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The document discusses the phases of the moon. It explains that the moon appears to have phases because it revolves around Earth while also rotating on its axis. As the moon orbits Earth in its elliptical path, the angle of the sunlit side facing Earth changes, leading to different portions being illuminated and visible from Earth over the course of a lunar cycle. The document outlines the eight main phases of the moon - new moon, waxing crescent, first quarter, waxing gibbous, full moon, waning gibbous, last quarter, and waning crescent - and provides a brief description and illustration of each phase.
Power Point notes that I use in class. I did not make this presentation. I got it from the internet, the reference is on the first page. I may have altered it from it\'s origninal state though.
The document summarizes the motions and phases of the Earth-Moon system. It explains that the moon orbits Earth over the course of about a month in an elliptical orbit, appearing larger when closer (perigee) and smaller when farther (apogee). The changing positions result in the phases of the moon as the illuminated side facing Earth waxes and wanes over the lunar cycle. Eclipses occur when the sun, Earth, and moon align, causing the moon to block the sun during a solar eclipse or Earth to block the sun's light during a lunar eclipse.
Astronomy lunar phases eclipses and tidesMaria Donohue
油
The phases of the moon are caused by the changing positions of the sun, Earth, and moon relative to one another. A new moon occurs when the moon is between the Earth and sun so its night side faces Earth. A full moon happens when the moon is on the opposite side of Earth from the sun, so its full day side faces Earth. Eclipses occur when the sun, Earth, and moon align so that one passes in front of the other, casting a shadow. Lunar eclipses happen during a full moon when Earth blocks the sun's light from reaching the moon. Solar eclipses occur during a new moon when the moon passes between the sun and Earth, casting its shadow on Earth. The moon
In depth description of the Moon/s phases and why they are as they are. Uses some great internet animations of various situations explaining why we see what we see from Earth. Also discusses the tides and why they are caused by the moon's gravity.
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 moon orbits around the Earth rather than the Sun. The different phases of the moon, such as new, crescent, quarter, gibbous, and full, are caused by the changing orientation of the illuminated half of the moon relative to the Earth and Sun over the course of its orbit. The moon progresses through eight phases from new to full and back to new over the course of around 29.5 days as it orbits the Earth.
The Moon is Earth's only natural satellite. It has no atmosphere and its surface is marked by craters and dust. The same side always faces Earth. The Moon's diameter is about one quarter that of Earth and it has lower gravity and density than Earth. Temperatures vary greatly from 130属C during the day to -110属C at night. Large flat plains called maria cover parts of the near side, formed by ancient lava flows. Craters and long valleys called rilles are also features of its surface. The Moon orbits Earth about every 27 days in a cycle linked to eclipses.
The document discusses various terms related to the moon including its phases, features, effect on tides, and history of exploration. It defines waxing as when the moon appears to grow in size, waning as when it decreases in size, and gibbous as between a half circle and full circle of illumination. It notes the moon's seas are dark patches formed by ancient lava flows and that phases refer to how much is illuminated each day. A harvest moon is a full moon near the autumn equinox that rises earlier each night. The first men on the moon were Neil Armstrong and Buzz Aldrin in 1969.
The document summarizes various topics relating to Earth's seasons, phases of the moon, eclipses, and tides. It explains that Earth's rotation causes day and night, while its revolution around the sun causes years. It describes how the tilt of the Earth on its axis causes seasons. It also discusses the phases of the moon and how they are caused by the relative positions of the Earth, moon, and sun. Lunar and solar eclipses occur when the moon passes between the Earth and sun. Tides are caused by the gravitational pull of the moon and sun on Earth's oceans.
The document discusses different types of eclipses including solar and lunar eclipses. A solar eclipse occurs when the moon passes between the earth and sun, blocking the sun from view. A lunar eclipse occurs when the earth passes between the sun and moon, casting the moon in earth's shadow. The document provides details on the different types of solar and lunar eclipses as well as explanations for why eclipses do not occur every month and why the moon appears red during a lunar eclipse.
The document discusses the phases of the Moon as seen from Earth. It explains that as the Moon orbits Earth over the course of about 27 days, we see it go through phases from New Moon to Full Moon and back to New Moon again. These phases include the crescent moon, first quarter moon, waxing and waning gibbous moons, and last quarter moon. The illuminated portion of the Moon changes depending on where it is in its orbit relative to the Earth and Sun.
