This document discusses celebrities speaking out about their experiences with bullying. Several celebrities like Taylor Swift, Beyonce, Zac Efron, Angelina Jolie, Corey Monteith, Tyra Banks, Eminem, Demi Lovato, Jackie Chan, Zooey Deschanel, Chris Rock, Kelly Clarkson, Ashton Kutcher, Jessica Simpson, Tom Cruise, Lady Gaga discuss being bullied for things like their interests, appearance, or for being new students. They faced bullying like being made fun of, beat up, excluded from groups. Some anti-bullying laws from different states are also mentioned.
Faults and Folds Geology Visual Quiz, Earth Science PowerPoint with Answerswww.sciencepowerpoint.com
This PowerPoint is one small part of the Geology Topics unit from www.sciencepowerpoint.com. This unit consists of a five part 6000+ slide PowerPoint roadmap, 14 page bundled homework package, modified homework, detailed answer keys, 12 pages of unit notes for students who may require assistance, follow along worksheets, and many review games. The homework and lesson notes chronologically follow the PowerPoint slideshow. The answer keys and unit notes are great for support professionals. The activities and discussion questions in the slideshow are meaningful. The PowerPoint includes built-in instructions, visuals, and review questions. Also included are critical class notes (color coded red), project ideas, video links, and review games. This unit also includes four PowerPoint review games (110+ slides each with Answers), 38+ video links, lab handouts, activity sheets, rubrics, materials list, templates, guides, 6 PowerPoint review Game, and much more. Also included is a 190 slide first day of school PowerPoint presentation.
Areas of Focus within The Geology Topics Unit: -Plate Tectonics, Evidence for Plate Tectonics, Pangea, Energy Waves, Layers of the Earth, Heat Transfer, Types of Crust, Plate Boundaries, Hot Spots, Volcanoes, Positives and Negatives of Volcanoes, Types of Volcanoes, Parts of a Volcano, Magma, Types of Lava, Viscosity, Earthquakes, Faults, Folds, Seismograph, Richter Scale, Seismograph, Tsunami's, Rocks, Minerals, Crystals, Uses of Minerals, Types of Crystals, Physical Properties of Minerals, Rock Cycle, Common Igneous Rocks, Common Sedimentary Rocks, Common Metamorphic Rocks.
This unit aligns with the Next Generation Science Standards and with Common Core Standards for ELA and Literacy for Science and Technical Subjects. See preview for more information
If you have any questions please feel free to contact me. Thanks again and best wishes. Sincerely, Ryan Murphy M.Ed www.sciencepowerpoint@gmail.com
The document discusses the classification of stars based on size, temperature, brightness, and lifespan. It describes how stars are born from nebulae and how their lifespan and death depends on their mass. Smaller stars have less violent deaths, becoming white dwarfs, while larger stars die in supernova explosions, potentially leaving behind neutron stars or black holes. It also provides an overview of the different types of galaxies including spiral, elliptical, and irregular galaxies.
Stars are born from clouds of gas and dust called nebulas. As the gas spins faster under gravity, it heats up and forms a protostar. Nuclear fusion then occurs, turning the protostar into a main sequence star that shines for millions of years by fusing hydrogen into helium. Eventually the hydrogen runs out, causing the star to expand into a red giant. From there, less massive stars will blow off their outer layers and collapse into white dwarfs, while more massive stars will explode in supernovas and collapse into neutron stars or black holes.
Stars are born from clouds of gas and dust called nebulae. Over billions of years, stars progress through various stages as they age. Lower mass stars begin as protostars and become main sequence stars fueled by nuclear fusion. As their hydrogen runs out, they become red giants and eventually white dwarfs. Higher mass stars explode as supernovae at the end of their lives, leaving behind neutron stars or black holes.
Stars are born from contracting nebulae of gas and dust. They spend most of their lives on the main sequence, fusing hydrogen into helium in their cores. Eventually they run out of fuel in their cores and their outer layers expand, forming red giants or supergiants. From there, smaller stars shed their outer layers to form planetary nebulae and white dwarfs, while larger stars explode as supernovae, leaving behind neutron stars or black holes.
Weathering breaks down rocks and minerals near Earth's surface through mechanical and chemical processes. Mechanical weathering causes physical breakdown without composition change through frost wedging, thermal expansion/contraction, and abrasion by various agents. Chemical weathering alters mineral composition through dissolving, oxidation, and hydrolysis. Erosion transports weathered materials by water, wind, ice, and gravity, depositing sediments that form layers over time.
All stars begin as clouds of dust and gas called nebulae. When gravity causes the nebula to collapse, a protostar forms at the center. The protostar grows in size and temperature through nuclear fusion reactions until it becomes a stable main sequence star. Small stars like our Sun will eventually expand into red giants and shed their outer layers, leaving behind dense white dwarf cores. Larger stars may explode as supernovae, collapsing into neutron stars or black holes. The life cycle of a star depends on its initial mass, with smaller stars ending as white dwarfs and more massive stars ending as black holes or neutron stars.
