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*** Genetics! ***

Posted by Jennifer Landham in Physics - Echols on Monday, April 16, 2012 at 1:35 am

​This blog post will basically touch the simple facts, the history of genetics, etc.

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1886: Gregor Mendel discovered that traits of offspring depend on the parents traits, which may be dominant or recessive. ( but this was somehow lost)

1902: Theodore Boveri & Walter Sutton used color to observe chromosomes 

1905: Nettle Stevens found out that all homologous chromosomes are the same except the ones that determines sex (X,Y)

1909: Thomas H Morgan made many important researches in fly genetics and linked analysis that apply to all diploid organisms

1941: Beadle and Tatum discovered that each gene encodes one protein

1944: Oswald Avery identified DNA as genetic material

1953: Rosalind Franklin and Maurice Wilkins showed that the DNA is a double helix, Thomas Watson and Frances Crick figured out that the base of the double helix enabled replication 

1970: Tamin and Baltimore found a enzyme used to clone genes 

1981: First transgenic mammals are made

1996: Iam Wilmut cloned the lamb Dolly from adult mammary gland tissue  


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Genetics is the features and characteristics that make up an organism. 

 

 Your genetics decipher what you will look like, and your features.

 

There are many things you can learn about your genetics like your DNA and what factors are inside of it to make it important, also your genotype/phenotype, and what a recessive gene and dominant gene is.

 

Lets start simple:

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DNA stands for Deoxyribonucleic acid. Your DNA is a molecule that carries all of your genetic information

 

Genotype describes what certain alleles are on a certain chromosome

 

Alleles are a form of a gene that play part on a specific chromosome, which controls a certain trait.

 

There are dominant and recessive alleles

 

Dominant alleles are upper case and usually the trait that comes out the most

 

Recessive is usually shown with an lower case letter, and in this allele it is usually the trait that does not show unless the organism is homozygous.

 

Homozygous just means that both of the alleles are either dominant or recessive

 

Heterozygous means that one of the alleles are dominant and one is recessive  

 

Phenotype is the physical characteristics of the gene



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There are many ways that you can determine what exactly an offspring’s traits will be by using genotype. One way is to look at the alleles of the two organisms. Also if you really wanted to be accurate you will put them in a punnet square.


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Punnet squares is just a fancy word to describe the separation of alleles to figure out what an offspring may look like, also to fish out the chances of having a certain child.

 

For example a mother and father are about to have a child they want a child with blue eyes. The mother has two alleles bb, which are homozygous. The father also has two alleles Gb, which are heterozygous. Knowing that the father has green eyes, because greens allele is dominant and blue is recessive you can figure out what is the chance of the child having blue eyes.  

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By looking at this you can see that the child has a 50% chance of having green eyes or having blue eyes. But what if the father was also homozygous?

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There would be no chance at the child being born with blue eyes. 


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In the PSSA I do not know exactly what kind of questions will be asked, but make sure you do the study island and also look up a few things to make sure you understand such as:

Where your DNA gets its information from and what it is made up of and how its held together

How many chromosomes a human has (46)

Different types of gene disorders and also different types oh names for each type of gene

What kind of diseases are gene orientated

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http://www.learner.org/interactives/dna/genetics.html
http://www.dnai.org/
http://www.nobelprize.org/educational/medicine/dna/
http://learn.genetics.utah.edu/content/begin/dna/builddna/

http://dnaandrna.com/RNA.html



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Structure & function

Posted by Jamelia Barrett in Physics - Echols on Sunday, April 15, 2012 at 11:09 pm

What is Structure and Function.

 Function and structure are related, because of a certain structure a living thing make contain makes the object function the way it does. The are a lot of structural future in humans, plants, animal and all living things. The relationship of a structure and function is the structuring levels from molecules to organism ensure successful functioning in all living organism and living system. Note one structure can have multiple function.From my under standing structure and function can be broken down in to several part like chemical level which deal with  atoms proton etc as the structure and what they do is the function.

 

 

Classification of Living Things

Living things are placed into groups based on both structural and functional similarities. For example, bacteria are prokaryotic cells, which means they lack a true nucleus. These are structural characteristics. A functional characteristic which defines bacteria is that they reproduce by binary fission. Plant cells are structurally different to other cells because they contain a large central vacuole and plastids such as chloroplasts. These structural features also support a plant’s function, since the presence of chloroplasts allows the plant to carry out photosynthesisExample of a structure and function:

Amino acids structure directly affects its function. It’s a lock and key method that cannot work unless the structure fit together. When they fit they can carry out the function of speeding up a chemical process.

