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Planet Packets
Planet Packets

... 3. Earth’s surface is split into plates. What are these plates called? Earth’s plates are called tectonic plates. 4. Earth is larger that what other three planets? Earth is larger than Mercury, Venus and Mars. 5. List two facts of how Earth is different from other planets. Open answer. ...
The origin, life, and death of stars
The origin, life, and death of stars

... helium fusion shed much of their mass  The ejected material expands and cools, becoming a planetary nebula (which actually has nothing to do with planets, but we didn’t know that in the 18th century when Herschel coined the term)  The core collapses to form a White Dwarf ...
HAT-P-7: A RETROGRADE OR POLAR ORBIT, AND A THIRD BODY
HAT-P-7: A RETROGRADE OR POLAR ORBIT, AND A THIRD BODY

... In the solar system, the planetary orbits are well aligned and prograde, revolving in the same direction as the rotation of the Sun. This fact inspired the “nebular hypothesis” that the Sun and planets formed from a single spinning disk (Laplace 1796). One might also expect exoplanetary orbits to be ...
Mankind`s Purple Dawn
Mankind`s Purple Dawn

... and Chauvet and other parts of the world, a people whose artistic merits cannot be questioned and whose obvious knowledge of self cannot be denied. And in the same way that our modern interest in them belies a fascination with our origins as a species, could it also be that they too wondered from wh ...
Abstract - The University of Akron
Abstract - The University of Akron

... Long ago in mankind's past, some self-aware human looked up into the sky and was the first to wonder about a world larger than his own immediate environment. Up until that time, the ever-pressing survival needs of food, shelter, and protection exclusively dominated the early human's thought processe ...
Oct 2011 - Bays Mountain Park
Oct 2011 - Bays Mountain Park

... suggested the name Triton, who was Poseidon’s son, but this was not adopted officially until many years later. The next moon of Neptune was not discovered until 1949, so for many years Triton was also known simply as “the satellite of Neptune.” Most of what we know about Triton comes from the Voyager ...
ASTR-100 - Jiri Brezina Teaching
ASTR-100 - Jiri Brezina Teaching

... Tidal heating slows the bodies' rotation until it becomes tidally locked, and the tidal bulge does not change any more. Two (from many) examples of tidal heating: Moon’s rotation, originally faster than now (the Moon showed all sides earlier), has been tidally locked to the Earth since 3.5 bill. y. ...
PowerPoint
PowerPoint

... Planet Comparisons • Mercury, Venus, Earth, and Mars are crowded close to the Sun. • The four large planets– Jupiter, Saturn, Uranus, and Neptune– are widely spaced • Pluto tends to be in unusual space • Mostly circular orbits, except Mercury and Pluto • Orbits all lie in a plane • Size varies cons ...
ASTR-100 - Jiri Brezina Teaching
ASTR-100 - Jiri Brezina Teaching

... 1 Error! Reference source not found., Error! Reference source not found. Error! Reference source not found. 09 ASTRONOMY (Greek: astron = star; -nomos from Greek nemein = to arrange; Greek “astronomos” = star-arranger). The New Columbia Encyclopedia (4th edition of The Columbia Encyclopedia, Columbi ...
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Outline Question of Scale Planets Dance

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ECCENTRICITY PRACTICE
ECCENTRICITY PRACTICE

... A Newly Discovered Planet Scientists studying a Sun-like star named Ogle-Tr-3 discovered a planet that is, on the average, 3.5 million kilometers away from the star’s surface. The planet was discovered as a result of observing a cyclic decrease in the brightness of Ogle-Tr-3 every 28.5 hours. The ch ...
East Valley Astronomy Club
East Valley Astronomy Club

... they do, and why the Late Heavy Bombardment of the inner solar system occurred (and the structure and size of the Kuiper Belt, and Jupiter’s Trojan asteroids, etc., etc.). If true, the planets formed closer to the Sun, which speeds up their formation, but still not < 10 Myr. However, if the planets ...
Subunit 2 - UNIT NAME
Subunit 2 - UNIT NAME

