Proficiency 4 astronomy science
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The document summarizes key information about the solar system. It describes the inner and outer planets, with the inner planets being terrestrial and the outer being gas giants. It explains that astronomers believe the sun formed from a rotating gas cloud that over time became a star through nuclear fusion. It also notes that the sun is about a third of the way through its lifespan and will eventually expand and shed its outer layers to become a white dwarf.
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The future of our solar system
By analyzing radioactive elements in meteorites, astronomers determined that the solar system formed 4.6 billion years ago from the gravitational collapse of a giant molecular cloud. This cloud collapsed over millions of years to form a rotating disk with the sun at the center. The planets formed from this disk, with the inner rocky planets closer to the sun and the outer gas giants farther away. In around 5 billion years, the Milky Way will collide with the Andromeda galaxy, and the solar system will be about 100,000 light years from the center of the new merged galaxy.
Proficiency #4 for astronomey in science
The document discusses the formation of the solar system. It describes how a large rotating cloud of dust and gas called the Solar Nebula collapsed, forming the sun at the center and flattening particles into planetesimals that became the planets, moons, and other objects in the solar system. It then compares the inner terrestrial planets of Mercury, Venus, Earth and Mars to the outer gas giant planets of Jupiter, Saturn, Uranus and Neptune.
Star life cycle
Stars form from collapsing clouds of gas and dust found in nebulae. A star's life cycle depends on its mass - smaller stars less than 3 times the Sun's mass will spend most of their existence on the main sequence fusing hydrogen. Larger stars evolve more quickly, becoming red giants and eventually exploding as supernovae, leaving behind neutron stars or black holes.
Our sun. Evolution and End.
About 5 billion years ago, a huge cloud of dust and gas in the galaxy collapsed under gravity. As it shrank and became denser, it began to glow and the first nuclear fusion reactions occurred, forming the Sun. Approximately 4.6 billion years later, the Sun has used half of its hydrogen fuel and nuclear reactions now involve carbon, nitrogen, and oxygen. In around 5 billion more years, the Sun will expand into a red giant and engulf the Earth before collapsing into a white dwarf.
History of the solar system
The solar system began as ice and dust that gathered into small rocks and then larger rocks. Over time, the sun formed and pushed away surrounding material as the planets grew and froze into their current forms. The inner planets are closer together and more affected by the sun, while the outer planets are further away. Eventually, the sun will explode in a supernova and destroy the inner three planets.
Origins of the solar system
The sun formed 4.6 billion years ago from a dust cloud that collapsed under gravity. It is made primarily of hydrogen and helium and is about 93 million miles from Earth. As the sun exhausts its hydrogen fuel over billions of years, it will expand into a red giant and later shrink into a white dwarf.
The moon's phases are caused by its orbit around Earth as the sun illuminates different parts of the moon each month from our perspective on Earth. As the moon revolves around us, we see more or less of the side illuminated by the sun, appearing as a waxing and waning crescent, half moon, and full moon over the course of about 29.5 days.
Sun & stars
Stars are huge balls of hot glowing gas that produce heat and light through nuclear fusion reactions. They can vary in temperature, size, brightness, and color, as shown on the Hertzsprung-Russell diagram. Our sun is a yellow middle-aged star around 5 billion years old that is made up mostly of hydrogen and helium. It produces energy through nuclear fusion and provides Earth with various types of electromagnetic radiation like visible light, infrared, and ultraviolet waves.
life cycle of a star
Stars are formed from clouds of gas and dust called nebulae. Nuclear fusion reactions at the center of stars provide energy, allowing them to shine brightly for many years. As stars age and exhaust their hydrogen fuel supply, they evolve through later stages such as red giants, red dwarfs, and white dwarfs. The death of very massive stars occurs in supernova explosions, which may result in the formation of neutron stars or black holes.
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The future of our solar system
By analyzing radioactive elements in meteorites, astronomers determined that the solar system formed 4.6 billion years ago from the gravitational collapse of a giant molecular cloud. This cloud collapsed over millions of years to form a rotating disk with the sun at the center. The planets formed from this disk, with the inner rocky planets closer to the sun and the outer gas giants farther away. In around 5 billion years, the Milky Way will collide with the Andromeda galaxy, and the solar system will be about 100,000 light years from the center of the new merged galaxy.
