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The Solar System and our Universe
The Solar System and our Universe

... • The universe will keep on expanding - The galaxies move fast enough to overcome the forces of gravity acting between them. • The expansion will slow down & stop – The galaxies will remain in a fixed position, The gravitational forces will exactly balance the ‘expansion forces. • The universe will ...
Exploring Space
Exploring Space

... Star Birth When the core of the Protostar reaches 10 million K, pressure is so great that nuclear fusion occurs- a star is born  Heat from fusion of hydrogen is released  When balance is maintained from inward pressure (gravity) and outward pressure (heat) the Main-Sequence stage is ...
TABLE OF CONTENTS Page Title Date 1
TABLE OF CONTENTS Page Title Date 1

... space object…it is called the Big Whack Theory. 2. It is moving away from the Earth at a rate of 1½ inches per year. 3. There are flat lands like seas called Marias. Moon Phases pg 12 12•11•14 ...
The universe - Villanova University
The universe - Villanova University

... Doesn’t get any better than that, does it?? ...
The Big Bang - Cobb Learning
The Big Bang - Cobb Learning

... of the other dots (galaxies) change each time you inflated the balloon? Did the galaxies near home or those farther away appear to move the greatest distance? How do you think that Hubble's Law: (the farther something is from Earth, the faster it seemed to be moving away), helped explain the Big Ban ...
P1 The Earth in the Universe
P1 The Earth in the Universe

... Fossils in the layers show which species lived when. Many species have become extinct. Cross-cutting features- if one type of rock cuts across another rock type, it is younger e.g. hot magma can fill cracks in existing rocks and solidify as new rock. These clues only tell us which rocks are older th ...
Astronomy
Astronomy

... The Sun is the closest star to us It is what gives us light and energy for life It is 92 million miles away from Earth = one astronomical unit (AU) It is like a giant nuclear power plant, constantly converting Hydrogen into Helium. (H -> He) It will eventually die out once it loses its fuel source, ...
Astro Unit 1 Notes - Intro to Astronomy
Astro Unit 1 Notes - Intro to Astronomy

Energy Supply Problem - Challenger Learning Center
Energy Supply Problem - Challenger Learning Center

... of the most imaginative writers of that day was Gene Roddenberry, a former war pilot and policeman. He was the man who wrote Star Trek about the starship Enterprise. In this wonderful story, a crew from many countries and many planets live and work together. They explore the far reaches of the unive ...
Benchmark lesson
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... One of the most important tools invented to study the sky was the telescope. Galileo Galilei (1564–1642) was the first to use a telescope to study the sky. Over time, as telescopes became a lot larger and much more powerful, scientists could see deeper and deeper into space. Over the years, scientis ...
Chapter 2 Assignment GEarthOL
Chapter 2 Assignment GEarthOL

... Self-Reflection Survey: Section 2.1 (page 27) Answer the questions below as a means of uncovering what you already know about Earth’s position in space. #1: Explain how we are influenced by Earth’s position in space on a daily basis. ...
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File

... hot, infinitely dense singularity. After its initial appearance, the universe inflated, expanded and cooled, going from very, very small and very, very hot, to the size and temperature of our current universe. It continues to expand and cool to this day and we are inside of it! There is currently de ...
Unit 6 – Earth
Unit 6 – Earth

... The Big Bang is thought to have occurred about 18 000 million years ago. What is the evidence for this? Galaxies are moving away from us as shown by red-shift; The further they are away from us, the faster they are going; Cosmic background microwave radiation is described as "the echoes of the Big B ...
Grade 9 Science – Unit 4
Grade 9 Science – Unit 4

...  The Sun is 109X larger than the Earth  The Sun is the largest object in our Solar System. The Sun contains about 98% of the total solar mass in our Solar System. The mass of the Sun is 332,830X greater than the Earth.  It takes sunlight and 8 MINUTES to reach the Earth from the Sun. How many LIG ...
3-D movies and Planetarium Two
3-D movies and Planetarium Two

... journey to Mars, with surface features based on data from NASA's Mars Global Surveyor spacecraft. Duration: 9 minutes After Stars A red supergiant star is about to end its life – but when the star explodes, will it produce a black hole or a pulsar? Join the reporter Margus, the scientist Dr Jozalin ...
The Sun Notes File
The Sun Notes File

