...times that of the Earth’s sun. Some of the most common stars are the orange, yellow, brown, blue, or white dwarf star. The lifespan of an average star is mostly around 10 billion years. All of the average stars come from the same place; a Stellar Nebula. A average star is pretty much a ball of hot gas/ plasma which is held together by gravity. If one of these stars has more mass it will explode into a supernova and collapse into a neutron star or a black hole. Planetary Nebula When a star shucks off it’s outer layers it creates a beautiful mixture of gas and dust which is called a Planetary nebula. Only 10,000 of these exist in the milky way and they don’t live very long, there has only been about 1,500 found while the rest are behind interstellar dust. The center of the nebula, the leftover part of the star, where it came from, can usually still be seen. A planetary nebula is very similar to a Stellar nebula but Stellar Nebula forms stars and a Planetary Nebula is formed from stars. The lifespan of a Planetary Nebula is about 5 Billion years. Massive Star Massive stars are born the exact same way average stars are, from a Stellar Nebula. A Massive Star is born if the cloud of dust is bigger than normal which will produce a Massive Star. A star is considered massive if it is eight times more massive than the sun. A Massive Star has an extremely high temperature it will be bright and luminous but its hydrogen will only last millions of years. Until the hydrogen in the core is...
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...Objects in the galaxy, such as stars, planets, and even our solar system, are all made of and started off as clouds of gas and dust in space called nebulas. Then, according to (The life cycle of a star), the gravitational force of the nebula attracts surrounding interstellar mediums, or gas and dust within space to gather together and then towards the nebula. Within this process, the mediums not only cause the nebula to become denser but also creating pressure from the gas, triggering a temperature increase and expansion of the nebula. At this point, the nebula is called a protostar, where it is in the process of becoming a formal star. Then, as gas\\ and dust are collected sufficiently and the temperature of the protostar has reached a certain...
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...Armando I Cortes Nov. 17. 2025 Mrs.Lisa Smith The Formation of a Star The basic idea of star formation is gravitational collapse – the contraction of a region of gas under the influence of gravity. This is a simple process that would be expected to occur in any region of material dense enough for collisions between atoms to radiate away energy. However, the gas must be dense enough for collisions to occur and the temperature must be low enough for the atomic velocities not to be able to escape the system's gravity, so star formation only occurs in a few areas. The sites of star formation in the galaxy are mostly located within molecular clouds – expansive, cool clouds of mostly hydrogen and helium gas. Molecular clouds are on average too diffuse to contract gravitationally, but within a cloud are regions of locally higher density, which are the sites of active star formation. It is not known exactly what causes molecular clouds and star-forming regions to be distributed as they are. However, it appears to be related to the spiral-arm structure of spiral galaxies, which is thought to be the result of density waves passing through the disk, compressing matter and igniting star formation in their wake, leaving the trails of young, hot, blue stars in their wake that are the primary feature of spiral galaxies. The distribution of gas in these regions is probably erratic enough that once a sufficient compression comes through a large number of separated...
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...Last update on September 24th 2015 Wish that I could say these words tonight Wish I have the courage, wish I might Have the chance to show you, speak what's on my mind While you're right next to me, I've loved you from the start Wish that I could walk you down the road Share each moment, have my hand to hold My imagination's, beginning to unfold Every wish is granted, every dream and hope Wish I may, wish I might find a way to your heart Wish that I'll be the sun to warm you all through your life Wish you may feel my love that is hidden in the stars Wish I may, wish I might be the one Maybe now I'm ready to be found That I'll be a part of who you are A promise of forever, never break your heart Always there to listen, always by your side Wish I may, wish I might find a way to your heart Wish that I'll be the sun to warm you all through your life Wish you may feel my love that is hidden in the stars Wish I may, wish I might be the one (Wish I may, wish I might find a way to your heart wish that I'll be the sun to warm you all through your life) Wish you may feel my love that is hidden in the stars Wish I may, wish I might be the one Wish I may, wish I might be the one...