Proficiency #4 for astronomey in science
The document discusses the formation of the solar system. It describes how a large rotating cloud of dust and gas called the Solar Nebula collapsed, forming the sun at the center and flattening particles into planetesimals that became the planets, moons, and other objects in the solar system. It then compares the inner terrestrial planets of Mercury, Venus, Earth and Mars to the outer gas giant planets of Jupiter, Saturn, Uranus and Neptune.
Star life cycle
Stars form from collapsing clouds of gas and dust found in nebulae. A star's life cycle depends on its mass - smaller stars less than 3 times the Sun's mass will spend most of their existence on the main sequence fusing hydrogen. Larger stars evolve more quickly, becoming red giants and eventually exploding as supernovae, leaving behind neutron stars or black holes.
Our sun. Evolution and End.
About 5 billion years ago, a huge cloud of dust and gas in the galaxy collapsed under gravity. As it shrank and became denser, it began to glow and the first nuclear fusion reactions occurred, forming the Sun. Approximately 4.6 billion years later, the Sun has used half of its hydrogen fuel and nuclear reactions now involve carbon, nitrogen, and oxygen. In around 5 billion more years, the Sun will expand into a red giant and engulf the Earth before collapsing into a white dwarf.
History of the solar system
The solar system began as ice and dust that gathered into small rocks and then larger rocks. Over time, the sun formed and pushed away surrounding material as the planets grew and froze into their current forms. The inner planets are closer together and more affected by the sun, while the outer planets are further away. Eventually, the sun will explode in a supernova and destroy the inner three planets.
Origins of the solar system
The sun formed 4.6 billion years ago from a dust cloud that collapsed under gravity. It is made primarily of hydrogen and helium and is about 93 million miles from Earth. As the sun exhausts its hydrogen fuel over billions of years, it will expand into a red giant and later shrink into a white dwarf.
The moon's phases are caused by its orbit around Earth as the sun illuminates different parts of the moon each month from our perspective on Earth. As the moon revolves around us, we see more or less of the side illuminated by the sun, appearing as a waxing and waning crescent, half moon, and full moon over the course of about 29.5 days.
Sun & stars
Stars are huge balls of hot glowing gas that produce heat and light through nuclear fusion reactions. They can vary in temperature, size, brightness, and color, as shown on the Hertzsprung-Russell diagram. Our sun is a yellow middle-aged star around 5 billion years old that is made up mostly of hydrogen and helium. It produces energy through nuclear fusion and provides Earth with various types of electromagnetic radiation like visible light, infrared, and ultraviolet waves.
life cycle of a star
Stars are formed from clouds of gas and dust called nebulae. Nuclear fusion reactions at the center of stars provide energy, allowing them to shine brightly for many years. As stars age and exhaust their hydrogen fuel supply, they evolve through later stages such as red giants, red dwarfs, and white dwarfs. The death of very massive stars occurs in supernova explosions, which may result in the formation of neutron stars or black holes.
Proficiency #4 for astronomey in science
The solar system formed from a large rotating cloud of dust and gas called the solar nebula. As the nebula collapsed, a section broke off to form the sun at the center, with planetesimals - small particles that formed the planets - orbiting around it. The inner planets of Mercury, Venus, Earth and Mars are smaller and more dense than the outer gas giants of Jupiter, Saturn, Uranus and Neptune. While the inner planets are rocky, the outer planets are large balls of gas.
Proficiency #4 for astronomey in science
The solar system formed from a large rotating cloud of dust and gas called the solar nebula. As the nebula collapsed, a section broke off to form the solar system with the sun at its center. Gravity drew particles together, forming the sun and other planetary bodies like planets, moons, and asteroids. The inner planets are rocky and close to the sun, while the outer planets, or gas giants, are large and more distant.
Proficiency #4 for astronomey in science
The solar system formed from a large rotating cloud of dust and gas called the solar nebula. As the nebula collapsed, a section broke off to form the sun at the center, with planetesimals - small particles that formed the planets - orbiting around it. Over time, gravity caused the particles to come together and form the eight planets in orbits around the growing sun. The inner planets are rocky, while the outer planets are gas giants.
Comets
The document discusses comets, asteroids, meteors, and the differences between them. It provides information on their composition, orbits, and how they are formed. Comets are made of ice and dust that formed in the early solar system. Their tails always point away from the sun due to solar winds. Asteroids are large chunks of rock and metal left over from the formation of the planets. Meteors are small pieces of debris from asteroids and comets that burn up as they fall through the Earth's atmosphere, appearing as shooting stars.