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 document provides an overview of the Moon including its location, physical characteristics, surface features, phases and movements. Key details include that the Moon is Earth's only natural satellite, has no atmosphere or liquid water, and its surface contains craters, highlands, and low-lying volcanic plains called maria. The Moon revolves around Earth every 27 days while rotating on its axis in the same time, keeping the same hemisphere facing Earth. Its phases are caused by the varying illumination of its surface from Earth's perspective over the course of its revolution.
The Moon is Earth's only natural satellite, located approximately 384,000 km away. It has no atmosphere and extreme surface temperatures, ranging from 130属C during the day to -190属C at night. The Moon's surface is marked by impact craters formed by meteorites, and it revolves around Earth every 27 days while rotating on its axis at the same rate, so the same side always faces Earth. The Moon has different illuminated phases that change as it orbits Earth, from new to waxing crescent to first quarter to waxing gibbous to full and then waning phases back to new. Humans first explored the Moon in the 1960s and 1970s through a series of Apollo missions that walked 12
The document provides information about the solar system and related space topics from a 4th grade science perspective. It discusses that the Sun is at the center of the solar system with 8 planets revolving around it, including Earth which is the only planet that supports life. It also mentions that the solar system is part of the Milky Way galaxy, and describes some of the other planets and objects that can be seen in the night sky like stars, constellations, comets, and meteors. Some key facts about the Sun and Earth are also highlighted such as their sizes, distances, and rotations.
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
Chapter 15 Earth Science: Sun-Earth-Moon Love Affair
-Sun
-Earth
-Moon
-Movement of Earth
-Tilt and Season
-Solstices and Equinoxes
-Latitude and Climate
-Phase of Moon
-Eclipes
-Tides
The solar system is made up of the Sun, the planets that orbit the Sun, their satellites, dwarf planets and many, many small objects, like asteroids and comets. All of these objects move and we can see these movements. We notice the Sun rises in the eastern sky in the morning and sets in the western sky in the evening. We observe different stars in the sky at different times of the year.
1) The Earth, Sun and Moon exist in a complex system of orbits where the Moon revolves around the Earth and the Earth revolves around the Sun.
2) As the Moon orbits the Earth, the illuminated portion that we see from Earth changes in a cycle called phases, ranging from new moon to full moon and back over about two weeks.
3) Lunar and solar eclipses occur when the Moon passes between the Earth and Sun, casting its shadow on either the Moon or Earth, and can be total or partial depending on the alignment of the three bodies.
The moon orbits the Earth in a nearly perfect circle over the course of approximately 27 days, with the same side always facing the Earth. The Earth rotates on its axis over the course of 24 hours, causing the cycle of day and night, and revolves around the sun over the course of 365 days, causing the seasons. Additionally, the sun rotates on its axis once every 27 days.
The document discusses key facts about the moon, including that it orbits Earth and reflects sunlight from its surface. It also explains the phases of the moon, which are caused by the moon orbiting Earth as the sun lights different parts of its surface over the course of about 29 days. The moon's gravitational pull causes ocean tides on Earth. Diagrams show each moon phase as the portion of the lit surface visible from Earth changes from new to full to new again in a repeating cycle.
The document discusses Earth's movements and their effects. It explains that Earth rotates daily on its axis and revolves yearly around the sun, causing seasons. It also describes the moon's phases as it revolves around Earth, and how eclipses occur when the sun, Earth, and moon are aligned. Further, it outlines how the moon's gravity creates tides on Earth, with high tide during maximum pull and low tide when the pull is weakest.
The document summarizes key facts about Earth:
- Earth is the third planet from the sun and formed around 4.5-4.6 billion years ago. It is the only known planet capable of sustaining life.
- With a diameter of around 8,000 miles, Earth is the fifth largest planet in the solar system and has one moon. The presence of water covering over 70% of the surface allows life to thrive.
- Earth rotates on its axis once every 24 hours and revolves around the sun once every 365 days, causing seasons and influencing climate.
The document discusses the phases of the moon, beginning with the New Moon phase where the illuminated side faces away from Earth. It then explains the order and characteristics of the subsequent phases: Waxing Crescent where a small portion is lit, First Quarter where half is lit on the right side, Waxing Gibbous where nearly all of the right side is lit, Full Moon where the entire side facing Earth is illuminated, Waning Gibbous where the left side becomes illuminated, Last Quarter where half is lit on the left, and Waning Crescent where a small portion on the left remains lit before repeating the cycle.
