Ch 9 -venus
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Venus is Earth's closest planetary neighbor with a rocky landscape and thick, toxic atmosphere composed primarily of carbon dioxide. It has no moons or rings and rotates backwards compared to Earth, resulting in sunrises in the west and sunsets in the east. The surface temperature is a scorching 900 degrees Fahrenheit due to a runaway greenhouse effect. Venus is studied through spacecraft missions as it may provide insight into climate change on Earth.
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Ch 8 -mercury
Mercury is the planet closest to the sun, with an eccentric orbit that causes surface temperatures to vary widely between 700K and 100K. It has a 3:2 spin-orbit resonance, resulting in a long day of 176 Earth days. Mercury likely formed from the remnants of a large collision that left it with a high iron content in its core. The MESSENGER mission provided insights into Mercury's weak magnetic field and thin exosphere composed of sodium and oxygen.
Ch 10 -mars
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Ch 11 -jupiter
Jupiter is the 5th planet from the Sun and over 1,300 Earths could fit inside it. It spins rapidly, completing a day in just over 10 hours, and has a year lasting over 12 Earth years. Jupiter has a solid core surrounded by liquid metallic hydrogen and molecular hydrogen. It has a thick atmosphere composed of hydrogen and helium with constant storms, including the Giant Red Spot which has raged for over 150 years. Jupiter has over 67 known moons, with the four largest called the Galilean satellites - Io, Europa, Ganymede, and Callisto.
Ch 12 -saturn1b
Saturn is a giant planet with a diameter of over 58,000 km. It has a hydrogen and helium atmosphere and a core made of metallic hydrogen. Saturn has over 60 moons, the largest being Titan which has a thick nitrogen atmosphere and landscapes resembling those found in Tolkien's books, with rivers and lakes of methane. Another notable moon is Mimas, which resembles the Death Star from Star Wars and shakes internally in a mysterious way.
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Ch 11 -jupiter
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Ch 12 -saturn1b
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Ch 17 -our dynamic sun
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Test automation. Part 1. Организация процесса.
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The document summarizes several innovations presented at an inclusive innovations event in 2013. It describes innovations such as:
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4) Several other medical devices and tools that improve access to healthcare in remote areas and for disabilities.
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Our Solar System contains the Sun and objects that orbit it, including 8 planets. The inner planets are Mercury, Venus, Earth, and Mars. The outer planets are Jupiter, Saturn, Uranus, and Neptune. Many planets have natural satellites (moons). The Sun is at the center and is made mostly of hydrogen and helium. The planets range greatly in size and composition. Smaller objects like asteroids, meteoroids, and comets also orbit the Sun.
The solar system
This document provides an overview of the key components of the solar system including the sun, eight planets, dwarf planets, asteroids, moons, comets, and other celestial bodies. It describes the formation of the solar system from a rotating cloud of gas and dust around the sun 5 billion years ago. Each planet is then summarized with details about its size, composition, distance from the sun, moons, temperature, and other characteristics. The document aims to educate the reader about the makeup and features of our solar system.
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This document provides an overview of the key components of the solar system including the sun, eight planets, dwarf planets, asteroids, moons, comets and other objects that orbit the sun. It describes the physical characteristics and composition of each planet from Mercury to Neptune as well as other bodies like asteroids and moons. Spacecraft missions have provided insights into these objects and uncovered details about their surfaces, atmospheres, temperatures and other attributes.
Planets
The document describes the 8 planets in our solar system (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune) and provides key details about each planet's average distance from the sun, temperature, diameter, composition, atmospheric makeup, number of moons and rings, length of day and year, and surface features. It also includes some additional interesting facts about each planet, such as Mercury possibly having an undiscovered planet interfering with its orbit and Europa and Titan being potential places where life could exist.
Earth's formation ppt
This document summarizes the formation of the solar system according to the core accretion model. It explains that the solar system began as a solar nebula that collapsed under gravity to form the sun. Heavier elements near the sun merged to form terrestrial planets, while lighter elements further from the sun formed gas giants. The earliest Earth had a hot molten surface and atmosphere of gases like hydrogen and carbon dioxide. Over time, the Earth cooled and developed layers, water was introduced via asteroids, and a water cycle, plate tectonics, and life emerged.
