Mars, our Neighbor Red Planet
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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.
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4 planet Mars
Mars is the fourth planet from the Sun and named after the Roman god of war. It has a thin atmosphere composed primarily of carbon dioxide. The surface is dry and cold, with temperatures ranging from about 80°F down to -207°F. Mars has two small moons called Phobos and Deimos that are irregularly shaped and may be captured asteroids. NASA has sent several orbiters and rovers to explore Mars, including Pathfinder, Spirit, Opportunity, and Curiosity. The rovers discovered evidence that Mars once had water on its surface.
Mars the red planet
Mars is the fourth planet from the Sun and is known as the "Red Planet" due to the iron oxide on its surface. It has a thin atmosphere composed primarily of carbon dioxide with traces of other gases. While early theories hypothesized life on Mars, the first flyby mission revealed desert-like terrain and no signs of life. Liquid water cannot exist on the surface today due to low atmospheric pressure, but evidence suggests water once flowed on Mars. With specific conditions like the presence of water and oxygen traces, human life may be possible on Mars in the future.
Mars By Tom
Mars is the fourth planet from the Sun, around 142 million miles away with surface temperatures ranging from about 20°C during the day to -150°C at night. It has an atmosphere composed primarily of carbon dioxide and features craters, volcanoes and mountains, including Olympus Mons which is the largest mountain in the solar system. While water exists on Mars in frozen form, current conditions are too cold and atmospheric composition unsuitable to support life, though some scientists speculate that terraforming efforts could make Mars habitable to life in over 100,000 years.
Ashish
The document provides information about several celestial bodies in our solar system:
The Moon is Earth's only natural satellite. It has dark volcanic maria and bright ancient crustal highlands marked by impact craters. Its prominence and cycle of phases have influenced culture.
Earth formed 4.54 billion years ago and life appeared within its first billion years. Estimates suggest the planet can support life for another 500 million to 2.3 billion years.
Mercury is the closest planet to the Sun with the greatest temperature variations. It has almost no atmosphere and its surface is heavily cratered, indicating geological inactivity for billions of years.
Mars ppt
Mars is the fourth planet from the Sun and has the largest volcano in the Solar System called Olympus Mons. It has polar ice caps and two small irregular moons named Phobos and Deimos that are likely captured asteroids. While no life has been found, some speculate there could be water or even Martians living on Mars.
Exploration Of Mars
this is the exploration of mars with everything including videos
the topics are :
-About Mars
-Atmosphere and surface on Mars
-The Largest Volcano on Mars
- The Seasons on Mars
-Mars, the god of War
-The First Rover
-Mars Exploration Rovers
-Future Exploration of Mars
-and videos
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Since Mars was discovered, mankind has been interested in this planet. Many people find that saving humanity depends on the colonization of the Red Planet. Here are 10 interesting facts about the Mars.
Planet Mars
Learn more about Planet Mars! Check out its characteristics, geological features, facts & figures, exploration efforts, and more.
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4 planet Mars
Mars is the fourth planet from the Sun and named after the Roman god of war. It has a thin atmosphere composed primarily of carbon dioxide. The surface is dry and cold, with temperatures ranging from about 80°F down to -207°F. Mars has two small moons called Phobos and Deimos that are irregularly shaped and may be captured asteroids. NASA has sent several orbiters and rovers to explore Mars, including Pathfinder, Spirit, Opportunity, and Curiosity. The rovers discovered evidence that Mars once had water on its surface.
Mars the red planet
Mars is the fourth planet from the Sun and is known as the "Red Planet" due to the iron oxide on its surface. It has a thin atmosphere composed primarily of carbon dioxide with traces of other gases. While early theories hypothesized life on Mars, the first flyby mission revealed desert-like terrain and no signs of life. Liquid water cannot exist on the surface today due to low atmospheric pressure, but evidence suggests water once flowed on Mars. With specific conditions like the presence of water and oxygen traces, human life may be possible on Mars in the future.
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Mars is the fourth planet from the Sun, around 142 million miles away with surface temperatures ranging from about 20°C during the day to -150°C at night. It has an atmosphere composed primarily of carbon dioxide and features craters, volcanoes and mountains, including Olympus Mons which is the largest mountain in the solar system. While water exists on Mars in frozen form, current conditions are too cold and atmospheric composition unsuitable to support life, though some scientists speculate that terraforming efforts could make Mars habitable to life in over 100,000 years.
