The document discusses facts about the Earth and the Moon. It begins by providing basic information about the spherical shape and orbital movement of the Earth, and its rotation on its axis that causes the day-night cycle. It then discusses details about the Moon, including that it is Earth's only natural satellite, its composition of rock and craters, and how its phases are caused by the positioning of the Moon in relation to the Sun and Earth during its orbit. The document uses various links and videos to help explain these concepts to students in an engaging way.
This document provides an overview of the solar system, including:
- The development of models of the solar system from ancient Greece to modern understanding.
- Descriptions of the inner planets Mercury, Venus, Earth, and Mars, including their atmospheres, temperatures, and exploration by spacecraft.
- Descriptions of the outer planets Jupiter, Saturn, Uranus, and Neptune, including their compositions, atmospheres, rings and moons.
The document explains how scientists believe the solar system formed from a nebula of gas and dust, and how the planets formed from the accretion of matter in the early solar system.
The document provides an overview of key concepts in physics and astronomy. It defines important terms like planets, satellites, phases and eclipses. It describes the structure of the solar system including terrestrial and gas giant planets. It explains theories of how the solar system formed and evolved over time from the geocentric to heliocentric models. It also summarizes characteristics of objects in our solar system like planets, moons, asteroids and comets.
'NEW Science project 9.19.2011 By Tony Leetummyblast
The document provides information about the planets in our solar system. It defines key terms like revolve, rotate, and orbit. It discusses the differences between the inner and outer planets, listing Mercury, Venus, Earth and Mars as inner planets and Jupiter, Saturn, Uranus and Neptune as outer planets. For each planet, some general facts are given about their composition, features, moons and other characteristics. The document also covers dwarf planets like Pluto, Ceres, and Eris.
1. The document contains a practice test on astronomy concepts related to the Moon, including its phases, orbit around Earth, and effects on ocean tides.
2. There are 25 multiple choice questions testing knowledge of the Moon's motion and position relative to Earth and how that determines what phase is visible from different locations on Earth's surface.
3. Additional concepts covered include solar eclipses, spring tides, and how the positions of the Moon cause highest and lowest ocean tides on Earth.
The document contains diagrams and questions about the seasons on Earth and how they are caused by the tilt of Earth's axis and its orbit around the Sun. It discusses how the amount of sunlight received at the North Pole and South Pole changes throughout the year, causing different seasons in each hemisphere. It also shows diagrams of Earth in different positions along its orbit and asks questions about which hemisphere would be experiencing summer or winter in each case.
This document provides an overview of the solar system, including:
- The development of models of the solar system from ancient Greece to modern understanding.
- Descriptions of the inner planets Mercury, Venus, Earth, and Mars, including their atmospheres, temperatures, and exploration by spacecraft.
- Descriptions of the outer planets Jupiter, Saturn, Uranus, and Neptune, including their compositions, atmospheres, rings and moons.
The document explains how scientists believe the solar system formed from a nebula of gas and dust, and how the planets formed from the accretion of matter in the early solar system.
The document provides an overview of key concepts in physics and astronomy. It defines important terms like planets, satellites, phases and eclipses. It describes the structure of the solar system including terrestrial and gas giant planets. It explains theories of how the solar system formed and evolved over time from the geocentric to heliocentric models. It also summarizes characteristics of objects in our solar system like planets, moons, asteroids and comets.
'NEW Science project 9.19.2011 By Tony Leetummyblast
The document provides information about the planets in our solar system. It defines key terms like revolve, rotate, and orbit. It discusses the differences between the inner and outer planets, listing Mercury, Venus, Earth and Mars as inner planets and Jupiter, Saturn, Uranus and Neptune as outer planets. For each planet, some general facts are given about their composition, features, moons and other characteristics. The document also covers dwarf planets like Pluto, Ceres, and Eris.
1. The document contains a practice test on astronomy concepts related to the Moon, including its phases, orbit around Earth, and effects on ocean tides.
2. There are 25 multiple choice questions testing knowledge of the Moon's motion and position relative to Earth and how that determines what phase is visible from different locations on Earth's surface.
3. Additional concepts covered include solar eclipses, spring tides, and how the positions of the Moon cause highest and lowest ocean tides on Earth.
The document contains diagrams and questions about the seasons on Earth and how they are caused by the tilt of Earth's axis and its orbit around the Sun. It discusses how the amount of sunlight received at the North Pole and South Pole changes throughout the year, causing different seasons in each hemisphere. It also shows diagrams of Earth in different positions along its orbit and asks questions about which hemisphere would be experiencing summer or winter in each case.
This document provides information about the Earth and its motion in the universe. It describes the Earth's daily rotation and yearly revolution around the Sun, which causes seasons and varying day and night lengths. It also explains the phases of the Moon and lunar and solar eclipses, noting that eclipses occur when the Sun, Moon, and Earth are aligned. Diagrams are included to illustrate these concepts.
The document provides information about the sun and our solar system over multiple days. It discusses that the sun is at the center of our solar system. It also notes that the planets in our solar system, including Earth, revolve around the sun. Additionally, it states that the sun is a medium sized star that is made up of gases like hydrogen and helium and gives off its own light and heat.
The document is a chapter from an astronomy textbook. It contains 13 multiple choice questions about topics relating to the solar system, including the differences between terrestrial and Jovian planets, asteroids, comets, meteor showers, and theories of the origin of the solar system. It also briefly discusses techniques for detecting exoplanets and why Earth-sized exoplanets have not yet been detected.
