The document discusses the Doppler effect, which is a change in frequency of waves observed by a detector as the source of the waves moves relative to the detector. It was first proposed by Christian Doppler in 1842 to explain the phenomenon for sound waves. The frequency observed is higher when the source approaches and lower when it recedes. Examples given include ambulance sirens, airplanes, and ducks swimming in water. The Doppler effect is applied in radar guns and explains the redshift of light from distant galaxies.
Space research involves scientific studies carried out in outer space using specialized equipment. It began in earnest in the mid-20th century as rockets were developed that could overcome Earth's gravity. Some key early milestones included the first artificial object in space in 1944, the detection of the Van Allen radiation belts in 1958, and the first photos of the far side of the Moon in 1959. In the 1960s, important firsts included the first animal and first human, Yuri Gagarin, in space. Ongoing space research through the late 20th and early 21st centuries has involved missions to planets, asteroids, and other celestial bodies to learn more about the solar system and expand scientific knowledge.
This document outlines the key steps in conducting research projects in secondary school: 1) selecting a precise and specific topic involving variables, 2) conducting a bibliographical search of libraries and databases to gather information, 3) defining clear objectives and hypotheses, 4) designing a methodology with independent, dependent, and controlled variables, 5) gathering and analyzing data, and 6) writing a report that introduces the topic, methodology, analysis, and conclusions.
This document discusses the field of space research. It covers the history of space research starting in the 20th century with rockets used by China and the space race between the US and USSR. Key areas of space research are explored using satellites and space stations to study topics like Earth observations, astronomy, and life sciences. Methods of potential faster-than-light travel are also mentioned.
Newton’s laws physics and chemistry 4ºAjuanalcar332
Isaac Newton was an influential English scientist born in 1642 who made fundamental contributions to physics, including establishing the laws of motion and universal gravitation. He formulated laws of motion and universal gravitation, published in his work "Philosophiæ Naturalis Principia Mathematica", demonstrating that the motions of celestial bodies and objects on Earth could be explained by the same principles. Newton also made advances in optics and mathematics, developing calculus independently of Gottfried Leibniz. His work was revolutionary and had a major impact on scientific thought.
Nicolaus Copernicus was a Polish astronomer who proposed the heliocentric model in the early 16th century, placing the Sun at the center of the universe rather than the Earth. He studied mathematics and astronomy at the University of Cracow and later held a position as a canon at Frombork Cathedral, which allowed him time for his astronomical research. His heliocentric theory challenged the geocentric Ptolemaic model that had been dominant for over 1,000 years, and it took some time for his ideas to gain acceptance due to conflicts with the dominant religious authorities of the time.
This document discusses satellites and spacecraft. It describes the first satellites Sputnik 1 and Sputnik 2, and the types of artificial satellites which include navigation, communication, and weather satellites. It also outlines the types of spacecraft such as flyby, orbiter, lander, and rover spacecraft. While there is no technical difference, a spacecraft is considered a satellite when it is placed in orbit around an astronomical object.
This document provides an overview of gravitation and cosmology. It first defines gravitation as the natural phenomenon by which all things with mass are attracted to one another, and summarizes Newton's theory of gravitation. It then defines cosmology as the study of the origin and evolution of the universe from the Big Bang to present and future times. The document also mentions it will discuss the history of cosmology and different types of cosmological models.
The document discusses the Doppler effect, which is a change in frequency of waves observed by a detector as the source of the waves moves relative to the detector. It was first proposed by Christian Doppler in 1842 to explain the phenomenon for sound waves. The frequency observed is higher when the source approaches and lower when it recedes. Examples given include ambulance sirens, airplanes, and ducks swimming in water. The Doppler effect is applied in radar guns and explains the redshift of light from distant galaxies.
Space research involves scientific studies carried out in outer space using specialized equipment. It began in earnest in the mid-20th century as rockets were developed that could overcome Earth's gravity. Some key early milestones included the first artificial object in space in 1944, the detection of the Van Allen radiation belts in 1958, and the first photos of the far side of the Moon in 1959. In the 1960s, important firsts included the first animal and first human, Yuri Gagarin, in space. Ongoing space research through the late 20th and early 21st centuries has involved missions to planets, asteroids, and other celestial bodies to learn more about the solar system and expand scientific knowledge.
