import work from year 2015-2016
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3e/Unites_et_grandeurs/Changement_unites/Exo/Exo_verres.pdf
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3e/Unites_et_grandeurs/Changement_unites/Exo/Exo_verres.tex
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3e/Unites_et_grandeurs/Changement_unites/Exo/Exo_verres.tex
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\documentclass[a5paper,12pt]{/media/documents/Cours/Prof/Enseignements/tools/style/classExo}
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\usepackage{/media/documents/Cours/Prof/Enseignements/2015_2016}
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% Title Page
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\titre{Changement d'unité - Exercices}
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% \seconde \premiereS \PSTMG \TSTMG
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\classe{Troisième}
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\date{Octobre 2015}
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\begin{document}
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% inspiré de http://www.ilemaths.net/forum-sujet-496010.html
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\vfill
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Pour une soirée d'inauguration, les serveurs décident de préparer le cocktail suivant (la recette est donnée pour 4 verres)
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\begin{itemize}
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\item $\frac{1}{3}$L de jus d'orange
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\item 1,6dL de jus d'abricot
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\item 8cL de jus de citron vert
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\item une banane (d'un volume d'environ $110cm^3$)
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\item 1 cuillère à café de miel (d'un volume d'environ $5cm^3$)
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\item 4mL de sirop de grenadine
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\end{itemize}
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\vfill
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\begin{enumerate}
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\item Quel est le volume d'un verre de ce cocktail? Donner le résultat en $cm^3$ arrondi à l'unité.
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\vfill
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\item Pour que les convives puissent apprécier leur cocktail, il doit être servi dans un beau verre ni trop rempli ni pas assez. Lequel de ces trois verres sera le plus approprier pour servir ce cocktail?
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\begin{center}
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\includegraphics[scale=0.4]{./fig/verres}
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\end{center}
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\vfill
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On rappelle que le volume d'un cône est $V = \frac{1}{3} \pi \times r^2 \times h$
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\end{enumerate}
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\vfill
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\end{document}
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%%% Local Variables:
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%%% mode: latex
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%%% TeX-master: "master"
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%%% End:
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3e/Unites_et_grandeurs/Changement_unites/Exo/fig/verres.pdf
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3e/Unites_et_grandeurs/Changement_unites/Exo/fig/verres.pdf
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3e/Unites_et_grandeurs/Changement_unites/Exo/fig/verres.svg
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sodipodi:role="line"
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x="881.90015"
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y="692.17175"
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id="tspan3127">h = 4cm</tspan></text>
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</g>
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</svg>
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|
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3e/Unites_et_grandeurs/Changement_unites/Exo/planetes.pdf
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3e/Unites_et_grandeurs/Changement_unites/Exo/planetes.pdf
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3e/Unites_et_grandeurs/Changement_unites/Exo/planetes.tex
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3e/Unites_et_grandeurs/Changement_unites/Exo/planetes.tex
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\documentclass[a4paper,10pt,landscape, twocolumn]{/media/documents/Cours/Prof/Enseignements/tools/style/classExo}
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\usepackage{/media/documents/Cours/Prof/Enseignements/2015_2016}
|
||||
|
||||
|
||||
% Title Page
|
||||
\titre{Changement d'unité notation scientifique - Exercices}
|
||||
% \seconde \premiereS \PSTMG \TSTMG
|
||||
\classe{Troisième}
|
||||
\date{Octobre 2015}
|
||||
|
||||
\pagestyle{empty}
|
||||
\geometry{left=5mm,right=5mm, bottom= 5mm, top=5mm}
|
||||
|
||||
|
||||
\begin{document}
|
||||
|
||||
|
||||
\begin{Exo}
|
||||
Voici les caractéristiques de plusieurs planètes du système solaire.
|
||||
\begin{multicols}{2}
|
||||
|
||||
\hspace{-0.5cm}
|
||||
\begin{tabular}{|c|p{2cm}|c|}
|
||||
\hline
|
||||
Planète & Rayon moyen (km) & Masse(kg) \\
|
||||
\hline
|
||||
Mercure & 2439,7 & $3,302\times 10^{23}$ \\
|
||||
\hline
|
||||
Terre & 6 371 & $5,9736 \times 10^{24}$ \\
|
||||
\hline
|
||||
Mars & 3390 & $6,4185 \times 10^{23}$ \\
|
||||
\hline
|
||||
Jupiter & 69 911 & $1,8986 \times 10^{27}$ \\
|
||||
\hline
|
||||
Neptune & 24 622 & $1,0243 \times 10^{26}$ \\
|
||||
\hline
|
||||
\end{tabular}
|
||||
\begin{enumerate}
|
||||
\item Classer ces planètes de la plus petite à la plus grande.
|
||||
\item Classer ces planète en fonction de leur masse.
|
||||
\item Classe les planètes selon leur masse volumique. La formule pour calculer la masse volumique est ($m$ représente la masse et $r$ le rayon).
|
||||
\begin{eqnarray*}
|
||||
\frac{3m}{4\pi\times r^3}
|
||||
\end{eqnarray*}
|
||||
\item Peut-on, à partir du calcul de la masse volumique faire deux groupes de planètes, les planètes gazeuses (planètes faites de gaz) et les planètes tellurique (planètes faites de roche)?
|
||||
|
||||
\end{enumerate}
|
||||
\end{multicols}
|
||||
|
||||
\end{Exo}
|
||||
\setcounter{exo}{0}
|
||||
|
||||
\begin{Exo}
|
||||
Voici les caractéristiques de plusieurs planètes du système solaire.