The document discusses key facts about the solar system and the Earth's movement. It notes that the solar system consists of the Sun and 8 planets, with Pluto no longer being classified as a planet. It explains that the Earth is the third planet from the Sun and is the only planet that can sustain life, due to the presence of water, air, food and temperature (WAFT). The document also describes how the Earth rotates on its axis daily and revolves around the Sun yearly, resulting in day/night and the seasons.
The document provides information about the sun and our solar system over multiple days. It covers that the sun is at the center of our solar system, the planets that revolve around it, and some key facts about the sun like that it is made of gases and gives off light and heat. It also discusses distances and time it would take to travel to the sun, as well as sizes of the sun compared to Earth.
This document contains a 25 question multiple choice test about concepts related to space, the solar system, and the Earth's rotation and revolution. The questions cover topics like the causes of day and night, seasons, phases of the moon, the order and relative distances of planets from the sun, and characteristics of objects like comets, asteroids, and sunspots.
The document summarizes key facts about the Moon's properties, surface characteristics, composition and formation history. It discusses how lunar exploration began with Soviet and American space programs in the late 1950s and 1960s, culminating in the Apollo 11 mission landing in 1969. It describes the Moon's surface features like highlands, maria, impact craters and lack of atmosphere or water. The composition is similar to Earth, consisting mainly of silicates. The widely accepted theory is that the Moon formed from debris after a giant impact between Earth and a Mars-sized object over 4 billion years ago.
The document provides information about celestial bodies like stars, constellations, and planets in our solar system. It discusses how ancient people used constellations like Ursa Major to determine directions. It describes the nine planets in our solar system, with Mercury being the closest to the sun and Pluto being the farthest, along with other objects like asteroids and meteoroids. The sun and these celestial bodies form our solar system. It also briefly mentions Neil Armstrong being the first person to walk on the moon.
Solar System Formation
Our theory must explain,
1Large bodies in the Solar System have orderly motions.
1.There are two types of planets as,
*Small, rocky terrestrial planets
*Large,hydrogen-rich Jovian planets
3. Asteroids & comets exist in certain regions of the Solar System.
4. There are exceptions to these planets
The document contains information and questions about the phases of the Moon as seen from Earth. It explains that the Moon orbits Earth about once a month, causing the monthly cycle of moon phases seen from our planet. Diagrams show the relative positions of the Moon, Earth, and Sun during different moon phases. Multiple choice questions test understanding of moon phases and their sequence over a month.
The document provides information about the solar system. It defines the solar system as a group of objects that interact with and orbit the sun. It describes the main objects in the solar system as planets, dwarf planets, moons, asteroids and comets. It explains that gravity is the force that causes objects to orbit the sun and interact with each other. It also discusses the differences between inner and outer planets, and how rotation and revolution cause seasons on Earth and variations in day length.
This document provides information about the solar system including:
1) It describes the solar system as including everything in the universe with Earth being a planet that revolves around the sun along with other objects like asteroids and comets.
2) It provides examples of matter like planets, animals, rocks that make up the solar system and examples of energy like electricity, heat, and light.
3) It explains that the sun is at the center of the solar system and lists the planets in their correct order from the sun.
The document provides an overview of the solar system, including information about the sun, planets, and other celestial bodies. It discusses the inner and outer planets, as well as characteristics of specific planets like Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. It also covers moons, asteroids, comets, dwarf planets, and phases of the moon. The summary focuses on key details about the structure of the solar system and different types of objects within it.
The document summarizes key components of the solar system. It describes the formation of the solar system and divides its members into four regions: inner planets, asteroid belt, outer planets, and Oort's cloud. It provides details on the composition and characteristics of objects within each region. The document also summarizes information about meteoroids, comets, Kuiper belt objects, and the structure and atmospheric layers of the Sun.
As the moon waxes (the amount of illuminated surface as seen from Earth is increasing), the lunar phases progress through new moon, crescent moon, first-quarter moon, gibbous moon, and full moon. The moon is then said to wane as it passes through the gibbous moon, third-quarter moon, crescent moon and back to new moon.
The document provides an overview of lessons covering physics topics related to astronomy. It outlines 24 lessons that will cover telescopes, lenses, different types of telescopes, stars, the sun, moon and earth, eclipses, star distances, galaxies, and more. Each lesson includes objectives, literacy and numeracy focuses, and extension questions.
The document discusses planetary motion and the movement of celestial bodies. It describes how early astronomers like Ptolemy, Copernicus, and Kepler developed models of the solar system. Johannes Kepler developed his three laws of planetary motion, establishing that planets orbit the sun in ellipses. Isaac Newton later explained that gravity is the force that causes planets to orbit the sun. The document also discusses the Earth's rotation, revolution, and axial tilt, which cause seasons. It describes the moon's orbit and how its phases, tides, and eclipses occur due to the positions of the Earth, moon, and sun.
The document discusses the formation of Earth and compares it to Venus and Mars. It begins by outlining the objectives, which are to understand how Earth formed, describe Earth, and recognize the differences between Earth and neighboring planets. It then discusses how Earth formed via accretion from a solar nebula and cooled to form a crust. A table compares physical properties of Venus, Earth, and Mars, noting they are rocky terrestrial planets but differ in characteristics like rotation, temperature, and presence of water. Earth stands out as the only planet that supports life.
The document discusses various facts about the Earth's rotation:
1) Day and night are caused by the Earth's rotation on its axis, with the sun rising in the east and setting in the west.
2) A sidereal day is 23 hours, 56 minutes and 4 seconds because the Earth moves slightly in its orbit each day.
3) Scientists can predict and track the Earth's rotation using satellite laser ranging, GPS satellites, and lunar laser ranging.
