The document discusses the four main layers of Earth: 1) the inner core, 2) the outer core, 3) the mantle, and 4) the crust. The crust is the outermost layer and is relatively light and brittle, with most earthquakes occurring within the crust.
The document discusses characteristics of the Sun such as its mass, diameter, and density. It describes how the Sun was formed from a giant nebula 4.6 billion years ago and will eventually become a white dwarf. The Sun has several layers including the photosphere, chromosphere, and corona. Phenomena on the Sun's surface like sunspots, prominences, and solar flares are discussed, which can impact the Earth's climate and communication systems. The Sun's energy comes from nuclear fusion in its core which radiates heat and light energy across the solar system.
1) The document summarizes a virtual field trip through the layers of the Sun, including stops in the core, photosphere, chromosphere, and corona.
2) Key points covered include that the Sun's core is over 27 million degrees Fahrenheit and produces heat and light through nuclear fusion. Sunspots appear darker on the photosphere.
3) The number of sunspots and solar prominences varies during the approximate 11-year solar maximum and minimum cycle.
Sunspots are cooler areas on the sun's surface with strong magnetic fields, sometimes as large as Earth. They occur in pairs and can be up to 6,400 K cooler than the surrounding photosphere. Sunspots follow an 11-year cycle of increasing and decreasing activity, with the last peak in 2001. When sunspots are most active, the sun is actually brighter due to surrounding brighter magnetic areas compensating for the dimmer spots. There are also much longer cycles of very low or high sunspot activity lasting around a century.
This document discusses a cropped photo that initially shows a pleasant scene but zooming out reveals trash and litter, representing how environmental destruction is often overlooked despite being increasingly severe. The full picture shows nature being damaged by human waste and neglect, hidden behind nicer views that people prefer to see.
You asked...What would happen to the Earth if the sun turned into a black hole?wonderdome
What would have happened to the Earth if the Sun suddenly turned into a black hole? That was the most frequent question we’ve been asked this Autumn.
And if you are already imagining the Earth spiralling towards the black-hole-Sun, being spaghettified and other similar horrors, you are not the only one! Let us put your fears to rest once and for all. None of those awful things are going to happen in real life!
Geothermal energy harnesses heat from the Earth's core that is transferred outward through the soil in areas with volcanic activity. Heat from radioactive decay and absorbed solar radiation is stored in the Earth and radiates outwards, heating rocks and water. Geothermal plants drill wells into hot underground reservoirs to access this thermal energy and use the heated water or steam to power turbine generators before reinjecting the water back underground, providing a renewable source of energy.
The corona is the outermost layer of the sun and is only visible during a solar eclipse. It is much hotter than the sun's visible surface. The sun is made up of hot gases like hydrogen and helium and is the center of our solar system around which all planets orbit. It provides light and heat for the solar system. The core of the sun produces most of its heat and light through nuclear fusion and energy moves outward from there.
The sun is vital for life on Earth, providing light, heat, and energy. It is approximately 92 million miles from Earth, though it appears close due to its immense size—its diameter is 1.3 million kilometers and 333 Earths could fit inside it. The sun has six layers from its core to corona, and features dark sunspots on its surface that occur every 11 years and can be over 50,000 kilometers wide. Scientists have learned the sun rotates by observing the movement of sunspots.
The document discusses characteristics of the Sun such as its mass, diameter, and density. It describes how the Sun was formed from a giant nebula 4.6 billion years ago and will eventually become a white dwarf. The Sun has several layers including the photosphere, chromosphere, and corona. Phenomena on the Sun's surface like sunspots, prominences, and solar flares are discussed, which can impact the Earth's climate and communication systems. The Sun's energy comes from nuclear fusion in its core which radiates heat and light energy across the solar system.
1) The document summarizes a virtual field trip through the layers of the Sun, including stops in the core, photosphere, chromosphere, and corona.
2) Key points covered include that the Sun's core is over 27 million degrees Fahrenheit and produces heat and light through nuclear fusion. Sunspots appear darker on the photosphere.
3) The number of sunspots and solar prominences varies during the approximate 11-year solar maximum and minimum cycle.
