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... prove p || r. 5. m2 = (5x + 20)°, m 7 = (7x + 8)°, and x = 6 m2 = 5(6) + 20 = 50° m7 = 7(6) + 8 = 50° m2 = m7, so 2 ≅ 7 ...
3. - Plain Local Schools
3. - Plain Local Schools

... prove p || r. 5. m2 = (5x + 20)°, m 7 = (7x + 8)°, and x = 6 m2 = 5(6) + 20 = 50° m7 = 7(6) + 8 = 50° m2 = m7, so 2 ≅ 7 ...
Flatland 2: Sphereland
Flatland 2: Sphereland

... Q How many degrees is the sum of the angle measurements in a triangle? A In plane geometry the sum is 180◦ . We’ll see that this fact is a key point in the plot of the movie. Let’s now watch the movie. ...
Downloadable PDF - Rose
Downloadable PDF - Rose

... In 1840, János Bolyai shook the foundations of mathematics and almost nobody noticed. He investigated the consequences of some axioms of Euclidean geometry combined with the assumption that intersecting lines could all miss a given line, and then published his study of this new geometry as an append ...
3D Tour of the Universe Template
3D Tour of the Universe Template

... found astronomical showpiece if the sky is dark, where suggestions of its spiral arms may be visible. As is also common with these types of galaxy interactions, the central region of M51 is home to a compact, energetic birth site of massive and luminous stars, whose genesis was triggered by interste ...
Formal Geometry - Washoe County School District
Formal Geometry - Washoe County School District

... A. Definition of angle bisector- If a ray is an angle bisector, then it divides the angle into two congruent angles. B. Definition of opposite rays- If a point on the line determines two rays are collinear, then the rays are opposite rays. C. Definition of ray- If a line begins at an endpoint and ex ...
4-6 Triangle Congruence: ASA, AAS, and HL Bellringer: 1. What are
4-6 Triangle Congruence: ASA, AAS, and HL Bellringer: 1. What are

... can be used to find the position of points A, B, and C. List the important information: The bearing from A to B is N 65° E. From B to C is N 24° W, and from C to A is S 20° W. The distance from A to B is 8 mi. ...
Hyperbolic Geometry in the High School Geometry Classroom
Hyperbolic Geometry in the High School Geometry Classroom

... lines since these lines do not intersect. This model represents a way of visualizing by “finding Euclidean objects that represent hyperbolic objects” (Greenberg, 1993,p. 226). Models help students with their visualization while they are learning new mathematical concepts. ...
1 - Philosophy, Theology, History, Science, Big Questions
1 - Philosophy, Theology, History, Science, Big Questions

... 1.2 Some Key Definitions, Terminology, and Abbreviations: In this section, I shall define some key terminology and abbreviations that are used in more than one section. This will help the reader keep track of my terms and symbolisms. 1. Embodied moral agents: An “embodied moral agent” will be define ...
File
File

... Distance Formula to verify that corresponding sides are congruent. Name the congruence transformation for ΔRST and ΔRST. ...
geometry - Calculate
geometry - Calculate

... Michael O’Connor: [email protected] ...
Geometry Lesson 4
Geometry Lesson 4

(4  5) + 2
(4 5) + 2

... geometry, the Greeks created the first formal mathematics of any kind by organizing geometry with rules of logic. ...
The Parallel Postulate is Depended on the Other Axioms
The Parallel Postulate is Depended on the Other Axioms

... Euclid’s results have been stated by earlier Greek mathematicians, Euclid was the first to show how these propositions could be fit together into a comprehensive deductive and logical system self consistent. Because nobody until now succeeded to prove the parallel postulate, many self consistent non ...
“180 IN A TRIANGLE”
“180 IN A TRIANGLE”

... system? How about one the size of an atom? I can discover that the Earth is not flat if I go to an extreme scale. Why don’t we ever go to extreme scales to test triangles? I’ve taught multiple sections of ninth and tenth grade geometry each and every year of my school teaching career. And I have thi ...
PDF
PDF

Math 3329-Uniform Geometries — Lecture 10 1. Hilbert`s Axioms In
Math 3329-Uniform Geometries — Lecture 10 1. Hilbert`s Axioms In

Holt Geometry 4-4
Holt Geometry 4-4

... of corresponding parts were congruent. (3 pair of congruent sides and 3 pair of congruent angles) ...
Holt McDougal Geometry
Holt McDougal Geometry

... Apply properties of similar polygons to solve problems. Holt McDougal Geometry ...
No Slide Title
No Slide Title

Introduction to Proof: Part I Types of Angles
Introduction to Proof: Part I Types of Angles

... Two angles are supplementary if the sum of their measures is 180 degrees. Each angle is called a supplement of the other. If the angles are adjacent and supplementary, they are called a linear ...
Non-Euclidean Geometry
Non-Euclidean Geometry

... through C in either direction that does not meet AB is called a parallel line. Other lines through C which do not meet AB are called nonintersecting lines. The two parallel lines through C are called the right-hand parallel and left-hand parallel. The angle determined by the line from C perpendicula ...
11/10 Notes - Converse Theorems
11/10 Notes - Converse Theorems

... A second style of proof is a flowchart proof, which uses boxes and arrows to show the structure of the proof. The justification for each step is written below the box. ...
Mathematicians have developed many different kinds of geometry
Mathematicians have developed many different kinds of geometry

... If corresponding angles in two triangles are equal, they will be similar triangles, i.e. the same shape. However, this does not apply to a figure with more than three sides, for example, a square and a rectangle have all four angles equal but they are not necessarily the same shape. ...
similar polygons
similar polygons

... 7-1 Ratios in Similar Polygons A similarity ratio is the ratio of the lengths of the corresponding sides of two similar polygons. The similarity ratio of ∆ABC to ∆DEF is ...
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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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