Answering Job Interview Questions for Opening Job at Chevron Co Essay

Answering Job Interview Questions for Opening Job at Chevron Co - Essay Example I have identified, developed and technically. I have Teaching and training capabilities as well. 2. Why did you choose your current university and major? What did you find most fulfilling and most difficult about your major? I had identified my aptitude for Engineering as I endeavored in many activities which were connected with the principles of engineering. Many of my hobbies were also closely associated with Engineering. I had participated in a number of co-curricular activities including science exhibitions which helped me develop my attitude towards Engineering. By the time I had to join for graduation I had decided to major in the current subject. My search for a cause effective engineering program ended up in †¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦University as its commitment to action-based-learning attracted me the most. The †¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦ is really an exciting program which can offer me great opportunities to work closely with my classmates and practically learn to face real challenges. I admire the †¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦ learning style which heavily emphasizes on practices and systematic learning cycle. The experience will empower me to be effective ‘in the team’ and ‘in leading the team’. †¦Ã¢â‚¬ ¦Ã¢â‚¬ ¦also holds the legacy of a strong alumni network and the collaborative culture will ensure guidance throughout the career. The most challenging experience about the subject was the vastness of its applicability. This forced me to read and research extensively on the subject. 3. Describe a situation, either professional or personal, where you faced a particular difficulty. What was the outcome, what did you learn from the experience and what would you do differently if faced with a similar situation again? One if the most difficult situations that I had faced were taking forward the voluntary work as the Work Instructor during my high school days. All through my of my High School days, my leadersh ip abilities and my affinity towards the society were proven as I enthusiastically led the show to arrange tutorials and allied events as a part of the voluntary work.  

The life of Peter Research Paper Example | Topics and Well Written Essays - 1750 words

The life of Peter - Research Paper Example During the life of Peter he faced accidental greetings, scenes which were divine and most importantly he faced refusal. Hence it is believed that the story of Peter in the bible is one of the greatest narrations that depict a transformation in the way of life. It has been observed that amongst all the twelve believers Jesus had during His rule on Earth, Peter is considered to be the most candid of all. Undoubtedly he was considered to be the part of the most gallant advocates of the belief. His birth was of a common man but the death was of a great apostle. It has been observed that the start of his life was very modest in origin. As mentioned earlier the original name of Peter was Simon. It was Jesus who improved his name to Peter. The name Peter has literally originated from the term Petra which means "rock". Peter was basically a fisherman from the Galilean times and is apparently the brother of Andrew. Peter and his brother are considered to have their origination from the settle ment of Bethsaida. It is said that Peter was also a follower of John (Baptist). He was married. Before he had experienced divinity was a corrupt and sinful man. The guilt of being sinful was seen at various occasions, especially when he was in the company of Jesus Christ. Peter and his brother Andrew have the honor of being the first believer. (Meyer, 35) Since the fishermen of that time were fierce, bold, fearless, hot tempered and often used abusive language all these aspects were also present in Peter. Since their job requires physical labor which had made them rough and tough. They were full of themselves and had a bossy attitude. Their life was rough and bold as they had encountered various ups and downs in life like storms and thunders which had shaped their personality. Peter before he had met Jesus was lost and did not have any goal in life. But once they found Jesus without any further thoughts they starting to believe Him and followed him. They did not question Jesus Chris t and left everything behind for the sake of being good humans and firm believers. Like I mentioned previously, peter was one of the first believers of Jesus Christ as well as he has the honor of being the spokesman of Jesus at various occasions irrespective of the good or the evil. The thing that separates Peter from any other disciple is the unique vision he possessed which was related to the image of Jesus. Jesus's title that is 'Son of the Living God – The Savior' was also given for the first time by this noble man. He was so humble and considered himself so guilty of the sins he did in his earlier life that he used to feel that he did not deserve to be in the company of such a holy man. The love Jesus had for his him and his brother made them distinct and the â€Å"fishers of men†. There were certain flaws that were associated with Peter. For instance, that the boldness Peter flaunted most of the times became wrong for him. It is said that once he scolded the God and claimed that he could even sacrifice his life for Jesus. Despite this when Jesus was arrested and trialed, Peter refused the Lord around three times. Jesus was insightful and he knew that among his disciples who is actually honest to him and who would ultimately cheat on him. Peter has the honor of witnessing many miracles associated with Jesus from his own eyes. Along with two other disciples he witnessed the Shekhinah Glory during the time of Transfiguration. This is considered to be the time when the humanity