Sunspots are cooler areas on the sun's surface with strong magnetic fields, sometimes as large as Earth. They occur in pairs and can be up to 6,400 K cooler than the surrounding photosphere. Sunspots follow an 11-year cycle of increasing and decreasing activity, with the last peak in 2001. When sunspots are most active, the sun is actually brighter due to surrounding brighter magnetic areas compensating for the dimmer spots. There are also much longer cycles of very low or high sunspot activity lasting around a century.
This document discusses a cropped photo that initially shows a pleasant scene but zooming out reveals trash and litter, representing how environmental destruction is often overlooked despite being increasingly severe. The full picture shows nature being damaged by human waste and neglect, hidden behind nicer views that people prefer to see.
You asked...What would happen to the Earth if the sun turned into a black hole?wonderdome
What would have happened to the Earth if the Sun suddenly turned into a black hole? That was the most frequent question we’ve been asked this Autumn.
And if you are already imagining the Earth spiralling towards the black-hole-Sun, being spaghettified and other similar horrors, you are not the only one! Let us put your fears to rest once and for all. None of those awful things are going to happen in real life!
Geothermal energy harnesses heat from the Earth's core that is transferred outward through the soil in areas with volcanic activity. Heat from radioactive decay and absorbed solar radiation is stored in the Earth and radiates outwards, heating rocks and water. Geothermal plants drill wells into hot underground reservoirs to access this thermal energy and use the heated water or steam to power turbine generators before reinjecting the water back underground, providing a renewable source of energy.
The corona is the outermost layer of the sun and is only visible during a solar eclipse. It is much hotter than the sun's visible surface. The sun is made up of hot gases like hydrogen and helium and is the center of our solar system around which all planets orbit. It provides light and heat for the solar system. The core of the sun produces most of its heat and light through nuclear fusion and energy moves outward from there.
The sun is vital for life on Earth, providing light, heat, and energy. It is approximately 92 million miles from Earth, though it appears close due to its immense size—its diameter is 1.3 million kilometers and 333 Earths could fit inside it. The sun has six layers from its core to corona, and features dark sunspots on its surface that occur every 11 years and can be over 50,000 kilometers wide. Scientists have learned the sun rotates by observing the movement of sunspots.
The moon measuring tape, showing the distance between the earth and the moon, is available as a separate file and can be used as a teaching aid or for other purposes. Some 4.6 billion years ago, gas and debris swirling around the sun coalesced to form the earth and other planets. The young earth was impacted by planetesimals, creating seas of magma. When the seas cooled, rain began to fall, forming the seas. This 19-piece papercraft globe model shows the earth, moon, and stand and can be assembled using the instruction sheets.
The Sun is our closest star, with a diameter of 1.4 million km and a mass 330,000 times that of Earth. Its surface temperature is around 5,800 K and it is expected to exist for another 10 billion years. The Sun is composed of three main layers - the core, radiative zone, and convective zone - as well as an atmosphere with the photosphere, chromosphere, and corona. Features on the Sun like sunspots and solar flares are produced by its magnetic field.
- Encke is currently the brightest comet visible, shining at a magnitude of 2 and visible through binoculars in the northern hemisphere. It will be brightest over the next month.
- Comet ISON may disappoint and not become bright enough to see with the naked eye. It faces an uncertain fate after passing close to the sun due to heat, gravity and radiation.
- Comet Linear has increased dramatically in brightness but is still difficult to observe, only visible low on the northeast horizon just before sunrise.
- Comet Lovejoy, discovered in September 2013, is now visible through small telescopes below Jupiter in the morning sky.
The chapter summarizes key aspects of the Sun including its interior structure, outer layers, and activity. The Sun's core powers it through nuclear fusion, while its luminosity can be calculated from Earth's fraction of received energy. Doppler shifts and models reveal details about the solar interior and convection zones. Sunspots occur in magnetic regions and follow an 11-year cycle, while flares and coronal mass ejections sometimes impact Earth. Neutrinos directly observed from the core have taught us more about neutrinos than the Sun's interior.
