Overview of the Solar System
... present solar system • crucial information about that history and origin of the solar system • outer asteroid belt – Kuiper belt, range from a few tens of metres to more than 1000km (Pluto is an example) • information from the Kuiper belt will help us understand more about the history of our solar s ...
... present solar system • crucial information about that history and origin of the solar system • outer asteroid belt – Kuiper belt, range from a few tens of metres to more than 1000km (Pluto is an example) • information from the Kuiper belt will help us understand more about the history of our solar s ...
Slides
... take place at the core of the sun. The entire supply of hydrogen will have been turned to helium. Once this happens, the sun will go from being a main sequence star to a red giant. The diameter of a red giant is typically 260 times larger than that of a main sequence star. The sun will decrease in t ...
... take place at the core of the sun. The entire supply of hydrogen will have been turned to helium. Once this happens, the sun will go from being a main sequence star to a red giant. The diameter of a red giant is typically 260 times larger than that of a main sequence star. The sun will decrease in t ...
Review Worksheet - Mrs. Sepulveda's Classes
... planetology and discuss its importance to solar system studies. Comparative planetology is the approach we use to study and understand our solar system. It involves comparing the worlds of our system, including planets, moons, asteroids, and comets, to one another. Its basic premise is that the simi ...
... planetology and discuss its importance to solar system studies. Comparative planetology is the approach we use to study and understand our solar system. It involves comparing the worlds of our system, including planets, moons, asteroids, and comets, to one another. Its basic premise is that the simi ...
vocabulary words to know
... SQUEEZE YOUR ANSWERS into the little space given!! Staple your paper to the back of the study guide. 9. How did Galileo’s observations support the idea of a heliocentric system? 10. Why does Mercury have only a thin atmosphere? 11. How do astronomers explain that Venus rotates in the opposite direct ...
... SQUEEZE YOUR ANSWERS into the little space given!! Staple your paper to the back of the study guide. 9. How did Galileo’s observations support the idea of a heliocentric system? 10. Why does Mercury have only a thin atmosphere? 11. How do astronomers explain that Venus rotates in the opposite direct ...
Chapter 28 - Trimble County Schools
... • First to develop was Jupiter –Increased in size through the merging of icy planetesimals that contained mostly lighter elements • Saturn and the other gas giants formed same way – Not as large because Jupiter collected so much material ...
... • First to develop was Jupiter –Increased in size through the merging of icy planetesimals that contained mostly lighter elements • Saturn and the other gas giants formed same way – Not as large because Jupiter collected so much material ...
Lec – History4
... Example: An object that orbits 4 A.U. from Sun a3 = 43 = 64 P = √a3 = √64 = 8 yrs Object will take 8 years to orbit Sun ...
... Example: An object that orbits 4 A.U. from Sun a3 = 43 = 64 P = √a3 = √64 = 8 yrs Object will take 8 years to orbit Sun ...
(“Wanderers”)
... Example: An object that orbits 4 A.U. from Sun a3 = 43 = 64 P = √a3 = √64 = 8 yrs Object will take 8 years to orbit Sun ...
... Example: An object that orbits 4 A.U. from Sun a3 = 43 = 64 P = √a3 = √64 = 8 yrs Object will take 8 years to orbit Sun ...
The Planets in our Solar System
... • (#5) The sun’s diameter is • (#6) The outer planets 1,394,000 km. If we used are much farther apart the scale 1 mm = 700 km, than the inner planets. the sun would be almost 2000 mm (1.9 m)! ...
... • (#5) The sun’s diameter is • (#6) The outer planets 1,394,000 km. If we used are much farther apart the scale 1 mm = 700 km, than the inner planets. the sun would be almost 2000 mm (1.9 m)! ...
Lecture 1
... Definition of a planet Simplest definition is based solely on mass • Stars: burn hydrogen • Brown dwarfs: burn deuterium • Planets: do not burn deuterium Deuterium burning limit occurs at around 13 Jupiter masses ...
... Definition of a planet Simplest definition is based solely on mass • Stars: burn hydrogen • Brown dwarfs: burn deuterium • Planets: do not burn deuterium Deuterium burning limit occurs at around 13 Jupiter masses ...