Stars
A supernova is a giant explosion that occurs at the end of a giant star's life, flashing with the brilliance of billions of suns. Pulsars are rapidly spinning neutron stars that emit intense radio pulses. Quasars are extremely luminous objects that are a source of electromagnetic energy and light, generally appearing red in color. Stars are constantly dying and being born, with more massive stars living for only millions of years while medium stars like our Sun will live for billions of years.
Life On Other Planets
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The Solar System
The Solar System consists of the Sun and objects that orbit it, including 8 planets. Mercury is the closest planet to the Sun. Venus is similar in size to Earth but has an intense greenhouse effect. Earth is the only known planet capable of supporting life. Mars is often described as the "Red Planet" with seasonal changes and two moons. Jupiter is the largest planet and has dark and light bands in its atmosphere. Saturn is recognizable by its prominent rings and numerous moons. Uranus rotates on its side and has 27 moons. Neptune has active storm systems and 13 known moons. Pluto is the smallest planet and was reclassified as a dwarf planet in 2006. The Moon is Earth's natural
How a star is born, lives,
Stars are born from clouds of hydrogen and helium gas that collapse under gravity. When the cloud becomes dense and hot enough, nuclear fusion begins at its core, causing the star to shine. A star's properties like size, temperature, and color depend on how much gas was in the original cloud. The Hertzsprung-Russell diagram classifies stars based on these properties and tracks their evolution over millions or billions of years as they fuse elements until dying in a supernova or becoming a black hole or white dwarf. Our sun is a medium-sized yellow star that has fused hydrogen for 4.6 billion years and will continue for another 5 billion years.
Death of a star
Stars eventually die when they exhaust their nuclear fuel. Small stars cool and shrink into white dwarfs, while larger stars that become red giants either shed their outer layers leaving behind dense neutron stars or explode in gigantic supernovae. The oldest stars are around 13.7 billion years old, formed shortly after the Big Bang, while big bright stars only live for around 10 million years and stars like the Sun will live for approximately 10 billion years.
El universo-presentación
Atoms are the smallest units that make up all elements and everything in the universe. Stars are composed mainly of hydrogen and form when clusters of atoms come together. Stars produce light and heat through nuclear fusion, transforming hydrogen into helium, but will eventually run out of fuel and die, shrinking into white and black dwarfs or expanding into red giants. Black holes are regions of extremely dense mass that nothing, not even light, can escape from, and come in supermassive, stellar, and microscopic sizes.
Stars
Stars originate from swirling clouds of gas and dust that condense under gravity to form dense spheres called protostars. As protostars gain mass through accretion, the internal pressure and temperature rises until nuclear fusion of hydrogen begins, forming a main sequence star. Over its lifetime, a main sequence star fuses hydrogen into helium in its core. More massive stars end as supernovae, leaving behind neutron stars or black holes, while less massive stars expand into red giants and later shed their outer layers, leaving behind a fading white dwarf.
Star life cycle
All stars form from collapsing clouds of gas and dust found in nebulae. A star's life cycle depends on its mass - less massive stars will spend most of their existence fusing hydrogen to helium in the main sequence, while more massive stars evolve more quickly. At the end of their lives, some stars will collapse into neutron stars or black holes in supernova explosions.
Solar system formation Claudia and Matthew
Our solar system formed over 4 billion years ago from a giant cloud of gas and dust. An explosion from a nearby star created this cloud, and gravity caused the cloud to collapse and spin, forming a dense, hot center that became our Sun. As the cloud flattened, particles stuck together in the outer regions to form planets like Jupiter, while only rocky planets could form near the Sun due to the intense heat. Over time, this process resulted in the current solar system containing the Sun and eight major planets.
Star formation
The document discusses the lifecycle of stars from their formation to death. It begins by defining what stars and constellations are. It then focuses on our sun as a medium-sized, yellow star at the center of our solar system. Stars are classified based on temperature and brightness as young dwarf stars or older, larger supergiant stars. The document outlines the typical stages a star like the sun will progress through over billions of years from birth from clouds of dust and gas, burning hydrogen through nuclear fusion as a main sequence star, and eventual death through expansion and explosion at the end of its life. Various nebulae and supernova remnants are used as examples of star birth and death.
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1) Earth formed 4.5 billion years ago from a great cloud of dust and gas that collapsed to form the solar system.
2) All planets orbit in the same direction and plane, evidence they formed from the same disk surrounding the young sun.
3) The nebular hypothesis proposes the solar system formed as a giant cloud of dust and gas collapsed, with denser matter clumping together to form planets and planetesimals.
