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What is the theorized life cycle of a star
Life Cycles of Stars essay
The life cycle of stars essay
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The Life Cycle of Our Star
Nebula
What is a nebula? A nebula is the birth of a new star. Cloud of gas and dust in space.
Mostly made up of Hydrogen and Helium. The cause of a nebula has come from a huge collapse of gas, also known as Interstellar Medium. A nebula’s lifecycle is less than 1 million years old before they burst into a supernova.
Because of gravity Nebula forms a star
Protostar
Giant clouds form around a star that creates pressure--nebula. Differences in temperature create a gravitational collapse which creates protostar
A protostar is formed when gravity causes the dust and gas of a nebula to clump together in a process called accretion
As gravity continues to pull ever more matter inward towards the core, its temperature,
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This is the beginning of a new star. It is a giant cloud of dust and gas that is mostly made up of hydrogen and helium. The creation of a Nebula is caused by a collapse of gas, also known as Interstellar Medium. A Nebula can live up to a million years old before they turn into a …show more content…
That’s older than my grandma,” said Ralphie.
“Excellent observation Ralphie,” said Ms. Frizzle. 3 page
PROTOSTAR
“Aside from Ralphie’s sidecomment, we are now moving on to the second stage of a star, the Protostar,” said Ms. Frizzle.
This is the protostar. A process called accretion occurs when a gravitational collapse causes dust and gas of a nebula to clump and then a protostar is formed. Say a star has an equivalent weight to our sun, that means that that star was a protostar for more than 10 million years. During the process of a protostar, gravity pulls more matter inward towards the core, which cause its pressure, density, and temperature to rise. Nuclear Fusion then begins once the high temperatures in the core of a protostar is reached, from then, a star is born.
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STABLE STATE
At last, we have reached the most relaxed area of a star. This area is called the Stable State. Our star, the sun is currently at its stable state and will be for another 3-5 billion years. The stable state is the longest period of the life of a star. When a star is at it’s stable state, it is constantly burning its fuel out. Once all the fuel burns out of the star, it means that the star has reached the red giant
The Lagoon Nebula featured as Nasa’s astronomy picture of the day was photographed by John Nemcik using various filters to capture the light emitted by the Hydrogen, Sulfur, and Oxygen. While photographed showing beautiful vibrant, eye-catching colors, the Nebula would appear naturally appear gray to human eye due to poor color sensitivity existing at low-light levels (spacetelescope.org). The Lagoon Nebula is home to the formation of new stars, as well as several other interesting phenomena such as Bok globules, and the hourglass nebula. It is these regions of the nebula that make it a continuous area of interest and study for astronomers.
Another group of stars, which are rather small, is found near the bottom left of the H-R Diagram.
Furthermore, there are five main types of nebulae; they include emission, reflection, planetary, dark and supernova remnants. Each type appears in a vast array of shapes, sizes and form in different ways. The unique appearance of each nebula depends on temperature, density and how the dust is spatially arranged with respect to the viewer. Although all nebulae are forms of interstellar matter some of them formed from the death of stars while others formed from atoms and simply reflect the light from the nearby stars.
Nebula away so that it can avoid certain things. In the short story, “The Star,” the priest stated,
Stars are born and reborn from an explosion of a previous star. The particles and helium are brought together the same way the last star was born. Throughout the life of a star, it manages to avoid collapsing. The gravitational pull from the core of the star has to equal the gravitational pull of the gasses, which form a type of orbit. When this equality is broken, the star can go into several different stages. Some stars that are at least thirty times larger than our sun can form black holes and other kinds of stars.
The Orion Nebula is a spectacular sight. Consequently, it has been a preferred target of the Hubble Space Telescope (HST) over recent years. The HST has provided a great deal of insight into the complicated process of star formation. In June of 1994, C.
Solar nebula is a rotating flattened disk of gas and dust in which the outer part of the disk became planets while the center bulge part became the sun. Its inner part is hot, which is heated by a young sun and due to the impact of the gas falling on the disk during its collapse. However, the outer part is cold and far below the freezing point of water. In the solar nebula, the process of condensation occurs after enough cooling of solar nebula and results in the formation into a disk. Condensation is a process of cooling the gas and its molecules stick together to form liquid or solid particles. Therefore, condensation is the change from gas to liquid. In this process, the gas must cool below a critical temperature. Accretion is the process in which the tiny condensed particles from the nebula begin to stick together to form bigger pieces. Solar nebular theory explains the formation of the solar system. In the solar nebula, tiny grains stuck together and created bigger grains that grew into clumps, possibly held together by electrical forces similar to those that make lint stick to your clothes. Subsequent collisions, if not too violent, allowed these smaller particles to grow into objects ranging in size from millimeters to kilometers. These larger objects are called planetesimals. As planetesimals moved within the disk and collide with one another, planets formed. Because astronomers have no direct way to observe how the Solar System formed, they rely heavily on computer simulations to study that remote time. Computer simulations try to solve Newton’s laws of motion for the complex mix of dust and gas that we believe made up the solar nebula. Merging of the planetesimals increased their mass and thus their gravitational attraction. That, in turn, helped them grow even more massive by drawing planetesimals into clumps or rings around the sun. The process of planets building undergoes consumption of most of the planetesimals. Some survived planetesimals form small moons, asteroids, and comets. The leftover Rocky planetesimals that remained between Jupiter and Mars were stirred by Jupiter’s gravitational force. Therefore, these Rocky planetesimals are unable to assemble into a planet. These planetesimals are known as asteroids. Formation of solar system is explained by solar nebular theory. A rotating flat disk with center bulge is the solar nebula. The outer part of the disk becomes planets and the center bulge becomes the sun.