This document provides information about the Earth and its motion in the universe. It describes the Earth's daily rotation and yearly revolution around the Sun, which causes seasons and varying day and night lengths. It also explains the phases of the Moon and lunar and solar eclipses, noting that eclipses occur when the Sun, Moon, and Earth are aligned. Diagrams are included to illustrate these concepts.
The document provides information about the sun and our solar system over multiple days. It discusses that the sun is at the center of our solar system. It also notes that the planets in our solar system, including Earth, revolve around the sun. Additionally, it states that the sun is a medium sized star that is made up of gases like hydrogen and helium and gives off its own light and heat.
The document is a chapter from an astronomy textbook. It contains 13 multiple choice questions about topics relating to the solar system, including the differences between terrestrial and Jovian planets, asteroids, comets, meteor showers, and theories of the origin of the solar system. It also briefly discusses techniques for detecting exoplanets and why Earth-sized exoplanets have not yet been detected.
The document discusses key facts about the solar system and the Earth's movement. It notes that the solar system consists of the Sun and 8 planets, with Pluto no longer being classified as a planet. It explains that the Earth is the third planet from the Sun and is the only planet that can sustain life, due to the presence of water, air, food and temperature (WAFT). The document also describes how the Earth rotates on its axis daily and revolves around the Sun yearly, resulting in day/night and the seasons.
The document provides information about the sun and our solar system over multiple days. It covers that the sun is at the center of our solar system, the planets that revolve around it, and some key facts about the sun like that it is made of gases and gives off light and heat. It also discusses distances and time it would take to travel to the sun, as well as sizes of the sun compared to Earth.
This document contains a 25 question multiple choice test about concepts related to space, the solar system, and the Earth's rotation and revolution. The questions cover topics like the causes of day and night, seasons, phases of the moon, the order and relative distances of planets from the sun, and characteristics of objects like comets, asteroids, and sunspots.
The document summarizes key facts about the Moon's properties, surface characteristics, composition and formation history. It discusses how lunar exploration began with Soviet and American space programs in the late 1950s and 1960s, culminating in the Apollo 11 mission landing in 1969. It describes the Moon's surface features like highlands, maria, impact craters and lack of atmosphere or water. The composition is similar to Earth, consisting mainly of silicates. The widely accepted theory is that the Moon formed from debris after a giant impact between Earth and a Mars-sized object over 4 billion years ago.
The document provides information about celestial bodies like stars, constellations, and planets in our solar system. It discusses how ancient people used constellations like Ursa Major to determine directions. It describes the nine planets in our solar system, with Mercury being the closest to the sun and Pluto being the farthest, along with other objects like asteroids and meteoroids. The sun and these celestial bodies form our solar system. It also briefly mentions Neil Armstrong being the first person to walk on the moon.
Solar System Formation
Our theory must explain,
1Large bodies in the Solar System have orderly motions.
1.There are two types of planets as,
*Small, rocky terrestrial planets
*Large,hydrogen-rich Jovian planets
3. Asteroids & comets exist in certain regions of the Solar System.
4. There are exceptions to these planets
The document contains information and questions about the phases of the Moon as seen from Earth. It explains that the Moon orbits Earth about once a month, causing the monthly cycle of moon phases seen from our planet. Diagrams show the relative positions of the Moon, Earth, and Sun during different moon phases. Multiple choice questions test understanding of moon phases and their sequence over a month.
The document provides information about the solar system. It defines the solar system as a group of objects that interact with and orbit the sun. It describes the main objects in the solar system as planets, dwarf planets, moons, asteroids and comets. It explains that gravity is the force that causes objects to orbit the sun and interact with each other. It also discusses the differences between inner and outer planets, and how rotation and revolution cause seasons on Earth and variations in day length.
This document provides information about the solar system including:
1) It describes the solar system as including everything in the universe with Earth being a planet that revolves around the sun along with other objects like asteroids and comets.
2) It provides examples of matter like planets, animals, rocks that make up the solar system and examples of energy like electricity, heat, and light.
3) It explains that the sun is at the center of the solar system and lists the planets in their correct order from the sun.
The document provides an overview of the solar system, including information about the sun, planets, and other celestial bodies. It discusses the inner and outer planets, as well as characteristics of specific planets like Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. It also covers moons, asteroids, comets, dwarf planets, and phases of the moon. The summary focuses on key details about the structure of the solar system and different types of objects within it.
The document summarizes key components of the solar system. It describes the formation of the solar system and divides its members into four regions: inner planets, asteroid belt, outer planets, and Oort's cloud. It provides details on the composition and characteristics of objects within each region. The document also summarizes information about meteoroids, comets, Kuiper belt objects, and the structure and atmospheric layers of the Sun.
As the moon waxes (the amount of illuminated surface as seen from Earth is increasing), the lunar phases progress through new moon, crescent moon, first-quarter moon, gibbous moon, and full moon. The moon is then said to wane as it passes through the gibbous moon, third-quarter moon, crescent moon and back to new moon.
The document provides an overview of lessons covering physics topics related to astronomy. It outlines 24 lessons that will cover telescopes, lenses, different types of telescopes, stars, the sun, moon and earth, eclipses, star distances, galaxies, and more. Each lesson includes objectives, literacy and numeracy focuses, and extension questions.
The document discusses planetary motion and the movement of celestial bodies. It describes how early astronomers like Ptolemy, Copernicus, and Kepler developed models of the solar system. Johannes Kepler developed his three laws of planetary motion, establishing that planets orbit the sun in ellipses. Isaac Newton later explained that gravity is the force that causes planets to orbit the sun. The document also discusses the Earth's rotation, revolution, and axial tilt, which cause seasons. It describes the moon's orbit and how its phases, tides, and eclipses occur due to the positions of the Earth, moon, and sun.
