<s xml:space="preserve">
This folio contains Harriot's proof of the angle preserving properties of stereographic projection.
For the diagram see Add MS 6789, f. 18
<lb/>
For further details, including a transcript and translation, see Jon Pepper,
'Harriot's calculation of the meridional parts as logarithimic tangents',
Archive for History of Exact Sciences, 4(1968), 359–413 (pages 366–367, and </s>
<s xml:space="preserve">]</s>
</p>
</div>
<head xml:space="preserve" xml:lang="lat">
Quod rumbus in planispærio nostro facit angulum cum meridiano
<lb/>
æqualem angulo facto a rumbo cum meridiano in
<lb/>
[
<emph style="bf">Translation: </emph>
That a rhumb in our planisphere makes an angle with the meridian
equal to the angle made by the rhumb with the meridian on the sphere.</head>
<p xml:lang="lat">
<s xml:space="preserve">
Sit
<math>
<mstyle>
<mi>A</mi>
<mi>B</mi>
<mi>E</mi>
</mstyle>
</math>
semicirculus pro
<lb/>
meridiano quolibet in globo
<lb/>
terrestri.
<lb/>
Cuius centrum
<math>
<mstyle>
<mi>e</mi>
</mstyle>
</math>
. poli
<math>
<mstyle>
<mi>A</mi>
</mstyle>
</math>
et
<math>
<mstyle>
<mi>E</mi>
</mstyle>
</math>
.
<lb/>
<emph style="st">In illo meridiano sumatur quoduis </emph>
<lb/>
<emph style="st">punctum
<math>
<mstyle>
<mi>B</mi>
</mstyle>
</math>
.</emph>
<lb/>
Sit,
<math>
<mstyle>
<mi>e</mi>
<mi>X</mi>
</mstyle>
</math>
, communis sectio
<emph style="st">plani</emph>
<lb/>
æquatoris et plani meridiani,
<lb/>
quæ meridianus est in nostro
<lb/>
planisphærio correlatiuus meridiano
<lb/>
in globo terrestri.
<lb/>
In semicirculo pro meridiano
<lb/>
sumatur quodvis punctum
<math>
<mstyle>
<mi>B</mi>
</mstyle>
</math>
.
<lb/>
Agatur recta
<math>
<mstyle>
<mi>A</mi>
<mi>B</mi>
</mstyle>
</math>
producta quæ
<lb/>
secabit,
<math>
<mstyle>
<mi>e</mi>
<mi>X</mi>
</mstyle>
</math>
, in puncto
<math>
<mstyle>
<mi>b</mi>
</mstyle>
</math>
,
<lb/>
et punctum
<math>
<mstyle>
<mi>b</mi>
</mstyle>
</math>
in planisphærio erit
<lb/>
correllatium puncto
<math>
<mstyle>
<mi>B</mi>
</mstyle>
</math>
in superficie
<lb/>
sphæræ.
<lb/>
Agatur etiam recta,
<math>
<mstyle>
<mi>e</mi>
<mi>B</mi>
</mstyle>
</math>
, et
<math>
<mstyle>
<mi>G</mi>
<mi>H</mi>
</mstyle>
</math>
<lb/>
tangens peripheriam in puncto,
<math>
<mstyle>
<mi>B</mi>
</mstyle>
</math>
.
<lb/>
Dico primo quod anguli
<math>
<mstyle>
<mi>H</mi>
<mi>B</mi>
<mi>b</mi>
</mstyle>
</math>
et
<math>
<mstyle>
<mi>H</mi>
<mi>b</mi>
<mi>B</mi>
</mstyle>
</math>
<lb/>
sunt æquales.
<lb/>
<math>
<mstyle>
<mi>H</mi>
<mi>B</mi>
<mi>b</mi>
<mo>+</mo>
<mi>A</mi>
<mi>B</mi>
<mi>e</mi>
<mo>=</mo>
</mstyle>
</math>
recto.
<lb/>
<math>
<mstyle>
<mi>e</mi>
<mi>b</mi>
<mi>A</mi>
<mo>+</mo>
<mi>e</mi>
<mi>A</mi>
<mi>B</mi>
<mo>=</mo>
</mstyle>
</math>
recto.
