Untitled - American School of Milan
Transcription
Untitled - American School of Milan
1 March Issue The Nucleus 2016 American School of Milan BIOLOGY AND ENVIRONMENTAL SCIENCE The Impacts of Global Climate Change on the Arctic Food Web By Scintilla Benevolo ABSTRACT— Global climate change is becoming a serious issue our society cannot find a solution to. Two outcomes of this phenomenon can be seen in the Artic, where the ice is rapidly melting along with the permafrost. This will have a drastic impact on the Arctic food webs, the energy flows, the nutrient flows and our society, which cannot ignore climate change anymore. The melting of the ice is having a dramatic impact on the species within the arctic food web. For example, the number of polar bears, which are at the top of the food web, will keep decreasing as the years go by. This is due to the fact that polar bears give birth and hunt on ice. It is essential for the mothers’ survival to be able to hunt rapidly and successfully since, when they emerge from their dens with the cubs, they have not eaten for five to seven months. Furthermore, the longer the female polar bears live without food, the harder for them it will become to reproduce since their fat stores will be impacted. The instability and shrinking of the ice, caused by warmer temperatures, is thus perilous for this specie. Also, with the rising temperatures, competition will increase because the temperature species will begin to spread northward. Consequently, there is a risk of hybridization between polar bears, brown bears and grizzly bears. With the extinction of a specie at the top of the food web, disruptions will occur. In fact, the disappearance of the polar bears will result in some populations booming, and others diminishing. Ice algae, as the ice melts, will no longer have a permanent habitat. Most of these algae have already died between the 1970s and the 1990s, and are being replaced by a lessproductive, freshwater specie. Some of the areas affected by this phenomenon are Bering Sea and Hudson Bay, which are situated in the lower artic. The death of this algae, which is a producer and therefore at the bottom of the marine food web, will have drastic effects since all organism depend on producers. Along with the arctic food web, the flows of nutrients and energy will also be heavily influenced. With the disappearance of the producers, there can be no decomposers, therefore carbon and hydrogen will not be recycled anymore. Also, the melting of the permafrost will release huge amounts of carbon in the atmosphere. This will disturb the balance of the carbon cycle, since there will be more carbon in the air than in the land, and it will also increase global warming. Furthermore, if most of the arctic decomposers die, the energy will remain blocked in the 2 March Issue The Nucleus 2016 detritus, which will disrupt the flow of energy within the ecosystem. Although the arctic food web may risk to be wiped out completely, this will have a positive impact on the temperate species which will be able to take over. As the ice melts and the temperatures increase, they will move northward and will have a better chance of surviving the competition with the arctic species since they are used to living in warm habitats. Also, if the arctic producers go extinct, they will be replaced by the temperate ones, which will favor the take-over of new species. Economically, global climate change has both advantages and disadvantages. Since the ice caps are melting, a new trading route, the Northern Sea route (NSR), is being established by Russia. This route will start in the Kara Sea and end in the Pacific Ocean, passing through the Artic. The NSR will encourage trade since the vessels will take two-thirds less of the time they would normally take if passing through the Suez Canal. Also, this route will be safer since pirate attacks at the Horn of Africa would be avoided, and there would therefore be no risk of losing cargo. Furthermore, Russia desires to build a port in Ob Bay, at Sabetta, which would help develop the natural gas resources that lie on the Yamal Peninsula. Although this would benefit most economies worldwide, it is also important to take into consideration that, most of the year, the route will be blocked by ice. Because of global climate American School of Milan change the ice will be thin and breakable, but this would mean travelling very slowly, and consuming much more fuel. Furthermore, building arctic bulk carrier vessels is much more expensive and, with the route being used by a small number of vessels, tariffs will remain high. The melting of the permafrost, which would result in a release of carbon, will also damage the economy since governments will need to spend more money on health care. Therefore, global climate change has more significant economic disadvantages than it does have advantages. From an ecological perspective, the Antarctic food web and life will be completely replaced by temperate species if we don’t put an end to global climate change. Gradually, more arctic species will die, adapt to the new temperatures, or hybridize with species from more southern regions. If this were to occur, a whole ecosystem would collapse. Esthetically, the geography of the world would also alter itself since, as the glaciers melt, the ice levels rise, and populations living on coasts will find themselves completely submerged. To conclude, the impacts of the global climate change are not ethical for they are unsustainable. Although the melting of the ice could conclude in some economic advantage, the release of carbon dioxide in the atmosphere would tragically impact health, and will therefore harm the future generations. 3 March Issue The Nucleus 2016 American School of Milan Biological 'clock' Discovered in Sea Turtle Shells By Gabriele Calabria ABSTRACT—Radiocarbon dating of atomic bomb fallout found in sea turtle shells can be used to reliably estimate the ages, growth rates and reproductive maturity of sea turtle populations in the wild, according researchers. The newly tested technique provides scientists with a more accurate means of estimating turtle growth and maturity and may help shed new light on the status of endangered sea turtles populations worldwide. Researchers have found that they can reliably estimate the ages, growth rates and reproductive maturity of sea turtle populations by performing radiocarbon dating of atomic bomb fallout found in their shells. While it may sound strange, the researchers say their technique provides more accurate estimates than other methods currently in use and may help shed new light on factors influencing the decline and lack of recovery of some endangered sea turtles populations. The most basic questions of sea turtle life history are also the most elusive, "said Kyle Van Houtan, fisheries research ecologist at NOAA’s Pacific Islands Fisheries Science