Try to sort a series of images to reflect the order of the stages in the life cycle of a star. You know more than you think!
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Meteor Belt, Meteors, Asteroids, Near Earth Objects, Lesson PowerPoint and To...www.sciencepowerpoint.com
This PowerPoint is one small part of the Astronomy Topics unit from www.sciencepowerpoint.com. This unit consists of a five part 3000+ slide PowerPoint roadmap, 12 page bundled homework package, modified homework, detailed answer keys, 8 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 and meaningful. The PowerPoint includes built-in instructions, visuals, and follow up 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, and much more. Also included is a 190 slide first day of school PowerPoint presentation. Teaching Duration = 5+ weeks. Areas of Focus in the Astronomy Topics Unit: The Solar System and the Sun, Order of the Planets, Our Sun, Life Cycle of a Star, Size of Stars, Solar Eclipse, Lunar Eclipse, The Inner Planets, Mercury, Venus, Earth, Moon, Craters, Tides, Phases of the Moon, Mars and Moons, Rocketry, Asteroid Belt, NEOs, The Torino Scale, The Outer Planets and Gas Giants, Jupiter / Moons, Saturn / Moons, Uranus / Moons, Neptune / Moons, Pluto's Demotion, The Kuiper Belt, Oort Cloud, Comets / Other, Beyond the Solar System, Types of Galaxies, Blackholes, Extrasolar Planets, The Big Bang, Dark Matter, Dark Energy, The Special Theory of Relativity, Hubble Space Telescope, Constellations, Spacetime and much more. 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
module 1 electronic structure of matter.pptxMaryroseBudhi1
Module 1: Electronic Structure of Matter
Objectives: Know atom and its sub - particles
determine the characteristics colors that metal salts emit
what is atom?
atom is the basic unit of chemical element
it composes three subatomic particle
proton with a positively electric charge
electron with a negatively electric charge
neutron no electric charge
What minerals produce the color in fireworks?
Mineral elements provide color in fireworks. Barium produces bright greens; strontium yields deep reds;' copper produces blues/ and sodium yields yellow. other colors can be made by mixing elements; strontium and sodium produce brilliant orange; titanium, zirconium, and magnesium alloys make silvery white; copper and strontium make lavender. gold sparks are produced by iron fillings and small pieces of charcoal. bright flashes and loud bangs come from aluminum powder.
Chiotelis Ioannis, Theodoropoulou Maria, “Searching for Black Holes. Photometry in our Classrooms”, Hellenic Conference on Innovating STEM Education, 16-18 December 2016, Athens, Greece.
Meteor Belt, Meteors, Asteroids, Near Earth Objects, Lesson PowerPoint and To...www.sciencepowerpoint.com
This PowerPoint is one small part of the Astronomy Topics unit from www.sciencepowerpoint.com. This unit consists of a five part 3000+ slide PowerPoint roadmap, 12 page bundled homework package, modified homework, detailed answer keys, 8 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 and meaningful. The PowerPoint includes built-in instructions, visuals, and follow up 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, and much more. Also included is a 190 slide first day of school PowerPoint presentation. Teaching Duration = 5+ weeks. Areas of Focus in the Astronomy Topics Unit: The Solar System and the Sun, Order of the Planets, Our Sun, Life Cycle of a Star, Size of Stars, Solar Eclipse, Lunar Eclipse, The Inner Planets, Mercury, Venus, Earth, Moon, Craters, Tides, Phases of the Moon, Mars and Moons, Rocketry, Asteroid Belt, NEOs, The Torino Scale, The Outer Planets and Gas Giants, Jupiter / Moons, Saturn / Moons, Uranus / Moons, Neptune / Moons, Pluto's Demotion, The Kuiper Belt, Oort Cloud, Comets / Other, Beyond the Solar System, Types of Galaxies, Blackholes, Extrasolar Planets, The Big Bang, Dark Matter, Dark Energy, The Special Theory of Relativity, Hubble Space Telescope, Constellations, Spacetime and much more. 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
module 1 electronic structure of matter.pptxMaryroseBudhi1
Module 1: Electronic Structure of Matter
Objectives: Know atom and its sub - particles
determine the characteristics colors that metal salts emit
what is atom?
atom is the basic unit of chemical element
it composes three subatomic particle
proton with a positively electric charge
electron with a negatively electric charge
neutron no electric charge
What minerals produce the color in fireworks?