<lb/>
Ergo:
<math>
<mstyle>
<mi>H</mi>
<mi>B</mi>
<mi>b</mi>
<mo>+</mo>
<mi>A</mi>
<mi>B</mi>
<mi>e</mi>
<mo>=</mo>
<mi>e</mi>
<mi>b</mi>
<mi>A</mi>
<mo>+</mo>
<mi>e</mi>
<mi>A</mi>
<mi>B</mi>
</mstyle>
</math>
.
<lb/>
Sed:
<math>
<mstyle>
<mi>A</mi>
<mi>B</mi>
<mi>e</mi>
<mo>=</mo>
<mi>e</mi>
<mi>A</mi>
<mi>B</mi>
</mstyle>
</math>
.
<lb/>
ergo:
<math>
<mstyle>
<mi>H</mi>
<mi>B</mi>
<mi>b</mi>
<mo>=</mo>
<mi>H</mi>
<mi>b</mi>
<mi>B</mi>
</mstyle>
</math>
<lb/>
[
<emph style="bf">Translation: </emph>
Let
<math>
<mstyle>
<mi>A</mi>
<mi>B</mi>
<mi>E</mi>
</mstyle>
</math>
be a semicircle on any meridian of the terrestrial sphere, with centre
<math>
<mstyle>
<mi>e</mi>
</mstyle>
</math>
, and poles
<math>
<mstyle>
<mi>A</mi>
</mstyle>
</math>
and
<math>
<mstyle>
<mi>E</mi>
</mstyle>
</math>
. Let
<math>
<mstyle>
<mi>e</mi>
<mi>X</mi>
</mstyle>
</math>
be the intersection of the equator and the meridional plane, which meridian in our planisphere corresponds to the meridian in the terrestrial sphere.
<lb/>
In the semicircle take any point
<math>
<mstyle>
<mi>B</mi>
</mstyle>
</math>
on the meridian. Construct the extended line
<math>
<mstyle>
<mi>A</mi>
<mi>B</mi>
</mstyle>
</math>
which will cut
<math>
<mstyle>
<mi>e</mi>
<mi>X</mi>
</mstyle>
</math>
in the point
<math>
<mstyle>
<mi>b</mi>
</mstyle>
</math>
, and the point
<math>
<mstyle>
<mi>b</mi>
</mstyle>
</math>
in the planisphere will correspond to the point
<math>
<mstyle>
<mi>B</mi>
</mstyle>
</math>
on the surface of the sphere. Also construct the lines
<math>
<mstyle>
<mi>e</mi>
<mi>B</mi>
</mstyle>
</math>
and
<math>
<mstyle>
<mi>G</mi>
<mi>H</mi>
</mstyle>
</math>
touching the circumference in the point
<math>
<mstyle>
<mi>B</mi>
</mstyle>
</math>
.
<lb/>
I say first that the angles
<math>
<mstyle>
<mi>H</mi>
<mi>B</mi>
<mi>b</mi>
</mstyle>
</math>
amd
<math>
<mstyle>
<mi>H</mi>
<mi>b</mi>
<mi>B</mi>
</mstyle>
</math>
are equal.
<lb/>
<math>
<mstyle>
<mi>H</mi>
<mi>B</mi>
<mi>b</mi>
<mo>+</mo>
<mi>A</mi>
<mi>B</mi>
<mi>e</mi>
<mo>=</mo>
</mstyle>
</math>
a right angle.
<lb/>
<math>
<mstyle>
<mi>e</mi>
<mi>b</mi>
<mi>A</mi>
<mo>+</mo>
<mi>e</mi>
<mi>A</mi>
<mi>B</mi>
<mo>=</mo>
</mstyle>
</math>
a right angle.
<lb/>
Therefore
<math>
<mstyle>
<mi>H</mi>
<mi>B</mi>
<mi>b</mi>
<mo>+</mo>
<mi>A</mi>
<mi>B</mi>
<mi>e</mi>
<mo>=</mo>
<mi>e</mi>
<mi>b</mi>
<mi>A</mi>
<mo>+</mo>
<mi>e</mi>
<mi>A</mi>
<mi>B</mi>
</mstyle>
</math>
.
<lb/>
But
<math>
<mstyle>
<mi>A</mi>
<mi>B</mi>
<mi>e</mi>
<mo>=</mo>
<mi>e</mi>
<mi>A</mi>
<mi>B</mi>
</mstyle>
</math>
.
