| Papers [1-15] of 100 :: [Page 1 of 7] | | Go to page : 1 2 3 4 5 6 7 —> | Search results on "STARS": |
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The Life Cycle of Stars, 2006.
An analysis of the regeneration of stars.
1,118 words (approx. 4.5 pages), 2 sources, MLA, $ 38.95
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Abstract
In order to shed some light onthe processes involved in the stars' life cycle, this paper discusses and analyzes how, throughout its 'life,' a star will remain dependent on other stars for its eventual re-birth--that is, the creation of another kind of a star. In line with the main topic of this paper, the discussion and analysis argue that the life cycle of a star is an interdependent and recurring process, mainly because stars depend on other stars to re-generate or create another star.
From the Paper
"The second phase, the star's death, occurs when the star has finally used up its hydrogen atoms, and can no longer generate energy from its stellar body. As this happens, the star is "pulled" by the gravity and will burn its helium to become carbon, becoming a red giant. The dying star will be pulled towards the gravity because it will no longer have the counterforce that it once had (force from the energy radiated from it) in order to balance the two forces (gravity and energy pressure). Once helium gases were burned out or exhausted from the stellar body, carbon will be produced and scattered. The dead star will eventually have a carbon core, cool down, and become a white dwarf."
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Formation of Stars, 2002.
An analysis of the processes involved in the formation of stars.
1,541 words (approx. 6.2 pages), 3 sources, MLA, $ 50.95
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Abstract
This paper explains that by viewing the gas that surrounds stars as a dynamic atmosphere, undergoing cycles of materials similar to those that go on in the Earth's own protective gases, astronomers are understanding more and more about the processes involved in the formation of stars. The paper deals with the questions of how the supernova of massive stars affect the formation of stars in the future, why star formation seems to occur in relative bursts, and how long the Milky Way will continue to produce stars.
From the Paper
"Beyond applying the atmospheric model to intergalactic gas, astronomers have also been studying more carefully exactly what components make up the gas and at what temperature these components exist. About 90% of the constituents of intergalactic atmosphere are various forms of hydrogen, with close to 10% being helium, and everything else, from lithium to uranium -- the whole spectrum of the periodic chart -- making up less than 0.1%. The majority of the hydrogen is present as neutral hydrogen, termed H I by astronomers. This form of hydrogen gas is identified by the spectral frequency of the light that it emits, namely 1,420 megahertz. Although scattered throughout the galaxy, the majority of H I is located around the galactic midplane, and forms a gaseous disk about 300 parsecs thick (Reynolds, 2002, p. 40)."
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Life Cycle of Stars, 2008.
This paper describes the life cycle of stars, which is a normal progression.
1,185 words (approx. 4.7 pages), 4 sources, APA, $ 40.95
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Abstract
This paper explains that stars have a life cycle that is simply too long for human life to perceive directly and even too long for all of human history to record. The author points out that astronomers have been able to categorize stars to show the different levels of development reached by different groups of stars. The paper relates that, over billions of years, the star slowly contracts, compensating for the heat and light energy it has lost. The author underscores that, as this contraction continues, the temperature, density and pressure at the core of the star increases. The paper tells that, as the temperature at the core rises and the star contracts, the tension between gravity pulling in and gas pressure pushing out determines the life of the star. The author describes this process through the star's life cycle from protostar to black holes.
From the Paper
"At this stage, the star is called a planetary nebula. The core of this star becomes a whiter dwarf, an extremely dense star now the size of a planet. Once the white dwarf uses all its energy, it stops shining and becomes a "black dwarf," or a dead star. Astronomers see this as the final stage for our own Sun. however, for stars with higher masses than the Sun (up to about 40 times greater), the outer layers of the star may be thrown off with much more force in a supernova, an explosion leading to the collapse of the star down to a very compact size, producing what is known as a "neutron star."
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"Stars in the Making", 2007.
An analysis and critique of "Stars in the Making", a 2001 article by Elana Harris.
1,189 words (approx. 4.8 pages), 0 sources, $ 40.95
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Abstract
This paper discusses sales and marketing management, from the point of view of "Stars in the Making", an article written by Elana Harris in 2001. The paper summarizes Harris' article and describes its relevance to sales management. The paper then provides a critique of the article and provides some suggestions for improving it.