Faults and Folds Geology Visual Quiz, Earth Science PowerPoint with Answerswww.sciencepowerpoint.com
This PowerPoint is one small part of the Geology Topics unit from www.sciencepowerpoint.com. This unit consists of a five part 6000+ slide PowerPoint roadmap, 14 page bundled homework package, modified homework, detailed answer keys, 12 pages of unit notes for students who may require assistance, follow along worksheets, and many review games. The homework and lesson notes chronologically follow the PowerPoint slideshow. The answer keys and unit notes are great for support professionals. The activities and discussion questions in the slideshow are meaningful. The PowerPoint includes built-in instructions, visuals, and review questions. Also included are critical class notes (color coded red), project ideas, video links, and review games. This unit also includes four PowerPoint review games (110+ slides each with Answers), 38+ video links, lab handouts, activity sheets, rubrics, materials list, templates, guides, 6 PowerPoint review Game, and much more. Also included is a 190 slide first day of school PowerPoint presentation.
Areas of Focus within The Geology Topics Unit: -Plate Tectonics, Evidence for Plate Tectonics, Pangea, Energy Waves, Layers of the Earth, Heat Transfer, Types of Crust, Plate Boundaries, Hot Spots, Volcanoes, Positives and Negatives of Volcanoes, Types of Volcanoes, Parts of a Volcano, Magma, Types of Lava, Viscosity, Earthquakes, Faults, Folds, Seismograph, Richter Scale, Seismograph, Tsunami's, Rocks, Minerals, Crystals, Uses of Minerals, Types of Crystals, Physical Properties of Minerals, Rock Cycle, Common Igneous Rocks, Common Sedimentary Rocks, Common Metamorphic Rocks.
This unit aligns with the Next Generation Science Standards and with Common Core Standards for ELA and Literacy for Science and Technical Subjects. See preview for more information
If you have any questions please feel free to contact me. Thanks again and best wishes. Sincerely, Ryan Murphy M.Ed www.sciencepowerpoint@gmail.com
The document discusses the classification of stars based on size, temperature, brightness, and lifespan. It describes how stars are born from nebulae and how their lifespan and death depends on their mass. Smaller stars have less violent deaths, becoming white dwarfs, while larger stars die in supernova explosions, potentially leaving behind neutron stars or black holes. It also provides an overview of the different types of galaxies including spiral, elliptical, and irregular galaxies.
Stars are born from clouds of gas and dust called nebulas. As the gas spins faster under gravity, it heats up and forms a protostar. Nuclear fusion then occurs, turning the protostar into a main sequence star that shines for millions of years by fusing hydrogen into helium. Eventually the hydrogen runs out, causing the star to expand into a red giant. From there, less massive stars will blow off their outer layers and collapse into white dwarfs, while more massive stars will explode in supernovas and collapse into neutron stars or black holes.
Stars are born from clouds of gas and dust called nebulae. Over billions of years, stars progress through various stages as they age. Lower mass stars begin as protostars and become main sequence stars fueled by nuclear fusion. As their hydrogen runs out, they become red giants and eventually white dwarfs. Higher mass stars explode as supernovae at the end of their lives, leaving behind neutron stars or black holes.
Stars are born from contracting nebulae of gas and dust. They spend most of their lives on the main sequence, fusing hydrogen into helium in their cores. Eventually they run out of fuel in their cores and their outer layers expand, forming red giants or supergiants. From there, smaller stars shed their outer layers to form planetary nebulae and white dwarfs, while larger stars explode as supernovae, leaving behind neutron stars or black holes.
Weathering breaks down rocks and minerals near Earth's surface through mechanical and chemical processes. Mechanical weathering causes physical breakdown without composition change through frost wedging, thermal expansion/contraction, and abrasion by various agents. Chemical weathering alters mineral composition through dissolving, oxidation, and hydrolysis. Erosion transports weathered materials by water, wind, ice, and gravity, depositing sediments that form layers over time.
All stars begin as clouds of dust and gas called nebulae. When gravity causes the nebula to collapse, a protostar forms at the center. The protostar grows in size and temperature through nuclear fusion reactions until it becomes a stable main sequence star. Small stars like our Sun will eventually expand into red giants and shed their outer layers, leaving behind dense white dwarf cores. Larger stars may explode as supernovae, collapsing into neutron stars or black holes. The life cycle of a star depends on its initial mass, with smaller stars ending as white dwarfs and more massive stars ending as black holes or neutron stars.