Discussion 4 Essay Example | Topics and Well Written Essays - 500 words - 4

Discussion 4 - Essay Example uring his era for revolutionizing the painting style with his style that was definitive, darkening the shadows and transfixing the subject in a blinding shaft of light. Caravaggio pioneered the method of acute observation of physical and psychological reality in his subjects as the foundation of all the paintings he was commissioned to do. He proved that it was possible to work speedily on a painting. He finished painting the Sistine Chapel, his most notable work still in existence, in a matter of 7 years. He was an expert at working with live models and was frowned upon by his peers because he preferred to paint directly on the canvass rather than drawing sketches on paper and working from those models for the final product. This was a unique skill of Caravaggio that at the time was considered to be detrimental to an artists masterpiece or commissioned work. However, Caravaggio proved his detractors wrong, creating his masterpieces exactly how he saw them, directly on the canvass. Your description of a typical reinassance painting is highly accurate and was obviously well researched. I am in agreement with you regarding the influence of Florentine painters over this particular era of the arts. However, you failed to fully or even partially discuss the actual influences in the painting style of Giotto di Bondone. Although his style was later on classified as Renaissance, there is no information as to which particular aspects of the art form can directly be attributed to him. My research actually shows that there were other artists from the same era who pioneered the same style so it may be likely that Bondone should not be ascribed to as the Father of Reinassance Art. Overall, you presented a very interesting discussion. You failed to present what it was that made the Reinassance Art era special. How these drawings and paintings were defined by the artists of their time and why these became part of the basis of modern art. You did not point out the method by

Passive movements Essay Example | Topics and Well Written Essays - 1500 words

Passive movements - Essay Example To optimise the benefits from the passive movements and passive therapeutic exercises, more experimental evidence needs to be gathered in order to better understand things like specific tissue effects and physiological mechanims of action involved (Frank et al. 1987). A clinical approach utilizing skilled, specific hands-on techniques, including but not limited to manipulation and mobilization, used by the physical therapist to diagnose and treat soft tissues and joint structures for the purpose of modulating pain; increasing range of motion (ROM); reducing or eliminating soft tissue inflammation; inducing relaxation; improving contractile and non-contractile tissue repair, extensibility, and/or stability; facilitating movement; and improving function (AAOMPT, 1999). Some recent research has demonstrated significantly better outcomes for patients who used manual therapy in conjunction with other forms of therapy, such as exercise and proprioception training, than when manual therapy was used alone (Jull et al. 2002). Within manual therapy, the administration of passive movements is generally denoted by the term "mobilization". The APTA (American Physical Therapy Association), and the AAOMPT (American Academy of Orthopedic Manual Physical Therapy) define mobilization as a manual therapy technique comprised of a continuum of skilled passive movements to joints and/or related soft tissues that are applied at varying speeds and amplitudes, including a small amplitude/high velocity therapeutic movement (Olson, 2004). In this essay, we are specifically concerned with joint mobilization, which differs from soft-tissue mobilization (massage therapy) or manipulation (chiropractic). We shall be discussing the specific physiological pathways underlying the manifest effects of passive movements. We shall begin, though, by better familiarizing ourselves with the nature and scope of passive movements as they are employed in a clinical setting. Neurophysiological Response to Joint Mobilization Physiotherapy aims to bring about musculoskeletal rehabilitation. To this end, PT prominently involves the use of a combination of exercise and manual therapy techniques. Joint mobilization is a manual therapy procedure involving loosening up of the restricted joints and increasing their range of motion by providing slow velocity and increasing amplitude movement directly into the barrier of a joint, moving the actual bone surfaces on each other in ways which individuals with compromised musculoskeletal function cannot move by themselves. By subjecting motion-restricted joints to gentle movement through a particular segment of the full range, joint receptors can be by and by reeducated to allow a range of motion. Such release from stiffness happens with a concomitant relief from pain in most cases. Administation of passive movements to an affected joint can lead to restoration of the optimal length of muscle fibres, besides resulting in the reduction of the pain-spasm cycle (American Academy of Orthopaedic Surgeons, 1991). A joint can primarily move in two ways: a) in physiological movements consisting of extension, flexion,