The Sun is the closest star to Earth and governs the Solar System. It is about 13,00,000 times bigger than Earth and composed of a dense core, radiative zone, and convective zone. Its atmosphere consists of the photosphere, chromosphere, and corona. Nuclear fusion in the core powers the Sun, primarily through the proton-proton chain. Magnetic activity on the Sun includes sunspots and solar flares. The Sun will eventually exhaust its nuclear fuel and expand into a red giant star before shrinking into a white dwarf over its lifetime of approximately 10 billion years.
The Sun is by far the largest object in the solar system, containing over 99% of the mass. It has a diameter over 100 times larger than Earth and generates energy through nuclear fusion of hydrogen into helium. Light from the Sun takes approximately 8 minutes to reach Earth. While the visible surface of the Sun appears solid, it actually consists of several layers including the core, radiative zone, convective zone, photosphere, chromosphere, and corona. Solar activity like sunspots, solar flares, and coronal mass ejections can impact power grids and communication systems on Earth. Astronomers study the Sun to better understand stars and how changes in solar output impact Earth's climate and atmosphere.
The document discusses the structure and composition of the Sun. It has 6 layers: the core, where fusion occurs at 15 million degrees Celsius; the radiative zone, where energy moves by radiation; the convection zone, where hot gas currents transfer energy; the photosphere, the visible surface; the chromosphere, a thin pinkish layer; and the corona, the outermost low density layer. The Sun is mostly made of hydrogen and helium and produces energy through the fusion of hydrogen into helium. It contains over 99% of the mass in the solar system and has prominent features like sunspots and solar winds.
Jupiter is the largest planet in the solar system. It is composed primarily of hydrogen and helium gases and has 67 known moons. Some key facts about Jupiter include that it is located about 750 million km from the sun, has a rocky core below its compressed hydrogen layers, and has four largest moons called Io, Europa, Ganymede, and Callisto that vary in size and orbital characteristics. NASA has explored Jupiter since the 1970s through missions like Pioneer, Voyager, and Galileo to learn more about its rings, moons, and composition.
The document discusses various cosmic events that pose dangers to life on Earth, including asteroids, comets, solar flares, supernovae, and gamma-ray bursts. These events have caused mass extinctions in the past and will continue to threaten life. Even relatively nearby occurrences of supernovae or gamma-ray bursts could damage the ozone layer and increase UV radiation, endangering life. Additionally, the Sun will gradually grow hotter over billions of years and eventually expand to engulf the Earth.
1) The universe is vast and dangerous, with our solar system and galaxy being relatively small parts of the larger universe.
2) Throughout Earth's history, there have been at least five mass extinctions caused by cosmic events like asteroids and comets. These events will continue to occur randomly in the future.
3) Other random cosmic events that can impact Earth include solar flares, supernovae, and gamma-ray bursts, with the latter having possibly contributed to a past mass extinction due to ozone depletion and increased UV radiation.
The document discusses the layers of the Earth and volcanoes. It describes how earthquakes are recorded by seismographs and occur along faults in the Earth's crust and mantle. It explains that the Earth has an inner core made of hot metals, an outer core made of liquid metals, a mantle below the crust, and a crust that forms the Earth's surface. It also defines a volcano as a mountain with a crater at the top, and explains volcanic eruptions are caused by tectonic plates pulling apart and allow magma, gases, and particles to escape. Finally, it lists the five layers of a volcano as the ash cloud, crater cone, lava, vent, and magma chamber below the surface.
The Sun is a G2V type star made of gas and dust from other stars. It is approximately 4.65 billion years old and has a lifetime of another 5.5 billion years. The Sun has different inner layers including a core with a temperature of 15 million Kelvin, a radiative zone, and a convective zone that moves the Sun's mass. The Sun's surface, called the photosphere, is about 5,800 Kelvin and features solar spots. The Sun's outer atmosphere, the corona, reaches temperatures over 20 million Kelvin and features magnetic coronal loops.
The document discusses the physical structure and properties of the Sun. It describes how the Sun generates energy through nuclear fusion reactions in its core, where hydrogen is fused into helium. This releases energy according to Einstein's equation. It also summarizes the Sun's interior structure, atmosphere, activity cycles, and how observations of neutrinos and vibrations have informed our understanding.