Center and adjunct associate professor at Duke’s Nicholas School of the Environment. The hawksbill sea turtles used in the study were already deceased, and either died of natural causes or were harvested for their decorative shells as part of the global tortoiseshell trade. The researchers worked with federal agencies, law enforcement and museum archives to obtain the specimens. Each turtle’s approximate age was calculated by comparing the bomb-testing radiocarbon accumulated in its shell to background rates of bomb-testing radiocarbon deposited in Hawaii’s corals. According to a statement from the researchers, levels of carbon14 increased rapidly in the biosphere from the mid-1950s to about 1970 as a result of Cold War-era nuclear tests but have dropped at predictable rates since then, allowing scientists to determine the age of an organism based on its carbon-14 content. In addition to their natural beauty, the shells of two deceased specimens of Hawksbill sea turtles (Eretmochelys imbricata) hold clues to the growth rates and sexual maturity of the endangered species. Credit: Duke University, Kyle Van Houtan This is the first time that carbon-14 dating of shell tissue has been used to estimate age, growth and maturity in sea turtles. Scientists typically employ other, less precise methods such as using turtle length as a proxy for age, or analyzing the incomplete growth layers in hollow bone tissue. Van Houtan also believes the new technique could help shed light on why some populations — including Hawaiian hawksbills, the smallest sea turtle population on Earth — aren’t rebounding as quickly as expected despite years of concerted conservation. “Our analysis finds that hawksbills in the Hawaii population deposit eight growth lines annually, which suggests that females begin breeding at 29 years — significantly later than any other hawksbill population in the world. This may explain why they haven’t yet rebounded,” Van Houtan said. The bomb radiocarbon tests also indicate another red flag. “They appear to have been omnivores as recently as the 1980s. Now, they appear to be primarily herbivores. Such a dramatic decline in their food supply could delay growth and maturity, and may reflect ecosystem changes that are quite ominous in the long term for hawksbill populations in Hawaii,” he said. 4 March Issue The Nucleus 2016 American School of Milan New Tarantula Named After Johnny Cash By Matteo De Palma ABSTRACT—The following article provides an explanation of the background and discovery of a new species of spiders in the United States. It is a milestone in biology as it is a deeper understanding of spiders, which could allow further expansion of knowledge in various other fields. A new species of tarantula has emerged, and been attributed the name of famous singer/songwriter Johnny Cash. The new tarantula is one of fourteen new spiders discovered in the southwestern United States, and the amount of information we have regarding their adaptability, anatomy, survival traits, etc. is very limited. Biologists at Auburn University and Millsaps College have described these hairy, large-bodied spiders in the open-access journal ZooKeys: "We often hear about how new species are being discovered from remote corners of the Earth, but what is remarkable is that these spiders are in our own backyard," says Dr. Chris Hamilton, lead author of the study. "With the Earth in the midst of a sixth mass extinction, it is astonishing how little we know about our planet's biodiversity, even for charismatic groups such as tarantulas." The Aphonopelma genus are among the most unique species of spider in the United States. One aspect that scientists find most intriguing is that there is no definite size among the species meaning that some can reach 15cm or more, whereas others can fit on the face of an American quarter-dollar coin. The Aphonopelma species can be found in twelve states across the southern third of the country, ranging west of the Mississippi River to California. These spiders are most seen during the warmer months when the adult males leave their burrows in search of mates, yet very little was known about the spiders prior to the study. Dr. Hamilton states that there are fifty different species of tarantulas which have been previously reported from the US, but that many of them were poorly defined and actually belonged to the same species. To reach a further understanding of the different characteristics that divide these tarantulas from the ordinary species, the research team implemented a modern and “integrative” approach to taxonomy by employing anatomical, behavioural, distributional, and genetic data. Their results provided enough evidence to note that there are 29 species in the US, of which 14 are completely new to science. Returning to the first paragraph, one of the species was named “Aphonopelma johnnycashi” after the influential American song writer Johnny Cash. Dr. Hamilton decided upon the name due to the scientist’s first encounter with the species in California near Folsom Prison (famous for Cash’s song “Folsom Prison Blues”) and because the males usually have a dark black pigment, giving tribute to Cash’s distinctive style of dress where he has been referred to as a “Men in Black”. Although never having been studied before, this new spider could be in use of conservation efforts in the not-so-distant future. This is because of the destruction of their habitats due to climate change and human intrusion in their homes. A co-author on the study, Brent Hendrixson, stated that “Two of the new species are confined to single mountain ranges in south-eastern Arizona, one of the United States' biodiversity hotspots,” and that “these fragile habitats are threatened by increased urbanization, recreation, and climate change. There is also some concern that these spiders will become popular in the pet trade due to their rarity, so we need to consider the impact that collectors may have on populations as well." 5 March Issue The Nucleus 2016 American School of Milan BIO AND ES: Crossword Puzzle From the New York Times! http://learning.blogs.nytimes.com/2014/07/24/student-crossword-endangered-species/?