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...important stars are given a special status in the field of celestial navigation. Of the approximately 6,000 stars are visible to the naked eye, the chosen stars are among the radiant and span thirty eight constellations of the celestial sphere. Most of the chosen stars were named in antiquity by the ancient Arabs, Greeks, Romans and Babylonians. Polaris “North Star”, is treated specially due to its proximity to the north celestial pole. All of stellar evolution can be understood from one simple rule: A star is always under the influence of its own gravity and is trying to make itself as small as possible. All the stages along the way can be described as pauses in the shrinkage. A star begins by collapsing out of the turbulent mixture of interstellar gas and dust. (The Main sequence is by far the longest stop in its life history.) The burning of hydrogen into helium builds so much internal pressure that the great squeeze is temporarily halted, and the star stabilizes along the left-hand edge of the band, on a locus called zero-age main sequence, or ZAMS. Just like human beings, however, stars are always aging and evolving. It’s just a matter of degree, at the rate at which transformation occurs. As they are born, stars begin using its finite fuel supply, and therefore must change. The close balance in the core between the diminishing fuel supply and the increasing burning rate maintains stellar luminosity. Without this stability stars would change instantly. (The Balance isn’t perfect)...
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...The Star: Summary The story opens with the unnamed first-person narrator musing that at one time he had believed that his travels in outer space could not alter his faith in God. The reader learns that he is a Jesuit as well as an astrophysicist. He is aboard a starship returning from a scientific mission three thousand light-years from Earth. Something he learned on this mission, as yet unknown to the rest of the scientists and crew, has caused him to question his faith. He reflects regretfully that the data gathered on the mission will soon make the cause of his own doubt—‘‘this ultimate irony’’—known to everyone. The narrator reflects on the ‘‘private, good-natured, but fundamentally serious war’’ that the largely irreligious crew has waged with him during the long mission. He thinks particularly of the ship’s doctor, Dr. Chandler, who sometimes professes himself willing to believe that ‘‘Something’’ created the infinite vastness of space and everything in it, but cannot accept that a being so powerful could possibly care about ‘‘us and our miserable little world.’’ The narrative goes on to reveal more details about the mission. The ship had been sent to examine the aftermath of a supernova—the explosion of a star, during which it burns with an intensity and a luminosity that may be a billion times that of the Earth’s sun. Following such an explosion, a star becomes a white dwarf, a body of very dense matter. These scientific details are imparted almost incidentally as the...
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...turns into an average star there is only one way the cycle will end, unlike when the Nebula turned into a massive star. The red giant will turn into a Planetary Nebula which will then turn into a white dwarf. A white dwarf is what a star like the sun will become after it will have exhausted its nuclear fuel. An example of a white dwarf is Sirius B. White dwarfs are mostly made of carbon and oxygen. There is no nuclear fusion in a white dwarf. Although a Nebula is the starting point for a star it has to be formed somehow. Universe today explains how a Nebula is formed by saying, “ A nebula is formed when portions of the interstellar medium undergo gravitational collapse. Mutual gravitational attraction causes matter to clump together, forming regions of greater and greater density. From this, stars may form in the center of the collapsing material, who’s ultraviolet ionizing radiation causes the surrounding gas to become visible at optical wavelengths.” Some facts that you might not have known about a Nebula is that the word Nebula is a Latin word that means cloud. They also may stretch over light years across the galaxy. The first Stellar Nebula was discovered by Charles Messier. Stars can form inside of a Nebula. A star can be formed in a Nebula when gas and dust...
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...Name Instructor Course Date Dark Nebulae Dark nebulae are nonluminous nebulae that are observable since it obscures light from other sources. Nebulae are diffuse clouds of interstellar dust and gas. The shape, size, and characteristics of nebulae may vary significantly because some are the remains of dead stars and others are star nurseries. Dark nebulae are found in areas with no nearby stars. These clouds do not emit or reflect enough light for them to be visible. In fact, the view from the stars behind them is usually blotted out by the dust particles. This paper will exclusively explore on dark nebulae. Normally, these clouds range from 1-10 AU and are less dense than the deepest vacuum in the laboratories of the Earth. They are also thick such that they obscure light from the stars behind them. However, the size of these clouds can be from a few light years up to 600 light years. Additionally, the total mass of dark nebulae can reach several million masses of solar. These clouds can appear to be big depending on the number of stars in it. If there are many stars, the clouds will appear huge, but it can appear small if there are a few stars in it. These clouds existed from a long time ago. Claudius Ptolemaeus did the first record of stars that appeared to be nebulous around 150 AD. Since then, many astronomers have continued discovering these clouds until an American astronomer Beverly Turner Lynds compiled and published a survey of dark nebulas in the year 1960. However...