Table of Contents:
A Summary of "Stars in the Making"
Relevance of "Stars in the Making"
A Critique of "Stars in the Making"
Suggested Changes to Harris' Article
From the Paper
"In Harris' article, she makes the point that there are ways to mentor, motivate, and lead new salespeople to their full potential as salespeople; this point is cleverly proven by success stories from such luminary companies as Bausch & Lomb and others. Perhaps the most important message that Harris puts forth in "Stars in the Making" is that training, motivation and development of the skills needed for overcoming challenges are keys to the growth of salespeople over the long term. Because of this, Harris continues, sales managers must be coaches or mentors to their team members as well."
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Astronomy, Stars and Extraterrestrial Life, 2007.
This paper explores life-supporting stars and the search for extraterrestrial life.
922 words (approx. 3.7 pages), 4 sources, MLA, $ 32.95
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Abstract
The paper explains that stars are set up to have planets circling around them and it is on those planets that scientists search to locate other life forms that may exist. The paper reveals that a growing body of scientists believe that there is/was life on Mars. The paper discusses how, with the advances in technology, it may not be long until we find a planet with living beings.
Outline:
Introduction
Stars
The Search For Life
Conclusion
From the Paper
"Man has been working on science since the beginning of time. As the human race continues to evolve, technology become more advanced and the ability to answer questions accurately grows stronger. One of the questions that has continued to stump mankind since the beginning of time is whether or not there is life out there. Songs are written about it, movies depicting aliens abound and books convey the belief that there is life on other planets and in other solar systems, however, to date no scientific evidence has been found that can support that belief. The technological advances that have occurred in recent history have allowed man to provide a more structured research setting to answer the questions about life bearing planets and alien life."
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The Stars, 2004.
This paper discusses the composition of stars and the method of studying this composition.
1,445 words (approx. 5.8 pages), 3 sources, MLA, $ 47.95
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Abstract
This paper explains that spectroscopy, the study of the spectral lines of the different atomic constituents, has been one of the oldest and most trusted methods of studying the elemental analysis of stars and other luminous heavenly objects. The author states that, by using spectroscopic observations, the radial velocities and the elemental abundances of the extra galactic objects has successfully been established. The paper reports that the availability of specific spectroscopy software has further hastened the study of the molecular mechanics and quantum mechanics.
Table of Contents
Introduction
Spectroscopy and Study of Stars
Spectral Lines (Elemental Abundance)
Classification according to Spectra
Spectroscopy Software
Conclusion
From the Paper
"The availability of spectroscopic software has allowed the possibility of quick and accurate study of quantum study of the spectral elements. GAMESS is one such software that can be used to calculate the SCF wave functions, perform automatic search for transition states, geometrical orientation and in analyzing the vibrational frequencies. GAMESS (General Atomic and Molecular Electronic Structure System) allows us to integrate quantum mechanics and molecular mechanics, which is essential for our understanding of the complex astronomical science. The software allows us to study chemical functions like dipole movements and to perform complex computations."
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"Stars in Their Courses", 2002.
A review of Shelby Foote's "Stars in Their Courses: The Gettysburg Campaign June-July 1863", an excerpt from a trilogy that details the history of the civil war.
1,134 words (approx. 4.5 pages), 1 source, MLA, $ 39.95
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Abstract
This paper discusses Shelby Foote's book "Stars in Their Courses: The Gettysburg Campaign June-July 1863", which offers a historical account of the true events of the campaign in a novel format. The paper describes the author's technique of building the characters and setting the scenes, thereby giving the reader an appreciation of the human side of this period of history.
From the Paper
"The major feature of Shelby Foote that impacts on the book is that he was both a historian and a novelist, with a special interest in the civil war. His previous book titled Shiloh was a fictional account of the civil war and was well-received. Because of the interest in this book, Shelby was requested to write a history of the civil war. His trilogy was the result, with Stars in Their Courses an excerpt from this trilogy. This background of Foote's explains his unique approach to writing the account. Foote combined his talents as a novelist and a historian to write an account that combined the best features of both. Foote was focused not only on the facts as a history book might list them, but on what the experience was like for the people involved. This resulted in the main aspect that sets the book apart from other historical accounts, the focus on not just describing the facts but telling a story."
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Stars, 2007.
An overview of the structure and characteristics of stars.
996 words (approx. 4.0 pages), 3 sources, MLA, $ 35.95
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Abstract
This paper examines how a star is a huge, shining ball in space that produces a tremendous amount of light and other forms of energy. It looks at their physical makeup, the different types, and the recycling effect of star evolution on the rest of the universe.