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The Moon is Earth's only natural satellite. It has dark volcanic maria and bright ancient crustal highlands marked by impact craters. Its prominence and cycle of phases have influenced culture.
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Mercury is the closest planet to the Sun with the greatest temperature variations. It has almost no atmosphere and its surface is heavily cratered, indicating geological inactivity for billions of years.
Mars ppt
Mars is the fourth planet from the Sun and has the largest volcano in the Solar System called Olympus Mons. It has polar ice caps and two small irregular moons named Phobos and Deimos that are likely captured asteroids. While no life has been found, some speculate there could be water or even Martians living on Mars.
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Planet Mars
Learn more about Planet Mars! Check out its characteristics, geological features, facts & figures, exploration efforts, and more.
Mars About
Mars is composed primarily of basalt and covered in fine iron oxide dust, giving it a red appearance. It has approximately half the radius and one-tenth the mass of Earth. Mars has two small moons called Phobos and Deimos and its day is 24 hours and 39 minutes with years lasting 1.6 Earth years. Surface temperatures vary from -140°C to 20°C and it experiences gigantic global dust storms when closest to the Sun.
Mars
Mars was named after the Roman god of war due to its red color which reminded Romans of blood and war. It orbits the sun every 687 Earth days, meaning a Martian year is about 1.88 Earth years. Mars has two small moons called Phobos and Deimos, and its surface features volcanoes, meteor impacts, and dust storms.
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Mars is the planet after Earth from the Sun, named after the Roman god of war. It is 142 million miles from the Sun, with surface temperatures ranging from -184 to 80 degrees Fahrenheit. While there is frozen water and ice on the surface, scientists have discovered evidence that water once flowed in the valleys. The thin atmosphere is made up of nitrogen, oxygen, argon and carbon dioxide, and scientists want to try building it up over years. Notable features include Olympus Mons, the tallest solar system mountain at over 15 miles high, and two moons named Phobos and Deimos.
Mars facts ppt
Mars is the fourth planet from the sun and is nicknamed the "Red Planet" due to its iron oxide surface. It has the largest volcano in the solar system called Olympus Mons, which is three times taller than Mount Everest. Mars also has the longest canyon in the solar system called Valles Marineris, which spans nearly the entire width of the United States. The surface conditions on Mars are very cold with an average temperature of -87 degrees Fahrenheit and a thin atmosphere composed mostly of carbon dioxide.
Mars
The document discusses key facts about the planet Mars. It describes Mars' thin atmosphere as hazy and red. It notes the Sojourner rover, launched in 1996, was the first to reach Mars' surface. Mars has two small moons named Phobos and Deimos. The document also provides basic facts about Mars' distance from the sun, length of year, size relative to Earth, and that it may have supported life in the past. It was written by four students.
Mars
Mars is named after the Roman god of war due to its red color. It has the largest volcano and canyon in the solar system. Mars has polar ice caps and evidence suggests water ice exists at the poles and mid-latitudes. Many space probes have explored Mars, with about 1/3 failing. The idea of intelligent life on Mars was popular in the late 19th century. Mars represents masculinity and youth in different cultures and is featured in many modern films and books.
Mars presentation
Mars has two moons named Phobos and Deimos. It earned the nickname "Red Planet" due to its reddish appearance that early Italians thought resembled blood, leading them to name it after the Roman god of war, Mars. Mars is the fourth planet from the sun, has a rotation period of 25.5 hours, and is located between Earth and Jupiter. While rovers and probes have explored Mars, no humans have visited due to lack of oxygen and livable conditions.
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To survive on Mars, humans would need protective equipment and shelters to withstand the thin carbon dioxide-rich atmosphere, average temperatures ranging from -120 to -5 degrees Celsius, and low surface gravity of 38% of Earth's. The conditions on Uranus present even greater challenges, with an atmosphere over 80% hydrogen and 15% helium, average temperature of -210 degrees Celsius, and no solid surface under its liquid methane ocean. Both planets would require enclosed self-sustaining environments and life support systems to enable human habitation.