<lb/>
Therefore
<math>
<mstyle>
<mi>H</mi>
<mi>B</mi>
<mi>b</mi>
<mo>=</mo>
<mi>H</mi>
<mi>b</mi>
<mi>B</mi>
</mstyle>
</math>
. </s>
</p>
<p xml:lang="lat">
<s xml:space="preserve">
Iam intelligitur
<math>
<mstyle>
<mi>B</mi>
</mstyle>
</math>
punctum esse centrum
<lb/>
circuli nautici qui vulgo compassus
<lb/>
dicitur; sive circuli horizontis visibilis.
<lb/>
cuius plano
<math>
<mstyle>
<mi>e</mi>
<mi>B</mi>
</mstyle>
</math>
, est ad angulos rectos.
<lb/>
<math>
<mstyle>
<mi>G</mi>
<mi>H</mi>
</mstyle>
</math>
est communis sectio plani meridiani
<lb/>
et
<emph style="super">illius</emph>
circuli nautici, et est linea dicta
<lb/>
meridiana in plano
<emph style="super">horizontis</emph>
<emph style="st">circuli nautici</emph>
.
<lb/>
Agatur
<emph style="super">quælibet</emph>
linea
<math>
<mstyle>
<mi>B</mi>
<mi>D</mi>
</mstyle>
</math>
<emph style="super">in plano horizontis</emph>
faciens
<emph style="st">quemvis</emph>
angulum
<math>
<mstyle>
<mi>D</mi>
<mi>B</mi>
<mi>G</mi>
</mstyle>
</math>
<lb/>
<emph style="st">cum meridiana
<math>
<mstyle>
<mi>B</mi>
<mi>G</mi>
</mstyle>
</math>
</emph>
<lb/>
et in illa linea sumatur quodvis punctum
<math>
<mstyle>
<mi>D</mi>
</mstyle>
</math>
<lb/>
et Agatur
<math>
<mstyle>
<mi>D</mi>
<mi>C</mi>
</mstyle>
</math>
perpendicularis ad
<math>
<mstyle>
<mi>G</mi>
<mi>H</mi>
</mstyle>
</math>
.
<lb/>
Conectantur puncta
<math>
<mstyle>
<mi>A</mi>
<mi>C</mi>
</mstyle>
</math>
: et
<math>
<mstyle>
<mi>A</mi>
<mi>D</mi>
</mstyle>
</math>
. et constituatur
<lb/>
pyramis cuius basis
<math>
<mstyle>
<mi>B</mi>
<mi>C</mi>
<mi>D</mi>
</mstyle>
</math>
, et vertex,
<math>
<mstyle>
<mi>A</mi>
</mstyle>
</math>
.
<lb/>
Quoniam
<math>
<mstyle>
<mi>C</mi>
<mi>D</mi>
</mstyle>
</math>
, perpendicularis est in plano
<lb/>
erecto ad planum meridionis circuli productum
<lb/>
erit etiam perpendicularis ad
<math>
<mstyle>
<mi>C</mi>
<mi>A</mi>
</mstyle>
</math>
, et planum
<lb/>
trianguli
<math>
<mstyle>
<mi>D</mi>
<mi>C</mi>
<mi>A</mi>
</mstyle>
</math>
erit erectum ad planum
<lb/>
meridiani.
<lb/>
Linea
<math>
<mstyle>
<mi>A</mi>
<mi>C</mi>
</mstyle>
</math>
, secat,
<math>
<mstyle>
<mi>e</mi>
<mi>X</mi>
</mstyle>
</math>
, in puncto
<math>
<mstyle>
<mi>c</mi>
</mstyle>
</math>
<lb/>
(non opus est ducere lineas
<lb/>
<math>
<mstyle>
<mi>D</mi>
<mi>F</mi>
</mstyle>
</math>
, et
<math>
<mstyle>
<mi>C</mi>
<mi>F</mi>
</mstyle>
</math>
. ideo
<lb/>
[
<emph style="bf">Translation: </emph>
Now it is to be understood that the point
<math>
<mstyle>
<mi>B</mi>
</mstyle>
</math>
is the centre of a nautical circle, which is commonly called the compass; or circle of the visible horizon, which is at right angles to the plane of
<math>
<mstyle>
<mi>e</mi>
<mi>B</mi>
</mstyle>
</math>
.
