Planet Venus
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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.
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Venus presentation
Venus is named after the Roman god of beauty and was the second planet from the sun. It has an extremely hot surface temperature that would instantly kill any human visitors due to its dense carbon dioxide atmosphere and surface of lava and volcanoes. Despite being similar in size to Earth, Venus has extreme environmental conditions that are inhospitable to life as we know it compared to the more temperate climate on Earth.
Planet Venus, the Veiled and Hottest Planet
Venus is Earth's closest planetary neighbor with similarities in size, mass, and composition. It has a dense carbon dioxide atmosphere and experiences extreme surface temperatures around 864 degrees F due to greenhouse gas warming. Venus rotates backwards compared to Earth and has no magnetic field. It has been explored by numerous spacecraft but cannot support life due to the hostile conditions.
The planet venus
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.
Venus
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
''Venus'' - The Second planet of our solar system.Lets discuss about this planet.
Hope You Like it
By:- slide_maker4u
(Abhishek Sharma)
Venus
Venus is the second planet from the Sun and is the hottest planet in our Solar System with surface temperatures reaching 480 degrees Celsius. Venus is similar in size to Earth, with radii of 6052 km and 6371 km respectively, and both planets are approximately 4.5 billion years old. Several spacecraft have explored Venus over the past 50 years, mapping over 98% of its surface and finding it to be covered in volcanoes and craters with an atmosphere composed primarily of carbon dioxide.
EarthScience Venus Report
Ancient astronomers did not understand that Venus was a planet orbiting the Sun. Copernicus first proposed that the Sun, not Earth, was the center of our solar system, with planets like Venus orbiting around it. Galileo later observed Venus through a telescope and confirmed this theory by seeing it go through phases like the Moon, showing it orbits the Sun rather than Earth. The first transit of Venus across the Sun's disk in 1639 provided further evidence of this heliocentric model of the solar system.
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Venus is named after the Roman god of beauty and was the second planet from the sun. It has an extremely hot surface temperature that would instantly kill any human visitors due to its dense carbon dioxide atmosphere and surface of lava and volcanoes. Despite being similar in size to Earth, Venus has extreme environmental conditions that are inhospitable to life as we know it compared to the more temperate climate on Earth.
Planet Venus, the Veiled and Hottest Planet
Venus is Earth's closest planetary neighbor with similarities in size, mass, and composition. It has a dense carbon dioxide atmosphere and experiences extreme surface temperatures around 864 degrees F due to greenhouse gas warming. Venus rotates backwards compared to Earth and has no magnetic field. It has been explored by numerous spacecraft but cannot support life due to the hostile conditions.
The planet venus
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.
Venus
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
''Venus'' - The Second planet of our solar system.Lets discuss about this planet.
Hope You Like it
By:- slide_maker4u
(Abhishek Sharma)
Venus
Venus is the second planet from the Sun and is the hottest planet in our Solar System with surface temperatures reaching 480 degrees Celsius. Venus is similar in size to Earth, with radii of 6052 km and 6371 km respectively, and both planets are approximately 4.5 billion years old. Several spacecraft have explored Venus over the past 50 years, mapping over 98% of its surface and finding it to be covered in volcanoes and craters with an atmosphere composed primarily of carbon dioxide.
EarthScience Venus Report
Ancient astronomers did not understand that Venus was a planet orbiting the Sun. Copernicus first proposed that the Sun, not Earth, was the center of our solar system, with planets like Venus orbiting around it. Galileo later observed Venus through a telescope and confirmed this theory by seeing it go through phases like the Moon, showing it orbits the Sun rather than Earth. The first transit of Venus across the Sun's disk in 1639 provided further evidence of this heliocentric model of the solar system.
Science project (powerpoint)
Venus is the second planet from the sun. It has no rings and its atmosphere is dense and cloudy, making the surface impossible to see from space. Venus has about 85% of Earth's gravity and would weigh a 100 lb person about 90 lbs. The document provides fictional descriptions of life, real estate, transportation, and shopping on Venus to entertain readers.
Red faction powerpoint
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.