This document outlines the key steps in conducting research projects in secondary school: 1) selecting a precise and specific topic involving variables, 2) conducting a bibliographical search of libraries and databases to gather information, 3) defining clear objectives and hypotheses, 4) designing a methodology with independent, dependent, and controlled variables, 5) gathering and analyzing data, and 6) writing a report that introduces the topic, methodology, analysis, and conclusions.
This document discusses the field of space research. It covers the history of space research starting in the 20th century with rockets used by China and the space race between the US and USSR. Key areas of space research are explored using satellites and space stations to study topics like Earth observations, astronomy, and life sciences. Methods of potential faster-than-light travel are also mentioned.
Newton’s laws physics and chemistry 4ºAjuanalcar332
Isaac Newton was an influential English scientist born in 1642 who made fundamental contributions to physics, including establishing the laws of motion and universal gravitation. He formulated laws of motion and universal gravitation, published in his work "Philosophiæ Naturalis Principia Mathematica", demonstrating that the motions of celestial bodies and objects on Earth could be explained by the same principles. Newton also made advances in optics and mathematics, developing calculus independently of Gottfried Leibniz. His work was revolutionary and had a major impact on scientific thought.
Nicolaus Copernicus was a Polish astronomer who proposed the heliocentric model in the early 16th century, placing the Sun at the center of the universe rather than the Earth. He studied mathematics and astronomy at the University of Cracow and later held a position as a canon at Frombork Cathedral, which allowed him time for his astronomical research. His heliocentric theory challenged the geocentric Ptolemaic model that had been dominant for over 1,000 years, and it took some time for his ideas to gain acceptance due to conflicts with the dominant religious authorities of the time.
This document discusses satellites and spacecraft. It describes the first satellites Sputnik 1 and Sputnik 2, and the types of artificial satellites which include navigation, communication, and weather satellites. It also outlines the types of spacecraft such as flyby, orbiter, lander, and rover spacecraft. While there is no technical difference, a spacecraft is considered a satellite when it is placed in orbit around an astronomical object.
This document provides an overview of gravitation and cosmology. It first defines gravitation as the natural phenomenon by which all things with mass are attracted to one another, and summarizes Newton's theory of gravitation. It then defines cosmology as the study of the origin and evolution of the universe from the Big Bang to present and future times. The document also mentions it will discuss the history of cosmology and different types of cosmological models.
The document discusses the Doppler effect and how it provides evidence for the Big Bang theory. It explains that the Doppler effect is when the frequency of a wave changes depending on whether the source of the wave is moving towards or away from an observer. It then asks what would happen to sound waves in front of and behind a moving object compared to a stationary object. Finally, it notes that the Doppler effect can cause absorption lines in spectra to shift towards the red or blue side when observing celestial objects, providing evidence that the universe is expanding.
This document discusses Kepler's laws of planetary motion. Kepler believed in the Copernican heliocentric model but could not ignore Tycho Brahe's geocentric model. When Kepler obtained Brahe's observational data on Mars, he realized planetary orbits were elliptical rather than circular. Kepler's first law states that planets move in elliptical orbits with the Sun at one focus. His second law concerns the speed of a planet as it sweeps out equal areas in equal times. Kepler's third law relates the orbital period of a planet to the semi-major axis of its orbit.
Dark matter makes up 27% of the universe, is an unidentified type of non-baryonic matter that does not interact with light but has gravitational effects. It cannot be detected with current instruments. Dark energy affects the expansion of the universe and makes up 68% of the universe, but is still a mystery. Early theorists like Fritz Zwicky and Vera Rubin provided evidence for dark matter through its gravitational effects on galaxy clusters and violations of Newton's laws of motion.
The Doppler effect is the apparent change in frequency of a wave due to relative motion between the source and observer. It has applications including determining the velocity of moving objects, discovering Saturn's rings and the spin of the sun, and detecting binary stars and whether stars are moving toward or away from Earth. An example calculation shows an increase in observed sound frequency when a source emitting 1600Hz sound waves approaches an observer at 80m/s.
Giant molecular clouds collapse under gravity to form protostars that grow into main sequence stars through nuclear fusion. As stars age, they expand into red giants and shed their outer layers, leaving behind white dwarfs that slowly cool over billions of years. More massive stars have shorter lifespans and die in spectacular supernovae, potentially leaving behind neutron stars or black holes.
