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How Telescopes Changed our Universe
How Telescopes Changed our Universe

... In our own solar system, telescopes found planets our eyes could not see. Are there other planets outside of our solar system? ...
ISP 205: Visions of the Universe
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... — It rotates on its axis once a day and orbits the Sun at a distance of 1 AU = 150 million km • How is our solar system moving in the Milky Way Galaxy? — Stars in the Local Neighborhood move randomly relative to one another and orbit the center of the Milky Way in about 230 million years ...
Chapter 12 Our Place in the Universe
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... • We’ve never observed anything like the edge of the Universe • Without any edges, there can’t be a “centre of the Universe” • Astronomers do know that the Universe must be larger than a certain size… ...
Our Place in the Universe (Chapter 1) The Structure and Size of the
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... • They kept getting a static signal, no matter how they tuned and oriented the antenna. At one point they even constructed a pigeon trap thinking that the guano being deposited in the horn of the antenna by the nesting pigeons was the source of the static. • Finally someone mentioned to them to talk ...
Tragedy vs. Hope: What Future in an Open Universe?
Tragedy vs. Hope: What Future in an Open Universe?

... major catastrophes. Their influence on the biological evolution was profound, but life on Earth has continued. This will not be the case forever. The Sun has fused already a few percent of its hydrogen fuel into helium. The pressure in the center has augmented and the fusion rate increases. Since th ...
Chapter 31 - The Galaxy & Universe
Chapter 31 - The Galaxy & Universe

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... which I throw the balloon. The terms "m" and "r" may be thought of as additional boundary conditions which are specific to the location of the tower on the surface of the earth (rather than some other location in the universe). The engineer has no control over the laws of nature and the mathematical ...
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Shape of the universe



The shape of the universe is the local and global geometry of the Universe, in terms of both curvature and topology (though, strictly speaking, the concept goes beyond both). The shape of the universe is related to general relativity which describes how spacetime is curved and bent by mass and energy.There is a distinction between the observable universe and the global universe. The observable universe consists of the part of the universe that can, in principle, be observed due to the finite speed of light and the age of the universe. The observable universe is understood as a sphere around the Earth extending 93 billion light years (8.8 *1026 meters) and would be similar at any observing point (assuming the universe is indeed isotropic, as it appears to be from our vantage point).According to the book Our Mathematical Universe, the shape of the global universe can be explained with three categories: Finite or infinite Flat (no curvature), open (negative curvature) or closed (positive curvature) Connectivity, how the universe is put together, i.e., simply connected space or multiply connected.There are certain logical connections among these properties. For example, a universe with positive curvature is necessarily finite. Although it is usually assumed in the literature that a flat or negatively curved universe is infinite, this need not be the case if the topology is not the trivial one.The exact shape is still a matter of debate in physical cosmology, but experimental data from various, independent sources (WMAP, BOOMERanG and Planck for example) confirm that the observable universe is flat with only a 0.4% margin of error. Theorists have been trying to construct a formal mathematical model of the shape of the universe. In formal terms, this is a 3-manifold model corresponding to the spatial section (in comoving coordinates) of the 4-dimensional space-time of the universe. The model most theorists currently use is the so-called Friedmann–Lemaître–Robertson–Walker (FLRW) model. Arguments have been put forward that the observational data best fit with the conclusion that the shape of the global universe is infinite and flat, but the data are also consistent with other possible shapes, such as the so-called Poincaré dodecahedral space and the Picard horn.
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