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Proficiency #4 for astronomey in science
The solar system formed from a large rotating cloud of dust and gas called the solar nebula. As the nebula collapsed, a section broke off to form the sun at the center, with planetesimals - small particles that formed the planets - orbiting around it. The inner planets of Mercury, Venus, Earth and Mars are smaller and more dense than the outer gas giants of Jupiter, Saturn, Uranus and Neptune. While the inner planets are rocky, the outer planets are large balls of gas.
Proficiency #4 for astronomey in science
The solar system formed from a large rotating cloud of dust and gas called the solar nebula. As the nebula collapsed, a section broke off to form the solar system with the sun at its center. Gravity drew particles together, forming the sun and other planetary bodies like planets, moons, and asteroids. The inner planets are rocky and close to the sun, while the outer planets, or gas giants, are large and more distant.
Proficiency #4 for astronomey in science
The solar system formed from a large rotating cloud of dust and gas called the solar nebula. As the nebula collapsed, a section broke off to form the sun at the center, with planetesimals - small particles that formed the planets - orbiting around it. Over time, gravity caused the particles to come together and form the eight planets in orbits around the growing sun. The inner planets are rocky, while the outer planets are gas giants.
Comets
The document discusses comets, asteroids, meteors, and the differences between them. It provides information on their composition, orbits, and how they are formed. Comets are made of ice and dust that formed in the early solar system. Their tails always point away from the sun due to solar winds. Asteroids are large chunks of rock and metal left over from the formation of the planets. Meteors are small pieces of debris from asteroids and comets that burn up as they fall through the Earth's atmosphere, appearing as shooting stars.
Stars
A supernova is a giant explosion that occurs at the end of a giant star's life, flashing with the brilliance of billions of suns. Pulsars are rapidly spinning neutron stars that emit intense radio pulses. Quasars are extremely luminous objects that are a source of electromagnetic energy and light, generally appearing red in color. Stars are constantly dying and being born, with more massive stars living for only millions of years while medium stars like our Sun will live for billions of years.
Life On Other Planets
This document discusses the possibility of life existing elsewhere in the universe. It describes evidence of water found on the moon and Mars. It also discusses Europa, one of Jupiter's moons, which may have oceans under its icy surface. The document introduces the Drake Equation, which is used to estimate the number of civilizations in the Milky Way galaxy that may be capable of communication. It notes that based on the Drake Equation, about 10,000 planets should have intelligent life. Finally, it mentions Gliese 581 d as a planet outside our solar system that lies in the habitable zone and may have water on its surface.
The Solar System
The Solar System consists of the Sun and objects that orbit it, including 8 planets. Mercury is the closest planet to the Sun. Venus is similar in size to Earth but has an intense greenhouse effect. Earth is the only known planet capable of supporting life. Mars is often described as the "Red Planet" with seasonal changes and two moons. Jupiter is the largest planet and has dark and light bands in its atmosphere. Saturn is recognizable by its prominent rings and numerous moons. Uranus rotates on its side and has 27 moons. Neptune has active storm systems and 13 known moons. Pluto is the smallest planet and was reclassified as a dwarf planet in 2006. The Moon is Earth's natural
How a star is born, lives,
Stars are born from clouds of hydrogen and helium gas that collapse under gravity. When the cloud becomes dense and hot enough, nuclear fusion begins at its core, causing the star to shine. A star's properties like size, temperature, and color depend on how much gas was in the original cloud. The Hertzsprung-Russell diagram classifies stars based on these properties and tracks their evolution over millions or billions of years as they fuse elements until dying in a supernova or becoming a black hole or white dwarf. Our sun is a medium-sized yellow star that has fused hydrogen for 4.6 billion years and will continue for another 5 billion years.
Death of a star
Stars eventually die when they exhaust their nuclear fuel. Small stars cool and shrink into white dwarfs, while larger stars that become red giants either shed their outer layers leaving behind dense neutron stars or explode in gigantic supernovae. The oldest stars are around 13.7 billion years old, formed shortly after the Big Bang, while big bright stars only live for around 10 million years and stars like the Sun will live for approximately 10 billion years.
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Atoms are the smallest units that make up all elements and everything in the universe. Stars are composed mainly of hydrogen and form when clusters of atoms come together. Stars produce light and heat through nuclear fusion, transforming hydrogen into helium, but will eventually run out of fuel and die, shrinking into white and black dwarfs or expanding into red giants. Black holes are regions of extremely dense mass that nothing, not even light, can escape from, and come in supermassive, stellar, and microscopic sizes.
