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11.2-11.3 PPT
11.2-11.3 PPT

... Formation of the Solar System Our solar system was formed more than 4.5 billion years ago. As the Sun burst into existence, the leftover material combined to form eight planets and numerous other planetary bodies: moons, asteroids, and comets. Closest to the Sun are the inner planets (terrestrial p ...
13.14 The Eight Planets
13.14 The Eight Planets

... Venus is the brightest object that we can see in the sky because it is so close to our planet Earth. Also, the atmosphere on Venus is very thick and the light it receives from the Sun is reflected to us. Venus’s atmosphere is made up from mainly carbon dioxide. This gas acts like the glass of a gree ...
Day-7
Day-7

... appear to move counterclockwise around the stationary North Star ...
Quantities every Physicist should know
Quantities every Physicist should know

... No calculators or tables of constants allowed. Pencil & paper encouraged. Answers are to be given either (i) in the form 10x , where x is integer or half integer, that is give log10 (answer), rounded to nearest half integer. This therefore accommodates answers like 1 × 105 or 3 × 1015 , since 3 ∼ 10 ...
Name the eight planets in order by increasing distance from the sun:
Name the eight planets in order by increasing distance from the sun:

... A: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune 2. What are two pieces of technology that have helped scientists explore the solar system? A: space shuttles, probes, telescopes 3. What two things combine/balance to keep planets in orbit around the sun? (as opposed to spiraling into ...
models
models

... But, since it was not permissible to ignore, those eight minutes pointed the road to a complete reformation in ...
Earth Science - Montville.net
Earth Science - Montville.net

... 8. Gather objects such as a golf ball, walnut, tennis ball, golf ball, etc. to compare/contrast the differences in size of the planets using ordinary objects. 9. Compare the sizes of the planets using a Venn diagram. Show how they are alike and how they are different. 10. Show makemegenius.com video ...
"WITH THE STARS" i - Royal Astronomical Society of Canada
"WITH THE STARS" i - Royal Astronomical Society of Canada

... much. This is still more than 3 times as ~ The Sun's Family much as all the other planets put together. It revolves around the Sun in just under 12 The Earth is one of 9 planets, dark solid of our years, and spins QIIl. its axis in less than bodies which revolve in elliptical (roughly 10 hours; henc ...
The Motions of Celestial Bodies, and Newton`s Laws of Motion
The Motions of Celestial Bodies, and Newton`s Laws of Motion

... 4. Because we are at the center of the Universe ...
solar-sy - WordPress.com
solar-sy - WordPress.com

... The reason for the seasons is not how close the earth is to the sun but the tilt of the earth. When the northern Hemisphere is tilted away from the sun (indirect sun light –spread out) it is our winter and when the northern hemisphere is tilted toward the sun (direct sunlight – more focused) it is o ...
Gravity and Orbits
Gravity and Orbits

... 1. Find the orbital period and speed of a satellite orbiting Earth at an altitude of 1800 km 2. A moon orbits planet Y in a circular path with a radius of 9600 km. If it takes 137 minutes to complete one orbit, find a) the acceleration , b) the mass of planet Y c) If planet Y has a radius of 5600 km ...
File
File

... years, which ought to allow plenty of time for the planets around them to evolve a life-form or two, but their habitable zones fall very close to the host star. A planet that forms there will swiftly become tidally locked and always show the same face toward the star (just as the Moon always shows t ...
Gravity in the Solar System Quiz
Gravity in the Solar System Quiz

... 9) If you are on the top of a mountain and drop an apple, it will fall to the ground, even though the apple is gravitationally attracted to you. Why? a) Earth is larger and has a much stronger gravitational pull. b) Apples always fall down. c) Centrifugal forces pull the apple to the Earth and that ...
Homework 2
Homework 2

... Earth is closer to the Sun in January than in July. Therefore, in accord with Kepler’s second law: (a) Earth travels faster in its orbit around the Sun in July than in January. (b) Earth travels faster in its orbit around the Sun in January than in July. (c) It is summer in January and winter in Jul ...
ch 2 the sky
ch 2 the sky

... Precession causes Earth’s axis to sweep around a cone with a period of 26,000 years, and that changes the location of the seasons around Earth’s orbit  Northern winters now occur when Earth is 1.7% closer to the sun, but in 13,000 northern winters will occur on the other side of Earth’s orbit where ...
Planets in the sky
Planets in the sky

... • Motion of planets very important in historical context of how we came to figure out the nature of the Solar System ...
Seasons
Seasons

