Ch 22 2
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The document provides an overview of exploring space through electromagnetic radiation and different forms of telescopes, satellites, space probes, and missions. It discusses Edwin Hubble discovering the expanding universe, the Hubble Space Telescope, early space missions using rockets, satellites orbiting Earth today for communication and weather, space probes like Voyager capturing images of planets, the first American and Soviet astronauts, Apollo missions landing on the Moon, space stations like Mir and the International Space Station, and past and future Mars missions including the Cassini probe to Saturn.
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Telescopes and space-based observation tools allow humans to observe and study objects in space. Telescopes use lenses and mirrors to collect electromagnetic radiation and produce magnified images. The largest optical telescopes are in Hawaii, with an even larger one currently under construction. Space-based tools like satellites, probes, and rovers have been launched to observe space without atmospheric interference and visit other celestial bodies. The Voyager probes left our solar system, carrying messages about humanity. The International Space Station is an orbiting laboratory built from parts delivered by shuttles and rockets.
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The document summarizes major events and accomplishments in space exploration from the 1950s to the present. It describes the early space race between the US and Soviet Union, including the first artificial satellite, first human in space, and US projects Mercury and Gemini. It then discusses the Apollo program that landed the first humans on the moon in 1969. Modern exploration topics covered include Voyager probes, the Space Shuttle, space stations, the Hubble Space Telescope, and Mars rover missions. Future exploration may involve renewed lunar studies and using the moon as a site for deep space missions.
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Hi !
I have made this presentation for you so that you know what is space and what is space technology.The one who will download it will be the one who has got 95% knowledge of space and
FOR MORE KNOWLEDGE JUST EMAIL ME ON THIS EMAIL ADDRESS
workplaceid154@gmail.com
Thanks for your downloading
(please spread this presentation to all schools and all institute so that the students or people can get to know about space)
NOTE:THIS IS MICROSOFT 2013 PRESENTATION)
I WILL UPLOAD LOWER VERSIONS OF THIS FILE
THANKS (MADE BY IRTAZA ZAFAR AND
HASEEB AHMED FROM THE CITY SCHOOL CHENAB CAMPUS FSD
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Hi !
I have made this presentation for you so that you know what is space and what is space technology.The one who will download it will be the one who has got 95% knowledge of space and
FOR MORE KNOWLEDGE JUST EMAIL ME ON THIS EMAIL ADDRESS
workplaceid154@gmail.com
Thanks for your downloading
(please spread this presentation to all schools and all institute so that the students or people can get to know about space)
NOTE:THIS IS MICROSOFT 2013 PRESENTATION)
I WILL UPLOAD LOWER VERSIONS OF THIS FILE
THANKS (MADE BY IRTAZA ZAFAR AND
HASEEB AHMED FROM THE CITY SCHOOL CHENAB CAMPUS FSD
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The document outlines several "firsts" in space exploration including the first artificial satellite (Sputnik 1), the first animal in space (Laika the dog), and the first human in space (Yuri Gagarin). It discusses early US space missions including Apollo 7 and plans for a space shuttle. In summary, the document traces the major milestones and developments in the early history of space exploration by both the Soviet Union and United States.
PRESENTACION
Space research began in the 20th century with the Chinese using rockets for military purposes. After World War II, the US and Soviet Union started researching outer space, launching early satellites. In 1957, the Soviets launched Sputnik 1, kicking off the Space Race. Major early events included Yuri Gagarin becoming the first human to orbit Earth in 1961. In 1969, Neil Armstrong was the first to walk on the moon. Space stations and satellites were also launched to research the upper atmosphere and space.
Report in science( studying the universe )
Artificial satellites are human-made objects that orbit Earth and other planets. They are used to study planets, help with communications, and observe the universe. Sputnik 1 was the first artificial satellite launched in 1957. Other notable satellites include Luna 2, the first to reach the moon, and Vanguard 1, the longest-living satellite still in space. Space probes like Voyager 1 have explored other planets and space beyond our solar system. The International Space Station is a modular space station in low Earth orbit operated by various space agencies. There are two main theories for the origin and evolution of the universe: the Big Bang theory and the Steady State theory.