The Moon orbits Earth and is illuminated by sunlight reflected off its surface. It takes approximately 29 days for the Moon to orbit Earth and undergo all its phases from New Moon to Full Moon and back again. The gravitational pull of the Moon causes ocean tides on Earth.
The document discusses eclipses and Jupiter's moon Ganymede. It begins with an introduction to astronomical objects like planets and asteroids. It then discusses shadows and the terms umbra and penumbra in relation to eclipses. It notes that Jupiter has 64 moons, and that its largest moon Ganymede is around 4.5 billion years old, similar in age to Jupiter. The document includes questions about eclipses and safety tips for viewing a solar eclipse. It concludes with a short assignment to research and report on eclipses in the Philippines.
An eclipse occurs when a celestial body passes in front of the sun, blocking its light. There are two types of eclipses: lunar eclipses, where the earth casts a shadow on the moon, and solar eclipses, where the moon casts a shadow on earth. During a lunar eclipse, the earth blocks the sun's light from reaching the moon, causing it to glow red. A total lunar eclipse occurs when the moon passes completely into the earth's shadow, while a partial lunar eclipse happens when it only partially enters the shadow.
The moon is tidally locked to Earth, meaning the same side always faces Earth. This is why there is a big difference between the appearance of the near side, which faces Earth, and the far side. The near side has many visible maria (dark plains) while the far side has fewer maria and a thicker crust with more craters. Additionally, the Earth and moon orbit a common center of gravity called the barycenter, located about 900 miles from Earth's surface. Both bodies revolve around this point, which itself revolves around the sun.
The document discusses various terms related to the moon including its phases, features, effect on tides, and history of exploration. It defines waxing as when the moon appears to grow in size, waning as when it decreases in size, and gibbous as between a half circle and full circle of illumination. It notes the moon's seas are dark patches formed by ancient lava flows and that phases refer to how much is illuminated each day. A harvest moon is a full moon near the autumn equinox that rises earlier each night. The first men on the moon were Neil Armstrong and Buzz Aldrin in 1969.
The document summarizes various topics relating to Earth's seasons, phases of the moon, eclipses, and tides. It explains that Earth's rotation causes day and night, while its revolution around the sun causes years. It describes how the tilt of the Earth on its axis causes seasons. It also discusses the phases of the moon and how they are caused by the relative positions of the Earth, moon, and sun. Lunar and solar eclipses occur when the moon passes between the Earth and sun. Tides are caused by the gravitational pull of the moon and sun on Earth's oceans.
The document discusses different types of eclipses including solar and lunar eclipses. A solar eclipse occurs when the moon passes between the earth and sun, blocking the sun from view. A lunar eclipse occurs when the earth passes between the sun and moon, casting the moon in earth's shadow. The document provides details on the different types of solar and lunar eclipses as well as explanations for why eclipses do not occur every month and why the moon appears red during a lunar eclipse.
The document discusses the phases of the Moon as seen from Earth. It explains that as the Moon orbits Earth over the course of about 27 days, we see it go through phases from New Moon to Full Moon and back to New Moon again. These phases include the crescent moon, first quarter moon, waxing and waning gibbous moons, and last quarter moon. The illuminated portion of the Moon changes depending on where it is in its orbit relative to the Earth and Sun.
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 document provides an overview of the Moon including its location, physical characteristics, surface features, phases and movements. Key details include that the Moon is Earth's only natural satellite, has no atmosphere or liquid water, and its surface contains craters, highlands, and low-lying volcanic plains called maria. The Moon revolves around Earth every 27 days while rotating on its axis in the same time, keeping the same hemisphere facing Earth. Its phases are caused by the varying illumination of its surface from Earth's perspective over the course of its revolution.
The Moon is Earth's only natural satellite, located approximately 384,000 km away. It has no atmosphere and extreme surface temperatures, ranging from 130属C during the day to -190属C at night. The Moon's surface is marked by impact craters formed by meteorites, and it revolves around Earth every 27 days while rotating on its axis at the same rate, so the same side always faces Earth. The Moon has different illuminated phases that change as it orbits Earth, from new to waxing crescent to first quarter to waxing gibbous to full and then waning phases back to new. Humans first explored the Moon in the 1960s and 1970s through a series of Apollo missions that walked 12
The document provides information about the solar system and related space topics from a 4th grade science perspective. It discusses that the Sun is at the center of the solar system with 8 planets revolving around it, including Earth which is the only planet that supports life. It also mentions that the solar system is part of the Milky Way galaxy, and describes some of the other planets and objects that can be seen in the night sky like stars, constellations, comets, and meteors. Some key facts about the Sun and Earth are also highlighted such as their sizes, distances, and rotations.