The Sun formed around 5 billion years ago from a cloud of gas and dust. Through the process of nuclear fusion at its core, the Sun generates immense heat and light by converting hydrogen into helium. It is a common yellow star that is part of a cycle that creates convection currents within its surface and sunspots that follow an 11-year cycle. The Sun provides the energy necessary to sustain life on Earth but will eventually exhaust its hydrogen fuel in around 5 billion years.
The sun is a huge glowing ball of gas at the center of our solar system that provides light, heat, and energy to Earth. It is made up primarily of hydrogen and helium and has a radius about 109 times that of Earth. The sun was formed around 4.6 billion years ago and will remain stable for another 5 billion years before expanding into a red giant. It emits electromagnetic radiation across the spectrum, including visible light and infrared that we experience as heat and light. Nuclear fusion in the sun's core converts hydrogen to helium and releases enormous amounts of energy.
The document provides an introduction to stars, focusing on the sun. It discusses the layers of the sun's atmosphere and interior. The sun's core generates its enormous energy output through nuclear fusion. The solar wind consists of high-energy particles escaping the sun's gravity. The sun emits across the electromagnetic spectrum, including x-rays studied by orbital telescopes. The sun's total luminosity is calculated based on the energy received by a detector at Earth's distance. Sunspots occur in pairs of opposite magnetic fields and vary in a roughly 11-year solar cycle.
The sun has a core temperature of 15 million Kelvin and a surface temperature of 9,932 degrees Fahrenheit. It is 4.5 billion years old and will exist in its current form for another 5 billion years before running out of hydrogen. Solar flares are sudden bursts of radiation caused by collisions between magnetic fields on the sun's surface. The sun is the largest mass in the solar system and emits solar wind, which causes phenomena like the Northern Lights and affects spacecraft trajectories.
The Midnight Sun is a phenomenon that allows the sun to be seen at midnight, occurring in Norway between June 21 and December 21 each year. It is caused by Norway's northern latitude location above the Arctic Circle. On clear days, the sun remains visible for a full 24 hours, but overcast conditions can block the Midnight Sun from being seen. Norway is nicknamed "The Land of the Midnight Sun" due to this special event.
Beyond Degrees - Empowering the Workforce in the Context of Skills-First.pptxEduSkills OECD
Iván Bornacelly, Policy Analyst at the OECD Centre for Skills, OECD, presents at the webinar 'Tackling job market gaps with a skills-first approach' on 12 June 2024
🔥🔥🔥🔥🔥🔥🔥🔥🔥
إضغ بين إيديكم من أقوى الملازم التي صممتها
ملزمة تشريح الجهاز الهيكلي (نظري 3)
💀💀💀💀💀💀💀💀💀💀
تتميز هذهِ الملزمة بعِدة مُميزات :
1- مُترجمة ترجمة تُناسب جميع المستويات
2- تحتوي على 78 رسم توضيحي لكل كلمة موجودة بالملزمة (لكل كلمة !!!!)
#فهم_ماكو_درخ
3- دقة الكتابة والصور عالية جداً جداً جداً
4- هُنالك بعض المعلومات تم توضيحها بشكل تفصيلي جداً (تُعتبر لدى الطالب أو الطالبة بإنها معلومات مُبهمة ومع ذلك تم توضيح هذهِ المعلومات المُبهمة بشكل تفصيلي جداً
5- الملزمة تشرح نفسها ب نفسها بس تكلك تعال اقراني
6- تحتوي الملزمة في اول سلايد على خارطة تتضمن جميع تفرُعات معلومات الجهاز الهيكلي المذكورة في هذهِ الملزمة
واخيراً هذهِ الملزمة حلالٌ عليكم وإتمنى منكم إن تدعولي بالخير والصحة والعافية فقط
كل التوفيق زملائي وزميلاتي ، زميلكم محمد الذهبي 💊💊
🔥🔥🔥🔥🔥🔥🔥🔥🔥
The moon measuring tape, showing the distance between the earth and the moon, is available as a separate file and can be used as a teaching aid or for other purposes. Some 4.6 billion years ago, gas and debris swirling around the sun coalesced to form the earth and other planets. The young earth was impacted by planetesimals, creating seas of magma. When the seas cooled, rain began to fall, forming the seas. This 19-piece papercraft globe model shows the earth, moon, and stand and can be assembled using the instruction sheets.
