Two Strange Constructions in the Euclidean Plane

We present two new constructions in the usual euclidean plane. We only deal with 'Grecian Geometry', with this phrase we mean elementary geometry in the two-dimensional space R 2 . We describe and prove two propositions about 'projections'. The proof…

Authors: Volker Th"urey

Tw o Strange Constru ctions in the E uclidean Plane V OLKER TH ¨ UREY No v em b er 1, 20 18 MSC-class: 51N20 Abstract W e present t wo new c onstructions in the usual euclidean plane. W e only deal with ’Grecian Geometry’, with this phr ase we mean elemen tary geometry in the t wo- dimensional sp ace R 2 . W e describ e and pro v e t wo prop ositions ab out ’p ro jections’. The pro ofs need only elemen tary analytical kno wledge. The reader ma y find the foun dations and assumptions of the follo wing prop ositiones in many b o oks ab ou t plane geometry , for instance in [1], p.1-29 . Or y ou can lo ok in [2 ] , [3] , [4] , [5] , [6], [7] . See also [8], p.224-2 34 . Prop osition 1. Let us ta k e R 2 = { ( x | y ) | x , y ∈ R } , the t wo-dimensional euclidean p lane, with the horizont al x -axis and the vertica l y -axis. Assume tw o p arallel s tr aigh t lines G S and G T . Assume a third line L , not parallel to G S , G T , resp ectiv ely , with th e prop erty that L do es not meet the origin (0 | 0). The intersectio n of L with G S is calle d S = ( x S | y S ), and the in tersection of L w ith G T is calle d T = ( x T | y T ) . Note that, in the case that G S , G T are distinct, the three points (0 | 0 ), S, T are n ot collinear. W e can dra w t w o lines Z S and Z T , Z S connects the origin (0 | 0) and S , and Z T connects (0 | 0) a nd T . Z S and Z T are distinct if G S and G T are distinct. No w we distinguish t wo cases (A) and (B) , but note that they o v erlap. (A) : In th e case that G S and G T are not parallel to the horizon tal x -axis, w e ha v e tw o in tersections a S , a T of G S and G T , resp ectiv ely , with the x -axis. Th en th ere is an uniqu e p oint P hor = ( x hor | y hor ) on L , such that ( x hor − a S | y hor ) ∈ Z T , and ( x hor − a T | y hor ) ∈ Z S . (B) : In the case that G S and G T are not parallel to the vertic al y -axis, w e ha v e tw o in ter- sections b S , b T of G S and G T , resp ectiv ely , with th e y -axis. Th en there is an unique p oint P ver = ( x ver | y ver ) on L , suc h that ( x ver | y ver − b S ) ∈ Z T , and ( x ver | y ver − b T ) ∈ Z S . Before reading the pro of of the prop osition y ou should tak e a look on Picture 1 . 1 Picture 1 x y ✲ ✻ a S G T : y = 2 x + 2 G S : y = 2 x + 4 L : y = +1 a T ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ S T ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ❆ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ ◗ Z S : y = − 2 3 x Z T : y = − 2 x × × P hor P ver b T b S Here: b S = 4 and b T = 2 , a S = − 2 and a T = − 1 , S = ( − 3 2 | 1) and T = ( − 1 2 | 1) . Hence P hor = ( − 5 2 | 1) and P ver = ( 3 2 | 1) . Pr o of. Note th at, if G S = G T , the prop osition is trivial. Hence we assume th at G S , G T are distinct. W e describ e the parallel straigh t lines G S , G T with equations G S := { ( x | y ) ∈ R 2 | e · y = m · x + b S } and G T := { ( x | y ) ∈ R 2 | e · y = m · x + b T } , with e, m, b S , b T ∈ R , ( m, e ) 6 = (0 , 0) . Without less of generalit y let either b e ( e = 0 and m = 1 ) or ( e = 1 ) . The straigh t line L can b e describ ed with t w o num b ers w 1 , w 2 ∈ R , ( w 1 , w 2 ) 6 = (0 , 0) . L := { ( x S | y S ) + t · ( w 1 | w 2 ) | t ∈ R } = { ( x T | y T ) + t · ( w 