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View Table of Contents in PDF
View Table of Contents in PDF

... Geometry Manual Vol. 1: Elementary I ...
Non-Euclidean Geometry - Department of Mathematics | Illinois
Non-Euclidean Geometry - Department of Mathematics | Illinois

... ◦ 3: Given a point and a distance a circle can be drawn with the point as center and the distance as radius ◦ 4: All right angles are equal ◦ 5: Given a point p and a line l, there is exactly one line through p that is parallel to l ...
SCIN 293-PL-New Course
SCIN 293-PL-New Course

... Lesson 1: Galactic Evolution Topic 1: The Milky Way Galaxy Topic 2: Formation of Galaxies Topic 3: Active Galactic Nuclei Topic Mastery: Based on the Hubble tuning fork compared the properties of the different classes of galaxies and their stellar populations. ...
Parallel Postulate
Parallel Postulate

... lines are non-existent. The non-Euclidean geometry developed by Gauss could be model on a sphere where as Lobachevskian’s geometry had no physical model. For this reason, Riemannian geometries are also referred to as a spherical geometry or elliptical geometry. Riemann also made several contribution ...
Spectroscopy Applications - Astrophysics and
Spectroscopy Applications - Astrophysics and

... Astrophysics and Cosmology It was further observed that ALL spectra form ALL deep space objects were shifted toward the red, ie, longer wavelengths The implications is that ALL objects in the universe, on the average, are moving away from the Earth. ...
Geometry Pretest Assessment Match the shape to its number of
Geometry Pretest Assessment Match the shape to its number of

... MAFS.2.G.1.1: Students will be able to Recognize and draw shapes having specified attributes, such as a given number of angles or a given number of equal faces. Identify triangles, quadrilaterals, pentagons, hexagons, and cubes. ...
Hubble - STScI
Hubble - STScI

... A Sun-like star's death is as colorful as maple leaves in autumn. Sun-like stars die gracefully by ejecting their outer gaseous layers into space. Eventually, the outer layers begin to glow in vibrant colors of red, blue, and green. The colorful glowing shroud is called a planetary nebula. Hubble re ...
Course Outline - Palisades School District
Course Outline - Palisades School District

...  Absences, lateness, and plagiarism will be dealt with according to school policy. See your student handbook for details.  If you miss class to participate in a school-approved trip or activity, the assignment is still due. (Student Handbook). HOMEWORK POLICY: Homework will be assigned regularly a ...
Course Outline - Palisades School District
Course Outline - Palisades School District

...  Absences, lateness, and plagiarism will be dealt with according to school policy. See your student handbook for details.  If you miss class to participate in a school-approved trip or activity, the assignment is still due. (Student Handbook). HOMEWORK POLICY: Homework will be assigned regularly a ...
A100H–Exploring the Universe: Dark Matter, Dark Energy Martin D
A100H–Exploring the Universe: Dark Matter, Dark Energy Martin D

... Either dark matter exists or our understanding of our gravity must be revised ...
attached  file
attached file

Document
Document

JSUNIL TUTORIAL, SAMASTIPUR, BIHAR Introduction to Euclid’s Geometry Ch-5 IX
JSUNIL TUTORIAL, SAMASTIPUR, BIHAR Introduction to Euclid’s Geometry Ch-5 IX

"Pop Goes the Universe", Scientific American - Harvard
"Pop Goes the Universe", Scientific American - Harvard

... dom warps in space that propagate as waves of spatial distortion across the universe once inflation ends. These disturbances, known as gravitational waves, are another source of hotspots and cold spots in the cosmic microwave background radiation, albeit ones that have a distinctive polarizing effec ...
Slide 1
Slide 1

... • A "true" color image or photograph recreates what our eyes would see in visible light under natural conditions • To create a color image from data at other wavelengths, astronomers represent it in "false" colors • Three of grayscale images from different wavelengths may be mapped to red, green, an ...
goes the universe - Physics Department, Princeton University
goes the universe - Physics Department, Princeton University

Six thousand versus 14 Billion: How large and how old is the
Six thousand versus 14 Billion: How large and how old is the

the group exercise in class on Monday March 28
the group exercise in class on Monday March 28

... 4. Construct two lines (great circles) on the sphere. It is important to remember that lines must divide the sphere into two identical pieces. In how many points do these lines intersect? 5. Remove one of these lines and keep the other. Now choose a point not on that line. How many lines are there w ...
chap8 (WP)
chap8 (WP)

1 A CLOSED NON-COLLAPSING 3-D UNIVERSE PREDICTING A
1 A CLOSED NON-COLLAPSING 3-D UNIVERSE PREDICTING A

Euclid`s Fifth Postulate
Euclid`s Fifth Postulate

... (a) \If a straight line intersects one of two parallels (i.e, lines which do not intersect however far they are extended), it will intersect the other also." (b) \There is one and only one line that passes through any given point and is parallel to a given line." (c) \Given any gure there exists a ...
Matter and antimatter in the same universe?
Matter and antimatter in the same universe?

... relativity (eq. (2)) it is not difficult to see that the existence of an initial singularity is unavoidable unless drastic things happen, like, for example, a hypothetic repulsive gravity [7, 8] above some critical temperature Tr Indeed, if the standard Big Bang theory is successful in explaining th ...
Generation of Cosmological Perturbations by a First
Generation of Cosmological Perturbations by a First

Hyperbolic Constructions using the Poincare Disk Model
Hyperbolic Constructions using the Poincare Disk Model

... 2. Create  any  triangle  using  hyperbolic  segment.    Use  the  hyperbolic  angle  tool  to   measure  the  angles  (the  three  points  must  be  selected  clockwise!).    You  can  add  the   three  measures  to  verify  that  the  sum  of  the  angles  is  less  than  180.   3. Can  you  make ...
Interpretation of the evolution of universe through the consciousness
Interpretation of the evolution of universe through the consciousness

... The acceptance of this theory by the scientific community is based on a number of observations. These observations confirm specific predictions of the Big Bang theory. Pidwirny [14] expressed that scientists test their theories through deduction and falsification. Predictions associated with the Big ...
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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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