Venus is the second planet from the sun and the brightest object in the sky after the sun. It appears luminous because it is comprised of dense carbon dioxide and sulfuric acid atmospheres. Venus has the hottest surface temperatures of any planet, averaging around 480°C due to extreme greenhouse effects. It revolves slowly, taking almost 225 Earth days to rotate once on its axis.
Venus is the second planet from the Sun and is similar in size, mass, and composition to Earth. However, Venus has an extremely hot atmosphere composed primarily of greenhouse gases like carbon dioxide that traps heat from the Sun, causing surface temperatures over 400 degrees Celsius. Venus lacks water on its surface due to the water having been broken down by sunlight and the hydrogen swept away by solar winds. The surface is a dry, desert-like landscape that is periodically renewed by volcanic activity.
The document provides an overview of Mercury, Venus, and Earth:
- Mercury is the closest planet to the Sun, with temperatures that vary greatly between day and night. It orbits the Sun every 88 days and rotates three times for every two orbits.
- Venus is similar in size to Earth but has a dense atmosphere that creates a greenhouse effect, leading to extremely high surface temperatures. It spins slowly in the opposite direction of most planets.
- Earth stands out for its abundance of water and life. It is the only known planet capable of supporting complex life due to its atmospheric and environmental conditions.
The document discusses the key characteristics of planets in our solar system. It describes how planets are classified into inner and outer planets, with Mercury, Venus, Earth and Mars as the inner planets and Jupiter, Saturn, Uranus and Neptune as the outer planets. An asteroid belt exists between the inner and outer planets. Details are then provided about the inner planets Mercury, Venus and Earth, describing their sizes, distances from the Sun, compositions and other notable features.
The document provides information about the planets in our solar system, various types of stars, and details about our sun. It describes the key characteristics of each planet from Mercury to Neptune. It also outlines different types of stars like black dwarfs, main sequence stars, red giants, and white dwarfs. Additionally, it explains the Hertzsprung-Russell diagram and provides specifics about the composition and properties of our sun.
The document summarizes the planets in our solar system. It describes the inner planets Mercury, Venus, Earth, and Mars, noting key details about each planet's distance from the sun, surface conditions, and composition. It then discusses the outer planets Jupiter, Saturn, Uranus, and Neptune, highlighting their sizes, distinctive features like rings and storms, and number of moons. The document concludes with a brief overview of Pluto, which is now classified as a dwarf planet.
The document categorizes the planets in the solar system into terrestrial and Jovian planets. The terrestrial planets consist of Mercury, Venus, Earth, and Mars. They are rocky, closer to the sun, and have few or no moons. The Jovian planets are larger gas giants beyond the terrestrial planets' orbits. They include Jupiter, Saturn, Uranus, and Neptune and are known for their multiple moons and rings. Each terrestrial planet is then described in 1-2 sentences, noting their size, composition and orbital properties.
The document provides information about the universe, our solar system, and the planets within it. It details that the universe is constantly expanding and contains billions of galaxies. Our Milky Way galaxy contains our solar system, which is made up of the Sun and eight planets in orbit around it. Each planet is described in terms of its size, composition, notable features, and other facts.
Venus is the second planet from the sun and the brightest object in the sky after the sun. It appears luminous because it is comprised of dense carbon dioxide and sulfuric acid atmospheres. Venus has the hottest surface temperatures of any planet, averaging around 480°C due to extreme greenhouse effects. It revolves slowly, taking almost 225 Earth days to rotate once on its axis.
Venus is the second planet from the Sun and is similar in size, mass, and composition to Earth. However, Venus has an extremely hot atmosphere composed primarily of greenhouse gases like carbon dioxide that traps heat from the Sun, causing surface temperatures over 400 degrees Celsius. Venus lacks water on its surface due to the water having been broken down by sunlight and the hydrogen swept away by solar winds. The surface is a dry, desert-like landscape that is periodically renewed by volcanic activity.
The document provides an overview of Mercury, Venus, and Earth:
- Mercury is the closest planet to the Sun, with temperatures that vary greatly between day and night. It orbits the Sun every 88 days and rotates three times for every two orbits.
- Venus is similar in size to Earth but has a dense atmosphere that creates a greenhouse effect, leading to extremely high surface temperatures. It spins slowly in the opposite direction of most planets.
- Earth stands out for its abundance of water and life. It is the only known planet capable of supporting complex life due to its atmospheric and environmental conditions.
The document discusses the key characteristics of planets in our solar system. It describes how planets are classified into inner and outer planets, with Mercury, Venus, Earth and Mars as the inner planets and Jupiter, Saturn, Uranus and Neptune as the outer planets. An asteroid belt exists between the inner and outer planets. Details are then provided about the inner planets Mercury, Venus and Earth, describing their sizes, distances from the Sun, compositions and other notable features.
The document provides information about the planets in our solar system, various types of stars, and details about our sun. It describes the key characteristics of each planet from Mercury to Neptune. It also outlines different types of stars like black dwarfs, main sequence stars, red giants, and white dwarfs. Additionally, it explains the Hertzsprung-Russell diagram and provides specifics about the composition and properties of our sun.
The document summarizes the planets in our solar system. It describes the inner planets Mercury, Venus, Earth, and Mars, noting key details about each planet's distance from the sun, surface conditions, and composition. It then discusses the outer planets Jupiter, Saturn, Uranus, and Neptune, highlighting their sizes, distinctive features like rings and storms, and number of moons. The document concludes with a brief overview of Pluto, which is now classified as a dwarf planet.
The document categorizes the planets in the solar system into terrestrial and Jovian planets. The terrestrial planets consist of Mercury, Venus, Earth, and Mars. They are rocky, closer to the sun, and have few or no moons. The Jovian planets are larger gas giants beyond the terrestrial planets' orbits. They include Jupiter, Saturn, Uranus, and Neptune and are known for their multiple moons and rings. Each terrestrial planet is then described in 1-2 sentences, noting their size, composition and orbital properties.
The document provides information about the universe, our solar system, and the planets within it. It details that the universe is constantly expanding and contains billions of galaxies. Our Milky Way galaxy contains our solar system, which is made up of the Sun and eight planets in orbit around it. Each planet is described in terms of its size, composition, notable features, and other facts.
The document discusses the solar system and its key components. It begins by providing context about the universe and galaxies before focusing on the Milky Way galaxy and how the solar system formed. It then describes the eight planets in our solar system - Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune - and provides one or two notable facts about each planet and its composition. The document concludes by stating that Pluto is no longer classified as a planet.
Venus is Earth's closest planetary neighbor and similar in size, but has extreme environmental conditions. It has a toxic atmosphere of thick clouds and strong winds, with surface temperatures reaching over 900°F due to its slow rotation. While once thought an Earth-like planet, it is now known to have volcanoes and landscapes unlike our own, rotating backwards with days lasting four months.
Earth is the third planet from the Sun and the largest of the terrestrial planets. Unlike the other planets, Earth's name comes from the Anglo-Saxon word "erda" meaning ground or soil. The Earth formed approximately 4.54 billion years ago and is the only known planet capable of supporting life. Additional facts: the Earth has one natural satellite (the Moon); it has a powerful magnetic field generated by its nickel-iron core that protects the planet; and it has the greatest density of all planets in the solar system.
