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a8ec7fd1
Commit
a8ec7fd1
authored
Aug 12, 2020
by
Claude Meny
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Update textbook.fr.md
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...
@@ -171,18 +171,18 @@ espacio por el **vector $`\overrightarrow{OM}`$**.<br>
...
@@ -171,18 +171,18 @@ espacio por el **vector $`\overrightarrow{OM}`$**.<br>
[
FR
]
*Dans l’espace*
, la
*position d’un point M*
est repérée à partir d’un
**point O origine**
de
[
FR
]
*Dans l’espace*
, la
*position d’un point M*
est repérée à partir d’un
**point O origine**
de
l’espace par le
**vecteur $`\overrightarrow{OM}`$**
.
<br>
l’espace par le
**vecteur $`\overrightarrow{OM}`$**
.
<br>
[
EN
]
*In space*
, the
*position of a point M*
is marked from a
**point origin O**
of
[
EN
]
*In space*
, the
*position of a point M*
is marked from a
**point origin O**
of
the space by the
**
vector $`\overrightarrow{OM}`$**
.
<br>
the space by the
**vector $`\overrightarrow{OM}`$**
.
<br>
*
[
ES
]
El
*espacio clásico*
de Newton tiene
**3 dimensiones**
. Esto significa que, desde el origen O del espacio,
*
[
ES
]
El
*espacio clásico*
de Newton tiene
**3 dimensiones**
. Esto significa que, desde el origen O del espacio,
la posición de cualquier punto M se puede definir de forma única mediante
la posición de cualquier punto M se puede definir de forma única mediante
**3 números reales $`(\alpha_M, \beta_M, \gamm
m
a_M )`$**
, llamados
** coordenadas **
(o coordenadas espaciales)
**3 números reales $`(\alpha_M, \beta_M, \gamma_M )`$**
, llamados
** coordenadas **
(o coordenadas espaciales)
del punto M. Escribimos $
`M=M(\alpha_M, \beta_M, \gamm
m
a_M)`
$.
<br>
del punto M. Escribimos $
`M=M(\alpha_M, \beta_M, \gamma_M)`
$.
<br>
[
FR
]
L’
*espace classique de Newton*
a
**3 dimensions**
. Cela signifie que, à partir de l’origine O de l’espace,
[
FR
]
L’
*espace classique de Newton*
a
**3 dimensions**
. Cela signifie que, à partir de l’origine O de l’espace,
la position de tout point M peut-être définie de façon unique par
**3 nombres réels**
, appelés
la position de tout point M peut-être définie de façon unique par
**3 nombres réels**
$
`(\alpha_M, \beta_M, \gamma_M )`
$
**
**coordonnées**
(ou coordonnées spatiales) du point M. On écrit $
`M=M(\alpha_M, \beta_M, \gam
mma_M)`
$.
<br>
, appelés
**coordonnées**
(ou coordonnées spatiales) du point M. On écrit $
`M=M(\alpha_M, \beta_M, \ga
mma_M)`
$.
<br>
[
EN
]
The Newton's
*classical space*
has
**3 dimensions**
. This means that, from the origin O of space,
[
EN
]
The Newton's
*classical space*
has
**3 dimensions**
. This means that, from the origin O of space,
the position of any point M can be uniquely defined by
**3 real numbers**
, called
**coordinates**
(or
the position of any point M can be uniquely defined by
**3 real numbers**
$
`(\alpha_M, \beta_M, \gamma_M )`
$
**
,
spatial coordinates) of point M. We write $
`M=M(\alpha_M, \beta_M, \gam
mma_M)`
$.
called
**coordinates**
(or spatial coordinates) of point M. We write $
`M=M(\alpha_M, \beta_M, \ga
mma_M)`
$.
*
[
ES
]
Hay
*varias formas posibles de definir unas coordenadas espaciales*
: Hablamos de
*
[
ES
]
Hay
*varias formas posibles de definir unas coordenadas espaciales*
: Hablamos de
** sistemas de coordenadas**
.
<br>
** sistemas de coordenadas**
.
<br>
...
...
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