cygnus X-1 system, the X-rays are explain by astronomers as A. strong radiation emitted by a supergiant star. B. a distant galaxy that has ...
Scientific Notation (Standard Form)
Scientific Notation (Standard Form)

... Scientific Notation (Standard Form) The distance from the Earth to the Sun is 152,000,000 km. The nearest star to our Sun is 3800000000000000km (4 Light Years) away - Alpha Centauri. The mass of an atom is approximately 0.00000000000000000000000042 kg !! There must be an easier way of writing these! ...
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Astronomical unit

The astronomical unit (symbol au, AU or ua) is a unit of length, roughly the distance from the Earth to the Sun. However, that distance varies as the Earth orbits the Sun, from a maximum (aphelion) to a minimum (perihelion) and back again once a year. Originally conceived as the average of Earth's aphelion and perihelion, it is now defined as exactly 7011149597870700000♠149597870700 meters (about 150 million kilometers, or 93 million miles). The astronomical unit is used primarily as a convenient yardstick for measuring distances within the Solar System or around other stars. However, it is also a fundamental component in the definition of another unit of astronomical length, the parsec.
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