_r=0 Solutions: 6 March Issue The Nucleus 2016 American School of Milan CHEMISTRY PVC and Plasticizers By Francesco Grechi ABSTRACT—This article seeks to provide a brief introduction to chemical polymers, and how substances called plasticizers can be used to manipulate their levels of rigidity. All explanations are done in reference to the Poly(1chloroethylene) polymer, commonly known as PVC. Poly(1-chloroethylene), better known by its abbreviation “PVC”, is the third-most widely produced synthetic plastic polymer. It exists in two main types commercially, rigid (RPVC) and flexible. As the names suggest, these two species of the polymer differ greatly in their elastic behavior. RPVC is used primarily in construction, and is perhaps most commonly associated with cheap plastic sewage pipes. On the other hand, flexible PVC is used as a substitute for elastomers (namely rubber) in a variety of fields, including plumbing and electrical engineering. This might seem puzzling; how is it possible that the same chemical species can display such radically different physical properties? The answer to this question lies in a technique called “plasticization”. If you were to ask a chemical engineer what the definition of plasticization is, he would probably tell you that it is the process by which plasticizers are added to polymers. Yet, this raises two more questions; what exactly is a polymer, and what is a plasticizer? A chemical polymer is defined as a large molecule composed of many repeated subunits (called “monomers”). To understand this, imagine a metal chain comprised of many identical metallic links attached to one another. In essence, a polymer is just like that metal chain, only that its fundamental monomers are identical molecules or atoms, not metallic links. For example, PVC’s monomer is chloroethene (CH2CHCl) This comparison is extremely useful to understand polymer chains, but can give the wrong impression. Unlike with a metallic chain, you will never have a single isolated polymer chain on its own. In fact, a sample of a polymer is composed of thousands of individual chains. These chains will be attracted to one another by electrostatic forces, known as “intermolecular forces”. As a result, the chains will be strongly linked to one another, increasing the rigidity of the polymer as a whole. In the case of PVC, these intermolecular forces are so large that, when synthesized, PVC is extremely hard and brittle. This is where plasticizers come into play. A plasticizer is a molecule that embeds itself between adjacent chains, and reduces the effect of intermolecular forces. This causes a decrease in the overall melting point of the polymer, resulting in increased flexibility and fluidity. Tying back to PVC, plasticizers that are commonly used to create flexible PVC belong to the phthalate family; the most commonly used is bis(2-ethylhexyl)phthalate [C8H4(C8H17COO)2]. Increasing the quantity of plasticizer added to the polymer will increase the flexibility of the polymer as a whole; RPVC contains less plasticizer than flexible PVC does. Therefore, by regulating the amount of plasticizer added, chemical engineers can synthesize polymers of differing rigidity levels. On an interesting side note, plasticizers tend to evaporate over time. Therefore, a sample of flexible PVC will eventually convert into RPVC if left alone. If you have ever driven in a new car, you will definitely have experienced this. PVC can be found in the inner linings of automobiles; over time the plasticizer contained in it will evaporate and contribute to the smell associated with the “new-ness” of the car. 7 March Issue The Nucleus 2016 American School of Milan The Modern Periodic Table By Anais Emanuele ABSTRACT— The following article strives to provide knowledge regarding the history of the periodic table of elements and the modern periodic table, mainly focusing on the scientist and genius, Mendeleev. Prior to Dimitri Mendeleev, many scientists including Alexandre Béguyer de Chancourtois, John Newlands and Julius Lothar Meyer, had attempted to organize in a certain order, which would later be systematized as a table, the elements that had been newly discovered. However none of the scientists’ attempts were proven to be effective. In 1869, Dimitri Mendeleev’s also endeavored to organize these elements in an effective and strategic approach, which was then considered to be so successful that it formed the foundation of the modern periodic table. The current periodic table, is in fact, similar to the one created by Mendeleev. After having arranged and rearranged the elements numerous times, Mendeleev realized that by ordering the elements by increasing atomic mass and by placing the elements with similar properties beneath each other, a trend arose. This trend consisted in the frequent reemergence of certain categories of elements. For instance, when a reactive non-metal appeared and was placed in a specific area, the element which followed up was usually a highly reactive light metal, which succeeded by a barely reactive light metal. Dimitri Mendeleev, who is considered father of the periodic table, was furthermore successful, in that he was able to fix two major problems, which kept occurring and whom nobody seemed to be able to fix. These two major problems consisted in the two elements Tellurium (Te) and Iodine (I), as well as the three unknown holes. Mendeleev recognized that Tellurium had a mass which was greater than that of Iodine, however its properties resembled more those of the halogens Oxygen (O), Sulfur (S) and Selenium (Se). Thus, in order to coherently and efficiently solve this problem, Mendeleev chose to swap the two elements, Te and I, over, allowing them to resemble their halogens. Subsequently having fixed the problem with the two elements, Tellurium and Iodine, he was left with an additional problem to solve, the three holes. The expert noticed that in his attempt in creating the periodic table, there were three holes, three elements which had not yet been discovered. He predicted the properties of the elements, which were later shown to be exceptionally accurate, and gave them the prefix eka, and the suffix of the halogen found above them. The three unknown elements were consequently called, eka-boron, eka-aluminum and eka-silicon. When the three elements were discovered, in the following years that past, they were respectively named Scandium (Sc), Gallium (Ga) and Germanium (Ge). Approximately six years after the death of the genius known as Dimitri Mendeleev, another very important scientist greatly contributed in the formation of the modern periodic table, Henry Mosley. In 1913, he arranged the elements by increasing positive charge, and hence by increasing atomic number, which almost always corresponded to the same order of atomic mass. Mosley was able to properly provide explanation, for his X-ray experiment, which allowed him to determine the atomic number. He explained that when an electron drops from a greater energy level, which in known as excited state, to a lower one, which is known as ground state, the energy is emancipated as electromagnetic waves, thus X-rays. The amount of energy that is released, is subject to the intensity of the electron attraction to the nucleus. The greater amount of protons an atom has in its nucleus, the greater the electrons will be attracted and the greater the energy that will be released. In addition, the number of protons, in an element corresponds to its atomic number. Thus it is clear to see how many great scientists’ minds, especially those of Dimitri Mendeleev and Henry Mosley, have largely contributed