1 senior - DOST Sci
Transcription
1 senior - DOST Sci
SENIOR 1 S Y 2000 - 2 0 0 1 V o l . 20 N o . 1 C O N T E N T S REACHING FOR THE STARS Can we possibly visit our neighboring galaxies? ib er s, De ar BB su bs cr THE SPACE SHUTTLE: DEPLOYING A SATELLITE PAYLOAD The U.S. Space Shuttle happens to be an intrepid space truck. ma ki ng ma ga zin e is Ba to Ba la ni ga zin e. ma e rit vo fa to yo ur called so me ch an ge s on cti se w ges is a ne nt ifi c ie Among the chan sc .” It de al s wi th th at ns “P se ud os ci en ce io pt ce on sc an d mi ve ha no tio ns , my th s, we , so at on e tim e. Al we re po pu la r ct io n to se ” rld wo er “C yb ex pa nd ed ou r se ct io n. lin ke d ac tiv ity in cl ud e a we bll help ese changes wi We hope that th le va nt re re mo nc e stu di es ma ke yo ur sc ie y! En jo an d mo re fu n! ON TARGET: THE STEALTH AIRPLANE How do you turn an entire plane invisible? Th e Ed ito r TWISTING IRON Riding in a roller coaster is exciting. And understanding the forces that governs its travel as it glides along the rail may create more excitement. R E G U L A R F E AT U R E S 3 Science & Technology News 5 Filipino Scientists and Inventors BOARD OF ADVISERS Violeta Arciaga, Jaime F. Bucoy Jose C. Calderon, Victoria V. Cervantes, Juanita M. Cruz, Belen P. Dayauon Medical Facts and Fallacies 9 Livelihood Technology / I’d Like to Know CONSULTANT Merle C. Tan, Ph.D. DIWA OFFICERS 10 Cyber World 14 Earth Care 16 Investigatory Projects EDITORIAL BOARD Saturnino G. Belen Jr. President Lourdes F. Lozano Executive Editor Amada J. Javellana Executive Vice President William S. Fernando Managing Editor Enrique A. Caballero,Reynaldo M. de la Cruz, Alvin Fl. Julian Magazine Editor 19 Pseudoscience Carlo F. De Leon,William S. Fernando, Virgie B. Naigan Art Director 23 More Activities To Do Jose Maria T. Policarpio, Elma L. Ropeta, SilvanoC. Santiago Cover Design Lourdes F. Lozano Vice Presidents 24 Mind Games Jose Valeriano P. Linay Layout Design Jun Mediavillo Illustrator R O R R BATO BALANI for Science and Technology is published bimonthly by Diwa Scholastic Press, Inc. Bato Balani is one of Diwa’s Scholastics Enhancement Materials (SEMO). The SEMO trademark refers to a new genre of scholastic publication, comprising a selection of premium - quality magazines for greater learning. All rights reserved. All articles in this publication may be reprinted provided due acknowledgement is given. All communications should be addressed to THE PRODUCT MANAGER, G/F Star Centrum, Gil Puyat Ave., Makati City,Philippines, Telephone numbers 843-4761 to 66. 2 SENIOR Jurassic Spark: I T’S NOT QUITE Jurassic Park, but it’s getting there. Engineers on a Europe-wide project are developing life-size robotic dinosaurs that will walk around museums, chew on plants and interact with visitors as if they had just stepped off the prehistoric plains. The designers want each 3.5-metre-long, 80-kilogram robotic iguanodon to be autonomous, making its own decisions about where to go and what to do. It will approach inquisitive visitors, stare at them, and even rear up on its back legs to browse on the nearest potted palm tree. “Usually you have to walk to museum exhibits. In this case the exhibit walks to you,” says designer Vassilios Papantoniou, who works for the European Association for Research in Legged Robots in Lamia, Greece. The robot will be built from composite resins and aviation-grade Electronic wizardry to bring dinosaurs back to life aluminum. Its movements are based on what is known from iguanodon fossils and studies of modern animals. “A real dinosaur has hundreds of muscles,” says zoologist R. McNeill Alexander of Leeds University, a scientific adviser to the project. “So we’ve had to compromise.” The major muscles are replicated using battery-powered actuators. “We’ve got three in each leg,” he says. The actuators are controlled by their own microprocessors, which are linked to the central processor that controls the beast. A two-metre-long prototype has already been completed. The robot is being funded by the European Union as part of a project to liven up museums. The designers hope to complete a full-size version by 2001. European Association for Research in Legged Robots Which Came First: Black Hole Or Galaxy? A TLANTA—A team of astronomers conducting a systematic search for supermassive black holes has discovered three more of the mysterious objects lurking in the centers of nearby elliptical galaxies. This brings the total number of supermassive black holes definitively identified so far to 20. The discovery was announced at a news conference held during the American Astronomical Society Meeting. “The formation and evolution of galaxies is intimately connected to the presence of a central massive black hole,” said Douglas Richstone, leader of the research team and a University of Michigan professor of astronomy. “Radiation and highenergy particles released by the formation and growth of black holes are the dominant sources of heat and kinetic energy for star-forming gas in protogalaxies.” Richstone says the team’s conclusions are inferred from two pieces of evidence. First, all or nearly all galaxies with spheroidal distributions of stars (bulges in spirals) seem to have massive black holes. The mass of these objects seems to correlate with the mass of the central part of the host galaxy. “The ubiquity of this association, as well as the correlation, points to a connection between the massive black hole and the galaxy, and poses a ‘chicken and egg’ dilemma of which came first,” Richstone said. Second, comparisons of the history of star formation in the universe with the history of quasars, conducted by other scientists, reveal that quasars developed well before most star formation in galaxies. Quasars are extremely powerful bright objects capable of generating the luminosity of one trillion suns within a region the size of Mars’ orbit. University of Michigan SENIOR 3 Nomad Robot Finds Meteorites in Antarctica P ITTSBURGH—Carnegie Mellon University’s Nomad robot, which conducted an autonomous search for meteorites in Antarctica from Jan. 20-30, has successfully completed its mission, examining more than 100 indigenous rocks, studying about 50 in detail and classifying seven specimens as meteorites. An expert from the National Science Foundation’s Antarctic Search for Meteorites (ANSMET) program, who collected the specimens after Nomad identified them in the field, has concluded that five of the seven are meteorites. The other two raise enough questions about their composition to merit further study. ANSMET is housed at Case Western Reserve University in Cleveland. Meteorites are curated at the Johnson Space Flight Center in Houston and made available to scientists around the world. “Nomad has found and correctly classified three indigenous meteorites insitu,” said Dimitrios Apostolopolous, a systems scientist at