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Stars formation and existence
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Cosmic Nurseries - Mommy, Where do Stars Come From?
Since my entire thesis for this paper is about how a star is born, I guess the first thing I should start out with is by telling you exactly what a star is. Stars are self-luminous gaseous spheres. They shine by generating their own energy and radiating it off into space. The stars' fuel for energy generation is the stuff they are made of --hydrogen, helium, carbon, etc. -- which they burn by converting these elements into heavier elements. Nuclear fusion occurs, which is when the nuclei of atoms fuse into nuclei of heavier atoms.
The energy given off by a star through nuclear burning heatsits interior to many millions and, even in some cases to Pleiades Star Cluster hundreds of millions to billions of degrees Fahrenheit. It causes heat to flow from the interior toward the surface, where it is released out into space and makes the star shine. Because stars are only so big, they will eventually use up their nuclear fuel and run out of energy. (University of Oregon, Unknown)
The first step in making new stars is to compress a cloud in order to strengthen gravity's effect so that the cloud material can contract and break-up into smaller units that eventually collapse to form stars. The clouds in the inter-stellar space are called Inter-stellar Medium, which are mainly made up Rho Ophiuchi of hydrogen and helium. The cloud itself is very cold, somewhere around a hundred degrees Kelvin, which is far below -150ºC. All particles in the cloud attract each other by gravitational force. According to calculations of scientists, a cloud having the mass comparable to the mass of our Sun will be able to hold itself together due to the gravity pushing against it. As traveling compression waves move past a cool molecular cloud, it compresses the cloud, driving the particles closer together. If the compressed cloud has no way to stop the contraction, it’ll continue to collapse and raise the gas pressure sufficiently to resist further contraction. Supernova 1994D Another possible explanation for the contraction that is occurring at this time is due to shockwaves from surround supernovas. (Kippenhahn, 1994).
At this point the contracted interstellar clouds are called Bok globules. Globules are usually a few light years in size and they are made up of hydrogen and dust. “At...
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... even possibly begin to imagine. The hydrogen inside the star is converted into helium by the means of nuclear fusion. Stars that start their lives with masses less than about eight solar masses stop their nuclear burning trip with helium burning at the core. Stars that start their lives with masses greater than about Model of Star’s internal process eight solar masses continue their nuclear burning and go on to produce such products as neon, magnesium, silicon, and sulfur. Eventually, silicon and sulfur ignite in the star's core to form iron and nickel. (Hansen, 1994)
Various info about star at mature stage
In conclusion, before I wrote this paper I would have to say that even though every night when I happen to glance upwards I see a whole bunch of stars, I never even had the slightest idea of where they came from until now. Stars come from these cosmic nurseries that scientists and astronomers refer to as nebulas in one of the oddest ways imaginable. I learned quite a bit about where stars come from and I hope to continue to learn even more about stars in the not so distant future.
Brown dwarfs are objects in space that sit between the lines of being a star and a planet. This object is dim and hard to distinguish from low mass stars at the early stages of the dwarf’s life. They are often called failed stars because they start their life the same way as regular stars. However, in some stage, they just didn’t have enough mass gathered to generate the fusion-powered energy of a star. Scientists are certain that brown dwarfs are the missing link between stars and planets but the formations of dwarfs are still a mystery.
Stars explode at the end of their lifetime, sometimes when they explode the stars leave a remnant of gasses and, dust behind. What the gasses come together to form depend on the size of the remnant. If the remnant is less than 1.4 solar masses it will become a white dwarf, a hot dead star that is not bright enough to shine. If the remnant is roughly 1.4 solar masses, it will collapse. “The protons and electrons will be squashed together, and their elementary particles will recombine to form neutrons”. What results from this reaction is called a neut...
The Orion Nebula contains one of the brightest star clusters in the night sky. With a magnitude of 4, this nebula is easily visible from the Northern Hemisphere during the winter months. It is surprising, therefore, that this region was not documented until 1610 by a French lawyer named Nicholas-Claude Fabri de Peiresc. On March 4, 1769, Charles Messier inducted the Orion Nebula, M42, into his list of stellar objects. Then, in 1771, Messier released his list of objects for its first publication in Memoires de l’Academie.1
Stars are born in the interstellar clouds of gas and dust called nebulae that are primarily found in the spiral arms of galaxies. These clouds are composed mainly of hydrogen gas but also contain carbon, oxygen and various other elements, but we will see that the carbon and oxygen play a crucial role in star formation so they get special mention. A nebula by itself is not enough to form a star however, and it requires the assistance of some outside force. A close passing star or a shock wave from a supernova or some other event can have just the needed effect. It is the same idea as having a number of marbles on a trampoline and then rolling a larger ball through the middle of them or around the edges. The marbles will conglomerate around the path of the ball, and as more marbles clump together, still more will be attracted. This is essentially what happens during the formation of a star (Stellar Birth, 2004).