... Great Pyramid and Thuban, the closest star to the rotational axis of the earth in 4420 B.C. • Betelguese, which marked the Vernal Equinox is also aligned with the southern shaft in the King’s chamber. • And others… ...
Earth`s Rotation
Earth`s Rotation

... Shade this diagram – leave the intended path (the straight arrows) black. Highlight the apparent path (the curved arrows). The apparent path of motion (the curved arrows) shows the Coriolis Effect – proof that Earth is rotating. ...
Celestial Sphere Lab
Celestial Sphere Lab

... The Earth rotates once every 24 hours. Since it makes a complete circle in that time, we can say that 360 degrees = 24 hours. How many degrees are there in one hour? _________ degrees = 1 hour Because the number of degrees and the number of hours can be set equal to each other, astronomers say that ...
Dead Earth – Lesson 2 – Solar System
Dead Earth – Lesson 2 – Solar System

... similarly sized objects had been found, but not classified as planets • These include the largest known asteroid - ‘Ceres’ and a large object beyond Pluto ‘Eris’ ...
Inner Planets
Inner Planets

... rotates in the opposite direction of the Earth. Looking from the north, Venus rotates clockwise, while the other planets rotate counterclockwise. Earth rotates in 24 hours and orbits the sun in 365 days. The planet Mars spins slowly. Its rotation of 1 day would be 176 Earth days. ...
Inner and Outer Planets
Inner and Outer Planets

... (primarily hydrogen & helium; smaller solid or liquid core). • They are very light for their size. • They move quickly in space. • They have rings and many moons. • They have a diameter of less than 48,000 km ...
WK8revised
WK8revised

... “Perhaps the greatest anomaly in this situation is the incredibly weak scientific case for the whole scenario of cosmic evolution. There can be no "experiments" or "observations" of stars evolving, in the very nature of the case, so it cannot be scientific, though it may be naturalistic - all based ...
7.1 Space Flight to the Stars
7.1 Space Flight to the Stars

... We will discuss our solar system in more detail later in this unit, but here is a brief overview: -A series of planets and celestial objects orbit around the Sun because of the Sun’s gravitational attraction -There are two parts to the solar system: Inner and Outer Solar ...
A time exposure photograph was taken for 8 hours. During that time
A time exposure photograph was taken for 8 hours. During that time

... North Pole than the equator WHY?- Closer to Earth’s center on Poles so force of gravity is greater ...
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Geocentric model



In astronomy, the geocentric model (also known as geocentrism, or the Ptolemaic system) is a description of the cosmos where Earth is at the orbital center of all celestial bodies. This model served as the predominant cosmological system in many ancient civilizations such as ancient Greece including the noteworthy systems of Aristotle (see Aristotelian physics) and Ptolemy. As such, they believed that the Sun, Moon, stars, and naked eye planets circled Earth.Two commonly made observations supported the idea that Earth was the center of the Universe. The stars, the sun, and planets appear to revolve around Earth each day, making Earth the center of that system. The stars were thought to be on a celestial sphere, with the earth at its center, that rotated each day, using a line through the north and south pole as an axis. The stars closest to the equator appeared to rise and fall the greatest distance, but each star circled back to its rising point each day. The second observation supporting the geocentric model was that the Earth does not seem to move from the perspective of an Earth-bound observer, and that it is solid, stable, and unmoving.Ancient Roman and medieval philosophers usually combined the geocentric model with a spherical Earth. It is not the same as the older flat Earth model implied in some mythology, as was the case with the biblical and postbiblical Latin cosmology. The ancient Jewish Babylonian uranography pictured a flat Earth with a dome-shaped rigid canopy named firmament placed over it. (רקיע- rāqîa').However, the ancient Greeks believed that the motions of the planets were circular and not elliptical, a view that was not challenged in Western culture until the 17th century through the synthesis of theories by Copernicus and Kepler.The astronomical predictions of Ptolemy's geocentric model were used to prepare astrological and astronomical charts for over 1500 years. The geocentric model held sway into the early modern age, but from the late 16th century onward was gradually superseded by the heliocentric model of Copernicus, Galileo and Kepler. There was much resistance to the transition between these two theories. Christian theologians were reluctant to reject a theory that agreed with Bible passages (e.g. ""Sun, stand you still upon Gibeon"", Joshua 10:12 – King James 2000 Bible). Others felt a new, unknown theory could not subvert an accepted consensus for geocentrism.
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