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The document describes the key features of Venus, Earth, and Mars. Venus is the hottest planet and has a thick, toxic atmosphere. Earth is unique for its abundance of life and oxygen in its atmosphere. Mars has the largest volcano and longest canyon in the solar system, and was once likely more Earth-like but now has a thin, inhospitable atmosphere. Though the planets differ in conditions, they share some basic compositional similarities from forming from the same initial cloud of dust and gases.
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Mars is approximately half the size of Earth and less dense, with a thin atmosphere composed mostly of carbon dioxide. Mars has a reddish surface and seasonal polar ice caps, as well as two moons named Phobos and Deimos. Current robotic missions are exploring the Martian surface and environment, with future crewed missions being tested in simulations like the Mars 500 project.
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Mars is the 4th planet from the sun and takes 687 days to complete its orbit. It rotates clockwise, taking 24.6 hours to complete a rotation. Mars has two moons called Phobos and Deimos and temperatures ranging from -87 to -5 degrees C. Evidence suggests there was once liquid water on Mars' surface. Notable features include Olympus Mons, the largest volcano, and Valles Marineris, the largest canyon, and Mars is sometimes called the "red planet" due to its reddish appearance.
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Mars is the fourth planet from the Sun and about half the size of Earth. It has a thin atmosphere composed mostly of carbon dioxide with traces of other gases. Mars has the largest volcano in the solar system called Olympus Mons and deep valleys like Valles Marineris. Past rover missions have found evidence that water once flowed on the Martian surface.
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The document summarizes key features of Mars. It notes that Mars has polar ice caps containing large quantities of water ice. The south polar ice cap contains enough water ice that if melted would cover the entire planet in 11 meters of water. Mars also has large volcanoes like Olympus Mons, the tallest planetary mountain, and deep canyons like Valles Marineris, one of the largest canyons in the solar system. The atmosphere of Mars is thin and has been stripped away over time by solar wind due to Mars losing its magnetosphere.
Mars
Mars has long evoked interest due to observations in 1877 by Italian astronomer Giovanni Schiaparelli who saw thin lines he called canals. Later probes showed these were optical illusions, not actual canals. The planet has a primarily carbon dioxide atmosphere with some nitrogen and water vapor. It experiences seasonal changes including shrinking and growing polar ice caps. Mars has two moons, Phobos and Deimos, with Phobos being larger and closer to Mars.
planet report
Mars is nicknamed the Red Planet due to the iron oxide in its soil. It has a thin atmosphere composed primarily of carbon dioxide. Mars is about half the diameter of Earth and has a day that is only slightly longer than an Earth day. It has two small moons, Phobos and Deimos, that are irregularly shaped and may be captured asteroids. The largest volcano in the solar system, Olympus Mons, and deepest canyon, Valles Marineris, are both located on Mars. Water ice is found at the poles and it is possible that liquid water exists underground. Seasonal dust storms can blanket the entire planet. Mars is considered Earth's closest planetary neighbor and is sometimes called the "Red Planet" or
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Mars About
Mars is composed primarily of basalt and covered in fine iron oxide dust, giving it a red appearance. It has approximately half the radius and one-tenth the mass of Earth. Mars has two small moons called Phobos and Deimos and its day is 24 hours and 39 minutes with years lasting 1.6 Earth years. Surface temperatures vary from -140°C to 20°C and it experiences gigantic global dust storms when closest to the Sun.
Mars
Mars was named after the Roman god of war due to its red color which reminded Romans of blood and war. It orbits the sun every 687 Earth days, meaning a Martian year is about 1.88 Earth years. Mars has two small moons called Phobos and Deimos, and its surface features volcanoes, meteor impacts, and dust storms.
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Mars is the planet after Earth from the Sun, named after the Roman god of war. It is 142 million miles from the Sun, with surface temperatures ranging from -184 to 80 degrees Fahrenheit. While there is frozen water and ice on the surface, scientists have discovered evidence that water once flowed in the valleys. The thin atmosphere is made up of nitrogen, oxygen, argon and carbon dioxide, and scientists want to try building it up over years. Notable features include Olympus Mons, the tallest solar system mountain at over 15 miles high, and two moons named Phobos and Deimos.