This document discusses the life cycle of stars from their formation to their death. It begins by explaining that stars are giant balls of exploding gas made up mainly of hydrogen and helium. The document then outlines the various stages of a star's life: nebula, protostar, main sequence star, red giant, white dwarf, supernova, neutron star, and black hole. For each stage, it provides a brief description of the physical changes occurring within the star. The document emphasizes that stars much more massive than our sun will end their lives as neutron stars or black holes through the supernova process.
1) The document discusses the possibility of life existing elsewhere in the universe, beyond Earth. It explores potential habitats on planets and moons in our solar system as well as exoplanets orbiting other stars.
2) Estimates suggest there could be over 10,000 civilizations in our galaxy alone, and many planets and moons in our solar system - such as Mars, Europa, Titan, and Enceladus - show signs of being able to support some form of life.
3) Scientists are discovering hundreds of new exoplanets each month, increasing the chances of finding a planet capable of supporting life outside our solar system, such as the exoplanet Gliese 581 c.
The life cycle of stars depends on their mass. Lower mass stars like our Sun will eventually become red giants then white dwarfs. Higher mass stars live shorter lives and end as supernovas, leaving behind neutron stars or black holes. All stars begin as nebulae of dust and gas that collapse under gravity into protostars and main sequence stars fueled by nuclear fusion.
The key factors that determine whether a planet can support life include being located within the circumstellar habitable zone (Goldilocks zone) around its star where liquid water can exist on the surface, having a planetary size that allows for an atmosphere to develop and be retained, and orbiting a stable star that provides a constant radiation level like our middle-aged G-type Sun. Other considerations include the planet having a chemistry that supports liquid water through a greenhouse gas atmosphere, and being located within the optimal area of its galaxy to avoid threats from supernovae while still forming necessary heavier elements.
Stars are giant balls of gas that produce light and heat through nuclear fusion at their cores. They vary greatly in size, from dwarf stars like our Sun to massive supergiant stars over 200 times the Sun's diameter. Stars end their lives in different ways depending on their mass - smaller stars become white dwarfs, while larger stars explode as supernovae or collapse into neutron stars and other compact objects.
The Sun is a middle-aged, average sized yellow star that is made up mostly of hydrogen and helium. It is about 4.6 billion years old and located 93 million miles from Earth. The Sun generates heat and light through nuclear fusion reactions in its core that convert hydrogen into helium. It is the center of our Solar System and contains over 99% of the mass in the entire system. The Solar System also includes eight official planets that orbit the Sun, along with dwarf planets, moons, asteroids, comets, and other small bodies.
Glaciers are large, slow-moving masses of ice that form from compacted snow. They are found in mountain ranges and polar regions. Glaciers are sensitive to climate conditions and influence sea levels and water resources. They are categorized based on their thermal characteristics, behavior, and location. Alpine glaciers are confined to valleys while continental glaciers span entire regions. As glaciers accumulate more snow than melts, they grow, but melting exceeds accumulation in warmer periods, causing glaciers to recede.
Mechanical, chemical, and biological processes all contribute to weathering of rocks. Mechanical weathering breaks rocks down physically through freezing and thawing of water or expansion and contraction from temperature changes. Chemical weathering uses chemical reactions like oxidation and hydrolysis that break bonds between minerals, especially when aided by water. Biological weathering is caused by living organisms like plant roots that grow into cracks and widen them over time.
1. The Sun is located at the center of our Solar System and is made up of hydrogen and helium.
2. It has a four-part structure including the core, photosphere, chromosphere, and corona, with temperatures ranging from 15 million degrees Celsius at its core to over 1 million degrees in its corona.
3. The Sun generates energy through nuclear fusion reactions at its core and exhibits phenomena like solar flares, prominences, and sunspots on its surface controlled by its magnetic field.
1. James Hutton established the theory of uniformitarianism, which states that the geological forces shaping Earth today are the same as in the past. He is considered the founder of modern geology.
2. Charles Darwin developed the theory of evolution through natural selection, which explained how species change over time in response to their environment.
3. Andrija Mohorovicic discovered the boundary between Earth's crust and mantle, known as the Mohorovicic discontinuity or "Moho".
4. Beno Gutenberg studied earthquakes and discovered that their waves can be used to investigate Earth's internal structure
This document discusses theories of how the Solar System formed and describes the planets in our Solar System. It begins by explaining different historical theories for how the Sun, Earth, and planets formed. The most widely accepted today is the nebular hypothesis, which suggests the Solar System formed from a rotating cloud of gas and dust that condensed. It then provides details on the classification of objects in our Solar System and defines planets. Finally, it gives brief descriptions of the eight planets - Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune.
This document discusses the four main agents of erosion: water, wind, vegetation, and human action. It provides examples of specific landforms created by each agent, including ravines formed by running water, sand dunes formed by wind, sugarloaf mountains formed by vegetation, and quarries formed by human activity. A variety of pictures accompany the text to illustrate different erosional features around the world.