Carnegie Mellon’s Robotics Institute and project manager of the Robotic Antarctic Meteorite Search initiative. “The robot correctly classified three other indigenous meteorites and misclassified one as terrestrial rock. Nomad achieved these results autonomously and without any prior knowledge about the samples.” Most of the chondrites that Nomad found are relatively common types, composed mainly of rock with small metallic infusions that probably originated from asteroids. One achondrite meteorite which Nomad classified as interesting is so rare that the robot didn’t have the data in its base to make a determination. Carnegie Mellon University U sing a technique called neutral atom imaging from a satellite high above the North Pole, researchers at the Department of Energy’s Los Alamos National Laboratory are developing pictures of the magnetosphere, an invisible magnetic layer around the Earth. These pictures will be essential to a better understanding of the “weather” in space, where a blast of solar wind particles can knock out a multimillion-dollar satellite. Developing what he calls “weather maps for the radiation belts,” Geoff Reeves 4 SENIOR Tracking Weather from the Sky of the Los Alamos Space and Atmospheric Sciences group and Mike Henderson of Los Alamos’ Space and Remote Sensing Sciences group devised a way to take rough, low-resolution satellite data and create more informative composite images of the solarwind-driven particles trapped in the magnetosphere. Used as still pictures or animated for time-lapse movies, their pictures show the ebb and flow of these particles as they near the earth and are drawn around and down the magnetic field lines. These images are especially critical for understanding the progress and structure of a space phenomenon called geomagnetic storms. Geomagnetic storms are the space equivalent of hurricanes in the Atlantic. For years scientists believed that geomagnetic storms were made up of smaller “substorms” which occur more frequently and in isolation. But more recently scientists have found that storms and substorms are related — but distinctly different — phenomena. This is similar to discovering that hurricanes and thunderstorms are related, but that a hurricane is not just a cluster of thunderstorms or a larger, more intense thunderstorm. Future missions to the magnetosphere will carry dedicated, Los Alamos-designed, neutral atom imaging instruments. These include NASA’s IMAGE mission and TWINS, which will provide the first stereoscopic images of the magnetosphere. Los Alamos National Laboratory University of California Dr. Julian Banzon Nuclear Chemist D r. Julian Banzon is a man who dedicated himself to the study and applications of chemistry. At age 23, he was already a noted professor at the University of the Philippines in Los Baños. In 1957, he held the position of chief scientist at the Philippine Atomic Energy Commission (PAEC). Thereafter, he became the first director of the Philippine Atomic Research Center (PARC). He came back to UPLB in 1963, and stayed there as chairman of the Department of Agricultural Chemistry for seven years. The numerous awards, plaque, and citations that Dr. Banzon received are testimony to his achievements as a scientist. The books and journal articles he had written prove his ability as a researcher and teacher. His active participation in local and international conferences, as well as his membership in RABIES Fallacy: One needs to submit to rabies vaccination whenever a dog scratches or bites him. Fact: The common practice whenever a person is scratched or bitten by a dog is to have anti-rabies shots. Actually, the injection is for any animal suspected of being rabid such as cat, fox, rat or even rabbit. A rabid animal is one afflicted with rabies. An anti-rabies injection is not always given whenever an animal bites a person. The animal is first sent to a veterinary clinic for observation. The animal is kept in a place where veterinarians can determine whether or not it develops rabies. If the animal professional and scientific organizations attest to his eminent stature as a chemist and academician. The science community is the richer for scientists like Dr. Banzon. The younger generation is indeed blessed with the research finds and intellectual depth of Dr. Banzon. Source : Saplala, Vivas, and Zafaralla. 1984. Profiles: Men and Women of UPLB, College, Laguna: University of the Philippines-Los Baños, Laguna. is found to be healthy, no immunization is necessary. In case the animal cannot be found, then the injection should be given as a safeguard. We cannot take any chances that rabies may develop as it has a very high mortality rate. The affected area, whether it was broken or not, should be washed thoroughly with soap and water. The washing should last for approximately 10 to 20 minutes. The rabies immunization vaccine is very effective against rabies. There is no danger of harmful side effects if somebody is given the rabies vaccine even if the animal in question does not develop rabies. SENIOR 5 P H Y S I C S A ssuming that the stars you see in the sky on a clear night were reduced into the size of the grains of sand, you can actually hold them all in the palm of your hand. However, the stars you see with your naked eye is just a tiny fraction of the stars that are in the universe. Scientists believe that the number of stars in the Cosmos is more than all the grains of sand on all the beaches of the world. The universe is so unimaginably huge beyond compare that most of it is empty of stars. Because of the great distances that separate us from neighboring stars, it will take years, even for light, to cross the interstellar space. For instance, the nearest star system to our Sun is Alpha Centauri with a distance of 4.35 light-years (a light-year is the distance light travels in a year, about 9.5 trillion kilometers). This means light will take 4.35 years, as measured in our time, to reach us. For light, however, time stands still. The great void seems to put a clamp on man’s dream to reach the stars. Moreover, Einstein’s special theory of relativity puts a limit to the speed a material object can attain — at lightspeed of 299,792,458 meters per second. But we have evolved with a brain that possesses unlimited capacities to go around what Nature has imposed upon us. Travelling at or near the speed of light produces paradoxes that run counter to common sense. According to the special theory of relativity, light travels at a constant velocity whether the source is moving or not. This means you just cannot add your speed to the speed of light. Otherwise, you could attain any speed you want by hitchhiking on a fast-moving mother vehicle. Another rule codified by Einstein in his special theory of relativity is that the laws of Nature must be applicable to everybody anywhere in the universe. This means that there is no fixed frame