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Solar System Mobile Activity - Lunar and Planetary Institute
Solar System Mobile Activity - Lunar and Planetary Institute

... Just guess my name to start this game, then you may surely enter…… I orbit fast, but s l o w l y turn, With a 1,416 hour day! I’m the first. My name is __________________, I’m small and I am gray. Because my ghastly atmosphere is mainly CO2, It’s like a scorching greenhouse of 900 degrees. It’s true ...
Ch. 23: “Touring Our Solar System”
Ch. 23: “Touring Our Solar System”

... The centrifugal force of this rotation flattens it out into a rotating disk with a protostar at the center. The nebula is hot because of gravitational energy released by the collapse, and when the protostar ignites at the centre it produces more heat. So there is a strong temperature gradient across ...
Homework #1 - Department of Physics and Astronomy
Homework #1 - Department of Physics and Astronomy

... There is really no need for a calculation for this problem. The synodic periods of Jupiter and Venus are given in Appendix 3. It is important to note that the synodic period of the Earth as seen from Jupiter is equal to the synodic period of Jupiter as seen from the earth. Since we are talking about ...
.~ Observing the Solar System
.~ Observing the Solar System

... able to work out the arrangement of the known planets and how they move around the sun. Galileo used the newly invented telescope to make discoveries that supported the heliocentric model. Kepler found that the orbit of each planet is an ellipse. • A system in which the sun is at the center is calle ...
Acquaintance with solar system. By Edgaras Montvila 6D
Acquaintance with solar system. By Edgaras Montvila 6D

... giant planet. Surface temperature varies from –108 °C to?°C. Jupiter has been called the Solar System’s vacuum cleaner, because of its immense gravity well and location near the inner Solar System. It receives the most frequent comet impacts of the Solar System’s planets. Jupiter has 67 satellites. ...
Orbits of the planets - University of Iowa Astrophysics
Orbits of the planets - University of Iowa Astrophysics

... far from the Sun. • In Ptolemy’s model, Venus and the Sun must move together with the epicycle of Venus centered on a line between the Earth and the Sun • Then, Venus can never be the opposite side of the Sun from the Earth, so it can never have gibbous phases – no “full Venus”. ...
Diapositiva 1 - Yale University
Diapositiva 1 - Yale University

... all suns, each with its own planets. Bruno saw a Solar System of a sun/star with planets as the fundamental unit of the universe. According to Bruno, infinite God necessarily created an infinite universe, formed of an infinite number of solar systems, separated by vast regions full of Aether, becau ...
AIM: What is Astronomy? Do Now:
AIM: What is Astronomy? Do Now:

... AIM: What is Astronomy? Do Now: Answer the following question in your notebook. ...
DIRECTIONS - Cloverleaf Local
DIRECTIONS - Cloverleaf Local

... • Read ALL of the following questions that have already been created. ...
Powerpoint - BU Imaging Science
Powerpoint - BU Imaging Science

... the Sun. Most are found in the asteroid belt between Mars and Jupiter. There are many asteroids. • Comets are small, icy bodies that orbit the Sun. Comets have very elliptical orbits, only becoming visible when they form tails in the inner solar system. There are many comets. ...
Our Planetary System (Chapter 7)
Our Planetary System (Chapter 7)

... the Sun. Most are found in the asteroid belt between Mars and Jupiter. There are many asteroids. • Comets are small, icy bodies that orbit the Sun. Comets have very elliptical orbits, only becoming visible when they form tails in the inner solar system. There are many comets. ...
Inventory of the Solar System
Inventory of the Solar System

... Composed largely of ices--- water ice, ammonia ice, methane ice--mixed with dust Inhabit two distinct regions of space: Kuiper Belt and Oort cloud. ...
The New Dwarf Planet and Plutoids
The New Dwarf Planet and Plutoids

... as a large celestial body orbiting a star. It is nearly round, has its own gravity, and must clear the neighborhood around its orbit. There are now 8 major planets in our solar system-Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. All other large celestial objects astronomers def ...
samSolar System powerpoint
samSolar System powerpoint

... also have ice mixed into them. They have very long orbits, and when they come close to the Sun, the heat melts the ice from them, and then it gets a long bright tail. Comets are bigger than meteors and they don’t have to enter our atmosphere to be seen. Comets can be seen for many weeks as they move ...
History of Astronomy
History of Astronomy

... • Assumed that the imperfect Earth was surrounded by perfect heavenly spheres Ptolomy’s model worked so well, it was not challenged for 1300 years! ...
File
File

... the smallest. Pluto is smaller than all nine of the solar system's planets. In fact its no longer really considered a planet. It’s orbit on average is 5,913,520,000 from the sun Pluto is the only planet that has not been visited by a spacecraft. Pluto has three moons: ...
Kepler - STScI
Kepler - STScI

... •Giant planets, as a class, are enriched in heavy elements •Enriched compared to the Sun •Enriched compared to their parent stars •Enrichment is a strong inverse function of mass, but with an apparent “floor” at high mass •The heavy element mass of an inflated planet could be estimated only from its ...
Mars as a Solar System Body Physical Properties and Composition
Mars as a Solar System Body Physical Properties and Composition

... This picture depicts the correct relative sizes of the 9 planets of the Solar System in the correct order. The planets ...
Homework #3 - UCLA - Earth, Planetary, and Space Sciences
Homework #3 - UCLA - Earth, Planetary, and Space Sciences

... 9. OK, here’s a slightly trickier question that requires combining what you’ve learned about the Moon and Mercury. Below you’re given five steps in a planet’s evolution (planet applies to the Moon here as well). Order the steps from 1 (earliest) to 5 (most recent). (5 points) ___3___ Heavier materia ...
worksheet.
worksheet.

Overview of the Solar System
Overview of the Solar System

... • the sizes of the all planets are known – angular size • masses of all the planets known – the ones with observable moons, can use Newton’s Laws – use perturbations used for Mercury and Venus (modern methods use satellites) • immense size of the solar system – Kuiper Belt 50 AU from the sun • plane ...
PowerPoint 演示文稿
PowerPoint 演示文稿

... nuclear reactions. Our Sun is an average yellow star, but seems bright because it is so close. Planets are the largest objects that circle around the stars. They may be rocky, like the earth, or made mostly of gas and liquid, like Jupiter. The word planet is Greek for "wanderer." The name comes from ...
Page 444 - ClassZone
Page 444 - ClassZone

... to answer the next five questions. ...
Formation of the Solar System
Formation of the Solar System

... 7. Solar wind (from the sun) blows off remaining dust and debris. • Inner planets are rocky and have metals. Heavy elements withstand the solar wind (gravity, again). • Outer planets are made of light elements, H and He. ...
Thinking Critically
Thinking Critically

... to answer the next five questions. ...
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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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