<lb/>
<math>
<mstyle>
<mi>G</mi>
<mi>H</mi>
</mstyle>
</math>
is common to the plane of the meridian and that nautical circle and is said to be the meridional line in the horizontal plane.
<lb/>
Construct any line
<math>
<mstyle>
<mi>B</mi>
<mi>D</mi>
</mstyle>
</math>
in the horizontal plane making any angle
<math>
<mstyle>
<mi>D</mi>
<mi>B</mi>
<mi>G</mi>
</mstyle>
</math>
with the meridian
<math>
<mstyle>
<mi>B</mi>
<mi>G</mi>
</mstyle>
</math>
and in that lane take any point
<math>
<mstyle>
<mi>D</mi>
</mstyle>
</math>
, and construct
<math>
<mstyle>
<mi>D</mi>
<mi>C</mi>
</mstyle>
</math>
perpendicular to
<math>
<mstyle>
<mi>G</mi>
<mi>H</mi>
</mstyle>
</math>
. Join the points
<math>
<mstyle>
<mi>A</mi>
<mi>C</mi>
</mstyle>
</math>
and
<math>
<mstyle>
<mi>A</mi>
<mi>D</mi>
</mstyle>
</math>
to make a pyramid whose base is
<math>
<mstyle>
<mi>B</mi>
<mi>C</mi>
<mi>D</mi>
</mstyle>
</math>
and vertex
<math>
<mstyle>
<mi>A</mi>
</mstyle>
</math>
. Since
<math>
<mstyle>
<mi>C</mi>
<mi>D</mi>
</mstyle>
</math>
is a perpendicular in a plane at right angles to the plane of the circle of the meridion, it is also perpendicular to
<math>
<mstyle>
<mi>C</mi>
<mi>A</mi>
</mstyle>
</math>
, and the plane of triangle
<math>
<mstyle>
<mi>D</mi>
<mi>C</mi>
<mi>A</mi>
</mstyle>
</math>
will be at right angles to the plane of the meridian.
<lb/>
The line
<math>
<mstyle>
<mi>A</mi>
<mi>C</mi>
</mstyle>
</math>
cuts
<math>
<mstyle>
<mi>e</mi>
<mi>X</mi>
</mstyle>
</math>
in the point
<math>
<mstyle>
<mi>c</mi>
</mstyle>
</math>
.
<lb/>
(there is no need to draw the lines
<math>
<mstyle>
<mi>D</mi>
<mi>F</mi>
</mstyle>
</math>
and
<math>
<mstyle>
<mi>C</mi>
<mi>F</mi>
</mstyle>
</math>
, therefore they are omitted). </s>
</p>
<p xml:lang="lat">
<s xml:space="preserve">
Et in plano
<math>
<mstyle>
<mi>A</mi>
<mi>C</mi>
<mi>D</mi>
</mstyle>
</math>
a puncto
<math>
<mstyle>
<mi>c</mi>
</mstyle>
</math>
<lb/>
in linea
<math>
<mstyle>
<mi>A</mi>
<mi>C</mi>
</mstyle>
</math>
erigatur,
<math>
<mstyle>
<mi>c</mi>
<mi>d</mi>
</mstyle>
</math>
, ad
<lb/>
angulos rectos, quæ secabit
<math>
<mstyle>
<mi>A</mi>
<mi>D</mi>
</mstyle>
</math>
<lb/>
in puncto
<math>
<mstyle>
<mi>d</mi>
</mstyle>
</math>
. Et erit communis
<lb/>
sectio æquatoris et trianguli
<math>
<mstyle>
<mi>A</mi>
<mi>C</mi>
<mi>D</mi>
</mstyle>
</math>
.
<lb/>
Connectantur puncta
<math>
<mstyle>
<mi>d</mi>
</mstyle>
</math>
,
<math>
<mstyle>
<mi>b</mi>
</mstyle>
</math>
.
<lb/>
Dico quod angulus
<math>
<mstyle>
<mi>d</mi>
<mi>b</mi>
<mi>c</mi>
</mstyle>
</math>
in plano
<lb/>
æquatoris est qualis angulo
<lb/>
<math>
<mstyle>
<mi>D</mi>
<mi>B</mi>
<mi>C</mi>
</mstyle>
</math>
in plano horizontis
<lb/>
sive circuli nauticis.