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Stars originate from swirling clouds of gas and dust that condense under gravity to form dense spheres called protostars. As protostars gain mass through accretion, the internal pressure and temperature rises until nuclear fusion of hydrogen begins, forming a main sequence star. Over its lifetime, a main sequence star fuses hydrogen into helium in its core. More massive stars end as supernovae, leaving behind neutron stars or black holes, while less massive stars expand into red giants and later shed their outer layers, leaving behind a fading white dwarf.
Star life cycle
All stars form from collapsing clouds of gas and dust found in nebulae. A star's life cycle depends on its mass - less massive stars will spend most of their existence fusing hydrogen to helium in the main sequence, while more massive stars evolve more quickly. At the end of their lives, some stars will collapse into neutron stars or black holes in supernova explosions.
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Our solar system formed over 4 billion years ago from a giant cloud of gas and dust. An explosion from a nearby star created this cloud, and gravity caused the cloud to collapse and spin, forming a dense, hot center that became our Sun. As the cloud flattened, particles stuck together in the outer regions to form planets like Jupiter, while only rocky planets could form near the Sun due to the intense heat. Over time, this process resulted in the current solar system containing the Sun and eight major planets.
Star formation
The document discusses the lifecycle of stars from their formation to death. It begins by defining what stars and constellations are. It then focuses on our sun as a medium-sized, yellow star at the center of our solar system. Stars are classified based on temperature and brightness as young dwarf stars or older, larger supergiant stars. The document outlines the typical stages a star like the sun will progress through over billions of years from birth from clouds of dust and gas, burning hydrogen through nuclear fusion as a main sequence star, and eventual death through expansion and explosion at the end of its life. Various nebulae and supernova remnants are used as examples of star birth and death.
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1) Earth formed 4.5 billion years ago from a great cloud of dust and gas that collapsed to form the solar system.
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Professor’s Questions Set 5Provide comprehensive answers to th.docx
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Chapter 7 and 8 Readings
1. Why is Jupiter so much richer in hydrogen and helium than Earth?
2. Why do astronomers conclude that none of the Jovian planets’ rings can be left over from the formation of the planets?
3. How can Jupiter have a liquid interior and not have a definite liquid surface?
4. Why are Uranus and Neptune respectively green-blue and blue?
5. What evidence indicates that catastrophic impacts have occurred in the solar system’s past?
6. Why do astronomers refer to carbonaceous chondrites as unmodified or “primitive” materials?
7. What evidence indicates that the asteroids are mostly fragments of larger bodies?
8. What is the difference between condensation and accretion?
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Origin of the Solar System and Extrasolar Planets
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The solar system is our home in the universe. As humans are an intelligent species, we have the right and the responsibility to wonder what we are. Our kind has inhabited this solar system for at least a million years. However, only within the last hundred years have we begun to understand what a solar system is.
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You are linked through a great chain of origins that leads backward through time to the first instant when the universe began 13.7 billion years ago.The gradual discovery of the links in that chain is one of the most exciting adventures of the human intellect.
The Great Chain of Origins
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Earlier, you have studied some of that story:Origin of the universe in the big bangFormation of galaxiesOrigin of starsProduction of the chemical elementsHere, you will explore further and consider the origin of planets.
The Great Chain of Origins
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By the time the universe was three minutes old, the protons, neutrons, and electrons in your body had come into existence. You are made of very old matter.
The History of the Atoms in Your Body
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Although those particles formed quickly, they were not linked together to form the atoms that are common today.Most of the matter was hydrogen and about
25 percent was helium. Very few of the heavier atoms were made in
the big bang.
The History of the Atoms in Your Body
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Although your body does not contain helium, it does contain many of those ancient hydrogen atoms that have remained unchanged since the universe began.
The History of the Atoms in Your Body
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Planet KF-15
The document describes the planet KF-15, where thousands lived happily until it was discovered that the planet was getting closer to its star Gobata and in danger of being destroyed. Zaid, the creator of all objects on the planet using his mind, realized there was no way to save everyone and sent his creations and knowledge in a video message as the planet was destroyed when the star imploded.
Science Squad An Introduction to STEAM
[Tiếng Việt bên dưới]
The zany characters of the Science Squad will guide kids ages 5-7 through this engaging, fact-packed book from Robert Winston all about the key STEAM subjects: science, technology, engineering, art, and maths.