Is Dubai Las Vegas on steroids Essay Example | Topics and Well Written Essays - 3000 words

Is Dubai Las Vegas on steroids - Essay Example This is especially so where the front runners happen to be two great cities, with one resting in the East, that is in the United Arab Emirates (UAE) and the other on the West, that is the United States. The two words, that is, bug and hook have been used symbolically in the description of the mental picture that one has when the two cosmopolitans are mentioned.The mention of the two cities triggers a feeling that is more of an enticement, rather than just a mere attention. The cities are scenarios that capture one’s interests fully.The term bugging is also being used as a slang to signify bulging or growing larger in all dimensions. Dubai and LasVegas both share these two characteristics. From what could be termed as scratch, the two cities have experienced enormous developments in both structural and technological fields, though at different rates, to an alarming level. The following essay gives an outline and a partial analysis of the past, the present and the expected futur e conditions of the cities, their similarities and their differences in terms of social and cultural aspects, and in relation to the definition of freedom. It starts with a description of the history of the two cities. ... Though mainly known for its speedily expanding city, Dubai is also a home to various landscapes ranging from the sand deserts, the coral reefs to the rugged Rock mountains (Quinn, 2006). In history, the Persian Gulf was one of the most relevant trading locations dating back to 3,000BC in the reign of Sumer kingdom, which was a Muslim empire. The kingdom carried out and influenced trade along the Gulf which harbors Dubai, and began civilization with Dubai as one of the trading centers. The trading spot later became an important link between Europe and India to the Portuguese and to the British. Due to numerous attacks by pirates, Dubai and the other neighboring emirates sought protection from the British and this led to the emirates being termed as the Trucial States. At the beginning of the seventeenth century, Dubai’s ruler, who was known as Sheikh Hasher gave a tax relief to the foreign traders. This offered them an incentive to expand their trade by locating their headquart ers to Dubai leading to a boost in development. Some major ports had also been established forming linkages between the trading blocks in the region. An example is the British port which was important in enabling trade between the British and the Indians. A further boost in trade was enhanced by Sheikh Rashid bin Saeed who authorized the dredging of a creek, giving way to larger cargo ships. The city of Dubai was hence born from the trade of imports and exports. This however received a major boost when oil was discovered in 1966. The huge revenues from oil trade transformed the state into one of the richest in the Middle East. When Britain withdrew its reign from the territory,

A diverse and interesting learning environment for all students Essay Example for Free

A diverse and interesting learning environment for all students Essay Accepting attitudes towards all human beings creates a diverse and interesting learning environment for all students. I recall an incident while at a summer program a few years ago. We, the students, were staying overnight on a college campus to participate in seminars that would further our growth and readiness for the future. As part of the program, we were required to stay overnight in the dorm rooms. We were each paired up with one other person who would be our roommate for the two days. I come from a neighborhood that is primarily white so I was pleasantly surprised to learn that I would be sharing a room with someone who was from the Middle East. We quickly settled into our rooms and prepared ourselves for the first of two days of learning activities. My roommate awoke, got up and spread a blanket on the floor to pray. I watched my roommate kneeling on the floor saying words in a language that I didn’t understand. When finished, I asked my roommate about this practice and learned a little bit about the Muslim religion and why prayers are said several times daily. See more: Satirical essay about drugs I also had the opportunity to share a little bit about my own faith. I had a large amount of respect for my roommate because it isn’t easy to pray in front of other people let alone people one doesn’t even know. I also gained respect because my roommate wasn’t ashamed of praying or of the Muslim faith. This experience has helped prepare me for life in a world made up of people from all over the world with different values, viewpoints and religions. My own background and life achievements would add to the diversity of University because I too have valuable ideas and customs that would add to the interesting mix of University life. My ability to gain respect for people who have different life values enables me to be a student of a University that embraces acceptance for other cultures. Even though I would be considered the majority, I welcome the opportunity to learn alongside people from different places.