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... Good Morning/afternoon Dr Henderson and 10C, today i am going to be presenting a speech about a space topic. My choose topic is the dark flow. In todays presentation I will be explaining and defining exactly what the dark flow is as well as its possible causes, theories and just how much limit of understanding we have on the phenomenon. The dark flow is an astrophysical term to describe a force which can not be explained by any of the known gravitational forces in the observable universe and is responsible for moving whole clusters of galaxies in convoy towards a single point in space between constellations Centaurus and Vela. In 2008 NASA scientists came across the dark flow while studying some of the largest structures in the cosmos. According to standard cosmological models the motion of galaxy clusters should be randomly distributed in all directions. When scientists analysed WMAP data they discovered that clusters were moving 3.2 km per hour towards a single region in space. This motion is separate from the expansion of the universe and does not change as distance increases. Scientists came to the conclusion that whatever is driving the movement of matter must lie beyond the observable universe. We do not know what the exact cause of the dark flow is due to our limited knowledge and research access, although some theories have been conducted. Astrologers have a theory called inflation posits that the universe we see is just a small segment of space time that got...
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...Life cycle of a star by Taris Bonner Stars begin as nebulae. Nebulae are clouds of gas and dust that have went through gravitational collapse, under their own gravity, then begin to stick or clump together to become thicker and more dense. Stars then begin to form in the center of the collapsing material. Which then allows its ultraviolet rays to glow or shine making them visible to the eye in color. Nebulae can have a variety of size. They can even be hundreds of light years in diameter, though they are less dense than the space surrounding them. An average star is formed when a cloud of dust or nebulae begins to collapse on itself, then a star is born. An average is a star with average mass or intermediate mass. It can be yellow, orange, blue or white, depending on the surface temperature. They live from 10 to 15 billion years. The sun is a middle aged average star. Next, a star becomes a red giant. A red giant is a reddish color as said in the name but has a little bit of orange on it. Red giants are really big and can expand outward. They can have measures of diameter from 100 million to 1 billion kilometers. Stars spend about a few thousand years to one billion years as a red giant. Once they run out of fuel they die a fiery death. Therefore with the “explosion” of the red giant you’re back at the nebula stage, but it’s called the planetary nebula stage. A planetary nebula is formed by the sun shedding the outside layers into space. Then the pieces are heated up and begin...
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...Sunspots are dark spots seen on the surface of the Sun. They vary in size and have been identified since Galileo observed the sun with a telescope for the first time. Sunspots appear dark as they are cooler than their surroundings.4 It is believed that sunspots are actually locations of disturbances in the magnetic field lines on the surface of the Sun, as they are linked by magnetic loops that extend upward into the solar atmosphere. Sunspots normally travel in connected pairs and the area around them is surrounded by powerful activity known as the active region.7 As there is intense field activity within a sunspot, the convection of heat to the surface is prevented, therefore reducing the sunspot’s temperature. This is why sunspots are about 1500 degrees Kelvin (K) cooler than their surroundings.4 Sunspots normally last several days or weeks and there is a sunspot cycle that occurs as the solar cycle is carried out. The frequency of sunspots increases and decreases in a cyclical pattern. Sunspots are the easiest features to observe and so the sunspot cycle is closely monitored in order to track the solar cycle. 4...