This bright and cheery illustrated book for kids ages 5-7 breaks down STEAM subjects, like science and technology, into fun and easily understandable chunks. Join Robert Winston and the Science Squad to unravel the mysteries of the world: find out how robots work, what a food chain is, where lightning comes from, how lungs allow you to breathe, and much more. The Science Squad characters (Science, Technology, Engineering, Art, and Maths) guide the reader through the book and are always on hand with tips, fun facts, and simple explanations. With pages covering living things, the human body, space, physics, geography, math, engineering, and chemistry, this book is a perfect introduction for kids starting to learn about science at school, or those who are just developing an interest in how the world works.
Source: collected by Reading Seed
About Reading Seed:
Website: https://readingseed.wixsite.com/readingseedvn
Facebook: https://www.facebook.com/readingseedvn
Youtube: https://www.youtube.com/channel/UCoNzrQH2XN9XrWSwKtecN9w/about
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Cuốn sách minh họa tươi sáng và vui nhộn này dành cho trẻ em từ 5-7 tuổi chia nhỏ các chủ đề STEAM, như khoa học và công nghệ, thành các phần vui nhộn và dễ hiểu. Hãy tham gia cùng Robert Winston và Biệt đội Khoa học để làm sáng tỏ những bí ẩn của thế giới: tìm hiểu cách thức hoạt động của robot, chuỗi thức ăn là gì, tia sét đến từ đâu, phổi cho phép bạn thở như thế nào, v.v. Các nhân vật của Biệt đội Khoa học (Khoa học, Công nghệ, Kỹ thuật, Nghệ thuật và Toán học) sẽ hướng dẫn người đọc tìm hiểu thông qua các mẹo, sự kiện thú vị và các giải thích đơn giản. Với các trang bao gồm các sinh vật sống, cơ thể con người, không gian, vật lý, địa lý, toán học, kỹ thuật và hóa học, cuốn sách này là một lời giới thiệu hoàn hảo cho trẻ em bắt đầu tìm hiểu về khoa học ở trường hoặc những người mới phát triển sự quan tâm đến cách thế giới hoạt động.
Nguồn: Reading Seed sưu tầm
Về Reading Seed:
Website: https://readingseed.wixsite.com/readingseedvn
Facebook: https://www.facebook.com/readingseedvn
Youtube: https://www.youtube.com/channel/UCoNzrQH2XN9XrWSwKtecN9w/about
Physics Of The Solar System
In our solar system, the differences between planets and other objects mostly occur because of their formation at the birth of our solar system. Although it is very difficult to tell, most scientists believe that our solar system formed from a small chunk of an interstellar gas cloud. If true, the composition of the gas cloud would have caused the composition of our sun as well as that of other objects in our solar system. Once the sun formed, that influenced the formation of the planets. Since it was much warmer closer to the sun, only denser, metallic elements were able to condense. This warmer region is now home to the terrestrial planets, which include Mercury, Venus, Earth, and Mars.
Proficiencies
The Solar System formed from a cloud of dust and gas that was disturbed by a nearby exploding star. This caused the cloud to collapse and spin, forming the Sun in the center and clumps of material that became the planets. The inner planets of Mercury, Venus, Earth and Mars are closer to the Sun and warmer, while the outer planets of Jupiter, Saturn, Uranus and Neptune are farther away and colder. Over time, the Sun will burn out and die, ending the Solar System.
Life on other planets
1) The document discusses the possibility of life existing elsewhere in the universe, beyond Earth. It explores potential habitats on planets and moons in our solar system as well as exoplanets orbiting other stars.
2) Estimates suggest there could be tens of thousands of civilizations in our galaxy alone, and planets like Mars may have supported life in the past or could still harbor microbes.
3) Moons such as Europa and Enceladus seem to have oceans below their icy surfaces that could support microbial life, while Titan has lakes of liquid methane on its surface. Over 400 exoplanets have been discovered so far in distant solar systems.
Life on Other Planets
1) The document discusses the possibility of life existing elsewhere in the universe, beyond Earth. It explores potential habitats on planets and moons in our solar system as well as exoplanets orbiting other stars.
2) Estimates suggest there could be over 10,000 civilizations in our galaxy alone, and many planets and moons in our solar system - such as Mars, Europa, Titan, and Enceladus - show signs of being able to support some form of life.
3) Scientists are discovering hundreds of new exoplanets each month, increasing the chances of finding a planet capable of supporting life outside our solar system, such as the exoplanet Gliese 581 c.