From the Paper
"Stars have many variants such as age, size, mass, and luminosity, but one thing they have in common is that "about 75 percent of all stars are members of a binary system, a pair of closely spaced stars that orbit each other" (Green, 2005, p. 1). Stars are also grouped together in galaxies such as the Milky Way which hosts more than 100 billion stars. "Three-dimensional computer models of star formation predict that the spinning clouds of dust may break up into two or three blobs; if true, this would explain why the majority of the stars in the Milky Way are paired or in groups of multiple stars" (science@nasa, p.1). Clearly, the structure and formation of individual stars mimics the structure of other important elements of the universe."
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Sports Stars, 2004.
This paper presents three essays on sports stars.
920 words (approx. 3.7 pages), 2 sources, MLA, $ 31.95
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Abstract
This paper creates three essays on athletes by using three different rhetorical modes--description, compare-and-contrast and cause-and-effect. The author discusses the difference in style in the three essays.
From the Paper
"A few seasons back Tiger Woods seemed unbeatable. On the most superficial level, the reason that no one seemed to be able to touch him was that he was simply better than anyone else. He made hitting an eagle seem as natural as walking."
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Sit-coms & Comic Stars, 1994.
Examines the role of stand-up comedians in the development of television situation comedies through the years.
2,025 words (approx. 8.1 pages), 7 sources, $ 71.95
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From the Paper
" Comedy comes in many different forms, and in recent years standup comedy has come into its own. The growth in comedy clubs across the nation and the creation of new outlets on cable television give comedians more exposure than ever before. Styles of comedy change over time, and one of the reasons comedy changes as rapidly as it does today is television. Television uses up material and requires a constant influx of new comedians and new material to satisfy the audience. Comedy has been a vital element in network programming since the beginning of the medium. The massive ratings success of I Love Lucy in the 1950s produced a continuing search for the next long-running hit. A number of comedians have made their mark in recent years with innovative programs or programs that featured their strong points. Several have used their popularity on television as a springboard to.."
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The Stars & Stripes vs. the Rising Sun, 1999.
Examines how World War II in the Pacific was a war of two economies, where the United States' productivity was able to give the nation an overwhelming advantage over Japan.
4,177 words (approx. 16.7 pages), 7 sources, MLA, $ 111.95
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Abstract
This paper explains how the course of World War II changed dramatically as the United States entered on the side of the Allies. An economic powerhouse, the United States' production capabilities and logistics outpaced most other nations combined during the course of the war. This paper discusses how the U.S.'s production prowess was the major reason behind the victory over Japan.
From the Paper
"Around the year 1931, the island nation of Japan was at a height of national pride. Her status had risen from that of a backward agricultural society to an industrially advanced power in mere decades. The Japanese national policy of that period could be best summed in one phrase, "hakko ichiu," or "bringing the eight corners of the world under one roof" (Morison, 5). Hakko ichiu was the declaration of the mythical Japanese ruler, Emperor Jimmu, who ruled a legendary kingdom circa 600 BC. In the year 1931, the phrase was resurrected by the militarists to summon support for the Japanese ambition over East Asia. History is a collection of all events that took place in the past. Seeing through the eyes of history, we watched the Allied forces, mainly American, defeat the Japanese and her once fearsome military war machine. Many historians and scholars had debated over the reasons that led to the Japanese unconditional surrender at the end of the Second World War. Many looked along the ideas of strategy and tactics, some pointed toward the direction of leadership, and a great many focused around the Manhattan Project that gave America nuclear capability. Being a student of the economics discipline, I, with this paper, would instead prove to the readers that the economic conditions played as an important role as the others, in which the American economy determined the outcome of the war in the Pacific. This paper would be helpful in proving so, leading to the conclusion which would state that the American economy was the real reason that led to the eventual defeat of the Rising Sun."
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Star Formation, 2004.
A look at the processes that cause the birth and life of stars.
1,515 words (approx. 6.1 pages), 6 sources, MLA, $ 49.95
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Abstract
The process of star formation is a complex one that takes millions of years to complete. While there are many types and sizes of stars, all come from the same basic properties. From clouds of gas and dust to protostars to the Main Sequence, star birth is a process dependent upon many factors. This paper examines how stars are formed and the reasons behind the various colors of stars.