Venus is the second planet from the Sun and has the densest atmosphere of the terrestrial planets. It rotates backwards compared to most planets and has no natural satellites. Venus is similar in size and mass to Earth but has extreme surface temperatures due to a runaway greenhouse effect. The surface is covered in volcanic plains and has few impact craters, indicating its surface is geologically young. The thick carbon dioxide atmosphere creates an intense greenhouse effect, trapping heat and causing surface temperatures over 460°C. Despite being closer to the Sun, Venus is the hottest planet due to its atmospheric composition. Venus has played an important role in many human cultures throughout history.
Venus is Earth's closest planetary neighbor and is often called Earth's "sister" or "twin" planet. It has similar size, mass, and composition to Earth, though its dense carbon dioxide atmosphere makes the surface extremely hot and inhospitable. Venus likely had oceans in the past that evaporated due to a runaway greenhouse effect. It has volcanoes and mountains, but no magnetic field or moon. Venus rotates in the opposite direction of Earth, so the sun would appear to rise in the west and set in the east.
The document provides information about the solar system including the eight planets and their characteristics. It describes the four inner planets - Mercury, Venus, Earth, and Mars which are made of rock and closest to the sun, and the four outer gas giants - Jupiter, Saturn, Uranus, and Neptune. It also discusses the planets' moons, Pluto's classification as a dwarf planet, and why some planets have more moons than others based on their gravitational pull and size.
The document lists the 8 planets and Pluto in our solar system, providing 1-3 facts about each celestial body. It notes that Mercury is the closest planet to the sun and has a unique orbit. It states that Uranus spins on its side and has low gravity. For Venus, it mentions the planet has a dry surface. The summary then points out Mars is known as the red planet with a dusty surface. It closes by saying the document provided an overview of the planets in our solar system along with 1-3 interesting facts about each one.
Jupiter is the 5th planet from the Sun and over 1,300 Earths could fit inside it. It spins rapidly, completing a day in just over 10 hours, and has a year lasting over 12 Earth years. Jupiter has a solid core surrounded by liquid metallic hydrogen and molecular hydrogen. It has a thick atmosphere composed of hydrogen and helium with constant storms, including the Giant Red Spot which has raged for over 150 years. Jupiter has over 67 known moons, with the four largest called the Galilean satellites - Io, Europa, Ganymede, and Callisto.
By Kalika Patil, PPT on Planets in our solar system. The Planets in our Solar System are Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune. To know more check out the ppt
The document provides an overview of space exploration topics including the sun, solar system, Milky Way galaxy, galaxies, future of the Milky Way, and black holes. Key points include that the sun has layers and will last another 5 billion years, our solar system has 8 planets that orbit the sun clockwise, the Milky Way contains 200 billion stars and it will collide with the Andromeda galaxy in 3 billion years, and black holes are regions of intense gravity from which nothing can escape.
The document provides information about the solar system, including its definition, composition, formation via the Big Bang theory, and details about the Sun and eight planets. It describes that the solar system formed nearly 5 billion years ago from a massive explosion called the Big Bang. It is comprised of the Sun, eight planets, dwarf planets, moons, and other celestial bodies that orbit the Sun. Each planet is then defined with key details about its composition, rotation, revolution, and notable features.
There are eight planets in our solar system: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. They all orbit and rotate around the Sun. Mercury is the smallest planet and closest to the Sun. Venus is the second planet and is covered in thick, toxic clouds. Earth is the third planet and the only one known to have life; it has one moon. Mars is the fourth planet, also known as the red planet, with a thin atmosphere and two moons.
This document provides information about the solar system and astronomy. It begins by discussing important astronomers throughout history and their contributions. It then provides facts about the solar system, including that it formed 4.6 billion years ago from a nebula and consists of the sun and objects that orbit it. The document outlines the terrestrial and gas giant planets, providing details about each. It also discusses the moon's phases and constellations. In the end, it lists the top 10 closest stars to our solar system.
The document provides an overview of the eight planets in our solar system. It describes the basic characteristics of each planet, including their size, composition, notable features, and position relative to the Sun and other planets. Mercury is the closest planet to the Sun and travels around it the fastest. Venus is similar in size to Earth but has an extremely hot surface. Earth is the third planet from the Sun and the only known planet capable of supporting life. Mars has volcanoes and valleys along with two small moons. Jupiter is the largest planet and gives off more heat than it receives from the Sun. Saturn is notable for its rings and rapid rotation. Uranus rotates on its side and has a blue-green color. Ne
The solar system consists of inner planets Mercury, Venus, Earth, and Mars that orbit closest to the sun, as well as outer gas giants Jupiter, Saturn, Uranus, and Neptune. Earth stands alone as the only planet with liquid water and ability to support life. Jupiter is the largest planet and has a Great Red Spot storm that has raged for over 300 years.
Saturn is a giant planet with a diameter of over 58,000 km. It has a hydrogen and helium atmosphere and a core made of metallic hydrogen. Saturn has over 60 moons, the largest being Titan which has a thick nitrogen atmosphere and landscapes resembling those found in Tolkien's books, with rivers and lakes of methane. Another notable moon is Mimas, which resembles the Death Star from Star Wars and shakes internally in a mysterious way.
The document summarizes key information about bodies in our solar system, including the eight major planets and three dwarf planets. It discusses the differences between inner and outer planets, as well as characteristics of each major planet like composition, rotation, and natural satellites. The three dwarf planets - Pluto, Ceres, and Eris - are also introduced along with basic facts about their orbits and moons. Overall, the document provides a broad overview of the planets, dwarf planets, and other objects that make up our solar system.
The Solar System formed 4.6 billion years ago from the collapse of a giant molecular cloud. It consists of the Sun and objects bound to it by gravity, including eight planets whose orbits are nearly circular, as well as dwarf planets, asteroids, comets, and other small bodies. The four inner terrestrial planets are composed mainly of rock, while the four outer gas giants are much more massive and composed largely of hydrogen and helium. Exploration of the Solar System has increased understanding of its formation and components.
1. The Sun: The Sun is a G-type main-sequence star, which means it is a relatively stable, middle-aged star. It makes up about 99.86% of the Solar System's total mass. The Sun is composed mainly of hydrogen (about 74% by mass) and helium (about 24% by mass), with traces of other elements. It is the source of light and energy for the entire Solar System through nuclear fusion in its core. The Sun has a diameter of about 1.4 million kilometers (870,000 miles) and a mass approximately 333,000 times that of Earth. It has a surface temperature of around 5,500 degrees Celsius (9,932 degrees Fahrenheit) and is about 4.6 billion years old. The Sun's gravitational influence keeps the planets of the solar system in orbit around it, and its solar wind extends far beyond the orbit of Pluto, defining the heliosphere
2. Inner Planets (Terrestrial Planets)
Outer Planets (Gas Giants)
Dwarf Planets and Trans-Neptunian Objects (TNOs)
Galaxies
Galaxies are vast systems that consist of stars, stellar remnants, interstellar gas, dust, and dark matter, all bound together by gravity. They are the fundamental building blocks of the universe, and their study provides crucial insights into the structure, composition, and evolution of the cosmos.