Mars facts ppt
Mars is the fourth planet from the sun and is nicknamed the "Red Planet" due to its iron oxide surface. It has the largest volcano in the solar system called Olympus Mons, which is three times taller than Mount Everest. Mars also has the longest canyon in the solar system called Valles Marineris, which spans nearly the entire width of the United States. The surface conditions on Mars are very cold with an average temperature of -87 degrees Fahrenheit and a thin atmosphere composed mostly of carbon dioxide.
Mars
The document discusses key facts about the planet Mars. It describes Mars' thin atmosphere as hazy and red. It notes the Sojourner rover, launched in 1996, was the first to reach Mars' surface. Mars has two small moons named Phobos and Deimos. The document also provides basic facts about Mars' distance from the sun, length of year, size relative to Earth, and that it may have supported life in the past. It was written by four students.
Mars
Mars is named after the Roman god of war due to its red color. It has the largest volcano and canyon in the solar system. Mars has polar ice caps and evidence suggests water ice exists at the poles and mid-latitudes. Many space probes have explored Mars, with about 1/3 failing. The idea of intelligent life on Mars was popular in the late 19th century. Mars represents masculinity and youth in different cultures and is featured in many modern films and books.
Mars presentation
Mars has two moons named Phobos and Deimos. It earned the nickname "Red Planet" due to its reddish appearance that early Italians thought resembled blood, leading them to name it after the Roman god of war, Mars. Mars is the fourth planet from the sun, has a rotation period of 25.5 hours, and is located between Earth and Jupiter. While rovers and probes have explored Mars, no humans have visited due to lack of oxygen and livable conditions.
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The document discusses the layers that make up the interior structure of the moon. It describes four main layers from the surface to the core: the regolith crust, the rigid mantle which is about 1,000 km thick, a non-rigid lower mantle that has been heated, and an inner core. The magnetic field of the moon is very weak, about one ten-millionth of Earth's field. The document also provides information about the number of moons orbiting different planets in our solar system and details on some of the larger and more unique moons.
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To survive on Mars, humans would need protective equipment and shelters to withstand the thin carbon dioxide-rich atmosphere, average temperatures ranging from -120 to -5 degrees Celsius, and low surface gravity of 38% of Earth's. The conditions on Uranus present even greater challenges, with an atmosphere over 80% hydrogen and 15% helium, average temperature of -210 degrees Celsius, and no solid surface under its liquid methane ocean. Both planets would require enclosed self-sustaining environments and life support systems to enable human habitation.
Mars
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Mars is approximately half the size of Earth and less dense, with a thin atmosphere composed mostly of carbon dioxide. Mars has a reddish surface and seasonal polar ice caps, as well as two moons named Phobos and Deimos. Current robotic missions are exploring the Martian surface and environment, with future crewed missions being tested in simulations like the Mars 500 project.
Presentación1
Mars is the 4th planet from the sun and takes 687 days to complete its orbit. It rotates clockwise, taking 24.6 hours to complete a rotation. Mars has two moons called Phobos and Deimos and temperatures ranging from -87 to -5 degrees C. Evidence suggests there was once liquid water on Mars' surface. Notable features include Olympus Mons, the largest volcano, and Valles Marineris, the largest canyon, and Mars is sometimes called the "red planet" due to its reddish appearance.
Lets talk about Planet Mars
Mars is the fourth planet from the Sun and about half the size of Earth. It has a thin atmosphere composed mostly of carbon dioxide with traces of other gases. Mars has the largest volcano in the solar system called Olympus Mons and deep valleys like Valles Marineris. Past rover missions have found evidence that water once flowed on the Martian surface.
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Presentation finish
This document provides a summary of each planet in our solar system from Mercury to Neptune as presented by Elliott Bolton. Key details are given for each planet, such as Mercury being the closest planet to the sun and having little atmosphere, Venus being covered in toxic gases and having extreme heat, Earth being the planet where life exists due to water, and Neptune having the strongest winds and coldest temperatures in the solar system. The sun is described as a big ball of gas at the center of the solar system, and Jupiter is noted as the largest planet with a famous long-lasting red spot storm.