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
Chapter 15 Earth Science: Sun-Earth-Moon Love Affair
-Sun
-Earth
-Moon
-Movement of Earth
-Tilt and Season
-Solstices and Equinoxes
-Latitude and Climate
-Phase of Moon
-Eclipes
-Tides
The solar system is made up of the Sun, the planets that orbit the Sun, their satellites, dwarf planets and many, many small objects, like asteroids and comets. All of these objects move and we can see these movements. We notice the Sun rises in the eastern sky in the morning and sets in the western sky in the evening. We observe different stars in the sky at different times of the year.
1) The Earth, Sun and Moon exist in a complex system of orbits where the Moon revolves around the Earth and the Earth revolves around the Sun.
2) As the Moon orbits the Earth, the illuminated portion that we see from Earth changes in a cycle called phases, ranging from new moon to full moon and back over about two weeks.
3) Lunar and solar eclipses occur when the Moon passes between the Earth and Sun, casting its shadow on either the Moon or Earth, and can be total or partial depending on the alignment of the three bodies.
The moon orbits the Earth in a nearly perfect circle over the course of approximately 27 days, with the same side always facing the Earth. The Earth rotates on its axis over the course of 24 hours, causing the cycle of day and night, and revolves around the sun over the course of 365 days, causing the seasons. Additionally, the sun rotates on its axis once every 27 days.
The document discusses key facts about the moon, including that it orbits Earth and reflects sunlight from its surface. It also explains the phases of the moon, which are caused by the moon orbiting Earth as the sun lights different parts of its surface over the course of about 29 days. The moon's gravitational pull causes ocean tides on Earth. Diagrams show each moon phase as the portion of the lit surface visible from Earth changes from new to full to new again in a repeating cycle.
The document discusses Earth's movements and their effects. It explains that Earth rotates daily on its axis and revolves yearly around the sun, causing seasons. It also describes the moon's phases as it revolves around Earth, and how eclipses occur when the sun, Earth, and moon are aligned. Further, it outlines how the moon's gravity creates tides on Earth, with high tide during maximum pull and low tide when the pull is weakest.
The document summarizes key facts about Earth:
- Earth is the third planet from the sun and formed around 4.5-4.6 billion years ago. It is the only known planet capable of sustaining life.
- With a diameter of around 8,000 miles, Earth is the fifth largest planet in the solar system and has one moon. The presence of water covering over 70% of the surface allows life to thrive.
- Earth rotates on its axis once every 24 hours and revolves around the sun once every 365 days, causing seasons and influencing climate.
The document discusses the phases of the moon, beginning with the New Moon phase where the illuminated side faces away from Earth. It then explains the order and characteristics of the subsequent phases: Waxing Crescent where a small portion is lit, First Quarter where half is lit on the right side, Waxing Gibbous where nearly all of the right side is lit, Full Moon where the entire side facing Earth is illuminated, Waning Gibbous where the left side becomes illuminated, Last Quarter where half is lit on the left, and Waning Crescent where a small portion on the left remains lit before repeating the cycle.
The Moon orbits Earth and is illuminated by sunlight reflected off its surface. It takes approximately 29 days for the Moon to orbit Earth and undergo all its phases from New Moon to Full Moon and back again. The gravitational pull of the Moon causes ocean tides on Earth.
The document discusses eclipses and Jupiter's moon Ganymede. It begins with an introduction to astronomical objects like planets and asteroids. It then discusses shadows and the terms umbra and penumbra in relation to eclipses. It notes that Jupiter has 64 moons, and that its largest moon Ganymede is around 4.5 billion years old, similar in age to Jupiter. The document includes questions about eclipses and safety tips for viewing a solar eclipse. It concludes with a short assignment to research and report on eclipses in the Philippines.
An eclipse occurs when a celestial body passes in front of the sun, blocking its light. There are two types of eclipses: lunar eclipses, where the earth casts a shadow on the moon, and solar eclipses, where the moon casts a shadow on earth. During a lunar eclipse, the earth blocks the sun's light from reaching the moon, causing it to glow red. A total lunar eclipse occurs when the moon passes completely into the earth's shadow, while a partial lunar eclipse happens when it only partially enters the shadow.