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The document provides information about the planets in our solar system, beginning with an overview of the inner planets Mercury, Venus, Earth, and Mars. It then provides more detailed descriptions of each planet, including how they were formed, their physical characteristics like composition, size, atmosphere, and weather. Key details are given about each planet's mass, diameter, distance from the sun, temperature, and when they were first observed.
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Venus is the second planet from the Sun and the hottest planet in the solar system with an average surface temperature of 467°C. Galileo first observed Venus in the 17th century and the Russian scientist Mikhail Lomonosov discovered its dense, cloudy atmosphere in 1761. To survive on Venus, one would need a suit that cools the body, a protective shell, a filter to prevent toxic gases from being inhaled, and a way to increase gravitational pull to account for Venus' 91% of Earth's gravity. Food and water could not be in liquid form due to the extreme heat.
Venus
Venus is the second planet from the Sun and the hottest planet in the solar system with an average surface temperature of 467°C. Galileo first observed Venus in the 17th century and the Russian scientist Mikhail Lomonosov discovered its dense, toxic atmosphere in 1761. To survive on Venus, specialized equipment would be needed to withstand the extreme heat such as a cooling suit, protective shell, air filtration system, and housing made of liquid nitrogen. The planet has evidence of geological features like volcanoes and mountains but its surface appears to consist of a single crustal plate unlike Earth which has plate tectonics.
Venus.ppt
Venus is the second planet from the Sun, with similarities but also key differences compared to Earth. It has no moons, a dense carbon dioxide atmosphere 90 times thicker than Earth's that causes intense surface heating through a runaway greenhouse effect. Radar mapping has revealed Venusian landscapes dominated by volcanic features like mountains and plains, with few impact craters due to ongoing volcanic resurfacing of its surface. The thick CO2 atmosphere is likely a result of Venus originally having oceans that evaporated due to its proximity to the Sun and the greenhouse gases trapping heat.
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The document provides an overview of the solar system, including information about the 8 planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune) and 3 dwarf planets (Pluto, Ceres, Eris). It describes key facts about each celestial body such as their composition, moons, rotation, and orbits. The document aims to inform readers about the general structure and characteristics of objects found in our solar system.
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This document provides an overview of celestial objects and Newtonian mechanics. It begins with definitions and images of different types of galaxies such as spiral, elliptical, lenticular, and irregular galaxies. It then discusses pre-Newtonian theories of planetary motion from Ptolemy to Kepler. Next, it covers Newton's universal law of gravitation and its applications by scientists like Halley, Adams, and Le Verrier for predicting comet orbits and deviations in Uranus' orbit. The document concludes with descriptions of objects in our solar system like planets, dwarf planets, moons, comets, and asteroids, followed by an introduction to exoplanet detection methods like the radial velocity and transit methods.
Facts About Venus
Venus is often referred to as Earth's sister planet due to their similar size and mass, with Venus having a diameter only 638 km smaller than Earth's and 81.5% of Earth's mass. However, Venus has an atmospheric pressure 92 times greater than Earth's due to its dense carbon dioxide atmosphere, which causes a greenhouse effect that makes its average surface temperature a scorching 462 degrees Celsius, with no seasonal variation.
The planets
The document provides information about the 8 planets and 3 dwarf planets in our solar system. It describes their key characteristics such as composition, size, orbital period, rotation period, and natural satellites. The inner planets are smaller rocky bodies, while the outer planets are large gas giants with rings. Features like impact craters, volcanoes, and storms shape the surfaces of different planets.
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Compare and Contrast Earth and Mars- 1st Formative Task
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Ch 20 -galaxies
The Milky Way is a barred spiral galaxy that is warped due to gravitational interactions with its neighboring dwarf galaxies, the Large and Small Magellanic Clouds. It is composed of stars, gas, dust, and contains over 200 billion stars. The Milky Way is home to our solar system and planet Earth.
Ch 19 -life and death of stars
1. Stars are born through nuclear fusion and spend most of their life fusing hydrogen into helium as a main sequence star.
2. When stars exhaust their hydrogen fuel, low mass stars become red giants and high mass stars explode as supernovae.
3. The remnants of dead stars are white dwarfs, neutron stars, or black holes depending on the original star's mass.
Other suns
1. There are three main ways to determine the distance to stars: comparing absolute and apparent magnitude, using parallax to calculate distance, and applying the inverse square law relating luminosity and brightness to distance.
2. Key properties of stars can be determined by their spectra, luminosity, temperature, and location on the Hertzsprung-Russell diagram showing the main sequence of star development.