of reference 6 SENIOR from which to view the universe. Everything is relative, depending on his position with respect to another. Hence, the name relativity. No one can travel at, or faster than, the speed of light. Nothing in physics, however, prevents you from traveling as close to the speed of light as you like, say at 99.99 percent lightspeed. Can we travel close to lightspeed? Let’s make a Gedanken experiment (a thought experiment, like what scientists do, including Einstein, when trying to explain the consequences of the relativity theory). Imagine that you hitch a ride in a futuristic spaceship that could accelerate up to lightspeed. As the spaceship gains speed, you begin to see around the corners of passing objects. You are facing forward in the direction of motion but things behind you appear within your forward field of vision. From the standpoint of a stationary observer, you appear red when you depart because light reflected off you is shifted to the red portion of the spectrum, and you appear blue when you return, a process that could be explained by the Doppler effect. If you approach the observer at almost the speed of light, you will return shining brightly — your invisible infrared spectrum will be shifted to the visible wavelengths. The observer will see that you become compressed in the direction of motion, that your mass increases, and that your time slows down — a consequence called time dilation. But from the standpoint of the persons you are travelling with inside the spaceship, neither of these effects occurs to you. But really, how close can we accelerate up to lightspeed in practical terms? Dr. Charles Pellegrino has an answer. In his book “Flying to Valhalla,” Dr. Pellegrino proposed a 92 percent lightspeed for his particular spaceship. Why 92 percent lightspeed? According to him, 92 percent lightspeed is a realistic velocity to aim for. At 92 percent lightspeed, you will age at a rate only one-third of the rest of the universe. To an outside observer, the spaceship would appear to have shrunk to less than half of its original length, and would seem three times as massive, meaning three times as resistant to acceleration. And from your point of view, the entire universe is being compressed ahead of the spaceship into a dome that occupies only one-third of the sky. Now as the spaceship accelerates further up to lightspeed, to outside observers, the spaceship appears to have no length at all (infinite compression). Of course, the power required demands infinite energy, which the spaceship could never have. At lightspeed, you and your companion including the spaceship, cease aging altogether. You will traverse the length and width and breadth of the universe in an instant. These strange things happen because our familiar ideas of space and time are no longer valid when you approach lightspeed. Speed is distance divided by time and since you cannot simply add speeds near the velocity of light, space and time must change. That is why you shrink and you hardly age at all. But in terms of practical engineering, is it possible to travel close to the speed of light? Can we build a kind of ‘lightship’ based on theories and principles we have today? Most of the time, revolutionary ideas are far advanced for technology to catch up to. For instance, in 1939, the British Interplanetary Society designed a rocketship whose objective was to take people to the Moon — using the technology of the 40s. However, it was only three decades later that the Moon mission was accomplished by Apollo 11 in 1969. Today, we have preliminary designs for starships whose ultimate design objective is to take SENIOR 7 P ○ ○ ○ ○ ○ ○ H ○ ○ ○ ○ Y ○ ○ ○ ○ S ○ ○ ○ I ○ ○ ○ C ○ ○ ○ S ○ ○ ○ ○ ○ ○ ○ ○ ○ ○ us to the stars. One of these is Orion, a design that calls for explosions of hydrogen bombs against an inertial plate as a means of propulsion. The Orion spacecraft seems practical from an engineering point of view, but will produce vast quantities of radioactive debris. Another design is Daedalus, using a nuclear fusion reactor, assuming we could develop a fusion engine in the next few decades. Orion and Daedalus might travel at 10 percent light speed. A trip to Alpha Centauri then would take 43 years, less than a human lifetime. Such designs, however, could not travel close enough to lightspeed for time dilation to become important. For voyages beyond the nearest stars, starships with velocity approaching the speed of light are in principle possible, though it would take our technology thousands of years to catch up with the ideas. An example of an interstellar starship is the Bussard ramjet. The Bussard spaceship will have a gigantic scoop to collect diffused matter in space (mostly hydrogen atoms), and accelerate it into a fusion engine, then eject it out. Dr. Pellegrino has made feasibility studies for a starship that could reach 92 percent lightspeed. His design is an antimatter spaceship (he calls it the Valkyrie) that uses antihydrogen as a propellant. Antimatter is so far the ultimate fuel for propulsion because one hundred percent of the mass of matter and antimatter is converted to pure energy. (In contrast, only one percent of the matter in a hydrogen bomb is converted to energy during explosion.) Ninety-two percent lightspeed is chosen because, according to Dr. Pellegrino, at speeds higher than this, particles of dust impacting against the spaceship will explode like large hand grenades. Furthermore, the amount of fuel required to accelerate from 92 to a higher speed, say 95 percent lightspeed, is twice as much as the acceleration from 0 to 92 percent. 8 SENIOR If you travel with the Valkyrie, the long space voyage from the Solar System to Alpha Centauri will take less than two years. With the Bussard spacecraft, a trip to the center of the Milky Way would take you 21 years. Of course, people on Earth would measure an elapsed time of 30,000 years. From the point of view of the travellers, relativistic flight is surely a one-way ticket to eternity. 1. Why is an antimatter spaceship suitable for travelling close to lightspeed? 2. From your own perspective, what happens to the universe if you can travel at lightspeed? 3. Why is 92 percent lightspeed significant from an engineering point of view? Doppler Effect – an apparent change in the frequency of sound, light, or radio waves reaching an observer when the wave source and the observer are in motion relative to one another. Interstellar space – the space between stars. Thought experiment – a fictitious story used to illustrate a scientific principle. REFERENCES Pellegrino, Charles. 