The moon is tidally locked to Earth, meaning the same side always faces Earth. This is why there is a big difference between the appearance of the near side, which faces Earth, and the far side. The near side has many visible maria (dark plains) while the far side has fewer maria and a thicker crust with more craters. Additionally, the Earth and moon orbit a common center of gravity called the barycenter, located about 900 miles from Earth's surface. Both bodies revolve around this point, which itself revolves around the sun.
This is a presentation about our Earth's moon. It is extremely extensive and is wonderful for academic purposes. It's extremely easy to edit, and this is sure to get you that A+ you've been wanting.
The document provides information about the Moon through a series of slides. It discusses the Moon's location in our solar system, its physical features such as craters and maria, phases of the Moon, lunar eclipses and solar eclipses. The document also covers tides caused by the Moon's gravity, past exploration of the Moon including Apollo missions, and possibilities for future lunar bases. Photos and diagrams accompany the text to illustrate different phases of the Moon, lunar terrain, and other concepts. Additional online photo resources are also listed.
The document describes key facts about the Earth, moon, eclipses, and lunar landforms. It states that the Earth orbits the sun in an elliptical path and rotates on its axis, causing day and night. The moon revolves around the Earth while the same side always faces it. Solar eclipses occur when the moon blocks the sun, and lunar eclipses happen when the Earth blocks the sun from the moon. Common lunar landforms include craters, maria (areas of hardened lava), and ray craters.
The Moon is Earth's only natural satellite and orbits our planet about every 27 days. It has no atmosphere and experiences extreme temperature ranges. The lunar surface features highlands, craters, and low-lying maria plains filled with hardened lava. The side facing Earth always appears the same while the far side has more craters and few maria. Phases and eclipses occur due to the relative positions of the Moon, Earth, and Sun. Twelve American astronauts walked on the Moon between 1969-1972, with future lunar bases potentially allowing long-term human habitation.
The Moon is Earth's only natural satellite and orbits our planet about every 27 days. It has no atmosphere and experiences extreme temperature ranges. The lunar surface features highlands, craters, and low-lying maria plains filled with hardened lava. The side facing Earth always appears the same while the far side has more craters and few maria. The Moon's phases and eclipses are caused by its orbit around Earth. Humans first explored the Moon in 1969 and collected rocks and data, but future missions may establish lunar bases.
There are two types of eclipses: solar and lunar. A lunar eclipse occurs when the moon passes into the Earth's shadow, appearing red or dark. A solar eclipse happens when the moon passes between the Earth and sun, casting its shadow on Earth. There are three types of each: total, partial, and penumbral/annular. Lunar eclipses are more common as anyone experiencing nighttime can see it, while only a small area experiences a solar eclipse due to the moon's small umbral shadow. Eclipses occur during eclipse seasons when the sun, Earth, and moon are directly aligned.
There are two types of eclipses: solar and lunar. A lunar eclipse occurs when the moon passes into the Earth's shadow, appearing red or dark. A solar eclipse happens when the moon passes between the Earth and sun, casting its shadow on Earth. There are three types of each: total, partial, and penumbral/annular. Lunar eclipses are more common as anyone experiencing nighttime can see it, while only a small area experiences a solar eclipse due to the moon's small umbral shadow. Eclipses occur during eclipse seasons when the sun, Earth, and moon are directly aligned.
There are two types of eclipses: lunar eclipses, which occur when the moon passes into Earth's shadow, and solar eclipses, which occur when the moon passes between Earth and the sun. Lunar eclipses can be total, partial, or penumbral depending on how far into Earth's shadow the moon passes. Solar eclipses can be total, partial, or annular depending on the moon's position in its orbit. Eclipses do not occur every month because the moon's orbit is tilted relative to Earth's orbit around the sun, so the three objects do not align perfectly except during eclipse seasons.
This document provides an overview of astronomy topics including:
- The basic properties of Earth, Moon, Sun and other planets in our solar system.
- How the tilt of Earth's axis causes the seasons and the celestial sphere model used to understand sky motions.
- Key events like solstices, equinoxes, and lunar phases that occur as Earth orbits the Sun and the Moon orbits Earth.
- The causes and viewing locations of solar and lunar eclipses when the Sun, Earth and Moon are directly aligned.
- Concepts like sidereal time, precession and time zones used to measure and communicate about time and sky positions.
Gravity causes planets to orbit stars in ellipses, with those closer to the star moving faster. The moon orbits Earth, causing tides and eclipses. Its phases are due to the changing portion illuminated by the sun from Earth's perspective over the lunar month.