Mineral elements provide color in fireworks. Barium produces bright greens; strontium yields deep reds;' copper produces blues/ and sodium yields yellow. other colors can be made by mixing elements; strontium and sodium produce brilliant orange; titanium, zirconium, and magnesium alloys make silvery white; copper and strontium make lavender. gold sparks are produced by iron fillings and small pieces of charcoal. bright flashes and loud bangs come from aluminum powder.
Chiotelis Ioannis, Theodoropoulou Maria, “Searching for Black Holes. Photometry in our Classrooms”, Hellenic Conference on Innovating STEM Education, 16-18 December 2016, Athens, Greece.
Since NASA launched its Hubble Space Telescope in 1990, space scientists at the University of Arizona in Tucson have used it to expand our knowledge of the Universe time and time again.
Sometimes taking a moment to appreciate the beauty, awesomeness and complexity of creation can reconnect us with our Creator and deepen our faith. We invite you to view our latest slideshow “God of All Creation” full of breathtaking images from space.
This is a 2024 NASA Calendar . This has information such as Rear Admiral Evelyn Fields is the first woman and first African American to lead
the NOAA Commissioned Officer Corps, which is one of the nation’s eight uniformed
services. Fields began her career at NOAA as a cartographer in 1972, only two years
after the agency formed. Less than a year later, the NOAA Corps began accepting
women into its commissioned officer ranks, and she became the first African American
woman to join. Fields became a rear admiral and director of both NOAA Corps
and the Office of Marine and Aviation Operations in 1999. She is the first woman
to become a NOAA Corps rear admiral. Fields retired in late 2003. Photo credit:
NOAA/Military Officer Association of America and Dr. Eric Cornell is a co-principal investigator on NASA’s Cold Atom Lab and
a fellow at JILA, a joint institute between the National Institute of Standards
and Technology (NIST) and the University of Colorado Boulder. His research
focuses on ultracold atoms and on precision metrology (the scientific study
of measurement) in the service of fundamental physics. Along with Dr. Carl
Wieman and Dr. Wolfgang Ketterle, he was awarded the 2001 Nobel Prize for
the first experimental realization of a Bose-Einstein condensate—a fifth state of
matter first predicted in 1917. Today, the techniques that Cornell helped develop
for cooling atoms to ultracold temperatures are used in laboratories around the
world and on the International Space Station by the Cold Atom Lab. Photo credit:
University of Colorado Boulder
“To what extent has the Modern Revolution been a positive or a negative force?” is the driving question for Unit 9. The purpose of this activity is to apply Unit 9’s driving question
to a modern-day infrastructure development: the Interoceanic Highway (La Carretera). Construction on La Carretera, which connects the east and west coasts of South America, began in the early twenty-first century. By studying the scenes depicted in a photojournalist’s photographic essay, students will come to their own conclusions about the extent to which this road has been a positive or negative force as related to certain trends and topics (economic development and natural environment, for example). This activity will also help prepare students for Investigation 9, in which they’re asked to identify good and bad outcomes of trends referenced in the Investigation texts.
This activity will give students a chance to review some of what they learned in this lesson, and use it to think more deeply about what and how they would communicate with an alien species.
Register to explore the whole course here: https://school.bighistoryproject.com/bhplive?WT.mc_id=Slideshare12202017
Circling one star among hundreds of billions, in one galaxy among a hundred billion more, in a Universe that is vast and expanding ever faster – perhaps toward infinity. It’s easy to forget that we live in a place of astonishing grandeur and mystery.
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Unit 9: Comparing the Costs of Renewable and Conventional Energy SourcesBig History Project
You can’t get too far in a discussion about the nation’s electric power sector without running into the question of costs.
Register to explore the whole course here: https://school.bighistoryproject.com/bhplive?WT.mc_id=Slideshare12202017
This quick activity will get students brainstorming about life on Mars and what they would need to survive there.