to the creation of the marvelous modern periodic table, to such an extent that we still use it to this very day. 8 March Issue The Nucleus 2016 American School of Milan The new era in carbon allotropes ABSTRACT—This article will talk about the uses and application of graphene. Some elements on the periodic table are said to be allotropic. That means that they have different physical structures of the same element. Carbon, for example, has five different allotropes: graphite, diamond, fullerene, silicon dioxide and finally graphene. In its structure, graphene is very similar to graphite. They are both made out of hexagonal rings. Graphite though, has hexagonal rings stacked one on top of each other. Graphene, on the other hand, is made out of a single layer of hexagonal rings. The first time graphene was produced by a team of scientists, they took a piece of graphite and made it as thein as possible by dissecting it layer by layer. This last process is known as mechanical exfoliation. Therefore graphene, is essentially one layer of graphite. As a result of making it so thin, graphene is only one atom thick. Its properties as the lightest and strongest material, compared to its ability to conduct heat and electricity better than anything else. In future scientists hope that graphene will be able to mix with other 2-D crystals, thus to create more even more complex compounds that would vary even in uses. One field in which graphene is hoped to be very profitable is bio engineering. Scientists hope that this allotrope might revolutionize this filed. In the first place graphene’s ample surface area, conductivity capabilities, strength and thinness could help bio engineers create faster and more efficient bioelectric sensory devices. These last ones should have the capability to measure hemoglobin levels and glucose levels. However, bio engineers are hoping that this technology be delivered by 2030. Furthermore graphene’s use will also be extended to optical electronics. For example touch screens. Today touch screens use liquid crystal displays (LCD) or organic light emitting diodes (OLED). Today the most used material is Indium Tin oxide (ITO). However, graphene has proven to work just as well since it can optically transmit 97.7% of light. Furthermore the fact that graphene is so flexible, thin and strong makes it the new candidate in optical electronics. Seeing as this carbon allotrope is so strong, light and stiff aerospace engineers are using carbon fiber in the production of aircraft. However, what they are really hoping to do is substitute the whole steel structure of the plane with a material that incorporates graphene. This is because it is o light and strong. Thus improving fuel efficiency, range and weight. Another application that could integrate graphene in the future is in photovoltaic cells. Today they use silicon or ITO. However, because of graphene’s light levels of absorption whilst offering a high electron mobility means that it could be used in photovoltaic cells. An advantage of using graphene is that it is more flexible than the other two. Thus it could be used in clothing, or to recharge our phones. However, one limitation of graphene is that if it is high-quality, in the sense that as a conductor it does not stop. This is why there still needs to be some research put into the use of graphene and it substituting other elements in technologies. 9 March Issue The Nucleus 2016 American School of Milan CHEMISTRY: Crossword Puzzle By: Giovanna Pinciroli HORIZONTAL VERTICAL 1. Its three isotopes are Protium, Deuterium and Tritium 2. It can replace Iodine - and form a red-brown color - but it is weaker than chlorine 3. A red-brick color originates from its flame, and it is the lightest of the alkali earth metals 4. Soft, silvery, and very abundant on the Earth's crust 6. The third noble gas 8. Mistaken by many for a transitional metal, this element is colorless 10. In the past, it was essential in the composition of thermometers 12. It makes up 21% of the atmosphere 15. Some people lack this element in their blood Gold 5. Aluminum 4. Calcium 3. Bromine 2. Hydrogen 1. 10. 9. 8. 7. 6. Mercury Sodium Zinc Chlorine Argon 15. 14. 13. 12. 11. 5. It is very valuable 7. The gas derived from this element was originally used to bleach textiles 9. A close friend of both Lithium and Potassium 11. Its octet is filled with six electrons 13. Commonly referred to as W 14. Friends with Germanium and Selenium 10 Iron Arsenic Tungsten Oxygen Boron March Issue The Nucleus 2016 American School of Milan MATHEMATICS Counting the Hard Way – Number Systems By Yookyung Kim ABSTRACT— This article explores the weaknesses of widely used decimal system. Show me 10 fingers. Now tell me. How many fingers did you just hold up? Most of you would find this question to be extremely pointless. It seems so obvious that I already know that the answer is ten. The truth is, there are infinitely many ways of interpreting the number ’10.’ This number could be any number: two in a binary system, twelve in a duodecimal system, and sixteen in a hexadecimal system. But most of us count in decimal system, which utilizes ten different symbols to express numbers in base ten. It is the default setting of our subconscious mind and the reason why we automatically interpreted the number ‘10’ as ten. Despite the difference in language, lifestyle and cultures, most countries have developed their own way of counting based on decimal system, primarily due to our simple biological feature – we have ten fingers. Today, the international collaboration in expanding the human knowledge has determined the decimal system using Arabic numerals as the standard way of counting. Most would think that the decimal system should be the most efficient system since the majority of modern humans has recognized it as the “simplest way of counting.” But consider reading clocks. Try to convert an hour and ten minutes in hours. Our natural instincts trained by the decimal system would first lead us to an erroneous answer – 1.10 hours. But then our educated mind would remind us that there are sixty minutes in an hour. So we divide 10 by 60, which would give us 1/6. Not the best fraction to work with. However, if we were to use a duodecimal system to calculate its value, 1/6 would be equal to simply 0.2. We confront the first limitation of decimal system since our measurements of time is based on the duodecimal system. It is easier for humans to use decimal because we have ten fingers. In the same way, it is much simpler to use binary system in computing as switches on a computer can have only two states – on and off. Due to its simplicity and mathematical operations unique to it, the binary system is used in programming in order to maximize the computing speed. On the other hand, we can observe the disadvantage of binary system when it comes to larger numbers ((1000)10 = (0000001111101000)2). People can easily lose track in the endless repetition of 0s and 1s, so binary number is not the most appropriate system to be used in daily life. Although different systems have own unique advantages and disadvantages, people think that it would be too cumbersome to change the counting system to suit different purposes. It seems that it would take considerable amount of time for people to stop relying on their ten fingers to count. However, the supporters of the duodecimal system claim that converting numbers into a new system can easily learned over time like learning a new language. The concept of counting in different number system may sound too challenging at the beginning. Still, it would be beneficial to diverge from the traditional way of counting and understand how to work with other number systems. 