... Illustrate the difference between “rotation” and “revolution”—have one student • CO 3, LO 2 stand up in the middle of the room and slowly turn in a circle (rotating). Then have another student walk around the spinning student (revolving). Ask the •2 volunteers class which student is revolving and wh ...
Planet Search Unit Overview Habitability Zone Around Other Stars in
Planet Search Unit Overview Habitability Zone Around Other Stars in

... weather allows life to exist. – B the range of distances from a star where a planet’s surface temperature is always above the freezing point of water. – C the range of distances from a star within which water could exist in liquid form on a suitably sized planet. ...
Search for Planets Lecture Notes
Search for Planets Lecture Notes

... climate would be Earth-like. • Venus is not in the habitable zone now, but it may have been in the past. • Venus is not in the habitable zone now, but in a few billion years from now it will be. ...
Voyage: A Journey through our Solar System Grades 5
Voyage: A Journey through our Solar System Grades 5

... Uranus’s rotation axis, however, is almost lying within its orbital plane. The cause of this unique feature is not certain, but it has been suggested that it was caused by an impact of a large object, such as a large asteroid or moon. Giant impacts like this were common during the early history of t ...
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Astro110-01 Lecture 7 The Copernican Revolution
Astro110-01 Lecture 7 The Copernican Revolution

... perfect, unchanging substance not found on the Earth. Copernicus challenged assumption 1, but not assumption 2. The Copernican model implicitly questions assumption 3 that the objects in the sky were made of special unchanging stuff: ◊ Since the Earth is just another planet, there will eventually be ...
Astronomy Exam Notes.docx
Astronomy Exam Notes.docx

... Saturn o Gaseous o Rings composed of ice, dust, small rocks o Many satellites “moons” (more than Jupiter) Uranus o Gaseous o Cold Neptune o Farthest “true” planet from the sun – 30 times farther from Sun than Earth is o Less noticeable rings o Space between Uranus and Neptune Kuiper Belt o Lies beyo ...
Feb 2017 - Astronomical Society of Northern New England
Feb 2017 - Astronomical Society of Northern New England

... each year, lasting about one day less than summer because the earth is now near its closest to the sun on its slightly elliptical orbit and therefor moving a little faster than in summer. Our average speed around the sun is 18.6 miles per second or about 67,000 mph. At that speed you could get all t ...
1. Uranus and Neptune
1. Uranus and Neptune

... Neptune, on the other hand, had been discovered in 1846, and it took 165 years to go around the Sun. By 1900 Neptune had gone only one-third the way around the Sun. For that reason it was safer to rely on the smaller errors in Uranus’s motion, rather than on what might eventually turn out to be larg ...
Zoom Astronomy - visit our webpage
Zoom Astronomy - visit our webpage

... Venus is the second planet from the sun in our solar system. It is the hottest planet in our Solar System. This planet is covered with fast-moving sulphuric acid clouds which trap heat from the Sun. Its thick atmosphere is mostly carbon dioxide. Venus has an iron core but only a very weak magnetic f ...
Notes 3 - 1 Notes 3: Formation of the solar system 3.1 Starting
Notes 3 - 1 Notes 3: Formation of the solar system 3.1 Starting

... Generally hydrogen, and helium are found in atomic form (as individual atoms), though hydrogen can also be found commonly as H2, it is usually most often observed in the galaxy as H I (neutral atomic form). Hydrogen and helium are thought to be originally from the Big Bang rather than as by-products ...
More on Stars and the Sky
More on Stars and the Sky

... objects appear stationary. Why? What is the typical parallax of a nearby star? Why is it not possible to measure the parallax better than 0.01” from ground based instruments, but can be done from space? What is the precession of the Earth. Which of the following would change due to precession celest ...
You in Outer Space Curriculum Map
You in Outer Space Curriculum Map

... Terrestrial planets share similar characteristics. 3. Saturn, Jupiter, Neptune, and Uranus are gaseous planets. They are very different from the terrestrial planets. 4. Each planet moves through space in a different manner. 5. Some planets have more moons than others. 6. Humans have been able to exp ...
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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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