1993. Flying to Valhalla. New York: Avon Books. Sagan, Carl. 1980. Cosmos. New York: Ballantine Books, Random House, Inc. Q:How fast is supersonic transport? Imagine yourself travelling faster than the speed of sound. That is how fast supersonic transport is! A: Travelling at speeds faster than sound is referred to as Glisa F. Sanchez Angeles University Foundation Angeles City supersonic flight, from the terms super (meaning “over” or “above”) and sonic (relating to sound waves). As compared to sound waves that travels at about 1,220 kilometres per hour through air at sea level, supersonic aircrafts can travel from one to five times the speed of sound! Gulaman G Bars ulaman Bars are processed substance from agar dhiella seaweeds. Used in different recipes, they are especially prepared for delightful desserts. People who live by the sea process gulaman bars as a small- or medium-scale industry. You can prepare your own gulaman bars just like the experts by following this simple procedure. Ingredients: seaweeds acetic acid or vinegar, water Procedure: 1. Gather the seaweeds and rinse them in clean water. 2. Dry them under the sun and soak overnight in clean water. 3. Add three litres of water and one teaspoon of acetic acid or vinegar for every 100 grams of seaweeds. 4. Boil the mixture for one hour and filter it through a cheesecloth. 5. Boil again and repeat the same procedure to maximize gelatin extraction. 6. Pour the collected substance called agar on aluminum molds 20 cm long and four cm deep. Allow the agar to solidify at room temperature. 7. Cut into four cm wide bars and put inside a freezer for five days. 8. Thaw the bars in running water and dry them under the sun. SENIOR 9 A good computer programs starts from As a convention, a flowchart begins on top a good design. One way of designing of the page and the end of the program is placed a program is by using a method at the bottom of the page. You need not know called flowcharting. Flowcharting is a programming code to flowchart. Simply use method of showing the flow of a ordinary language first and as you grow into program using symbols. If the flowchart is designed programming you will learn to use actual properly, then it becomes very easy to create the computer codes in your flowchart. For now it is program code. Below are some conventional symbols sufficient to use simple words (See the sample used for flowcharting. flowcharts). 10 Process Box The rectangle represents an action, computation or process that needs to take place. Input/Output Box (I/O Box) The parallelogram is used when a value has to be entered or something has to be displayed on screen. Decision Box The diamond is used to signify that a decision has to be made. Each decision can have only two possible outcomes, true or false. Flowlines These arrows point in the direction of the next action to be performed. Think of these as directional signs that point you in the right way. Connectors These circles indicate a “jump” in the program. Sometimes your program needs to jump to another part of the flowchart. Terminal Symbol These ovals will signify the beginning or end of the program. Simply write START or END inside the oval. SENIOR www.batobalani.com START START Would you like to become Interactive? Enter 2 nos.X,Y Input A,B X+Y=Z SUM = A + B Display C Print SUM END END These are two flowcharts for the same program. The flowchart on the left uses plain English to explain what the program will do. The flowchart on the right uses actual programming code from BASIC* to show what the program will do. Try to understand both flowcharts. Can you guess what the program does? *Beginners All-purpose Symbolic Instruction Code (BASIC) B atobalani magazine is now on the internet. In the Batobalani website are archives of current and past issues as well as a variety of activities and additional topics for the inquisitive student of science. In subsequent issues of the magazine, we will discuss the different activities we have prepared for you. One useful feature in the website is a feedback or response page. This allows you to send us your comments and even contribute your own article. By simply typing it in or pasting it on the dialogue box. You will need to have a computer unit with a modem and a valid account with any authorized internet service provider (ISP) such as Mozcom, Infocom, Philonline, or any other ISPs. To write us, simply follow these steps: 1). On your computer, open up an internet browser program. For most of you, this would be Microsoft’s Internet Explorer or Netscape’ Navigator’s program. Make sure you are connected to your Internet Service Provider. 2). On the address window of your browser program, type www.batobalani.com, then hit the “enter” key. 3). You will see Batobalani’s homepage on your screen. Also, you will see a menu of sections you can go to on the lower right side of the screen. Choose “Feedback” and click the left button of your mouse. 4). The feedback page will show you different boxes for you to fill in. Go ahead and fill the information. You may skip the items that you cannot fill up. Then on the Message box, type in your message or your opinion or even a simple “hello.” 5). Once you’re finished with your message, hit the “send” button by clicking the left button of your mouse. Presto! You’ve sent us your message. There are many other interesting things you can do inside Batobalani’s website. Feel free to explore. If you have questions or need further instructions, why don’t you try sending it to us using the feedback page. We hope to hear from you soon! WSF SENIOR 11 A n artificial satellite is any object placed into orbit around the earth and used for a variety of scientific and technological purposes. The former Union of Soviet Socialist Republics (USSR) launched the first artificial satellite, Sputnik 1, on October 4, 1957. The first United States satellite, Explorer 1, was launched on January 31, 1958, and was instrumental in the discovery of the radiation belts around the earth. In the years that followed, several thousand satellites were launched, monopolized by the United States and the former USSR in a battle for space supremacy until 1983, when the European Space Agency began launching from a space center in French Guiana. On August 27, 1989, for the first time in aerospace history, a privately owned rocket was used to launch a satellite. The rocket, built and launched by a U.S. company, placed a British television broadcasting satellite into geosynchronous orbit. Satellites are usually placed into orbit by multistage rockets. In part to reduce satellite launching costs, the National Aeronautics and Space Administration (NASA) uses the space shuttle to carry satellites in its cargo bay and launch them into orbit. The minimum initial velocity required for an object to escape the gravitational pull of an astronomical body, and to continue traveling away from it without the use of propulsive machinery is called escape velocity. The escape velocity is usually given in terms of the surface-launch velocity, disregarding aerodynamic friction. Objects traveling at less than 0.71 × 11.2 km/s (the escape velocity of Earth) cannot achieve a stable 12 