The Life Cycles of Stars In the universe‚ there are hundreds of billions of stars. They are formed when gas and dust from space "clump" together. As the mass grows larger‚ gravity takes over and a core begins to form. The core becomes extremely dense and this compaction causes temperatures within it to rise to the point where nuclear fusion (the burning of hydrogen in a chain reaction) can begin. The heat generated by fusion can reach 24 million degrees F (Fahrenheit). "That amount of heat keeps
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the core as a gaseous shell. The gas that surrounds the core is called a "Planetary Nebula". The core that is left then becomes a "white dwarf". After the white dwarf cools down enough it stops shining and dies‚ forming a "black dwarf". Another life cycle of a star involves a star with a mass of 10 solar masses or more. These stars evolve similarly to stars of about 1 solar mass until they reach "main sequence". The star shines bright until all of its hydrogen has fused to form helium. This takes
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Eventually though a passing star or shock wave from a supernova will disturb the gas and dust. The dust and gas may then start to clump together‚ gravity will then clump more and more gas together‚ this is when the star starts the next part of its life cycle. Protostar: A protostar is when the gas has clumped together and it getting hot but has not reached what is known as critical mass. At this point the gas will be hot enough to glow. but since there is still a large amount of dust su
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every type of environment. Edoga got bored so he made humans‚ but they need some sort of cycle and that makes everything change so he created mythical beast.
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Organizational life cycle Prof.univ.dr. Ion Gh. ROŞCA Prof.univ.dr. George MOLDOVEANU Academ de Studii Economice din Bucureşti Abstract This paper proposes an analogy between rational biological model and the organizations’ development during their existence. So‚ organizations’ "born" or creation are considered the result of genetic algorithms‚ transformations are identified with changes that aim the adapting to the environment‚ and finally the ”death” treats the state of
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4 Do you use a shampoo? A- Yes (2) B- No (0) View Details Download this question Download data(Format 1) Download data(Format 2) 5 From the 10 shampoos given below which one do you prefer the most? A- Pantene (0) B- Fiama Di Wills (0) C- Garnier (0) D- Vatika (0) E- Sunsilk (0) F- Head and shoulders (0) G- Clinic all clear (0) H- Himalaya (0) I- Dove (1) J- Clinic plus (0) K- Home made herbal shampoo (1) L- Any other
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Dove: Evolution of a brand Case write up Sources: Dove: Evolution of a brand‚ Harvard Business School case 9-508-047‚ 2008; Dove`s big ideal: from real curves to growth curves‚ 2009 (IPA); Social Media‚ Harvard Business School case 9-510-095‚ 2011 Question 1: How did Dove`s brand positioning change from the mid 2000`s? Functional era Prior to the establishment of Dove as a Masterbrand in February 2000‚ the brand was positioned differentiated in the health and beauty sector. The brand
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GARNIER SHAMPOO PROJECT OBJECTIVE: The objective of our project is to comprehensively research on one of the most successful sub-brands of L’Oreal- GARNIER. * Within Garnier‚ we have incurred a study on the hair care product range of Garnier that is Garnier Fructis and Ultra Doux. We have essentially focused on shampoos and conditioners. * We have researched on the brand perception of the product by the customers and customer loyalty towards the product. * The stress however has been
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Mars Dove Chocolate Brand Audit IMC 613 Brand Equity Management Chocolate is one of America’s favorite treats‚ and companies like Hershey’s‚ Ghirardelli and Dove‚ have captured consumers minds‚ body and emotions with delicious tasting chocolates for more than 100 years. After examining three brands in Dove’s competitive set- Hershey’s‚ Ghirardelli and Unilever Dove- it became obvious that the Dove Chocolate brand has an unfavorable brand association with Unilever Dove soap and does not resonate
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LIFE CYCLE OF A STAR Stars are formed in nebulae‚ interstellar clouds of dust and gas (mostly hydrogen). These stellar nurseries are abundant in the arms of spiral galaxies. In these stellar nurseries‚ dense parts of these clouds undergo gravitational collapse and compress to form a rotating gas globule. The globule is cooled by emitting radio waves and infrared radiation. It is compressed by gravitational forces and also by shock waves of pressure from supernova or the hot gas released
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