Explore the Solar System - Museum of Science, Boston
... A typical Explore the Solar System show begins on the Earth, examining several constellations, planets, and stars of interest visible in the night sky. Students are asked to identify daily motions of the sky and its objects. The show then progresses to a space-based perspective of the solar system o ...
... A typical Explore the Solar System show begins on the Earth, examining several constellations, planets, and stars of interest visible in the night sky. Students are asked to identify daily motions of the sky and its objects. The show then progresses to a space-based perspective of the solar system o ...
.~ Observing the Solar System
... Key Concept: In a geocentric system, Earth is at the center of the revolving planets and stars. • Most early Greek astronomers believed Earth was the center of the universe. • A model of the universe in which Earth is at the center is called a geocentric (jee oh SEN trik) system. In a geocentric sys ...
... Key Concept: In a geocentric system, Earth is at the center of the revolving planets and stars. • Most early Greek astronomers believed Earth was the center of the universe. • A model of the universe in which Earth is at the center is called a geocentric (jee oh SEN trik) system. In a geocentric sys ...
Study Guide Our Solar System Student Note: The upcoming test on
... Like the sun’s interior, its atmosphere is composed mainly of hydrogen and helium. The sun’s atmosphere includes the photosphere, the chromosphere and the corona. Each layer has unique properties. The photosphere is the inner layer which you see when you look at the sun. The chromosphere is the midd ...
... Like the sun’s interior, its atmosphere is composed mainly of hydrogen and helium. The sun’s atmosphere includes the photosphere, the chromosphere and the corona. Each layer has unique properties. The photosphere is the inner layer which you see when you look at the sun. The chromosphere is the midd ...
Size of Sun and Size of Planets
... 1. On which planet would you weigh the most? _______________________ 2. Why do you think this is true? ______________________________________ 3. On which planet(s) would you weigh the least? __________________________ 4. Why do you think this is true? _______________________________________ Conclusi ...
... 1. On which planet would you weigh the most? _______________________ 2. Why do you think this is true? ______________________________________ 3. On which planet(s) would you weigh the least? __________________________ 4. Why do you think this is true? _______________________________________ Conclusi ...
slides
... NOT solid; they are made of countless small chunks of ice and rock, each orbiting like a tiny moon. Artist’s conception ...
... NOT solid; they are made of countless small chunks of ice and rock, each orbiting like a tiny moon. Artist’s conception ...
POWERPOINT with Facts - Mrs. Brown`s Third Grade Class
... The Outer Planets • The outer planets are made mostly of frozen gases and they are much further from the sun. This makes their surface cooler than the inner planets. They are all larger than the inner planets. They also have many moons and some ...
... The Outer Planets • The outer planets are made mostly of frozen gases and they are much further from the sun. This makes their surface cooler than the inner planets. They are all larger than the inner planets. They also have many moons and some ...
Document
... The Sun, planets, asteroids, comets, planetesimals all revolve in the same direction with some exceptions. ...
... The Sun, planets, asteroids, comets, planetesimals all revolve in the same direction with some exceptions. ...
The Solar System
... Astronomers have classified Pluto as a dwarf planet. Dwarf means “small.” Pluto is made of ice. It has a moon almost as large as it is. It takes Pluto 249 years to orbit the sun. ...
... Astronomers have classified Pluto as a dwarf planet. Dwarf means “small.” Pluto is made of ice. It has a moon almost as large as it is. It takes Pluto 249 years to orbit the sun. ...
Lecture Exam 1 Review
... understand how the scientific method works? What the major limitations astronomers face in studying celestial objects? Can you provide any examples of such limitations? Do you have a good understanding of the following terms? Rotation vs. Revolution Facts, Laws, Theories, Models What properties ...
... understand how the scientific method works? What the major limitations astronomers face in studying celestial objects? Can you provide any examples of such limitations? Do you have a good understanding of the following terms? Rotation vs. Revolution Facts, Laws, Theories, Models What properties ...
Planet - Tasker Milward Physics Website
... together to make Helium. Lots of energy is released in the process as heat and light. ...
... together to make Helium. Lots of energy is released in the process as heat and light. ...
asteroids - WordPress.com
... Over three successive orbits each Hilda asteroid passes through all of these three points in sequence. They do not form a true asteroid family, in the sense that they do not descend from a common parent object. The namesake is 153 Hilda, discovered by Johann Palisa in 1875. There are more th ...