The Sun is our closest star, with a diameter of 1.4 million km and a mass 330,000 times that of Earth. Its surface temperature is around 5,800 K and it is expected to exist for another 10 billion years. The Sun is composed of three main layers - the core, radiative zone, and convective zone - as well as an atmosphere with the photosphere, chromosphere, and corona. Features on the Sun like sunspots and solar flares are produced by its magnetic field.
- Encke is currently the brightest comet visible, shining at a magnitude of 2 and visible through binoculars in the northern hemisphere. It will be brightest over the next month.
- Comet ISON may disappoint and not become bright enough to see with the naked eye. It faces an uncertain fate after passing close to the sun due to heat, gravity and radiation.
- Comet Linear has increased dramatically in brightness but is still difficult to observe, only visible low on the northeast horizon just before sunrise.
- Comet Lovejoy, discovered in September 2013, is now visible through small telescopes below Jupiter in the morning sky.
The chapter summarizes key aspects of the Sun including its interior structure, outer layers, and activity. The Sun's core powers it through nuclear fusion, while its luminosity can be calculated from Earth's fraction of received energy. Doppler shifts and models reveal details about the solar interior and convection zones. Sunspots occur in magnetic regions and follow an 11-year cycle, while flares and coronal mass ejections sometimes impact Earth. Neutrinos directly observed from the core have taught us more about neutrinos than the Sun's interior.
The Sun is the closest star to Earth and governs the Solar System. It is about 13,00,000 times bigger than Earth and composed of a dense core, radiative zone, and convective zone. Its atmosphere consists of the photosphere, chromosphere, and corona. Nuclear fusion in the core powers the Sun, primarily through the proton-proton chain. Magnetic activity on the Sun includes sunspots and solar flares. The Sun will eventually exhaust its nuclear fuel and expand into a red giant star before shrinking into a white dwarf over its lifetime of approximately 10 billion years.
The Sun is by far the largest object in the solar system, containing over 99% of the mass. It has a diameter over 100 times larger than Earth and generates energy through nuclear fusion of hydrogen into helium. Light from the Sun takes approximately 8 minutes to reach Earth. While the visible surface of the Sun appears solid, it actually consists of several layers including the core, radiative zone, convective zone, photosphere, chromosphere, and corona. Solar activity like sunspots, solar flares, and coronal mass ejections can impact power grids and communication systems on Earth. Astronomers study the Sun to better understand stars and how changes in solar output impact Earth's climate and atmosphere.
The document discusses the structure and composition of the Sun. It has 6 layers: the core, where fusion occurs at 15 million degrees Celsius; the radiative zone, where energy moves by radiation; the convection zone, where hot gas currents transfer energy; the photosphere, the visible surface; the chromosphere, a thin pinkish layer; and the corona, the outermost low density layer. The Sun is mostly made of hydrogen and helium and produces energy through the fusion of hydrogen into helium. It contains over 99% of the mass in the solar system and has prominent features like sunspots and solar winds.
Jupiter is the largest planet in the solar system. It is composed primarily of hydrogen and helium gases and has 67 known moons. Some key facts about Jupiter include that it is located about 750 million km from the sun, has a rocky core below its compressed hydrogen layers, and has four largest moons called Io, Europa, Ganymede, and Callisto that vary in size and orbital characteristics. NASA has explored Jupiter since the 1970s through missions like Pioneer, Voyager, and Galileo to learn more about its rings, moons, and composition.
The document discusses various cosmic events that pose dangers to life on Earth, including asteroids, comets, solar flares, supernovae, and gamma-ray bursts. These events have caused mass extinctions in the past and will continue to threaten life. Even relatively nearby occurrences of supernovae or gamma-ray bursts could damage the ozone layer and increase UV radiation, endangering life. Additionally, the Sun will gradually grow hotter over billions of years and eventually expand to engulf the Earth.
1) The universe is vast and dangerous, with our solar system and galaxy being relatively small parts of the larger universe.