Mercury
Mercury is the planet closest to the Sun, located about 36 million miles away. It is named after the Roman messenger god Mercury. Mercury has extreme temperature variations between day and night, with daytime temperatures reaching 800 degrees Fahrenheit and nighttime temperatures plunging to -280 degrees. Mercury also has a very thin atmosphere and no moons or evidence of current geological activity.
Facts About Venus
Venus is often referred to as Earth's sister planet due to their similar size and mass, with Venus having a diameter only 638 km smaller than Earth's and 81.5% of Earth's mass. However, Venus has an atmospheric pressure 92 times greater than Earth's due to its dense carbon dioxide atmosphere, which causes a greenhouse effect that makes its average surface temperature a scorching 462 degrees Celsius, with no seasonal variation.
The Planet Mercury
The document provides information about the planet Mercury:
- Mercury is the closest planet to the sun and orbits it the fastest of all planets due to its small orbital radius.
- It has no moons and rotates very slowly, with a day lasting almost two of its months.
- NASA's Mariner 10 and MESSENGER probes helped reveal Mercury's heavily cratered surface and thin atmosphere through fly-bys and orbital observations.
Mercury
Mercury is the planet closest to the Sun. It has extreme temperature variations between day and night due to its proximity to the Sun and lack of atmosphere. The landscape is heavily cratered due to asteroid impacts over billions of years. Only two spacecrafts have visited Mercury, finding a terrain shaped by ancient impacts. Future missions aim to better understand Mercury's composition, magnetic field, and two sunrises visible from certain locations due to its long days.
Venus
Venus is the second planet from the sun and has no moons. It is slightly smaller than Earth but has the hottest surface temperature of any planet at 462 degrees Celsius. Venus rotates counter-clockwise and has a day that lasts longer than its year, making it unique among the planets in the solar system.
Mercury
Mercury is the smallest planet in the solar system and orbits the Sun every 88 Earth days. It rotates slowly, with a day lasting almost 60 Earth days. Mercury has almost no atmosphere and its surface is heavily cratered due to meteor impacts. It is named after the Roman messenger god Mercury and is the closest planet to the Sun, with surface temperatures varying greatly between very hot and very cold.
Sophie & char formation of the solar system
The solar system formed from a giant cloud of gas and dust that collapsed under gravity around the sun approximately 4.6 billion years ago. A supernova may have triggered the collapse of the cloud. The planets formed from circling disks of debris left over from the formation of the sun. While the sun contains 99.9% of the mass of the solar system, the planets combined contain 99.7% of its angular momentum due to their orbital motion. Water and other volatiles are found throughout the outer solar system, though Earth has by far the largest stores of liquid water.
The planets in the solar system
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.
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2 planet Venus
Venus is the second planet from the Sun and named after the Roman goddess of beauty. It is a terrestrial planet similar in composition to Earth but has extreme surface temperatures due to its dense carbon dioxide atmosphere. The first images of Venus' surface were obtained by Soviet spacecraft in the late 1960s as earlier spacecraft struggled to photograph the surface through the thick cloud cover. Venus rotates backwards compared to Earth and has no natural satellites.
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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.
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The document discusses evidence that asteroids, comets, and dwarf planets originated from a planet called Astra that was destroyed billions of years ago. Data from the Rosetta mission showed that Comet 67P resembled material from Earth's oceans, supporting the theory that it originated from Astra's oceans. Images of asteroids revealed some have spherical shapes, likely from molten rock ejected during Astra's destruction. The document argues this new data contradicts older theories and supports Astra being shattered to form the asteroids and comets we observe today.
The inner planets and the jupiter
Jupiter is the largest planet in the solar system with over 67 moons. It has a diameter over 11 times larger than Earth and is made up primarily of gas. Jupiter rotates very quickly, taking under 10 hours to complete a rotation. It has a strong magnetic field and the iconic Great Red Spot storm has raged for over 300 years.
J avier polanco-venus-20130919
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.
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Venus is the second planet from the sun. It has no rings and its atmosphere is dense and cloudy, making the surface impossible to see from space. Venus has about 85% of Earth's gravity and would weigh a 100 lb person about 90 lbs. The document provides fictional descriptions of life, real estate, transportation, and shopping on Venus to entertain readers.
Red faction powerpoint
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- 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.
