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Reading Practice Answers

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Course 2013:

Are Mobile Phones Dangerous?

  1. It is not clear at all. Some studies support this theory, while others completely contradict it. Therefore, the article is not entirely clear on the matter.
  2. No, they are not the only dangerous devices. Other wireless devices such as laptops, cordless phones, or gaming consoles can also be dangerous for our health.
  3. Because mobile phones emit Electromagnetic Radiation, which can be dangerous for children whose brains are not yet fully developed.
  4. FALSE. (lines 4-5): "Mobile phone...in radio frequency"
  5. TRUE. (lines 13-14): "Many years ago,...on their health"
  • 6. Concern
  • 7. Healthy
  • 8. Scare
  • 9. Device
  • 10. What do some health professionals point out?
  • 11. In spite of being very expensive, she bought the car.
  • 12. Smoking
  • 13.
... Continue reading "Reading Practice Answers" »

Discovering Extrasolar Planets: Methods and Significance

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Extrasolar Planets

An extrasolar planet is a planet orbiting a star other than our Sun. There are two general ways of learning about a distant object: directly, which means by obtaining images or spectra of the object, and indirectly, which means by inferring the object’s existence or properties without actually seeing it. There are two major indirect approaches to finding and studying extrasolar planets:

  1. Observing the motion of a star to detect the subtle gravitational tugs
  2. Observing changes to a star’s brightness that occur when one of its planets passes in front of the star as viewed from Earth.

Planets exert gravitational tugs on their star, causing the star to orbit around the system center of mass. Gravitational tugs: we can detect a... Continue reading "Discovering Extrasolar Planets: Methods and Significance" »

Stellar Energy Generation and Star Classification

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The Proton-Proton Chain: Powering Low-Mass Stars

The proton-proton chain is the series of nuclear reactions by which low-mass stars, including our Sun, fuse hydrogen into helium. This process is crucial for stellar energy generation.

Gravitational equilibrium and energy balance work together as a natural thermostat, maintaining the Sun’s core temperature and fusion rate at a steady level.

Unraveling the Sun's Energy Source

Early scientific theories proposed that the Sun's energy came from chemical reactions or gravitational collapse. However, these theories were disproven:

  • Chemical burning: Ruled out because it cannot account for the Sun’s immense luminosity.
  • Gravitational collapse: The conversion of gravitational potential energy into heat as
... Continue reading "Stellar Energy Generation and Star Classification" »

I choose to live

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Introduction


"The Breedlove´s did not live in a storefront because they were having temporary difficulties adjusting to the cutbacks at the plant. They lived there because they were poor and black, and they stayed there because they believed they were ugly" (The Bluest Eye, Toni Morrison, page 38).

Toni Morrison has portrayed in a very special way an specific social group all allong the novel (as you saw on the quote), this specific group is very related to Morrison, That´s why many other writers admire Morrison, by her hability to describe the background on her novels.

The social group/class described in the novel is the african american middle-low class which is represented by the main character family.
Morrison is able to write about this
... Continue reading "I choose to live" »

Stellar Endpoints: Supernovae, Neutron Stars, and Black Holes

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White Dwarf Stellar Explosions

Novae: Recurrent Stellar Flares

The hydrogen build-up on the surface of a white dwarf can ignite into an explosive fusion reaction that blows off a shell of gas. Because so little mass is blown off during a nova, the explosion does not disrupt the binary system. Ignition of the infalling hydrogen can recur again with periods ranging from months to thousands of years.