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).
A star begins as nothing more than a very light distribution of interstellar gases and dust particles over a distance of a few dozen lightyears. Although there is extremely low pressure existing between stars, this distribution of gas exists instead of a true vacuum. If the density of gas becomes larger than .1 particles per cubic centimeter, the interstellar gas grows unstable. Any small deviation in density, and because it is impossible to have a perfectly even distribution in these clouds this is something that will naturally occur, and the area begins to contract. This happens because between about .1 and 1 particles per cubic centimeter, pressure gains an inverse relationship with density. This causes internal pressure to decrease with increasing density, which because of the higher external pressure, causes the density to continue to increase. This causes the gas in the interstellar medium to spontaneously collect into denser clouds. The denser clouds will contain molecular hydrogen (H2) and interstellar dust particles including carbon compounds, silicates, and small impure ice crystals. Also, within these clouds, there are 2 types of zones. There are H I zones, which contain neutral hydrogen and often have a temperature around 100 Kelvin (K), and there are H II zones, which contain ionized hydrogen and have a temperature around 10,000 K. The ionized hydrogen absorbs ultraviolet light from it’s environment and retransmits it as visible and infrared light. These clouds, visible to the human eye, have been named nebulae. The density in these nebulae is usually about 10 atoms per cubic centimeter. In brighter nebulae, there exists densities of up to several thousand atoms per cubic centimete...
Our solar system, as we see it today, originally formed from the collapse of a very cold and low-density cloud of gas. The mass of this cloud was composed of 98% hydrogen and helium, 1.4% hydrogen compounds, .4% rock, and .2% metal. The nebula was thought to be a few light years across and was roughly spherical in shape. The cloud was in a state of balance, it was neither contracting or expanding, until a cataclysmic event, most likely a supernova, created a shock wave through the nebula, resulting in an area of higher mass. Once this area became more massive than the rest of the nebula it begin to collapse with the area of hig...
In 1610, two years after the invention of the telescope, the Orion Nebula, which looks like a star to the naked eye, was discovered by a scholar named Nicolas-Claude Fabri Peiresc. In 1656 Christan Huygens, the Dutch scholar and scientist, using his own greatly improved instruments, was the first to describe the inner region of the nebula, and to determine that its inner star is not single but a compact quadruple system.
In this state the outward force of the fusion balances inward force of gravity thus balancing out the star for about 90% of its lifetime. The life of a star depends on how massive the star is. Larger stars have hotter centers and will burn through the hydrogen core faster. The largest know stars last only a couple of millions of years. Smaller stars, like our own Sun, have cooler cores and burn the fuel at a slower rate and will last for billions of years. The smallest stars or dwarf stars burn so slowly that they could potentially last 100 billion years in their adult stage. For comparisons sake think of large stars as an F-150 and a smaller star as a Prius, although the F-150 has a larger tank it will burn through the fuel faster than the Prius with the smaller tank will. After a star’s fuel core is exhausted it will experience a
Generally, the universe began as a composition of radiation and subatomic particles, which proceeded with galaxies formation. Galaxies are made up of hydrogen, helium, 100-200 billions of stars, planets and most having a black hole at the center, which attracts everything present in galaxies by force of gravity. Galaxies can be classified as either spiral (Milky Way- galaxy which human kind has been found to exist), elliptical, lenticular and irregular, where the structure is determined by neighboring galaxies with most galaxies are moving away from each other. Classification of galaxies is being conducted by online programs such as Galaxy zoo, using pictures from telescopes and is making significant progress.
It is not understood well, but in some supernovae the gravity is so intense within the red supergiant that the electrons are forced into the atomic nuclei where they combine with protons to form neutrons. The electromagnetic forces keeping apart the seperate nuclei are gone and the entire core becomes a dense ball of neutrons or an atomic nucleus about the size of Manhatten called a Neutron Star. If the mass is great enough though, when the star turns into a red supergiant it will collapse under its on gravity into a radius smaller than the Schwarzchild Radius and turn into a Black Hole.
Solar System:The solar system has a collection of nebulas along with multiple planets,moons, stars,comets, meteoroids and asteroids. There are eight main planets in our solar system with a moon or many moons orbiting it. There are other planets in the solar system that are smaller and they’re called dwarf planets, they also have moons in their orbit. They’re stars being formed by nebulas everyday in this solar system along with comets, meteoroids and asteroids charging around, blasting into planets at high speeds.