11 March Issue The Nucleus 2016 American School of Milan What to know before playing the lottery By Edoardo Rundeddu ABSTRACT—This article will analyze Superenalotto, an Italian lottery in terms of probability of winning and cost of the game. Superenalotto, the most popular Italian lottery, is based on a very simple game. You first choose six numbers between 1 and 90, and if either part of them or all correspond to the six winner numbers you win a prize. The cost to play one combination is €0.50. The question I have always asked myself is - to what extent is this a fair game? and the number of combinations that can occur. Therefore, Fair return=€0.50×622'614'630=€311'301'315, which is slightly less than twice the largest prize ever allocated. While €177’729’043 is certainly a huge amount of money, the problem is that it is not enough. And, if we look at the issue from a different point of To simplify this problem I will only consider the event of view, it is obvious that Superenalotto is not a fair game. getting the jackpot prize. Firstly, it is necessary to In many countries, Italy included, gambling is an activity determine the probability of having six numbers controlled by the government, which gains revenue by extracted as winners. The number of different keeping the money that does not become the jackpot. If combinations of six elements is given by the formula n! the fair return calculated previously was actually real, / (n-k)! k! where n is the total available numbers and k then theoretically someone could play all the possible is the amount of winner numbers, so in this case we combinations and then win the 1st prize without losing have 90! / (84)! 6! =622'614'630. The probability of anything. winning the maximum prize is therefore only 1 / Therefore, from a mathematical point of view, it is clear 622'614'630 (pretty low right?). that, in the long run, those betting in a lottery will To give a meaning to this number, the odds of being hit always lose, and the government will always win. by a lightning in the US in a given year is estimated to However, math cannot clarify why many people be 1 in 700’000. The chances of finding a pearl in an routinely gamble at games like Superenalotto. The oyster is 1 in 12’000. And, unless you are Leonardo di explanation lies in the fact that humans are generally Caprio, the odds for anyone winning a Hollywood Oscar willing to invest little amount of money in the dream of an enormous return, even when the probability that this award is 1 in 12,200. event occurs is insignificantly small. So it easy to understand that for such a rare event, a very high prize must be associated. But is €177’729’043, the greatest sum ever won (October 30th, 2010) enough? To better understand Superenalotto, I will use a different example. Let’s assume you are playing a dice game, where you bet €1 that you get a 3. Because getting a 3 has the probability of 16 then the fair return would be €6. This because the product of the probability and the prize is equal to the initial bet. The lottery works in the same way! To find the fair return, we would have to multiply the cost of the game 12 March Issue The Nucleus 2016 American School of Milan Prime Numbers By Matteo De Angelis ABSTRACT— This article will focus on the nature, history and properties of prime numbers. Prime numbers have always been a mystery since their discovery, approximately 8th to 6th century BC during the ancient Greece. But what makes this numbers so special that scientists haven’t found a straightforward formula yet? Why are this numbers even studied? I mean they are just numbers, right? This reasoning is not completely wrong, but there must be a reason why big price awards are given nowadays to whoever is able to find new prime numbers with an extremely high numbers of digits. showed that giving n=5 so 232 + 1 the result is not a prime number as it can be divided by 641. The more the time passed the more prime numbers were discovered and it became a serious issue to find others. But as more numbers were discovered, technology advanced and developed and since 1951 all the largest known primes have been found by computers. The search for ever larger primes has generated interest outside mathematical circles. The Great Internet Mersenne Prime Search (Marin Mersenne was a monk that made a big contribution in trying to understand better prime numbers looking at them in the form 2p – 1 where p is a prime number) and other distributed computing projects to find large primes have become popular, while mathematicians continue to struggle with the theory of primes. First of all what is a prime number? It’s any natural number greater than 1 that can be divided by itself or by 1 without a reminder. This definition makes clear that prime numbers are not something common. For example 2 is the only even prime number as, obviously, every even number can be divided by 2. This already takes away half of the numbers and Now a question that you could be asking to yourself is: there are a lot of other little tricks to find out if a number can be Other than for money, why would I care about prime numbers? divided by the first 10 numbers. The problem comes when the Well, for a long time, prime numbers were thought to have extremely limited application outside of pure mathematics. This numbers start to get bigger. changed in the 1970s when the concepts of public-key Even though the bigger the numbers become the rarer cryptography were invented, in which prime numbers formed the they get to be prime, these are infinite. This was first proved by basis of the first algorithms such as the RSA cryptosystem Euclid. He proved this by contradiction, which means that he algorithm. But primes can be seen also in nature. One example proved his point by showing that the opposite must be false. of the use of prime numbers in nature is as an evolutionary What he affirms is that if prime numbers are not infinite, there strategy used by cicadas of the genus Magicicada. They only must be a bigger one, let’s call it n. Now if we calculate the pupate and