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Age and Origin of the Earth
Age and Origin of the Earth

... to form esteroids. Grew bigger in size became planets. ...
Unit 2 Study Guide (word)
Unit 2 Study Guide (word)

... Served Us Nachos. The beginning of each word in the sentence begins with the same letter of the planet in order from the sun. Inner vs Outer Planets Earth is similar to other planets in many ways. All planets are spheres, rotate on their axis, have gravity, revolve around the sun, have density, and ...
Unit 2 Study Guide - Grant County Schools
Unit 2 Study Guide - Grant County Schools

... Served Us Nachos. The beginning of each word in the sentence begins with the same letter of the planet in order from the sun. Inner vs Outer Planets Earth is similar to other planets in many ways. All planets are spheres, rotate on their axis, have gravity, revolve around the sun, have density, and ...
Aug 2015 supplement - Hermanus Astronomy
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... Big Bang, the universe was full of a fog of hydrogen gas. But as more and more brilliant sources - both stars and quasars powered by huge black holes started to shine, they cleared away the mist and made the universe transparent to ultraviolet light. Astronomers call this the epoch of reionisation, ...
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... Today, the largest telescopes can see about 1011 (100 billion ) galaxies. They are sprinkled throughout the universe. Only three galaxies outside the Milky Way are easily visible to the unaided eye -- the great galaxy in Andromeda and the Large and Small Magellanic Clouds. The distance to the Andro ...
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Our Solar System - sci9sage-wmci

... Dwarf planets are similar to planets in that they orbit the Sun and have a roughly spherical shape, but unlike planets, they have an unusual orbit or orbit in a zone that ...
PPT - University of Arizona
PPT - University of Arizona

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... Huygens is the name of a smaller spacecraft that landed on Titan in 2005. Titan is an interesting moon because it has a thick atmosphere that is thought to be similar to Earth’s atmosphere when the planet was very young. The planet Saturn is 1.4 billion km away from the Sun and it took the spacecraf ...
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... in turn cause sea levels to rise and diminish Earth’s ability to cool itself. Over time, the planet will continue to warm until the oceans evaporate, the surface is blazed, and the entire planet is vaporized by the inferno of the bloated red giant. Although this event is some 5 billion years away, w ...
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... Counting them all When the Universe was young, it was nearly smooth and featureless. As it grew older and developed, it became organised. We know that our solar system is organized into planets (including the Earth) orbiting around the Sun. On a scale much larger than the solar system (about 100 mil ...
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... Borealis or Northern Lights (and the Aurora Australis or Southern Lights). As the solar wind approaches the earth, it gets caught in the earth’s magnet field, the magnetosphere, some of the particles, especially after a massive solar storm, get funneled along the lines of the earth’s magnet field do ...
Paradigm Shifts in Cosmology
Paradigm Shifts in Cosmology

... force so that its effect on the expansion rate is only deceleration. In order to accelerate the expansion, a sort of repulsive force, namely, something that exerts anti-gravity is needed. What we can readily think of is Einstein s cosmological constant. The vacuum energy that caused inflation is al ...
Diameter of the Milky Way
Diameter of the Milky Way

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... such as Iron and Nickel metal, will "sink" to the center of the planet. Lighter material, such as silicates, will float to the top, and as the planet cools, form a solid crust. Secondly, the molten planet will release any gases that were originally trapped in its interior. This outgassing will remov ...
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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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