... Over three successive orbits each Hilda asteroid passes through all of these three points in sequence. They do not form a true asteroid family, in the sense that they do not descend from a common parent object. The namesake is 153 Hilda, discovered by Johann Palisa in 1875. There are more th ...
The Solar System
... • Neptune is the eighth , but sometimes it is the ninth planet from the Sun. • Neptune has eight moons. • Its largest moon is called Triton. • It has two thick and two thin rings around it. • One day on Neptune lasts about 18 Earth hours. • It takes 165 years to orbit the Sun. www.worldalmanacforkid ...
... • Neptune is the eighth , but sometimes it is the ninth planet from the Sun. • Neptune has eight moons. • Its largest moon is called Triton. • It has two thick and two thin rings around it. • One day on Neptune lasts about 18 Earth hours. • It takes 165 years to orbit the Sun. www.worldalmanacforkid ...
Some 250 years ago, the philosopher Immanuel Universal
... or another site in Luoyang. The atlas shows 1,339 stars arranged in 257 groups, or asterisms, two of which resemble the constellations of the Big Dipper and Orion. It includes faint stars that are difficult to see with the naked eye, and several in the Southern Hemisphere. The styles of the dots dif ...
... or another site in Luoyang. The atlas shows 1,339 stars arranged in 257 groups, or asterisms, two of which resemble the constellations of the Big Dipper and Orion. It includes faint stars that are difficult to see with the naked eye, and several in the Southern Hemisphere. The styles of the dots dif ...
Announcements
... planetary interiors. Describe the importance of planetary size on its evolution. ...
... planetary interiors. Describe the importance of planetary size on its evolution. ...
Dwarf planet
A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite. That is, it is in direct orbit of the Sun, and is massive enough for its shape to be in hydrostatic equilibrium under its own gravity, but has not cleared the neighborhood around its orbit.The term dwarf planet was adopted in 2006 as part of a three-way categorization of bodies orbiting the Sun, brought about by an increase in discoveries of objects farther away from the Sun than Neptune that rivaled Pluto in size, and finally precipitated by the discovery of an even more massive object, Eris. The exclusion of dwarf planets from the roster of planets by the IAU has been both praised and criticized; it was said to be the ""right decision"" by astronomer Mike Brown, who discovered Eris and other new dwarf planets, but has been rejected by Alan Stern, who had coined the term dwarf planet in 1990.The International Astronomical Union (IAU) currently recognizes five dwarf planets: Ceres, Pluto, Haumea, Makemake, and Eris. Brown criticizes this official recognition: ""A reasonable person might think that this means that there are five known objects in the solar system which fit the IAU definition of dwarf planet, but this reasonable person would be nowhere close to correct.""It is suspected that another hundred or so known objects in the Solar System are dwarf planets. Estimates are that up to 200 dwarf planets may be found when the entire region known as the Kuiper belt is explored, and that the number may exceed 10,000 when objects scattered outside the Kuiper belt are considered. Individual astronomers recognize several of these, and in August 2011 Mike Brown published a list of 390 candidate objects, ranging from ""nearly certain"" to ""possible"" dwarf planets. Brown currently identifies eleven known objects – the five accepted by the IAU plus 2007 OR10, Quaoar, Sedna, Orcus, 2002 MS4 and Salacia – as ""virtually certain"", with another dozen highly likely. Stern states that there are more than a dozen known dwarf planets.However, only two of these bodies, Ceres and Pluto, have been observed in enough detail to demonstrate that they actually fit the IAU's definition. The IAU accepted Eris as a dwarf planet because it is more massive than Pluto. They subsequently decided that unnamed trans-Neptunian objects with an absolute magnitude brighter than +1 (and hence a diameter of ≥838 km assuming a geometric albedo of ≤1) are to be named under the assumption that they are dwarf planets. The only two such objects known at the time, Makemake and Haumea, went through this naming procedure and were declared to be dwarf planets. The question of whether other likely objects are dwarf planets has never been addressed by the IAU. The classification of bodies in other planetary systems with the characteristics of dwarf planets has not been addressed.