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ASTRONOMY 110G Review Questions for
ASTRONOMY 110G Review Questions for

... Summarize the basic differences between the Ptolemaic, Copernican, and Keplerian descriptions of planetary, solar, and lunar motions. Explain why our Moon exhibits phases. Describe them, and explain why they occur in the observed sequence. What are the synodic and sidereal months and why do they dif ...
GAYNES SCHOOL SCHEME OF WORK – SCIENCE
GAYNES SCHOOL SCHEME OF WORK – SCIENCE

... What is in the sky tonight? Show picture on tonight's night sky http://www.schoolsobservatory.org.uk/ What do you know? Sketch the solar system Is earth special? Day and night ...
the sun moon and the earth!
the sun moon and the earth!

... Sun What is the distance from the Sun to the Moon? 238,857 miles. What is the distance from the Sun to the Earth? 93,000,000 miles. How do the characteristics of the Sun affect life on the Sun? The Sun is so hot that it is impossible for there to be a living person on the Sun. Explain how day and ni ...
Ch 22-2
Ch 22-2

... • Phases of the moon • Solar eclipse • Lunar eclipse ...
Episode 24 - Vigyan Prasar
Episode 24 - Vigyan Prasar

... shadow of another moon. A binary star system can also produce eclipses if the plane of their orbit intersects the position of the observer. A lunar eclipse occurs when the moon enters Earth’s shadow. If the moon becomes completely immersed in the umbra, the dark shadow, the eclipse is termed total. ...
astronomy 31 - UNC Physics
astronomy 31 - UNC Physics

... Copernicus Galileo Kepler Ptolemy ...
History of Astronomy
History of Astronomy

... Copernicus • First Astronomer to theorize that Earth was revolving around the sun = heliocentric • Was not accepted until after his death • First book published on the day of his Death ...
Stars
Stars

... Observed motions of the Sun can be described if either 1) The Sun goes around the Earth once per day, or 2) The Earth rotates about its axis. ...
Lec2_2D
Lec2_2D

... If you’re on the edge of an eclipse path and only a slice of the Sun is blocked out, it’s called a partial eclipse. These are not very exciting, since the uneclipsed part of the Sun is still extremely bright. ...
The Earth - Eniscuola
The Earth - Eniscuola

... above our heads, and the revolution around the Sun in a slightly elliptical orbit. The two main units of time, days and years, derive respectively from the rotation and revolution movements. The length of a day can be measured as the time interval between two consecutive transits of the Sun or of a ...
Sir Isaac Newton was born in the same year that Galileo died. His
Sir Isaac Newton was born in the same year that Galileo died. His

... Sir Isaac Newton was born in the same year that Galileo died. His accomplishments include the development of the universal law of gravitation that explained the motion of the planets, comets, and the moon and the nature of light and He also developed calculus. Isaac Newton’s most famous and importan ...
Inverse Square Law
Inverse Square Law

... Gravitational Force is the mutual force of attraction between particles of matter This force always exists between two masses, regardless of the medium that separates them It is not just between large masses, like the sun and the Earth. The chair you are sitting on is attracted to the person next to ...
Solar System Review - answer key
Solar System Review - answer key

... They seem to rotate around Polaris because the axis of the Earth is pointed towards it. ...
Document
Document

... Why does the force of gravity between the Earth and the Moon seem to have a greater effect on the moon? Moon has less inertia, so it accelerates more ...
PPT: The Scientific Revolution
PPT: The Scientific Revolution

... act of thinking proved his own existence (I think, therefore, I am.) Challenges to Religion: The idea that the universe worked like a machine according to natural laws and without the intervention of God challenged established religious ideas. This position was adopted by the Deists in the 18th cent ...
solution
solution

... Since the Moon has no atmosphere, there is no scattering of light. This means that if you’re not looking at the Sun directly, there is nothing to cause the sunlight to be deflected to your eyes, so you see only the black of space (or other stars). On Earth, blue light scatters more easily than red, ...
Monday, October 20
Monday, October 20

... • Smaller than Earth • Density similar to that of the moon ...
Simple astronomy within the solar system
Simple astronomy within the solar system

... The two amateurs find that the second step necessary is to measure the velocity of the moon in its orbit about the center of the earth. They accomplish this indirectly by determining the times at which some particular star, as seen from two different points on the earth‘s surface, is eclipsed by the ...
Word - UW-Madison Astronomy
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 ...
PH109 Exploring the Universe
PH109 Exploring the Universe

... d) Jupiter was not perfect but had moving clouds of gas. 2) When Galileo viewed the Moon, what discovery helped change our view of the solar system? a) Because the Moon rises in the East and sets in the West, its orbit must be opposite that of the planets. b) The Moon went through phases like Jupite ...
Planets and Stars Study Guide Test Date: ______ Vocabulary to
Planets and Stars Study Guide Test Date: ______ Vocabulary to

... 3. What does a “new moon” look like? When do we usually have one? A new moon is when no light is being reflected because the earth’s shadow is blocking the sun. It is going to look similar to a full moon, but not as bright. We usually see a full moon 2 weeks after a new moon. ...
Jan. 14 – Jan. 21
Jan. 14 – Jan. 21

... Mystic (music of spheres/nested geometric shapes) Kepler’s Laws 1. elliptical orbits with sun at one focus 2. Sweep out equal areas in equal time 3. period (years) squared is equal to semimajor axis (A.U.) cubed Coined the word Satellite ...
chart_set_2 - Physics and Astronomy
chart_set_2 - Physics and Astronomy

... Aristotle: Sun, Moon, Planets and Stars rotate around fixed Earth. Aristarchus: Used geometry of eclipses to show Sun bigger than Earth (and Moon smaller), so guessed Earth orbits Sun. Also guessed Earth spins on axis once a day => apparent motion of stars. Difficulty with Aristotle's "Geocentric" m ...
Review for Exam I PHYS 1050
Review for Exam I PHYS 1050

... • Planetary Motions and Configurations –all planets orbit EASTWARD around the Sun –the further from Sun, the slower the angular speed of the planet in orbit –describe cause of retrograde motion, observed planetary phases –define configurations • inferior planets – conjunction »inferior ...
Homework #1 10 points Question #1 (2 pts) Even in ancient times
Homework #1 10 points Question #1 (2 pts) Even in ancient times

... Even in ancient times, astronomers knew that planets vary in brightness over the course of several months or even years. Explain, why this observation can not be used to rule out the geocentric model, in which all planets and the Sun orbit the Earth on circular orbits. Ignore the epicycles, i.e. ass ...
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Lunar theory

Lunar theory attempts to account for the motions of the Moon. There are many irregularities (or perturbations) in the Moon's motion, and many attempts have been made to account for them. After centuries of being problematic, lunar motion is now modeled to a very high degree of accuracy (see section Modern developments).Lunar theory includes: the background of general theory; including mathematical techniques used to analyze the Moon's motion and to generate formulae and algorithms for predicting its movements; and also quantitative formulae, algorithms, and geometrical diagrams that may be used to compute the Moon's position for a given time; often by the help of tables based on the algorithms.Lunar theory has a history of over 2000 years of investigation. Its more modern developments have been used over the last three centuries for fundamental scientific and technological purposes, and are still being used in that way.
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