2) Throughout Earth's history, there have been at least five mass extinctions caused by cosmic events like asteroids and comets. These events will continue to occur randomly in the future.
3) Other random cosmic events that can impact Earth include solar flares, supernovae, and gamma-ray bursts, with the latter having possibly contributed to a past mass extinction due to ozone depletion and increased UV radiation.
The document discusses the layers of the Earth and volcanoes. It describes how earthquakes are recorded by seismographs and occur along faults in the Earth's crust and mantle. It explains that the Earth has an inner core made of hot metals, an outer core made of liquid metals, a mantle below the crust, and a crust that forms the Earth's surface. It also defines a volcano as a mountain with a crater at the top, and explains volcanic eruptions are caused by tectonic plates pulling apart and allow magma, gases, and particles to escape. Finally, it lists the five layers of a volcano as the ash cloud, crater cone, lava, vent, and magma chamber below the surface.
The Sun is a G2V type star made of gas and dust from other stars. It is approximately 4.65 billion years old and has a lifetime of another 5.5 billion years. The Sun has different inner layers including a core with a temperature of 15 million Kelvin, a radiative zone, and a convective zone that moves the Sun's mass. The Sun's surface, called the photosphere, is about 5,800 Kelvin and features solar spots. The Sun's outer atmosphere, the corona, reaches temperatures over 20 million Kelvin and features magnetic coronal loops.
The document discusses the physical structure and properties of the Sun. It describes how the Sun generates energy through nuclear fusion reactions in its core, where hydrogen is fused into helium. This releases energy according to Einstein's equation. It also summarizes the Sun's interior structure, atmosphere, activity cycles, and how observations of neutrinos and vibrations have informed our understanding.
The Sun formed around 5 billion years ago from a cloud of gas and dust. Through the process of nuclear fusion at its core, the Sun generates immense heat and light by converting hydrogen into helium. It is a common yellow star that is part of a cycle that creates convection currents within its surface and sunspots that follow an 11-year cycle. The Sun provides the energy necessary to sustain life on Earth but will eventually exhaust its hydrogen fuel in around 5 billion years.
The sun is a huge glowing ball of gas at the center of our solar system that provides light, heat, and energy to Earth. It is made up primarily of hydrogen and helium and has a radius about 109 times that of Earth. The sun was formed around 4.6 billion years ago and will remain stable for another 5 billion years before expanding into a red giant. It emits electromagnetic radiation across the spectrum, including visible light and infrared that we experience as heat and light. Nuclear fusion in the sun's core converts hydrogen to helium and releases enormous amounts of energy.
The document provides an introduction to stars, focusing on the sun. It discusses the layers of the sun's atmosphere and interior. The sun's core generates its enormous energy output through nuclear fusion. The solar wind consists of high-energy particles escaping the sun's gravity. The sun emits across the electromagnetic spectrum, including x-rays studied by orbital telescopes. The sun's total luminosity is calculated based on the energy received by a detector at Earth's distance. Sunspots occur in pairs of opposite magnetic fields and vary in a roughly 11-year solar cycle.
The sun has a core temperature of 15 million Kelvin and a surface temperature of 9,932 degrees Fahrenheit. It is 4.5 billion years old and will exist in its current form for another 5 billion years before running out of hydrogen. Solar flares are sudden bursts of radiation caused by collisions between magnetic fields on the sun's surface. The sun is the largest mass in the solar system and emits solar wind, which causes phenomena like the Northern Lights and affects spacecraft trajectories.
The Midnight Sun is a phenomenon that allows the sun to be seen at midnight, occurring in Norway between June 21 and December 21 each year. It is caused by Norway's northern latitude location above the Arctic Circle. On clear days, the sun remains visible for a full 24 hours, but overcast conditions can block the Midnight Sun from being seen. Norway is nicknamed "The Land of the Midnight Sun" due to this special event.
