词条 | projective geometry |
释义 | projective geometry Introduction branch of mathematics that deals with the relationships between geometric figures and the images, or mappings (mapping), that result from projecting them onto another surface. Common examples of projections (projection) are the shadows cast by opaque objects and motion pictures displayed on a screen. Projective geometry has its origins in the early Italian Renaissance, particularly in the architectural drawings of Filippo Brunelleschi (Brunelleschi, Filippo) (1377–1446) and Leon Battista Alberti (Alberti, Leon Battista) (1404–72), who invented the method of perspective drawing. By this method, as shown in the figure-->, the eye of the painter is connected to points on the landscape (the horizontal reality plane, RP) by so-called sight lines. The intersection of these sight lines with the vertical picture plane (PP) generates the drawing. Thus, the reality plane is projected onto the picture plane, hence the name projective geometry. See also geometry: Linear perspective (geometry). Although some isolated properties concerning projections were known in antiquity, particularly in the study of optics, it was not until the 17th century that mathematicians returned to the subject. The French mathematicians Girard Desargues (Desargues, Girard) (1591–1661) and Blaise Pascal (Pascal, Blaise) (1623–62) took the first significant steps by examining what properties of figures were preserved (or invariant) under perspective mappings. The subject's real importance, however, became clear only after 1800 in the works of several other French mathematicians, notably Jean-Victor Poncelet (Poncelet, Jean-Victor) (1788–1867). In general, by ignoring geometric measurements such as distances and angles, projective geometry enables a clearer understanding of some more generic properties of geometric objects. Such insights have since been incorporated in many more advanced areas of mathematics. Parallel lines and the projection of infinity A theorem from Euclid's Elements (c. 300 BC) states that if a line is drawn through a triangle such that it is parallel to one side (see the figure-->), then the line will divide the other two sides proportionately; that is, the ratio of segments on each side will be equal. This is known as the proportional segments theorem, or the fundamental theorem of similarity, and for triangle ABC, with line segment DE parallel to side AB, the theorem corresponds to the mathematical expression CD/DA=CE/EB. Now consider the effect produced by projecting these line segments onto another plane as shown in the figure-->. The first thing to note is that the projected line segments A′B′ and D′E′ are not parallel; i.e., angles are not preserved. From the point of view of the projection, the parallel lines AB and DE appear to converge at the horizon, or at infinity, whose projection in the picture plane is labeled Ω. (It was Desargues who first introduced a single point at infinity to represent the projected intersection of parallel lines. Furthermore, he collected all the points along the horizon in one line at infinity.) With the introduction of Ω, the projected figure corresponds to a theorem discovered by Menelaus of Alexandria in the 1st century AD: C′D′/D′A′=C′E′/E′B′∙ΩB′/ΩA′. Since the factor ΩB′/ΩA′ corrects for the projective distortion in lengths, Menelaus's theorem can be seen as a projective variant of the proportional segments theorem. Projective invariants With Desargues (Desargues's theorem)'s provision of infinitely distant points for parallels, the reality plane and the projective plane are essentially interchangeable—that is, ignoring distances and directions (angles), which are not preserved in the projection. Other properties are preserved, however. For instance, two different points have a unique connecting line, and two different lines have a unique point of intersection. Although almost nothing else seems to be invariant under projective mappings, one should note that lines are mapped onto lines. This means that if three points are collinear (share a common line), then the same will be true for their projections. Thus, collinearity is another invariant property. Similarly, if three lines meet in a common point, so will their projections. The following theorem is of fundamental importance for projective geometry. In its first variant, by Pappus of Alexandria (fl. AD 320) as shown in the figure-->, it only uses collinearity:Let the distinct points A, B, C and D, E, F be on two different lines. Then the three intersection points—x of AE and BD, y of AF and CD, and z of BF and CE—are collinear. The second variant, by Pascal, as shown in the figure-->, uses certain properties of circles:If the distinct points A, B, C, D, E, and F are on one circle, then the three intersection points x, y, and z (defined as above) are collinear. There is one more important invariant under projective mappings, known as the cross ratio (see the figure-->). Given four distinct collinear points A, B, C, and D, the cross ratio is defined as CRat(A, B, C, D)=AC/BC∙BD/AD. It may also be written as the quotient of two ratios: CRat(A, B, C, D)=AC/BC:AD/BD. The latter formulation reveals the cross ratio as a ratio of ratios of distances. And while neither distance nor the ratio of distance is preserved under projection, Pappus first proved the startling fact that the cross ratio was invariant—that is, CRat(A, B, C, D)=CRat(A′, B′, C′, D′). However, this result remained a mere curiosity until its real significance became gradually clear in the 19th century as mappings became more and more important for transforming problems from one mathematical domain to another. Projective conic sections (conic section) Conic sections can be regarded as plane sections of a right circular cone (see the figure-->). By regarding a plane perpendicular to the cone's axis as the reality plane (RP), a “cutting” plane as the picture plane (PP), and the cone's apex as the projective “eye,” each conic section can be seen to correspond to a projective image of a circle (see the figure-->). Depending on the orientation of the cutting plane, the image of the circle will be a circle, an ellipse, a parabola, or a hyperbola. A plane Ω passing through the apex and parallel to PP defines the line at infinity in the projective plane PP. The situation of Ω relative to RP determines the conic section in PP: If Ω intersects RP outside the base circle (the circle formed by the intersection of the cone and RP), the image of the circle will be an ellipse. If Ω is tangent to the base circle (in effect, tangent to the cone), the image will be a parabola. If Ω intersects the base circle (thus, cutting the circle in two), a hyperbola will result. Pascal's theorem, quoted above, also follows easily for any conic section from its special case for the circle. Start by selecting six points on a conic section and project them back onto the base circle. As given earlier, the three relevant intersection points for six points on the circle will be collinear. Now project all nine points back to the conic section. Since collinear points (the three intersection points from the circle) are mapped onto collinear points, the theorem holds for any conic section. In this way the projective point of view unites the three different types of conics. Similarly, more complicated curves and surfaces in higher-dimensional spaces can be unified through projections. For example, Isaac Newton (Newton, Sir Isaac) (1643–1727) showed that all plane curves defined by polynomials in x and y of degree 3 (the highest power of the variables is 3) can be obtained as projective images of just five types of polynomials. Additional Reading All of the following books contain some discussion of projective geometry by one of the greatest expositors of geometry, H.S.M. Coxeter: with S.L. Greitzer, Geometry Revisited (1967), suitable for high school students; Introduction to Geometry, 2nd ed. (1969), suitable for advanced high school students and general undergraduates; and Projective Geometry, 2nd ed. (1974, reprinted with corrections, 1994); The Real Projective Plane, 3rd ed. (1993); and Non-Euclidean Geometry, 6th ed. (1998), all suitable for undergraduate mathematics students. |
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