Types of Galaxies
1. Elliptical Galaxies: Elliptical, ranging from nearly spherical (E0) to highly elongated (E7). Comprised mainly of older stars, with little interstellar gas and dust. Generally, lack ongoing star formation and are often found in galaxy clusters.
2. Spiral Galaxies: Contain a mix of old and young stars, along with significant amounts of gas and dust. Ongoing star formation in the spiral arms, and they often have a rotating disk structure.
3. Irregular Galaxies: Lack a distinct regular structure. Varied mix of young and old stars, as well as gas and dust. Often the result of gravitational interactions or mergers between galaxies.
Milky Way Galaxy:
- The Milky Way is the barred spiral galaxy that includes our solar system.
- It has a central bar-shaped structure with spiral arms extending outward.
- The Milky Way is part of the Local Group, a collection of galaxies that also includes the Andromeda Galaxy and many smaller galaxies.
Galaxy Clusters:
- Galaxies are not randomly distributed; they often form groups and clusters.
- Galaxy clusters are massive structures containing hundreds or thousands of galaxies bound together by gravity.
- The Virgo Cluster is one of the closest galaxy clusters to the Milky Way.
Galaxy Formation and Evolution:
- Galaxies form through the gravitational collapse of gas and dark matter.
- Interactions between galaxies, such as mergers, can significantly impact their structure and star formation.
- Galaxies evolve over time, with factors like star formation, supernova explosions, and feedback from supermassive black holes playing key roles.
The document discusses the solar system and its key components. It begins by providing context about the universe and galaxies before focusing on the Milky Way galaxy and how the solar system formed. It then describes the eight planets in our solar system - Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune - and provides one or two notable facts about each planet and its composition. The document concludes by stating that Pluto is no longer classified as a planet.
Venus is Earth's closest planetary neighbor and similar in size, but has extreme environmental conditions. It has a toxic atmosphere of thick clouds and strong winds, with surface temperatures reaching over 900°F due to its slow rotation. While once thought an Earth-like planet, it is now known to have volcanoes and landscapes unlike our own, rotating backwards with days lasting four months.
Earth is the third planet from the Sun and the largest of the terrestrial planets. Unlike the other planets, Earth's name comes from the Anglo-Saxon word "erda" meaning ground or soil. The Earth formed approximately 4.54 billion years ago and is the only known planet capable of supporting life. Additional facts: the Earth has one natural satellite (the Moon); it has a powerful magnetic field generated by its nickel-iron core that protects the planet; and it has the greatest density of all planets in the solar system.
Venus is the second planet from the Sun and has the densest atmosphere of the terrestrial planets. It rotates backwards compared to most planets and has no natural satellites. Venus is similar in size and mass to Earth but has extreme surface temperatures due to a runaway greenhouse effect. The surface is covered in volcanic plains and has few impact craters, indicating its surface is geologically young. The thick carbon dioxide atmosphere creates an intense greenhouse effect, trapping heat and causing surface temperatures over 460°C. Despite being closer to the Sun, Venus is the hottest planet due to its atmospheric composition. Venus has played an important role in many human cultures throughout history.
Venus is Earth's closest planetary neighbor and is often called Earth's "sister" or "twin" planet. It has similar size, mass, and composition to Earth, though its dense carbon dioxide atmosphere makes the surface extremely hot and inhospitable. Venus likely had oceans in the past that evaporated due to a runaway greenhouse effect. It has volcanoes and mountains, but no magnetic field or moon. Venus rotates in the opposite direction of Earth, so the sun would appear to rise in the west and set in the east.
The document provides information about the solar system including the eight planets and their characteristics. It describes the four inner planets - Mercury, Venus, Earth, and Mars which are made of rock and closest to the sun, and the four outer gas giants - Jupiter, Saturn, Uranus, and Neptune. It also discusses the planets' moons, Pluto's classification as a dwarf planet, and why some planets have more moons than others based on their gravitational pull and size.
The document lists the 8 planets and Pluto in our solar system, providing 1-3 facts about each celestial body. It notes that Mercury is the closest planet to the sun and has a unique orbit. It states that Uranus spins on its side and has low gravity. For Venus, it mentions the planet has a dry surface. The summary then points out Mars is known as the red planet with a dusty surface. It closes by saying the document provided an overview of the planets in our solar system along with 1-3 interesting facts about each one.
Jupiter is the 5th planet from the Sun and over 1,300 Earths could fit inside it. It spins rapidly, completing a day in just over 10 hours, and has a year lasting over 12 Earth years. Jupiter has a solid core surrounded by liquid metallic hydrogen and molecular hydrogen. It has a thick atmosphere composed of hydrogen and helium with constant storms, including the Giant Red Spot which has raged for over 150 years. Jupiter has over 67 known moons, with the four largest called the Galilean satellites - Io, Europa, Ganymede, and Callisto.
By Kalika Patil, PPT on Planets in our solar system. The Planets in our Solar System are Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune. To know more check out the ppt
The document provides an overview of space exploration topics including the sun, solar system, Milky Way galaxy, galaxies, future of the Milky Way, and black holes. Key points include that the sun has layers and will last another 5 billion years, our solar system has 8 planets that orbit the sun clockwise, the Milky Way contains 200 billion stars and it will collide with the Andromeda galaxy in 3 billion years, and black holes are regions of intense gravity from which nothing can escape.
The document provides information about the solar system, including its definition, composition, formation via the Big Bang theory, and details about the Sun and eight planets. It describes that the solar system formed nearly 5 billion years ago from a massive explosion called the Big Bang. It is comprised of the Sun, eight planets, dwarf planets, moons, and other celestial bodies that orbit the Sun. Each planet is then defined with key details about its composition, rotation, revolution, and notable features.
There are eight planets in our solar system: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. They all orbit and rotate around the Sun. Mercury is the smallest planet and closest to the Sun. Venus is the second planet and is covered in thick, toxic clouds. Earth is the third planet and the only one known to have life; it has one moon. Mars is the fourth planet, also known as the red planet, with a thin atmosphere and two moons.
This document provides information about the solar system and astronomy. It begins by discussing important astronomers throughout history and their contributions. It then provides facts about the solar system, including that it formed 4.6 billion years ago from a nebula and consists of the sun and objects that orbit it. The document outlines the terrestrial and gas giant planets, providing details about each. It also discusses the moon's phases and constellations. In the end, it lists the top 10 closest stars to our solar system.
The document provides an overview of the eight planets in our solar system. It describes the basic characteristics of each planet, including their size, composition, notable features, and position relative to the Sun and other planets. Mercury is the closest planet to the Sun and travels around it the fastest. Venus is similar in size to Earth but has an extremely hot surface. Earth is the third planet from the Sun and the only known planet capable of supporting life. Mars has volcanoes and valleys along with two small moons. Jupiter is the largest planet and gives off more heat than it receives from the Sun. Saturn is notable for its rings and rapid rotation. Uranus rotates on its side and has a blue-green color. Ne
The solar system consists of inner planets Mercury, Venus, Earth, and Mars that orbit closest to the sun, as well as outer gas giants Jupiter, Saturn, Uranus, and Neptune. Earth stands alone as the only planet with liquid water and ability to support life. Jupiter is the largest planet and has a Great Red Spot storm that has raged for over 300 years.