Stars originate from swirling clouds of gas and dust that condense under gravity to form dense spheres called protostars. As protostars gain mass through accretion, the internal pressure and temperature rises until nuclear fusion of hydrogen begins, forming a main sequence star. Over its lifetime, a main sequence star fuses hydrogen into helium in its core. More massive stars end as supernovae, leaving behind neutron stars or black holes, while less massive stars expand into red giants and later shed their outer layers, leaving behind a fading white dwarf.
AIR POLLUTION GRADE 6 ASSIGNMENT INTRO BY E. BAIRD (C) 2008Errol Baird
basics of modern concerns about pollution of the atmosphere - adapated from my Natural Sciences workbooks for South African Schools Gr 4 - 7 - beggs@vodamail.co.za or on Facebook
The document summarizes Earth's geologic history condensed into one calendar year. Key events include:
- By March, oceans formed but no life existed on the barren planet.
- First life emerged in April in the form of single-celled organisms near ocean vents.
- By December, more complex sea creatures evolved and the first plants colonized land despite heavy rains.
- On December 31st, early humans appeared in the last hour of the year along with Neanderthals and cave drawings. Modern civilizations emerged in the final minutes.
1st qtr - earth and life science - (1) How layers of rocks formed - (2) met...Ashley Minerva
1st qtr - earth and life science - (1) How layers of rocks formed - (2) methods to determine the age of stratified rocks: relative dating and absolute dating
Dropbox es un servicio gratuito que permite sincronizar y compartir archivos entre diferentes dispositivos al guardarlos en una carpeta especial en la nube, de modo que los archivos pueden editarse desde cualquier lugar y los cambios se actualizan automáticamente en todos los equipos.
The document outlines the responsibilities of an individual working as a Windows/VMware Engineer and vCloud Automation Engineer from December 2011 to March 2014. Their key responsibilities included building and managing a VMware environment, implementing vCloud Automation for provisioning, and providing Windows administration support. They also led a team to develop an automation tool called ICP that used PowerShell and the VMware API to automate various repetitive tasks related to virtual machine provisioning, monitoring, and decommissioning.
This document discusses the life cycle of stars from their formation to their death. It begins by explaining that stars are giant balls of exploding gas made up mainly of hydrogen and helium. The document then outlines the various stages of a star's life: nebula, protostar, main sequence star, red giant, white dwarf, supernova, neutron star, and black hole. For each stage, it provides a brief description of the physical changes occurring within the star. The document emphasizes that stars much more massive than our sun will end their lives as neutron stars or black holes through the supernova process.
1) The document discusses the possibility of life existing elsewhere in the universe, beyond Earth. It explores potential habitats on planets and moons in our solar system as well as exoplanets orbiting other stars.
2) Estimates suggest there could be over 10,000 civilizations in our galaxy alone, and many planets and moons in our solar system - such as Mars, Europa, Titan, and Enceladus - show signs of being able to support some form of life.
3) Scientists are discovering hundreds of new exoplanets each month, increasing the chances of finding a planet capable of supporting life outside our solar system, such as the exoplanet Gliese 581 c.
The life cycle of stars depends on their mass. Lower mass stars like our Sun will eventually become red giants then white dwarfs. Higher mass stars live shorter lives and end as supernovas, leaving behind neutron stars or black holes. All stars begin as nebulae of dust and gas that collapse under gravity into protostars and main sequence stars fueled by nuclear fusion.
The key factors that determine whether a planet can support life include being located within the circumstellar habitable zone (Goldilocks zone) around its star where liquid water can exist on the surface, having a planetary size that allows for an atmosphere to develop and be retained, and orbiting a stable star that provides a constant radiation level like our middle-aged G-type Sun. Other considerations include the planet having a chemistry that supports liquid water through a greenhouse gas atmosphere, and being located within the optimal area of its galaxy to avoid threats from supernovae while still forming necessary heavier elements.
Stars are giant balls of gas that produce light and heat through nuclear fusion at their cores. They vary greatly in size, from dwarf stars like our Sun to massive supergiant stars over 200 times the Sun's diameter. Stars end their lives in different ways depending on their mass - smaller stars become white dwarfs, while larger stars explode as supernovae or collapse into neutron stars and other compact objects.
The Sun is a middle-aged, average sized yellow star that is made up mostly of hydrogen and helium. It is about 4.6 billion years old and located 93 million miles from Earth. The Sun generates heat and light through nuclear fusion reactions in its core that convert hydrogen into helium. It is the center of our Solar System and contains over 99% of the mass in the entire system. The Solar System also includes eight official planets that orbit the Sun, along with dwarf planets, moons, asteroids, comets, and other small bodies.
Glaciers are large, slow-moving masses of ice that form from compacted snow. They are found in mountain ranges and polar regions. Glaciers are sensitive to climate conditions and influence sea levels and water resources. They are categorized based on their thermal characteristics, behavior, and location. Alpine glaciers are confined to valleys while continental glaciers span entire regions. As glaciers accumulate more snow than melts, they grow, but melting exceeds accumulation in warmer periods, causing glaciers to recede.