SENIOR orbit. At such velocity, the orbit becomes circular, and at higher velocities, the orbit becomes elliptical until escape velocity is reached. Then, the orbit becomes parabolic. (Escape velocity is thus also known as parabolic velocity). The escape velocity of an object from a spherical astronomical body (like the Earth) is proportional to the square root of the mass of the body divided by the distance between the object and the center of the body. A space shuttle designed to leave the earth as a vertically launched rocket must weigh at least 2 million kg with 3 million kg of thrust from its multiple propulsion systems. The two solid rocket boosters (SRBs), with a combined thrust of some 2.6 million kg, will provide most of the power for the first two minutes of flight. The SRBs will take the space shuttle to an altitude of 45 km and a speed of 4973 km/hr before they separate and fall back Jerard F. Beltran into the ocean to be retrieved, refurbished, and prepared for another flight. After the boosters fall away, the three main engines continue to provide thrust. These engines are clustered at the rear end of the orbiter and will have a combined thrust of almost 540,000 kg. The space shuttle’s liquid-propellant engines will be the world’s first reusable rocket engines. They fire for only eight minutes for each flight, just until the shuttle reaches orbit, and are designed to operate for 55 flights. The engines are very large—4.2 m long and 2.4 m in diameter at the wide end of the cone-shaped nozzle at the rear of the orbiter. Another propulsion system takes over once the space shuttle’s main engines shut down as the ship approaches the altitude at which it will begin orbiting around the earth, known as the orbital insertion point. Two orbital maneuvering system (OMS) engines, mounted on either side of the aft fuselage, provide thrust for major orbital changes. For more exacting maneuvers in orbit, 44 small rocket engines (known as the reaction control system), clustered on the shuttle’s nose and on either side of the tail, are used. They have proven indispensable in performing the shuttle’s important work of retrieving, launching, and repairing satellites in orbit. The giant, cylindrical, external fuel tank, with a length of 47 m and a diameter of 8.4 m, is the largest single piece of the space shuttle. It fuels the orbiter’s three main engines. During launch, the external tank also acts as a support for the orbiter and SRBs to which it is attached. Made from aluminum alloys, the space shuttle’s external fuel tank is the only part of the launch vehicle that currently is not reused. After its 1.99 million liters of fuel are consumed during the first 8.5 minutes of the flight, the external tank is jettisoned from the orbiter and breaks up in the upper atmosphere, its pieces falling into remote ocean waters. After placing the satellite in orbit, the orbiter segment returns from space—withstanding the intense heat when entering the earth’s atmosphere. Flown by the shuttle crew much like an aircraft, the shuttle lands horizontally on a conventional airport runway. 1). What are the benefits of satellites? Orbit — the path an object takes as it travels around another object. "Satellite, Artificial,” Microsoft® Encarta® 97 Encyclopedia. © 1993-1996 Microsoft Corporation. All rights reserved. "Escape Velocity,” Microsoft® Encarta® 97 Encyclopedia. © 1993-1996 Microsoft Corporation. All rights reserved. "Space Shuttle,” Microsoft® Encarta® 97 Encyclopedia. © 1993-1996 Microsoft Corporation. All rights reserved. SENIOR 13 Save Our Seas: A Crusade for Coral Reefs Mary Ann Aleli V. Barbieto O n September 11, 1992, a terrible Their mission - hurricane swept through Hawaii’s “To preserve, protect, island of Kauai. Surprised that such and restore the health destruction could happen in such a and well-being of the short time, three people got together and organized a world’s oceans for truly dynamic group whose main purpose was to future generations.” – protect and preserve the fragile marine ecosystem. was integrated into the These three were Carl Stepath, the owner and laws of the state of operator of Nawiliwili Marine and Sailboards Kauai; Hawaii within the next Teresa Tico, a lawyer who was into bodysurfing, yacht year, and with much racing and windsurfing; and Nicholas Barran, a enthusiasm, they set computer programmer who also loved yacht racing. out on their first Through the efforts project. This was the of these Open Seas Recycling Program, which they launched concerned during the 1993 Trans Pac Yacht Race, a racing citizens, Save competition where yachts ran from the coast of Los Our Seas Angeles to Honolulu. The board of directors who held (SOS), was the contest were thrilled with their proposed project, born. 14 SENIOR Our and immediately decided that recycling should not participate in this “adopt a reef” program, where the only be a part of a program, but a requirement for students survey corals, marine life, and measure those who were competing in the race. They added a water quality, then report back to SOS via the new regulation that all trash must be kept on board, Internet. These results are then compiled and used and all recyclable materials - paper, aluminum and for future reference in finding ways to save our glass - were the responsibility of the racers and must speedily vanishing coral reefs. be recycled before they reached the finish line. At These children become responsible for the reefs, the end of the race, the project proved to be so and are then called “reef keepers.” SOS hopes that successful that it was adopted by yacht clubs in these children will realize how important it is to care Japan and Australia. for our coral reefs and our entire ocean ecosystem. The Philippines is taking part in another project sponsored by Save Our Seas, “Ocean Pulse.” Its aim is to educate the community about our coral reef’s complex ecology though direct interaction with the living, breathing corals that surround our Through their hands-on experience, they learn how to be more careful in dealing with nature. Do you want to become a part of SOS and contribute to the preservation and care of our oceans? You can visit their website at: archipelago. This project involves students from all over the country and began in their native Hawaii, where they enlisted the help of seventh and eighth http://hookomo.aloha.net/~sos~/ . You can also write to them at sos@aloha.net. graders whose schools have volunteered to create Resources: SOS homepage databases for Save Our Seas. Schools who SENIOR 15 I N C O O P E R AT I O N W I T H T H E DEPARTMENT OF SCIENCE AND TECHNOLGY UV IRRADIATION TO CONTROL GROWTH OF ASPERGILLUS FLAVUS IN COPRA ABSTRACT: control. A. flavus growth in copra was alfatoxin tolerance level of 0.2 parts per then determined. Previously dried copra million (ppm) for copra meal and 20 parts of controlling the