1 | w 2 ) | t ∈ R } , with w 1 · y T 6 = w 2 · x T , and w 1 · y S 6 = w 2 · x S , ( b ecause (0 | 0) / ∈ L ) , and with e · w 2 6 = m · w 1 , ( b ecause L is not parallel to G S and G T , resp ectiv ely) . Lemma 1. In the case of (A) , (that means that G S and G T are n ot parallel to the horizonta l x -axis), w e h a v e m 6 = 0 , and a S = − b S /m , a T = − b T /m . Then th ere are un iquely thr ee n um b ers , α, β ∈ R whic h solv e the system of four linear equations (1) x S +  · w 1 − a S = α · x T , (2) y S +  · w 2 = α · y T , (3) x S +  · w 1 − a T = β · x S , (4) y S +  · w 2 = β · y S . In the case of (B) , (that means that G S and G T are not p arallel to the v ertical y -axis), there are uniquely three n um b ers e , e α, e β ∈ R whic h solv e the system of four equations f (1) y S + e  · w 2 − b S = e α · y T , f (2) x S + e  · w 1 = e α · x T , f (3) y S + e  · w 2 − b T = e β · y S , f (4) x S + e  · w 1 = e β · x S . Pr o of. In ca se (A) the t wo equations (1),(2) yield  [1] , and the t w o equations (3),(4) yield  [2] ,  [1] = y S · x T − x S · y T + a s · y T w 1 · y T − w 2 · x T and  [2] = y S · a T w 1 · y S − w 2 · x S . 2 Because of ( x S | y S ) , ( x T | y T ) ∈ L , there is a ˘ t ∈ R suc h that ( x T | y T ) = ( x S | y S ) + ˘ t · ( w 1 , w 2 ), hence w 1 · y T − w 2 · x T = w 1 · y S − w 2 · x S . An d with ( x S | y S ) ∈ G S , ( x T | y T ) ∈ G T follo ws easily that y S · x T − x S · y T + a s · y T = y S · a T , hence  [1] =  [2] =:  . In the case of (B) the t w o equations f (1) f (2) yield e  [1] , and f (3) f (4) yield e  [2] , e  [1] = y T · x S − x T · y S + b s · x T w 2 · x T − w 1 · y T and e  [2] = x S · b T w 2 · x S − w 1 · y S . and with similar steps as only just follo ws e  [1] = e  [2] =: e  , and the lemma is prov ed. T o finish the pr o of of p rop osition 1 w e set in the case (A) : P hor = ( x hor | y hor ) := ( x S | y S ) +  · ( w 1 | w 2 ) , and in the case (B) : P ver = ( x ver | y ver ) := ( x S | y S ) + e  · ( w 1 | w 2 ) . The u niqueness of P hor and P ver is trivial, f or instance, for a non v ertical L , the horizon tal distance (with signs) from a p oint on L to Z S or Z T , resp ectiv ely , x 7− → the horizon tal distance (with sign) from a p oint ( x | y ) on L to Z S and x 7− → the horizon tal distance (with sign) from a p oint ( x | y ) on L to Z T , resp ectiv ely , are strictly monotone functions. This w as the last wh at we had to do to pro v e the prop osition. F or completeness, we wr ite d o w n other representa tions of P hor and P ver , resp ectiv ely . Note that if G S , G T are not parallel to the v ertical y -axis, they ha v e equations G S = { ( x | y ) ∈ R 2 | y = m · x + b S } and G T = { ( x | y ) ∈ R 2 | y = m · x + b T } , and if G S , G T are v ertical, they ha v e equations G S = { ( x | y ) ∈ R 2 | x = − b S =: a S } and G T = { ( x | y ) ∈ R 2 | x = − b T =: a T } . If L is not v ertical, we hav e w 1 6 = 0 , and L = { ( x S | y S ) + t · ( w 1 | w 2 ) | t ∈ R } = { ( x | y ) ∈ R 2 | y = m L · x + b L } , with m L := w 2 /w 1 and b L := y S − x S · m L , ( b L 6 = 0 , b ecause (0 | 0) / ∈ L ) . If L is v ertica l , w e s et a L := x S = x T , and L = { ( x | y ) ∈ R 2 | x = a L } . No w assume th at n either L n or G S , G T are parallel to one of the axes. Then P hor = ( x hor | y hor ) =  x T · b L + y T · a S b L | m L · x T · b L + y T · a S b L + b L  =  x S · b L + y S · a T b L | m L · x S · b L + y S · a T b L + b L  =  b L 2 · m + b S · b T · m L − m · b L · ( b S + b T ) b L · m · ( m − m L ) | b L 2 · m 2 + b S · b T · m L 2 − m · m L · b L · ( b S + b T ) b L · m · ( m − m L )  , P ver = ( x ver | y ver ) =  x T · ( b L − b S ) b L | m L · x T · ( b L − b S ) b L + b L  =  x S · ( b L − b T ) b L | m L · x S · ( b L − b T ) b L + b L  =  ( b L − b T ) · ( b L − b S ) b L · ( m − m L ) | m L · ( b S · b T − b L · b S − b L · b T ) + b 2 L · m b L · ( m − m L )  . 