
Uranus is considered to be the brightest planet in our solar
... Asteroids are rocky formation that travel through space. ...
... Asteroids are rocky formation that travel through space. ...
Formation of Solar System
... charged particles creates a magnetic field. The nucleus of the solar nebula thus had a magnetic field associated with it. Matter close to the nucleus was also partially ionised and moved with it. T for disc fell as we moved away from the nucleus so that more and more electrically neutral molecules ...
... charged particles creates a magnetic field. The nucleus of the solar nebula thus had a magnetic field associated with it. Matter close to the nucleus was also partially ionised and moved with it. T for disc fell as we moved away from the nucleus so that more and more electrically neutral molecules ...
Solar Motion and Velocity Dispersions
... position moving in a perfectly circular orbit about the galactic center). ...
... position moving in a perfectly circular orbit about the galactic center). ...
Astronomy 1001/1005 Midterm (200 points) Name:
... any large astronomical distance. Earth’s average distance from the Sun. any planet’s average distance from the Sun. None of the above ...
... any large astronomical distance. Earth’s average distance from the Sun. any planet’s average distance from the Sun. None of the above ...
Which of the following statements is TRUE
... Week 5 – Quiz #6 Star X has a surface temperature that is 3 times higher than that of the Sun. Both stars have exactly the same radius. Which of the following statements is TRUE? A. The luminosity of the Sun is 81 times that of the star X B. The typical photon emitted by star X has a lower energy t ...
... Week 5 – Quiz #6 Star X has a surface temperature that is 3 times higher than that of the Sun. Both stars have exactly the same radius. Which of the following statements is TRUE? A. The luminosity of the Sun is 81 times that of the star X B. The typical photon emitted by star X has a lower energy t ...
Astronomy Practice Test
... 22. Stars much more massive than our sun begin their lives very similarly; however, they end quite differently. How would one of these massive stars (more than 10X bigger) end its life? A. red giant B. white dwarf C. neutron star D. all of the above 23. Which of the following units are in the correc ...
... 22. Stars much more massive than our sun begin their lives very similarly; however, they end quite differently. How would one of these massive stars (more than 10X bigger) end its life? A. red giant B. white dwarf C. neutron star D. all of the above 23. Which of the following units are in the correc ...
Solar System.3rd.Mark Vega
... out circle) counterclockwise direction. The inner planets orbit much faster then the outer planets. Venus is the one inner planet that has a different rotation – it rotates in a clockwise rotation while all the other inner planets rotate in a counter-clockwise direction. The outer planets all rotate ...
... out circle) counterclockwise direction. The inner planets orbit much faster then the outer planets. Venus is the one inner planet that has a different rotation – it rotates in a clockwise rotation while all the other inner planets rotate in a counter-clockwise direction. The outer planets all rotate ...
Take Home #2 Complete the following on your own paper. Do not
... D. Research would have stopped if Laplace had NOT given enough evidence for the hypothesis. 19) Which answer below best describes the future of models of the life cycles of stars? A. Models will probably stay the same because scientists do not enjoy creating new models. B. Models will probably stay ...
... D. Research would have stopped if Laplace had NOT given enough evidence for the hypothesis. 19) Which answer below best describes the future of models of the life cycles of stars? A. Models will probably stay the same because scientists do not enjoy creating new models. B. Models will probably stay ...
Montage of Jupiter and the Galilean satellites
... while blue indicates the electrons are whirling around the magnetic field of the inner nebula. In the nebula's very center lies a pulsar: a neutron star rotating, in this case, 30 times a second. November 22, 1999 ...
... while blue indicates the electrons are whirling around the magnetic field of the inner nebula. In the nebula's very center lies a pulsar: a neutron star rotating, in this case, 30 times a second. November 22, 1999 ...
4th Grade Earth Science Unit Guide:
... Identify how technology is used to observe distant objects in the sky. Essential Questions (Students should be able to fully answer by the und of the unit). 1. What is a star? A star is a hot ball of gas that gives off light and other forms of energy; it looks like a little, shiny point of light ...
... Identify how technology is used to observe distant objects in the sky. Essential Questions (Students should be able to fully answer by the und of the unit). 1. What is a star? A star is a hot ball of gas that gives off light and other forms of energy; it looks like a little, shiny point of light ...
ExoplanetWorksheet
... *All of the rocky planets in our Solar System are at least 3 times more dense than Jupiter. Does it look like we’ve found very many or very few rocky exoplanets? __________________________________ * White dwarf stars have a mass that is comparable to the Sun, but are about 100 times smaller. Have we ...
... *All of the rocky planets in our Solar System are at least 3 times more dense than Jupiter. Does it look like we’ve found very many or very few rocky exoplanets? __________________________________ * White dwarf stars have a mass that is comparable to the Sun, but are about 100 times smaller. Have we ...
ppt - Faculty Virginia
... Jupiter and Saturn are. - The significant portion of their mass likely made up by water leads to Uranus and Neptune being called “ice giants” ...
