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Size of Sun and Size of Planets
Size of Sun and Size of Planets

... our solar system. The Sun is over 93 million miles away from the earth. It’s light takes about 8 minutes to reach the earth. Without its heat and light there would be no life on our planet. A planet is a large body that shines by reflected light and travels in a stable path around a star. The Sun is ...
Lecture 1: The Universe: a Historical Perspective
Lecture 1: The Universe: a Historical Perspective

... Galileo Galilei Galileo (1564 – 1642); died year Newton was born ● first astronomical user of the telescope (1609); read about the Dutch invention (1608) and made his own ● published The Starry Messenger (1610) ● lunar surface full of irregularities ● Milky Way composed of faint stars ● four moons ...
A105 –Stars and Galaxies
A105 –Stars and Galaxies

... in terms of AU (1 AU = 1 astronomical unit, the average distance between the Earth and the Sun, about 150,000,000 kilometers). Again we will use the laws of orbital motion from Chapter 5. The formula is ...
Getting to Know: Rotation, Orbits, and the Seasons
Getting to Know: Rotation, Orbits, and the Seasons

... Misconception 1: Do all objects in the solar system rotate in the same direction? If viewed from above, most objects in the solar system rotate counterclockwise. Earth rotates toward the east, which is why the Sun “sets” in the west. Interestingly, Venus rotates in the opposite direction of Earth, a ...
Our Space Journey
Our Space Journey

... Uranus is the seventh planet from the sun. It' s not visible to the naked eye. Uranus make one trip around the sun every 84 earth days.Uranus is the coldest planet. Uranus is a gas planet. The whole of Uranus is covered with a think , blue green fog. One year on Uranus is the same as 84 earth days. ...
2b. Which of Kepler`s laws did this illustrate? (State the law – don`t
2b. Which of Kepler`s laws did this illustrate? (State the law – don`t

... 3. Imagine another solar system with a star of the same mass as the Sun. In this solar system there is a planet with a mass twice that of Earth orbiting at a distance of 1 AU from the star. What is the orbital period of that planet? Explain your answer based on what you observed in this activity. 4. ...
  To learn how the shape and period of...    To learn how the shape of the orbit... Gravity, Orbits and Kepler’s Laws
 To learn how the shape and period of...  To learn how the shape of the orbit... Gravity, Orbits and Kepler’s Laws

... 3. Imagine another solar system with a star of the same mass as the Sun. In this solar system there is a planet with a mass twice that of Earth orbiting at a distance of 1 AU from the star. What is the orbital period of that planet? Explain your answer based on what you observed in this activity. 4. ...
Earth Science Library wk 2 (WP)
Earth Science Library wk 2 (WP)

... Perhaps Galileo’s most striking discovery was the moons of Jupiter: Upon first observing Jupiter he noted four stars curiously in a line with Jupiter. Moved with Jupiter! Alternated between being east and west of the planet. How could this be explained? ...
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keplers laws and newton - Fort Thomas Independent Schools
keplers laws and newton - Fort Thomas Independent Schools

... Earth has less mass, less inertia, same gravitational force; thus, more easily accelerated ...
Excellence
Excellence

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Slide 1

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ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy
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... ●   Formation of the solar system was likely due to the Condensation Theory which follows that the planets were formed from a process of dust condensation, accretion and fragmentation. ●   The inner and outer planets are separated by the asteroid belt and among the Terrestrial and Jovian planets, th ...
ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy
ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy

... ● Formation of the solar system was likely due to the Condensation Theory which follows that the planets were formed from a process of dust condensation, accretion and fragmentation. ● The inner and outer planets are separated by the asteroid belt and among the Terrestrial and Jovian planets, there ...
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... – hypotheses that have withstood observational or experimental tests  Theory – a body of related hypotheses can be pieced together into a self consistent description of nature  Laws of Physics – theories that accurately describe the workings of physical reality, have stood the test of time and bee ...
Tayler Vence PHYS 1010 5/5/2013 The Copernican Revolution The
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... The book was hardly even touched or looked over for the next eighty years, until the Italian scientist Galileo Galilei took up an interest in planetary motions. With the utilization of the telescope (which was newly invented), he found convincing evidence that gave credibility to the Copernican mode ...
Unit Review Name
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... how development in one area leads to advancement in the other. You have taken part in a number of activities that required creative solutions to a variety of problems. Many of the activities have resulted in a number of different solutions for the same problem. These solutions may have involved diff ...
The Synodic and Orbit Periods of the Planets
The Synodic and Orbit Periods of the Planets