Beyond Degrees - Empowering the Workforce in the Context of Skills-First.pptxEduSkills OECD
Iván Bornacelly, Policy Analyst at the OECD Centre for Skills, OECD, presents at the webinar 'Tackling job market gaps with a skills-first approach' on 12 June 2024
🔥🔥🔥🔥🔥🔥🔥🔥🔥
إضغ بين إيديكم من أقوى الملازم التي صممتها
ملزمة تشريح الجهاز الهيكلي (نظري 3)
💀💀💀💀💀💀💀💀💀💀
تتميز هذهِ الملزمة بعِدة مُميزات :
1- مُترجمة ترجمة تُناسب جميع المستويات
2- تحتوي على 78 رسم توضيحي لكل كلمة موجودة بالملزمة (لكل كلمة !!!!)
#فهم_ماكو_درخ
3- دقة الكتابة والصور عالية جداً جداً جداً
4- هُنالك بعض المعلومات تم توضيحها بشكل تفصيلي جداً (تُعتبر لدى الطالب أو الطالبة بإنها معلومات مُبهمة ومع ذلك تم توضيح هذهِ المعلومات المُبهمة بشكل تفصيلي جداً
5- الملزمة تشرح نفسها ب نفسها بس تكلك تعال اقراني
6- تحتوي الملزمة في اول سلايد على خارطة تتضمن جميع تفرُعات معلومات الجهاز الهيكلي المذكورة في هذهِ الملزمة
واخيراً هذهِ الملزمة حلالٌ عليكم وإتمنى منكم إن تدعولي بالخير والصحة والعافية فقط
كل التوفيق زملائي وزميلاتي ، زميلكم محمد الذهبي 💊💊
🔥🔥🔥🔥🔥🔥🔥🔥🔥
Temple of Asclepius in Thrace. Excavation resultsKrassimira Luka
The temple and the sanctuary around were dedicated to Asklepios Zmidrenus. This name has been known since 1875 when an inscription dedicated to him was discovered in Rome. The inscription is dated in 227 AD and was left by soldiers originating from the city of Philippopolis (modern Plovdiv).
A Visual Guide to 1 Samuel | A Tale of Two HeartsSteve Thomason
These slides walk through the story of 1 Samuel. Samuel is the last judge of Israel. The people reject God and want a king. Saul is anointed as the first king, but he is not a good king. David, the shepherd boy is anointed and Saul is envious of him. David shows honor while Saul continues to self destruct.
Chapter wise All Notes of First year Basic Civil Engineering.pptxDenish Jangid
Chapter wise All Notes of First year Basic Civil Engineering
Syllabus
Chapter-1
Introduction to objective, scope and outcome the subject
Chapter 2
Introduction: Scope and Specialization of Civil Engineering, Role of civil Engineer in Society, Impact of infrastructural development on economy of country.
Chapter 3
Surveying: Object Principles & Types of Surveying; Site Plans, Plans & Maps; Scales & Unit of different Measurements.
Linear Measurements: Instruments used. Linear Measurement by Tape, Ranging out Survey Lines and overcoming Obstructions; Measurements on sloping ground; Tape corrections, conventional symbols. Angular Measurements: Instruments used; Introduction to Compass Surveying, Bearings and Longitude & Latitude of a Line, Introduction to total station.
Levelling: Instrument used Object of levelling, Methods of levelling in brief, and Contour maps.
Chapter 4
Buildings: Selection of site for Buildings, Layout of Building Plan, Types of buildings, Plinth area, carpet area, floor space index, Introduction to building byelaws, concept of sun light & ventilation. Components of Buildings & their functions, Basic concept of R.C.C., Introduction to types of foundation
Chapter 5
Transportation: Introduction to Transportation Engineering; Traffic and Road Safety: Types and Characteristics of Various Modes of Transportation; Various Road Traffic Signs, Causes of Accidents and Road Safety Measures.
Chapter 6
Environmental Engineering: Environmental Pollution, Environmental Acts and Regulations, Functional Concepts of Ecology, Basics of Species, Biodiversity, Ecosystem, Hydrological Cycle; Chemical Cycles: Carbon, Nitrogen & Phosphorus; Energy Flow in Ecosystems.