Mercury
Mercury is the planet closest to the Sun, located about 36 million miles away. It is named after the Roman messenger god Mercury. Mercury has extreme temperature variations between day and night, with daytime temperatures reaching 800 degrees Fahrenheit and nighttime temperatures plunging to -280 degrees. Mercury also has a very thin atmosphere and no moons or evidence of current geological activity.
Facts About Venus
Venus is often referred to as Earth's sister planet due to their similar size and mass, with Venus having a diameter only 638 km smaller than Earth's and 81.5% of Earth's mass. However, Venus has an atmospheric pressure 92 times greater than Earth's due to its dense carbon dioxide atmosphere, which causes a greenhouse effect that makes its average surface temperature a scorching 462 degrees Celsius, with no seasonal variation.
The Planet Mercury
The document provides information about the planet Mercury:
- Mercury is the closest planet to the sun and orbits it the fastest of all planets due to its small orbital radius.
- It has no moons and rotates very slowly, with a day lasting almost two of its months.
- NASA's Mariner 10 and MESSENGER probes helped reveal Mercury's heavily cratered surface and thin atmosphere through fly-bys and orbital observations.
Mercury
Mercury is the planet closest to the Sun. It has extreme temperature variations between day and night due to its proximity to the Sun and lack of atmosphere. The landscape is heavily cratered due to asteroid impacts over billions of years. Only two spacecrafts have visited Mercury, finding a terrain shaped by ancient impacts. Future missions aim to better understand Mercury's composition, magnetic field, and two sunrises visible from certain locations due to its long days.
Venus
Venus is the second planet from the sun and has no moons. It is slightly smaller than Earth but has the hottest surface temperature of any planet at 462 degrees Celsius. Venus rotates counter-clockwise and has a day that lasts longer than its year, making it unique among the planets in the solar system.
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Sophie & char formation of the solar system
The solar system formed from a giant cloud of gas and dust that collapsed under gravity around the sun approximately 4.6 billion years ago. A supernova may have triggered the collapse of the cloud. The planets formed from circling disks of debris left over from the formation of the sun. While the sun contains 99.9% of the mass of the solar system, the planets combined contain 99.7% of its angular momentum due to their orbital motion. Water and other volatiles are found throughout the outer solar system, though Earth has by far the largest stores of liquid water.
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Mercury hanhan
Mercury is the closest planet to the Sun and has the shortest year of any planet. It rotates once every 58 Earth days. Mercury has a very thin atmosphere and experiences extreme temperature variations between day and night, with daytime temperatures reaching up to 840°F and nighttime temperatures dropping as low as -275°F. Mercury has a heavily cratered surface and its interior is mostly metallic iron and rock.
Our solar system
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.
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2 planet Venus
Venus is the second planet from the Sun and named after the Roman goddess of beauty. It is a terrestrial planet similar in composition to Earth but has extreme surface temperatures due to its dense carbon dioxide atmosphere. The first images of Venus' surface were obtained by Soviet spacecraft in the late 1960s as earlier spacecraft struggled to photograph the surface through the thick cloud cover. Venus rotates backwards compared to Earth and has no natural satellites.
The solar system
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.
Slide 4
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 Solar System
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.
1 hrly gs ch 01 solar system part 1
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.
The Fifth Planet I
The document discusses evidence that asteroids, comets, and dwarf planets originated from a planet called Astra that was destroyed billions of years ago. Data from the Rosetta mission showed that Comet 67P resembled material from Earth's oceans, supporting the theory that it originated from Astra's oceans. Images of asteroids revealed some have spherical shapes, likely from molten rock ejected during Astra's destruction. The document argues this new data contradicts older theories and supports Astra being shattered to form the asteroids and comets we observe today.
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J avier polanco-venus-20130919
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.
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Inside the planets of the solar system
The document summarizes information about the inner planets Mercury, Venus, Earth, and Mars. Mercury is the smallest planet and closest to the Sun. Venus has a dense atmosphere composed primarily of carbon dioxide and has the hottest surface temperature. Earth has three main layers that support life - the atmosphere, hydrosphere, and geosphere. Mars has a thin carbon dioxide atmosphere, polar ice caps, evidence of past liquid water, and the largest volcano in the solar system.