3 No w assume th at G S , G T are n ot parallel to one of the axes, and L is horizon tal. ( See the previous picture, to o.) Then w e ha ve an equation L : y = b L , and w e get P hor = ( x hor | y hor ) = ( x T + a S | b L ) = ( x S + a T | b L ) =  b L − b S − b T m | b L  , P ver =  x T · ( b L − b S ) b L | b L  =  x S · ( b L − b T ) b L | b L  =  ( b L − b S ) · ( b L − b T ) b L · m | b L  . Assume that G S , G T are not parallel to one of the axes, and L is v ertical. Then we h a v e an equation L : x = a L , and w e get P hor = ( x hor | y hor ) =  a L | m · a L + b S + b T + b S · b T a L · m  =  a L | ( m + b S a L ) · ( a L + b T m )  , P ver = ( x ver | y ver ) = ( a L | m · a L + b T + b S ) . No w assume that G S , G T are parallel to the horizon tal x -axis, and L is not parallel to the y -axis (and, of course, not parallel to the x -axis, to o) . Then w e get no P hor , and P ver = ( x ver | y ver ) =  x T · ( b L − b S ) b L | m L · x T · ( b L − b S ) b L + b L  =  x S · ( b L − b T ) b L | m L · x S · ( b L − b T ) b L + b L  =  ( b T − b L ) · ( b L − b S ) b L · m L | b L · b S + b L · b T − b S · b T b L  . If w e assume that G S , G T are p arallel to th e horizon tal x -axis, and L is p arallel to th e y -axis, then w e get no P hor , of course, and P ver = ( x ver | y ver ) = ( a L | b S + b T ) . No w assum e that G S , G T are p arallel to the vertic al y -axis, and L is not parallel to the x -axis (and, of course, not parallel to the y -axis, to o) . Then w e get no P ver , and P hor = ( x hor | y hor ) =  a T · b L + y T · a S b L | m L · a T · b L + y T · a S b L + b L  =  a S · b L + y S · a T b L | m L · a S · b L + y S · a T b L + b L  =  b L · ( a S + a T ) + m L · a S · a T b L | m L · x hor + b L  . And finally if we assume that G S , G T are parallel to th e y -axis, and L is p arallel to the x -axis, w e get P hor = ( x hor | y hor ) = ( a S + a T | b L ) . Remark 1. Note a few sp ecial trivial cases. Assume that G S , G T are not parallel to the h orizon tal x -axis (case (A) ) . If S = ( a S | 0) , then we ha ve Z S = x -axis and P hor = S = ( a S | 0) . If T = ( a T | 0) , then we ha ve Z T = x -axis and P hor = T = ( a T | 0) . Assume no w th at G S , G T are not parallel to the v ertical y -axis (case (B) ) . If S = (0 | b S ) , th en we h a v e Z S = y -axis and P ver = S = (0 | b S ) . If T = (0 | b T ) , th en we h a v e Z T = y -axis and P ver = T = (0 | b T ) . 4 No w w e describ e another p rop osition wh ich seems to b e more general, but indeed it is equiv alent, see lemma 2. Because w e pro v ed prop osition 1 , p r op osition 2 also is true. Prop osition 2. Let us tak e R 2 , the t w o-dimens ional euclidean p lane. Assume t wo p arallel straigh t lines G S and G T . Ass ume a thir d line L , not parallel to G S and G T , resp ectiv ely . The inte rsection of L with G S is called S , and the in tersection of L with G T is called T . Assume a fourth line Axis , Axis 6 = L , and Axis is not p arallel to G S and G T . The in tersection of Axis with G S is calle d S Axis , and the intersec tion of Axis w ith G T is calle d T Axis . F urther w e choose a p oint O r ig in on Axis \ L . W e can dra w t wo str aigh t lines Z S and Z T , Z S connects O r ig in and S , and Z T connects O r ig in and T . As ev er y line, Z S and Z T , resp ectiv ely , divide the plane in t w o halfplanes. Z S and Z T are distinct if G S and G T are d istinct. Then there is an unique p oint P ∈ L with the f ollo wing prop erties: W e dr aw the straigh t line Axis P whic h meets P and whic h is parallel to Axis . W e hav e to distinguish three cases, the main one (1) and t w o trivial ones (2),(3) . (1) S Axis 6 = S and T Axis 6 = T . Then Axis P 6 = Axis , th e inte rsection of Axis P with Z S is called S P , and the in tersection of Axis P with Z T is calle d T P . Then the distance of S Axis and O r ig in is equal to the d istance of P and T P , and the distance of T Axis and Or igin is equal to the distance of P and S P . F urthermore, S Axis and P are on the same sid e of Z T , and T Axis and P are on the same sid e of Z S , resp ectiv ely . ( S ee Pictur e 2 ) . (2) S Axis = S . ( Hence, if G S 6 = G T then T Axis 6 = T ) . Then P := S Axis = S , and Axis P = Axis = Z S . The in tersection of Axis P with Z T is T P := O r ig in . Then, b y trivialit y , the distance of S Axis and O r ig in is equal to the distance of P and T P , and furthermore, by trivialit y , S Axis and P are on the same side of Z T . (3) T Axis = T . ( Hence, if G S 6 = G T then S Axis 6 = S ) . Then P := T Axis = T , and Axis P = Axis = Z T . The in tersection of Axis P with Z S is S P := O r ig in . Then, by trivialit y , the d istance of T Axis and O r igin is equal to the distance of P and S P , and furtherm ore, by trivialit y , T Axis and P are on the same side of Z S . Axis O r ig in Axis P G T G S L ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ✏ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ ❤ S T ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✱ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ Z S Z T S Axis T Axis P × T P S P Picture 2 5 Lemma 2. W e ha v e that p rop osition 1 ⇐ ⇒ pr op osition 2 . Pr o of. prop osition 1 ⇐ = prop osition 2: Ob viously , the t w o situations whic h are d escrib ed in prop osition 1 are sp ecia l cases of the general situation in prop osition 2 . More detailed, we ha v e O r ig in := (0 | 0) and if we define Axis := x -axis we get P hor = P , and Axis := y -axis yields P ver = P , resp ectiv ely . prop osition 1 = ⇒ prop osition 2: With an easy transformation of co ordinates, w e get (0 | 0) = Or igin , and x -axis = Axis , hence P = P hor . No w follo ws another p iece of ’Grecian Geometry’. Prop osition 3. Let us agai n tak e R 2 = { ( x | y ) | x , y ∈ R } . with the horizon tal x -axis and the vertic al y -axis. Consider the tw o parallel lines G, P ( P m eans ’pro jection line’) , with the prop erty that G do es n ot meet (0 | 0). Assum e a fi xed ε ∈ R . Let us c ho ose a p oin t ( b x | b y ) on G , b y 6 = 0 , such that neither the line that conn ects (0 | 0) and S := ( b x − ε | b y ), nor the line that connects (0 | 0) and T := ( b x + ε | b y ) is parallel to G and P . W e call S the pro jection of S on the lin e P , and T the pro jection of T on th e line P . (That means that th e three p oin ts (0 | 0) , S, S , and the three p oin ts (0 | 0) , T , T , r esp ectiv ely , are collinear, S , T ∈ P .) The four p oints S , T , − S , − T a re the corners of a parallel ogram. W e call ′ ν ′ the in tersection of the line that connects T and − S with the horizon tal x -axis. F or the claim we d istin gu ish tw o disjoin t cases: (A) If P and G are parallel to th e v ertical y -axis, then ν dep end s only on ε and on the in tersections