Solar System Essay
The document is a solar system essay that discusses:
1) How our solar system formed from a giant gas cloud that collapsed under gravity 5 billion years ago, forming the sun and planets.
2) It describes the nine major planets - Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune and Pluto.
3) It also mentions smaller bodies like asteroids and comets that orbit the sun.
P1 lesson part one
The document provides an overview of a course on Earth science and the universe. It includes 12 lessons covering topics like mapping the seafloor, plate tectonics, earthquakes and volcanoes, the origin of the universe, the solar system, what we are made of, the extinction of dinosaurs, and whether life exists elsewhere. The first lesson introduces concepts of time, space, the structure of Earth, and the rock cycle. Subsequent lessons will explore these topics in more depth.
The Universe
The document provides an overview of what is known about the universe based on observations from the Hubble Space Telescope. It discusses how ancient models placed Earth at the center, whereas it is now known that Earth revolves around the sun, which is one of billions of stars. Distances to stars are enormous, measured in light years. Stars appear to move due to Earth's rotation. Stars are giant balls of plasma undergoing nuclear fusion, and their life cycles depend on their mass. Galaxies contain billions of stars and come in different shapes. The universe began in a massive explosion known as the Big Bang around 13.8 billion years ago.
Unit 4: How Our Solar System Formed
As stars die out and explode into supernovae, planets begin to form.
Register to explore the whole course here: https://school.bighistoryproject.com/bhplive?WT.mc_id=Slideshare12202017
Origins of the solar system
The sun formed 4.6 billion years ago from a dust cloud that collapsed under gravity. It is made primarily of hydrogen and helium and is about 93 million miles from Earth. As the sun uses up its hydrogen fuel over billions of years, it will expand into a red giant and later shrink into a white dwarf.
The moon's phases are caused by its orbit around Earth as the sun illuminates different parts of the moon each month from our perspective on Earth. As the moon revolves around us, we see more or less of the side that is illuminated by the sun, appearing as a waxing and waning crescent, half moon, and full moon over the course of about 29.5 days.
Formations of the solar system final- Sophie
Stars form from clouds of dust and gas that collapse under their own gravity. As the cloud collapses, a hot protostar forms at the center. Nearby clouds may break into blobs, explaining why most stars exist in pairs or groups. Planets form from disks of dust and gas that surround young stars. As the disk spins, dust clumps stick together, growing into planetesimals that eventually collide and merge into planets. Moons can form alongside planets from leftover material, be captured asteroids, or form from debris after a large impact. Eventually the sun will run out of hydrogen fuel and expand into a red giant, likely consuming the inner planets before collapsing into a white dwarf.
Michael SeedsDana BackmanChapter 8Origin of the So.docx
Michael Seeds
Dana Backman
Chapter 8
Origin of the Solar System and Extrasolar Planets
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The solar system is our home in the universe. As humans are an intelligent species, we have the right and the responsibility to wonder what we are. Our kind has inhabited this solar system for at least a million years. However, only within the last hundred years have we begun to understand what a solar system is.
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You are linked through a great chain of origins that leads backward through time to the first instant when the universe began 13.7 billion years ago.The gradual discovery of the links in that chain is one of the most exciting adventures of the human intellect.
The Great Chain of Origins
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Earlier, you have studied some of that story:Origin of the universe in the big bangFormation of galaxiesOrigin of starsProduction of the chemical elementsHere, you will explore further and consider the origin of planets.
The Great Chain of Origins
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By the time the universe was three minutes old, the protons, neutrons, and electrons in your body had come into existence. You are made of very old matter.
The History of the Atoms in Your Body
*
Although those particles formed quickly, they were not linked together to form the atoms that are common today.Most of the matter was hydrogen and about
25 percent was helium. Very few of the heavier atoms were made in
the big bang.
The History of the Atoms in Your Body
*
Although your body does not contain helium, it does contain many of those ancient hydrogen atoms that have remained unchanged since the universe began.
The History of the Atoms in Your Body
*
During the first few hundred million years after the big bang, matter collected to form galaxies containing billions of stars. You have learned how nuclear reactions inside stars combine low-mass atoms, such as hydrogen, to make heavier atoms.
The History of the Atoms in Your Body
*
Generation of stars cooked the original particles, fusing them into atoms such as carbon, nitrogen, and oxygen. Those are common atoms in your body.Even the calcium atoms in your bones were assembled inside stars.