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  • Chemical level – the structure of molecules determines the properties of substances, which, in turn, determine their functions. For example, the chemical structure of metals allows them to conduct electricity, which makes metals useful as conductors

     

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Cellular level – the structure of cells is linked to their function. For example, lung cells are very thin, which allows gases to diffuse easily through the cells. 


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Cellular Processes

There are several types of cellular processes that occur in the cells of living things. 

Photosynthesis is the process where plant cells use sunlight energy to produce glucose and oxygen. The opposite process to this is cellular 
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Meiosis and mitosis are two forms of cell reproduction. In mitosis, a cell produces an exact copy of itself. This is a form of asexual reproduction. It also occurs for other processes, such as hair growth, skin repair, and cell regeneration. In meiosis, a cell is produced that is not an exact copy. Instead, the cell has only half the number of chromosomes as the parent cell.Meiosis is the basis for sexual reproduction, where a cell with a complete set of chromosomes is produced when two gamete cells combine. 


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DNA replication   is a biological process that occurs in all living organisms and copies their DNA; it is the basis for biological inheritance

 

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Practice Question

For this question we know that cellular respiration    
The process of cell in which cells turn food into usable energy in the form of ATP. We know we consume oxygen and then release carbon dioxide. Looking on the option a only part it true .We consume energy, but we don’t absorb energy we use our stored energy. B is no right at all we don’t produce oxygen. C is the correct answer we consume oxygen and release energy. D is like B so it wrong also.

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We know that the nucleus is the the center of the cell.We can use common sense.you can say that since it the center it control the whole cell. Number two say it controls the cell. number three say control also but it not the answer.Three is say some .but the nucleus controls all of the cell.
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​Ok some of you might be wondering what  is a sap vacuole.one Suggestion is you dont know what is  use context clue. Vacuole sounds like vacum and a vacum suck in stuff and stores it .Looking on the choices two  two say control and other say support and stores. if you remember the question before that the nucleus controls the cell.so 3 is out of it. the only one that comes close to the context clue is number 4 .
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Influences on Climate - Prezi

Posted by Siani Widman in Physics - Echols on Sunday, April 15, 2012 at 9:56 pm

By Siani Widman and Loren Jenkins.


*​If the view is hard to see just scroll and it will zoom in

Influences on Climate on Prezi

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Environmental Consequences of Renewable Energy Sources

Posted by Quinn Platzer in Physics - Echols on Sunday, April 15, 2012 at 7:18 pm

Dwindling supply and negative environmental impact is pushing the public to embrace renewable energy sources in exchange of conventional fossil fuels. When burned, coal and oil release tons of carbon dioxide, methane, and other greenhouse gasses into the atmosphere, with the potential to cause catastrophic impacts on the environment. The impending threat of global warming is pressing environmental scientists and engineers to improve the systems we use to gather renewable energy from unlimited natural resources. Each method of generating usable electricity has its own set of environmental problems, but people are always researching ways to improve them. Compared to the environmental consequences of burning fossil fuel to generate electricity, the pros of using renewable energy sources outweigh the cons.


Wind Power:

diagram_wind

Wind is a natural phenomenon that has no foreseeable end. It is a source of unlimited energy, and the turbines used to generate usable power from wind are relatively safe for the environment and produce no greenhouse emissions. The main cons of wind power are the amount of space they use, and their potential impact on local bird populations. Improvements are constantly being applied and are based on the many studies and assessments done to examine the ways the turbines impact the environment around them.


While large amounts of land are required to have a productive wind farm, the space between turbines is not exclusively for the turbines only. The towers can be constructed on leased farmland, where they can sit amongst the crops and animals. Cattle and other farm animals are often seen grazing nearby, resting in their shade, or using them as a scratching post. Farmers can plant crops right up to the base and several studies have shown that crops like corn and soybeans benefit from the decreased frosts and fungus caused by the turbines’ presence. An unexpected benefit is that wind turbines are already combating global warming in their own way. Studies have shown that the turbulence generated by the turning of their blades can keep the surrounding temperatures from getting too hot in the day and too cold in the night. Studies imply that crops planted near the turbines are protected from damaging frost and fungi because of the impact they have on the surrounding temperature. The most extreme issue raised by the use of wind turbines is the impact they have on local bird populations. By doing a population count before construction, during construction, and after construction, scientists are able to gauge whether or not the wind farm produces a negative effect on local populations. There are cases in which rare and endangered bird species have died after flying into the spinning blades. Studies on the common causes of bird death place wind farms towards the bottom of the list, with the worst offenders being the Transmission lines of conventional fossil fuel power plants, hunters, and domestic cats. (graph in Wikipedia of bird casualties)



