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PHYS 175 (2014) Final Examination Name: ___SOLUTION_____
PHYS 175 (2014) Final Examination Name: ___SOLUTION_____

... Massive  objects  warp  spacetime.    If  a  massive  object  is  aligned  between  an  observer  and  a  light  source,   some  rays  of  light  from  the  source,  which  would  not  normally  be  directed  toward  the  observer,  can  be   deflected  toward  the  observer.    The  effect  may  ma ...
CMBR and BH evaporation
CMBR and BH evaporation

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Diameter of the Milky Way

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UNIT 4 - Rowan County Schools
UNIT 4 - Rowan County Schools

... Radio Waves (RF) Radio waves • Have very low energy • Used to gather information about: – Supernova – Quasars/blazars (activie galaxies) – Pulsars – The interstellar medium – The big bang ...
Astronomy 114 Problem Set # 7 Due: 30 Apr 2007 SOLUTIONS 1
Astronomy 114 Problem Set # 7 Due: 30 Apr 2007 SOLUTIONS 1

... gravitational pull at some radius R is induced by the mass within R, we denote it M(R). For the centrifugal force, we have ...
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PHY 150

... Kepler’s Law of Periods (derived from Newton’s 2nd Law) relates the period of an object to the radius of the object when the object is circling some massive object, i.e. T 2 ≈ r 3 . Most of the mass in the Milky Way galaxy lies in the galactic nucleus. Thus, stars in the spiral arms can be envisione ...
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... most stable burning object in Milky Way galaxy with a very low .1% variance (over 11 years span), so small it has no impact on Earth's climate. The search for a very stable burning star like our sun is called a solar twin. An identical solar twin has yet to be found, closest is stars with about 3% v ...
November 2013 - Pomona Valley Amateur Astronomers
November 2013 - Pomona Valley Amateur Astronomers

... In this article there is a great deal of speculation but it indicates the areas that are being investigated. Science can never “prove” a theory. But one observation can “falsify” it. So long as a concept is consistent with all observations it can be considered reasonable. If it can hold up under int ...
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Cosmos & Contact - Access Research Network

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Big Bang and Beyond

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Presentation available here - Lunar and Planetary Institute

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Uranometria 2000.0`s Dark Nebulae Database
Uranometria 2000.0`s Dark Nebulae Database

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Page 25 - Types of Galaxies

... • These galaxies are neither spiral nor elliptical. • They tend to be smaller objects that are without definite shape and tend to have very hot newer stars mixed in with lots of gas and dust. • These galaxies often have active regions of star formation. Sometimes the irregular shape of these galaxie ...
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... west with the onset of darkness, bringing the spring constellations of Leo, Virgo, Coma Bernices and Ursa Major into prominence. It is within these that hosts of galaxies reside. The North Galactic Pole, the point in the sky directly over the centre of our galaxy, is in the constellation Coma Bernic ...
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The Adventures of π-Man: Measuring the Universe

... π-man explains. Here is a “paradox” from the early days of Einstein’s Special Theory of Relativity. Consider a spinning disc (the merry-go-round in π-man’s adventure). As measured by an observer outside the disc, the relation between the circumference and the radius of the disc, whether the disc is ...
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The Universe Starring Man? The Impact of Scientific

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Ch. 5 The Universe and Solar System
Ch. 5 The Universe and Solar System

... universe is expanding. • Red shift—means movement is away. • Proof 2: 1965 Arno Penzlas and Robert Wilson discovered background radiation—a remnant of the Big Bang. It is evenly distributed. • Proof 3: 1995 NASA discovered deuterium (heavy isotope of H) scattered throughout the universe. ...
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Hubble`s Expansion of the Universe

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Astronomy Review revised Key

... 16. Explain how Barnard's star and Mira are similar and how they are different. _____________ _______They are both red, but Mira is a giant and Barnard’ star is main sequence. 17. Describe three features of the star Deneb. white__ ___supergiant__ _very bright__ ...
STATES OF MATTER
STATES OF MATTER

...  Particles of liquids are tightly packed, but are far enough apart to slide over one another.  Liquids have an indefinite shape and a definite volume. ...
Galaxy - Bama.ua.edu
Galaxy - Bama.ua.edu

... was 8 minutes ago. • The nearest star, 4LY away, as it was 4 years ago. • Andromeda galaxy as it was about 2 million yr ago. • If we look ~14 billion LY away, expect to see universe in its early, hot, compressed, uniform gas state. ...
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Structure formation

In physical cosmology, structure formation refers to the formation of galaxies, galaxy clusters and larger structures from small early density fluctuations. The Universe, as is now known from observations of the cosmic microwave background radiation, began in a hot, dense, nearly uniform state approximately 13.8 billion years ago. However, looking in the sky today, we see structures on all scales, from stars and planets to galaxies and, on still larger scales still, galaxy clusters and sheet-like structures of galaxies separated by enormous voids containing few galaxies. Structure formation attempts to model how these structures formed by gravitational instability of small early density ripples.The modern Lambda-CDM model is successful at predicting the observed large-scale distribution of galaxies, clusters and voids; but on the scale of individual galaxies there are many complications due to highly nonlinear processes involving baryonic physics, gas heating and cooling, star formation and feedback. Understanding the processes of galaxy formation is a major topic of modern cosmology research, both via observations such as the Hubble Ultra-Deep Field and via large computer simulations.
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