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In the beginning… Astronomical Observations of Star Formation
In the beginning… Astronomical Observations of Star Formation

... such as sulfur, lead, and indium. Planetesimal accretion took place before these elements could condense.  Final assembly of the terrestrial planets took longer and was not complete until gas had cleared from inner solar system. ...
Quick facts #1: Orbital motion
Quick facts #1: Orbital motion

... where m1 and m2 are the masses of the two bodies and r is motion: their separation. This is Newton’s Universal Law of Gravitation, and dominates motion in the large-scale Universe. Kepler 1 A planet orbits the Sun in an ellipse, with the Sun The subsequent motion of each body can take the form of a ...
HERE - Gallopade International
HERE - Gallopade International

... January 17: The evening sky was clear and the moon had not yet come up. I could see the Evening Star shining brightly on the horizon. However, the Evening Star is not a star at all—it is the planet Venus! From Earth, a planet in our solar system might look like a star, but a planet does not ”twinkle ...
NEXT MEETING THURSDAY, 18 th October 2012
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... landed on October 22, 1975, and sent back the first black and white images of the surface of Venus. It survived for 53 minutes before being destroyed by the heat and pressure. Venera 11 and 12 recorded 143 gamma-ray bursts between them on the way to Venus and on December 21, 1978 Venera 12 recorded ...
Scaling the Solar System
Scaling the Solar System

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The Motion of Celestial Bodies
The Motion of Celestial Bodies

... Kepler’s laws of planetary motion and Newton’s laws of universal gravity are presented. It is shown that the orbit of a body moving under the gravitational attraction of another body can be represented by a conic section. The six orbital elements are defined, and it is indicated how they can be dete ...
Planets
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Cosmology questions (Introduction)

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Formation of the Solar System
Formation of the Solar System

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The Motion of Celestial Bodies
The Motion of Celestial Bodies

... Kepler’s laws of planetary motion and Newton’s laws of universal gravity are presented. It is shown that the orbit of a body moving under the gravitational attraction of another body can be represented by a conic section. The six orbital elements are defined, and it is indicated how they can be dete ...
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... traveled daily around the Earth called the celestial sphere. • The Greeks also believed that all heavenly bodies remained in the same relative position to one another, except the seven “wanderers” which were: the sun, the moon, Mercury, Venus, Mars, Jupiter, and Saturn. ...
The History of Astronomy
The History of Astronomy

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... 3. Planetesimals begin to form within the swirling disk. 4. As the largest planetesimals grown in size, their gravity attracts more gas and dust. 5. Smaller planetesimals collide with the larger ones, and planets begin to grow 6. A star is born, and the remaining gas and dust are blown out of the ne ...
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astrofe –astronomy ofe

... • Because the force of gravity at the surface of an object is the result of the object's mass and size, the surface gravity of the moon is only one-sixth that of the Earth. The force gravity exerts on a person determines the person's weight. Even though your mass would be the same on Earth and the m ...
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... The Solar System is often portrayed as a line of planets, closely packed to each other. But this picture is misleading! There is a lot of space in space! Astronomical distances are measured in km and in Astronomical Units (AU). 1 AU is 149,600,000km and is the same distance between the Sun and the E ...
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Stephen John Kortenkamp - Lunar and Planetary Laboratory | The

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Angular Momentum

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... Once The Sky is open, go to Data → Location and confirm the location is Seattle, Washington (if not, you can choose this from the predefined list). Next go to Data → Time and set the time for 9 p.m. tonight. If you have time, you may wish to play with some of the following controls: on the second li ...
EARTH IN THE UNIVERSE TOPIC 3 2011-2012
EARTH IN THE UNIVERSE TOPIC 3 2011-2012

... At that very moment, unknown to the audience, an asteroid named Hermes halfway between Mars and Jupiter was beginning a long plunge toward our planet. Six months later it would pass 300,000 miles from Earth’s orbit, only a little more than the distance to the Moon…. Hermes approaches Earth’s orbit t ...
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Chapter 8 Formation of the Solar System Agenda What properties of

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Picture File - WordPress.com
Picture File - WordPress.com

... 4. Objects in the sky move in regular and predictable patterns. As a basis for understanding this concept: B. Students know the way in which the Moon’s appearance changes during the four-week lunar cycle. ...
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PowerPoint Presentation - Planetary Configurations

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Earth and Space

... It is approximately 100 light years in diameter. All objects in the Galaxy revolve around the ...
The Roots of Astronomy
The Roots of Astronomy

... philosophers to realize that ideas must be proven with empirical evidence. • He realized that more data meant more certainty in the idea or model ...
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Definition of planet



The definition of planet, since the word was coined by the ancient Greeks, has included within its scope a wide range of celestial bodies. Greek astronomers employed the term asteres planetai (ἀστέρες πλανῆται), ""wandering stars"", for star-like objects which apparently moved over the sky. Over the millennia, the term has included a variety of different objects, from the Sun and the Moon to satellites and asteroids.By the end of the 19th century the word planet, though it had yet to be defined, had become a working term applied only to a small set of objects in the Solar System. After 1992, however, astronomers began to discover many additional objects beyond the orbit of Neptune, as well as hundreds of objects orbiting other stars. These discoveries not only increased the number of potential planets, but also expanded their variety and peculiarity. Some were nearly large enough to be stars, while others were smaller than Earth's moon. These discoveries challenged long-perceived notions of what a planet could be.The issue of a clear definition for planet came to a head in 2005 with the discovery of the trans-Neptunian object Eris, a body more massive than the smallest then-accepted planet, Pluto. In its 2006 response, the International Astronomical Union (IAU), recognised by astronomers as the world body responsible for resolving issues of nomenclature, released its decision on the matter. This definition, which applies only to the Solar System, states that a planet is a body that orbits the Sun, is massive enough for its own gravity to make it round, and has ""cleared its neighbourhood"" of smaller objects around its orbit. Under this new definition, Pluto and the other trans-Neptunian objects do not qualify as planets. The IAU's decision has not resolved all controversies, and while many scientists have accepted the definition, some in the astronomical community have rejected it outright.
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