|
||||
\begin{multicols}{2}
|
||||
|
||||
\hspace{-0.5cm}
|
||||
\begin{tabular}{|c|p{2cm}|c|}
|
||||
\hline
|
||||
Planète & Rayon moyen (km) & Masse(kg) \\
|
||||
\hline
|
||||
Mercure & 2439,7 & $3,302\times 10^{23}$ \\
|
||||
\hline
|
||||
Terre & 6 371 & $5,9736 \times 10^{24}$ \\
|
||||
\hline
|
||||
Mars & 3390 & $6,4185 \times 10^{23}$ \\
|
||||
\hline
|
||||
Jupiter & 69 911 & $1,8986 \times 10^{27}$ \\
|
||||
\hline
|
||||
Neptune & 24 622 & $1,0243 \times 10^{26}$ \\
|
||||
\hline
|
||||
\end{tabular}
|
||||
\begin{enumerate}
|
||||
\item Classer ces planètes de la plus petite à la plus grande.
|
||||
\item Classer ces planète en fonction de leur masse.
|
||||
\item Classe les planètes selon leur masse volumique. La formule pour calculer la masse volumique est ($m$ représente la masse et $r$ le rayon).
|
||||
\begin{eqnarray*}
|
||||
\frac{3m}{4\pi\times r^3}
|
||||
\end{eqnarray*}
|
||||
\item Peut-on, à partir du calcul de la masse volumique faire deux groupes de planètes, les planètes gazeuses (planètes faites de gaz) et les planètes tellurique (planètes faites de roche)?
|
||||
|
||||
\end{enumerate}
|
||||
\end{multicols}
|
||||
|
||||
\end{Exo}
|
||||
\pagebreak
|
||||
\setcounter{exo}{0}
|
||||
|
||||
\begin{Exo}
|
||||
Voici les caractéristiques de plusieurs planètes du système solaire.
|
||||
\begin{multicols}{2}
|
||||
|
||||
\hspace{-0.5cm}
|
||||
\begin{tabular}{|c|p{2cm}|c|}
|
||||
\hline
|
||||
Planète & Rayon moyen (km) & Masse(kg) \\
|
||||
\hline
|
||||
Mercure & 2439,7 & $3,302\times 10^{23}$ \\
|
||||
\hline
|
||||
Terre & 6 371 & $5,9736 \times 10^{24}$ \\
|
||||
\hline
|
||||
Mars & 3390 & $6,4185 \times 10^{23}$ \\
|
||||
\hline
|
||||
Jupiter & 69 911 & $1,8986 \times 10^{27}$ \\
|
||||
\hline
|
||||
Neptune & 24 622 & $1,0243 \times 10^{26}$ \\
|
||||
\hline
|
||||
\end{tabular}
|
||||
\begin{enumerate}
|
||||
\item Classer ces planètes de la plus petite à la plus grande.
|
||||
\item Classer ces planète en fonction de leur masse.
|
||||
\item Classe les planètes selon leur masse volumique. La formule pour calculer la masse volumique est ($m$ représente la masse et $r$ le rayon).
|
||||
\begin{eqnarray*}
|
||||
\frac{3m}{4\pi\times r^3}
|
||||
\end{eqnarray*}
|
||||
\item Peut-on, à partir du calcul de la masse volumique faire deux groupes de planètes, les planètes gazeuses (planètes faites de gaz) et les planètes tellurique (planètes faites de roche)?
|
||||
|
||||
\end{enumerate}
|
||||
\end{multicols}
|
||||
|
||||
\end{Exo}
|
||||
\setcounter{exo}{0}
|
||||
|
||||
\begin{Exo}
|
||||
Voici les caractéristiques de plusieurs planètes du système solaire.
|
||||
\begin{multicols}{2}
|
||||
|
||||
\hspace{-0.5cm}
|
||||
\begin{tabular}{|c|p{2cm}|c|}
|
||||
\hline
|
||||
Planète & Rayon moyen (km) & Masse(kg) \\
|
||||
\hline
|
||||
Mercure & 2439,7 & $3,302\times 10^{23}$ \\
|
||||
\hline
|
||||
Terre & 6 371 & $5,9736 \times 10^{24}$ \\
|
||||
\hline
|
||||
Mars & 3390 & $6,4185 \times 10^{23}$ \\
|
||||
\hline
|
||||
Jupiter & 69 911 & $1,8986 \times 10^{27}$ \\
|
||||
\hline
|
||||
Neptune & 24 622 & $1,0243 \times 10^{26}$ \\
|
||||
\hline
|
||||
\end{tabular}
|
||||
\begin{enumerate}
|
||||
\item Classer ces planètes de la plus petite à la plus grande.
|
||||
\item Classer ces planète en fonction de leur masse.
|
||||
\item Classe les planètes selon leur masse volumique. La formule pour calculer la masse volumique est ($m$ représente la masse et $r$ le rayon).
|
||||
\begin{eqnarray*}
|
||||
\frac{3m}{4\pi\times r^3}
|
||||
\end{eqnarray*}
|
||||
\item Peut-on, à partir du calcul de la masse volumique faire deux groupes de planètes, les planètes gazeuses (planètes faites de gaz) et les planètes tellurique (planètes faites de roche)?
|
||||
|
||||
\end{enumerate}
|
||||
\end{multicols}
|
||||
|
||||
\end{Exo}
|
||||
\pagebreak
|
||||
|
||||
|
||||
|
||||
\pagebreak
|
||||
\end{document}
|
||||
|
||||
%%% Local Variables:
|
||||
%%% mode: latex
|
||||
%%% TeX-master: "master"
|
||||
%%% End:
|
||||
|
||||
Reference in New Issue
Block a user