Hydropower:


hydro-power-plant

Hydropower plants harness the natural energy of flowing water, and produce zero emissions. Any of the negative impact a dam causes on its environment is often magnified by the size of the dam.  New, large-scale dams are rare because the most suitable sites are usually under environmental protection. As a result, the demand for hydropower is failing. The development of new dams is further impacted by frequent protests from environmental activists who seek to preserve the natural flow of the river and the preservation of local fish populations. Fish counts confirm that the spinning blades of the generators can kill unwary fish, and not all fish will think to use the built in fish ladders many power plants install to please activists. Some power plants use flashing lights to direct the fish away from the turbines, but so far, the safest solution seems to be to shut them down during fish migrations. This solution is ineffective for the power plant, and the company looses money during this time. Fish aren’t the only animals that are affected by a hydropower dam. When a new dam is built, the flow may need to be redirected in order to maximize power generation, which can impact wildlife on land and their environment. The dam reserves water upstream, creating a man-made lake that floods the surrounding forest while downriver of the dam; the water level is liable to drop. Case studies of the current impact of established dams provide scientists with the information they need to improve the dams and reduce environmental consequences. 


Solar Energy:


solar-energy-diagram

Solar power cells are growing in popularity, especially in urban areas on roofs above the trees. The main con of solar energy is the hazardous materials used in production of the solar cells, and waste materials left behind, as well as the necessary space required for installation and the large price tag. Large-scale solar energy farms are very expensive, and they take up a lot of space, since they need to have the sun on them at all times. The space in between cells cannot be used for anything, since there isn’t much space left. Because they take up so much space, smaller cells meant for personal use have started appearing in cities and towns. Instead of filling fields, they are being places on the roofs of homes, airport hangers, and other places with space may have otherwise been left vacant. In addition to generating a lot of energy for personal use, a building that generates more energy then they can use are able to earn money by putting that power onto the grid. A problem with small-scale urban solar cells is that they are made of the same hazardous materials as the large-scale cells, and may produce toxic fumes during a fire. These fumes are dangerous for firefighters who may need to enter the building. Current research on experimental solar power aims to reduce hazardous materials and waste in production, as well as to improve the efficiency of the small-scale solar cells. One of the several improvements in progress is a solar concentrator, which is used to generate electricity, and when mounted on solar trackers, can adjust its position to optimize solar energy gathered. Another option being researched is space-based solar power designed to sit on satellites, and have the potential to gather ten times the amount of energy then they would on earth. By installing efficient solar panels in cities, it is possible to generate much of the power needed there daily, and severely reducing the need for coal and oil power plants. 


Sample Question:


What are the potential consequences of using Hydropower?

  1. a. Fish will get caught in the blades of the turbines
  2. b. The river upstream might flood the surrounding woods
  3. c. Concerned local activists may protest
  4. d. All of the above


By reading the passage on hydropower, you can judge what will happen when you build a hydropower dam. That way, you can eliminate any answer that doesn’t make sense, and pick the answer that you think is correct.


Why are scientists trying to improve the design of solar energy cells?

  1. a. Because the sun is patchy, and it’s difficult to gather enough energy
  2. b. Because solar energy cells may release toxic fumes during a house fire
  3. c. Because the materials used during production are expensive and hazardous
  4. d. Because the large energy farms are less efficient then small urban solar cells


Many of these answer might seem like the correct answer, in this case, you would need to look back at the passage and start eliminating answers. If you can’t judge which answer would be the right one, go with the answer that either feels the best, or that seems least wrong.