then emerge from their burrows after 7, 13 or 17 product of all these numbers together (n included) we will obtain years, at which point they fly about, breed, and then die after a a number (call it “a”) which is divisible by every apparent prime few weeks at most. The logic for this is believed to be that the number. The final step is to add 1 to the number found, this prime number intervals between emergences make it very result will lead to a new prime number greater than the others. difficult for predators to evolve that could specialize as Many others, after him, proved the infinity of prime numbers, but predators on Magicicadas. Euclid was the first. To conclude I must say prime numbers are amazing. They are at Instead the first one who attempted to find a formula in the basis of cryptosystem algorithms that protect your credit order to find a prime number was, in 1640, Pierre de Fermat, card and can be even be found in nature. My suggestion is to get who stated, without proving it, that all the numbers that can be involved and try to find a new prime number or better a way too written as 22^n + 1 are prime. This was later denied by Euler who find them all, because it will be worth it! 13 March Issue The Nucleus 2016 American School of Milan MATH: Sudoku Evil Sudoku (http://sudoku.math.com/) Solutions: 14 March Issue The Nucleus 2016 American School of Milan PHYSICS We measured gravitational waves By Eleonora Pigoli Abstract: This article is about the recent detection of gravitational waves, by the hands of the LIGO group. If you have been following the news lately, you might have heard that on February 11th the LIGO group were finally able to accurately detect gravitational waves. That is huge news in the physics world because it finally proves, or to put more accurately does not disprove, Einstein’s theory of General Relativity. Now, unless you’re taking an IB physics class or are really passionate about the subject, you probably don’t know what that is and how gravitational waves come into the picture. So let me help. First things first, what is general relativity and why is it important? Well, in 1915 a man named Albert Einstein described gravity as a bending of space-time geometry. Now hold up, what is space-time geometry and why does it bend? Space- time is what you can picture as the fabric that makes up the universe. Think of it as a rubber sheet that we all float on. Now, anything that has mass, according to Einstein, affects the space-time fabric by bending it. So, if you have mass and bend the fabric, everything else on the sheet will be affected by it. Taking a person as an example is not quite fitting as you mass is way too small to make a difference in the grand scheme of things. Let’s think of the Earth or the Sun instead. When they make a bend in space-time, everything around them is affected and when something with mass comes close to them instead of going straight through, they follow the path that is dictated by the bend in the fabric. They are drawn into the gravitational field of the sun or of the earth. This is why we have orbits. 15 March Issue The Nucleus 2016 Alright. Now that we have a better understanding of gravity and space-time, where do waves come in? Einstein described gravity as a bend of space-time geometry, but also wrote a series of equations, known as field equations, to back up his theory. These equations describe how gravity reacts and behaves when there is a change in matter on the space-time fabric we were talking about before. These equations can be derived into others which relate space and time and gravity. The solution to these equations is represented by a wave function. So, from a purely mathematical standpoint, if Einstein was right then we should be able to detect waves as a result of gravity. From a physics point of view the idea is that if you create a bend in space-time you should see the ripples caused by it. Think of it like a lake. If you throw in a pebble, you see ripples on the surface of the water. It is the same idea. The gravitational waves are the ripples. American School of Milan compression in space-time with say a ruler, we would fail because the space between the ticks on the ruler would also stretch. To detect the waves and the stretch we need a ruler that is not affected by these distortions. The LIGO group used light. They set up two 4km tunnels to make up an L shape and bounced lasers back and forth between the ends of the tunnels. If the light took more time to get back than what it was supposed to, then they could say with certainty that there had been a distortion. By now you will have realized that it takes a stunning amount of precision to get an accurate result and be sure that you measured a gravitational wave and not an error. The LIGO group had a little help in this, in that they used the waves from something very big and very fast. We were lucky enough to find out that two black holes had recently (1.3 billion years ago) collided. This event had always been predicted but never observed, at least until The real issue however is that gravitational waves now. The gravitational waves from these two black holes are tiny. Really tiny. So tiny in fact that they can very easily were big enough to be detected with accuracy. be confused with noise. So, how do we measure them? First, we need to figure out what instrument to use. We So, we detected gravitational waves. We proved must understand that gravitational waves are produced Einstein’s theory of general relativity. Why does that whenever something with mass accelerates, changing the matter? Well, we now know a little more about our universe distortion of space-time. Now that brings us to our main and how it works. Isn’t that amazing? I think it most problem. If we decided to measure a stretch or definitely is. A Deeper Look at Gravitational Waves: Their Detection By Hongseok Lee ABSTRACT—“Every time you go on the news, the hot topic is the detection of gravitational waves. But what are gravitational waves and why are they so significant? This article will explain to you all you need to know about them. In February 11, 2016, Washington D.C., the LIGO (Laser Interferometer Gravitational-Wave Observatory) announced the discovery of gravitational waves, a physical phenomenon proposed by Albert Einstein a 100 years ago. This announcement brought shock and cheers to the scientific community. But what is it that makes this discovery of gravitational waves so significant? But before we go into that topic, let’s first see what gravitational waves are. Gravitational waves are ripples in the fabric of space-time that take the form of waves. For example, let’s assume the universe as a giant piece of fabric. If you place an object on it, it would cause it to sag, forcing the other objects to be attracted towards it. Einstein described this as gravity. He also stated that gravitational waves are the ripples that objects create when they move through the fabric of space-time. Although the space is not a 2D surface, this analogy can help us visualize what happens when an object accelerates through space. However, this concept of gravitational waves has been causing disputes within the scientific community, for gravitational waves goes directly against the Newtonian theory of gravitation. 