Mechanical, chemical, and biological processes all contribute to weathering of rocks. Mechanical weathering breaks rocks down physically through freezing and thawing of water or expansion and contraction from temperature changes. Chemical weathering uses chemical reactions like oxidation and hydrolysis that break bonds between minerals, especially when aided by water. Biological weathering is caused by living organisms like plant roots that grow into cracks and widen them over time.
1. The Sun is located at the center of our Solar System and is made up of hydrogen and helium.
2. It has a four-part structure including the core, photosphere, chromosphere, and corona, with temperatures ranging from 15 million degrees Celsius at its core to over 1 million degrees in its corona.
3. The Sun generates energy through nuclear fusion reactions at its core and exhibits phenomena like solar flares, prominences, and sunspots on its surface controlled by its magnetic field.
1. James Hutton established the theory of uniformitarianism, which states that the geological forces shaping Earth today are the same as in the past. He is considered the founder of modern geology.
2. Charles Darwin developed the theory of evolution through natural selection, which explained how species change over time in response to their environment.
3. Andrija Mohorovicic discovered the boundary between Earth's crust and mantle, known as the Mohorovicic discontinuity or "Moho".
4. Beno Gutenberg studied earthquakes and discovered that their waves can be used to investigate Earth's internal structure
This document discusses theories of how the Solar System formed and describes the planets in our Solar System. It begins by explaining different historical theories for how the Sun, Earth, and planets formed. The most widely accepted today is the nebular hypothesis, which suggests the Solar System formed from a rotating cloud of gas and dust that condensed. It then provides details on the classification of objects in our Solar System and defines planets. Finally, it gives brief descriptions of the eight planets - Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune.
This document discusses the four main agents of erosion: water, wind, vegetation, and human action. It provides examples of specific landforms created by each agent, including ravines formed by running water, sand dunes formed by wind, sugarloaf mountains formed by vegetation, and quarries formed by human activity. A variety of pictures accompany the text to illustrate different erosional features around the world.
Stars originate from swirling clouds of gas and dust that condense under gravity to form dense spheres called protostars. As protostars gain mass through accretion, the internal pressure and temperature rises until nuclear fusion of hydrogen begins, forming a main sequence star. Over its lifetime, a main sequence star fuses hydrogen into helium in its core. More massive stars end as supernovae, leaving behind neutron stars or black holes, while less massive stars expand into red giants and later shed their outer layers, leaving behind a fading white dwarf.
AIR POLLUTION GRADE 6 ASSIGNMENT INTRO BY E. BAIRD (C) 2008Errol Baird
basics of modern concerns about pollution of the atmosphere - adapated from my Natural Sciences workbooks for South African Schools Gr 4 - 7 - beggs@vodamail.co.za or on Facebook
The document summarizes Earth's geologic history condensed into one calendar year. Key events include:
- By March, oceans formed but no life existed on the barren planet.
- First life emerged in April in the form of single-celled organisms near ocean vents.
- By December, more complex sea creatures evolved and the first plants colonized land despite heavy rains.
- On December 31st, early humans appeared in the last hour of the year along with Neanderthals and cave drawings. Modern civilizations emerged in the final minutes.
1st qtr - earth and life science - (1) How layers of rocks formed - (2) met...Ashley Minerva
1st qtr - earth and life science - (1) How layers of rocks formed - (2) methods to determine the age of stratified rocks: relative dating and absolute dating
Dropbox es un servicio gratuito que permite sincronizar y compartir archivos entre diferentes dispositivos al guardarlos en una carpeta especial en la nube, de modo que los archivos pueden editarse desde cualquier lugar y los cambios se actualizan automáticamente en todos los equipos.
The document outlines the responsibilities of an individual working as a Windows/VMware Engineer and vCloud Automation Engineer from December 2011 to March 2014. Their key responsibilities included building and managing a VMware environment, implementing vCloud Automation for provisioning, and providing Windows administration support. They also led a team to develop an automation tool called ICP that used PowerShell and the VMware API to automate various repetitive tasks related to virtual machine provisioning, monitoring, and decommissioning.
Kenneth J. Voellinger has over 20 years of experience as a Chemical Process Manager and Machine Process Operator specializing in chemical manufacturing. He is skilled in troubleshooting, safety practices, multitasking, training employees, and collaborating with technical teams to solve processing errors. Voellinger has certifications in chemical process operations, self-contained breathing apparatus use, hazardous materials handling, and forklift operation.