Implications of the TRAPPIST-1 Discovery

Implications of the TRAPPIST-1 Discovery The Search for Extra-Terrestrial Life in the Universe and the Implications of the TRAPPIST-1 Discovery Abstract Despite the absence of any discovery of life beyond the Earth in the Solar System, or communication in the form of radio signals from beyond the Solar System, humankinds quest to answer the question whether there is life elsewhere in the Universe continues apace. The answer to the question could be tantalizingly close now with some ambitious missions being planned in the Solar System to try and find life itself, and surveys of unprecedented scale being conducted with space and terrestrial telescopes to identify potentially habitable exoplanets showing evidence for the existence of life. One such survey (the TRAPPIST survey) led to the discovery of a nearby solar system with a dwarf star at its centre, and in February this year the existence of seven Earth-sized planets orbiting the star was confirmed, with at least three lying in the habitable zone. Studies are continuing to see if there is evidence for the existence of life on any of these planets, with profound astronomical implica tions. This dissertation considers the question of what is life, before reviewing the history and future of the search for extra-terrestrial life in the Universe. The techniques employed and the results from the TRAPPIST survey are reviewed and the implications of the follow-on studies that are now planned are discussed. It concludes by considering the question whether humankind will ever encounter intelligent life in the Universe.      Ã‚   Thomas Zurbuchen Associate administrator of the Science Mission Directorate at NASA speaking at the press briefing about the TRAPPIST-1 exoplanets in February 2017 The Search for Extra-Terrestrial Life in the Universe Contents 1.Introduction 2.What is Life? 3.Pre-requisites for Life 5.History of the Search for Life Beyond Earth Works Cited References The Search for Extra-Terrestrial Life in the Universe Introduction Despite the absence of any discovery of life beyond the Earth in the Solar System, or communication in the form of radio signals from beyond the Solar System, humankinds quest to answer the question whether there is life elsewhere in the Universe continues apace. Exobiology the search for life or for evidence of it has been stimulated by the extraordinary success of missions to planets and other bodies in the Solar System and the rapid advances that have been made in telescope technology in recent decades. The answer to the question could be tantalizingly close now with some ambitious missions being planned in the Solar System to try and find life itself, and surveys of unprecedented scale being conducted with space and terrestrial telescopes to identify potentially habitable exoplanets showing evidence for the existence of life. One such survey (the TRAPPIST survey) led to the discovery of a nearby solar system with a dwarf star at its centre, and in February this year the existence of seven Earth-sized planets orbiting the star was confirmed, with at least three lying in the habitable zone. Studies are continuing to see if there is evidence for the existence of life on any of these planets, with profound astronomical implications. This dissertation considers the question of what is life, before reviewing the history and future of the search for extra-terrestrial life in the Universe. The techniques employed and the results from the TRAPPIST survey are reviewed and the implications of the follow-on studies that are now planned are discussed. It concludes by considering the question whether humankind will ever encounter intelligent life in the Universe. What is Life? Is there life elsewhere in the universe? Before setting out to answer that question we need to understand what we mean by life. In popular culture extra-terrestrial life is usually characterised by intelligent humanoid creatures with whom mankind can interact and communicate, but one only has to look at the diversity of life on Earth to appreciate that there are countless life forms, each unique and a product of the environment it inhabits. Nor can all life forms on Earth necessarily be described as intelligent, perhaps as defined by the Oxford Concise Dictionary: The ability to acquire and apply knowledge and skills. It is reasonable to assume that an ability to communicate is essential if a species is to be described as intelligent, but intelligence is not