Saturn is a giant planet with a diameter of over 58,000 km. It has a hydrogen and helium atmosphere and a core made of metallic hydrogen. Saturn has over 60 moons, the largest being Titan which has a thick nitrogen atmosphere and landscapes resembling those found in Tolkien's books, with rivers and lakes of methane. Another notable moon is Mimas, which resembles the Death Star from Star Wars and shakes internally in a mysterious way.
The document summarizes key information about bodies in our solar system, including the eight major planets and three dwarf planets. It discusses the differences between inner and outer planets, as well as characteristics of each major planet like composition, rotation, and natural satellites. The three dwarf planets - Pluto, Ceres, and Eris - are also introduced along with basic facts about their orbits and moons. Overall, the document provides a broad overview of the planets, dwarf planets, and other objects that make up our solar system.
The Solar System formed 4.6 billion years ago from the collapse of a giant molecular cloud. It consists of the Sun and objects bound to it by gravity, including eight planets whose orbits are nearly circular, as well as dwarf planets, asteroids, comets, and other small bodies. The four inner terrestrial planets are composed mainly of rock, while the four outer gas giants are much more massive and composed largely of hydrogen and helium. Exploration of the Solar System has increased understanding of its formation and components.
1. The Sun: The Sun is a G-type main-sequence star, which means it is a relatively stable, middle-aged star. It makes up about 99.86% of the Solar System's total mass. The Sun is composed mainly of hydrogen (about 74% by mass) and helium (about 24% by mass), with traces of other elements. It is the source of light and energy for the entire Solar System through nuclear fusion in its core. The Sun has a diameter of about 1.4 million kilometers (870,000 miles) and a mass approximately 333,000 times that of Earth. It has a surface temperature of around 5,500 degrees Celsius (9,932 degrees Fahrenheit) and is about 4.6 billion years old. The Sun's gravitational influence keeps the planets of the solar system in orbit around it, and its solar wind extends far beyond the orbit of Pluto, defining the heliosphere
2. Inner Planets (Terrestrial Planets)
Outer Planets (Gas Giants)
Dwarf Planets and Trans-Neptunian Objects (TNOs)
Galaxies
Galaxies are vast systems that consist of stars, stellar remnants, interstellar gas, dust, and dark matter, all bound together by gravity. They are the fundamental building blocks of the universe, and their study provides crucial insights into the structure, composition, and evolution of the cosmos.
Types of Galaxies
1. Elliptical Galaxies: Elliptical, ranging from nearly spherical (E0) to highly elongated (E7). Comprised mainly of older stars, with little interstellar gas and dust. Generally, lack ongoing star formation and are often found in galaxy clusters.
2. Spiral Galaxies: Contain a mix of old and young stars, along with significant amounts of gas and dust. Ongoing star formation in the spiral arms, and they often have a rotating disk structure.
3. Irregular Galaxies: Lack a distinct regular structure. Varied mix of young and old stars, as well as gas and dust. Often the result of gravitational interactions or mergers between galaxies.
Milky Way Galaxy:
- The Milky Way is the barred spiral galaxy that includes our solar system.
- It has a central bar-shaped structure with spiral arms extending outward.
- The Milky Way is part of the Local Group, a collection of galaxies that also includes the Andromeda Galaxy and many smaller galaxies.
Galaxy Clusters:
- Galaxies are not randomly distributed; they often form groups and clusters.
- Galaxy clusters are massive structures containing hundreds or thousands of galaxies bound together by gravity.
- The Virgo Cluster is one of the closest galaxy clusters to the Milky Way.
Galaxy Formation and Evolution:
- Galaxies form through the gravitational collapse of gas and dark matter.
- Interactions between galaxies, such as mergers, can significantly impact their structure and star formation.
- Galaxies evolve over time, with factors like star formation, supernova explosions, and feedback from supermassive black holes playing key roles.
What is Solar system? FORMATION OF SOLAR SYSTEM. SOLAR SYSTEM: StructureUday Kumar Shil
The document summarizes the structure and components of the solar system. It describes:
1. The solar system formed from a large rotating cloud of gas and dust called the solar nebula approximately 4.6 billion years ago. As it contracted, the nebula flattened into a disk and kilometer-sized protoplanets began to form.
2. The solar system consists of the Sun and celestial objects bound to it by gravity, including eight planets composed of rock/metal or gas/hydrogen that orbit in nearly circular paths within the ecliptic plane.
3. Most planets have their own moons, and the gas giants have rings composed of tiny particles orbiting them. The solar system can be divided into
The Solar System formed 4.6 billion years ago from a giant molecular cloud and is made up of the Sun and objects that orbit it. It contains 8 major planets, with the inner terrestrial planets like Earth composed mostly of rock and metal, and the outer gas giants like Jupiter made of hydrogen and helium. Venus is the second planet from the Sun, taking 224.7 Earth days to orbit and rotating in the opposite direction of most planets with no natural moon.
The document provides details about the composition and formation of the solar system. It can be summarized as follows:
1) The solar system formed from the gravitational collapse of part of a large cloud of gas and dust known as the solar nebula. This led to the formation of the Sun and a protoplanetary disk surrounding it.
2) As the Sun formed and began generating heat, the protoplanetary disk flattened into a plane and began to condense, resulting in the formation of the planets, asteroids, comets and other bodies that make up the solar system.
3) Over time, scientific understanding of solar system formation has progressed from early hypotheses to the current nebular model, which views
The universe contains everything that exists, including stars, planets, and all life and matter within them. It is impossible to comprehend the universe's immense size. Our solar system contains eight planets that orbit our star, the Sun. The planets differ in their composition, with gas giants like Jupiter and Saturn composed primarily of hydrogen and helium, and terrestrial planets like Earth, Venus, and Mars made up of rock and metals. Beyond our solar system exist phenomena like asteroids, comets, and other celestial objects that have formed over billions of years since the theorized Big Bang event that created the known universe.
The document provides an overview of Earth, its atmosphere, and its place in the solar system. It describes Earth's composition, unique characteristics that support life, and ongoing geological changes. It discusses Earth's orbit and rotation, seasons, and atmospheric layers. Recent space exploration has increased understanding of Earth and how it compares to other planets and moons in the solar system.
The solar system consists of the Sun and everything that orbits around it, including 8 planets, dwarf planets, moons, comets, and asteroids. The Sun contains over 99% of the mass of the entire solar system. The terrestrial planets like Earth are rocky, while the gas giants like Jupiter are made of gas. Our solar system formed over 4.6 billion years ago and continues to be explored by spacecraft.
The solar system consists of the Sun and everything that orbits around it, including 8 planets, dwarf planets, moons, comets, and asteroids. The Sun contains over 99% of the mass of the entire solar system. The terrestrial planets like Earth are rocky, while the gas giants like Jupiter are made of gas. Our solar system formed over 4.6 billion years ago and NASA's Voyager probes are exploring its outer limits.
