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Chapter 19
Chapter 19

... differences between terrestrial and Jovian planets? a. The temperature of the accretion disk was high close to the Sun and low far from the Sun. b. Terrestrial planets formed closer to the Sun, and are thus made of high-density rocky materials. c. Jovian planets are large and have high-mass because ...
A WALK THROUGH THE SOLAR SYSTEM
A WALK THROUGH THE SOLAR SYSTEM

... Ancient astronomers observed points of light that appeared to move among the stars, and they called these objects planets, meaning wanderers. They were named after Roman legends. Jupiter was the king of the gods, Mars the god of war, Mercury was messenger of the gods, Venus was the god of beauty, an ...
Our Star: The Sun
Our Star: The Sun

... WASHINGTON (AP) -- A large solar flare was reported Wednesday and forecasters warned of potential electrical and communications disruptions. The flare was reported by the National Oceanic and Atmospheric Administration's Space Environment Center in Boulder, Colorado. Significant solar eruptions are ...
constellations
constellations

... objects all move relative to the ‘fixed’ background stars. Mostly this motion is direct, i.e. in the same direction as the Sun’s annual motion. However, at times the solar system objects appear to move in the opposite direction relative to the background stars, i.e. their motion is retrograde. The p ...
September 2013 - Joliet Junior College
September 2013 - Joliet Junior College

... The Autumnal Equinox is at 3:44 pm on September 22nd. It is the end of astronomical summer and the beginning of fall. On that date, the sun is directly above the equator and will continue to move southward over the southern hemisphere to 23 degrees below the equator. Here in the Midwest, it means th ...
The Basics of the Universe
The Basics of the Universe

... magnetic disturbances that can cause Solar Prominences, loops protruding from the Sun that can last for days. These are multiple times the size of the Earth. ...
Combining Practices with Core Ideas in the NGSS
Combining Practices with Core Ideas in the NGSS

... logical? What evidence could they suggest that was so? What evidence would suggest the sun is not a star? Then I could have them look at an image of a long road with streetlights, where the closest looks very large and bright and the most distant looks tiny and dim—although we know the lights are al ...
Day 1212
Day 1212

... The outer layers expand and cool. In this late stage of its life cycle, an average star like our Sun is called a giant. ...
Tides on Earth
Tides on Earth

...  Mars has two tiny moons named Phobos and Deimos, which revolve around Mars relatively quickly. ...
Part 1 – The Universe
Part 1 – The Universe

... When a book like this comes into existence, it is very hard to name and thank all the people that helped me shape this book. It took me over 6 years to consolidate and format all the content in a manner that may benefit the readers. However, I would like to start by thanking my wife Suman Bansal for ...
Quiz 2 review sheet - Rice Space Institute
Quiz 2 review sheet - Rice Space Institute

... less). You can then tell the age of a cluster by the lifetime of the heaviest star still on the main sequence in the H-R diagram for the group. (heavier stars will have blown up) 4. That smaller stars are redder and cooler, and have very long lifetimes (up to hundreds of billions of years). 5. That ...
1 1. The Solar System
1 1. The Solar System

... The solar system consists of the Sun; the nine planets, over 100 satellites of the planets, a large number of small bodies (the comets and asteroids), and the interplanetary medium (There are also many more planetary satellites that have been discovered but not yet officially named). The inner solar ...
1. Base your answer to the following question
1. Base your answer to the following question

... (1) gas captured as Earth passed through a gas cloud (2) the gas surrounding Earth at the time of its formation (3) escaped gas from the sun (4) gas released from the interior of our planet 10. What was the most abundant gas present in the original planetary atmosphere? (1) water vapor (3) hydrogen ...
Final Exam from 2004 - Onondaga Community College
Final Exam from 2004 - Onondaga Community College

... to Austin TX never to be heard from again. Please, in an outline form, list the points you would make that described how Saturn became so much larger than the Earth. You do not have to write a narrative, simply a list of relevant events, concepts or processes is sufficient. (7 points) 3. The extra-s ...
Document
Document

... Sun’s rays must pass through. Winter is colder than summer because the Sun is lower in winter which means the Sun’s rays aren’t directly hitting Earth and have more atmospheres to pass through. In summer the Sun is higher which means the Sun’s rays are directly hitting the Earth and have fewer atmo ...
The Moon - Kaufman ISD
The Moon - Kaufman ISD

... Why does a year on Jupiter last longer than a year on the Earth? ...
brock university answers
brock university answers

... 11. The Sun generates energy in its core primarily by (a) converting gravitational potential energy to thermal energy. (b) hydrostatic equilibrium. (c) magnetohydrodynamics. (d) * nuclear reactions that convert hydrogen into helium. 12. The distance from the Sun to Neptune, the farthest known planet ...
The Sun
The Sun