Sources:

http://www.ucsusa.org/clean_energy/technology_and_impacts/impacts/environmental-impacts-of.html 

http://en.wikipedia.org/wiki/Solar_power#Experimental_solar_power

http://en.wikipedia.org/wiki/Wind_farm#Environmental_and_aesthetic_impact

http://www.businessgreen.com/bg/news/2167515/report-wind-turbines-little-impact-bird-populations

http://en.wikipedia.org/wiki/Environmental_impact_of_wind_power#Impact_on_wildlife

http://www.hydroquebec.com/sustainable-development/documentation/etudes_impacts.html


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Characteristics of the Universe

Posted by Matt Rinaldi in Physics - Echols on Sunday, April 15, 2012 at 5:56 pm

What is the Universe?
The universe is all matter and energy, including the Earth, the galaxies, and the contents of intergalactic space regarded as a whole.

How large is the Universe?
The universe is expansive. To give you sense of the size of the universe, let's compare it to us: human beings.

Here we have everyday people like you and me on the surface of the Earth.

people-at-times-square-downtown-manhattan-nyc-new-york-city-usa-dscn8526

Let's expand a bit and go up to an altitude of 100km. We have now reached space, according to The Federation Aeronautique Internationale, and can see the Earth as a whole.

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Now let's compare the Earth to our whole solar system: containing our many planets and the sun.

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Let's get a bigger picture of where our solar system is located. Our solar system, which is centered around our sun, is but a spec of light in our galaxy: The Milky Way Galaxy.

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Our galaxy is a spiral galaxy, we'll get into that more later on. It consists of hundreds of billions of stars, which are similar to our sun. And each star most likely consists of its own version of a solar system. 

You can see now that we're pretty small in our galaxy, but let's expand one last time so you can really see how small we are. 

lmc

If you venture out an unknown number (but most likely, very large) amount of light-years, we can see that there isn't just one galaxy, but also hundreds of billions of them. Each containing hundreds of billions of stars, that contain their own versions of a solar system, which are bound to consist of masses or planets of many sizes.

The Life of a Star
Now that you have a sense of the scale of the universe, let's get into the main thing that fills up almost every corner of the universe. Let's talk about stars. What is a star? A star is a self-luminous celestial body consisting of a mass of gas held together by its own gravity in which the energy generated by nuclear reactions in the interior is balance by the outflow of energy to the surface, and the inward-directed gravitational forces are balanced by the outward-directed gas and radiation pressures.

Nebula
The life of a star begins in a nebula. Nebulae are the birthplaces of stars. A nebulas is a diffuse of interstellar of dust or gas or both, visible as luminous patches or areas of darkness depending on the way the mass absorbs or reflects incident radiation. Nebulas often consist of Hydrogen an Helium. There are five types of nebulae: 

Emission Nebula: clouds of high temperature gas.

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Reflection Nebula: clouds of dust which are simply reflecting the light of a nearby star or stars.

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Dark Nebula: clouds of dust which are simply blocking the light from whatever is behind.

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Planetary Nebula: shells of gas thrown out by some stars near the end of their lives.

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Supernova Remnant: appears when a massive star ends its life.

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Protostar
Inside a nebula, certain varying regions cause this dust and gas to cluster. As these clusters collect more atoms, which results in an increase of mass, it collects even more atoms in the process. As the materials pull in tighter and contract, it achieves and maintains equilibrium. In this case, equilibrium is the balance between gravity pulling atoms towards the center and gas pressure pushing heat and light away from the center. This cluster is now a Protostar. A circumstellar disk of additional matter surrounds the Protostar. Parts of this disk still spiral inwards towards the center of the Protostar to layer on more mass, while other parts remain in order to form a planetary system. This phase lasts for about 100,000 years. 

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T Tauri Star
The T Tauri phase begins when matter cease to spiral into the Protostar and the star releases an enormous amount of energy. The T Tauri phase lasts for about 100 million years.

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Main Sequence
This is the phase that a star spends most of its life in. Once a star has achieved nuclear fusion, converting protons of hydrogens into atoms of helium, it exudes a tremendous amount of energy into space. Over the span of billions of years, the star slowly contracts in order to compensate for the amount of energy it is releasing. As it slowly contracts, the temperature, density and apressure at its core continue to increase. This contraction due to gravity pulling in and gas pressure pushing out will last throughout the entire life span of the star to maintain equilibrium.

