Note: Your web browser must have Javascript turned on in order to see a solar eclipse path plotted on Google Maps. As a consequence, eclipse paths at high latitudes will appear highly distorted and may degrade into a series of straight line segments. Google Maps uses the Web Mercator projection, and therefore cannot accurately show areas around the poles. Good weather is the key to successful eclipse viewing - better to see a shorter eclipse from clear sky that a longer eclipse under clouds. It's much more important to watch the weather forecasts a day or two before the eclipse and choose a location with the best chance of a cloud-free sky during the eclipse. You can be hundreds of miles from the theoretical point of Greatest Duration and still enjoy totality lasting within a second of the maximum possible (as long as you stay within several miles of the central line). For the sake of speed and simplicity, the effects of the lunar limb profile are NOT used in the predictions and map presented on this page. This prediction does not take into account the mountains and valleys along the edge of the Moon. In this case, the Greatest Duration is 04m28.2s. This is the location where the total eclipse lasts the longest along the entire path. The green marker labeled GD is the point of Greatest Duration. The red marker labeled GE is the point of Greatest Eclipse. The yellow lines crossing the path indicate the position of maximum eclipse at 10-minute intervals. The eclipse is longest on the central line (red). You MUST be somewhere within the central path (shaded zone framed by the blue lines) to see the total phase of the eclipse. The northern and southern path limits are blue and the central line is red. This is the geographic region from which the total eclipse can be seen. The narrow track running through rhe penumbral shadow is the path of the Moon's umbral shadow. Outside this region no eclipse is visible. You MUST be somewhere within the region enclosed by these curves in order to see the partial eclipse. The Key to Google Eclipse Maps illustrates a map with each of these curves. An orange curve also appears inside this region and represents the locus of all locations where the partial eclipse is at its maximum phase at sunrise or sunset. Inside these regions the partial eclipse is in progress at sunrise or sunset. The magenta loops represent the locus of all locations where the partial eclipse begins or ends at sunrise or sunset. The northern and/or southern penumbral shadow path limits are plotted as green curves. This is the geographic region from which a partial eclipse can be seen. The large saddle-shapped region is the path of the Moon's penumbral shadow. The interactive Google map below uses the Web Mercator projection to display the eclipse track. The small global map to the right is for reference and illustrates the overall visibility of the eclipse (for an explanation of this map's features, see Key to Solar Eclipse Maps). Clicking the cursor on any location will immediately generate a prediction of the eclipse circumstances from that location. The Google map allows the user to zoom and scroll the map as desired. This page features an interactive Google map showing the regional visibility of the Total Solar Eclipse of 2024 Apr 08.
0 Comments
Leave a Reply. |
AuthorWrite something about yourself. No need to be fancy, just an overview. ArchivesCategories |