a pre-requisite for the development of life. There are many scientific definitions of life, such as that offered by the Merriam-Webster Dictionary; An organismic state characterized by capacity for metabolism, growth, reaction to stimuli, and reproduction. This definition is helpful but it does not explicitly recognise that the ability to evolve, particularly in a changing environment, is vital for the development of sustainable life. Mankind has expended considerable effort over the millennia trying to understand the cosmos. The ancients saw it as a place inhabited by the gods, but as astronomy developed, and with it our understanding of the Solar System and the Universe, we began to ask the question, Are we alone?, or perhaps more precisely, Are there others out there like us? Perhaps the question we have been seeking to answer should really have been in two parts; Is there life elsewhere in the universe, and if so is it intelligent and would we be able to interact with it in some way? Pre-requisites for Life Earth is the only place where it is possible today to study living things and fossils to understand life, its evolution and the habitats where it can thrive. On Earth life is found in many extreme environments including; around volcanic vents on the mid-ocean ridges; in deeply-buried porous sedimentary rocks (Bruckner, 2017); permanently in caves; in glacier ice (Edwards, 2014); in thermal springs; in the stratosphere (Major, 2016) and in naturally toxic environments that would be poisonous to most other life forms. Despite the abundance of life on the surface of the Earth it has been suggested that there may even be more life below the surface than there is above (Cox, 2013). Figure 1: Colony of Deepsea Tube Worms and other fauna at the Galapagos Rift. (Photo: NOAA 2011 Galapagos Rift Expedition) Figure 2: A loach, a permanent cave-dwelling fish that crawls out of the water to feed on bacteria growing on damp rocks. (Photo: Dantà © Fenolio) All terrestrial life exhibits metabolism, which is a chemical process to harvest energy from the environment to maintain the living state of the cells that make up an organism. Metabolism involves moving and breaking down nutrients in order to produce energy to synthesize new proteins, nucleic acids etc. that are essential to sustain life (Dr Ananya Mandal, 2013). All terrestrial life is based on the carbon atom, which can form chemical bonds to create the long and complex organic molecules that are the essential building blocks for life (Freeman, 2011). All terrestrial life is also reliant on liquid water as the medium within which the metabolic process occurs. Without liquid water there can be no metabolism and therefore no life, as demonstrated by the Atacama Desert the driest place on Earth where there is no evidence for the existence of any living organisms (Cox, 2013). It is generally accepted that the pre-requisites for life are; Access to nutrients that contain the chemical elements necessary for life; An energy source that can be harvested directly or indirectly; and Liquid water. Given that all elements occur throughout the Universe, as do stars that emit energy in the form of photons, the most obvious place to look for extra-terrestrial life is on the surface of planets where there is likely to be liquid water. In any solar system there will be a region around the star within which the temperature is such that water will exist as a liquid. This is known as the Habitable Zone. The distance of the habitable zone from the star and its extent will be a function of the spectral type (and therefore mass) of the star and can be estimated using the Inverse Square Law, assuming the existence of an atmosphere with sufficient density to prevent sublimation of the water. The figure below shows the extent of the habitable zone for various star masses, with the Solar System planets and the exoplanets orbiting the red dwarf star Gliese 581 superimposed. Figure 3: The habitable zone as a function of stellar mass and distance from the star (Chester Harman, Planets: PHL at UPR Arecibo, NASA/JPL/APL/Arizona) Another potential habitat for life is on the moons of large planets with elliptical orbits are subjected to tidal heating caused by tidal friction. Orbital and rotational energy is dissipated as heat in the crust of the moon, in some cases melting the ice and forming an ocean beneath the ice crust. Two known examples of this in the Solar System are Jupiters moon Europa and Saturns moon Enceladus. It