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Red Giant
Since throughout its life a star is constantly converting hydrogen into helium, the hydrogen fuel runs out while the helium builds up. When a star depletes its fuel of hydrogen, its internal reactions cease. Without this gas pressure, the star begins to contract inward due to gravitational forces. In order to still maintain equilibrium between gravity and gas pressure, the star must re-ignite fusion by increasing temperatures in its core. To maintain stability, the star is forced to burn up its supply of helium. Helium burns inside the core, but a hydrogen reaction occurs faster in the shell of around the core. As the temperature of the shell increases, the outer layer of the star expands. At this stage, the star is larger, but less stable due to fusion releasing more energy during helium burning than the main sequence phase.

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White Dwarf
The Red Giant will eventually burn up its helium fuel supply. In order to maintain equilibrium, the star will contract again to commence the last type of fusion: carbon burning. To contract, the star must expel its outer layers into space. The Red Giant has now become a White Dwarf. A White Dwarf will start out hot, but over time (hundreds of billions of years), it will gradually cool down.

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Supernova
A Supernova can be divided into two basic physical types:
Type Ia.: These result from some binary star systems in which a carbon-oxygen white dwarf is accreting matter from a companion.
Type II.: These occur at the end of a star's lifetime, when its nuclear fuel and is depleted and it is no longer supported by the release of nuclear energy. If the star's iron core is massive enough, it will collapse and become a supernova.

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Neutron Star
Neutron stars are created in the cores of massive stars during a supernova explosion. When the core of the sar collapses, portons are crushed together with a corresponding electron, which transforms every electron-proton pair into a neutron. In this case however, the neutrons remain to form a neutron star.

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Black Holes
Black holes are believed to be formed when a massive star collapses in on itself. When a supernova occurs, a neutron star is able to form due to neutron degeneracy. But if the degenerating neutrons are not able to prevent the collapse of the star because of gravitational forces, it contracts and compresses into an infinite void of blackness- also known ans a stellar mass black hole. The gravitational pull from a black hole is so strong that nothing can escape them, including light. Their density is immeasurable. Black holes are able to distort space around them and even absorb neighboring matter, including stars.

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The Telescope
How do we know so much about stars you ask? Well, you can thank Hans Lippershey for that. Thanks to him, we have now been able to modify and improve his integral invention: the telescope, in order to conduct our study of astronomy and the universe. Lippershey's patent for the invention of the telescope is credited as the earliest, on September 25, 1608. Most people credit Galileo Galilei for its invention, though this is inaccurate. Galileo was the first to use a telescope for the purposes of astronomy in 1609, not invent it. 

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The Hertzsprung-Russel Diagram

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This diagram was created by Danish astronomer, Ejnar Hertzsprung and American astronomer, Henry Norris Russell in 1919. The Hertzsprung-Russell Diagram helped create a classification system for discovered stars. This diagrams has become an important tool in stellar astronomy. 

Each dot represents a star. The diagram is a plot of stars' luminosity (absolute magnitude) and its temperature. The color of the stars range from the high-temperature, blue-white stars on the left side of the diagram, to the low-temperature, red stars on the right side. The Y-axis represents the star's luminosity or absolute magnitude. Luminosity is basically the amount of energy a star radiates in one second or how bright it is. In either case, the scale is a ratio scale in which stars are compared to each other based on the reference of our star, the sun. On the other hand, the X-axis represents the surface temperature of a star. Going to the left side of the x-axis means that the stars are hotter, while going to right of the axis means that the stars are cooler. The X-axis is usually represented in either Kelvins or Colour (B-V).

Sample Question
1. What process has to occur in order for a star to achieve/maintain equilibrium?

                                a. contraction
                                b. nuclear fusion
                                c. supernova
                                d. accretion

Firstly, eliminate answers that are wrong. For example, a. is contraction. The meaning of equilibrium is balance. Contraction is only one side of it. And if you did your reading, there has to be another process that takes place to counter contraction and achieve equilibrium. So a. can't be the answer. Let's eliminate another answer. It's a safe bet that you can take out c. supernova. This due to the fact that supernova is the phase in which a star dies. How can a star achieve/maintain anything if it dies? So let's cross that off. Now you have two answers, leaving you with a 50/50 chance. If you knew the definition of accretion, you can take it right off and be left with the right answer. But if you didn't, then look at the other answer b. nuclear fusion. Like I mentioned before: if equilibrium means balanced and the word fusion means combine, then you can add one and one together and get the answer. For equilibrium to happen, there needs to be two things happening. The word fusion means combine, which implies there are two things occurring. By using the elimination method, you were able to figure out the correct answer.