<lb/>
producatur
<math>
<mstyle>
<mi>A</mi>
<mi>B</mi>
</mstyle>
</math>
et sit
<math>
<mstyle>
<mi>C</mi>
<mi>F</mi>
</mstyle>
</math>
perpen-
<lb/>
dicularis ad illam.
<lb/>
fiat
<math>
<mstyle>
<mi>F</mi>
<mi>P</mi>
<mo>=</mo>
<mi>F</mi>
<mi>B</mi>
</mstyle>
</math>
<lb/>
et agantur
<math>
<mstyle>
<mi>F</mi>
<mi>C</mi>
</mstyle>
</math>
,
<math>
<mstyle>
<mi>F</mi>
<mi>D</mi>
</mstyle>
</math>
,
<math>
<mstyle>
<mi>P</mi>
<mi>C</mi>
</mstyle>
</math>
, et
<math>
<mstyle>
<mi>P</mi>
<mi>D</mi>
</mstyle>
</math>
.
<lb/>
Quoniam
<math>
<mstyle>
<mi>D</mi>
<mi>C</mi>
</mstyle>
</math>
est perpendicularis
<lb/>
ad planum meridiani, facit
<lb/>
rectos angulos cum
<math>
<mstyle>
<mi>C</mi>
<mi>A</mi>
</mstyle>
</math>
,
<math>
<mstyle>
<mi>C</mi>
<mi>B</mi>
</mstyle>
</math>
,
<math>
<mstyle>
<mi>C</mi>
<mi>F</mi>
</mstyle>
</math>
,
<lb/>
et
<math>
<mstyle>
<mi>C</mi>
<mi>P</mi>
</mstyle>
</math>
.
<lb/>
Cum etiam
<math>
<mstyle>
<mi>C</mi>
<mi>B</mi>
</mstyle>
</math>
et
<math>
<mstyle>
<mi>C</mi>
<mi>P</mi>
</mstyle>
</math>
, sunt æquales
<lb/>
triangula rectangula
<math>
<mstyle>
<mi>B</mi>
<mi>C</mi>
<mi>D</mi>
</mstyle>
</math>
<lb/>
et
<math>
<mstyle>
<mi>P</mi>
<mi>C</mi>
<mi>D</mi>
</mstyle>
</math>
, sunt æqualia et
<lb/>
æquiangula, et angulus
<math>
<mstyle>
<mi>C</mi>
<mi>B</mi>
<mi>D</mi>
</mstyle>
</math>
<lb/>
æqualis est
<math>
<mstyle>
<mi>C</mi>
<mi>P</mi>
<mi>D</mi>
</mstyle>
</math>
.
<lb/>
Sed angulus
<math>
<mstyle>
<mi>c</mi>
<mi>b</mi>
<mi>d</mi>
</mstyle>
</math>
<emph style="super">in æquatore</emph>
est æqualis
<lb/>
<math>
<mstyle>
<mi>C</mi>
<mi>P</mi>
<mi>D</mi>
</mstyle>
</math>
, ob parallelismum
<lb/>
triangulorm
<math>
<mstyle>
<mi>c</mi>
<mi>b</mi>
<mi>d</mi>
</mstyle>
</math>
et
<math>
<mstyle>
<mi>C</mi>
<mi>P</mi>
<mi>D</mi>
</mstyle>
</math>
<lb/>
nam
<math>
<mstyle>
<mi>c</mi>
<mi>d</mi>
</mstyle>
</math>
est parallela
<math>
<mstyle>
<mi>C</mi>
<mi>D</mi>
</mstyle>
</math>
<lb/>
et
<math>
<mstyle>
<mi>c</mi>
<mi>b</mi>
</mstyle>
</math>
,
<math>
<mstyle>
<mi>C</mi>
<mi>P</mi>
</mstyle>
</math>
, quia:
<lb/>
<math>
<mstyle>
<mi>c</mi>
<mi>b</mi>
<mi>A</mi>
<mo>=</mo>
<mi>C</mi>
<mi>P</mi>
<mi>A</mi>
<mo>=</mo>
<mi>C</mi>
<mi>B</mi>
<mi>P</mi>
<mo>=</mo>
<mi>H</mi>
<mi>B</mi>
<mi>b</mi>
<mo>=</mo>
<mi>H</mi>
<mi>b</mi>
<mi>B</mi>
</mstyle>
</math>
<lb/>
ergo tertium latus
<math>
<mstyle>
<mi>d</mi>
<mi>b</mi>
</mstyle>
</math>
<lb/>
est parallelum
<math>
<mstyle>
<mi>D</mi>
<mi>P</mi>
</mstyle>
</math>
<lb/>
ergo plana triang-
<lb/>
ulorum
<math>
<mstyle>
<mi>c</mi>
<mi>b</mi>
<mi>d</mi>
</mstyle>
</math>
et CPD
<math>
<mstyle/>
</math>
<lb/>
sunt parallela. Et
<lb/>
similia, et angulus
<lb/>
<math>
<mstyle>
<mi>c</mi>
<mi>b</mi>
<mi>d</mi>
<mo>=</mo>
<mi>C</mi>
<mi>P</mi>
<mi>D</mi>
</mstyle>
</math>
.