is postulated that life could also exist below the surface of Jupiters moon Io where there is plentiful heat to keep any water that was trapped in a liquid state, and where living organisms would be protected from Jupiters radiation (Choi, 2010). The Origin and Evolution of Life on Earth and Elsewhere Through the study of living organisms the pre-requisites for life are reasonably well understood, as is the evolutionary process through inter alia the study of fossils. However, to answer the question of how life came to be established on Earth it is also necessary to look beyond the Earth for clues. The elements that make up organic molecules are very abundant in the Universe and are known to originate from non-biological processes (e.g. volcanic activity on Mars (Carnegie Instution, 2012)) and there is a lot of evidence to suggest organic molecules are widespread in the galaxy, e.g.: Iso-propyl cyanide has been detected by examining microwave emission lines in inter-stellar clouds in the Milky Way (BBC, 2014). Organic molecules have been detected using spectral analysis in the tails of comets. The Rosetta mission to comet 67P/Churyumov-Gerasimenko also detected organic molecules (ESA, 2016). Organic molecules have also been found in certain types of meteorite collected on Earth. Carbonaceous chondrites are rare meteorites that have not melted at any stage of their life so are thought to pre-date the Solar System. They contain substantial amounts of carbon, including complex organic compounds and occasionally amino acids, and up to 20% water (Freeman, 2011). In the early Solar System comets and meteorides were very numerous and according to the Panspermia Hypothesis they seeded the Universe with simple life forms that got trapped in ejecta thrown into space when collisions occurred between planets and moons. This theory was given credence when living bacteria was found in a sealed camera recovered and brought back to Earth by the Apollo 12 astronauts from the Surveyor 3 spacecraft. Surveyor 3 had been on the lunar surface for three years. Another possibility is that organic molecules were formed on Earth, as hypothesised by Oparin and Haldane (Oparin, 1924). In 1952 Miller and Urey conducted their famous laboratory experiment which simulated conditions on early Earth. They mixed water, ammonia, methane and hydrogen in an atmosphere of water vapour, through which electric sparks were fired regularly to simulate lightening. At the end of the experiment they discovered that amino acids had indeed formed, giving credence to this hypothesis (Miller, 1953). Figure 4: The Miller-Uray apparatus Once all the right ingredients were present something kick-started life on Earth, and/or elsewhere in the Universe if the Panspermia Hypothesis is right. It is not possible today to conclude how life originated on Earth, but in any event the fossil record shows that the first simple living organisms appeared on Earth around 3.8 billion years ago, and so began the process of evolution producing the incredible diversity of life on Earth today. Whether life was kick-started on Earth or arrived from elsewhere is arguably one of the most important factors influencing the possible distribution of extra-terrestrial life, and is discussed again in Section xx. History of the Search for Life Beyond Earth NASA was established by an act of the US Congress in 1958, mainly in response to the launch by the Soviet Union of Sputnik 1. Most of its efforts were initially concentrated on the development of manned and unmanned space flight, but in the 1970s exploration of the Solar System using scientific probes began, driven to a large extent by the search for life beyond Earth. NASA began a broad-based effort to learn how to look for the presence both ancient and current of life beyond Earth, giving birth to a new science which became known as Exobiology. The fundamental questions that NASA set out to answer were; What is needed for life to thrive? How does life evolve? Where else in the Universe could it have evolved? How do we find it? In time it was acknowledged that to help answer these questions the detailed study of life on Earth was necessary to understand the origins and evolution of life and the habitats where it is found. The scope of exobiology expanded and it became known as Astrobiology (Freeman, 2011). During the 1960s a number of European countries started to get involved in space exploration, eventually clubbing together to form the European Space Agency (ESA) in 