diff --git a/R1.02/tp/tp1/correction/exercice1.html b/R1.02/tp/tp1/correction/exercice1.html new file mode 100644 index 0000000..af8c871 --- /dev/null +++ b/R1.02/tp/tp1/correction/exercice1.html @@ -0,0 +1,23 @@ + + + + + + + Exercice 1 + + +

Le W3C

+

+ Le W3C est un consortium créé + le par Tim Berners-Lee, + principal inventeur du World Wide Web en , pour promouvoir + la compatibilité et donc la normalisation des technologies du World Wide Web. Avant le + W3C, c'était l'IETF, + un autre organisme important de l'Internet, qui était en charge de cette mission. +

+

+ Le W3C a par exemple standardisé les technologies HTML et XML. +

+ + diff --git a/R1.02/tp/tp1/correction/exercice2.html b/R1.02/tp/tp1/correction/exercice2.html new file mode 100644 index 0000000..da8af22 --- /dev/null +++ b/R1.02/tp/tp1/correction/exercice2.html @@ -0,0 +1,54 @@ + + + + + + + + Exercice 2 + + +

Emoticons

+ +

+ Emoticons are textual portrayals of a writer's moods or facial + expressions in the form of icons. Originally, these icons + consisted of ASCII art. +

+ +

+ Emoticons can generally be divided into two groups: Western (mainly + from America and Europe) or horizontal; Eastern or vertical (mainly + from east Asia). +

+ +

Western

+ +

+ Western style emoticons are mostly written from left to right as + though the head is rotated counter-clockwise 90 degrees. +

+ + + +

Eastern

+ +

+ Eastern emoticons generally are not rotated sideways. They first + arose in Japan, where they are referred to as kaomoji. +

+ + + + diff --git a/R1.02/tp/tp1/correction/exercice3.html b/R1.02/tp/tp1/correction/exercice3.html new file mode 100644 index 0000000..d0c6e94 --- /dev/null +++ b/R1.02/tp/tp1/correction/exercice3.html @@ -0,0 +1,40 @@ + + + + + + + Exercice 3 + + + + + + +

Sites

+ + + + + +

Sites

+
    +
  1. WEB iut : Site web IUT
    2. +
  2. GIT iut : Service Git de l'IUT
    3. +
+ + + +

Sites

+
+
WEB iut
+
Site web IUT
+
GIT iut
+
Service Git de l'IUT
+
+ + + diff --git a/R1.02/tp/tp1/correction/exercice4.html b/R1.02/tp/tp1/correction/exercice4.html new file mode 100644 index 0000000..4ef0734 --- /dev/null +++ b/R1.02/tp/tp1/correction/exercice4.html @@ -0,0 +1,50 @@ + + + + + + + + Exercice 4 + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + +
Orbites des planètes du Système solaire
PlanèteDistance moyenne (UA)Exentricité Inclinaison  (°)Période de révolution (an)Photo
Mercure0,387098930,20570,241Mercure
Venus0,723331990,0073,40,615Venus
Terre10,01701Terre
Mars1,523662310,0941,91,881Mars
Jupiter5,203363010,0491,311,862Jupiter
Saturne9,60,0572,529,452Saturne
Uranus2872,50,897,830,589Uranus
Neptune4495,11,828,359,8Neptune
+ + diff --git a/R1.02/tp/tp1/correction/exercice5.html b/R1.02/tp/tp1/correction/exercice5.html new file mode 100644 index 0000000..0afa383 --- /dev/null +++ b/R1.02/tp/tp1/correction/exercice5.html @@ -0,0 +1,23 @@ + + + + + + + + Exercice 5 + + + web stack + + + + + + + JS + CSS + html + + +