... Look up each planet's mean orbit radius (semimajor axis length) in millions of kilometers. Calculate the speed of each planet in km/hour from this radius and the time period P, assuming that its orbit is a circle in shape. Plot speed vs. planet number. Comment on the shape of the plot and why Copern ...
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Vagabonds of the Universe

... • Vagabond- a person with out a fixed home who moves from place to place and has no apparent means of support, wander… • These objects do have fixed homes…. ...
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1 The Synodic and Orbit Periods of the Planets

... Look up each planet's mean orbit radius (semimajor axis length) in millions of kilometers. Calculate the speed of each planet in km/hour from this radius and the time period P, assuming that its orbit is a circle in shape. Plot speed vs. planet number. Comment on the shape of the plot and why Copern ...
Scaling the SEM reading
Scaling the SEM reading

... 4.5 billion years. There are many theories about how the Moon was formed. Some astronomers think the Moon may have been formed when a Mars-sized asteroid collided with Earth about 100 million to 200 million years after Earth was formed approximately 4.5 billion years ago. The debris from that collis ...
Atmospheres in the Solar System • The speed at which molecules
Atmospheres in the Solar System • The speed at which molecules

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Decline of Western Civilization (extended) knowledge of ancient

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DO IT YOURSELF SIMPLE TEMPLATE FORMAT
DO IT YOURSELF SIMPLE TEMPLATE FORMAT

... Our Solar System consists of many types of objects circling around the Sun, held in their orbits by gravity. Name all of the objects you can think of that orbit the Sun. Write down what you know about each one. This activity will look specifically at planets, which are relatively large objects circl ...
Inner Planets Mercury
Inner Planets Mercury

... moons, their names are Deimos and Phobos ...
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Satellite system (astronomy)



A satellite system is a set of gravitationally bound objects in orbit around a planetary mass object or minor planet. Generally speaking, it is a set of natural satellites (moons), although such systems may also consist of bodies such as circumplanetary disks, ring systems, moonlets, minor-planet moons and artificial satellites any of which may themselves have satellite systems of their own. Some satellite systems have complex interactions with both their parent and other moons, including magnetic, tidal, atmospheric and orbital interactions such as orbital resonances and libration. Individually major satellite objects are designated in Roman numerals. Satellite systems are referred to either by the possessive adjectives of their primary (e.g. ""Jovian system""), or less commonly by the name of their primary (e.g. ""Jupiter system""). Where only one satellite is known, or it is a binary orbiting a common centre of gravity, it may be referred to using the hyphenated names of the primary and major satellite (e.g. the ""Earth-Moon system"").Many Solar System objects are known to possess satellite systems, though their origin is still unclear. Notable examples include the largest satellite system, the Jovian system, with 67 known moons (including the large Galilean moons) and the Saturnian System with 62 known moons (and the most visible ring system in the Solar System). Both satellite systems are large and diverse. In fact all of the giant planets of the Solar System possess large satellite systems as well as planetary rings, and it is inferred that this is a general pattern. Several objects farther from the Sun also have satellite systems consisting of multiple moons, including the complex Plutonian system where multiple objects orbit a common center of mass, as well as many asteroids and plutinos. Apart from the Earth-Moon system and Mars' system of two tiny natural satellites, the other terrestrial planets are generally not considered satellite systems, although some have been orbited by artificial satellites originating from Earth.Little is known of satellite systems beyond the Solar System, although it is inferred that natural satellites are common. J1407b is an example of an extrasolar satellite system. It is also theorised that Rogue planets ejected from their planetary system could retain a system of satellites.
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