La dureza del agua es causada por las sales solubles en ella; puede ser temporal o permanente. La dureza temporal es causada por bicarbonato cálcico o de magnesio y puede ser eliminada con la ebullición. Los bicarbonatos alcalinos generalmente son escasos en el agua. La dureza permanente del agua es causada por los sulfatos y los cloruros de calcio y magnesio. La suma de la dureza temporal y la permanente se llama dureza total del agua.
El plan de clase trata sobre una lección de 30 minutos sobre los colores en español para estudiantes de primer año de enseñanza media. Los objetivos son demostrar aspectos de la lengua española, presentar y reconocer los colores. La profesora utilizará estrategias como trabajar la pronunciación y escritura de los colores, así como hojas en blanco e identificación de colores. La evaluación incluirá descripciones orales y escritas de creaciones con los colores, repaso del contenido y una actividad grupal.
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⭐⭐⭐⭐⭐ Ejemplo de Taller Sistema Digital Completo (2do Parcial)Victor Asanza
✅ Se tiene un grupo de 32 electrodos distribuidos con el estándar internacional 10-2 0 en el cuero cabelludo de un paciente, con el fin de detectar las intensiones motoras procesando las señales de Electroencefalografía (EEG). Estas señales fueron adquiridas a una frecuencia de muestreo de 100 muestras por segundo (sps) con una resolución de 8 bits.
La Unión Europea ha propuesto un nuevo paquete de sanciones contra Rusia que incluye un embargo al petróleo ruso. El embargo se aplicaría gradualmente durante seis meses para el petróleo crudo y ocho meses para los productos refinados. Este paquete de sanciones requiere la aprobación unánime de los 27 estados miembros de la UE.
La arteria femoral se origina de la ilíaca externa y discurre por el muslo hasta convertirse en la arteria poplítea. Describe su trayecto a través del conducto crural, el triángulo de Scarpa y el conducto de Hunter, y sus principales ramas como la femoral profunda y superficial. Finalmente, la arteria poplítea continúa en la parte posterior de la rodilla hasta bifurcarse en las arterias tibial anterior y tronco tibioperoneo.
Este documento presenta una secuencia didáctica para una clase de Formación Cívica y Ética sobre la resolución pacífica de conflictos. Los estudiantes trabajarán en equipos en actividades que involucran rompecabezas y la recreación de historias para desarrollar habilidades de comunicación no verbal, toma de decisiones y manejo de emociones. El propósito es que los estudiantes aprendan a identificar conflictos y resolverlos de manera pacífica y respetuosa de los derechos de los demás.
This document provides an excerpt from the book "The 6 Most Important Decisions You'll Ever Make" by Sean Covey. It introduces the premise that there are six key decisions teenagers make that can significantly impact their future. These decisions relate to school, friends, parents, dating/sex, addictions, and self-worth. The excerpt discusses two fictional teenagers, Allie and Desiree, who made different choices in these areas and ended up in very different places as a result ten years later. It emphasizes that teenagers have free will to choose their path and control their destiny through the decisions they make during these formative years.
The document introduces Emelie, who currently has Facebook, Twitter, and Myspace accounts. In 5 years, she expects to have a website supporting her singing career, with a new album coming out and some press about charity events. Emelie enjoys singing, taking care of kids, and voicing her opinion. She does not want to settle for less than she deserves. The document provides some personal details about Emelie and ends by thanking the reader.
The essay describes the author's experience learning to play the violin as a senior in high school, noting that their progress was slow and fingers would tense up, making the music sound horrible. However, their violin instructor encouraged them to continue practicing and not hesitate, even if mistakes were made. The narrative focuses on the author's determination to develop a new talent on the violin despite challenges.
American Hookup: The New Culture of Sex on Campuslisawadephd
The media both celebrates and condemns “hookup culture,” a mythical environment in which college students have an endless string of casual sexual partners. In fact, students are having a lot less sex than these stories suggest. More, they report that the sex they are having is disappointing, to say the least. In this talk, I discuss the difference between hooking up as a behavior, a script, and a culture; what it means to live in a hookup culture; and why students report distress, disappointment, and trauma. The solution? Not to abandon the casual hookup (it has some interesting advantages), but to even the playing field on college campuses by taking power away from privileged students, giving everyone the information they need to make informed decisions, and then let students themselves nurture and innovate new sexual cultures, thus diversifying sexual options on campus.
The document discusses themes of isolation in J.D. Salinger's novel "The Catcher in the Rye". The story follows Holden Caulfield who constantly feels isolated and judges those around him. He isolates himself both mentally and socially. Nearly the entire story is told from Holden's isolated perspective as he struggles with feelings of loneliness and depression.
This document contains an interview with Ella Bella, a famous pop singer. In the interview, Ella discusses how she got her start in the music industry by uploading a video of herself singing to YouTube which went viral. She talks about overcoming stressful situations by staying positive and being grateful for her fans and family. Ella also answers fans' questions, saying her next tour will likely be next year and that she couldn't choose the most famous person in her phone contacts because there are so many celebrities.