Sources
http://thefreedictionary.com/universe
http://www.universetoday.com/25410/how-far-is-space/ 
http://www.thefreedictionary.com/nebula 
http://www.telescope.org/pparc/res8.html
http://aspire.cosmic-ray.org/labs/star_life/starlife_proto.html 
http://www.thefreedictionary.com/star 
http://www.universetoday.com/24629/life-cycle-of-stars/ 
http://www.sciencedaily.com/releases/2010/01/100113131454.htm 
http://imagine.gsfc.nasa.gov/docs/science/know_l2/supernovae.html
http://www.atlasoftheuniverse.com/hr.html 
http://aspire.cosmic-ray.org/labs/star_life/hr_diagram.html 
http://imagine.gsfc.nasa.gov/docs/science/know_l1/neutron_stars.html
http://www.universetoday.com/33454/how-do-black-holes-form/ 
http://www.universetoday.com/41889/who-invented-the-telescope/ 
http://burro.astr.cwru.edu/stu/stars_hrdiagram.html 

Images
http://blog.petaflop.de/2008/02/ 
http://thewordzombie.com/2010/07/19/review-the-great-global-warming-blunder-by-roy-w-spencer/earth-from-space-clouds/#.T4oAq5pSQdU 
http://aaarf.net/planets-solarsystem.htm 
http://www.windows2universe.org/the_universe/Milkyway.html
http://ircamera.as.arizona.edu/NatSci102/NatSci102/lectures/galaxytypes.htm
http://www.atlasoftheuniverse.com/hr.html
http://aspire.cosmic-ray.org/labs/star_life/hr_diagram.html 
http://apod.nasa.gov/apod/ap060213.html 
http://www.universetoday.com/83338/stunning-new-look-at-reflection-nebula
messier-78/ 
http://www.werbeagentur.org/oldwexi/gal_dsk_neb.html 
http://phys.org/news131721414.html 
http://www.nasa.gov/multimedia/imagegallery/image_feature_342.html
http://en.wikipedia.org/wiki/Protostar 
http://apod.nasa.gov/apod/ap090803.html 
http://www.mpia.de/MCs_MPIA/mc_programs.html 
http://www.astronomy-blog.com/blogs/permalinks/3-2011/a-look-inside-red
giant-stars.html 
http://www.universetoday.com/44836/unusual-massive-white-dwarf-stars-have
oxygen-atmospheres/ 
http://wind.caspercollege.edu/~marquard/astronomy/highmass.htm 
http://imagine.gsfc.nasa.gov/docs/science/know_l1/neutron_stars.html
http://news.nationalgeographic.com/news/2010/04/100409-black-holes-alternate-universe-multiverse-einstein-wormholes/ 
http://www.progressivenewsdaily.com/?p=25415 
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Energy Transfer

Posted by Heather Campbell in Physics - Echols on Sunday, April 15, 2012 at 2:08 pm

Energy Transfer

Energy Transfer on Prezi

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Behavior of Gasses

Posted by Callie Monroe in Physics - Echols on Sunday, April 15, 2012 at 12:40 am

Introduction:

- The behavior of gasses is a very broad and vast topic that covers a multitude of sub topics. Under this subject, the state of Pennsylvania has picked three main ideas that they require students to know. These three things are Boyle's law, Charle's law, and the ideal gas law. This blog post has an explanation of the three, a bit about their history, and how they will be used in the PSSA testing. 

Boyle's Law:

- Boyle's law explains the relationship between the volume of a gas and its pressure. It states that as the pressure of a gas increases the volume decreases and in the same manner that as the volume of a gas increases the pressure decreases (assuming that the temperature of the gas is constant). This relationship can be expressed as PV=k, where "p" represents the pressure of the system, "v" represents the volume of the gas, and "k" represents a constant. Robert Boyle, a chemist and physicist, discovered this in the mid 1600's and published his findings in 1662. Boyle executed a series of experiments consisting of confining a fixed amount of gas into a curved glass. He then added different amounts of mercury to the gas sample in order to change its pressure. These findings were then related to this equation: P1V1 = P2V2, which expresses "the before and after volumes and pressures of a fixed amount of gas" (wikipedia). **Note** This equation is the one that will be used on the PSSA test. 

boyle
chfa_02_img0350

On the PSSA this type of material could be expressed in a question asking for one to solve for one of the variables in the equation. For example, a question could state the starting volume and pressure as well as the final amount of pressure and ask for you to solve for the final volume. Ex:

 1. If the pressure of an ideal gas is changed from 145 atm to 290 atm, what is the gasses change in volume, assuming the original volume was 75.0mL?
a. 150 mL
b. 37.5 mL
c.72.5
d. Not enough information is given

A link to the answers is provided later.