... Jupiter and Saturn are. - The significant portion of their mass likely made up by water leads to Uranus and Neptune being called “ice giants” ...
Global Warming_Notes_for_Test_Review[1]
... 27. Our sun is an example of a main sequence star. The time necessary for a star to complete this stage and move on to the next stage of a star’s life depends on its mass. True or False questions. If false, explain why the answer is false. 1. Only Earth has gravity. False All things have gravity 2. ...
... 27. Our sun is an example of a main sequence star. The time necessary for a star to complete this stage and move on to the next stage of a star’s life depends on its mass. True or False questions. If false, explain why the answer is false. 1. Only Earth has gravity. False All things have gravity 2. ...
The Heliocentric Model of the Solar System
... The relative position of the stars, for example the 3 stars on a line at the center of the picture, seems to be ‘fixed’ relative to each other, i.e. they do not change relative positions in the course of many years. ...
... The relative position of the stars, for example the 3 stars on a line at the center of the picture, seems to be ‘fixed’ relative to each other, i.e. they do not change relative positions in the course of many years. ...
The Newtonian Revolution: The discovery of natural law
... decent quantitative model of the planets’ motion • It had the Earth at the center • It placed the planets Mercury and Venus carefully to match the observed angle offsets between the sun and these planets. • Accounted for retrograde motion with epicycles. Then needed to offset the center of epicycles ...
... decent quantitative model of the planets’ motion • It had the Earth at the center • It placed the planets Mercury and Venus carefully to match the observed angle offsets between the sun and these planets. • Accounted for retrograde motion with epicycles. Then needed to offset the center of epicycles ...
Our Solar System
... -Distinguish between questions that can be answered by science and those that cannot, and between problems that can be solved by technology and those that cannot with regards to solar system formation. -Estimate quantities of distances in parsec. Estimate the age of the solar system. -Describe and a ...
... -Distinguish between questions that can be answered by science and those that cannot, and between problems that can be solved by technology and those that cannot with regards to solar system formation. -Estimate quantities of distances in parsec. Estimate the age of the solar system. -Describe and a ...
Terestialplanets
... Jupiter, Saturn, Uranus, Neptune, and Pluto First four are called Jovian Planets (Jupiter-like) Massive in nature They are gaseous Outer layers mostly hydrogen gas, and compressed to a hot liquid • Closer to the planet’s center ...
... Jupiter, Saturn, Uranus, Neptune, and Pluto First four are called Jovian Planets (Jupiter-like) Massive in nature They are gaseous Outer layers mostly hydrogen gas, and compressed to a hot liquid • Closer to the planet’s center ...
Untitled - Dommelroute
... of growing from the size of a large pinhead to a mountain may have taken one hundred thousand years or so. Then the process began to slow down. The original dust and gas had been used up, and the cloud thinned. Several stars—such as Beta Pictoris—have been observed with large, thin disks of dust sur ...
... of growing from the size of a large pinhead to a mountain may have taken one hundred thousand years or so. Then the process began to slow down. The original dust and gas had been used up, and the cloud thinned. Several stars—such as Beta Pictoris—have been observed with large, thin disks of dust sur ...
Stars
... Sun 4.5 Byr ago from the gravitational collapse of an interstellar cloud of gas and dust. The planets and Sun formed from the same reservoir of interstellar matter and are therefore composed of primarily the same elements. As the cloud collapsed under the force of gravity it began to spin rapidly an ...
... Sun 4.5 Byr ago from the gravitational collapse of an interstellar cloud of gas and dust. The planets and Sun formed from the same reservoir of interstellar matter and are therefore composed of primarily the same elements. As the cloud collapsed under the force of gravity it began to spin rapidly an ...
Skinner Chapter 2
... planet's average distance from the Sun. 43. Mercury, Venus, Earth, Mars They are called "terrestrial" because they are similar to the Earth, in having relatively high overall densities, rocky compositions, and differentiated (layered) internal structures. 44. A supernova is the most likely source fo ...
... planet's average distance from the Sun. 43. Mercury, Venus, Earth, Mars They are called "terrestrial" because they are similar to the Earth, in having relatively high overall densities, rocky compositions, and differentiated (layered) internal structures. 44. A supernova is the most likely source fo ...
or view
... The formation of the Sun had a dramatic effect on the temperatures across the solar nebula, introducing a temperature range that stretched from about 2000K near the Sun to less than 50K at the outer regions. The heat in the inner Solar System only allowed materials with high condensation temperature ...
... The formation of the Sun had a dramatic effect on the temperatures across the solar nebula, introducing a temperature range that stretched from about 2000K near the Sun to less than 50K at the outer regions. The heat in the inner Solar System only allowed materials with high condensation temperature ...
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.