If you're reading this, it is because you wish to know what it is like to suffer from autism from the perspective of someone on the spectrum. Why you should want such a thing is beyond my comprehension. Was it a child of your own who also suffers? Or was it, perhaps, a morbid curiosity? I'm telling you right now, if you're looking for some words to inspire hope then you can stop reading right now. I'm a thirty-year-old who delivers pizza and still lives with his parents, I have none to give.
The document discusses how the individual enjoys working out through running and yoga to relieve stress, and has recently taken up cooking and baking in their downtime, enjoying experimenting with recipes by swapping out ingredients. They also mention traveling for work and bringing a book along to read.
Similar to Celebrity Bullying Presentation Nov 2012 (8)
2. “The kids at school thought it was weird that I
liked country music. They’d make fun of me.”
Taylor Swift
3. Taylor Lautner
“I was viewed as a little bit of outcast. I didn’t
have one group of friends who I hung out with
every single day”
4. Beyonce
“I’m like everyone else – I have days when I look
in the mirror and I’m like, Oh my god, I wish I
could change this or that. The more you mature,
you realize that those imperfections make you
more beautiful.”
5. Zac Efron
“I got made fun of constantly [in high school]. When you get
made fun of, when people point out your weaknesses, that’s
just another opportunity for you to rise above.”
6. “I’ve often felt unattractive or different looking. As I’ve
grown up, I’ve felt more comfortable in my own skin. It
may sound cliché, but when you feel beautiful and
strong on the inside, it shows on the outside.”
Angelina Jolie
7. “I never fit in, so I started pretending I was other people I
thought were cool and dress how they dressed, talk how
they talked, do whatever they were into.”
Corey Monteith
8. “In elementary school I was the
mean girl, I would kick girls out
of our group and make them go
play with the non-popular kids.”
“I became the freak, the weirdo
that everyone would stare at.”
“I used to get picked on a lot. But
now I can get my own back.”
Tyra Banks
9. “ I got beat up in the bathroom, beat up in the
hallways, shoved into lockers. You know, just
for being the new kid.”
Eminem
10. “Bullying happens more than you think. I
was bullied in school and it affected me so
much I decided to be home schooled.”
Demi Lovato
11. “ I was bullied until I
prevented a new
student from being
bullied. By standing up
for him, I learned to
stand up for myself.”
Jackie Chan
12. “I think every year I become happier because I am more
confident and more comfortable in my own skin.”
Zooey Deschanel
13. “I got beat up just
about every day…
I got kicked and
whatever”
Chris Rock
14. “In junior high, I had glasses and braces, my face
was broken out and I was chubby.”
Kelly Clarkson
15. “I’m still in my awkward phase! My voice has been
creaky since I was 13 and I can’t get it to stop. I
think everyone feels awkward.”
Ashton Kutcher
16. Jessica Simpson
“ I had girls egging my home, writing curse words on the
sidewalk in paint – just saying really nasty things about
me. I quit cheerleading because I didn’t know what I was
cheering for anymore.”
17. “ I had no really close friend, someone who
understands you. I was always the new kid with
the wrong shoes, the wrong accent. I didn’t have
the friend to share things with and confide in.”
Tom Cruise
18. “ I didn’t fit in at high school. I felt like a freak. It
took a long time for me to be OK with myself.”
Lady Gaga
20. Anti-Bullying
Anti-Bullying Legislation
Arkansas Anti-Bullying Policy for
Schools
California “Seth’s Law”
Colorado House Bill 1254
Massachusetts Bullying Law
Michigan –
“Matt’s Safe School Law”
New Jersey “Anti-Bullying Bill of Rights”
Texas Anti-Bullying Bill
Virginia House Bill 1624
Washington Cyberbullying Law
Editor's Notes
TAYLOR SWIFT says just because you look perfect doesn't mean you feel perfect"Tied Together With a Smile" is about a girl I knew my freshman year. She was absolutely Miss Popular, a pageant girl, and she looked perfect every day! Always had the cutest outfits, always looked the best at prom. But sometimes when you get a little closer to people who look that perfect, you realize that they don't feel perfect. They feel like they're ugly. And that's what happened with this girl--I became closer friends with her, and one day she confessed that she was bulimic.Everybody looks in the mirror and is like, I wonder why her eyes are huge and mine are smaller. But I realized that if you're lucky enough to be different from everybody else, don't change. Seventeen
Taylor Lautner – Twilight
“I was viewed as a little bit of an outcast. I didn’t have one group of friends who I hung out with every single day. I would have friends on my football team, friends in drama, friends in video production, and I would hang out with different people. I know that wasn’t the normal thing to do in high school. The normal thing is to be part of a clique. But for me, I love hanging out with different people and just having fun.”