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The document summarizes key features of Mars. It notes that Mars has polar ice caps containing large quantities of water ice. The south polar ice cap contains enough water ice that if melted would cover the entire planet in 11 meters of water. Mars also has large volcanoes like Olympus Mons, the tallest planetary mountain, and deep canyons like Valles Marineris, one of the largest canyons in the solar system. The atmosphere of Mars is thin and has been stripped away over time by solar wind due to Mars losing its magnetosphere.
Mars
Mars has long evoked interest due to observations in 1877 by Italian astronomer Giovanni Schiaparelli who saw thin lines he called canals. Later probes showed these were optical illusions, not actual canals. The planet has a primarily carbon dioxide atmosphere with some nitrogen and water vapor. It experiences seasonal changes including shrinking and growing polar ice caps. Mars has two moons, Phobos and Deimos, with Phobos being larger and closer to Mars.
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Mars is nicknamed the Red Planet due to the iron oxide in its soil. It has a thin atmosphere composed primarily of carbon dioxide. Mars is about half the diameter of Earth and has a day that is only slightly longer than an Earth day. It has two small moons, Phobos and Deimos, that are irregularly shaped and may be captured asteroids. The largest volcano in the solar system, Olympus Mons, and deepest canyon, Valles Marineris, are both located on Mars. Water ice is found at the poles and it is possible that liquid water exists underground. Seasonal dust storms can blanket the entire planet. Mars is considered Earth's closest planetary neighbor and is sometimes called the "Red Planet" or
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This document provides a summary of the planets in our solar system. It describes each planet's key features such as size, composition, notable landmarks, and distance from the sun. The planets included are Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. The sun is also described as a massive ball of gas that provides heat and energy for life on Earth.
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Mars is named after the Roman god of war and appears red due to the presence of iron oxide dust. It has two moons called Phobos and Deimos and a thin atmosphere composed primarily of carbon dioxide. The surface conditions on Mars include low atmospheric pressure, cold temperatures ranging from about -153 to 22 degrees Celsius, and occasional strong winds. Future human travel to Mars faces challenges including developing sufficient propulsion and ensuring crew health and survival on the Martian surface.
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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 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 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.
Contents 3 planets
The document provides an overview of the solar system, including the nine planets and their characteristics. It discusses the inner and outer planets, the rocky and gas planets, and their compositions, sizes, temperatures, and features such as rings and moons. It also describes the asteroid belt and provides details on each planet such as mythology connections, exploration missions, physical properties, and recent reclassification of Pluto as a dwarf planet.
Similar to Mars, our Neighbor Red Planet (20)
All Aboute milky gelaxy (solar system, sun to neptune).pdf
All Aboute milky gelaxy (solar system, sun to neptune).pdf
Solar System - Asiya Bint Ehtesham - Basic Level 3
Solar System - Asiya Bint Ehtesham - Basic Level 3
The Solar System is the Sun and all the objects that orbit around it
The Solar System is the Sun and all the objects that orbit around it
More from Amita Vadlamudi
The Mystery of Black Holes
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.
Our Closest Star, the Sun
Exploring our closest star, the Sun, its makeup, evolution, its place in the universe, and its significance to life on earth.
An Introduction to Japan
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.
Serengeti National Park
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, Our Natural Satellite
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.
Milky way galaxy
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.
Planet Venus
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.
California
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.
Niagara falls
The beautiful Niagara Falls, one of the most visited tourist destinations, located at the border of the United States and Canada.
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.
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Women of the American Revolution - Elizabeth Schuyler Hamilton
Women of the American Revolution - Elizabeth Schuyler Hamilton
Recently uploaded
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.
The cost of acquiring information by natural selection
This is a short talk that I gave at the Banff International Research Station workshop on Modeling and Theory in Population Biology. The idea is to try to understand how the burden of natural selection relates to the amount of information that selection puts into the genome.
It's based on the first part of this research paper:
The cost of information acquisition by natural selection
Ryan Seamus McGee, Olivia Kosterlitz, Artem Kaznatcheev, Benjamin Kerr, Carl T. Bergstrom
bioRxiv 2022.07.02.498577; doi: https://doi.org/10.1101/2022.07.02.498577
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.