3. Binary star systems provide information about stellar characteristics and evolution through their gravitational interactions, and some binaries involve mass transfer or lead to supernovae.
Ch 16 -cometsmeteorsasteroids
Asteroids are rocky airless worlds that orbit the sun and are too small to be considered planets. They come in three main types - C, S, and M - and some are potentially hazardous if they come close to Earth. While asteroid impacts were more common in the past, Earth still suffers impacts about once every 2,000 years from asteroids the size of a football field. Comets are made of ice, dust, and rock and form tails when close to the sun as their ices sublimate. Meteors are flashes of light seen when meteorids burn up in Earth's atmosphere, meteorites are meteorids that survive entry and hit the ground.
Ch 15 -the five dwarfs
High School Informaton Power point regarding the Dwarf Planets, the Asteroid Belt and the Kuiper Belt
Ch 13 -uranus
Uranus has a unique axial tilt of 98 degrees, causing its poles to face the sun for 42 years before flipping to face away for the next 42 years. It is an ice giant made up of icy materials like water, methane and ammonia. Uranus has rings and 27 moons, with its largest moons being Titania and Oberon. Its blue-green color is caused by methane in its atmosphere absorbing red light.
Ch 7 -earth
The document discusses several topics related to Earth science, including:
1) The layers of Earth's interior including the crust, mantle, and core. The mantle is partially melted lower down and rigid upper mantle.
2) Plate tectonics and how the movement of tectonic plates at a rate of 3 cm per year explains continental drift and mountain range formation.
3) The atmosphere is divided into four layers - troposphere, stratosphere, mesosphere, and thermosphere - based on temperature, composition, and density.
4) The ozone layer is an atmospheric filter that protects from UV rays, and holes in the ozone are caused by interactions with pollutant gases.
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A simple without much math details about generalities of telescopes for a high school beginning level astronomy class.
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Ch 5 -lensproperties
This document discusses the properties and behavior of convex and concave lenses. It explains that convex lenses form real, inverted images unless the object is placed between the focal point and the lens, in which case it forms a virtual, upright image. It also explains that concave lenses always form virtual, upright images that are smaller than the object. The document provides formulas for calculating the location and size of images formed by lenses and works through two example problems.
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A limited math presentation of the concept of gravitational force for a high school astronomy class.
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Ch 1 - intro
This document summarizes the history and key figures in astronomy from Ptolemy to Newton. It discusses their major contributions, including: Ptolemy's geocentric model of epicycles; Aristotle's observations supporting a spherical Earth; Copernicus' proposal of a heliocentric model; Brahe's observations of supernovae; Galileo's discoveries with telescopes that supported heliocentrism and got him in trouble with the church; Kepler's laws of planetary motion based on Brahe's data; and Newton's laws of motion and universal gravitation, building on prior work.
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Ch 9 -venus
- 1. Venus The hot neighbor next door.
- 2. Stats • Distance from the sun: 67 million miles • Rocky, cratered, and volcanic landscape • Thick and toxic atmosphere made of • CO2, Nitrogen, and clouds of Sulfuric • acid (H2SO4) droplets • Has no moons and no rings • Spins retrograde rotation (backwards) • This means the sun rises in the west • and sets in the east.
- 3. A day on Venus • 1 day = 243 Earth days. • Orbital period around the sun is • 225 Earth days. • Forecast: Cloudy, Cloudy, Cloudy • The temperatures • are hot enough to • melt lead. • 900 degrees F. •
- 4. Gravity on Venus • The acceleration of gravity is 8.87 m/s2 • Mass: 4.87E24 Kg, radius: 6052 km • The planet has been studied by over 40 spacecraft. • Most likely the inhospitable environment • was caused by a runaway greenhouse • effect.
- 5. Transits of Venus • The transits of venus occur in pairs. • More than a century separates • the pairs. Next one in 2117. • Recorded transits: • 1631, 1639, • 1761, 1769, • 1874, 1882, • 2004, 2012,
- 7. Inclination
- 8. Venus Videos • https://www.youtube.com/watch?v=HqF VxWfVtoo • Nasa: Documentary • https://www.youtube.com/watch?v=L1m Ea_Mnc0c
- 9. Videos Continued • https://www.youtube.com/watch?v=TR-IWhZZDJY • This is a documentary 25 minutes long.