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Inside the planets of the solar system
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Inside the planets of the solar system
The document summarizes information about the inner planets Mercury, Venus, Earth, and Mars. Mercury is the smallest planet and closest to the Sun. Venus has a dense atmosphere composed primarily of carbon dioxide and has the hottest surface temperature. Earth has three main layers that support life - the atmosphere, hydrosphere, and geosphere. Mars has a thin carbon dioxide atmosphere, polar ice caps, the largest volcano and canyon in the solar system, and evidence suggests it once had liquid water on its surface.
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The document provides an overview of astronomy presented by Hassan Abdullah and Mujtaba Yar Khan. It defines astronomy as the study of celestial bodies such as stars, planets, comets, galaxies and other phenomena in space. It discusses key topics including stars, which are spheres of gas held together by gravity; planets like Earth, Mars and Jupiter; asteroids, meteoroids and meteorites; comets; black holes; and quasars, the brightest objects in the universe. The life cycle of stars is also summarized, from their formation in nebulae through nuclear fusion and eventual explosion in a supernova.
The Solar System by VI - Edison (PASAY CITY WEST HIGH SCHOOL, 2012)
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
Planets
The document summarizes key information about the planets in our solar system. It discusses the inner planets Mercury, Venus, Earth, and Mars, as well as the outer planets Jupiter, Saturn, Uranus, Neptune. It also covers dwarf planets Pluto, Ceres, and Eris. Some of the key details provided include Mercury having cliffs up to 3km high, Venus rotating backwards and having the hottest surface, Earth having water and life, and Mars having the largest volcano and a thin atmosphere.
Solar System Compfor Teachers 1
The document is an educational piece about the solar system that consists of 9 planets revolving around the sun. It provides details about each planet from an astronomy and mythology perspective, including facts about their physical characteristics and the Greek/Roman gods they were named after. It concludes with a short quiz testing knowledge about the planets.
Solar System Compfor Teachers 1
The document is an illustrated guide to the solar system that provides facts about the sun and eight planets in 3 sentences or less per planet. It includes information about the mythology and physical characteristics of each celestial body, and concludes with multiple choice questions about the content.
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There are 8 major planets in our solar system: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. The inner planets are made of rock and include Mercury, Venus, Earth, and Mars. The outer planets are mostly made of gases and include Jupiter, Saturn, Uranus, and Neptune. There are also 3 dwarf planets: Pluto, Ceres, and Eris. Each planet has unique characteristics such as atmospheric composition, rotation, and presence of moons.
Planets of the solar system kevin yu
There are 8 major planets in our solar system: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. The inner planets are made of rock and include Mercury, Venus, Earth, and Mars. The outer planets are made mostly of gases and include Jupiter, Saturn, Uranus, and Neptune. There are also 3 dwarf planets: Pluto, Ceres, and Eris. Each planet has unique characteristics such as atmospheric composition, rotation, and presence of moons.
Solar system 2011
The document provides information about the planets in our solar system:
- Mercury is the closest planet to the sun and has no moons. It has large temperature variations.
- Venus is very hot and cloudy with sulfuric acid clouds. It rotates in the opposite direction of other planets.
- Jupiter is the largest planet and has 49 moons. It has a big red storm on its surface.
- Saturn has rings made of ice, dust and rocks. It is the second largest planet and has 18 moons.
Planets of Solar System
The document provides information about the sun and 9 astronomical bodies in our solar system. It describes each object's key facts such as its distance from the sun, size, composition, discovery, and naming. The sun is a medium-sized star that is over 5 billion years old and will live for another 5 billion years. It provides light and heat to power life on Earth. The planets range significantly in size, from Mercury being slightly larger than Earth's moon to Jupiter being the largest planet in the solar system.
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The Solar System by VI - Edison (PASAY CITY WEST HIGH SCHOOL, 2012)
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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.
An Exploration of the Comet
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.
A Brief History of Texas
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.
Solar System’s Most Enigmatic Planet: Saturn
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, the 50th State of U.S.A.
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
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.
Facts about flags
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".
Communication skills
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 Careers
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 World's First Computer
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.
Understanding Solar Eclipses
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 Hamilton
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.
Mexico's Chichen Itza
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.