growth of Aspergills (‘kokum”) were moistened, inoculated per billion (ppb) for coconut oil. flavus in copra with ultraviolet (UV) with A. flavus, then exposed to 15- minute radiation. UV irradiation. The growth of the fungus This study explores the possibility Pure cultures of A. flavus were prepared in nutrient agar. These were exposed to different durations of exposure to UV radiation (quartz tube-mercury vapor source, wavelength approximately 240nm-270nm): 1, 3, 6, 10, and 15 minutes. The growth rate of the fungus was observed in three replications. Among the five treatments, UV radiation of 15 minutes controlled the growth of the fungus to the greatest extent. This could be due to the damage on the DNA which led to abnormal physiological functions and death of the cell. irradiation inhibited up to 92% of the fungal growth. INTRODUCTION A few years ago, the Philippines lost much of the United States market for SENIOR fungus, Aspergillus fluvus. It has been found to cause cancer in animals ingesting it. It is very potent in this respect with no more than 0.05 ppm capable of inducing illness. Aflatoxin is also a natural mutagen. The control of aflatoxin copra because it took very little notice of contamination in copra depends mainly on the restrictions imposed on copra the inhibition of the growth of A. flavus. contaminated with aflatoxin. Last Growth of A. flavus is enhanced by December 1990, the European Economic factors such as high relative humidity, Community (EEC)— which absorbs 46.6 high moisture content and warm percent of the country’s coconut oil export temperature. and 30 percent of copra— implemented a policy to standardize aflatoxin (Lorito, The effectivity of UV radiation to 16 was observed after five days. 15-minutes Aflatoxin is produced by the 1990). This regulation imposes an This study aimed at determining the relative sensitivity of A. flavus to highenergy radiation. Specifically it determined the effects of UV on the high-energy radiation such as ultraviolet growth rate of A. flavus. rays, X-rays and gamma rays. Radiation REVIEW OF LITERATURE causes dimerizations (linking) and synthesis is proceeding. Increasing the causing metabolic abnormalities. This fungus classified under Division prevents further growth or reproduction of Eumycophuta, Class Ascomycetes. It fungi in copra. present. Because of this, its growth in agricultural products is difficult to control. Moreover, the spores of the fungus are all around so that the possibility of contamination is great (Gloria, 1989). The presence of A. flavus is undesirable especially in copra, peanuts, corn, soybeans and potatoes. In copra, contamination can start after harvest when the nut is broken on the ground and the coconut meat scooped from the shell. Placing the copra in sacks which may be laden with. A flavus spores further increases the chances of contamination. Contamination is usually dose of UV light both increases the probability of mutation per unit of time (Fincham, 1965). usually grows in moist warm environments where carbohydrate is The mutagenic effects of UV depends on the stage at which protein ionizations in th DNA of the fungus A. flavus is a brownish-green (Sylianco, 1983). Low doses of UV delays budding or germination of the fungus. Cells MATERIALSAND METHODS: A. flavus used in this study was a irradiated with UV of wavelengths ranging from 280nm – 380 nm did not begin to pure culture derived from the RP-UK bud as early as the controls – in some Aflatoxin Research Project of the cases they never budded. A small Philippine Coconut Authority, Mintal, percentage of spores which survive Davao City. exposure to UV radiation may produce A quartz tube-mercury vapor mutants. source from the Ateneo de Davao During UV irradiation the normal University with wavelength ranging from hydrogen bond-interaction between bases 240nm to 270nm was used. Treatment are cleaved. This may lead to interruption was done on A. flavus for 1 min. (T1), 3 of replication, or division may stop short mins. (T2), 6 mins. (T3), 10 mins. (T4) or may proceed incorrectly with an altered and 15 mins. (T5) base sequence. Therfore, the effects of UV The other materials were: radiation on living tissues is a consequence of its effect on the bases of 10 mL coconut extract DNA and RNA (Sylianco, 1981) 10g dextrose powder minimized if the coconut is dried within four hours after splitting. Drying in the “tapahan” is usually favored over sun drying because it reduces the moisture content to about 10-15 percent in a short time. If the copra is properly dried, the possibility of contamination is nil. But again, the chances of contamination increases during storage, when the Changes produced by radiation 100g “kokum” may be a direct effect on the molecules where the energy has been absorbed, or 700 mL distilled water indirect effects in which molecular changes are bought about by the chemical 1 pressure cooker reactions of free redicals produced as 1 inoculating set primary effect radiations (Lea, 1955). Calculations shows that radiation humidity inside the storehouse is high and which destroys perhaps only one molecule air circulation is inadequate (Gloria,1989). in a million can have profound biological A. flavus could be susceptible to 18 petri dishes 1 improvised inoculating box Part 1. 5 mL of agar with coconut extract consequence and can kill the cell SENIOR 17 to the A1, A2, and A3 setups. B1, B2 and were poured into 18 petri dishes at a depth sq. cm/day, with about 90% mutation. B3 were made as control. of about 2mm. The dishes were covered and sterilized for about 15 minutes. They were then placed in an inoculating box and were allowed to cool and solidify. The coconut-agar media were innoculated with A. flavus spores using Observations were made on the five days. Gloria, M. “Aflatoxin and Copra”. contaminated with A. flavus was determined. The percentage contamination Southern News Scope. August 1989. Vol. was then calculated. From the difference, 2 p.8 the percentage inhibition was determined. the disc method and were placed in a dark chamber with 29 to 30oC temperature for SELECTED REFERENCES: fifth day, after which the mass of the copra RESULTSANDANALYSIS Gincham, J.R.S. 1965. “Fungal Genetics”. Blackwell Scientific publications. The average growth rate of A. The growth rate of A. flavus was determined in sq. cm. Counting was performed using a graphing paper with a 1 sq. cm. grid placed underneath. flavus in the control and in treated medium are as follows: University Press. From day 1 to day 2, the fungus in the controlled setup covered a very much Growth rate was determined by the formula: Lea, D.E. 1963. “Actions of Radiation on Living Cells”. Cambridge Lonito, D.L. 1990. “Behind the bigger area as compared with those in T1, Aflatoxin Scare”. Mindano Farmers T2, T3, T4 and T5. However, its growth Journal. tapered off after the second day. The Sylianco, C.Y. 1981. “Modern s = a/d fungus in T1, T2, T3 and T4 covered a Biochemistry” Philippine Graphic Arts, where: smaller area during the first two days. It Manila. then accelerated after the second until the a is the area in sq. cm fifth day. The setups in T5 showed least growth of the fungus. d is the time in days s is the rate in sq. cm/day Microscopic examinations of the irradiated molds were conducted every 24 hours. Irradiation of 1,3, and 6 min. duration caused little damage to A. flavus. 