My space presentation
The document provides a summary of important space facts from the 1950s through the 2000s. Some key events included the first satellite launched by the USSR in 1957, the first American weather satellite in 1960, Yuri Gagarin becoming the first person in space in 1961, the first woman in space Valentina Tereshkova in 1963, the first lunar soft landing and return of lunar soil samples in the 1960s and 1970s, and the launches of the Voyager and Pioneer probes to explore the outer planets in the 1970s. The space shuttle program and International Space Station construction continued through the 1980s and 1990s.
My space presentation
The document provides a summary of important space facts from the 1950s through the 2000s. Some key events included the first satellite launched by the USSR in 1957, the first American weather satellite in 1960, Yuri Gagarin becoming the first person in space in 1961, the first woman in space Valentina Tereshkova in 1963, the first lunar soft landing and return of lunar soil samples in the 1960s and 1970s, and the launches of the Voyager and Pioneer probes to explore the outer planets in the 1970s. The document also mentions several "firsts" for women in space and spacewalks in the 1980s and the development of the International Space Station in the 2000s.
Space exploration facts
This document summarizes major milestones in space exploration from the past to the present and future. It discusses how Hipparchus created the first accurate star map in 130 BC. It then outlines Galileo's improvements to the telescope in 1609 that allowed him to make discoveries. The document also summarizes the launch of Sputnik 1 in 1957 as the first satellite to orbit Earth and Yuri Gagarin as the first human in orbit in 1961. Major events like the Apollo 11 moon landing in 1969 and Voyager 1 space probe launch in 1977 are highlighted. More recent developments such as the Hubble Space Telescope launched in 1990 and the ongoing International Space Station project are briefly described. The document concludes with details about Virgin Galactic's plans
Space exploration facts
Hipparchus created the first accurate star map around 130 BC. Galileo used the first telescope in 1609 to discover Jupiter's moons and study the sun. The Soviet Union launched Sputnik, the first satellite to orbit Earth in 1957. Yuri Gagarin became the first human in orbit in 1961. NASA landed Neil Armstrong and Buzz Aldrin on the moon in 1969. Voyager 1 is the farthest man-made object in space, launched in 1977. The Hubble Space Telescope was launched in 1990 and has provided the deepest views of the universe. The International Space Station, a collaboration between several countries, began assembly in 1998. Virgin Galactic aims to offer commercial space flights to space tourists starting in the 2010s
F3-Sc-C9.pptx
The document discusses the structure and composition of the Sun. It describes the three main layers of the Sun - the photosphere, chromosphere, and corona. The photosphere is the visible surface and is about 400km thick with a temperature of 6000°C. The chromosphere is about 9600km thick and has a temperature of 15,000°C. The corona has a temperature of over 2,000,000°C. The core of the Sun is over 15,000,000°C and is where hydrogen is fused into helium, releasing energy that powers the Sun.
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Development of space technologies from ancient times up to the present
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Chapter25
Ancient cultures used mythology and everyday objects to name constellations, and modern astronomy recognizes 88 constellations. Some constellations are only visible part of the year as the Earth revolves around the Sun, but circumpolar constellations in the northern sky appear to circle around Polaris and can be seen all year. Astronomers measure stars' absolute and apparent magnitudes, parallax, distance in light-years, and determine temperature based on color, with hotter stars appearing blue-white and cooler stars orange or red.
Comets, asteroids, meteors
Comets are made of dust, rock and frozen gases that vaporize as they near the Sun, forming a coma and tail. Comets eventually break apart after passing by the Sun multiple times. Small pieces of comets are called meteoroids, which appear as meteors or "shooting stars" when burning up in Earth's atmosphere, or meteorites if they reach the ground. Asteroids are rocky bodies like planets that mainly orbit in a belt between Mars and Jupiter.
Chapter 24
The document provides an overview of the solar system, including its origin and components. It discusses:
1) The modern view that the solar system formed from a rotating cloud of gas and dust that condensed to form the Sun and planets as it contracted.
2) The inner planets Mercury, Venus, Earth, and Mars, including characteristics such as temperatures, atmospheres, and evidence of past water on Mars.
3) The outer planets Jupiter, Saturn, Uranus, and Neptune, noting their large sizes and gaseous compositions. Moons and rings are also mentioned.