The document discusses the formation of Earth and compares it to Venus and Mars. It begins by outlining the objectives, which are to understand how Earth formed, describe Earth, and recognize the differences between Earth and neighboring planets. It then discusses how Earth formed via accretion from a solar nebula and cooled to form a crust. A table compares physical properties of Venus, Earth, and Mars, noting they are rocky terrestrial planets but differ in characteristics like rotation, temperature, and presence of water. Earth stands out as the only planet that supports life.
The document discusses various facts about the Earth's rotation:
1) Day and night are caused by the Earth's rotation on its axis, with the sun rising in the east and setting in the west.
2) A sidereal day is 23 hours, 56 minutes and 4 seconds because the Earth moves slightly in its orbit each day.
3) Scientists can predict and track the Earth's rotation using satellite laser ranging, GPS satellites, and lunar laser ranging.
Presentation; The Earth in the universerafakarmona
The document discusses the Big Bang theory of the creation of the universe. It begins by stating that according to the Big Bang theory, all matter in the universe was originally concentrated in a single place, which then exploded and caused billions of particles to travel outward in all directions, later forming celestial bodies. It then poses some questions about the Big Bang and what existed before and after it.
1. Astronomy is the science that studies the universe outside of our planet. It deals with heavenly bodies.
2. Some examples of astronomical phenomena that can be observed without a telescope include the diurnal motion of stars, the annual motion of Earth orbiting the sun, precession of the equinoxes, and the changing phases of the moon as it revolves around Earth.
3. The moon appears to change shape throughout the month in a cycle called phases, from new moon when it is not illuminated to full moon when the entire side facing Earth is lit by the sun.
This document provides information about the Sun, Earth, and Moon through text and images. It compares the sizes of these celestial bodies and explains that the Sun would be the size of a basketball, Earth a pea, and the Moon a pinhead. It then discusses the key differences between the rotation and revolution of Earth and the Moon around the Sun. Finally, it summarizes how Earth's rotation causes day and night and its revolution causes seasons.
The document provides information about astronomy and the structure of the universe. It begins with a vocabulary list for "Unit 1: The study of stars and space" and defines key terms related to the Big Bang theory, such as that all matter and energy was once condensed in a single point around 13.8 billion years ago. It then discusses evidence for the Big Bang, the expansion of the universe, properties and life cycles of stars, Earth's place in the universe, and characteristics of the moon such as its phases and the causes of tides.
The document summarizes key concepts about the sun-earth-moon system:
1) The moon rotates on its axis at the same rate that it revolves around Earth, so the same side always faces Earth.
2) It takes the moon 29.5 days to rotate on its axis and revolve around Earth.
3) The moon's most obvious effect on Earth is ocean tides.
4) The document defines new and full moons and the phases of the moon. Eclipses occur when the sun or moon are blocked by Earth or the moon.
The document provides an overview of astronomy and the progression of models of the universe. It discusses early geocentric models with Earth at the center, Copernicus' heliocentric model placing the Sun at the center, and Kepler's model showing elliptical orbits. Newton later explained gravitational forces and inertia keeping planets in orbit. The effects of Earth's rotation and revolution are described, including day/night cycles and the seasons.
This document provides information about space, including the sizes of the Sun, Earth, and Moon. It explains that the Sun would be the size of a basketball, the Earth a pea, and the Moon a pinhead. It also discusses the difference between rotation and revolution, and how the Earth's rotation causes day and night and its revolution causes seasons. Additional topics covered include the Moon's phases, tides, facts about the Sun and Moon, an overview of the solar system, and highlights of the NASA Apollo program that landed astronauts on the Moon.
Introduction to SOLAR SYSTEM_Grade 6 Lesson.pptxJeniferPecson1
This document provides information about activities to teach students about the solar system. It includes 4 group activities: 1) watching an instructional video on the solar system, 2) arranging planetary bodies in order of their distance from the sun, 3) filling in a table with characteristics of the planets, and 4) checking for misconceptions about the solar system. The activities aim to teach students about the components of the solar system and their properties.
The document provides an overview of the Earth, solar system and universe from a science perspective. It begins by outlining relevant TEKS and NGSS standards around developing models of the Earth-sun-moon system and patterns in space. It then provides a brief introduction to the solar system and identifies the 8 planets in order from the sun. The bulk of the document focuses on explaining the phases of the moon through diagrams and relying on the position of the moon in relation to the sun and earth. It also addresses the causes of seasons resulting from the earth's tilted axis.
This is a PowerPoint that is about Exploring Earth Science. This is geared towards 3rd grade students. This is very picture heavy so it will easily keep the attention of young children. It is also full of helpful information
The document discusses the phases of the moon, including terminology like waxing, waning, and gibbous. It notes that the moon revolves around Earth every 28 days and goes through phases as the illuminated portion changes from new to full and back again. Key phases mentioned are new, crescent, quarter, and full moon. The document also briefly discusses lunar and solar eclipses.
The document summarizes key information about the Earth. It describes the Earth as a planet within the Solar System that is able to support life due to features like its temperature, atmosphere, and abundance of water. It discusses the Earth's shape as a spheroid called a geoid and its rotation on its axis, which causes day and night, as well as its revolution around the Sun, which causes the seasons. It also describes tools like maps, coordinates, and map projections that are used to represent and locate places on the Earth's surface.
