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Difference between revisions of "Parallel displacement"

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A special case of a [[Motion|motion]] in which all points of the space are transferred in one and the same direction (along a line in that space) over one and the same distance. In other words, if <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/p/p071/p071340/p0713401.png" /> is the original and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/p/p071/p071340/p0713402.png" /> is the shifted position of a point, then the vector <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/p/p071/p071340/p0713403.png" /> is one and the same for all pairs of points corresponding to each other under the given transformation.
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$#C+1 = 7 : ~/encyclopedia/old_files/data/P071/P.0701340 Parallel displacement
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In the plane a parallel displacement may analytically be expressed in a rectangular coordinate system <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/p/p071/p071340/p0713404.png" /> by the formulas
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<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/p/p071/p071340/p0713405.png" /></td> <td valign="top" style="width:5%;text-align:right;">(*)</td></tr></table>
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A special case of a [[Motion|motion]] in which all points of the space are transferred in one and the same direction (along a line in that space) over one and the same distance. In other words, if  $  M $
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is the original and  $  M  ^  \prime  $
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is the shifted position of a point, then the vector  $  {MM  ^  \prime  } vec $
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is one and the same for all pairs of points corresponding to each other under the given transformation.
  
where <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/p/p071/p071340/p0713406.png" />.
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In the plane a parallel displacement may analytically be expressed in a rectangular coordinate system  $  ( x, y) $
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by the formulas
  
The collection of all parallel displacements forms a group, which in a Euclidean space is a subgroup of the group of motions, and in an affine space is a subgroup of the group of affine transformations.
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$$ \tag{* }
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\widetilde{x}  =  x+ a,\ \
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\widetilde{y}  =  y+ b,
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$$
  
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where  $  {MM  ^  \prime  } vec = ( a, b) $.
  
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The collection of all parallel displacements forms a group, which in a Euclidean space is a subgroup of the group of motions, and in an affine space is a subgroup of the group of affine transformations.
  
 
====Comments====
 
====Comments====
In the absolute plane a parallel displacement (cf. [[Absolute geometry|Absolute geometry]]) is the product of reflections in two parallel lines (cf. [[Reflection|Reflection]]). Thus, in [[Euclidean geometry|Euclidean geometry]] a parallel displacement is a [[Translation|translation]], expressible in affine (or Cartesian) coordinates by <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/p/p071/p071340/p0713407.png" /> (see (*)).
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In the absolute plane a parallel displacement (cf. [[Absolute geometry|Absolute geometry]]) is the product of reflections in two parallel lines (cf. [[Reflection|Reflection]]). Thus, in [[Euclidean geometry|Euclidean geometry]] a parallel displacement is a [[Translation|translation]], expressible in affine (or Cartesian) coordinates by ( x, y) \rightarrow ( \widetilde{x}  , \widetilde{y}  ) $(
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see (*)).
  
 
But in [[Lobachevskii geometry|Lobachevskii geometry]] a parallel displacement moves each point along a horocycle, whereas a translation is different, namely the product of half-turns about two distinct points, or the product of reflections in two lines that have a common perpendicular.
 
But in [[Lobachevskii geometry|Lobachevskii geometry]] a parallel displacement moves each point along a horocycle, whereas a translation is different, namely the product of half-turns about two distinct points, or the product of reflections in two lines that have a common perpendicular.

Latest revision as of 08:05, 6 June 2020


A special case of a motion in which all points of the space are transferred in one and the same direction (along a line in that space) over one and the same distance. In other words, if $ M $ is the original and $ M ^ \prime $ is the shifted position of a point, then the vector $ {MM ^ \prime } vec $ is one and the same for all pairs of points corresponding to each other under the given transformation.

In the plane a parallel displacement may analytically be expressed in a rectangular coordinate system $ ( x, y) $ by the formulas

$$ \tag{* } \widetilde{x} = x+ a,\ \ \widetilde{y} = y+ b, $$

where $ {MM ^ \prime } vec = ( a, b) $.

The collection of all parallel displacements forms a group, which in a Euclidean space is a subgroup of the group of motions, and in an affine space is a subgroup of the group of affine transformations.

Comments

In the absolute plane a parallel displacement (cf. Absolute geometry) is the product of reflections in two parallel lines (cf. Reflection). Thus, in Euclidean geometry a parallel displacement is a translation, expressible in affine (or Cartesian) coordinates by $ ( x, y) \rightarrow ( \widetilde{x} , \widetilde{y} ) $( see (*)).

But in Lobachevskii geometry a parallel displacement moves each point along a horocycle, whereas a translation is different, namely the product of half-turns about two distinct points, or the product of reflections in two lines that have a common perpendicular.

References

[a1] H.S.M. Coxeter, "Non-Euclidean geometry" , Univ. Toronto Press (1965) pp. 224–240
How to Cite This Entry:
Parallel displacement. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Parallel_displacement&oldid=15883
This article was adapted from an original article by A.B. Ivanov (originator), which appeared in Encyclopedia of Mathematics - ISBN 1402006098. See original article