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Our Solar System
Our Solar System

... The Greeks also noticed that while the stars move across the sky, their patterns do not change. But five points of light did move among the stars. The Greeks called these objects planets, which means “wandering star.” They made careful observations of these planets, which we call Mercury, Venus, Mar ...
Wind Patterns - Mrs. Shaw's Science Site
Wind Patterns - Mrs. Shaw's Science Site

... SMALLER OBJECTS IN SPACE Most small objects are found in three areas: •Asteroid belt- region of the solar system between Jupiter and Mars. •Kuiper belt- extends to about 100 times Earth’s distance from the sun. •Oort cloud- stretches out more than 1,000 times the distance between the sun and Neptun ...
Kinesthetic Astronomy: Earth`s Rotation
Kinesthetic Astronomy: Earth`s Rotation

... Many people have a hard time interpreting drawn diagrams and understanding how the earth moves in relationship to the sun. In a 2008 California Academy of Sciences Survey we discovered that many adults don’t know that the earth takes 365 days to travel around the sun. This concept was also shown in ...
The Science of Astronomy 3.1 Multiple
The Science of Astronomy 3.1 Multiple

... D) the fine line between science and pseudoscience E) the shaving implement of a medieval scholar Answer: C 44) Which of the following statements about scientific theories is not true? A) A theory cannot be taken seriously by scientists if it contradicts other theories developed by scientists over t ...
Earth-Moon-Sun Answer Key
Earth-Moon-Sun Answer Key

... Answer Key MEAP-like practice questions formally released items from Oakland Schools. S.IP.04.11 Your teacher asked you to look at the moon for a few minutes a day for 5 days. Which sentence is an observation you may make from this lesson? A. The moon circles the Earth. B. The moon spins as it trave ...
Astronomical distances and Stellar magnitudes
Astronomical distances and Stellar magnitudes

... 1. What is meant by a light year? 2. What is meant by an astronomical unit (AU)? 3. What is meant by a parsec (pc)? 4. What is meant by a mega parsec (Mpc)? 5. What is meant by the apparent magnitude of an astronomical object? 6. Give the approximate distance of the following in AU: (a) Sun to the E ...
File - Mrs. Ratzlaff
File - Mrs. Ratzlaff

... Comets are also a part of our solar system. They are often called __________ __________. Comets are small _______ bodies containing __________, __________ , carbon dioxide, ammonia and methane. Like planets, comets also ________ the Sun, but their orbits run ______________ to the planets’ orbits. Th ...
Digital Moon - Net Start Class
Digital Moon - Net Start Class

... Weather for $500 A class is planning a trip to the beach. They would like to choose a day that will be the most sunny yet have a lower temperature for the daily high. Based on this five-day prediction, which day should they ...
ASTR100 Class 01 - University of Maryland Astronomy
ASTR100 Class 01 - University of Maryland Astronomy

... decays into argon-40 every 1.25 billion years. You open the rock and find 3 atoms of argon-40 for every 1 atom of potassium-40. How old is the rock? A. 1.25 billion years. B. 2.5 billion years. C. 5 billion years. D. It is impossible to determine. ...
Final Exam Space Unit Review
Final Exam Space Unit Review

... Azimuth: angle clockwise from North, the direction we must face to see the star (i.e. 180oS or “at an azimuth of 180oS). Azimuth coordinates MUST have degrees PLUS direction.  Do the 3 practice problems on pg. 359 and the Alt-Azimuth Coordinates Practice Sheet (BLM 5Draw and label “altitude” and “a ...
Galileo, Newton and Gravity 1/31
Galileo, Newton and Gravity 1/31

... could be the center of motion); there were many more stars, mountains on moon  Book Starry Messenger • Venus had definite phases and clearly orbiting Sun • Observed sunspots (patches on Sun). Sun revolved on own axis. Wasn’t “perfect” and changes in unpredictable manner • Observed Saturn’s rings bu ...
Chpt 26- Studying Space:
Chpt 26- Studying Space:

... • Explain how the change in apparent positions of constellations provides evidence of Earth’s rotation and revolution around the sun. • Summarize how Earth’s rotation and revolution provide a basis for measuring time. • Explain how the tilt of Earth’s axis and Earth’s movement cause seasons. The Rot ...
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... Base your answers to question 5 on the diagram in below. The diagram shows Earth revolving around the Sun. Letters A, B, C, and D represent Earth’s location in its orbit on the first day of the four seasons. Aphelion (farthest distance from the Sun) and perihelion (closest distance to the Sun) are l ...
moon earth sun - Conrad Public Schools
moon earth sun - Conrad Public Schools

... The pull of Earth’s gravity while the moon was still molten pulled the denser parts towards Earth This makes the moon egg shaped with the pointy end towards Earth The crust is the least dense portion and it is 60km thick on the Earth side and 100km thick on the backside The gravity also pulled the h ...
ASTR 2310: Chapter 2
ASTR 2310: Chapter 2

... Early Greek Astronomy ...
PDF format - Princeton University Press
PDF format - Princeton University Press

... on to Alexandria, which became the center of Hellenistic culture for several centuries.2 Unfortunately, although that golden age saw great advances in observational astronomy and mathematics, physics did not keep pace with these sciences. Thus, lacking a firm theoretical base and constrained by meta ...
Midterm exam
Midterm exam

... 24. At the time of the Summer Solstice (the start of summer) the Sun is a. Farthest south of the celestial equator. b. Farthest north of the celestial equator. c. On the celestial equator moving north. d. On the celestial equator moving south. 25. The Sun’s position in space is best described as th ...
Friday Feb 25th, 2000
Friday Feb 25th, 2000

... period = against the stars) ~ month – Similar to a woman’s cycle – Luna always a female association in all cultures ...
Power Point Version
Power Point Version

... period = against the stars) ~ month – Similar to a woman’s cycle – Luna always a female association in all cultures ...
the earth in space - North Salem Schools Teachers Module
the earth in space - North Salem Schools Teachers Module

... a. model was the product of Ptolemy - celestial objects revolved westward around the Earth b. outer planets moved on an epicycle while the epicycle followed a deferent c. it does explain what you see in the nighttime sky - it could be correct d. it does NOT account for terrestrial motions and phenom ...
Ancient Astronomy - Sierra College Astronomy Home Page
Ancient Astronomy - Sierra College Astronomy Home Page

...  Invented the latitude and longitude system  Wrote a book on astronomy – megisth – Often referred to as Almagest = “The Greatest” – Contained improved methods to find distance to the Sun and Moon – May have taken some ideas from Hipparchus ...
Planets and Stars Key Vocabulary: Comparing and Contrasting
Planets and Stars Key Vocabulary: Comparing and Contrasting

... There are more stars in the sky than a person can count one-at-a-time during an entire lifetime. There is just one star in our solar system - the sun. The sun is a medium-sized star, but it appears larger than other stars because it is so close to Earth. ...
THE 3-D UNIVERSE CONCEPTS
THE 3-D UNIVERSE CONCEPTS

... It is impossible to determine the distance to a star using your eyes alone. You are able to judge the distance to nearby objects because each eye views them from a different angle. Your brain combines these two perspectives to give you a 3-D view of the world, which allows you to judge distances up ...
brock university answers
brock university answers

... (b) 1 month (c) 1 year (d) 365.25 years (e) 200 million years 6. Geological evidence shows that the interior of the Earth is (a) much colder than its surface. (b) about the same temperature as its surface. (c) * much hotter than its surface. (d) [It’s impossible to tell from geological evidence.] 7. ...
Cosmic Distance Ladder
Cosmic Distance Ladder

... • Kepler’s third law give only the ratios of the distances: P2=ka3 • Although by the 17th century astronomers could calculate each planet's relative distance from the Sun in terms of the distance of the Earth from the Sun, an accurate absolute value of this distance had not been calculated. ...
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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 ↑
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