... Plasma is another state of matter The temperature is so high that electrons ...
Lecture 27 (pdf from the powerpoint)
Lecture 27 (pdf from the powerpoint)

... packet contains all the information needed to build an organism ...
Earth`s Moon and Solar System Outline
Earth`s Moon and Solar System Outline

... ● The ________________ and other observations led scientists to the conclusion that the universe is ___________________ ● Computer models that _______________ the expansion, lead to the idea that at one time the universe was a ________________ object of incredible mass and density that ...
Earth`s Moon and Solar System Outline
Earth`s Moon and Solar System Outline

...  The ________________ and other observations led scientists to the conclusion that the universe is ___________________  Computer models that _______________ the expansion, lead to the idea that at one time the universe was a ________________ object of incredible mass and density that ...
20.1 A Solar System is Born
20.1 A Solar System is Born

... The Solar Nebula Nebula – a large cloud of gas and dust in interstellar space • Where stars are born or explode at the end of their lives • Hydrogen, helium, carbon, iron • Two forces that interact with nebulas to create planets and stars – Gravity & Pressure ...
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... “Astronomy is more than the study of stars and planets. It is the study of the universe in which we humans exist. You and I live on a small planet circling a small sun drifting through the universe, but astronomy can take us beyond these boundaries and help us not only see where we are in the univer ...
Galaxy and Beyond
Galaxy and Beyond

... the Sun (can range from 30 - 50 Aus) Astronomical Unit (AU) - is distance b/w Earth & Sun (about 93 million miles) ...
Public Lecture - Size of the Universe
Public Lecture - Size of the Universe

... Clusters of galaxies are grouped into superclusters. Superclusters form filaments and walls around voids. ...
10 Scientific Laws and Theories You Really Should Know
10 Scientific Laws and Theories You Really Should Know

... empirical evidence and coming up with conclusions. – other scientists must be able to replicate the results if the experiment is destined to become the basis for a widely accepted law or theory. ...
Kg m/s2=SI(G) kg2/m2
Kg m/s2=SI(G) kg2/m2

... appears to be around 46x109 light-years not 13.7x109 light-years (as I had previously thought when I had neglected the acceleration of the universe), because the universe is not only expanding in space and advancing forward in time, but for the last several billion years the rate of expansion has be ...
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Outer space



Outer space, or just space, is the void that exists between celestial bodies, including the Earth. It is not completely empty, but consists of a hard vacuum containing a low density of particles, predominantly a plasma of hydrogen and helium as well as electromagnetic radiation, magnetic fields, neutrinos, dust and cosmic rays. The baseline temperature, as set by the background radiation from the Big Bang, is 2.7 kelvin (K). Plasma with a number density of less than one hydrogen atom per cubic metre and a temperature of millions of kelvin in the space between galaxies accounts for most of the baryonic (ordinary) matter in outer space; local concentrations have condensed into stars and galaxies. In most galaxies, observations provide evidence that 90% of the mass is in an unknown form, called dark matter, which interacts with other matter through gravitational but not electromagnetic forces. Data indicates that the majority of the mass-energy in the observable Universe is a poorly understood vacuum energy of space which astronomers label dark energy. Intergalactic space takes up most of the volume of the Universe, but even galaxies and star systems consist almost entirely of empty space.There is no firm boundary where space begins. However the Kármán line, at an altitude of 100 km (62 mi) above sea level, is conventionally used as the start of outer space in space treaties and for aerospace records keeping. The framework for international space law was established by the Outer Space Treaty, which was passed by the United Nations in 1967. This treaty precludes any claims of national sovereignty and permits all states to freely explore outer space. Despite the drafting of UN resolutions for the peaceful uses of outer space, anti-satellite weapons have been tested in Earth orbit.Humans began the physical exploration of space during the 20th century with the advent of high-altitude balloon flights, followed by manned rocket launches. Earth orbit was first achieved by Yuri Gagarin of the Soviet Union in 1961 and unmanned spacecraft have since reached all of the known planets in the Solar System. Due to the high cost of getting into space, manned spaceflight has been limited to low Earth orbit and the Moon.Outer space represents a challenging environment for human exploration because of the dual hazards of vacuum and radiation. Microgravity also has a negative effect on human physiology that causes both muscle atrophy and bone loss. In addition to these health and environmental issues, the economic cost of putting objects, including humans, into space is high.
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