From the Paper
"Stars use nuclear fusion to convert, generally, hydrogen to helium, a process called nucleosynthesis. Nucleosynthesis is the production of new elements via nuclear reactions. The mass of the star at the time of the nuclear fusion determines what types of nucleosynthesis are needed. For smaller stars, hydrogen is converted to helium. For mid sized stars, like the sun, helium is turned to oxygen and carbon, as the hydrogen supply burns out. For massive stars, as hydrogen becomes depleted, helium is turned to carbon and oxygen, which are then turned to neon, sodium, magnesium, sulfur and silicon. Later, those elements are transformed to elements like calcium, iron, nickel, chromium, copper, and other elements. It is this process of nuclear fusion and nucleosynthesis that allow stars, even massive, old stars, to continue to exist. It is this stage that is called the Main Sequence for a star (Enchanted Learning, 100)."
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The Star System and Hollywood PR, 2007.
A discussion of the star system and its contribution to the development of Hollywood public relations and advertising strategies.
1,726 words (approx. 6.9 pages), 6 sources, MLA, $ 55.95
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Abstract
This paper explores the creation of the Hollywood star system, set up to encourage people to go to the cinema. This system, beginning in the 1920s, transformed the film actor into a kind of popular studio 'brand', which kept audiences coming back. The paper notes that the Hollywood star system contrasted with European cinema culture, which tended to be far more director- (rather than star-) driven and less oriented toward developing a brand. Finally, the paper discusses how the star system has contributed to Hollywood's enduring success, as is evident in today's star-centered movie culture.
Outline:
Introduction
Origins of the Star System
1920's: Rise of Star Power
Conclusion: The Breakdown of the Star System
From the Paper
"The Impact of the Star System on Film The star system is so intimately intertwined with Hollywood of the pre-World War II era that celluloid and stars cannot be separated. Indeed, the Star System is what created an American dominance in a medium that was, after all, developed by the French and Germans, and in which the Americans were relative latecomers to the genre.
"The Star System is about more than the actors who played in Hollywood films. The stars were those special beings who created a link with their audiences. In many cases, and particularly during the silent movie era, the stars' draw was universal: Charlie Chaplin (a British native but naturalized American) was a universal "brand," known as Charlie around the world (and "Charlot" in the French-speaking world), equally powerful in Berlin or Miami.
"There is only one Hollywood in the world. Movies are made in London, Paris, Milan and Moscow, but the life of these cities is relatively uninfluenced by their production. Hollywood is a unique American phenomenon with a symbolism not limited to this country. It means many things to many people. For the majority it is the home of favored, godlike creatures (Powdermaker)."
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Star and Speed Motifs in "Romeo and Juliet", 2005.
Discusses instances of star and speed motifs found in "Romeo and Juliet" by William Shakespeare.
3,383 words (approx. 13.5 pages), 1 source, MLA, $ 96.95
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Abstract
Stars and their metaphorical relationship to fate is a major theme in "Romeo and Juliet" by Shakespeare. The paper shows that stars are mentioned throughout the play in various circumstances that are indicative of fate and the foreshadowing of events. It also looks at another theme present throughout the work, that of speed. The speed at which events happen and the fate controlling those events have an enormous impact on the lives of Romeo and Juliet.
From the Paper
"When Romeo meets Juliet at the Capulet's feast, he is only able to spend a very short amount of time with her before Benvolio rushes him away with, "Away, begone; the sport is at the best" (1.5.119). We see the same haste in the nurse's dealing with Juliet. The nurse realizes who Romeo is and discourages Juliet from speaking to him. She urges the girl away saying, "Anon, anon! / Come, let's away; the strangers all are gone" (1.5.143-144). So here the pressing issue of time is affecting the first encounter between Romeo and Juliet. All of their encounters with one another throughout the play will take place in the same rushed manner. This first meeting of the two foreshadows the rest of their time together."
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" Star Trek and Sacred Ground", 2002.
Reviews the popular 1960's "Star Trek" television series and the guiding values behind the show.
650 words (approx. 2.6 pages), 1 source, $ 26.95
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Abstract
This is a review of "Star Trek and Sacred Ground". The "Star Trek" series and films are marked by an evolutionary process whereby by religion as irrational and mere superstition is displaced by religion with meaning and possible value. Above all, the portrayal of religion reflects Roddenberry's "guiding values: a love of humanity and an optimism concerning the human prospect".
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