16 March Issue The Nucleus 2016 American School of Milan So what makes this discovery so significant? First of all, it proves that Einstein was right. Although he did propose this theory in 1916, he did not have sufficient data to confirm his theory. However, after a century, his idea was finally proven to be true. waves cover this distance in less than ten thousandth’s of a second. And in these pipes, there are lasers that reflect back and forth. So how does this facility work? Basically, as the binary black holes spin around each other, they stretch and squeeze each other, causing vibrations. These vibrations (a.k.a. gravitational waves) causes the lasers in Also, this discovery is important in the sense that it would the two different pipes to change their distance. One completely change the method which we would observe the stretches while the other shrinks. However, the universe. Previously, the primary method of analyzing the displacement is so minimal that high-tech detector is universe was through light emitted from the (astronomic needed to detect this. So this is how the LIGO detected the reactions) within the galaxy. However, this method had its gravitational waves in 11th of February. weaknesses in the (fact) that it could not observe (important) physical phenomenon such as black holes. But some might question, “Well, all of this is interesting, However, the detection of gravitational waves allows the but how can this be useful in real life?” It can be replied scientists to successfully analyze such phenomenon with the analogy of the X-ray. When Wilhelm Roentgen first without too much difficulty and it may lead to discoveries of discovered X-Rays in 1895, nobody thought that these radiations would be applicable to daily life. What do we new physics and astronomical phenomena. have now? From simple diagnosis to serious treatment, One example of this would be the discovery of the binary these radioactive waves are used extensively. Like so, the black holes. The LIGO actually had managed to speculate gravitational waves can be put to practical purposes if we the motions of the binary black holes and their put them to use. characteristics through detection of gravitational waves that only lasted 20 millionth of a second. The discovery of To conclude, it has been 100 years since Einstein first gravitational waves confirmed that binary black holes proposed the general relativity and gravitational waves. actually existed and it also analyzed their motions as well. Although he did not manage to back up his theory with sufficient data, his successors managed to do so a century So how did the LIGO actually “discover” gravitational later. Gravitational waves are not just some cosmic data waves? The secret lies in the gigantic L-shaped pipes. The that is insignificant. Rather, it is a discovery and a tool that distance from one edge of the facility to the other is 19 would completely change the course of human physics. hundred miles, which may seem like a lot, but gravitational 17 March Issue The Nucleus 2016 American School of Milan Physics behind the Leap Year By Federica Arcidiaco ABSTRACT—“By this point in our lives, we have all lived through at least three leap years, the most recent being just this year. But do you really know the reason for this extra day? The truth is that this periodic phenomenon can all be explained thanks to the physics of the Earth’s rotation around itself and the sun. A leap year is a year that contains an extra day, which is added to maintain the calendar’s synchronization with the astronomical year. This day happens to occur at the end of the shortest month of the year, creating the elusive entity that is February 29th. But why does this happen? However, there is another astronomical factor that is important to mention as it also explains why the tropical year does not consist of a whole 360 degree revolution: precession. Axial precession, the more specific term, is the movement of the rotational axis of an astronomical body. What this means, is that the gravitational pull of the sun on the Earth is changing the orientation of the rotational axis of the planet. The Earth’s precessional cycle is approximately 26,000 years. This is why the relative position of the North Star We all know that the Earth rotates, both around itself (from our point of view) changes by approximately 1 and around the sun. This is what we base our 24-hour degree every 72 years, drawing a circle that takes days and our 365 or 366-day years on. However, 25,771 years to complete. This messes with the length these numbers aren’t completely accurate. The Earth of the tropical year as it affects the orientation, which is doesn’t actually take 24 hours to complete one full one of the key references used in the calculations. rotation. It actually takes 23 hours, 56 minutes and 4.09 seconds. The difference seems like nothing (we are only talking about adding an extra 3 minutes and 55.91 seconds to our days), but if we actually stuck to this precise measurement, it would throw the whole system off as the sun would be shining at midnight for half of the year. The second imprecision in our astronomical years is the length year itself. We measure a year by finding how long it takes for the Earth to return to the point where it was oriented the exact same way towards the sun and at the same distance. However, the result of this calculation is actually slightly larger than what we believe our years to be. A tropical year actually terminates when the Earth has revolved approximately 359.986 degrees around the sun, which is enough to make the calculated tropical year 20 minutes shorter So, if you combine the Earth’s rotation around itself, its than that of the Gregorian calendar (our current revolution around the Sun, and the effect of precession, calendar). we can find out exactly how many days actually make up a tropical year. This digit is 365.242188931, which 18 March Issue The Nucleus 2016 American School of Milan is as far as our 2016 technology can measure. If we chose to completely ignore the extra 0.25 of this number and say that every year is composed of 365 days, we would end up being off by slightly less than a month every century! This is why we put in an extra day every 4 years, to amount for the missing 25%. years from three out of four century marks, the years gained three whole days every four centuries. This difference was large enough that, by the time that the Gregorian Calendar was instilled in 1582, 10 days had to be added