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1. Base your answer to the following question
1. Base your answer to the following question

... (3) ultraviolet-ray end of the electromagnetic spectrum (4) gamma-ray end of the electromagnetic spectrum 27. The diagram below shows a standard spectrum compared to a spectrum produced from a distant star. ...
10 Million light-years Million light
10 Million light-years Million light

... Million light-years. Our galaxy is indistinguishable from the other galaxies in our Local Group. It would take light over 10 million years to travel across this image. ...
www.astro.utu.fi
www.astro.utu.fi

... Gravitational radiation--orbits of stars left in the central parts of the Galaxy will eventually decay for a star like the Sun, the decay timescale is of order 1024 years the few stars which were not ejected eventually settle in the Galactic core, ...
the Scientia Review
the Scientia Review

... A Supernova is a giant explosion created by a dying star. As the star starts to decay, the outer shell grows larger and larger. The core of the star cannot hold the rest of it together. The star then violently explodes, and the burning gases shoot across space. The supernova releases about the amoun ...
telescope
telescope

... National Science Foundation and NASA. Private foundations and industry also fund research in astronomy ...
April 2006 - Otterbein University
April 2006 - Otterbein University

... Conclusions from our Observations • The Universe has a finite age, so light from very distant galaxies has not had time to reach us, therefore the night sky is dark. ...
What are your ideas about The Universe? - Harvard
What are your ideas about The Universe? - Harvard

... Some notes: Almost all students will grab the Sun, Moon and Saturn pictures together, demonstrating that they, like most astronomers, have a theory about solar system formation. But which is the exact order of age? Current theories of moon formation suggest it was formed by a collision of a Mars-siz ...
New Planet Definition Proposed by IAU
New Planet Definition Proposed by IAU

... (1) A planet is a celestial body that (a) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape1, and (b) is in orbit around a star, and is neither a star nor a satellite of a planet.2 (2) We distinguish between the e ...
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19ism1s

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Origins of the Universe
Origins of the Universe

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Unit 1 The Universe
Unit 1 The Universe

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QSOs . Continuum Radiation Energy Source

... The Black Hole at the the Galactic Center Velocities of stars in very center  4 million M black hole at position of Sagittarius A* ...
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... Conclusions from our Observations • The Universe has a finite age, so light from very distant galaxies has not had time to reach us, therefore the night sky is dark. ...
Perspectives of the Earth, Moon and Sun
Perspectives of the Earth, Moon and Sun

... 3. Students know that our solar system consists of one star, eight planets and numerous other smaller objects. (10 mins) The view zooms into our solar system, showing the eight planets, the Sun and the asteroid belt in between the terrestrial planets and the gas giants. Students consider what the Ea ...
What is a Star? - Yale Astronomy
What is a Star? - Yale Astronomy

... •  #1 should be easy -- This is something you should understand after the reading. •  #2 more challenging -– answer may not be directly given in reading. Think about it, but only for a few minutes, then give your best answer. In most (but not all) cases, this is something you should understand after ...
Phys 214. Planets and Life
Phys 214. Planets and Life

... could be many worlds that had plenty of time for life to arise and evolve. These worlds might have had civilizations millions or billions of years ago. The scale of time holds sobering lessons for our own future. Species have come and gone in the months of the cosmic calendar, and there is no reason ...
Standard Set 2 - Atascadero High School
Standard Set 2 - Atascadero High School

... Students should know that scientists catalog galaxies and stars according to the coordinates of their positions in the sky, their brightness, and their other physical characteristics. Spectroscopic analysis of the light from distant stars indicates that the same elements that make up nearby stars a ...
COSMOLOGY A FLAT EARTH GEOCENTRIC MODEL or the
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... The galaxies inside the cube stay the same size. ...
Origin of Our Solar System
Origin of Our Solar System

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Lecture 1 - University of Maryland Astronomy
Lecture 1 - University of Maryland Astronomy

... that a high-eccentricity orbit (rather than the nearly circular one we have) would subject any life to variations too extreme to survive. Also, if the planet in question is too small it can’t retain an atmosphere and will lose its internal heat quickly. A planet that is too large might have any soli ...
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Chapter 2
Chapter 2

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Astrobiology 101
Astrobiology 101

... SO THAT’S WHERE THE ELEMENTS COME FROM!! The first four elements were present after the big bang. Elements up through magnesium were created in red giants. Elements up through iron were created in supergiants and the elements from iron to uranium were created in ...
Chapter 9: Our Star, the Sun
Chapter 9: Our Star, the Sun

... other atmospheric phenomena • prominences • solar flares ...
ASTR100 Class 01 - University of Maryland Department of
ASTR100 Class 01 - University of Maryland Department of

... C. The temperature starts low and ends high in both the raisin cake and the universe. D. The raisins stay roughly the same size as the cake expands, just as galaxies stay roughly the same size as the universe expands. E. The average distance increases with time both between raisins in the cake and b ...
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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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