Ch 23
The document summarizes key properties and motions of Earth and the Moon. It describes how Earth rotates on its axis, causing day and night, and revolves around the Sun, causing years. It also explains that the Moon rotates on its axis and revolves around Earth, and that the changing angles of sunlight cause its phases to cycle over 29.5 days.
Ch 23
Earth rotates on its axis, causing day and night. It also revolves around the sun in an elliptical orbit, causing seasons due to its tilt. The tilt causes different angles of sunlight between the hemispheres throughout the year. The moon rotates at the same rate as it revolves around Earth, always keeping the same face visible. The moon has different phases as it orbits Earth due to the varying amounts of illumination visible from Earth. Eclipses occur when Earth or the moon block sunlight from the other.
Ch 19 ppt
The document summarizes different features of the seafloor geography. It describes the continental shelf, continental slope, abyssal plains, seamounts, mid-ocean ridges, subduction zones, and resources found in different areas of the seafloor. It also discusses life in the oceans including producers, consumers, food chains, reproduction, plankton, nekton, benthos, beach habitats, estuaries, coral reefs, and pollution sources affecting the oceans.
Chapter 18 section iii
Ocean waves are formed by wind blowing over water, with wavelength being the horizontal distance between wave crests and wave height being the vertical distance between crest and trough. Breakers occur when the top of a wave moves faster than the bottom, causing it to collapse. Tides are large gravitational waves caused by the moon and sun, with high tide occurring when the tidal crest reaches shore and low tide when the trough arrives, and tidal range referring to the difference between high and low tide levels. Tidal bores can form when a rising tide enters a narrow river from a wider sea area.
Climate good one
1. A climate is determined by averaging temperature, precipitation, and other factors over many years and influences the types of plants and animals and how people live in a particular area.
2. Latitude, proximity to large bodies of water, ocean currents, mountains, and urban environments impact local climates by affecting temperatures and precipitation patterns.
3. Climate changes over short term seasons and long term periods due to factors like the Earth's orientation to the Sun, volcanic eruptions, and human activities like burning fossil fuels.
Ch 16 weather
Weather refers to the current state of the atmosphere regarding elements like temperature, wind, and moisture. Various factors influence weather, including the sun heating the air and evaporating water from surfaces, which forms clouds and can lead to precipitation when the water condenses. Weather patterns result from the movement of air masses with different properties interacting, such as cold fronts where colder air advances under warmer air. Meteorologists study weather to make forecasts by analyzing weather maps, temperature and pressure readings, and storm conditions.
Atmosphere 15
The document summarizes key aspects of Earth's atmosphere. It describes the early atmosphere and how it has changed over time with the introduction of oxygen and the ozone layer. It then discusses the composition of the modern atmosphere and layers, including the troposphere where humans live and the protective ozone layer in the stratosphere. It also addresses how atmospheric gases transfer heat energy via radiation, conduction and convection, and how wind patterns are formed.
Geologic time chapter 14
The document summarizes major periods in geologic time from the Precambrian era to present day. It describes how trilobites and other early life evolved and adapted to changing environments over millions of years. Major events included the formation of Pangaea during the Paleozoic era and mass extinctions at the boundaries of the Paleozoic and Mesozoic eras. During the Mesozoic, dinosaurs and early mammals appeared while flowering plants evolved in the Cretaceous period. The Cenozoic era saw continued evolution of mammals, mountain building, and the emergence of humans.
Chapter 13
Paleontologists study fossils to reconstruct prehistoric organisms. Fossils form if organisms are quickly buried, with those having hard parts more likely to fossilize. Different types of fossils provide evidence of ancient life, including permineralized remains, carbon films, molds, and casts. Trace fossils provide evidence of organism activities through tracks, burrows, and other traces. Index fossils are abundant fossils that existed for short periods and can be used to correlate rock layers. Examining undisturbed rock layers using the principle of superposition reveals their relative ages, while radiometric dating provides absolute ages in years.
Chapter 12 Volcanoes
Volcanoes form at boundaries where tectonic plates meet, such as at divergent boundaries like the Mid-Atlantic Ridge or at convergent boundaries. The type of eruption depends on the composition of the magma and amount of gases; basaltic magma produces quiet eruptions while magma rich in silica or water causes explosive eruptions. The resulting volcano shape is also influenced by the eruption - shield volcanoes form from fluid basalt lava, cinder cones from tephra ejected in explosions, and composite volcanoes feature layers from both eruption types.