Shklovskii, Iosif S. Stars: Their Birth, Life, and Death. Moscow: Central Press for Literature in Physics and Mathematics, 1975.
The Big Bang, the alpha of existence for the building blocks of stars, happened approximately fourteen billion years ago. The elements produced by the big bang consisted of hydrogen and helium with trace amounts of lithium. Hydrogen and helium are the essential structure which build stars. Within these early stars, heavier elements were slowly formed through a process known as nucleosynthesis. Nucleosythesis is the process of creating new atomic nuclei from pre-existing nucleons. As the stars expel their contents, be it going supernova, solar winds, or solar explosions, these heavier elements along with other “star stuff” are ejected into the interstellar medium where they will later be recycled into another star. This physical process of galactic recycling is how or solar system's mass came to contain 2% of these heavier elements.
After a supernova, the core is likely to travel someplace else within space. When the core is less size than about 5 solar masses, the neutrons will halt the collapse of the star. This will create a Neutron Star. Neutron stars are observed as pulsars or X-ray binaries. When the core is very large, nothing that h...
The Sun is the star that is closest to the Earth, and is the source of a great deal of our energy. The fusion of hydrogen ( H) and helium (He) is part of what gives the sun or any star its shine. This happens when energy is released during the reaction.
Stars are one of the most widely recognized astronomical objects in the known universe. These celestial bodies are the building blocks of galaxies and their age, composition, and distribution are used to trace their galaxy’s history. Stars are also responsible for the existence of heavy elements such as carbon, nitrogen, oxygen, and iron. These elements are the result of the thermonuclear fusion that takes place in the stars’ cores over millions to trillions of years, making them the most effective and productive nuclear reactors in the the cosmos. In the case of the solar system stars also provide the light and heat required to support life which is a near impossible and extremely rare phenomenon. Stars are extraordinary objects in the entirety
Stars are born using the ingredients of hydrogen and gravity. Nebulae, clouds of stardust and gas, are “star nurseries where m...
Human fascination with the stars is as ancient as Babylonians and has been suggested to be older than Stonehenge. From “be fruitful and multiply” to “live long and prosper,” the instinct to protect and propagate the species has manifested in religion, art, and the imaginations of countless individuals. As human understanding of space treks out of the fantastical and into the scientific, the realities of traveling through and living in space are becoming clearer. Exploring, investigating, and living in space pose an expansive series of problems. However, the solutions to the problems faced by mankind's desire to reach beyond the horizon, through the night sky, and into the stars are solutions that will help in all areas of life on Earth.
The first person to ever observe the Milky Way was Greek philosopher, Democritus, who said the galaxy may consist of distant stars. In 1610, Galileo Galilei used a telescope to study the Milky Way and came to the conclusion that it was composed of billions and billions of faint stars. Then, in 1750, Thomas Wright c...
Movie stars. They are celebrated. They are perfect. They are larger than life. The ideas that we have formed in our minds centered on the stars that we idolize make these people seem inhuman. We know everything about them and we know nothing about them; it is this conflicting concept that leaves audiences thirsty for a drink of insight into the lifestyles of the icons that dominate movie theater screens across the nation. This fascination and desire for connection with celebrities whom we have never met stems from a concept elaborated on by Richard Dyer. He speculates about stardom in terms of appearances; those that are representations of reality, and those that are manufactured constructs. Stardom is a result of these appearances—we actually know nothing about them beyond what we see and hear from the information presented to us. The media’s construction of stars encourages us to question these appearances in terms of “really”—what is that actor really like (Dyer, 2)? This enduring query is what keeps audiences coming back for more, in an attempt to decipher which construction of a star is “real”. Is it the character he played in his most recent film? Is it the version of him that graced the latest tabloid cover? Is it a hidden self that we do not know about? Each of these varied and fluctuating presentations of stars that we are forced to analyze create different meanings and effects that frame audience’s opinions about a star and ignite cultural conversations.
Gravity forces the gases and metals to compress at an increasing speed, until the pressures build up at the core and produce a tremendous amount of heat. This stream of energy causes a huge explosion that sends most of the gases, and metals back into space to form a nebula. During a supernova, heavier metals such as uranium and lead can be produced. The earliest recorded supernova, called SN 185, was discovered by Chinese astronomers in 185 AD.
As per Morrison-Valfre (2013), schizophrenia is described as “a condition associated with disturbing thought patterns, behaviours, and loss of contact with reality to the point at which it impairs functioning”. The psychotic disorder affects approximately 1% of individuals worldwide, resulting in 2.5 million Americans suffering from the mental ailment (Morrison-Valfre, 2013, p.362). Individuals experiencing schizophrenia suffer from many different types, including catatonic, disorganized, paranoid, undifferentiated, and residual schizophrenia (Morrison-Valfre, 2013, p.362). When schizophrenia is diagnosed, individuals suffer from severe adverse effects such as hallucinations, illusions, altered internal sensations, negative self-perception,