Dark matter is invisible matter that accounts for approximately 27% of the mass-energy in the universe. Although it cannot be directly observed, astronomers deduce its existence through its gravitational effects, such as the anomalous rotation curves of galaxies. Dark matter is classified as cold, warm, or hot depending on the size of protogalaxies, and may consist of either baryonic matter like protons and neutrons or nonbaryonic particles like axions. It plays a prominent role in science fiction works but descriptions are often inconsistent with scientific understanding.
Stars are born when a nebula contracts and forms a protostar. Most stars spend about 90% of their lifetime on the main sequence fusing hydrogen into helium. Later in their lives, stars grow into red giants and then supergiants as they fuse heavier elements. When stars die, they expel their outer layers as planetary nebulae, leaving behind dense white dwarfs, neutron stars, or black holes depending on their original mass.
Black holes are regions of spacetime where gravity is so strong that nothing, not even light, can escape. They are defined by an event horizon surrounding a singularity of unknown composition. There are three main types - stellar black holes formed by collapsed stars, supermassive black holes found at the center of galaxies, and primordial black holes theorized to have formed in the early universe. Black holes vary greatly in size from 10 to 100 solar masses for stellar black holes up to billions of solar masses for supermassive black holes located in galaxies.
This document provides an overview of the solar system, including its formation over 4.6 billion years ago with one star (the Sun) and eight known planets along with hundreds of smaller planets and asteroids. It describes each planet's key characteristics such as Mercury being the smallest terrestrial planet with no atmosphere or moons. Earth is the only planet that supports life and has one moon, while Mars has a thin atmosphere and two small moons. The outer gas giants include Jupiter, the largest planet composed primarily of hydrogen and helium, Saturn with its prominent ring system and 62 moons, Uranus which was discovered in the 19th century and rotates parallel to the solar plane, and Neptune with its blue atmosphere due to methane
Nicolaus Copernicus developed the heliocentric theory that the sun, not the earth, is at the center of our solar system. This contradicted the prevailing geocentric view of Ptolemy that the earth is the center. Copernicus published his theory in 1543, noting the sun is stationary and the earth and planets revolve around it. His work helped initiate the Copernican revolution and shifted the view of astronomy and humanity's place in the universe, though his model was later refined by scientists like Galileo and Kepler.
The document discusses the Big Bang theory, which proposes that the universe began approximately 13.8 billion years ago from an extremely dense and hot state and has been expanding and cooling ever since. It provides an overview of the theory's history, key scientists like Friedman, Lemaître and Hubble who contributed to its development, and major evidence that supports it, including cosmic microwave background radiation, the abundance of light elements, and the observable expansion of the universe. The document also notes there were four fundamental forces in the early universe and that the theory was named by Fred Hoyle in 1950.
Black holes are celestial objects with immense gravitational pull that not even light can escape. They are classified by size into primordial, stellar, and supermassive black holes. Black holes form through supernovae or the gravitational collapse of matter in the early universe. Key components include the singularity at the center, the event horizon boundary, and accretion disks of orbiting material. Theories explore phenomena like wormholes, the grandfather paradox in time travel, and the Novikov self-consistency principle governing causality near black holes. Astronomers detect black holes indirectly through their effects on nearby objects.
it describes the bony anatomy including the femoral head , acetabulum, labrum . also discusses the capsule , ligaments . muscle that act on the hip joint and the range of motion are outlined. factors affecting hip joint stability and weight transmission through the joint are summarized.
How to Make a Field Mandatory in Odoo 17Celine George
In Odoo, making a field required can be done through both Python code and XML views. When you set the required attribute to True in Python code, it makes the field required across all views where it's used. Conversely, when you set the required attribute in XML views, it makes the field required only in the context of that particular view.
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
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.)
Communicating effectively and consistently with students can help them feel at ease during their learning experience and provide the instructor with a communication trail to track the course's progress. This workshop will take you through constructing an engaging course container to facilitate effective communication.
The document discusses the Doppler effect and how it provides evidence for the Big Bang theory. It explains that the Doppler effect is when the frequency of a wave changes depending on whether the source of the wave is moving towards or away from an observer. It then asks what would happen to sound waves in front of and behind a moving object compared to a stationary object. Finally, it notes that the Doppler effect can cause absorption lines in spectra to shift towards the red or blue side when observing celestial objects, providing evidence that the universe is expanding.