The document summarizes the key components of the solar system. It begins by defining the solar system and describing its formation. It then discusses each of the major components, including the sun, the eight planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune), and provides 1-2 sentences on each planet's characteristics and composition. It also classifies the planets into inner and outer planets and provides brief descriptions of asteroids and comets.
The Sun is a middle-aged, average sized yellow star that is made up mostly of hydrogen and helium. It is about 4.6 billion years old and located 93 million miles from Earth. The Sun generates heat and light through nuclear fusion reactions in its core that convert hydrogen into helium. It is the center of our Solar System and contains over 99% of the mass in the entire system. The Solar System also includes eight official planets that orbit the Sun, along with dwarf planets, moons, asteroids, comets, and other small bodies.
The Solar System by VI - Edison (PASAY CITY WEST HIGH SCHOOL, 2012)Fatimah Sol Jalmaani
We did last year (2012), with my classmates Gloriele and Abegail for a report. Anyone can get information from it, but if you plan to use ALL OF IT, make sure to site the source, okay????! That's all! :D
The document provides information about the Solar System. It describes the eight planets in our Solar System, with the four inner terrestrial planets of Mercury, Venus, Earth, and Mars composed mainly of rock and metal, and the four outer gas giants of Jupiter, Saturn, Uranus, and Neptune being substantially more massive. It also discusses the discovery and exploration of the Solar System through history and provides details on key components like the Sun, inner Solar System, and individual inner planets.
The document discusses the universe and the solar system. It begins by explaining that the Big Bang occurred approximately 13.7 billion years ago and provides evidence for this theory. It then describes different models of the universe throughout history, from the geocentric to heliocentric models. The document also discusses the size of the universe, noting that galaxies are vast collections of stars, dust and gases that appear in clusters. Our galaxy is the Milky Way. It then provides details about the components of the solar system, including the sun, inner and outer planets, dwarf planets, asteroids, comets and moons.
The Sun dominates the solar system, accounting for 99.86% of its total mass. There are 8 planets that orbit the Sun - Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. The inner planets are rocky, while the outer planets are gaseous. Planets differ in their distances from the Sun, sizes, temperatures, and orbital periods. Earth is the only known planet capable of supporting life.
The Sun dominates the solar system, accounting for 99.86% of its total mass. There are eight planets that orbit the Sun - Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. The inner planets are rocky, while the outer planets are gaseous. The planets vary in their distances from the Sun, sizes, temperatures, and orbital periods. Earth is the only known planet capable of supporting life.
The document provides information about the planets and other objects in our solar system. It begins by listing the planets in order from the Sun: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune. It then provides more detailed information about each planet, including their composition, features, orbits and other characteristics. It also mentions asteroids, dwarf planets, and the overall formation and composition of the solar system.
1) Our solar system is located in the Milky Way Galaxy, which contains 200 billion stars.
2) Spiral galaxies have a central dense area and spiraling arms where stars often form. There are two types of spiral galaxies.
3) Our solar system consists of the sun and objects that orbit it like planets, moons, asteroids, comets, and meteors. The inner planets are small and rocky while the outer planets are large and gaseous.
Black holes were first predicted by Einstein's theory of relativity in 1916. They are regions of space where gravity is so strong that not even light can escape. Black holes are formed when massive stars collapse at the end of their life cycles. There are two main types - stellar black holes, which are 10-20 times the mass of our sun, and supermassive black holes at the centers of galaxies, which can be millions of times more massive than the sun. Though once theoretical, black holes are now understood to exist throughout the universe and have profound effects on the structure and evolution of galaxies.
Learn how, over the centuries, Japan changed from a nation that possessed ancient cultural traditions to become one of the most economically and technologically advanced societies in the world.
History, Geography, and other interesting facts about the Serengeti National Park in Tanzania, which is a natural wonder as well as a popular tourist attraction.
The Moon, earth's natural satellite and its nearest companion brings much fascination and adoration to the humankind. This article provides some interesting facts and figures associated with the Moon.
The Milky Way galaxy is home to our solar system and contains approximately 100 billion stars. While astronomers have estimated the number of stars, the galaxy's exact mass is still unknown due to the presence of dark matter, which accounts for over 80% of the galaxy's mass. In a few billion years, the Milky Way galaxy will collide with the neighboring Andromeda galaxy. The document discusses several other interesting facts about the Milky Way galaxy's composition and future collision with Andromeda.
California has a long history and was originally inhabited by many Native American tribes like the Chumash and Maidu who spoke different languages. The first Europeans to arrive were Juan Rodriguez Cabrillo in 1542 and Sir Francis Drake in 1579. Spain began colonizing California in 1769 through building missions to convert Native Americans to Catholicism. After Mexico gained independence from Spain in 1821, California became a Mexican province. American settlers revolted against Mexico and formed the short-lived Bear Flag Republic in 1846 before California joined the United States later that year after the Mexican-American War.
Mars is the second smallest planet in the solar system nicknamed the "Red Planet" due to its iron-rich soil. It has the largest volcano in the solar system called Olympus Mons, which is over 3 times taller than Everest. Mars also has two small moons called Phobos and Deimos and an atmosphere that is 100 times less dense than Earth's but can still support weather. While no current life has been found, water ice exists on Mars and research continues to understand if it could support human habitation.
Comets are microscopic bodies made of ice and dust that formed during the early formation of the solar system. Their nuclei contain water, methane, and other ices. When heated by the Sun, these ices melt and form two tails - a dust tail and an ion tail. Comets originate from the Oort cloud and Kuiper belt, and are believed to have brought water and organic molecules to Earth. Famous comets include Halley's Comet which returns every 75 years, as well as Hale-Bopp and Hyakutake.
Texas has a long and diverse history dating back 11,000 years. Various indigenous tribes inhabited the land for millennia before Europeans arrived in the 1500s, including the Karankawa, Caddo, and Apache tribes who lived as hunters, farmers, and artisans. Spain first colonized Texas in the late 1500s, though French settlers also attempted colonization in the late 1600s. Texas broke from Spanish rule in 1821 when it became part of Mexico. American settlers immigrated but faced resistance from Mexican officials, leading to the Texas Revolution and Texas becoming an independent nation in 1836. Texas then joined the United States in 1845 as the 28th state.
The document discusses Saturn, the second largest planet in the solar system. It is known for its mystical rings and takes approximately 30 Earth years to orbit the Sun. Saturn is mostly gaseous and has no solid surface, with powerful winds moving 10 times faster than hurricanes on Earth. Saturn's ring system is the most complicated in the solar system, made of ice and rock particles, and their existence has puzzled scientists. Saturn has over 50 moons, with Titan being the largest and possibly able to sustain life. Extensive research of Saturn and its moons will continue for years to come.
Hawaii is an island state located in the Pacific Ocean about 2,400 miles southwest of the mainland United States. It was originally inhabited by Polynesians and became a kingdom in the early 1800s before being overtaken by American and European settlers who developed plantation economies of sugar and pineapple. Hawaii went on to become a US territory in 1900 and finally the 50th state in 1959.