Gravity causes planets to orbit stars in ellipses, with those closer to the star moving faster. The moon orbits Earth, causing tides and eclipses. Its phases are due to the changing portion illuminated by the sun from Earth's perspective over the lunar month.
Gravity causes planets to orbit stars in ellipses, with those closer to the star moving faster. The moon's gravity also causes ocean tides on Earth. Eclipses occur when the sun, Earth, and moon align, blocking light. The phases of the moon are caused by the changing portion of the moon illuminated by the sun as it orbits Earth monthly.
Gravity causes planets to orbit stars in ellipses, with those closer to the star moving faster. The moon's gravity also causes ocean tides on Earth. Eclipses occur when the sun, Earth, and moon align, blocking light. The phases of the moon are caused by the changing portion of the moon illuminated by the sun as it orbits Earth monthly.
Gravity causes planets to orbit stars in ellipses, with those closer to the star moving faster. The moon's gravity also causes ocean tides on Earth. Eclipses occur when the sun, Earth, and moon align, blocking light. The phases of the moon are caused by the changing portion of the moon illuminated by the sun as it orbits Earth monthly.
- Historical models assumed Earth was the center of the solar system, with planets circling it. Copernicus developed the first sun-centered model. Galileo observed moons orbiting Jupiter, showing Earth was not uniquely orbited.
- Earth rotates on a tilted axis once every 24 hours, causing day and night. Its yearly revolution around the sun and axial tilt cause the seasons.
- The solar system includes the sun and objects that orbit it, such as planets, asteroids, comets, and other planetary bodies. It is located within the Milky Way galaxy.
The document discusses different types of eclipses. It explains that a solar eclipse occurs when the moon passes in front of the sun, casting its shadow on Earth. There are three types of solar eclipses: total, annular, and partial. A lunar eclipse occurs when the moon passes through Earth's shadow. The moon's shadow consists of the umbra, where the sun is completely covered, the penumbra where it is only partially covered, and the antumbra. Students are assigned group projects to diagram and present the alignments of celestial bodies during eclipses, compare solar and lunar eclipses, and provide safety guidelines for viewing a solar eclipse.
There are two types of eclipses: lunar eclipses, which occur when the moon passes into Earth's shadow, and solar eclipses, which occur when the moon passes between Earth and the sun. Lunar eclipses can be total, partial, or penumbral depending on how far into Earth's shadow the moon passes. Solar eclipses can be total, partial, or annular depending on the moon's position in its orbit. Eclipses do not occur daily because the moon's orbit is tilted relative to Earth's orbit around the sun, so the three bodies do not align perfectly most months.
Finals of Rass MELAI : a Music, Entertainment, Literature, Arts and Internet Culture Quiz organized by Conquiztadors, the Quiz society of Sri Venkateswara College under their annual quizzing fest El Dorado 2025.
Blind Spots in AI and Formulation Science Knowledge Pyramid (Updated Perspect...Ajaz Hussain
油
This presentation delves into the systemic blind spots within pharmaceutical science and regulatory systems, emphasizing the significance of "inactive ingredients" and their influence on therapeutic equivalence. These blind spots, indicative of normalized systemic failures, go beyond mere chance occurrences and are ingrained deeply enough to compromise decision-making processes and erode trust.
Historical instances like the 1938 FD&C Act and the Generic Drug Scandals underscore how crisis-triggered reforms often fail to address the fundamental issues, perpetuating inefficiencies and hazards.
The narrative advocates a shift from reactive crisis management to proactive, adaptable systems prioritizing continuous enhancement. Key hurdles involve challenging outdated assumptions regarding bioavailability, inadequately funded research ventures, and the impact of vague language in regulatory frameworks.
The rise of large language models (LLMs) presents promising solutions, albeit with accompanying risks necessitating thorough validation and seamless integration.
Tackling these blind spots demands a holistic approach, embracing adaptive learning and a steadfast commitment to self-improvement. By nurturing curiosity, refining regulatory terminology, and judiciously harnessing new technologies, the pharmaceutical sector can progress towards better public health service delivery and ensure the safety, efficacy, and real-world impact of drug products.
How to Modify Existing Web Pages in Odoo 18Celine George
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In this slide, well discuss on how to modify existing web pages in Odoo 18. Web pages in Odoo 18 can also gather user data through user-friendly forms, encourage interaction through engaging features.