10 min. exposures caused greater damage to A. flavus. 15 min. exposures actually inhibited the growth of A flavus on Part 2. experimental copra samples, by about Six sets at 20g each of “kokum” dried copra were soaked in water for 5 91.8%. The fastest growth rate was minutes, then drained and placed in petri observed in the control, 8.3 ± 0.6 sq. cm/ dishes. The dishes were labelled A1, A2, day, followed by those exposed for 1 min, A3, B1, B2, and B3. The copra samples 3 min, then 6 min. and 10 min. Those were all inoculated with A. flavus spores. treated for 15 min. showed only a total of A 15 minute irradiation was given 18 SENIOR 12.5 ± 3.1 sq. cm or a growth rate of 0.83 UV Treatment Control 1 min. 3 min. 6 min. 10 min. 15 min. Growth rate (sq. cm/day) 8.3 ± 0.6 5.4 ± 0.5 4.8 ± 0.6 4.5 ± 0.6 2.7 ± 0.6 0.83 ± 0.5 The Philadelphia Experiment Joe Bert G. Lazarte Remember the 1984 film The Philadelphia Experiment? T he movie was based on an alleged United States Navy experiment(Project Rainbow) done on October 28, 1943. According to legend, the destroyer USS Eldridge was made invisible, dematerialized, and teleported from Philadelphia, Pennsylvania, to Norfolk, Virginia, and back again to the Philadelphia Naval Yard. The experiment allegedly had such terrible sideeffects, such as making sailors invisible and eventually going mad, that the Navy quit exploring this exciting new technology. The experiment was allegedly done by Dr. Franklin Reno as an application of Einstein’s unified field theory. The experiment supposedly demonstrated a successful connection between gravity and electromagnetism: electromagnetic space-time warping. One Carlos Allende, or Carl Allen, claimed that he witnessed the experiment. In fact, he was one major source of stories about the experiment, who, as further writings and probings into his background surfaced, later proved to be a conman who weaved the hoax. Surprisingly, one retired military man, Alfred Bielek, picked up where Allen left the story. Bielek’s memories apparently came back to him after watching the 1984 film, coming up with more detailed explanations of the experiment. He co-authored a book, The Philadelphia Experiment and Other Conspiracies, which merely rehashes the usual stories of CIA plots, government conspiracies, secret meetings with aliens, trips to Mars, visits from the Men in Black, etc. He also came out with a video in which he presented himself as someone who was part of the team that conducted the experiment, time-traveled in 1943 to 1983 during the experiment and lived to tell the story, only to be harassed by the U.S. government for his troubles. But in the face of these myths, the Navy came out with its official documents that take note of the story’s salient points, such as: (1)there was no such project as the Philadelphia Experiment, no experiments into invisibility. There were projects codenamed Rainbow, but they were warplans to defeat Italy, Germany, and Japan; (2) The Office of Naval Research, under which the experiment was supposedly conducted, did not even exist until 1946; (3) The U.S.S. Eldridge was never even in Philadelphia during the fall of 1943, and the deck log that proves this is available on microfilm via the web. What the Navy documents do add, moreover, are some valid points on the subject of degaussing, which is a process, and when correctly done, makes a ship “invisible” to the sensors of magnetic mines, but remains visible to the human eye, radar, and underwater listening devices. They also note that while experimenting with 1,000 hz generators in the 1950s, “the higher frequency generator produced corona discharges, and other well-known phenomena associated with high frequency generators,” which can be exciting when viewed. This sounds plausibly like the genuine seed for the story, which people like Jessup, Carl Allen, and Bielek weaved stories from. Such is the stuff urban legends are made of. SENIOR 19 P H Y S I C S On Target: The Stealth Airplane R adar, or radio directing and ranging, is one of the most vital devices needed by the defense department of any country. It is very valuable in tracing the position of enemy ships and airplanes during wars and conflicts. But since its invention however, a lot of research and technology has been developed to counter-attack it. One of this is stealth technology. The main purpose of this system study is for antidetection. This technology had already begun development in World War II when snorkels of German U-boats were coated with radar- absorbing materials. Since then, researches were done in secret laboratories to determine other ways radar detection can be avoided or at least minimized. Special attention was given to aircrafts. In the early 1970s, The US Department of Defense and US Air Force collaborated for this work. Studies were conducted and bore fruitful results. These studies 20 SENIOR ranged from chemistry and composite materials to likewise strategically placed all over the plane. computer-aided design and manufacture, all aiming for Suggested paint color is black in order to elude visual the reduction of the identification of future-weapons detection since a the stealth airplane is designed to delivery and surveillance systems used in air warfare. operate by night. However, further research is made With this quality, any type of aircraft will have a higher concerning visibility in order to make the plane invisible chance of survival in the battle arena. even during daytime. The first process in making a stealth Exhausts from an aircraft are also detectable by airplane is to create a special design for radar. Scientists in stealth research also have given the aircraft. One may notice the unique this keen focus. Since the engine emits geometry of a Northrop B-2, for example. To infrared or heat-source radiation, the understand this better, it is necessary to know stealth’s exhaust sections are how radar works. Regardless of whether it is flattened into thin, long slots that airborne or ground-based, the radar ‘sees’ its are layered with cold air. Direct target object within a range of 30 degrees around injections of powerful chemical its own horizontal plane by emitting radio beams coolants are then applied to the exhaust and waiting for them to bounce back upon contact gases, so that they would mix with the with the object. It can then measure the length that outside air unnoticeably. the beams