diff --git a/assets/common.less b/assets/common.less
index 17bbe0f9..cd897d55 100644
--- a/assets/common.less
+++ b/assets/common.less
@@ -336,18 +336,24 @@ body {
}
/* Video and text dialogs */
-.video-wrapper {
+
+.video-wrapper {
+ display: flex;
height: 100%;
- background: black;
+ background: rgba(0, 0, 0, 0.5);
+ backdrop-filter: blur(2px);
text-align: center;
z-index: 1000;
}
video {
- height: 100%;
+ margin: auto;
+ height: 85%;
width: auto;
max-width: 100%;
object-fit: contain;
+ // aspect-ratio: 9/17;
+ border: 5px solid white;
}
#video-container {
@@ -360,6 +366,28 @@ video {
overflow: hidden;
padding: 0px;
z-index: 1000;
+
+ #video-close-icon {
+ top: 2rem;
+ right: 2rem;
+ transform: scale(2);
+ }
+}
+
+.close-icon {
+ position: absolute;
+ top: 10px;
+ right: 10px;
+ z-index: 15;
+
+ &:hover {
+ cursor: pointer;
+ }
+
+ &:focus {
+ color: white;
+ border: 2px solid white;
+ }
}
.bottom-sheet {
diff --git a/radwave/src/GifPlayPause.vue b/radwave/src/GifPlayPause.vue
new file mode 100644
index 00000000..2856b2de
--- /dev/null
+++ b/radwave/src/GifPlayPause.vue
@@ -0,0 +1,177 @@
+
+
+
+
+
+ For most of human history, we have not known how far the stars are from us. + It wasn't until the 20th century that we developed the tools to measure distances to stars. + By studying the distances to stars astronomers can learn a great deal about the structure of our galaxy. +
++ In and amongst the stars are star forming regions - clouds of gas and dust where stars form. + Because dust is between us and the stars, astronomers can also measure the distances to these star forming regions. + It was by looking at the distances to nearby star forming regions that astronomers discovered a large structure which they called + the Radcliffe Wave. + While shaped like a wave, the question remained…phot +
+After a great deal of work, the answer is yes. + By analyzing the velocities of young star clusters associated with the star forming regions, + they determined that their motions match what one would expect if they were riding on a wave as it travels through the galaxy. + The wave goes up and down every 95 million years or so! + However, the clusters and star forming clouds we see surfing the wave right now will dispers before a full cycle is complete +
+ The clusters follow a "damped traveling wave" pattern. This type of wave motion is practically visualized below by two of the astronomers involved in this discovery, + Catherine Zucker and Ralf Konietzka. + ++ The Radcliffe Wave spans about 100° of the sky between the constellations of Cygnus (The Swan) and Orion (The Hunter). + It is about 1000 lightyears away at it's closest point, with a length of about 9000 lightyears. + Despite ~100 clusters and star forming regions being associated with the wave, their connection is not obvious from the view point on Earth. + It was not until astronomers looked at the positions and distances in 3D that the structure became apparent. +
+