How to attach file using upload button Odoo 18Celine George
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In this slide, well discuss on how to attach file using upload button Odoo 18. Odoo features a dedicated model, 'ir.attachments,' designed for storing attachments submitted by end users. We can see the process of utilizing the 'ir.attachments' model to enable file uploads through web forms in this slide.
How to Manage Putaway Rule in Odoo 17 InventoryCeline George
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Inventory management is a critical aspect of any business involved in manufacturing or selling products.
Odoo 17 offers a robust inventory management system that can handle complex operations and optimize warehouse efficiency.
Computer Application in Business (commerce)Sudar Sudar
油
The main objectives
1. To introduce the concept of computer and its various parts. 2. To explain the concept of data base management system and Management information system.
3. To provide insight about networking and basics of internet
Recall various terms of computer and its part
Understand the meaning of software, operating system, programming language and its features
Comparing Data Vs Information and its management system Understanding about various concepts of management information system
Explain about networking and elements based on internet
1. Recall the various concepts relating to computer and its various parts
2 Understand the meaning of softwares, operating system etc
3 Understanding the meaning and utility of database management system
4 Evaluate the various aspects of management information system
5 Generating more ideas regarding the use of internet for business purpose
APM People Interest Network Conference 2025
-Autonomy, Teams and Tension: Projects under stress
-Tim Lyons
-The neurological levels of
team-working: Harmony and tensions
With a background in projects spanning more than 40 years, Tim Lyons specialised in the delivery of large, complex, multi-disciplinary programmes for clients including Crossrail, Network Rail, ExxonMobil, Siemens and in patent development. His first career was in broadcasting, where he designed and built commercial radio station studios in Manchester, Cardiff and Bristol, also working as a presenter and programme producer. Tim now writes and presents extensively on matters relating to the human and neurological aspects of projects, including communication, ethics and coaching. He holds a Masters degree in NLP, is an NLP Master Practitioner and International Coach. He is the Deputy Lead for APMs People Interest Network.
Session | The Neurological Levels of Team-working: Harmony and Tensions
Understanding how teams really work at conscious and unconscious levels is critical to a harmonious workplace. This session uncovers what those levels are, how to use them to detect and avoid tensions and how to smooth the management of change by checking you have considered all of them.
How to Setup WhatsApp in Odoo 17 - Odoo 際際滷sCeline George
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Integrate WhatsApp into Odoo using the WhatsApp Business API or third-party modules to enhance communication. This integration enables automated messaging and customer interaction management within Odoo 17.
How to Configure Restaurants in Odoo 17 Point of SaleCeline George
油
Odoo, a versatile and integrated business management software, excels with its robust Point of Sale (POS) module. This guide delves into the intricacies of configuring restaurants in Odoo 17 POS, unlocking numerous possibilities for streamlined operations and enhanced customer experiences.
Database population in Odoo 18 - Odoo slidesCeline George
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In this slide, well discuss the database population in Odoo 18. In Odoo, performance analysis of the source code is more important. Database population is one of the methods used to analyze the performance of our code.
Database population in Odoo 18 - Odoo slidesCeline George
油
Is moon
2. What is the moon?
A natural satellite
One of more than the 96 moons in
our solar system
The only moon of the planet Earth
3. LOCATION AND SIZE
About 384,000
kilometers (240,000
miles) from Earth
3,468 kilometers
(2,155 miles) in
diameter
About 村 the size of
Earth
4. Movements of the Moon
Orbit is an ellipse, not circular
Apogee (farthest from Earth)
Perigee (closest to Earth)
Revolution Moon orbits the
Earth every 27 1/3 days
The moon rises in the East and
sets in the West
The moon rises and sets 50
minutes later each day
Rotation Moon turns on its axis
every 27 days
Same side of the Moon always
faces Earth
5. As the Moon
completes its
revolution in about a
months time, we
always see the same
side facing us.
Movements of the Moon
6. Because the moons
period of rotation is
equal to its period of
revolution (Scientists
call this
SYNCHRONOUS
ROTATION).
Movements of the Moon
7. Galileo, with the aid of his telescope,
was the first to explore the moons
surface. He found that its surface is
covered with crates, mountains, valleys
and flat plains.
Movements of the Moon
8. The Moons Surface
No atmosphere
No liquid water
Extreme temperatures
Daytime = 130属C
(265属 F)
Nighttime = -190属C
(-310属F)
1/6 of Earths gravity
9. The Moons Surface
Lunar rocks and dust cover most of the surface
This layer is called the regolith
1 6 meters deep
The lack of an atmosphere let many more meteorites
strike the moons surface, creating this layer of
crushed rock.