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...TF essay A/ Write a passage 1. Airplanes and helicopters can be used to saved people’s lives. First helicopters can be used for rescuing people in trouble. Try to imagine, when you’re lost in the dense forest or in the mountaintop, airplanes and helicopters are very essential. At that time, they’re your last hope! Second, planes can transport food and supplies when disasters- earthquake, volcano, flood, etc- strike. Third, both types off aircraft can transport people to hospitals in emergencies. For example, transform suddenly, blood poisoning, cardiac infarction, etc. Finally, helicopters and airplanes can be used to provide medical services to people who live in remote areas. They haven’t full live. They are destute of many things. So, people in the cities want to collect for them. But, the transportion by cars or trains is not simple and very long. That is why people need the helping of aircraft. In summary, airplanes and helicopters are very useful to save people. 2. Studying in another country is advantageous in many ways. A student is exposed to a new culture. He or she is able to have knowledge about that country’s condition of life, festivals, etc. That student’ll be in contact with many interesting and useful things. He or she can tell his/her friends in this country about traditional culture of their country and scenic beauties,etc. That’s also a form of cultural exchange among 2 countries. Sometimes he or she can learn a new language. Learning a new...
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...Case Study – Effective Communication: Partnership in Italy Melissa Chang was asked to travel to Venice, Italy and meet with her company’s partnering company. Preparation for the trip was stressful. Not only had her colleague cancelled their recent trip to Moscow at the last minute, making the US partner look bad, but the Italian partner had made several requests for information which none of Melissa’s colleagues had fulfilled. She learned all of this information upon making phone contact with their office to confirm her travel plans. After that initial phone call, Melissa was not looking forward to the trip. She felt that her company had not upheld basic business standards, and adding a language barrier to the equation did not make things any smoother. She was very hesitant to make the trip and felt very guarded. She knew her Italian counterparts were frustrated and she could relate to their feelings. However, she also had a job to do – get more work out of them. If things did not get cleared up quickly, they could potentially loose the partnership. Melissa dreaded having to be the one to deliver that piece of news. Once in Venice and face-to-face with the partners, Melissa quickly realized their source of frustration. From their perspective, the US partner had not upheld their end of the business deal by providing some basic product information. Melissa had that information with her and easily provided the files. She was able to answer all their questions...
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...As we know, not everybody may like the same thing as one another. Bob may enjoy the taste of coffee while Mary finds it awful. Everybody is different. Which connects to my next point, we must keep in mind that not everybody has the same motivation to travel. Two people can be travelling to the same destination but with different motives. Being in the hospitality and tourism industry, it is important for us to know what motivates our consumers in order to fulfill and exceed their expectations, and how to better ourselves to ensure they return home happier than before they left. The number one reason as to why consumers have a desire to travel is to fulfill a need what ever that may be. According to Maslow’s hierarchy of needs, a trip may satisfy one’s disparate need. It is important for us to recognize these needs since it will allow for a successful business. When tourism operations meet or exceed the consumer’s expectations, the particular tourism operation can expect repeat business and for the consumers to spread the word to friends and family about the great service. Also, the company will have the ability to maintain or even increase their current service charges. Take Disneyland for example, when Disneyland first opened their doors it cost a few cents to a few dollars to enter the theme park. Decades later, tickets cost nearly hundreds of dollars if not more, yet consumers are willing to pay for their service because they had a great experience, or heard about it from...
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...My Adventurous Journey Travelling has always excited me and when it gets more adventurous it is more interesting. I love travelling and so do my parents. So whenever they get time, we set out for our great journeys that are filled with lots of adventures, fun and excitement. This time we thought we would go trekking. I was so excited that I could not sleep for days. I have only seen in movies and read in books how difficult it is and how one does trekking. My father told me that I would not be allowed great heights and no fuss at the location and so I had no choice, other than listen to him. We, along with our family friends, on our holidays planned our trip and started preparations for it. We used to do our daily exercises so that it would strengthen our bones and muscles for the climb. On the D-day we were so excited that we kids could not control it. With lots of instructions and warnings we stared our journey and the much awaited journey came to an end. When we reached our destination. It was real fun. First we kids were allowed to climb for a small height. It was really adventurous. Stepping on the foot of a mountain to climb it is really exciting. We tried hard, but could not make it to a good height that we could. Then our parents went and they too had a tough time. Slipping and falling and then again retrying, it was all so much fun. We then took a break and tried climbing once again, this time getting better. We were briefed with the risks involved and so...
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