This document discusses Kepler's laws of planetary motion. Kepler believed in the Copernican heliocentric model but could not ignore Tycho Brahe's geocentric model. When Kepler obtained Brahe's observational data on Mars, he realized planetary orbits were elliptical rather than circular. Kepler's first law states that planets move in elliptical orbits with the Sun at one focus. His second law concerns the speed of a planet as it sweeps out equal areas in equal times. Kepler's third law relates the orbital period of a planet to the semi-major axis of its orbit.
Dark matter makes up 27% of the universe, is an unidentified type of non-baryonic matter that does not interact with light but has gravitational effects. It cannot be detected with current instruments. Dark energy affects the expansion of the universe and makes up 68% of the universe, but is still a mystery. Early theorists like Fritz Zwicky and Vera Rubin provided evidence for dark matter through its gravitational effects on galaxy clusters and violations of Newton's laws of motion.
The Doppler effect is the apparent change in frequency of a wave due to relative motion between the source and observer. It has applications including determining the velocity of moving objects, discovering Saturn's rings and the spin of the sun, and detecting binary stars and whether stars are moving toward or away from Earth. An example calculation shows an increase in observed sound frequency when a source emitting 1600Hz sound waves approaches an observer at 80m/s.
Giant molecular clouds collapse under gravity to form protostars that grow into main sequence stars through nuclear fusion. As stars age, they expand into red giants and shed their outer layers, leaving behind white dwarfs that slowly cool over billions of years. More massive stars have shorter lifespans and die in spectacular supernovae, potentially leaving behind neutron stars or black holes.
Dark matter is invisible matter that accounts for approximately 27% of the mass-energy in the universe. Although it cannot be directly observed, astronomers deduce its existence through its gravitational effects, such as the anomalous rotation curves of galaxies. Dark matter is classified as cold, warm, or hot depending on the size of protogalaxies, and may consist of either baryonic matter like protons and neutrons or nonbaryonic particles like axions. It plays a prominent role in science fiction works but descriptions are often inconsistent with scientific understanding.
Stars are born when a nebula contracts and forms a protostar. Most stars spend about 90% of their lifetime on the main sequence fusing hydrogen into helium. Later in their lives, stars grow into red giants and then supergiants as they fuse heavier elements. When stars die, they expel their outer layers as planetary nebulae, leaving behind dense white dwarfs, neutron stars, or black holes depending on their original mass.
Black holes are regions of spacetime where gravity is so strong that nothing, not even light, can escape. They are defined by an event horizon surrounding a singularity of unknown composition. There are three main types - stellar black holes formed by collapsed stars, supermassive black holes found at the center of galaxies, and primordial black holes theorized to have formed in the early universe. Black holes vary greatly in size from 10 to 100 solar masses for stellar black holes up to billions of solar masses for supermassive black holes located in galaxies.
This document provides an overview of the solar system, including its formation over 4.6 billion years ago with one star (the Sun) and eight known planets along with hundreds of smaller planets and asteroids. It describes each planet's key characteristics such as Mercury being the smallest terrestrial planet with no atmosphere or moons. Earth is the only planet that supports life and has one moon, while Mars has a thin atmosphere and two small moons. The outer gas giants include Jupiter, the largest planet composed primarily of hydrogen and helium, Saturn with its prominent ring system and 62 moons, Uranus which was discovered in the 19th century and rotates parallel to the solar plane, and Neptune with its blue atmosphere due to methane
Nicolaus Copernicus developed the heliocentric theory that the sun, not the earth, is at the center of our solar system. This contradicted the prevailing geocentric view of Ptolemy that the earth is the center. Copernicus published his theory in 1543, noting the sun is stationary and the earth and planets revolve around it. His work helped initiate the Copernican revolution and shifted the view of astronomy and humanity's place in the universe, though his model was later refined by scientists like Galileo and Kepler.
The document discusses the Big Bang theory, which proposes that the universe began approximately 13.8 billion years ago from an extremely dense and hot state and has been expanding and cooling ever since. It provides an overview of the theory's history, key scientists like Friedman, Lemaître and Hubble who contributed to its development, and major evidence that supports it, including cosmic microwave background radiation, the abundance of light elements, and the observable expansion of the universe. The document also notes there were four fundamental forces in the early universe and that the theory was named by Fred Hoyle in 1950.