Alaska is the largest state in the United States, joining the union in 1959. It was originally explored by Europeans in the 1700s and became a Russian territory in the late 18th century, with Russian traders establishing settlements. The United States purchased Alaska from Russia in 1867 for $7.2 million. Gold rushes in the late 19th century increased settlement and Alaska gained importance during World War II due to its strategic location. Congress admitted Alaska as the 49th state in 1959.
Flags come in various shapes and colors and represent different entities like countries, states, organizations, and religions. The study of flags is called vexillology. Most flags are made of cloth in a rectangular shape with emblems or color combinations. Common colors used are red, white, and blue which symbolize bravery, peace, and loyalty respectively. The United States flag was first adopted on June 14, 1777 and has undergone modifications over time but is still affectionately known as the "Red, White and Blue" or the "Stars and Stripes".
Public speaking is one of people's biggest fears. The document recommends taking communication classes or joining Toastmasters to practice and improve communication skills. Toastmasters provides a supportive environment for members to develop public speaking and leadership abilities. The author is a long-time member of Toastmasters and has used their training to enhance her own communication and leadership skills.
How Public Speaking Skills Can Impact CareersAmita Vadlamudi
Information technology professional Amita Vadlamudi has more than three decades of experience as a computer systems engineer. To stay current within the industry, Amita Vadlamudi continues her education, taking courses on topics such as HTML and JavaScript. She also focuses on honing her communication skills through membership with Toastmasters International.
The document discusses the world's first known mechanical computer, the Antikythera mechanism, which was discovered in 1901 in a shipwreck off the Greek island of Antikythera. Dating back to the 1st century BC, the mechanism was comprised of a complex system of over 30 bronze gears that could track and display astronomical information like the lunar phases, positions of the sun and moon, a 19-year calendar, and predict eclipses 223 months into the future. This discovery showcases the advanced engineering and astronomical knowledge of the ancient Greeks, with the technology then lost until the 14th century development of mechanical clocks in Europe.
With a degree in computer sciences, Amita Vadlamudi went on to a career as a computer systems engineer with over three decades of experience. In her spare time, Amita Vadlamudi enjoys volunteering and serves as a shelf reader at her local library. She especially appreciates reading about astronomy.
Women of the American Revolution - Elizabeth Schuyler HamiltonAmita Vadlamudi
Amita Vadlamudi is experienced as a computer systems engineer in financial services. Amita Vadlamudi also takes a personal interest in American history. One area of history often neglected by scholars is the contribution of women to the American Revolution and subsequent early American political life; and one woman of particular interest to scholars of early America is Elizabeth Schuyler Hamilton, the wife of Alexander Hamilton.
A computer science graduate of St. Peter’s College in New Jersey, Amita Vadlamudi has extensive experience in the information technology sector. In her free time, Amita Vadlamudi studies a wide range of topics, including ancient cultures such as the Incan and Mayan civilizations.
JAMES WEBB STUDY THE MASSIVE BLACK HOLE SEEDSSérgio Sacani
The pathway(s) to seeding the massive black holes (MBHs) that exist at the heart of galaxies in the present and distant Universe remains an unsolved problem. Here we categorise, describe and quantitatively discuss the formation pathways of both light and heavy seeds. We emphasise that the most recent computational models suggest that rather than a bimodal-like mass spectrum between light and heavy seeds with light at one end and heavy at the other that instead a continuum exists. Light seeds being more ubiquitous and the heavier seeds becoming less and less abundant due the rarer environmental conditions required for their formation. We therefore examine the different mechanisms that give rise to different seed mass spectrums. We show how and why the mechanisms that produce the heaviest seeds are also among the rarest events in the Universe and are hence extremely unlikely to be the seeds for the vast majority of the MBH population. We quantify, within the limits of the current large uncertainties in the seeding processes, the expected number densities of the seed mass spectrum. We argue that light seeds must be at least 103 to 105 times more numerous than heavy seeds to explain the MBH population as a whole. Based on our current understanding of the seed population this makes heavy seeds (Mseed > 103 M⊙) a significantly more likely pathway given that heavy seeds have an abundance pattern than is close to and likely in excess of 10−4 compared to light seeds. Finally, we examine the current state-of-the-art in numerical calculations and recent observations and plot a path forward for near-future advances in both domains.
Evidence of Jet Activity from the Secondary Black Hole in the OJ 287 Binary S...Sérgio Sacani
Wereport the study of a huge optical intraday flare on 2021 November 12 at 2 a.m. UT in the blazar OJ287. In the binary black hole model, it is associated with an impact of the secondary black hole on the accretion disk of the primary. Our multifrequency observing campaign was set up to search for such a signature of the impact based on a prediction made 8 yr earlier. The first I-band results of the flare have already been reported by Kishore et al. (2024). Here we combine these data with our monitoring in the R-band. There is a big change in the R–I spectral index by 1.0 ±0.1 between the normal background and the flare, suggesting a new component of radiation. The polarization variation during the rise of the flare suggests the same. The limits on the source size place it most reasonably in the jet of the secondary BH. We then ask why we have not seen this phenomenon before. We show that OJ287 was never before observed with sufficient sensitivity on the night when the flare should have happened according to the binary model. We also study the probability that this flare is just an oversized example of intraday variability using the Krakow data set of intense monitoring between 2015 and 2023. We find that the occurrence of a flare of this size and rapidity is unlikely. In machine-readable Tables 1 and 2, we give the full orbit-linked historical light curve of OJ287 as well as the dense monitoring sample of Krakow.