Here is a link to an animation of this: http://www.grc.nasa.gov/WWW/k-12/airplane/boyle.html

Charle's Law 
- Charle's law explains the relationship between the temperature of a gas and its volume. It states that as the temperature of a gas increases the volume of that gas will as well (assuming that the pressure of the gas remains constant). Another thing to note is that they do this proportionately meaning that they increase and decrease at the same scale factor. This relationship was found in a similar manner that Boyle's law was found in. Jacques Charles was the scientist that made this discovery and he did so by confining a gas in a curved class tube and changing its temperature while keeping its pressure constant. The relationship that he discovered can be expressed as V1/T1 = V2/T2 where "V" represents the volume of the gas and "T" represents the temperature of the gas. **Note** This equation is the one that will be used on the PSSA test. 

glussac

charles's-law
On the PSSA this type of material could be expressed in a question asking for one to solve for one of the variables in the equation. For example, a question could state the starting volume and temperature as well as the final temperature and ask for you to solve for the final volume. Ex:

2. Bob wants to find the volume of a gas in a cylinder. He knows that at a temperature of 30˚C the gas had a volume of 6.0 L. The temperature of the gas is now 35˚C. What is the volume of the gas now? **Note you must convert the temperature from Celsius to Kelvin by adding 273 to the Celsius measure**
a. 7.0 L
b. 175 L 
c. 6.09 L 
d. 15 L
A link to the answers is provided later.

Here is a link to an animation of this: http://www.grc.nasa.gov/WWW/k-12/airplane/glussac.html

Ideal Gas Equation
- The ideal gas equation is a combination of Boyle's law, Charles's law and Avogadro's law. This law can be an approximation of the state and behavior of a gas. The ideal gas law was not discovered and no experiments were directly done to find out this law, but the relationships expressed within this law are a compilation of three laws. This relationship can be expressed through the following equation: PV = nRT equation where "P" represents the pressure of the gas, "V" represents the volume of the gas, "n" represents the number of moles of gas, "R" represents the ideal gas constant, and "T" represents the temperature of the gas. The ideal gas constant is approximately 8.3145 J and can be used to plug into this equation. Another thing to not is that if any two of the variables in the equation are kept constant, the relationship between the other two can be observed.  

eqstat

ideal_gas

On the PSSA this type of material could be expressed in a question asking for one to solve for one of the variables in the equation. Ex. 

3. A gas exerts a pressure of .0892 atm in a 5.0 L container at 15˚C. What is the molecular mass of the gas?
a. 0.191 mol
b.  5 mol
c. 0.56 mol
d. 19 mol

Link to answers:
https://docs.google.com/document/d/1R5SF7QKNLUxS0rOfAdHVabXKqcGsOg7hAcP9tn1n9Pw/edit


Sources:

http://www.shodor.org/unchem/advanced/gas/

http://hyperphysics.phy-astr.gsu.edu/hbase/kinetic/idegas.html

http://en.wikipedia.org/wiki/Ideal_gas_law

http://www.metric-conversions.org/temperature/celsius-to-kelvin.htm

http://www.chm.davidson.edu/vce/gaslaws/charleslaw.html

http://www.chm.davidson.edu/vce/gaslaws/boyleslaw.html

http://en.wikipedia.org/wiki/Boyle's_law

http://www.grc.nasa.gov/WWW/k-12/airplane/eqstat.html

http://www.grc.nasa.gov/WWW/k-12/airplane/glussac.html

http://www.grc.nasa.gov/WWW/k-12/airplane/boyle.html
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Theory of Evolution - Aja and Jésus

Posted by Jesus Jimenez in Physics - Echols on Saturday, April 14, 2012 at 7:16 pm

Something things that have been tested or experimented happened with Darwin and his exploration. He began this world known theory when he started to explore how different genes work and the processes in which they create new life forms.