More from Amita Vadlamudi (20)
Women of the American Revolution - Elizabeth Schuyler Hamilton
Women of the American Revolution - Elizabeth Schuyler Hamilton
Recently uploaded
Summary Of transcription and Translation.pdf
Hello Everyone Here We are Sharing You with The process of protien Synthesis in very short points you will be Able to understand It Very well
HUMAN EYE By-R.M Class 10 phy best digital notes.pdf
Class 10 human eye notes physics
Handwritten best quality
Direct Seeded Rice - Climate Smart Agriculture
Direct Seeded Rice - Climate Smart AgricultureInternational Food Policy Research Institute- South Asia Office
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 young
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.
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...
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
Authoring a personal GPT for your research and practice: How we created the Q...
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.
Describing and Interpreting an Immersive Learning Case with the Immersion Cub...
Current descriptions of immersive learning cases are often difficult or impossible to compare. This is due to a myriad of different options on what details to include, which aspects are relevant, and on the descriptive approaches employed. Also, these aspects often combine very specific details with more general guidelines or indicate intents and rationales without clarifying their implementation. In this paper we provide a method to describe immersive learning cases that is structured to enable comparisons, yet flexible enough to allow researchers and practitioners to decide which aspects to include. This method leverages a taxonomy that classifies educational aspects at three levels (uses, practices, and strategies) and then utilizes two frameworks, the Immersive Learning Brain and the Immersion Cube, to enable a structured description and interpretation of immersive learning cases. The method is then demonstrated on a published immersive learning case on training for wind turbine maintenance using virtual reality. Applying the method results in a structured artifact, the Immersive Learning Case Sheet, that tags the case with its proximal uses, practices, and strategies, and refines the free text case description to ensure that matching details are included. This contribution is thus a case description method in support of future comparative research of immersive learning cases. We then discuss how the resulting description and interpretation can be leveraged to change immersion learning cases, by enriching them (considering low-effort changes or additions) or innovating (exploring more challenging avenues of transformation). The method holds significant promise to support better-grounded research in immersive learning.
Randomised Optimisation Algorithms in DAPHNE
Slides from talk:
Aleš Zamuda: Randomised Optimisation Algorithms in DAPHNE .
Austrian-Slovenian HPC Meeting 2024 – ASHPC24, Seeblickhotel Grundlsee in Austria, 10–13 June 2024
https://ashpc.eu/
Anti-Universe And Emergent Gravity and the Dark Universe
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.
Immersive Learning That Works: Research Grounding and Paths Forward
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.
Compexometric titration/Chelatorphy titration/chelating titration
Classification
Metal ion ion indicators
Masking and demasking reagents
Estimation of Magnisium sulphate
Calcium gluconate
Complexometric Titration/ chelatometry titration/chelating titration, introduction, Types-
1.Direct Titration
2.Back Titration
3.Replacement Titration
4.Indirect Titration
Masking agent, Demasking agents
formation of complex
comparition between masking and demasking agents,
Indicators/Metal ion indicators/ Metallochromic indicators/pM indicators,
Visual Technique,PM indicators (metallochromic), Indicators of pH, Redox Indicators
Instrumental Techniques-Photometry
Potentiometry
Miscellaneous methods.
Complex titration with EDTA.
Gadgets for management of stored product pests_Dr.UPR.pdf
Insectsplayamajorroleinthedeteriorationoffoodgrainscausingbothquantitativeandqualitativelosses
Wellprovedthatnogranariescanbefilledwithgrainswithoutinsectsastheharvestedproducecontainegg(or)larvae(or)pupae(or)adultinsectinthembecauseoffieldcarryoverinfestationwhichcannotbeavoidedindevelopingcountrieslikeIndia
Simpletechnologiesfortimelydetectionofinsectsinthestoredproduceandtherebyplantimelycontrolmeasures
Sexuality - Issues, Attitude and Behaviour - Applied Social Psychology - Psyc...
A proprietary approach developed by bringing together the best of learning theories from Psychology, design principles from the world of visualization, and pedagogical methods from over a decade of training experience, that enables you to: Learn better, faster!