of the horizon tal x -axis with G and P , resp ectiv ely . (B) If P an d G are not parallel to the v ertical y -axis, then ν dep ends only on ε and on the in tersections of the v ertical y -axis with G and P , resp ectiv ely . ( See Picture 3 ) . In other w ords we claim that the v alue of ν do es not d ep end on the c hoice of ( b x | b y ) on G , and also, ( in case (B) ) , that ν do es not dep end on the slop e of G and P . x y ✲ ✻ S S − S T T ν ( b x | b y ) P : y = 2 · x + 2 G : y = 2 · x + 4 y = 1 2 · x − 1 ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅                           ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ W e fix t w o lines P , G (with slop e 2) , and ε := 4 . W e choose ( b x | b y ) := (0 | 4) . W e get S = ( − 2 3 | 2 3 ) , T = ( − 2 | − 2) . Hence w e get ν = 2 . Picture 3 6 Pr o of. First the trivial cases. If P meets the origin (0 | 0) , then (0 | 0) = T = S , and the parallelogram collapses into a single p oin t (0 | 0) = ν . If ε = 0 , th en T = S , and the parallelogram degenerates to a line b etw een T and − S , that meets (0 | 0 ) = ν . Hence we assume that P do es not meet th e origin (0 | 0) , and we tak e (without loss of generalit y) an ε > 0 . W e distinguish b et ween v ertical G, P and not v ertical G, P . Thus assume v ertical lines G and P with equations G : x = r a nd P : x = p . After choosing a p oin t ( b x | b y ) on G , b y 6 = 0 , we can compu te S and T . Because G do es not m eet (0 | 0) w e ha v e r 6 = 0 , and some easy calculations yield ν = p · ε/r . In the case that G, P are not v ertical th ey ha v e a s lop e m ∈ R , and there are equations G : y = m · x + b G and P : y = m · x + b P with m, b G , b P ∈ R , b G , b P 6 = 0 . After c ho osing a p oin t ( b x | b y ) on G , b y 6 = 0 , w e get with elemen tary calculatio ns S = b P b G + m · ε · ( b x − ε | b y ) and T = b P b G − m · ε · ( b x + ε | b y ) . Some more calculati ons yield the form u la y = m · b x + b G b x · b G + m · ε 2 · [ b G · x − b P · ε ] for a non vertic al straight line that intersect s T and − S , and finally w e get ν = b P · ε/b G . If the lin e th at connects T and − S is ve rtical we get the same f orm ula for ν , and the pro of of the prop osition is complete. Remark 2. The four p oints S , T , − S , − T form the corners of a parallelogram, and, corre- sp ond ing to th e the v alue of ν wh ic h is the intersecti on of the line through T and − S with th e horizon tal axis, the line through S and − T mee ts the same axis in − ν , hence in − p · ε/r , (if b oth lines G, P are v ertical ) , or in − b P · ε/b G (if b oth lines G, P are n ot vertica l ) . Corollary 1 . If w e reve rse the roles of th e x -axis and y -axis, w e are able to form ulate a corresp ondin g statemen t: Consider the t w o parallel lines G, P , with the prop erty that G do es not meet (0 | 0). Assume a fixed ε ∈ R . Let u s choose a p oint ( b x | b y ) on G , b x 6 = 0 , such that neither the line that connects (0 | 0 ) and S v := ( b x | b y − ε ) , n or the line that co nnects (0 | 0) and T v := ( b x | b y + ε ) is p arallel to G and P . W e call S v the pro jection of S v on the line P , and T v the pro jection of T v on the line P . (That means that th e three p oints (0 | 0) , S v , S v , and the th ree p oin ts (0 | 0) , T v , T v , resp ectiv ely , are col linear, S v , T v ∈ P .) Th e four p oints S v , T v , − S v , − T v are the corners of a paralle logram. W e call ′ µ ′ the inte rsection of the line that conn ects T v and − S v with the v ertical y -axis , and we claim that th e v