One popular experiment/observation was Darwin’s Finches. New species of finches in the Galapagos Islands sprung around area, with different beaks and characteristics. He was intrigued by this discovery and only aided to develop the modern theory of evolution. What made the finches so interesting was that they basically evolved to depending on what food they need in a certain area. From bugs, to leaves, to seeds, these were the foods different finches ate. And believe it or not, they each needed different beaks for them.

l_016_02_l
l_016_02_l
FinchTypes
FinchTypes

The Earth is approximately 4.6 billion years old and humans appeared within the last-2 million years. Microorganisms appeared first - 3.4 million years ago. The plants of the land appeared about 400 million years ago and it was about 225 million years ago when mammals and dinosaurs walked the earth. Which evolves into the topic of Natural selection which acts upon the mutation that are inherited from one generation to the next. Out of all the type of  genes there are only the genes in the sperm cell will get passed on to the future generations. Thus causing any potential alter to the configuration of any population. Enabling us to keep track of how things change over time, which is what we call Evolution.


Sample Questions


1. In what ways would an animal that eats earthworms with its beak evolve to eat berries off a tree?
a. It’s beak would get smaller for more precise grabbing.
b. They will change color to resemble a tree.
c. Their claws will be able to cling on trees.
d. Nothing will change.

2. An animal that lived in water and adapted to live on land, would most likely be a:
a. amphibian
b. invertebrate  
c. Cold - blooded
d. Reptiles

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Chemical reactions

Posted by Toni Marshall in Physics - Echols on Thursday, April 12, 2012 at 2:28 pm

​ By: Toni and Taahir

There are six chemical reactions.

Combustion is when oxygen combines with another compound to create water and carbon dioxide, this reaction is considered to be exothermic which simply means that this reaction creates heat.

combustion-safety-carbon-monoxide-bpi-single-point-test

Synthesis this reaction is when two or more simple compounds come together in order to create a complicated compound.

synthesis

Decomposition is the complete opposite of synthesis, this occurs when a molecule that is complex breaks down into simpler molecules.

decomposition

Single displacement is when one element trades places with another element while in a compound.

singlereplacement

Double displacement is when the anions and cations of two different molecules switch places, which then turns into two complete different compounds.

doubledisplacement

Acid-Base is a certain kind of double displacement reaction that happens when a acid and base react with one another. The H+ion in the acid reacts with the OH ion in the base.

acid-base-chemistry-3284

Some experiments that have been conducted by us are mixing potassium promaginite and glycerin that causes an exothermic reaction. Based on the six different types of Chemical reactions which type of chemical reaction does this experiment give?

7

Another experiment example: Sodium and water in chlorine gas which produces a lot of heat but it also turns into sodium chloride which is just common salt. What reaction does it give?

SodiumChlorineReaction

A third example is when Helium is cooled to -271 degrees Celsius. It is called lambda point. Once it hits this point it is considered helium II or helium superfluid.

What reaction is this?

 

helium-3 

Try to balance equations here and testing reactions here: http://phet.colorado.edu/en/simulation/reactants-products-and-leftovers

Resources:

http://edtech2.boisestate.edu/halej/573/jigsaw2.html

 http://antoine.frostburg.edu/chem/senese/101/thermo/faq/exothermic-endothermic-examples.shtml

Things that affect Reaction are


AGITATION:  Anything that cause particles to move, shaking and stirring are actions that result in  the movement of particles. This leads to more collisions, and a higher reaction rate.


CATALYST: Is something that helps initiate a reaction, but isn't considered a reactant or a product. It increases the rate at which chemical reactions can occur. The catalyst is not depleted during the reaction. 


CONCENTRATION:

When there are more particles in a given volume, the amount of times these particles will collide is greater when the are less particles. The more  particles/less space per volume, the faster the reaction will occur.


PRESSURE: The higher the pressure there is on a container, the lower the volume will be (less space, which leads to more collision and more often), which will also increase the speed of the reaction.




SURFACE AREA:  The amount of particles found on the surface of that are open to collision.  Larger objects have surfaces with particles that are less exposed, which means fewer collisions.  Objects that are smaller have more particles in contact with a surface, which would allow for more collisions to occur.  Chemical reactions occur at a higher rate when their reactants cover more surface area.





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PHYS-005

Term
2011-12

Teacher

  • Rosalind Echols
Science Leadership Academy @ Center City · Location: 1482 Green St · Shipping: 550 N. Broad St Suite 202 · Philadelphia, PA 19130 · (215) 400-7830 (phone)
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