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Chapter 16 - Follow “Ironmtn.wordpress.com”
Chapter 16 - Follow “Ironmtn.wordpress.com”

... Difficulty Level: Easy 18. An astronaut standing on Mars and attempting to look at Jupiter might have her view partly blocked by the intervening ...
Lec06_ch07_outerplanets
Lec06_ch07_outerplanets

... • Does Jupiter have continents and oceans? – No, Jupiter is comprised mainly of a dense mantle of liquid hydrogen and helium. There is a solid core at it’s center. ...
astro-ph/0507149 PDF
astro-ph/0507149 PDF

... Arc simulations showed multiple areas of enhanced concentration, which also encouraged binary formation as well as the appearance of retrograde orbits, which are inherently more unstable than are prograde orbits which can also result. Figures 5 and 6 show two such distinct populations for each set o ...
the orbits of neptune`s outer satellites
the orbits of neptune`s outer satellites

... All six known outer irregular satellites were easily recovered without knowing their precise positions within the two fields (Figure 1). Because the fields were off opposition, foreground asteroids and background Kuiper Belt Objects could mimic the motion of a Neptune satellite over a few hours. The ...
session 3.2 - Let There Be Night
session 3.2 - Let There Be Night

... it. Hans Lippershey, a Dutch spectacle maker, applied for the first patent in 1608, but two others—Jacob Metier and Zacharias Janssen, who were also Dutch spectacle makers—applied a short time later. They all claimed to have invented it first and accused the others of stealing the idea. The idea had ...
Standard Four: Earth in Space
Standard Four: Earth in Space

... be seen in the sky including the Sun, the Moon, stars, and manmade objects. 3. The Sun and Moon appear to move slowly across the sky. 4. The pattern of day and night repeats every 24 hours. The Sun can only be seen in the daytime. 5. The Moon can be observed sometimes at night and sometimes during t ...
swiss ephemeris - Welcome, but
swiss ephemeris - Welcome, but

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Orbital Perturbations of the Galilean Satellites During Planetary
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Year 7 Module 3 Practice Paper
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Did Saturn`s rings form during the Late Heavy Bombardment?
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... strong implications for the survival of the saturnian satellites: all satellites smaller than Mimas would have been destroyed during the LHB, whereas Enceladus would have had from 40% to 70% chance of survival depending on the disruption model. In conclusion, these results suggest that the LHB is th ...
Comet Catalina 2016 - Fraser Heights Chess Club
Comet Catalina 2016 - Fraser Heights Chess Club

... Comets formed at the same time our solar system did, 4.6 billion years ago, perhaps even in among the planets. By examining them up close with satellites and landers, scientists hope to learn more about what our Solar System looked like in its earliest days. ...
Our Solar System
Our Solar System

... © All rights reserved. Digital duplication, electronic transmission or posting of the contents contained, printing, photocopying, and/or distribution of copies of content is prohibited with the exception of the purchaser reproducing as many copies as necessary for use by their own family or single c ...
Asteroids and Comets and Meteors, Oh My!
Asteroids and Comets and Meteors, Oh My!

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Asimov, Isaac - Lucky Starr 05 - and the Moons of Jupiter
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The Voyager pictures show four additional faint rings. Saturn`s rings
The Voyager pictures show four additional faint rings. Saturn`s rings

PowerPoint
PowerPoint

... needed forces along the direction of the velocity, not perpendicular to it. • So Newton realized that like an apple falling from a tree or a really big tree, the moon must have a force toward the ...
Course Description: This is an introductory course in Descriptive
Course Description: This is an introductory course in Descriptive

PDF format
PDF format

... •  What are Saturn's rings like? –  They are made up of countless individual ice particles. –  They are extremely thin with many gaps. •  How do other jovian ring systems compare to Saturn's? –  The other jovian planets have much fainter ring systems with smaller, darker, less numerous particles. •  ...
orbital perturbations of the galilean satellites during planetary
orbital perturbations of the galilean satellites during planetary

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Ch 13 Death of Stars(4-5?-13)
Ch 13 Death of Stars(4-5?-13)

... • White Dwarfs: very dense, about mass of Sun in size of Earth. Atoms stop further collapse. M less than 1.4 solar masses • Neutron Stars: even denser, about mass of Sun in size of Orlando. Neutrons stop further collapse. M between 1.4 and 3 solar masses. Some neutron stars can be detected as pulsar ...
Ch. 13 Death of Stars(11-16-10)-3
Ch. 13 Death of Stars(11-16-10)-3

... • White Dwarfs: very dense, about mass of Sun in size of Earth. Atoms stop further collapse. M less than 1.4 solar masses • Neutron Stars: even denser, about mass of Sun in size of Orlando. Neutrons stop further collapse. M between 1.4 and 3 solar masses. Some neutron stars can be detected as pulsar ...
Hands On Astronomy
Hands On Astronomy

... surprised at how far apart the two objects are? What’s Going On? Most people are very surprised when they see the scaled size and distance between the earth and the moon. Studies of the astronomy misconceptions held by students (and even adults!) reveal that most people believe that the moon is much ...
Chapter 13
Chapter 13

... Internal Structure Magnetic fields of Uranus and Neptune must not be produced by dynamos, as the other planets’ fields are Interior structure of Uranus and Neptune, compared to that of Jupiter and Saturn ...
Dark Matter In The 21st Century
Dark Matter In The 21st Century

... 2) Coma cluster is not in equilibrium are needed to see this picture. (galaxies are in the process of flying apart) ...
Jupiter – friend or foe? III: the Oort cloud comets
Jupiter – friend or foe? III: the Oort cloud comets

... massless particles, and were unable to gravitationally interact with each other. They felt the gravitational influence of the Sun, Jupiter and Saturn, but did not exert any force on those bodies. Whereas in Papers I and II we counted the number of collisions on an (inflated) Earth, for the Oort clo ...
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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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