The document discusses planetary motion, eclipses, tides, and phases of the moon. It explains that planets orbit stars in ellipses rather than perfect circles, and that closer planets move faster due to gravity. It describes solar and lunar eclipses, noting that solar eclipses occur when the moon passes between Earth and the sun, while lunar eclipses occur when Earth passes between the sun and moon. It also discusses how the moon's gravity causes ocean tides, with high tide occurring when the moon is overhead or opposite the tide location. Finally, it outlines the phases of the moon as it revolves around Earth.
This presentation explains Present Simple by using facts related to the Solar System. Adverbs of frequency are also explained.
For more information go to
http://englishverywell33.blogspot.com.co/2017/03/welcome.html
For the full video of this presentation, please visit: https://www.edge-ai-vision.com/2024/06/building-and-scaling-ai-applications-with-the-nx-ai-manager-a-presentation-from-network-optix/
Robin van Emden, Senior Director of Data Science at Network Optix, presents the “Building and Scaling AI Applications with the Nx AI Manager,” tutorial at the May 2024 Embedded Vision Summit.
In this presentation, van Emden covers the basics of scaling edge AI solutions using the Nx tool kit. He emphasizes the process of developing AI models and deploying them globally. He also showcases the conversion of AI models and the creation of effective edge AI pipelines, with a focus on pre-processing, model conversion, selecting the appropriate inference engine for the target hardware and post-processing.
van Emden shows how Nx can simplify the developer’s life and facilitate a rapid transition from concept to production-ready applications.He provides valuable insights into developing scalable and efficient edge AI solutions, with a strong focus on practical implementation.
TrustArc Webinar - 2024 Global Privacy SurveyTrustArc
How does your privacy program stack up against your peers? What challenges are privacy teams tackling and prioritizing in 2024?
In the fifth annual Global Privacy Benchmarks Survey, we asked over 1,800 global privacy professionals and business executives to share their perspectives on the current state of privacy inside and outside of their organizations. This year’s report focused on emerging areas of importance for privacy and compliance professionals, including considerations and implications of Artificial Intelligence (AI) technologies, building brand trust, and different approaches for achieving higher privacy competence scores.
See how organizational priorities and strategic approaches to data security and privacy are evolving around the globe.
This webinar will review:
- The top 10 privacy insights from the fifth annual Global Privacy Benchmarks Survey
- The top challenges for privacy leaders, practitioners, and organizations in 2024
- Key themes to consider in developing and maintaining your privacy program
HCL Notes and Domino License Cost Reduction in the World of DLAUpanagenda
Webinar Recording: https://www.panagenda.com/webinars/hcl-notes-and-domino-license-cost-reduction-in-the-world-of-dlau/
The introduction of DLAU and the CCB & CCX licensing model caused quite a stir in the HCL community. As a Notes and Domino customer, you may have faced challenges with unexpected user counts and license costs. You probably have questions on how this new licensing approach works and how to benefit from it. Most importantly, you likely have budget constraints and want to save money where possible. Don’t worry, we can help with all of this!
We’ll show you how to fix common misconfigurations that cause higher-than-expected user counts, and how to identify accounts which you can deactivate to save money. There are also frequent patterns that can cause unnecessary cost, like using a person document instead of a mail-in for shared mailboxes. We’ll provide examples and solutions for those as well. And naturally we’ll explain the new licensing model.
Join HCL Ambassador Marc Thomas in this webinar with a special guest appearance from Franz Walder. It will give you the tools and know-how to stay on top of what is going on with Domino licensing. You will be able lower your cost through an optimized configuration and keep it low going forward.
These topics will be covered
- Reducing license cost by finding and fixing misconfigurations and superfluous accounts
- How do CCB and CCX licenses really work?
- Understanding the DLAU tool and how to best utilize it
- Tips for common problem areas, like team mailboxes, functional/test users, etc
- Practical examples and best practices to implement right away
Building Production Ready Search Pipelines with Spark and MilvusZilliz
Spark is the widely used ETL tool for processing, indexing and ingesting data to serving stack for search. Milvus is the production-ready open-source vector database. In this talk we will show how to use Spark to process unstructured data to extract vector representations, and push the vectors to Milvus vector database for search serving.
Driving Business Innovation: Latest Generative AI Advancements & Success StorySafe Software
Are you ready to revolutionize how you handle data? Join us for a webinar where we’ll bring you up to speed with the latest advancements in Generative AI technology and discover how leveraging FME with tools from giants like Google Gemini, Amazon, and Microsoft OpenAI can supercharge your workflow efficiency.
During the hour, we’ll take you through:
Guest Speaker Segment with Hannah Barrington: Dive into the world of dynamic real estate marketing with Hannah, the Marketing Manager at Workspace Group. Hear firsthand how their team generates engaging descriptions for thousands of office units by integrating diverse data sources—from PDF floorplans to web pages—using FME transformers, like OpenAIVisionConnector and AnthropicVisionConnector. This use case will show you how GenAI can streamline content creation for marketing across the board.
Ollama Use Case: Learn how Scenario Specialist Dmitri Bagh has utilized Ollama within FME to input data, create custom models, and enhance security protocols. This segment will include demos to illustrate the full capabilities of FME in AI-driven processes.
Custom AI Models: Discover how to leverage FME to build personalized AI models using your data. Whether it’s populating a model with local data for added security or integrating public AI tools, find out how FME facilitates a versatile and secure approach to AI.
We’ll wrap up with a live Q&A session where you can engage with our experts on your specific use cases, and learn more about optimizing your data workflows with AI.
This webinar is ideal for professionals seeking to harness the power of AI within their data management systems while ensuring high levels of customization and security. Whether you're a novice or an expert, gain actionable insights and strategies to elevate your data processes. Join us to see how FME and AI can revolutionize how you work with data!