White Dwarf Supernovae (Type Ia)

Subrahmanyan Chandrasekhar predicted that gravity will overcome the pressure of electron degeneracy if a white dwarf has a mass > 1.4 M¤. Energetic electrons, which cause this pressure, reach the speed of light. If accretion brings the mass of a white dwarf above the Chandrasekhar limit, electron degeneracy can no... Continue reading "Stellar Endpoints: Supernovae, Neutron Stars, and Black Holes" »

Fundamental Concepts in Thermodynamics and Gas Behavior

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Shock Waves: Formation and Mach Cone Angle

If the speed of a source relative to the medium exceeds the speed of sound in the medium, the Doppler equation no longer applies. In such a case, shock waves result. The half-angle of the Mach cone is given by:

Temperature Measurement and Thermometers

Temperature is an SI base quantity related to our sense of hot and cold. It is measured with a thermometer, which contains a working substance with a measurable property, such as length or pressure, that changes in a regular way as the substance becomes hotter or colder.

Zeroth Law of Thermodynamics: Thermal Equilibrium

When a thermometer and some other object are placed in contact with each other, they eventually reach thermal equilibrium. The reading of... Continue reading "Fundamental Concepts in Thermodynamics and Gas Behavior" »

During a climb, if the total pressure head is rapidly clogged up by ice, the sensed total pressure remains constant and:

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Write your text here!Bernoulli's theorem, in fluid dynamics, relation among the pressure, velocity, and elevation in a moving fluid (liquid or gas), the compressibility and viscosity (internal friction) of which are negligible and the flow of which is steady, or laminar.


he principle of work and kinetic energy (also known as the work-energy theorem) states that the work done by the sum of all forces acting on a particle equals the change in the kinetic energy of the particle.

The law of conservation of momentum states that for two objects colliding in an isolated system, the total momentum before and after the collision is equal. This is because the momentum lost by one object is equal to the momentum gained by the other.

 the law
... Continue reading "During a climb, if the total pressure head is rapidly clogged up by ice, the sensed total pressure remains constant and:" »

Quantum Phenomena Explained

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Photons and Electrons in the Double Slit Experiment

Evidence for Wave-Particle Duality

  • A single electron or photon leaves the source with particle-like discreteness and creates a single discrete spot on the screen.
  • The interference pattern, which occurs over time, is a wave property.

Diffraction Pattern and Heisenberg’s Uncertainty Principle

  • We cannot measure the exact position of each electron or its exact momentum as it approaches the slit; there is uncertainty in both position and momentum.
  • The uncertainty in each electron’s y-position is reduced to the width of the slit (since we are certain it passes through the slit). This increases its uncertainty in the momentum of the y-direction.
  • The uncertainty in the momentum in the y-direction means
... Continue reading "Quantum Phenomena Explained" »

Understanding Electrostatics: Charge, Fields, and Lightning

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Understanding Electrostatics

Electrostatics is the branch of physics that studies the phenomena produced by charges that do not vary or move.

History of Electrostatics

6th century BC: The Greeks discovered the electrical properties of amber. When rubbed, it could attract light objects.

18th century: Benjamin Franklin conducted experiments with different materials and observed that rubbed materials could either attract or repel each other.

Franklin's Theory of Electricity

  • There are only two types of electricity: positive and negative.
  • Electricity is a sort of fluid present in all objects and it can flow from one object to another by rubbing them.
  • When there's an excess of electricity, objects have positive electricity, and when there's a lack of electricity,
... Continue reading "Understanding Electrostatics: Charge, Fields, and Lightning" »

Evolution of Soccer Balls: From Superball to Jabulani

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Good morning today we are going to present the evolution of soccer balls.


Superball

The superball was a soccer ball that consisted of a chamber composed of a valve that prevented the air from coming out and a seam from outside to inside that was invisible and without a flange. This ball was the first ball made without tiento


Invention of the Invisible Tiento

In Bell Ville, in the Argentine province of Córdoba between 1929 and 1931 Romano Polo, Antonio Tossolini and Juan Valbonessi conducted numerous tests and trials that culminated in the invention of the ball with an invisible tiento, a ball that continued to be used for a couple of years.


Professional Use and Commemoration

The superball was first used professionally in the same year of its invention... Continue reading "Evolution of Soccer Balls: From Superball to Jabulani" »