BEYONCE offers great "relationship" advice"You have to know exactly what you need out of a relationship. You should be finding out what makes you happy in life. I know it sounds preachy, but I'm happy that I knew that. I think everyone has her own body type and looks good at different weights - that's what's so beautiful.” Seventeen
Zac Efron
“I got made fun of constantly (in high school)! That's what built my character. That's what makes you who you are. When you get made fun of-when people point out your weaknesses-that's just another opportunity for you to rise above." Twist
Angelina Jolie
Corey Monteith – Glee
Corey started using drugs and alcohol and when his family gave him an ultimatum to get clean or they’d report him to the police Corey said, “I was done fighting myself. I finally said, “I’m gonna start looking at my life and figure out why I am doing this.” He quit using, got a job and surrounded himself with sober people and today is a star on Glee.
Tyra Banks
Tyra has identified herself as BOTH a bully and someone who was bullied. She was picked on for being tall and skinny in middle school. Then she went to another school where they thought she was pretty BECAUSE she was skinny. She says that beauty can be cultural as well.
Eminem – Marshall Mathers
EMINEM on judging people:
"...you gotta learn to judge people for the individuals that they are." Cosmo Girl
Demi Lovato
“At 12 years old, I was bullied in school. Girls were calling me fat, so I thought, “That’s the reason I don’t have any friends.” So I stopped eating. I became very weight-conscious, and I lost 30 lbs. I went down to 95 lbs.”
Jackie Chan – The (New) Karate Kid
Zooey Deschanel – New Girl
Plot of New Girl - After a bad break-up, Jess, an offbeat young woman, moves into an apartment loft with three single men. Although they find her behavior very unusual, the men support her
Zooey Deschanel was once asked if the character was written for her specifically, to which she replied that it was not, but "should have been"
Chris Rock – Everybody Hates Chris
Plot of Everybody Hates Chris - Motivated by his childhood experiences, Emmy Award-winner/actor/comedian Chris Rock narrates this very hilarious and touching story of a teenager growing up as the oldest of three children in Brooklyn, NY, in 1982. With his mom determined to see him in a good school, Chris reluctantly faces multiple bus transfers every day to attend Corleone Junior High in the fiercely Italian neighborhood, South Shore. Despite being an immediate target for bullies, Chris' innate charm and sharp wit enable him to make new friends.
Kelly Clarkson
The reporter asked Kelly if there was anything else that helped her feel more comfortable in her own skin. She said, ".....I was always involved and always doing stuff. I did sports, drama, choir and I was also in senior council. Exercise and staying active always makes me feel great."
Nobody has my eyes. Nobody has my nose. It's all mine. And that's what makes me different from everyone.“ -Twist
Ashton Kutcher
"I'm still in my awkward phase! My voice has been creaky since I was 13, and I still can't get it to stop. During my freshman year in high school, I weighted, like 103 pounds. I was the little kid in school. Then there was a period where I grew, like, six inches and put on 50 pounds in one year. I was growing so fast that I couldn't afford new pants. I was wearing unintentional high waters. And when I was a kid, my teeth were too big for my face. I think everybody feels awkward."
Jessica Simpson
"I didn't start feeling comfortable in my own skin until I was 20. Natural beauty is really happiness with who you are. If you like who you are on the inside, that'll come through on the outside." – Twist
"You're never going to look perfect to yourself even if you might look perfect to somebody else. The thing I've had to learn the most is to accept compliments and steer away from all the negativity. A lot of people can feel shy about what they really want to do, and it did take a while for me to say, 'You know what? I do want to do this.“ - Cosmopolitan
Tom Cruise
Tom was in 15 different schools in 12 years. Like many kids today, he had a reading disability so instead of putting him in with the "normal" kids they put him in remedial classes. A lot of our readers can understand that and how that makes you feel. Tom said he felt excluded and being small he was bullied a lot. "So many times the big bully comes up, pushes me. Your heart's pounding, you sweat, and you feel like you're going to vomit. I'm not the biggest guy, I never liked hitting someone, but I know if I don't hit that guy hard he's going to pick on me all year. I go, 'You better fight.' I just laid it down. I don't like bullies."
Lady Gaga
Led by Lady Gaga and her mother Cynthia Germanotta, the Born This Way Foundation was founded in 2011 to foster a more accepting society, where differences are embraced and individuality is celebrated. The Foundation is dedicated to creating a safe community that helps connect young people with the skills and opportunities they need to build a kinder, braver world.
We believe that everyone has the right to feel safe, to be empowered and to make a difference in the world. Together, we will move towards acceptance, bravery and love.
President Barack Obama
Many of the photos you have seen here were found at heyugly.org
Hey U.G.L.Y.- Unique Gifted Lovable You was founded in 2002 under the name, Hey U.G.L.Y., Inc. We are dedicated to empowering youth be WHO THEY ARE instead of having to act how they think they need to be in order to fit in.