GraphSummit Singapore | The Future of Agility: Supercharging Digital Transfor...Neo4j
Leonard Jayamohan, Partner & Generative AI Lead, Deloitte
This keynote will reveal how Deloitte leverages Neo4j’s graph power for groundbreaking digital twin solutions, achieving a staggering 100x performance boost. Discover the essential role knowledge graphs play in successful generative AI implementations. Plus, get an exclusive look at an innovative Neo4j + Generative AI solution Deloitte is developing in-house.
GraphSummit Singapore | The Art of the Possible with Graph - Q2 2024Neo4j
Neha Bajwa, Vice President of Product Marketing, Neo4j
Join us as we explore breakthrough innovations enabled by interconnected data and AI. Discover firsthand how organizations use relationships in data to uncover contextual insights and solve our most pressing challenges – from optimizing supply chains, detecting fraud, and improving customer experiences to accelerating drug discoveries.
Unlocking Productivity: Leveraging the Potential of Copilot in Microsoft 365, a presentation by Christoforos Vlachos, Senior Solutions Manager – Modern Workplace, Uni Systems
GraphRAG for Life Science to increase LLM accuracyTomaz Bratanic
GraphRAG for life science domain, where you retriever information from biomedical knowledge graphs using LLMs to increase the accuracy and performance of generated answers
Best 20 SEO Techniques To Improve Website Visibility In SERPPixlogix Infotech
Boost your website's visibility with proven SEO techniques! Our latest blog dives into essential strategies to enhance your online presence, increase traffic, and rank higher on search engines. From keyword optimization to quality content creation, learn how to make your site stand out in the crowded digital landscape. Discover actionable tips and expert insights to elevate your SEO game.
Dr. Sean Tan, Head of Data Science, Changi Airport Group
Discover how Changi Airport Group (CAG) leverages graph technologies and generative AI to revolutionize their search capabilities. This session delves into the unique search needs of CAG’s diverse passengers and customers, showcasing how graph data structures enhance the accuracy and relevance of AI-generated search results, mitigating the risk of “hallucinations” and improving the overall customer journey.
Goodbye Windows 11: Make Way for Nitrux Linux 3.5.0!SOFTTECHHUB
As the digital landscape continually evolves, operating systems play a critical role in shaping user experiences and productivity. The launch of Nitrux Linux 3.5.0 marks a significant milestone, offering a robust alternative to traditional systems such as Windows 11. This article delves into the essence of Nitrux Linux 3.5.0, exploring its unique features, advantages, and how it stands as a compelling choice for both casual users and tech enthusiasts.
Removing Uninteresting Bytes in Software FuzzingAftab Hussain
Imagine a world where software fuzzing, the process of mutating bytes in test seeds to uncover hidden and erroneous program behaviors, becomes faster and more effective. A lot depends on the initial seeds, which can significantly dictate the trajectory of a fuzzing campaign, particularly in terms of how long it takes to uncover interesting behaviour in your code. We introduce DIAR, a technique designed to speedup fuzzing campaigns by pinpointing and eliminating those uninteresting bytes in the seeds. Picture this: instead of wasting valuable resources on meaningless mutations in large, bloated seeds, DIAR removes the unnecessary bytes, streamlining the entire process.
In this work, we equipped AFL, a popular fuzzer, with DIAR and examined two critical Linux libraries -- Libxml's xmllint, a tool for parsing xml documents, and Binutil's readelf, an essential debugging and security analysis command-line tool used to display detailed information about ELF (Executable and Linkable Format). Our preliminary results show that AFL+DIAR does not only discover new paths more quickly but also achieves higher coverage overall. This work thus showcases how starting with lean and optimized seeds can lead to faster, more comprehensive fuzzing campaigns -- and DIAR helps you find such seeds.
- These are slides of the talk given at IEEE International Conference on Software Testing Verification and Validation Workshop, ICSTW 2022.
Full-RAG: A modern architecture for hyper-personalizationZilliz
Mike Del Balso, CEO & Co-Founder at Tecton, presents "Full RAG," a novel approach to AI recommendation systems, aiming to push beyond the limitations of traditional models through a deep integration of contextual insights and real-time data, leveraging the Retrieval-Augmented Generation architecture. This talk will outline Full RAG's potential to significantly enhance personalization, address engineering challenges such as data management and model training, and introduce data enrichment with reranking as a key solution. Attendees will gain crucial insights into the importance of hyperpersonalization in AI, the capabilities of Full RAG for advanced personalization, and strategies for managing complex data integrations for deploying cutting-edge AI solutions.
Observability Concepts EVERY Developer Should Know -- DeveloperWeek Europe.pdfPaige Cruz
Monitoring and observability aren’t traditionally found in software curriculums and many of us cobble this knowledge together from whatever vendor or ecosystem we were first introduced to and whatever is a part of your current company’s observability stack.
While the dev and ops silo continues to crumble….many organizations still relegate monitoring & observability as the purview of ops, infra and SRE teams. This is a mistake - achieving a highly observable system requires collaboration up and down the stack.
I, a former op, would like to extend an invitation to all application developers to join the observability party will share these foundational concepts to build on:
Observability Concepts EVERY Developer Should Know -- DeveloperWeek Europe.pdf
Earth and moon webquest
1. The Earth and the Moon
Emily
Atkinson
Grade:
3
Objective:
Students
will
understand
that
the
shape
of
Earth
and
the
moon
are
spherical
and
that
Earth
rotates
on
its
axis
to
produce
the
appearance
of
the
sun
and
moon
moving
through
the
sky.