Black holes are celestial objects with immense gravitational pull that not even light can escape. They are classified by size into primordial, stellar, and supermassive black holes. Black holes form through supernovae or the gravitational collapse of matter in the early universe. Key components include the singularity at the center, the event horizon boundary, and accretion disks of orbiting material. Theories explore phenomena like wormholes, the grandfather paradox in time travel, and the Novikov self-consistency principle governing causality near black holes. Astronomers detect black holes indirectly through their effects on nearby objects.
it describes the bony anatomy including the femoral head , acetabulum, labrum . also discusses the capsule , ligaments . muscle that act on the hip joint and the range of motion are outlined. factors affecting hip joint stability and weight transmission through the joint are summarized.
How to Make a Field Mandatory in Odoo 17Celine George
In Odoo, making a field required can be done through both Python code and XML views. When you set the required attribute to True in Python code, it makes the field required across all views where it's used. Conversely, when you set the required attribute in XML views, it makes the field required only in the context of that particular view.
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
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.)
Communicating effectively and consistently with students can help them feel at ease during their learning experience and provide the instructor with a communication trail to track the course's progress. This workshop will take you through constructing an engaging course container to facilitate effective communication.
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
Main Java[All of the Base Concepts}.docxadhitya5119
This is part 1 of my Java Learning Journey. This Contains Custom methods, classes, constructors, packages, multithreading , try- catch block, finally block and more.
বাংলাদেশের অর্থনৈতিক সমীক্ষা ২০২৪ [Bangladesh Economic Review 2024 Bangla.pdf] কম্পিউটার , ট্যাব ও স্মার্ট ফোন ভার্সন সহ সম্পূর্ণ বাংলা ই-বুক বা pdf বই " সুচিপত্র ...বুকমার্ক মেনু 🔖 ও হাইপার লিংক মেনু 📝👆 যুক্ত ..
আমাদের সবার জন্য খুব খুব গুরুত্বপূর্ণ একটি বই ..বিসিএস, ব্যাংক, ইউনিভার্সিটি ভর্তি ও যে কোন প্রতিযোগিতা মূলক পরীক্ষার জন্য এর খুব ইম্পরট্যান্ট একটি বিষয় ...তাছাড়া বাংলাদেশের সাম্প্রতিক যে কোন ডাটা বা তথ্য এই বইতে পাবেন ...
তাই একজন নাগরিক হিসাবে এই তথ্য গুলো আপনার জানা প্রয়োজন ...।
বিসিএস ও ব্যাংক এর লিখিত পরীক্ষা ...+এছাড়া মাধ্যমিক ও উচ্চমাধ্যমিকের স্টুডেন্টদের জন্য অনেক কাজে আসবে ...
ISO/IEC 27001, ISO/IEC 42001, and GDPR: Best Practices for Implementation and...PECB
Denis is a dynamic and results-driven Chief Information Officer (CIO) with a distinguished career spanning information systems analysis and technical project management. With a proven track record of spearheading the design and delivery of cutting-edge Information Management solutions, he has consistently elevated business operations, streamlined reporting functions, and maximized process efficiency.
Certified as an ISO/IEC 27001: Information Security Management Systems (ISMS) Lead Implementer, Data Protection Officer, and Cyber Risks Analyst, Denis brings a heightened focus on data security, privacy, and cyber resilience to every endeavor.
His expertise extends across a diverse spectrum of reporting, database, and web development applications, underpinned by an exceptional grasp of data storage and virtualization technologies. His proficiency in application testing, database administration, and data cleansing ensures seamless execution of complex projects.
What sets Denis apart is his comprehensive understanding of Business and Systems Analysis technologies, honed through involvement in all phases of the Software Development Lifecycle (SDLC). From meticulous requirements gathering to precise analysis, innovative design, rigorous development, thorough testing, and successful implementation, he has consistently delivered exceptional results.
Throughout his career, he has taken on multifaceted roles, from leading technical project management teams to owning solutions that drive operational excellence. His conscientious and proactive approach is unwavering, whether he is working independently or collaboratively within a team. His ability to connect with colleagues on a personal level underscores his commitment to fostering a harmonious and productive workplace environment.
Date: May 29, 2024
Tags: Information Security, ISO/IEC 27001, ISO/IEC 42001, Artificial Intelligence, GDPR
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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.