Register to explore the whole course here: https://school.bighistoryproject.com/bhplive?WT.mc_id=Slideshare12202017
Use www.gapminder.org/data to fill out the data in each of the tables below. To find the data you need, make sure that you have the name of the category. On the gapminder.org/data page, you’ll see a table called “List of indicators in “Gapminder World.” Beneath that title, on the right side of the table, find the
Search box. Type the name of the category into that search area. Once you find the category, click on the magnifying glass on the right. That link will have the data you need to fill out each of the tables below.
Register to explore the whole course here: https://school.bighistoryproject.com/bhplive?WT.mc_id=Slideshare12202017
Spanning three centuries of history, from the dawn of the industrial age to modern times, three diverse
thinkers developed their own landmark theories on commerce, labor, and the global economy.
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In the final essay of a four-part series, David Christian explains
how advances in communication and transportation accelerated
collective learning.
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Lesson 9.2 Activity: The Impact of Population Growth EssayBig History Project
For this closing activity, students will construct an essay in which they discuss what they think are the three biggest impacts of human population growth in the modern era. By looking more closely at population growth, they will deepen their understanding of the impact of acceleration and will think about themselves in relation to population growth and the effect it might have on their own futures.
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Unit 8: Guns, Germs, and Steel: The Fates of Human SocietiesBig History Project
Jared Mason Diamond (1937 — ) is an American scientist and author whose work draws from a variety of fields. He is currently a professor of geography and of physiology at UCLA. His 1997 book, Guns, Germs, and Steel: The Fates of Human
Societies, from which the following passages are excerpted, won the 1998 Pulitzer Prize for general nonfiction and the Aventis Prize for Best Science Book. The basic premise of the book is to explain why Eurasian civilizations have survived
and conquered others, while refuting the idea that Eurasian hegemony is due to intellectual, moral, or genetic superiority.
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Making comparisons is an important intellectual tool for all people and especially for historians and scientists. Historians, in particular, make comparisons across time to understand what
has changed and what has remained constant. This question looks at the spread of plague and our collective reaction to plague at two different times in human history—the fourteenth century and the nineteenth century. Such a comparison enables us to see clearly how we have changed.
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Lesson 8.3 Activity: Revising Investigation Writing - Sentence Starters Part 2Big History Project
Students have examined and revised an Investigation writing sample based on Criteria A, B, and C of the rubric. Now, they’ll undergo the same process with a peer essay. In addition, they’ll do this alone instead of in groups. So, although the process is the same as in the last Investigation writing activity, this one might be more difficult since students will move away from group work and will complete this worksheet on their own. However, it’s important for students to be able to accomplish this exercise on their own since in the next lesson, they’ll apply this same process to their own writing. Again, while the categories in the rubric are a useful tool for initially understanding the different elements of writing, they need to be looked at as a whole since the areas of focus are interrelated.
Register to explore the whole course here: https://school.bighistoryproject.com/bhplive?WT.mc_id=Slideshare12202017
Unit 8: When Humans Became Inhumane: The Atlantic Slave TradeBig History Project
Once Europeans had figured out how to be effective middlemen — buying and selling silver, tea, and fur, they turned to figuring out how to also become producers of the commodities they were trading.
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Unit 8: Investigating the Consequences of the Columbian ExchangeBig History Project
A new era in human history began in 1492 as the four world zones became connected. For the first time, humans created truly global networks.
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The account of the travels of the Muslim legal scholar Ibn Battuta in the first half of the fourteenth century reveals the wide scope of the Muslim world at that time.
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This collection of biographies provides students with detailed information about the voyages of these explorers including information about their motivation and how they inspired future generations of explorers. These men opened the door to a more interconnected world as the contacts they made helped to create connections between distant peoples and stimulate the growth of exchange networks and long-distance trade.
Register to explore the whole course here: https://school.bighistoryproject.com/bhplive?WT.mc_id=Slideshare12202017
Lesson 7.2 Activity: Essay - Were They Pushed or Did They Jump?Big History Project
You’re going to pick a civilization you’ve already researched, and then use the information from your Early Civilizations Museum Project, your Comparing More Civilizations Worksheet, and your Rise, Fall, and Collapse of Civilizations Worksheet to write a five-paragraph essay about whether that civilization was pushed (external forces were the main cause of its downfall) or it jumped (something internal was responsible—they were their own worst enemy). A “pushed” example: Two empires went to war. You might say the winning empire “pushed” the losing empire into collapse. An example of a civilization having “jumped” can be found in the Easter Island Activity earlier in the course: One of the theories for the collapse of Easter Island is that the inhabitants depleted the natural resources they needed to survive. The people were, in a sense, the cause of their own destruction—they “jumped.”