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
Pests of Storage_Identification_Dr.UPR.pdf
InIndia-post-harvestlosses-unscientificstorage,insects,rodents,micro-organismsetc.,accountforabout10percentoftotalfoodgrains
Graininfestation
Directdamage
Indirectly
•theexuviae,skin,deadinsects
•theirexcretawhichmakefoodunfitforhumanconsumption
About600speciesofinsectshavebeenassociatedwithstoredgrainproducts
100speciesofinsectpestsofstoredproductscauseeconomiclosses
Travis Hills of MN is Making Clean Water Accessible to All Through High Flux ...
By harnessing the power of High Flux Vacuum Membrane Distillation, Travis Hills from MN envisions a future where clean and safe drinking water is accessible to all, regardless of geographical location or economic status.
在线办理(salfor毕业证书)索尔福德大学毕业证毕业完成信一模一样
学校原件一模一样【微信：741003700 】《(salfor毕业证书)索尔福德大学毕业证》【微信：741003700 】学位证，留信认证（真实可查，永久存档）原件一模一样纸张工艺/offer、雅思、外壳等材料/诚信可靠,可直接看成品样本，帮您解决无法毕业带来的各种难题！外壳，原版制作，诚信可靠，可直接看成品样本。行业标杆！精益求精，诚心合作，真诚制作！多年品质 ,按需精细制作，24小时接单,全套进口原装设备。十五年致力于帮助留学生解决难题，包您满意。
本公司拥有海外各大学样板无数，能完美还原。
1:1完美还原海外各大学毕业材料上的工艺：水印，阴影底纹，钢印LOGO烫金烫银，LOGO烫金烫银复合重叠。文字图案浮雕、激光镭射、紫外荧光、温感、复印防伪等防伪工艺。材料咨询办理、认证咨询办理请加学历顾问Q/微741003700
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三.真实教育部学历学位认证（教育部存档！教育部留服网站永久可查）
四.办理各国各大学文凭(一对一专业服务,可全程监控跟踪进度)
如果您处于以下几种情况：
◇在校期间，因各种原因未能顺利毕业……拿不到官方毕业证【q/微741003700】
◇面对父母的压力，希望尽快拿到；
◇不清楚认证流程以及材料该如何准备；
◇回国时间很长，忘记办理；
◇回国马上就要找工作，办给用人单位看；
◇企事业单位必须要求办理的
◇需要报考公务员、购买免税车、落转户口
◇申请留学生创业基金
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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Methods of grain storage Structures in India.pdf
•Post-harvestlossesaccountforabout10%oftotalfoodgrainsduetounscientificstorage,insects,rodents,micro-organismsetc.,
•Totalfoodgrainproductioninindiais311milliontonnesandstorageis145mt.InIndia,annualstoragelosseshavebeenestimated14mtworthofRs.7,000croreinwhichinsectsaloneaccountfornearlyRs.1,300crores.
•InIndiaoutofthetotalproduction,about30%ismarketablesurplus
•Remaining70%isretainedandstoredbyfarmersforconsumption,seed,feed.Hence,growerneedstoragefacilitytoholdaportionofproducetosellwhenthemarketingpriceisfavourable
•TradersandCo-operativesatmarketcentresneedstoragestructurestoholdgrainswhenthetransportfacilityisinadequate
ESA/ACT Science Coffee: Diego Blas - Gravitational wave detection with orbita...
ESA/ACT Science Coffee: Diego Blas - Gravitational wave detection with orbita...Advanced-Concepts-Team
Presentation in the Science Coffee of the Advanced Concepts Team of the European Space Agency on the 07.06.2024.
Speaker: Diego Blas (IFAE/ICREA)
Title: Gravitational wave detection with orbital motion of Moon and artificial
Abstract:
In this talk I will describe some recent ideas to find gravitational waves from supermassive black holes or of primordial origin by studying their secular effect on the orbital motion of the Moon or satellites that are laser ranged.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. 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.
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
Evidence of Jet Activity from the Secondary Black Hole in the OJ 287 Binary S...
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.
Mending Clothing to Support Sustainable Fashion_CIMaR 2024.pdf
Ozturkcan, S., Berndt, A., & Angelakis, A. (2024). Mending clothing to support sustainable fashion. Presented at the 31st Annual Conference by the Consortium for International Marketing Research (CIMaR), 10-13 Jun 2024, University of Gävle, Sweden.