<lb/>
Ergo
<math>
<mstyle>
<mi>c</mi>
<mi>b</mi>
<mi>d</mi>
<mo>=</mo>
<mi>C</mi>
<mi>B</mi>
<mi>D</mi>
</mstyle>
</math>
.
<lb/>
quod demonstrandum
<lb/>
fuit.
<lb/>
Aliter
<lb/>
<math>
<mstyle>
<mi>d</mi>
<mi>b</mi>
</mstyle>
</math>
est parall.
<math>
<mstyle>
<mi>D</mi>
<mi>P</mi>
<mo>,</mo>
<mi>q</mi>
<mi>u</mi>
<mi>i</mi>
<mi>a</mi>
</mstyle>
</math>
<lb/>
[
<emph style="bf">Translation: </emph>
And in the plane
<math>
<mstyle>
<mi>A</mi>
<mi>C</mi>
<mi>D</mi>
</mstyle>
</math>
, there is constructed
<math>
<mstyle>
<mi>c</mi>
<mi>d</mi>
</mstyle>
</math>
from point
<math>
<mstyle>
<mi>c</mi>
</mstyle>
</math>
at right angles to the line
<math>
<mstyle>
<mi>A</mi>
<mi>C</mi>
</mstyle>
</math>
, which will cut
<math>
<mstyle>
<mi>A</mi>
<mi>D</mi>
</mstyle>
</math>
in the point
<math>
<mstyle>
<mi>d</mi>
</mstyle>
</math>
. And it will be common to the equatorial plane and the triangle
<math>
<mstyle>
<mi>A</mi>
<mi>C</mi>
<mi>D</mi>
</mstyle>
</math>
. Join the points
<math>
<mstyle>
<mi>d</mi>
</mstyle>
</math>
and
<math>
<mstyle>
<mi>b</mi>
</mstyle>
</math>
.
<lb/>
I say that the angle
<math>
<mstyle>
<mi>d</mi>
<mi>b</mi>
<mi>c</mi>
</mstyle>
</math>
in the equatorial plane is equal to angle
<math>
<mstyle>
<mi>D</mi>
<mi>B</mi>
<mi>C</mi>
</mstyle>
</math>
in the horizontal plane, or nautical circle.
<lb/>
Let
<math>
<mstyle>
<mi>A</mi>
<mi>B</mi>
</mstyle>
</math>
be extended, and let
<math>
<mstyle>
<mi>C</mi>
<mi>F</mi>
</mstyle>
</math>
be perpendicular to it. Make
<math>
<mstyle>
<mi>F</mi>
<mi>P</mi>
<mo>=</mo>
<mi>F</mi>
<mi>B</mi>
</mstyle>
</math>
and construct
<math>
<mstyle>
<mi>F</mi>
<mi>C</mi>
</mstyle>
</math>
,
<math>
<mstyle>
<mi>F</mi>
<mi>D</mi>
</mstyle>
</math>
,
<math>
<mstyle>
<mi>P</mi>
<mi>C</mi>
</mstyle>
</math>
, and
<math>
<mstyle>
<mi>P</mi>
<mi>D</mi>
</mstyle>
</math>
.
<lb/>
Since
<math>
<mstyle>
<mi>D</mi>
<mi>C</mi>
</mstyle>
</math>
is perpendicular to the plane of the meridian, it makes right angles with