alue of µ do es not dep end on the c h oice of ( b x | b y ) on G . Pr o of. T rivial with the previous prop osition. Again w e write do wn the last pr op osition in a seemingly more general form. Prop osition 4. Let us again tak e the eu clidean space R 2 . Consider the t w o parallel lines G, P ( P means ’pro jection line’) , and an arbitrary third line ( 6 = G ) that w e call Axis . W e fix a p oin t Or ig in on Axis \ G , an d an ε ≥ 0 . Let us c ho ose a p oin t ( b x | b y ) on G \ Axis , and dra w the straigh t line [ Axis , meeting ( b x | b y ) and p arallel to Axis . W e m ark tw o uniqu e p oints S, T on [ Axis , suc h that the distance of b oth to ( b x | b y ) is ε . W e assume the extra prop erty that the line that connects O r igin and S and the line that connects O r ig in and 7 T are not p arallel to G and P , resp ectiv ely . Th us we are ab le to ’pr o ject’ S and T onto P . W e call S the pr o jection of S on the line P , and T the p r o jection of T on the line P , b oth pro jections relativ ely to Or ig in . (That means th at the three p oin ts O r ig in, S, S , and the three p oin ts O r ig in, T , T , r esp ectiv ely , a re collinear, S , T ∈ P .) F urther we denote t w o p oint s − S , − T , s uc h that the f our p oin ts O r ig in, S, S , − S , and the four p oints O r ig in, T , T , − T , resp ectiv ely , are collinear, and the distance of O r igin and S is equal to the distance of O r ig in and − S , and the d istance of O r igin and T is equal to the distance of O r ig in an d − T , resp ectiv ely . The four p oin ts S , T , − S , − T form a parallelo gram with cen tre Or ig in . W e call ′ ν ′ the in tersection of the line that connects T an d − S with Axis , and we claim that ν do es not d ep end on the c hoice of ( b x | b y ) on G . (See Picture 4) . Axis S S − S T − T × T ν ( b x | b y ) P O r ig in G ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ ✁ [ Axis ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅ ❅                         ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ ✟ Picture 4 Lemma 3. W e hav e that prop ositio n 3 = ⇒ pr op osition 4 . Pr o of. With an easy transform ation of coord inates, we get (0 | 0) = Or ig in , and x -axis = Axis . Remark 3. F or all prop ositions it w ould b e desirable to h a v e a construction with compass and ruler, using the classical metho ds of the ’old Greeks’. Ac knowledgemen ts W e thank Dr. Genc ho S k ordev, V erena Th ¨ urey , Dr. Nils Th ¨ urey and sp ecial ly Prof. Dr. Eb erh ard O eljeklaus f or int eresting discussions, critical commen ts and some new ideas. V OLKER TH ¨ UREY Rheinstr. 91 28199 Bremen, German y T: 49 (0)421 /5917 77 E-Mail: v olk er@thuerey .de 8 References [1] W. G¨ otz, W. Sc h w eize r, W. F ranke , K. Sc h¨ onw ald, ’ Analytisc he Geometrie ’ , Ernst Klett V erlag , Stuttgart 1954 [2] Robin Hartsh orn e , ’ Geometry: Euclid and Bey ond ’ , Sp ringer 1997 [3] D. W. Hall , St. Szab o , ’ Plane Geometry ’ , Prentice- Hall, E nglew oo d Cliffs, New Jers ey , 1971 [4] H. K in der, U. Sp engler, ’ Die Bew egungsgrupp e einer euklidischen Eb ene ’ , T eubn er 1980 [5] An dreas Filler, ’ Euklidische und nic h teuklidische Geomet rie ’ , BI Wissens c h aftsv erlag 1993 [6] H.S.M. C o xeter ’ Intro ductions to Geometry ’ , Wiley , New Y ork, 1969 [7] J ohn Ro e, ’ Elemen tary Geometry ’ , Oxford Un iv ersit y Press, 1993 [8] G.A. Bac kman, R.G. Cromie, ’ Intro d uction to C oncepts of Ge ometry ’ , Pren tice -Hall, Englew oo d Cliffs, New Jersey , 1971 9

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