The History of the Atoms in Your Body
*
Most of the iron in your body was produced by:Carbon fusion in type Ia supernovae Decay of radioactive atoms in the expanding matter ejected by type II supernovae
The History of the Atoms in Your Body
*
Atoms heavier than iron, such as iodine, were created by:Rapid nuclear reactions that can occur only during supernova explosions
The History of the Atoms in Your Body
*
Elements uncommon enough to be expensive—gold, silver, and platinum in the jewelry that humans wear—also were produced: during the violent deaths of rare, massive stars.
The History of the Atoms in Your Body
*
Our galaxy contains at least
100 billion stars, of which the sun is one.The sun formed from a cloud of gas and dust about 5 billion years ago.The atoms in your body were part of that cloud.
Th ...
Solar system ms santos
Here are the key differences between asteroids, comets, and meteoroids:
- Asteroids: Asteroids orbit the Sun and are made of rock and metals. They are usually found in the asteroid belt between Mars and Jupiter.
- Comets: Comets are small icy bodies that orbit the Sun and have long tails made of dust and gas that form when they are heated by the Sun as they orbit. They come from farther out in the Solar System.
- Meteoroids: Meteoroids are much smaller than asteroids and comets, ranging from small grains to large boulders. They orbit the Sun like asteroids. When meteoroids enter Earth's atmosphere, they glow from friction and are called
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Professor’s Questions Set 5Provide comprehensive answers to th.docx
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Proficiency 4 astronomy science
- 1. Proficiency 4 Jessica Brothers
- 2. All eight planets are categorized into 2 different sections, inner and outer planets. Inner planets are the first four planets closet to the Sun. Mercury, Venus, Earth, and Mars. Outer planets are Jupiter, Saturn, Uranus, and Neptune. The planets are characterized by their different features. The inner planets are terrestrial meaning they solid surfaces similar to Earth. And the outer planets are gas giants because they have no solid surfaces and are made of liquids. Planets
- 5. Planet Order
- 6. The Sun and Solar System
- 7. Astronomers believe that the Sun was formed from a giant cloud which was rotating slowly and that the Sun is slightly older than the Earth. Most of this cloud that formed the Solar System was made of hydrogen gases but also contained some oxygen, silicon, and carbon. Solar System’s Birth
- 8. The gases in this cloud started rotating faster and faster until eventually the core became a hot and very dense core. It could now start generating energy through nuclear fusion of the hydrogen. This is when the Sun became a star. The rest of the cloud material broke off and made the planets we know today, this is the Big Bang Theory.
- 10. Our Sun is predicted to be about 1/3 of its way through life. In the next billions and trillions of years the Sun will eventually die. How exactly? Well, over these MANY years the Sun will keep increasing its brightness until it will shed most of its outer layers and the core will become a smoldering white dwarf . The Sun’s Death
- 11. Even though the Sun will eventually end, it does not mean that the human race has to. Scientists and astronomers can explore life on Mars and the Moon for an alternative way of living. But right now, is the spending really worth it? I think that when the time is necessary, and when we have more knowledge of technology and science, in a couple billions of years we should look into these explorations and spend money but as of right now we do not need it. Opinion
- 12. The Sun
- 13. " Death of our Sun." Frontier Homepage Powered by Yahoo!. N.p., n.d. Web. 9 Feb. 2011. <http://www.frontiernet.net/~docbob/sun.htm>. "Inner and Outer Planets." Universe Today. N.p., n.d. Web. 9 Feb. 2011. <http://www.universetoday.com/34577/inner-and-outer-planets/>. "Primer on Space Weather." NOAA / NWS Space Weather Prediction Center. N.p., n.d. Web. 9 Feb. 2011. <http://www.swpc.noaa.gov/primer/primer.html>. "Solar System ." MWCS - Home of the YellowJackets. N.p., n.d. Web. 9 Feb. 2011. <http://mwcs-inet.mwcsk12.org/faculty/tdashnaw/stusites/weblh/solarsystemlh.htm>. "Space." MWCS - Home of the YellowJackets. N.p., n.d. Web. 9 Feb. 2011. <http://163.153.62.5/faculty/tdashnaw/stusites/webng/spaceng.htm>. Strickland, Jonathan. "HowStuffWorks "The Big Bang, Gravity and General Relativity"." Howstuffworks "Science". N.p., n.d. Web. 9 Feb. 2011. <http://science.howstuffworks.com/dictionary/astronomy-terms/space-shape1.htm>. Bibliography