快速办理(UAM毕业证书)马德里自治大学毕业证学位证一模一样
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留信网认证的作用:
1:该专业认证可证明留学生真实身份
2:同时对留学生所学专业登记给予评定
3:国家专业人才认证中心颁发入库证书
4:这个认证书并且可以归档倒地方
5:凡事获得留信网入网的信息将会逐步更新到个人身份内，将在公安局网内查询个人身份证信息后，同步读取人才网入库信息
6:个人职称评审加20分
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8:在国家人才网主办的国家网络招聘大会中纳入资料，供国家高端企业选择人才
Alternate Wetting and Drying - Climate Smart Agriculture
Alternate Wetting and Drying - Climate Smart AgricultureInternational Food Policy Research Institute- South Asia Office
PPT on Alternate Wetting and Drying 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. Recently uploaded (20)
HUMAN EYE By-R.M Class 10 phy best digital notes.pdf
HUMAN EYE By-R.M Class 10 phy best digital notes.pdf
The debris of the ‘last major merger’ is dynamically young
The debris of the ‘last major merger’ is dynamically young
Tissue fluids_etiology_volume regulation_pressure.pptx
Tissue fluids_etiology_volume regulation_pressure.pptx
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...
Authoring a personal GPT for your research and practice: How we created the Q...
Authoring a personal GPT for your research and practice: How we created the Q...
Describing and Interpreting an Immersive Learning Case with the Immersion Cub...
Describing and Interpreting an Immersive Learning Case with the Immersion Cub...
Anti-Universe And Emergent Gravity and the Dark Universe
Anti-Universe And Emergent Gravity and the Dark Universe
Immersive Learning That Works: Research Grounding and Paths Forward
Immersive Learning That Works: Research Grounding and Paths Forward
Compexometric titration/Chelatorphy titration/chelating titration
Compexometric titration/Chelatorphy titration/chelating titration
Gadgets for management of stored product pests_Dr.UPR.pdf
Gadgets for management of stored product pests_Dr.UPR.pdf
Sexuality - Issues, Attitude and Behaviour - Applied Social Psychology - Psyc...
Sexuality - Issues, Attitude and Behaviour - Applied Social Psychology - Psyc...
Alternate Wetting and Drying - Climate Smart Agriculture
Alternate Wetting and Drying - Climate Smart Agriculture
Planet Venus
- 2. The most Luminous Planet in the Solar System
- 3. The planet Venus is named after the Roman Goddess of Love and Beauty, also known as Aphrodite in Greek mythology. It is given such a name because it is the most luminous planet of all. It is one of the few planets that people have been aware of since prehistoric times. Ancient historians believed that Venus was comprised of two separate heavenly bodies: Eosphorus (the morning star) and Hesperus (the evening star). In Latin, these stars were known as Vesper and Lucifer respectively.
- 4. Venus, is the second planet from the sun. Enfolded in volcanoes, it has the hottest atmosphere. Research indicates that Venus is mainly comprised of carbon dioxide and sulfuric acid, resulting in the densest atmosphere than any other planet. Venus revolves itself every 224.7 Earth days, having the slowest and longest solar rotation period.
- 5. Regarded as Earth’s sister, Venus is close to Earth’s size. Its mass is close to 80% of Earth’s. Its diameter is slightly smaller than that of the Earth. Like a moon, Venus goes through phases. When it is observed through a telescope, it appears in a crescent shape. However, when the planet is at a considerable distance, it emerges in a circular shape. To the human eye, Venus may appear floating in a yellow-white color. Up close, it may have a reddish-brown surface.
- 6. Venus has the hottest surface of all planets in the solar system. Various gases, including carbon monoxide, sulfuric acid and carbon dioxide are trapped in the planet’s surface. The planet also contains extremely low levels of water vapors, making the planet as the driest and warmest of all. There is high degree of volcanic activity continuously taking place inside the planet.
- 7. Venus is mainly comprised of 96.5% of carbon dioxide and 3.5% of nitrogen. Due to these gases, the surface temperature of Venus is extreme, averaging about 900 °F (480 °C). This extreme temperature is the reason why armored spacecraft has never been able to survive for more than an hour on its surface.
- 8. Amita Vadlamudi, a former Computer Engineer is a prolific blogger, whose subjects range from history and science to art and fitness. Amita Vadlamudi has published many articles on various subjects on many of her websites, such as Behance and Issuu.