WEBVTT 00:03.833 --> 00:07.200 align:left position:20% line:83% size:70% ELLO THERE ECLIPSE ENTHUSIASTS TRACE HERE~ 00:07.200 --> 00:11.666 align:left position:10% line:77% size:80% THIS WEEK IS AN ANNULAR SOLAR ECLIPSE OVER THE PACIFIC OCEAN AND THE TIP 00:11.666 --> 00:15.533 align:left position:10% line:77% size:80% OF SOUTH AMERICA. SORRY. BUT, THIS IS AN OPPORTUNITY TO EXPLAIN WHY ECLIPSES COME 00:15.533 --> 00:19.700 align:left position:20% line:83% size:70% WITH FRIENDS! FIRST WE NEED TO FIND THE ECLIPTIC. 00:19.700 --> 00:22.633 align:left position:10% line:71% size:80% HERE’S THE SKY AT SUNSET ON OCTOBER 5. THE BRIGHT DOT THERE IS THE PLANET VENUS HEY GIRL! NOW, 00:25.266 --> 00:29.566 align:left position:10% line:77% size:80% TRACE A LINE ACROSS THE SKY TO SATURN IN THE SOUTHEAST THAT IMAGINARY LINE IS THE ECLIPTIC! 00:29.566 --> 00:32.466 align:left position:10% line:77% size:80% IF YOU TRACK THE MOON YOU’D NOTE IT RUNS ALMOST PARALLEL TO THE ECLIPTIC, BUT NOT 00:32.466 --> 00:36.033 align:left position:10% line:83% size:80% QUITE THEY ACTUALLY CROSS. THAT POINT IS CALLED A NODE! 00:36.033 --> 00:39.366 align:left position:10% line:77% size:80% WHEN THE MOON CROSSES A NODE WE SEE AN ECLIPSE EITHER LUNAR ECLIPSE OR 00:39.366 --> 00:42.766 align:left position:10% line:77% size:80% SOLAR ECLIPSE DEPENDING. IT TAKES TWO WEEKS TO MOVE FROM NODE TO NODE. SO, 00:42.766 --> 00:46.066 align:left position:10% line:77% size:80% IF WE SEE AN ECLIPSE ON ONE, WE’LL LIKELY SEE ANOTHER IN TWO WEEKS! 00:46.066 --> 00:48.933 align:left position:20% line:83% size:70% THE NODES WOBBLE ALONG WITH THE EARTH’S ROTATION, 00:48.933 --> 00:59.733 align:left position:10% line:77% size:80% WHICH IS WHY SOMETIMES ECLIPSES ARE TOTAL, AND SOMETIMES NOT. KEEP LOOKIN’ UP!