1975, bringing more resources to the exploration effort. The Search for Evidence of Intelligent Life In 1959 Guiseppe Cocconi and Philip Morrison observed that if intelligent extra-terrestrial life had been attempting to communicate it would probably have been doing so using radio waves transmitted at the wavelength of neutral hydrogen (21.1 cm), which is in a region of the radio spectrum dubbed the water hole due to its proximity to the hydrogen and hydroxyl radical spectral line. These radio waves do not experience diminution when they travel through the interstellar medium or through the Earths atmosphere and they argued that it should therefore be possible to detect such signals with terrestrial radio telescopes because (Cocconi Morrison, 1959). In 1960 Dr Frank Drake used the radio telescope at the National Astronomy Observatory in West Virginia to search for four months for radio signals with a wavelength of 21.1 cm emanating from the vicinity of nearby stars Epsilon Eridani and Tau Ceti (Drake, 1961). He failed to detect any signals but this heralded the beginning of SETI (the Search for Extra-Terrestrial Intelligence). Since the 1980s there has been an international collaborative effort to detect meaningful signals across an increasingly wide range of wavelengths, but although occasional signals have been detected they have not been sustained or repeated, which suggests they were not produced by an intelligent life form seeking to communicate. Notwithstanding this, the search continues. The Search for Suitable Habitats and Evidence for the Existence of Life Aristotle was the first to observe life in snow as a snow algal bloom. These occur as algae produce reddish-pink blooms (watermelon snow) as seen in this sample of Svalbard snow. The reddish-pink pigments are a microbial sunscreen, protecting the algae from UV radiation. Photo credit: Dr Arwyn Edwards (Edwards, 2014) Drake Stars w/ mass > 1.5o unlikely to support life humans took 4bn + yrs Small stars long life but low temp, planets have to be close but then gravity locked v. low POS based on current understanding = sun-like star- low rate of formation; 1:10 w/ habitable zone Implications of Trappist-1 results and historical assumptions The Probability of There Being Extra-Terrestrial Life in the Universe The Drake Equation The Drake equation is: N = Rà ¢Ã‹â€ - à ¢Ã¢â‚¬ ¹Ã¢â‚¬ ¦ fp à ¢Ã¢â‚¬ ¹Ã¢â‚¬ ¦ ne à ¢Ã¢â‚¬ ¹Ã¢â‚¬ ¦ fà ¢Ã¢â‚¬Å¾Ã¢â‚¬Å" à ¢Ã¢â‚¬ ¹Ã¢â‚¬ ¦ fi à ¢Ã¢â‚¬ ¹Ã¢â‚¬ ¦ fc à ¢Ã¢â‚¬ ¹Ã¢â‚¬ ¦ L where: N = the number of civilizations in our galaxy with which communication might be possible (i.e. which are on our current past light cone); and R* = the average rate of star formation in our galaxy fp = the fraction of those stars that have planets ne = the average number of planets that can potentially support life per star that has planets fl = the fraction of planets that could support life that actually develop life at some point fi = the fraction of planets with life that actually go on to develop intelligent life (civilizations) fc = the fraction of civilizations that develop a technology that releases detectable signs of their existence into space L = the length of time for which such civilizations release detectable signals into space No table of figures entries found. 2. Prof BBC. (2014). Complex organic molecule found in interstellar space. Bruckner, M. (2017). Endoliths-Microbes Living within Rocks. Microbial Life. Carnegie Instution. (2012). Organic carbon from Mars, but not biological. Science Daily. Cox, P. B. (2013). Wonders of the Solar System. Dr Ananya Mandal, M. (2013). What is Metabolism? Edwards, D. A. (2014). Glacier Ecosystems. Antarctic Glaciers. ESA. (2016). Rosettas comet contains ingredients for life. Freeman, R. (2011). Universe Ninth Edition. J. Mayo Greenberg, C. X.-G. (1992). The seeding of life by comets. Advances in Space Research. Major, J. (2016). Hunting for High Life: What Lives in Earths Stratosphere? Universe Today. Oparin, A. I. (1924). The Origin Of Life. The Oxford Concise Dictionary. (n.d.).   Ã‚   http://www.news-medical.net/life-sciences/What-is-Metabolism.aspx https://www.sciencedaily.com/releases/2012/05/120524143450.htm https://en.wikipedia.org/wiki/Panspermia https://history.nasa.gov/factsheet.htm https://astrobiology.nasa.gov/about/history-of-astrobiology/ http://www.esa.int/About_Us/Welcome_to_ESA/ESA_history/History_of_Europe_in_space Ken Rice : The Detection and Characterization of Extrasolar Planets; Published: 19 September 2014