had traveled and equate it as the distance of the object from the radar source, thus determining the target’s position. And yet, along with this great innovation comes a great price: Both in dollars and performancewise. Each of the first fifteen Northrop B-2 costs $776 This suggests that a stealth aircraft’s design needs million, making it the most expensive warplane built in to be as flat as a straight line as possible when viewed the last few years. The stealth program has amassed a horizontally. If it did need to curve however, it ought to total of $43 billion expenditures to date, just by making be the double-curvature type so that reflection can be an aircraft that cannot be detected by radar. Other minimized. Known as reflective faceting, the plane is problems encountered aside from the high cost is its designed to have slabs or facets having angular relativity lower acceleration rate compared to ordinary fighter so as to divert the radio beams away from the source. planes because it had to use turbofan engines with no Another process in anti-radar detection is coating the stealth with radar-absorbing materials, namely pyroceramics, polyurethanes, silicones, and rubber and carbon compounds. Several corner reflectors designed afterburners. Add to that is the plane’s need of a repainting job after every mission. Microsoft® Encarta® Encyclopedia Deluxe 2000. © 1993-1999 Microsoft Corporation. to catch, trap and scatter radio frequency energy are SENIOR 21 P H Y S I C S TWISTING IRON TWISTING IRON n many theme parks around the globe, one of the most sought-after ride is the roller coaster. In Laguna, the Enchanted Kingdom theme park offers the mind-numbing “Space Shuttle,” a 1minute ride that takes you through two 360 degree loops and varying side-twists and turns. Then you go through the whole thing again, this time backwards! Most kids find the ride fun and enervating. The serpentine iron rail gleams like some giant torture instrument in the daytime. And the shrieks and screams from those in the hurtling train seems to confirm that. I “wanting” to break out of the loop. Many brave kids try to lift their arms above their heads as they turn upside down going through the 360 degree loop. They are trying to resist the action of the centrifugal force. But roller coasters are governed by natural laws that permit its riders to have fun while seemingly courting disaster with its neck-breaking speed and jaw-breaking twists and turns. There are other roller coaster rides in the Philippines. The next time you try one, try to observe the various forces that act on your body as it turns, twists and turns upside down. It is best to remember to keep your sunglasses, hat and other paraphernalia tucked in securely in your pockets before they are wrested from you by the various natural forces that govern the movement of the roller coaster. As the shuttle’s wheels clamp down against the rail in a sharp sideways turn, the friction between the tires and the rail must sustain sufficient sideways force to provide the necessary centripetal force for curved motion. Centripetal (“center-seeking”) force is the radial force required to keep an object continually diverted in its path so that it travels in a circle. In this instance, centripetal force keeps the shuttle along a curved path as it travels along the rail. Centrifugal (“center-fleeing”) force refers to the same phenomenon as centripetal force but may be considered the equal but opposite reaction to the action of the centripetal force. The roller coaster shuttle hurtling along the 360 degree vertical loop of the rail, for instance, will manifest centrifugal force by 22 SENIOR Centrifugal force is proportional to the mass of the object it is exerting upon. It can simulate earth’s gravitational force. That is why, in sharp turns and the full vertical loop, the rider feels weighed down and feels his head and arms being drawn towards the floor of the shuttle. Surface Tension T hroughout a liquid, the molecules are attracted to one another. At the surface of the liquid, the forces of attraction lead to an effect called surface tension. The two soap-film tricks shown here demonstrate surface tension action. Procedure Materials liquid soap glass water wire thread The jumping wire 1. Put some liquid soap in a glass and add water to make a strong, soapy solution. 2. Bend a piece of wire to form a rectangular frame and handle, as shown above. The frame should be small enough to fit into the glass. 3. Dip the frame into the solution and then remove it. The frame should now be covered with a soap film. 4. Hold the frame horizontally and place a straight piece of wire across it. 5. Break the soap film on one side of the wire with your finger. Forces of surface tension on the other side will pull on the wire, causing it to jump from the frame. The magic loop 1. Tie a short piece of thread to form a loop. 2. Form a soap film on a wire frame, as previously described. Carefully place the thread on the film. 3. Now break the film inside the loop. Surface tension forces around the loop will put it into a neat circle. SENIOR 23 And the law says THERMODYNAMICS BOX C O N Y C A R N B E A H A E A A X B D R A N K I N E K R R M H I Z E T I R E R K H H A U O I S S O S G P N N G V E N S X C O M B U S T I O N X T D S D H B Y D O W Y G S T S S U E R E A T R A R P N A J C Y D R E N R C U I S O E C P K Y A P L O I D E A L G A S O X M C W A I C S H E U R O Z W L A T L T T T E W P R V Y L E M O C E E C U L K A D I A B A T I C K N E I O R R K L C P R E S P R T V T A X Q O J V B W A O L F H N A N D C F W X K C W D N O E O L X Y P O R T N E G B I H A Look for all the hidden words listed below from the letter box that are related to the study of thermodynamics. C U M E R U T A R E P M E T T CONVECTION ISOBARIC ENTROPY POWER LATENT HEAT PRESSURE RANKINE COMBUSTION ENGINE IDEAL GAS ADIABATIC CARNOT CYCLE TEMPERATURE WORK C R O S S W O R D Across 1 Not bottom 3 Where bees live 4 House 7 Extraterrestrial (abbr.) 9 _ _ _ic_e, small bones in the ear 10 _ _us, presiding Greek god 12 Unit of power 13 Charged particles 14 Refers to ear 17 Oxygen (symbol) 19 _ _ _ _zoic, a geologic era 21 Small opening 22 milli_ _ _ _ , a crawling organism with a thousand “limbs” 24 Po_ _ , to transfer a liquid 25 Not right (direction) 28 Electromagnetic 29 Story 30 Uranium (symbol) 31 Self-fulfilling love 32 Stiff stick 24 1 2 7 7 4 8 3 5 6 9 10 11 16 17 13 12 14 15 18 18 15 16 19 19 21 24 22 25 26 27 SENIOR 23 28 30 29 31 20 32 Down 2 Source of energy which are triggered off by light 3 Airbone vehicle, capable of vertical take off 5 Osmium (symbol) 6 Miss/Mrs (abbr.) 7 Female sheep 8 Tantalum (symbol) 10 Zinc (symbol) 11 _ _ _phagus, food tube 15 Tellurium (symbol) 16 Not out 18 Address of respect to a nun (Sp.) 20 Fermented drink 21 Free from contaminants 23 Electromagnetic unit (abbr.) 26 Indicates early period of time 27 From (abbr.)