A School Geometry Parts i and ii Experimental and Theoretical Course of Geometry Elementary Geometry Solid Geometry

Nature ◽  
1903 ◽  
Vol 68 (1755) ◽  
pp. 147-148
1974 ◽  
Vol 67 (2) ◽  
pp. 175-178
Author(s):  
Charles A. Reeves

The last decade has ushered in numerous changes in the teaching of high school geometry—changes due primarily to the impetus of curriculum committees such as the Commission on Mathematics. One trend is that of integrating plane and solid geometry “topicwise” into one course; that is, as each topic is studied in two dimensions, the concept is immediately extended to three dimensions if possible. This pedagogical technique undoubtedly helps students grasp related ideas more readily than if those ideas were presented as separate entities.


1988 ◽  
Vol 36 (3) ◽  
pp. 11-17 ◽  
Author(s):  
Michael T. Battista ◽  
Douglas H. Clements

Geometry is an essential part of mathematics. Unfortunately, according to evaluations of mathematics learning, such as the National Assessment of Educational Progress (NAEP), students are failing to understand basic geometric concepts and are failing to develop adequate geometric problem-solving skills (Carpenter et al. 1980; Fey et al. 1984; Kouba et al. 1988). This poor performance is due, in part, to the current elementary school geometry curriculum, which focuses on recognizing and naming geometric shapes and learning to write the proper symbolism for simple geometric concepts (cf. Carpenter et al. [1980]; Flanders [1987]). In contrast, we believe that elementary geometry should be the study of objects, motions, and relationships in a spatial environment (Clements and Battista [1986]; cf. Trafton and LeBlanc [1973]). First experiences with geometry should emphasize informal study of physical shapes and their properties and have as their primary goal the development of students' intuition and knowledge about their spatial environment. Subsequent experiences should involve analyzing and abstracting geometric concepts and relationships in increasingly formal settings.


2004 ◽  
Vol 97 (4) ◽  
pp. 228-231
Author(s):  
Alan W. Hirshfeld

The ancient Greek mathematician Aristarchus demonstrated for the first time how it was possible, using simple observations and elementary geometry, to measure distances to bodies in the solar system. Aristarchus' methods used a lunar elcipse to approximate the diameter of the Earth, and used the shadow cone of a lunar eclipse to form similar triangles and proportional measurements. The mathmatics can be easily understood by a high school geometry student.


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