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1 Lecture 8: Uranus and Neptune
1 Lecture 8: Uranus and Neptune

Pluto, the dwarf planet
Pluto, the dwarf planet

... Pluto's moons are named for other mythological figures associated with the underworld. Charon is named for the river Styx boatman who ferries souls in the underworld — as well as honoring Sharon, the wife of discoverer James Christy. Nix is named for the mother of Charon, who is also the goddess of d ...
Gravitational Field
Gravitational Field

... attracted to the star with only onefourth the force (inverse square law). Since the force is the same for both, the mass of the farthermost satellite must be four times as great as the mass of the closer satellite. ...
Lecture 5: Saturn, Neptune, … A. P. Ingersoll  1
Lecture 5: Saturn, Neptune, … A. P. Ingersoll 1

... 7.
Saturn’s
winds
measured
in
1980
and
2004.
Maybe
some
change
at
the
equator,
 but
that
might
be
due
to
change
in
cloud
height
coupled
with
vertical
wind
shear.
 The
westward
jet
at
35
degrees
South
has
been
the
most
active
during
the
past
four
 years.
Winds
are
measured
relative
to
a
rotating
refe ...
No Slide Title
No Slide Title

... as Earth, even close-in • As orbital period increases, the Doppler Wobble method becomes insensitive to planets less massive than Jupiter • The length of time that the DW surveys have been active (since 1989) sets the upper orbital period limit – But imaging surveys can find the widest planets ...
HERE - Montana State University Extended University
HERE - Montana State University Extended University

... of liquid water on a planet’s surface. This suggests we should first search for a planet that rests in orbit around a Sun-like star (classes F, G or K) within the star’s zone of habitability. In addition to the distance from the star, the planet must also have a suitable atmosphere. This requires th ...
Document
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... ISP 209 -- 3B ...
Is our solar system unique?
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... • Look at our own solar system, and think about how it might have formed • Look at other solar systems while they form • Look for and study other solar systems • Create computer models and see if you can produce a solar system ...
How did the Solar System form?
How did the Solar System form?

... •  Look at our own solar system, and think about how it might have formed •  Look at other solar systems while they form •  Look for and study other solar systems •  Create computer models and see if you can produce a solar system ...
The Jovian Planets
The Jovian Planets

... Umbriel, Titania, Oberon); now 22 more are known (total ...
Isaac Newton and the Laws of Motion and Gravitation 2
Isaac Newton and the Laws of Motion and Gravitation 2

... Five planets (“wandering stars”) were known since antiquity. ...
Jupiter – friend or foe? II: the Centaurs Accepted for publication in
Jupiter – friend or foe? II: the Centaurs Accepted for publication in

... the tabulated data that the rate at which the objects are removed from the Solar System increases with the mass of Jupiter. The value of Nejected has been adjusted to take account of the fact that, in each of the runs, 883 of the initial population of objects were placed on orbits so eccentric that ...
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02_LectureOutline

... Astronomical unit: mean distance from Earth to Sun First measured during transits of Mercury and Venus, using triangulation ...
2011 - Edexcel
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... 8 A group of students were observing the Perseid meteor shower that occurs annually in August. This shower is caused by a short-period comet. (a) Where is the origin of most short-period comets? ...
The Gas Giants Astronomy Lesson 13
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... and more massive than Earth, and they do not have solid surfaces. Because these planets are so large and composed of gases, they are commonly referred to as the gas giants. Like the sun, the gas giants are comprised of mainly hydrogen and helium. Because they are so massive, the gas giants have a mu ...
AE Module 5 Presentation
AE Module 5 Presentation

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... Objective 2: Describe the appearance and apparent motion of groups of stars in the night sky relative to Earth and how various cultures have understood and used them. a. Locate and identify stars that are grouped in patterns in the night sky. b. Identify ways people have historically grouped stars i ...
Concepts and Skills
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... than did the mass of the planet. Newton generalized from his thinking about planets to formulate his law of universal gravitation. The law says that every body in the universe attracts every other body in the universe with a force that varies directly with the product of the masses and inversely wit ...
Planet Presentation
Planet Presentation

... Something Special: Is there anything special about your planet? This can often be the best part of the report, taking you off on interesting topics. For example, are there 100-year-long storms on your planet? Are there giant volcanos? Does your planet have a very tilted axis (giving it extreme seaso ...
Astronomy 07 Life in the Universe Final Exam Test Bank Homework
Astronomy 07 Life in the Universe Final Exam Test Bank Homework

... 31. The heavy bombardment occurred A) five times in the last 570 million years B) at the end of the Cretaceous, and the beginning of the Tertiary C) several times, at more or less regular intervals throughout the Hadean and Archaean D) during much of the Hadean E) only during a short spike at the en ...
July 2014 BRAS Newsletter - The Baton Rouge Astronomical Society
July 2014 BRAS Newsletter - The Baton Rouge Astronomical Society

... also quantified the fraction of planets that might have been missed by their census, either because the planes of their orbits were tilted so the planets could not transit the host star as seen from Earth, or those that the TERRA software itself could have missed. Shedding (the right amount of) ligh ...
The Jovian Planets - Sierra College Astronomy Home Page
The Jovian Planets - Sierra College Astronomy Home Page

... Umbriel, Titania, Oberon); now 22 more are known (total ...
Reflected Light From Extra Solar Planets
Reflected Light From Extra Solar Planets

... • No reflected light from extra solar planets detected to date, however the albedo of τ Boo constrained by lack of signal (Charbonneau et al.,1999, ApJ, 522, L145). ...
Timeline, Topics, and Resources for iMovie Projects
Timeline, Topics, and Resources for iMovie Projects

... natural circular motion, since that is the simplest uniform motion that repeats itself endlessly, as their motion did. However, although the "fixed stars" did in fact move in simple circles about the North star, the sun, moon and planets traced out much more complicated paths across the sky. These p ...
PLANETS
PLANETS

... solar system. Only a minority of the nearby stars are so young. Even for them, planets— and particularly those in the terrestrial planet/asteroidal region—are faint and are lost in the glare of their central stars. However, when bodies in this zone collide, they initiate cascades of further collisio ...
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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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