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Lesson 7.2 Activity: Social Status, Power, and Human BurialsBig History Project
This activity provides students with an opportunity to start thinking about the impact that farming can have on the way humans live and relate to each other. It will also allow them to think about the kinds of questions archaeologists and historians might ask when they must rely upon artifacts rather than written evidence to learn about the past.
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Unit 7: Greco-Roman: Early Experiments in Participatory GovernmentBig History Project
Instead of rule by a single person, Athens and Rome developed governments with widespread participation by male elites, which lasted about 170 years in Athens and 480 years in Rome.
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During the same narrow sliver of cosmic time, cities, states, and civilizations emerged independentlyin several places around the world.
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Instructions for Submissions thorugh G- Classroom.pptxJheel Barad
This presentation provides a briefing on how to upload submissions and documents in Google Classroom. It was prepared as part of an orientation for new Sainik School in-service teacher trainees. As a training officer, my goal is to ensure that you are comfortable and proficient with this essential tool for managing assignments and fostering student engagement.
2024.06.01 Introducing a competency framework for languag learning materials ...Sandy Millin
http://sandymillin.wordpress.com/iateflwebinar2024
Published classroom materials form the basis of syllabuses, drive teacher professional development, and have a potentially huge influence on learners, teachers and education systems. All teachers also create their own materials, whether a few sentences on a blackboard, a highly-structured fully-realised online course, or anything in between. Despite this, the knowledge and skills needed to create effective language learning materials are rarely part of teacher training, and are mostly learnt by trial and error.
Knowledge and skills frameworks, generally called competency frameworks, for ELT teachers, trainers and managers have existed for a few years now. However, until I created one for my MA dissertation, there wasn’t one drawing together what we need to know and do to be able to effectively produce language learning materials.
This webinar will introduce you to my framework, highlighting the key competencies I identified from my research. It will also show how anybody involved in language teaching (any language, not just English!), teacher training, managing schools or developing language learning materials can benefit from using the framework.
A Strategic Approach: GenAI in EducationPeter Windle
Artificial Intelligence (AI) technologies such as Generative AI, Image Generators and Large Language Models have had a dramatic impact on teaching, learning and assessment over the past 18 months. The most immediate threat AI posed was to Academic Integrity with Higher Education Institutes (HEIs) focusing their efforts on combating the use of GenAI in assessment. Guidelines were developed for staff and students, policies put in place too. Innovative educators have forged paths in the use of Generative AI for teaching, learning and assessments leading to pockets of transformation springing up across HEIs, often with little or no top-down guidance, support or direction.
This Gasta posits a strategic approach to integrating AI into HEIs to prepare staff, students and the curriculum for an evolving world and workplace. We will highlight the advantages of working with these technologies beyond the realm of teaching, learning and assessment by considering prompt engineering skills, industry impact, curriculum changes, and the need for staff upskilling. In contrast, not engaging strategically with Generative AI poses risks, including falling behind peers, missed opportunities and failing to ensure our graduates remain employable. The rapid evolution of AI technologies necessitates a proactive and strategic approach if we are to remain relevant.
Biological screening of herbal drugs: Introduction and Need for
Phyto-Pharmacological Screening, New Strategies for evaluating
Natural Products, In vitro evaluation techniques for Antioxidants, Antimicrobial and Anticancer drugs. In vivo evaluation techniques
for Anti-inflammatory, Antiulcer, Anticancer, Wound healing, Antidiabetic, Hepatoprotective, Cardio protective, Diuretics and
Antifertility, Toxicity studies as per OECD guidelines
Introduction to AI for Nonprofits with Tapp NetworkTechSoup
Dive into the world of AI! Experts Jon Hill and Tareq Monaur will guide you through AI's role in enhancing nonprofit websites and basic marketing strategies, making it easy to understand and apply.