to compensate for the days that had been gained. This means that in Italy, Spain, Portugal and Poland, October 5th through October 14th, 1582 never People have been following this logic for a long time, actually existed! since the Julian Calendar, introduced by Julius Caesar in This is the physics that exists behind the existence of 45BC. This ancient calendar, though, lacked one the leap day, an example that truly shows how accurate seemingly insignificant but crucial detail that is and precise the study of astronomy is, as 25% of a day incorporated in today’s Gregorian Calendar. can lead to months of lost time. However, Earth’s days and years are constantly, even if imperceptibly, You may already know that not every turn of the changing. For example, the recent earthquake in Japan century is a leap year. Only the century marks that are actually shortened the day by 1.8 microseconds. divisible by four get the extra day, meaning that while 2000 was a leap year, 1900 was not. This isn’t a detail that Pope Gregory XIII’s astronomers included just to So enjoy the leap year, as with all these constant confuse people when they were making their calendar changes in rotation and revolution, these extra days in the late 1500s. This measure was necessary as, by won’t be reoccurring forever. following the Julian Calendar and not taking away leap 19 March Issue The Nucleus 2016 American School of Milan PHYSICS: Crossword Puzzle Taken from: http://www.armoredpenguin.com /crossword/bin/crossword.cgi?c md=solve&filefrag=best/physics /amazing.physics.01.html HORIZONTAL VERTICAL 3.Particles of a medium vibrate perpendicularly to the direction of the motion of the wave. 4.Work done divided by the time taken to do the work. 8.The perpendicular distance from the axis of rotation to the point where the force is exerted. 11.The bending around obstacles. 15.The speed of sound depends on … 16.Combination of transverse and longitudinal water waves. 18.Particles of a medium travel parallel to the direction of the wave. 19.Source of all waves is something that … 20.The net force of an object moving in a circle towards the center of the circle. 21.The change in angular velocity divided by the time required to make the change. 1.The change in direction or bending of light at the boundary between two media. 2.Light rays converge at a point (can be projected onto a screen). 5.The distance from one crest to the other crest. 6.This wave needs a medium through which they can travel. 7.The force of attraction between two objects must be proportional to the object's masses. 9.The incident angle that causes the refracted ray to lie right along the boundary of the substance is unique to the substance. 10.Light rays do not converge at a point (can't be projected on a screen). 12.Number of oscillations in pressure each second heard as pitch. 13.Determines speed of light in the medium. 14.Which of Kepler's law states that the planets move in elliptical orbits, with the sun at one focus? 17.What mirror reflects light from its inner curved surface. Solutions: 20 March Issue The Nucleus 2016 American School of Milan STAFF AND CREDITS CREATORS: Director and Editor—Giovanna Pinciroli Layout and Design — Gabriele Calabria Editor—Francesco Maiocchi DIRECTORS OF DEPARTMENT: Biology and Environmental Science—Scintilla Benevolo Chemistry—Leo Segre Math—Edoardo Rundeddu Physics—Federica Arcidiaco ARTICLES BY: Scintilla Benevolo Gabriele Calabria Matteo De Palma Francesco Grechi Anais Emanuele Leo Segre Yookyung Kim Edoardo Rundeddu Matteo De Angelis Eleonora Pigoli Hongseok Lee Federica Arcidiaco SPECIAL THANKS: Mr. Bonifacio—Supervisor Ms. Rizzuto—CAS Coordinator Mr. Amodio— Publishing Francesco Grechi—Former Director 21 March Issue The Nucleus 2016 American School of Milan SOURCES (In order of appearance) Article: The impacts of global climate change on the arctic food web "The Impact of Climate Change on the World's Marine Ecosystems." The Impact of Climate Change on the World's Marine Ecosystems. Accessed March 14, 2016. http://science.sciencemag.org/content/328/5985/1523. Nature.com. Accessed March 14, 2016. http://www.nature.com/nature/journal/v416/n6879/abs/416389a.html. “Canada's Action on Climate Change." Climate Change - Government of Canada. December 10, 2013. Accessed November 1, 2015. http://www.climatechange.gc.ca/default.asp?lang=en&n=65CD73F4-1. Article: Biological 'clock' discovered in sea turtle shells "Biological Clock Discovered in Sea Turtle Shells." Science Daily. Accessed March 9, 2016. https://www.sciencedaily.com/releases/2016/01/160106114719.htm "Biological 'Clock' Discovered in Sea Turtle Shells." Science Newsline. Accessed March 9, 2016. http://www.sciencenewsline.com/summary/2016010620010018.html. Article: New Tarantula Named After Johnny Cash “Pensoft Publishers. "New tarantula named after Johnny Cash among 14 spider species found in the United States." ScienceDaily. www.sciencedaily.com/releases/2016/02/160204175445.htm (accessed February 29, 2016). 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Article: The new era in carbon allotropes Hirsch, Andreas. "The Era of Carbon Allotropes." Nature.com. October 22, 2010. Accessed March 20, 2016. http://www.nature.com/nmat/journal/v9/n11/abs/nmat2885.html. Article: Counting the hard way Dvorsky, George. "Why We Should Switch To A Base-12 Counting System." Io9. January 18, 2013. Accessed February 28, 2016. http://io9.gizmodo.com/5977095/why-we-should-switch-to-a-base-12-counting-system. "Introducing Binary." BBC Bitesize. Accessed February 28, 2016. http://www.bbc.co.uk/education/guides/zwsbwmn/revision. Article: What to know before playing the lottery "Flash Facts About Lightning." National Geographic. June 24, 2005. Accessed February 13, 2016. http://news.nationalgeographic.com/news/2004/06/0623_040623_lightningfacts.html. "Ten Things You Have Better Odds Of Than Winning The Mega Millions." 94.7 The Wave. March 27, 2012. 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"We've Detected Gravitational Waves, So What? : DNews." DNews. Accessed February 28, 2016. http://news.discovery.com/space/weve-detected-gravitational-waves-so-what-160213.htm. Radford, Tim. "Gravitational Waves: Breakthrough Discovery after a Century of Expectation." The Guardian. 2016. Accessed February 28, 2016. https://www.theguardian.com/science/2016/feb/11/gravitational-waves-discoveryhailed-as-breakthrough-of-the-century. 24 March Issue The Nucleus 2016 American School of Milan Twilley, Nicola. "Gravitational Waves Exist: The Inside Story of How Scientists Finally Found Them." The New Yorker. Accessed February 28, 2016. http://www.newyorker.com/tech/elements/gravitational-waves-exist-hereshow-scientists-finally-found-them. Article: The Physics behind the Leap Year Sabur, Rozina. "Leap Year 2016: Why Does February Have 29 Days Every Four Years?" The Telegraph. 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