Water Pollution: Water Quality standards, Introduction to Treatment & Disposal of Waste Water. Reuse and Saving of Water, Rain Water Harvesting. Solid Waste Management: Classification of Solid Waste, Collection, Transportation and Disposal of Solid. Recycling of Solid Waste: Energy Recovery, Sanitary Landfill, On-Site Sanitation. Air & Noise Pollution: Primary and Secondary air pollutants, Harmful effects of Air Pollution, Control of Air Pollution. . Noise Pollution Harmful Effects of noise pollution, control of noise pollution, Global warming & Climate Change, Ozone depletion, Greenhouse effect
Text Books:
1. Palancharmy, Basic Civil Engineering, McGraw Hill publishers.
2. Satheesh Gopi, Basic Civil Engineering, Pearson Publishers.
3. Ketki Rangwala Dalal, Essentials of Civil Engineering, Charotar Publishing House.
4. BCP, Surveying volume 1
Leveraging Generative AI to Drive Nonprofit InnovationTechSoup
In this webinar, participants learned how to utilize Generative AI to streamline operations and elevate member engagement. Amazon Web Service experts provided a customer specific use cases and dived into low/no-code tools that are quick and easy to deploy through Amazon Web Service (AWS.)
Andreas Schleicher presents PISA 2022 Volume III - Creative Thinking - 18 Jun...EduSkills OECD
Andreas Schleicher, Director of Education and Skills at the OECD presents at the launch of PISA 2022 Volume III - Creative Minds, Creative Schools on 18 June 2024.
Philippine Edukasyong Pantahanan at Pangkabuhayan (EPP) CurriculumMJDuyan
(𝐓𝐋𝐄 𝟏𝟎𝟎) (𝐋𝐞𝐬𝐬𝐨𝐧 𝟏)-𝐏𝐫𝐞𝐥𝐢𝐦𝐬
𝐃𝐢𝐬𝐜𝐮𝐬𝐬 𝐭𝐡𝐞 𝐄𝐏𝐏 𝐂𝐮𝐫𝐫𝐢𝐜𝐮𝐥𝐮𝐦 𝐢𝐧 𝐭𝐡𝐞 𝐏𝐡𝐢𝐥𝐢𝐩𝐩𝐢𝐧𝐞𝐬:
- Understand the goals and objectives of the Edukasyong Pantahanan at Pangkabuhayan (EPP) curriculum, recognizing its importance in fostering practical life skills and values among students. Students will also be able to identify the key components and subjects covered, such as agriculture, home economics, industrial arts, and information and communication technology.
𝐄𝐱𝐩𝐥𝐚𝐢𝐧 𝐭𝐡𝐞 𝐍𝐚𝐭𝐮𝐫𝐞 𝐚𝐧𝐝 𝐒𝐜𝐨𝐩𝐞 𝐨𝐟 𝐚𝐧 𝐄𝐧𝐭𝐫𝐞𝐩𝐫𝐞𝐧𝐞𝐮𝐫:
-Define entrepreneurship, distinguishing it from general business activities by emphasizing its focus on innovation, risk-taking, and value creation. Students will describe the characteristics and traits of successful entrepreneurs, including their roles and responsibilities, and discuss the broader economic and social impacts of entrepreneurial activities on both local and global scales.
This document provides an overview of wound healing, its functions, stages, mechanisms, factors affecting it, and complications.
A wound is a break in the integrity of the skin or tissues, which may be associated with disruption of the structure and function.
Healing is the body’s response to injury in an attempt to restore normal structure and functions.
Healing can occur in two ways: Regeneration and Repair
There are 4 phases of wound healing: hemostasis, inflammation, proliferation, and remodeling. This document also describes the mechanism of wound healing. Factors that affect healing include infection, uncontrolled diabetes, poor nutrition, age, anemia, the presence of foreign bodies, etc.
Complications of wound healing like infection, hyperpigmentation of scar, contractures, and keloid formation.
2. QUICK TIP
Try right clion a photo
and using "Replace
Image" to build your own
flash cards..
Earth
3.
4. Layers of Earth
The earth is divided into four main layers
1. Inner core
2. Outer core
3. Mantle
4. Crust
5. The Earth’s layers
The earth outermost surface of the
is called crust . The cust is
relatively light and brittle .Most
earthquakes occur within the crust.