Welcome to TechSoup New Member Orientation and Q&A (May 2024).pdfTechSoup
In this webinar you will learn how your organization can access TechSoup's wide variety of product discount and donation programs. From hardware to software, we'll give you a tour of the tools available to help your nonprofit with productivity, collaboration, financial management, donor tracking, security, and more.
The Roman Empire A Historical Colossus.pdfkaushalkr1407
The Roman Empire, a vast and enduring power, stands as one of history's most remarkable civilizations, leaving an indelible imprint on the world. It emerged from the Roman Republic, transitioning into an imperial powerhouse under the leadership of Augustus Caesar in 27 BCE. This transformation marked the beginning of an era defined by unprecedented territorial expansion, architectural marvels, and profound cultural influence.
The empire's roots lie in the city of Rome, founded, according to legend, by Romulus in 753 BCE. Over centuries, Rome evolved from a small settlement to a formidable republic, characterized by a complex political system with elected officials and checks on power. However, internal strife, class conflicts, and military ambitions paved the way for the end of the Republic. Julius Caesar’s dictatorship and subsequent assassination in 44 BCE created a power vacuum, leading to a civil war. Octavian, later Augustus, emerged victorious, heralding the Roman Empire’s birth.
Under Augustus, the empire experienced the Pax Romana, a 200-year period of relative peace and stability. Augustus reformed the military, established efficient administrative systems, and initiated grand construction projects. The empire's borders expanded, encompassing territories from Britain to Egypt and from Spain to the Euphrates. Roman legions, renowned for their discipline and engineering prowess, secured and maintained these vast territories, building roads, fortifications, and cities that facilitated control and integration.
The Roman Empire’s society was hierarchical, with a rigid class system. At the top were the patricians, wealthy elites who held significant political power. Below them were the plebeians, free citizens with limited political influence, and the vast numbers of slaves who formed the backbone of the economy. The family unit was central, governed by the paterfamilias, the male head who held absolute authority.
Culturally, the Romans were eclectic, absorbing and adapting elements from the civilizations they encountered, particularly the Greeks. Roman art, literature, and philosophy reflected this synthesis, creating a rich cultural tapestry. Latin, the Roman language, became the lingua franca of the Western world, influencing numerous modern languages.
Roman architecture and engineering achievements were monumental. They perfected the arch, vault, and dome, constructing enduring structures like the Colosseum, Pantheon, and aqueducts. These engineering marvels not only showcased Roman ingenuity but also served practical purposes, from public entertainment to water supply.
1. STUDENT MATERIALS
Name: Date:
BIG HISTORY PROJECT / LESSON 3.0
LIFE OF A STAR WORKSHEET
Directions: Place the images in the correct order from the birth of a star to its death. Briefly describe what stage in the lifecycle of a star is represented in each
image.
1.
2.
3.
4.
A B C D
Sources: Credit: O. Krause (Steward Obs.) et al., SSC, JPL, Caltech, NASA; Credit: Daniel Huber, University of Sydney; Credit: DG Tau artist’s conception, W.M Keck Observatory; Credit: EIT - SOHO Consortium, ESA, NASA
2. TEACHER MATERIALS
BIG HISTORY PROJECT / LESSON 3.0
LIFE OF A STAR WORKSHEET (answer key)
Directions: Place the images in the correct order from the birth of a star to its death. Briefly describe what stage in the lifecycle of a star is represented in each
image.
C D B A
1. = C - Protostar - A star that has not yet reached the fusion stage. It grows by accretion, acquiring mass from surrounding interstellar dust and gas.
2. = D - Star - The star shines as nuclear reactions inside produce light and heat. The vast majority of stars in the Universe are in this stage, including our Sun.
3. = B - Red Giant - The star expands and glows red as it cools, eventually blasting away its outer layers.
4. = A - Supernova Remnant - The result of an explosion of a star; consists of material ejected from the explosion. Only the most massive stars become supernovae.
Sources: Credit: A - O. Krause (Steward Obs.) et al., SSC, JPL, Caltech, NASA; B - Credit: Daniel Huber, University of Sydney; Credit: C - DG Tau artist’s conception, W.M Keck Observatory; D - Credit: EIT - SOHO Consortium,
ESA, NASA