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.
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Tissue fluids_etiology_volume regulation_pressure.pptx
Tissue fluids_etiology_volume regulation_pressure.pptx
Immersive Learning That Works: Research Grounding and Paths Forward
Immersive Learning That Works: Research Grounding and Paths Forward
The cost of acquiring information by natural selection
The cost of acquiring information by natural selection
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...
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...
Travis Hills of MN is Making Clean Water Accessible to All Through High Flux ...
Travis Hills of MN is Making Clean Water Accessible to All Through High Flux ...
ESA/ACT Science Coffee: Diego Blas - Gravitational wave detection with orbita...
ESA/ACT Science Coffee: Diego Blas - Gravitational wave detection with orbita...
GBSN - Biochemistry (Unit 6) Chemistry of Proteins
GBSN - Biochemistry (Unit 6) Chemistry of Proteins
Alternate Wetting and Drying - Climate Smart Agriculture
Alternate Wetting and Drying - Climate Smart Agriculture
Describing and Interpreting an Immersive Learning Case with the Immersion Cub...
Describing and Interpreting an Immersive Learning Case with the Immersion Cub...
Evidence of Jet Activity from the Secondary Black Hole in the OJ 287 Binary S...
Evidence of Jet Activity from the Secondary Black Hole in the OJ 287 Binary S...
Mending Clothing to Support Sustainable Fashion_CIMaR 2024.pdf
Mending Clothing to Support Sustainable Fashion_CIMaR 2024.pdf
Anti-Universe And Emergent Gravity and the Dark Universe
Anti-Universe And Emergent Gravity and the Dark Universe
Mars, our Neighbor Red Planet
- 1. By Amita Vadlamudi Mars, our Neighbor Red Planet
- 2. Exploration of Mars, our Neighbor Red Planet
- 3. Introduction Mars is the fourth planet from the Sun and is the second smallest planet in the solar system after Mercury. It is named after the Roman god of war and is also often described as the Red Planet. It derives its name from the reddish appearance which it gives off. Needless to say, this reddish appearance is pretty distinctive among the astronomical bodies that are visible to the naked eye.
- 4. Geological Makeup of Mars Mars is a terrestrial planet which has a solid surface made of rocks and metals. Its surface features are reminiscent of the Moon and valleys, deserts and polar ice caps of the Earth. The bright red appearance of rust that Mars gives is because of the iron-rich minerals present, as the loose dust and rock that covers its surface. The soil of the Earth is thought to be similar to this except that it also has some other organic contents to it. When the iron minerals oxidize they cause the soil to look red.
- 5. Mountains of Mars The planet is home to the largest mountain in the entire solar system called Olympus Mons which is roughly 17 miles (27 km) high, that is about 3 times as tall as Mount Everest, and 370 miles (600 km) wide in diameter which is enough to cover New Mexico! This mountain contributes to one of the most volatile volcanoes on Mars, being the largest ones in the entire solar system.
- 6. Moons of Mars Mars has two moons Phobos and Deimos, which were discovered in 1877. The two moons are made entirely of carbon-rich rock mixed with ice and are covered in dust and lose rocks. Mars’s moons are tiny next to the Earth’s moon and are irregularly shaped. They lack the gravity needed to pull themselves into a more circular form.
- 7. Atmosphere on Mars Mars is much colder than Earth, mostly due to its greater distance from the sun. It is said that the Sun is seen as half its size than we see in the Earth. The average temperature is minus 80 degrees in Fahrenheit and minus 60 degrees in Celsius although it can vary from time to time. The carbon dioxide-rich atmosphere of the planet is also roughly 100 less dense than Earth’s but it is still thick enough to support weather, clouds, and winds. It is thought that there was once life on this planet and it might still be capable of supporting human life.
- 8. Life on Mars Though no trace of currently active life has been found on Mars so far, water has been found in the form of ice. Exploration and Research continues full swing on this very interesting red planet.
- 9. About the Author Amita Vadlamudi is the author of many articles on varied subjects including astronomy, science and history. Read Amita Vadlamudi’s latest article “A Look into the Process of Sugar Production” on her Wix site https://amitavadlamudi.wixsite.com/mysite