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...Sérgio Sacani
Context. The observation of several L-band emission sources in the S cluster has led to a rich discussion of their nature. However, a definitive answer to the classification of the dusty objects requires an explanation for the detection of compact Doppler-shifted Brγ emission. The ionized hydrogen in combination with the observation of mid-infrared L-band continuum emission suggests that most of these sources are embedded in a dusty envelope. These embedded sources are part of the S-cluster, and their relationship to the S-stars is still under debate. To date, the question of the origin of these two populations has been vague, although all explanations favor migration processes for the individual cluster members. Aims. This work revisits the S-cluster and its dusty members orbiting the supermassive black hole SgrA* on bound Keplerian orbits from a kinematic perspective. The aim is to explore the Keplerian parameters for patterns that might imply a nonrandom distribution of the sample. Additionally, various analytical aspects are considered to address the nature of the dusty sources. Methods. Based on the photometric analysis, we estimated the individual H−K and K−L colors for the source sample and compared the results to known cluster members. The classification revealed a noticeable contrast between the S-stars and the dusty sources. To fit the flux-density distribution, we utilized the radiative transfer code HYPERION and implemented a young stellar object Class I model. We obtained the position angle from the Keplerian fit results; additionally, we analyzed the distribution of the inclinations and the longitudes of the ascending node. Results. The colors of the dusty sources suggest a stellar nature consistent with the spectral energy distribution in the near and midinfrared domains. Furthermore, the evaporation timescales of dusty and gaseous clumps in the vicinity of SgrA* are much shorter ( 2yr) than the epochs covered by the observations (≈15yr). In addition to the strong evidence for the stellar classification of the D-sources, we also find a clear disk-like pattern following the arrangements of S-stars proposed in the literature. Furthermore, we find a global intrinsic inclination for all dusty sources of 60 ± 20◦, implying a common formation process. Conclusions. The pattern of the dusty sources manifested in the distribution of the position angles, inclinations, and longitudes of the ascending node strongly suggests two different scenarios: the main-sequence stars and the dusty stellar S-cluster sources share a common formation history or migrated with a similar formation channel in the vicinity of SgrA*. Alternatively, the gravitational influence of SgrA* in combination with a massive perturber, such as a putative intermediate mass black hole in the IRS 13 cluster, forces the dusty objects and S-stars to follow a particular orbital arrangement. Key words. stars: black holes– stars: formation– Galaxy: center– galaxies: star formation
Immersive Learning That Works: Research Grounding and Paths ForwardLeonel Morgado
We will metaverse into the essence of immersive learning, into its three dimensions and conceptual models. This approach encompasses elements from teaching methodologies to social involvement, through organizational concerns and technologies. Challenging the perception of learning as knowledge transfer, we introduce a 'Uses, Practices & Strategies' model operationalized by the 'Immersive Learning Brain' and ‘Immersion Cube’ frameworks. This approach offers a comprehensive guide through the intricacies of immersive educational experiences and spotlighting research frontiers, along the immersion dimensions of system, narrative, and agency. Our discourse extends to stakeholders beyond the academic sphere, addressing the interests of technologists, instructional designers, and policymakers. We span various contexts, from formal education to organizational transformation to the new horizon of an AI-pervasive society. This keynote aims to unite the iLRN community in a collaborative journey towards a future where immersive learning research and practice coalesce, paving the way for innovative educational research and practice landscapes.
Discovery of An Apparent Red, High-Velocity Type Ia Supernova at 𝐳 = 2.9 wi...Sérgio Sacani
We present the JWST discovery of SN 2023adsy, a transient object located in a host galaxy JADES-GS
+
53.13485
−
27.82088
with a host spectroscopic redshift of
2.903
±
0.007
. The transient was identified in deep James Webb Space Telescope (JWST)/NIRCam imaging from the JWST Advanced Deep Extragalactic Survey (JADES) program. Photometric and spectroscopic followup with NIRCam and NIRSpec, respectively, confirm the redshift and yield UV-NIR light-curve, NIR color, and spectroscopic information all consistent with a Type Ia classification. Despite its classification as a likely SN Ia, SN 2023adsy is both fairly red (
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(
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−
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)
∼
0.9
) despite a host galaxy with low-extinction and has a high Ca II velocity (
19
,
000
±
2
,
000
km/s) compared to the general population of SNe Ia. While these characteristics are consistent with some Ca-rich SNe Ia, particularly SN 2016hnk, SN 2023adsy is intrinsically brighter than the low-
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Ca-rich population. Although such an object is too red for any low-
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cosmological sample, we apply a fiducial standardization approach to SN 2023adsy and find that the SN 2023adsy luminosity distance measurement is in excellent agreement (
≲
1
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) with
Λ
CDM. Therefore unlike low-
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Ca-rich SNe Ia, SN 2023adsy is standardizable and gives no indication that SN Ia standardized luminosities change significantly with redshift. A larger sample of distant SNe Ia is required to determine if SN Ia population characteristics at high-
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truly diverge from their low-
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counterparts, and to confirm that standardized luminosities nevertheless remain constant with redshift.
Microbial interaction
Microorganisms interacts with each other and can be physically associated with another organisms in a variety of ways.
One organism can be located on the surface of another organism as an ectobiont or located within another organism as endobiont.
Microbial interaction may be positive such as mutualism, proto-cooperation, commensalism or may be negative such as parasitism, predation or competition
Types of microbial interaction
Positive interaction: mutualism, proto-cooperation, commensalism
Negative interaction: Ammensalism (antagonism), parasitism, predation, competition
I. Mutualism:
It is defined as the relationship in which each organism in interaction gets benefits from association. It is an obligatory relationship in which mutualist and host are metabolically dependent on each other.
Mutualistic relationship is very specific where one member of association cannot be replaced by another species.
Mutualism require close physical contact between interacting organisms.
Relationship of mutualism allows organisms to exist in habitat that could not occupied by either species alone.
Mutualistic relationship between organisms allows them to act as a single organism.
Examples of mutualism:
i. Lichens:
Lichens are excellent example of mutualism.
They are the association of specific fungi and certain genus of algae. In lichen, fungal partner is called mycobiont and algal partner is called
II. Syntrophism:
It is an association in which the growth of one organism either depends on or improved by the substrate provided by another organism.
In syntrophism both organism in association gets benefits.
Compound A
Utilized by population 1
Compound B
Utilized by population 2
Compound C
utilized by both Population 1+2
Products
In this theoretical example of syntrophism, population 1 is able to utilize and metabolize compound A, forming compound B but cannot metabolize beyond compound B without co-operation of population 2. Population 2is unable to utilize compound A but it can metabolize compound B forming compound C. Then both population 1 and 2 are able to carry out metabolic reaction which leads to formation of end product that neither population could produce alone.
Examples of syntrophism:
i. Methanogenic ecosystem in sludge digester
Methane produced by methanogenic bacteria depends upon interspecies hydrogen transfer by other fermentative bacteria.
Anaerobic fermentative bacteria generate CO2 and H2 utilizing carbohydrates which is then utilized by methanogenic bacteria (Methanobacter) to produce methane.
ii. Lactobacillus arobinosus and Enterococcus faecalis:
In the minimal media, Lactobacillus arobinosus and Enterococcus faecalis are able to grow together but not alone.
The synergistic relationship between E. faecalis and L. arobinosus occurs in which E. faecalis require folic acid
CLASS 12th CHEMISTRY SOLID STATE ppt (Animated)eitps1506
Description:
Dive into the fascinating realm of solid-state physics with our meticulously crafted online PowerPoint presentation. This immersive educational resource offers a comprehensive exploration of the fundamental concepts, theories, and applications within the realm of solid-state physics.
From crystalline structures to semiconductor devices, this presentation delves into the intricate principles governing the behavior of solids, providing clear explanations and illustrative examples to enhance understanding. Whether you're a student delving into the subject for the first time or a seasoned researcher seeking to deepen your knowledge, our presentation offers valuable insights and in-depth analyses to cater to various levels of expertise.
Key topics covered include:
Crystal Structures: Unravel the mysteries of crystalline arrangements and their significance in determining material properties.
Band Theory: Explore the electronic band structure of solids and understand how it influences their conductive properties.
Semiconductor Physics: Delve into the behavior of semiconductors, including doping, carrier transport, and device applications.
Magnetic Properties: Investigate the magnetic behavior of solids, including ferromagnetism, antiferromagnetism, and ferrimagnetism.
Optical Properties: Examine the interaction of light with solids, including absorption, reflection, and transmission phenomena.