Describe
the
appearance
of
Earth
and
the
moon.
Describe
the
movement
of
Earth
and
the
moon
and
the
apparent
movement
of
other
bodies
through
the
sky.
http://www.flashearth.com/
Here
is
a
view
of
the
Earth
from
space!
Before
clicking
on
the
next
link,
list
some
things
you
already
know
about
Earth:
http://www.frontiernet.net/~kidpower/earth.html
A. Here
are
some
facts
about
Earth.
Maybe
there
are
some
things
you
didn’t
even
know
about!
1. How
many
days
does
it
take
the
Earth
to
make
one
COMPLETE
orbit
around
the
sun?
2. How
much
of
Earth
is
covered
by
water?
2. 3. How
many
satellites
does
Earth
have?
What
is
it
called?
http://www.onr.navy.mil/focus/spacesciences/observingsky/motion1.htm
Motion
of
the
Earth
Click
play
to
watch
the
motion
of
the
Earth
http://www.windows2universe.org/the_universe/uts/earth2.html
B. Earth’s
rotation
1. What
is
the
Earth
rotating
on?
2. Is
Earth
on
a
vertical
or
horizontal
axis?
To
what
degrees
is
it
“tipped”?
3. How
long
does
it
take
Earth
to
make
on
full
rotation?
What
do
we
call
one
rotation?
http://spaceplace.nasa.gov/dr-‐marc-‐earth/en/
Ask
Dr.
Marc
about
the
rotation
of
the
Sun
and
Moon!
Click
on
the
link
that
says
“Why
is
Earth
rotating?
Did
it
always
have
the
same
rotation
period?
Will
it
always
have
the
same
rotation
period?”
Before
clicking
the
next
link,
list
some
things
Dr.
Marc
said
about
why
the
Earth
rotates
and
its
rotational
period:
http://www.windows2universe.org/earth/moons_and_rings.html
C. The
Moon
–
facts
and
information
1. What
is
another
name
for
the
Moon?
(First
sentence)
What
is
it’s
diameter?
2. How
many
regions
make
up
the
Moon?
What
kinds
of
regions
are
they?
3. What
is
the
Moon’s
top
layer
made
of?
3.
4. What
is
under
the
Moon’s
top
layer?
Go
back
to
Dr.
Marc!
What
does
he
have
to
say
about
the
Moon?
http://spaceplace.nasa.gov/dr-‐marc-‐earth/en/
What
does
he
know
about
our
Moon?
List
some
things
Dr.
Marc
says
about
the
moon.
http://btc.montana.edu/ceres/html/Birthday/birthdayphases.html
D. The
Phases
of
the
Moon
1. Define
what
PHASES
are:
2. How
long
is
the
Moon’s
complete
cycle?
3. How
many
phases
of
the
Moon
are
there?
What
are
they
called?
4. What
are
some
other
names
for
these
phases?
(Bottom
of
the
page)
http://www.fearofphysics.com/SunMoon/phases.html
E. Causes
of
the
Moon
Phases
1. Because
the
Moon’s
light
is
just
a
reflection
from
the
Sun,
what
causes
the
Moon
phases?
4. http://www.harcourtschool.com/activity/moon_phases/
Watch
the
Phases
of
the
Moon!
Now
that
you
know
what
each
phase
looks
like
tonight,
look
at
the
moon
and
see
what
phase
it
is
in!
Come
back
to
school
tomorrow
with
an
answer
and
a
picture
you
have
drawn
of
the
moon.
http://www.bbc.co.uk/schools/scienceclips/ages/9_10/earth_sun_moon.shtml
F. Watch
this
video
on
how
the
Earth,
Moon
and
Sun
all
rotate
together!
Make
FULL
SCREEN,
Click
PLAY
and
play
with
the
number
of
hours,
days
and
months
1. Can
you
make
the
Earth
orbit
just
once
around
the
Sun?
How
many
MONTHS
does
it
take?
2. Can
you
make
the
Moon
orbit
just
once
around
the
Earth?
How
many
DAYS
does
this
take?
3. Can
you
make
the
Earth
turn
just
once
on
its
axis?
How
many
HOURS
does
this
take?
4. Click
on
LABELS
and
then
click
on
each
magnifying
glass
to
find
out
more
details
about
the
Earth,
Moon
and
Sun.
5.
Answer
Sheet
A. Facts
about
the
Earth
1. Makes
one
complete
orbit
around
the
Sun
every
365.27
days.
2. Is
mostly
covered
by
water
(75%).
3. Has
a
total
of
1
satellite
(the
Moon).
B. Earth’s
Rotation
1. The
Earth
is
rotating
around
an
axis
(called
its
rotational
axis).
2. Some
objects
rotate
about
a
horizontal
axis,
like
a
rolling
log.
Some
objects,
such
as
a
skater,
rotate
about
a
vertical
axis.
The
Earth's
axis
is
tipped
over
about
23.5°
from
vertical
3. The
Earth
rotates
around
once
in
24
hours
-‐
that's
a
rate
of
1000
miles
per
hour!.
The
time
it
takes
for
the
Earth
to
rotate
completely
around
once
is
what
we
call
a
day.
It's
Earth's
rotation
that
gives
us
night
and
day.
C. The
Moon
–
Facts
and
Information
1. The
Earth's
one
natural
satellite,
the
Moon,
is
more
than
one
quarter
the
size
of
Earth
itself
(3,474
km
diameter).
2. While
there
are
only
two
basic
types
of
regions
on
the
Moon's
surface,
there
are
many
interesting
surface
features
such
as
craters,
mountain
ranges,
rilles,
and
lava
plains.