Anorthosites are light-colored, coarse-grained rocks
found in the lunar highlands.
Breccia contains fragments of other rocks that have
melted together, and are found everywhere on the
moon.
10. Lunar Features Craters
Bowl shaped depressions
Up to 2500 kilometers (1,553 miles) across
Most formed by meteorite impact on the Moon
Some formed by volcanic action inside the Moon
11. Lunar Features Craters
When meteorites struck
the surface they
displaced material
Like a splash
Marks left are called
rays
15. 1. New Moon
The Moon's not
illuminated side is
facing the Earth.
The Moon is not visible
(except during a solar
eclipse).
16. 2. Waxing Crescent
The Moon appears to be
partly but less than one-
half illuminated by direct
sunlight.
The fraction of the Moon's
disk that is illuminated is
increasing.
17. 3. First Quarter
One-half of the Moon
appears to be illuminated
by direct sunlight.
The fraction of the
Moon's disk that is
illuminated is
increasing.
18. 4. Waxing Gibbous
The Moon appears to be
more than one-half but
not fully illuminated by
direct sunlight.
The fraction of the
Moon's disk that is
illuminated is
increasing.
19. 5. Full Moon
The Moon's illuminated
side is facing the Earth.
The Moon appears to be
completely illuminated
by direct sunlight.
20. 6. Waning Gibbous
The Moon appears to be
more than one-half but
not fully illuminated by
direct sunlight.
The fraction of the
Moon's disk that is
illuminated is
decreasing.
21. 7. Last Quarter
One-half of the Moon
appears to be illuminated
by direct sunlight.
The fraction of the
Moon's disk that is
illuminated is
decreasing.
22. 8. Waning Crescent
The Moon appears to be
partly but less than one-
half illuminated by
direct sunlight
The fraction of the
Moon's disk that is
illuminated is
decreasing.
23. Waxing or Waning?
Waxing means the moon is
growing. If the moon is
getting bright from the right,
it is waxing.
Waning means the moon is
shrinking. If the moon is
dark on the right, it is waning.
25. Lunar Eclipse
A lunar eclipse occurs when
the Moon passes directly
behind Earth and into its
shadow. This can occur only
when the Sun, Earth, and
Moon are exactly or very
closely aligned (in syzygy),
with Earth between the other
two.
26. Two types of Lunar Eclipse
1. Partial Lunar Eclipse
A portion of the Moon passes
through Earth's umbral
shadow.
These events are easy to see,
even with the unaided eye.
27. 2. Total Lunar Eclipse
Two types of Lunar Eclipse
The entire Moon passes
through Earth's umbral
shadow.
These events are quite
striking due to the Moon's
vibrant red color during the
total phase (totality).
28. Solar Eclipse
A solar eclipse occurs when an
observer (on Earth) passes
through the shadow cast by the
Moon which fully or partially
blocks ("occults") the Sun.
29. Two types of Solar Eclipse
1. Partial Solar Eclipse
A partial solar eclipse
happens when the Moon
only partially covers the
disk of the Sun.
30. Two types of Solar Eclipse
2. Total Solar Eclipse
A total solar eclipse happens when the Moon totally
covers the disk of the Sun.
An annular solar eclipse occurs when the Moon
appears smaller than the Sun as it passes centrally
across the solar disk and a bright ring, or annulus, of
sunlight remains visible during the eclipse.
31. Saros is the roughly 18-year periodic cycle of the
Earth-Moon-Sun system. Every 6,585 days, the
Earth, Moon, and Sun are in exactly the same
position. When there is a lunar eclipse, there will
also be one exactly 6,585 days later.
Saros
#4: About 384,000 kilometers (240,000 miles) from Earth
3,468 kilometers (2,155 miles) in diameter
About 村 the size of Earth
#5: Orbit is an ellipse, not circular
***Apogee*** (farthest from Earth)
***Perigee*** (closest to Earth)
Revolution Moon orbits the Earth every 27 1/3 days
The moon rises in the East and sets in the West
The moon rises and sets 50 minutes later each day
Rotation Moon turns on its axis every 27 days
Same side of the Moon always faces Earth
#14: Mountains up to 7500 meters (25,000 feet) tall
Rilles (trenchlike valleys)