With visually engaging slides, informative content, and interactive elements, our online PowerPoint presentation serves as a valuable resource for students, educators, and enthusiasts alike, facilitating a deeper understanding of the captivating world of solid-state physics. Explore the intricacies of solid-state materials and unlock the secrets behind their remarkable properties with our comprehensive presentation.
PPT on Direct Seeded Rice presented at the three-day 'Training and Validation Workshop on Modules of Climate Smart Agriculture (CSA) Technologies in South Asia' workshop on April 22, 2024.
The debris of the ‘last major merger’ is dynamically youngSérgio Sacani
The Milky Way’s (MW) inner stellar halo contains an [Fe/H]-rich component with highly eccentric orbits, often referred to as the
‘last major merger.’ Hypotheses for the origin of this component include Gaia-Sausage/Enceladus (GSE), where the progenitor
collided with the MW proto-disc 8–11 Gyr ago, and the Virgo Radial Merger (VRM), where the progenitor collided with the
MW disc within the last 3 Gyr. These two scenarios make different predictions about observable structure in local phase space,
because the morphology of debris depends on how long it has had to phase mix. The recently identified phase-space folds in Gaia
DR3 have positive caustic velocities, making them fundamentally different than the phase-mixed chevrons found in simulations
at late times. Roughly 20 per cent of the stars in the prograde local stellar halo are associated with the observed caustics. Based
on a simple phase-mixing model, the observed number of caustics are consistent with a merger that occurred 1–2 Gyr ago.
We also compare the observed phase-space distribution to FIRE-2 Latte simulations of GSE-like mergers, using a quantitative
measurement of phase mixing (2D causticality). The observed local phase-space distribution best matches the simulated data
1–2 Gyr after collision, and certainly not later than 3 Gyr. This is further evidence that the progenitor of the ‘last major merger’
did not collide with the MW proto-disc at early times, as is thought for the GSE, but instead collided with the MW disc within
the last few Gyr, consistent with the body of work surrounding the VRM.
Authoring a personal GPT for your research and practice: How we created the Q...Leonel Morgado
Thematic analysis in qualitative research is a time-consuming and systematic task, typically done using teams. Team members must ground their activities on common understandings of the major concepts underlying the thematic analysis, and define criteria for its development. However, conceptual misunderstandings, equivocations, and lack of adherence to criteria are challenges to the quality and speed of this process. Given the distributed and uncertain nature of this process, we wondered if the tasks in thematic analysis could be supported by readily available artificial intelligence chatbots. Our early efforts point to potential benefits: not just saving time in the coding process but better adherence to criteria and grounding, by increasing triangulation between humans and artificial intelligence. This tutorial will provide a description and demonstration of the process we followed, as two academic researchers, to develop a custom ChatGPT to assist with qualitative coding in the thematic data analysis process of immersive learning accounts in a survey of the academic literature: QUAL-E Immersive Learning Thematic Analysis Helper. In the hands-on time, participants will try out QUAL-E and develop their ideas for their own qualitative coding ChatGPT. Participants that have the paid ChatGPT Plus subscription can create a draft of their assistants. The organizers will provide course materials and slide deck that participants will be able to utilize to continue development of their custom GPT. The paid subscription to ChatGPT Plus is not required to participate in this workshop, just for trying out personal GPTs during it.
Anti-Universe And Emergent Gravity and the Dark UniverseSérgio Sacani
Recent theoretical progress indicates that spacetime and gravity emerge together from the entanglement structure of an underlying microscopic theory. These ideas are best understood in Anti-de Sitter space, where they rely on the area law for entanglement entropy. The extension to de Sitter space requires taking into account the entropy and temperature associated with the cosmological horizon. Using insights from string theory, black hole physics and quantum information theory we argue that the positive dark energy leads to a thermal volume law contribution to the entropy that overtakes the area law precisely at the cosmological horizon. Due to the competition between area and volume law entanglement the microscopic de Sitter states do not thermalise at sub-Hubble scales: they exhibit memory effects in the form of an entropy displacement caused by matter. The emergent laws of gravity contain an additional ‘dark’ gravitational force describing the ‘elastic’ response due to the entropy displacement. We derive an estimate of the strength of this extra force in terms of the baryonic mass, Newton’s constant and the Hubble acceleration scale a0 = cH0, and provide evidence for the fact that this additional ‘dark gravity force’ explains the observed phenomena in galaxies and clusters currently attributed to dark matter.
3. The sun – the center of our universe – is a
sphere of hot plasma around which the Earth
and all other planets revolve. It is a dominant
body of the solar system and constitutes
approximately 99 percent of its entire mass.
Not only is the Sun a significant source of
energy, but it also provides sufficient light and
heat needed on the Earth’s surface.
4. Located at the center of the solar system, the
Sun is approximately 99.3 million miles away
from the Earth. It lies to the inner rim of the
Milky Way galaxy’s Orion Arm. The exact
location is known as the Local Interstellar
Cloud or Gould Belt, approximately 7.5 to 8.5
kiloparsecs away from the Galactic Center – the
rotational center of the Milky Way galaxy.
5. The diameter of the sun is approximately 864,000
miles or 109 times more than the Earth. Its mass is
330,000 times than that of the Earth
6. Sun consists mostly of hydrogen. The rest of the
components are helium and other elements,
including oxygen, carbon, neon, and iron.
In the process of fusion consistently occurring, the
Sun fuses approximately 600 million tons of
hydrogen into helium every second, including
which 4 million is converted to the energy needed
for planets such as the Earth. In a state where
hydrogen fusion in the Sun’s core has diminished,
there will be a significant increase in temperature
and density with its outer layer expanding and
transforming into a red giant.
7. The Sun’s chemical composition is gained from
an interstellar medium which has evolved over
the past 4.6 billion years. Within the core, the
amount of helium has altered from 24 percent
to 60 percent due to the process of fusion.
Moreover, gravity has also allowed helium and
some of the other elements to settle from the
Sun’s photosphere towards the center.
8. The photosphere is a star’s outer shell. It is also
the visible surface of the Sun that is marked by
bright granules of plasma. The chemical
composition of this sphere is usually
considered as a representation of the
primordial Solar System. The elements
comprising the Sun are usually measured by
studying the spectroscopy of the photosphere
and the meteorites that haven’t heated fully to
melting temperatures as yet.
9. The Sun has eight planets as part of the
Planetary System. It includes the four
terrestrial planets i.e., Mercury, Venus, Mars,
and Earth, two gas planets i.e., Jupiter and
Saturn, and two ice planets i.e., Uranus and
Neptune. There are several other comets, dwarf
planets, and icy bodies that lie within the same
Solar System as well.
10. Some of the first satellites designed for the
observation of the Sun were NASA Pioneers 6,
7, 8, and 9 which launched between the years
1959 and 1968. They orbited the sun at a similar
distance to which the Earth is currently at, and
made measurements on the solar wind and
solar magnetic field. As times progressed and
newer innovations emerged, discoveries were
made on the coronal mass ejections, coronal
transients, and coronal holes – all that played a
significant impact in understanding solar wind.
11. The Sun plays a scientific, symbolic and
religious role across various cultures. Without
the intense energy provided by the Sun, there
would be no life on Earth.