The
structure
of
the
Moon's
interior
is
more
difficult
to
study.
3. The
Moon's
top
layer
is
a
rocky
solid,
perhaps
800
km
thick.
4. Beneath
this
layer
is
a
partially
molten
zone.
Although
it
is
not
known
for
certain,
many
lunar
geologists
believe
the
Moon
may
have
a
small
iron
core,
even
though
the
Moon
has
no
magnetic
field.
D. The
Phases
of
the
Moon
1. The
revolution
of
the
Moon
around
the
Earth
makes
the
Moon
appear
as
if
it
is
changing
shape
in
the
sky.
This
is
caused
by
the
different
angles
from
which
we
see
the
bright
part
of
the
Moon's
surface.
These
are
called
"phases"
of
the
Moon.
2. The
Moon
passes
through
four
major
shapes
during
a
cycle
that
repeats
itself
every
29.5
days.
3. Below are pictures of the four major shapes and a description of each.
New Moon: The lighted side of the Moon faces away from the Earth. This means
that the Sun, Earth, and Moon are almost in a straight line, with the Moon in
between the Sun and the Earth. The Moon that we see looks very dark.
6. First Quarter: The right half of the Moon appears lighted and the left side of the
Moon appears dark. During the time between the New Moon and the First
Quarter Moon, the part of the Moon that appears lighted gets larger and larger
every day, and will continue to grow until the Full Moon.
Full Moon: The lighted side of the Moon faces the Earth. This means that the
Earth, Sun, and Moon are nearly in a straight line, with the Earth in the
middle. The Moon that we see is very bright from the sunlight reflecting off it.
Last Quarter: Sometimes called Third Quarter. The left half of the Moon appears
lighted, and the right side of the Moon appears dark. During the time between the
Full Moon and the Last Quarter Moon, the part of the Moon that appears lighted
gets smaller and smaller every day. It will continue to shrink until the New Moon,
when the cycle starts all over again.
4. There are also four other phases of the Moon sometimes used. They are as follows:
This is known as a Waxing Crescent Moon. This Moon can be seen after the New
Moon, but before the First Quarter Moon. The crescent will grow larger and larger
every day, until the Moon looks like the First Quarter Moon.
This Moon is known as a Waxing Gibbous Moon. This Moon can be seen after
the First Quarter Moon, but before the Full Moon. The amount of the Moon that
we can see will grow larger and larger every day. ("Waxing" means increasing, or
growing larger.)
This Moon is called a Waning Gibbous Moon. This Moon can be seen after the
Full Moon, but before the Last Quarter Moon. The amount of the Moon that we
can see will grow smaller and smaller every day. ("Waning" means decreasing, or
growing smaller.)
7. This Moon is called the Waning Crescent Moon. This Moon can be seen after the
Last Quarter Moon and before the New Moon. The crescent will grow smaller and
smaller every day, until the Moon looks like the New Moon.
E. Causes
of
the
Moon
Phases
1. So
here's
where
the
phases
of
the
moon
come
from:
Unless
it
moves
behind
the
Earth,
half
of
the
moon
(that
faces
the
Sun)
is
always
lit
by
the
Sun.
That's
why
the
moon
always
appears
like
a
bright
round
ball
in
the
left
video.
But
look
at
where
your
green
city
viewpoint
is
in
the
left
video;
sort
of
off
to
the
side
of
the
moon.
You
are
not
looking
at
the
moon
directly-‐-‐
from
the
side,
you
see
part
of
the
lit
side,
and
part
of
the
dark
side.
How
much
of
each
depends
on
exactly
where
you
are,
and
where
the
Sun,
Moon,
and
Earth
are.
What
the
moon
would
look
like
from
your
green
city
is
shown
in
the
right
video.
F. Video
on
Earth,
Moon
and
Sun
1. 12
months
2. 28
days
3. 24
hours
4. Earth
i. What
is
it?
The
Earth
is
a
planet
made
of
rock,
air
and
water.
ii. What
shape
is
it?
Roughly
spherical,
like
a
slightly
squashed
ball.
iii. How
big
is
it?
It
has
a
circumference
of
about
40,000
km
iv. How
fast
does
it
move?
The
Earth
travels
around
the
Sun
once
every
year,
at
the
speed
of
about
100,000
km
per
hour.
v. Did
you
know?
The
Earth
also
spins
on
its
axis
(an
imaginary
line
through
its
center)
once
every
24
hours
5. Moon
i. What
is
it?
A
large
ball
of
rock
that
moves
around
the
Earth
ii. What
shape
is
it?
Roughly
spherical
iii. How
big
is
it?
About
a
quarter
of
the
size
of
the
Earth
iv. How
fast
does
it
move?
The
Moon
travels
around
the
Earth
once
every
28
days,
at
a
speed
of
over
3,000
km
per
hour
v. Did
you
know?
Sometimes
we
see
the
whole
Moon,
and
sometimes
we
see
only
part
of
the
Moon,
This
is
because
of
the
way
the
light
from
the
Sun
falls
on
it
6. Sun
i. What
is
it?
The
Sun
is
a
star,
it
is
very
hot
and
it
gives
us
heat
and
light
ii. What
shape
is
it?
Roughly
spherical
iii. How
big
is
it?
The
Sun
is
more
than
100
times
bigger
than
the
Earth
iv. How
hot
is
it?
15
million
degrees
at
the
center
v. Did
you
know?
Our
Sun
is
just
one
of
about
400
thousand
million
stars
in
the
galaxy
we
call
the
Milky
Way