Chapter 11 Earthquakes
Earthquakes occur when rocks break along faults due to forces inside the Earth. This causes the rocks on one side of the fault to move relative to the other side. There are three main types of faults - normal, reverse, and strike-slip - which are caused by different forces. Earthquakes generate seismic waves that move the ground in various directions. Seismographs are used to measure these waves and determine details about the earthquake location and epicenter. The structure of the Earth consists of layers with different densities that seismic waves pass through. While earthquakes are natural, they can cause significant damage, so preparation and building design can help reduce risks to human life and infrastructure.
Chapter 10 ii
1) Scientists discovered underwater mountain ranges called mid-ocean ridges using sound waves, and Harry Hess proposed the theory of seafloor spreading to explain them.
2) Seafloor spreading involves hot material rising at ridges and flowing sideways, carrying the seafloor away as new material cools and forms at the cracks.
3) Evidence for seafloor spreading includes younger rocks at ridges and magnetic reversals recorded in strips of rock parallel to ridges.
Chapter 10 ii
The document summarizes key aspects of plate tectonics theory including:
1) Continents were once joined together in a supercontinent called Pangaea before drifting apart to their current locations, as evidenced by matching coastlines and fossil/rock formations.
2) Seafloor spreading was discovered at mid-ocean ridges and explained how new crust is formed through magma rising at these ridges and pushing plates apart over time.
3) Earth's crust is broken into plates that move atop the mantle, interacting at plate boundaries through spreading, subduction, and transformation, causing volcanic and seismic activity.
Erosional forces
Erosion is the wearing away and movement of surface materials by forces like water, wind, or glaciers. There are several types of erosion including plucking by glaciers, which picks up debris, and abrasion, where wind acts like a sandblaster wearing down rocks. Wind erosion can scatter dust over large areas through deflation and form sand dunes or dust storms in dry, unvegetated regions. Glaciers are powerful erosion agents that can carve U-shaped valleys and leave behind deposits like moraines, eskers, and till when they melt. Erosion shapes the Earth's surface over time.
Erosional forces
Erosion is the wearing away and movement of surface materials by forces like water, wind, or glaciers. There are several types of erosion including plucking by glaciers, which picks up debris, and abrasion, where wind acts like a sandblaster wearing down rocks. Wind erosion can scatter dust over large areas through deflation and form sand dunes or dust storms in dry, unvegetated regions. Glaciers are powerful erosion agents that can carve U-shaped valleys and leave behind deposits like moraines, eskers, and till when they melt. Erosion shapes the Earth's surface over time.
Section ii and iii
Soil formation is a long process influenced by climate, rock type, vegetation, and time. Soil is composed of mineral particles, organic matter, air, and water. It has distinct layers called horizons that differ in composition and depth of organic matter and minerals. Soil type depends on climate, parent rock material, vegetation, and time for development, with some soils taking thousands of years to form.
Ch 7 1 - weathering
Weathering breaks down rocks into sediment through mechanical or chemical processes. Mechanical weathering physically breaks rocks into fragments through forces like wind, water, plant roots, or ice wedging. Chemical weathering uses chemical reactions to dissolve or change minerals, often involving carbonic acid, plant acids, or oxidation when iron is exposed to oxygen. The rates of mechanical versus chemical weathering depend on climate, with mechanical weathering dominating in cold climates and chemical weathering faster in warm, wet climates.
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Ch 22 2
- 1. Chapter 22 Exploring Space
- 9. Edwin P. Hubble Discovered: Universe is Expanding Hubble Space Telescope named after him.
- 11. Hubble Telescope
- 12. Hubble Pictures
- 25. Saturn Taken by Voyager II 1981
- 26. Images from Voyager Space Probes Voyager 2: 1981 Rings of Saturn
- 27. Images from Voyager Space Probes - Voyager 2 - 1989 - Neptune
- 29. Images from Voyager Space Probes
- 32. Men in Space Yuri Gagarin 1 st man to orbit Earth
- 33. Men in Space Alan Shepherd John Glenn