...  The sun is an average or medium size star. There are stars that smaller and larger than our sun. The sun is just the right size and distance from Earth so that there can be life on our planet.  There are stars that are much larger than our sun. A star in the Orion constellation called Betelgeuse ...
Physics@Brock - Brock University
Physics@Brock - Brock University

... 11. The Sun generates energy in its core primarily by (a) converting gravitational potential energy to thermal energy. (b) hydrostatic equilibrium. (c) magnetohydrodynamics. (d) nuclear reactions that convert hydrogen into helium. 12. The distance from the Sun to Neptune, the farthest known planet, ...
Quiz4 - UNLV Physics
Quiz4 - UNLV Physics

... A) It is the same size and mass. B) It is about 10 times larger both in size and mass. C) It is about 10 times larger in size and the same mass. D) It is about the same size but is 10 times more massive. E) Jupiter doesn't have a core!it is made entirely from hydrogen and helium. Answer: D ...
Solar System Text - Spring Creek Elementary
Solar System Text - Spring Creek Elementary

... The sizes of the planets in this picture are shown to scale—objects compared to a standard for accurate size perception. The distances between the planets are NOT to scale. Comparing these objects to a standard helps to show how big and how small the planets are compared to Earth. It can be difficu ...
CH 27 PPT
CH 27 PPT

... The outer planets are those found beyond the asteroid belt (located between Mars and Jupiter): Jupiter, Saturn, Uranus, and Neptune. The outer planets are known as the Jovian (Jupiter-like) planets. The first four of the outer planets are considerably larger than Earth, and are gaseous planets with ...
PHYSICS 1500 - The University of Sydney
PHYSICS 1500 - The University of Sydney

... The illustration at left shows an artist’s impression of a ‘hot Jupiter’ – a giant planet in a very close orbit around its parent star. The first such planet discovered was 51 Pegasi b which takes 4.23 days to orbit a sun-like star. The system is about 50 light years from Earth. The planet was found ...
Pluto and the Kuiper Belt
Pluto and the Kuiper Belt

... Starting in 1992, astronomers discovered a vast population of small bodies that orbit the Sun beyond Neptune. At least 70,000 have diameters larger than 100 km. They extend outward from ~30 AU to ~50 AU. Most are in a thick band around the ecliptic — a ring called the “Kuiper Belt”. The Kuiper Belt ...
The Formation of Planetary Systems
The Formation of Planetary Systems

... but will not be available for some time The most promising detection method involves looking for changes in a star’s brightness as a planet transits across it Until we can observe such planets, we will not be able to draw conclusions about the uniqueness of our own system ...
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Solar System



The Solar System comprises the Sun and the planetary system that orbits it, either directly or indirectly. Of those objects that orbit the Sun directly, the largest eight are the planets, with the remainder being significantly smaller objects, such as dwarf planets and small Solar System bodies such as comets and asteroids. Of those that orbit the Sun indirectly, two are larger than the smallest planet.The Solar System formed 4.6 billion years ago from the gravitational collapse of a giant interstellar molecular cloud. The vast majority of the system's mass is in the Sun, with most of the remaining mass contained in Jupiter. The four smaller inner planets, Mercury, Venus, Earth and Mars, are terrestrial planets, being primarily composed of rock and metal. The four outer planets are giant planets, being substantially more massive than the terrestrials. The two largest, Jupiter and Saturn, are gas giants, being composed mainly of hydrogen and helium; the two outermost planets, Uranus and Neptune, are ice giants, being composed largely of substances with relatively high melting points compared with hydrogen and helium, called ices, such as water, ammonia and methane. All planets have almost circular orbits that lie within a nearly flat disc called the ecliptic.The Solar System also contains smaller objects. The asteroid belt, which lies between Mars and Jupiter, mostly contains objects composed, like the terrestrial planets, of rock and metal. Beyond Neptune's orbit lie the Kuiper belt and scattered disc, populations of trans-Neptunian objects composed mostly of ices, and beyond them a newly discovered population of sednoids. Within these populations are several dozen to possibly tens of thousands of objects large enough to have been rounded by their own gravity. Such objects are categorized as dwarf planets. Identified dwarf planets include the asteroid Ceres and the trans-Neptunian objects Pluto and Eris. In addition to these two regions, various other small-body populations, including comets, centaurs and interplanetary dust, freely travel between regions. Six of the planets, at least three of the dwarf planets, and many of the smaller bodies are orbited by natural satellites, usually termed ""moons"" after the Moon. Each of the outer planets is encircled by planetary rings of dust and other small objects.The solar wind, a stream of charged particles flowing outwards from the Sun, creates a bubble-like region in the interstellar medium known as the heliosphere. The heliopause is the point at which pressure from the solar wind is equal to the opposing pressure of interstellar wind; it extends out to the edge of the scattered disc. The Oort cloud, which is believed to be the source for long-period comets, may also exist at a distance roughly a thousand times further than the heliosphere. The Solar System is located in the Orion Arm, 26,000 light-years from the center of the Milky Way.
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