formation of solar systems | | This paper concludes some scientific explanation of how the universe was created. | | | 8/1/2011 | | SCI224 Fundamentals of Astronomy Final Paper ------------------------------------------------- Instructor: William McMullen‚ Ph.D. Name: Johanne Val ------------------------------------------------- Due Date: 8/1/11-Revised Copy For your final paper‚ pick of the three topics below. 1. The formation of solar systems What is the
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Regoliththe layer of unconsolidated rocky material covering bedrock. FusionProcess in a star’s core in which lightweight hydrogen nuclei combined into heavier helium nuclei Descriptions: Sun ● Energy created by nuclear fusion ● Coronae are unique to this solar system component ● Its surface temperature is approximately 5800 K ● Produces wind that reaches high speeds near the Earth ● Dark spots are cooler than other regions of its surface Mercury: ● Size: 1516 mi ● Distance from sun: 35980000 mi
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The Formation of the Solar System is one of the oldest problems in science. There have been many theories on how the Solar System formed‚ but there is only one theory that has been accepted. That would be the nebular theory. Also known as the nebular hypothesis and solar nebula hypothesis. The nebular hypothesis is a model that explains the evolution of the Solar System. Also‚ the nebular hypothesis is the most accepted model in the field of cosmogony. This model explains subjectively many features
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The Origin of the Solar System A cloud of interstellar gas and/or dust (the "solar nebula") is disturbed and collapses under its own gravity. The disturbance could be‚ for example‚ the shock wave from a nearby supernova. As the cloud collapses‚ it heats up and compresses in the center. It heats enough for the dust to vaporize. The initial collapse is supposed to take less than 100‚000 years. The center compresses enough to become a protostar and the rest of the gas orbits/flows around it
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THE SOLAR SYSTEM T The Solar System consists of the Sun and the astronomical objects gravitationally bound in orbit around it‚ all of which formed from the collapse of a giant molecular cloud approximately 4.6 billion years ago. The vast majority of the system’s mass (well over 99%) is in the Sun. Of the many objects that orbit the Sun‚ most of the mass is contained within eight relatively solitary planets whose orbits are almost circular and lie within a nearly flat disc called the ecliptic
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The Universe and Our Galaxies The Universe and Our Galaxies Examples of Elliptical (Messier 87 ) and Spiral Galaxies (NGC 3559) Examples of Elliptical (Messier 87 ) and Spiral Galaxies (NGC 3559) Edwin Hubble was one of the first people to actually realise what a galaxy is‚ the measurement of the “Hubble Tuning Fork” Classification scheme shows how round or rightly wound their “arms” are. E0 means that an elliptical galaxy is extremely round‚ whilst E7 is flat. However not all galaxies
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AQUA-MARIE Solar System Nebular Hypothesis. According to the nebular hypothesis‚ these clouds collapsed from some kind of turbulence that caused it to heat up and eventually turn into a star. My understanding of the origin and evolution of the solar system is still very limited. Development is made by pushing through the scientific process of hypothesis‚ prediction‚ measurement‚ theory‚ and hypothesis. However‚ there is still a lot of guesswork to be tested before we can really talk about
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that no one really knows why it ’s like that. What people have figured out so far is that gravity is a force‚ and a force is anything that changes the state of rest or motion of an object. In the absence of outside forces‚ the momentum of a system remains constant. This means that if there was no gravity‚ when one would relinquish one ’s hold on the textbook‚ it would remain at rest in the air. If a force acts on a body‚ the body accelerates in the direction of the force. In the example
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The Solar System The solar system still to this day one of the most fascinating subjects of study in the science world. In our time‚ we are one of the first generations to see the planets of our solar system up close‚ and we have been able to view evolution of these planets through time. Our solar system consists of a middle aged star called the Sun‚ 9 planets‚ about 100 moons‚ thousands of asteroids‚ millions of icy bodies‚ and many comets revolving around all of it. We can begin by looking
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Planets of our Solar System The Earth: The earth is the fifth largest planet of the solar system. The life is possible on the earth because its gravity is sufficient to hold atmosphere and best conditions for sustaining life. It contains a large amount of water in the form of oceans. 71% parts of the total area is covered with water and the remaining 29% is covered with land. The temperature of the centre of the earth is 2000° C. The circumference of the earth is 40‚000 km. The earth completes
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