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➡ Click here: Eclipse solar 2017 21 agosto
There was a watch party on campus for the students of the , and the MU Health Care system released eye safety information. A watch party was also hosted on campus the day of the eclipse. Retrieved July 13, 2017.
Venezuela Na Venezuela, será possível apreciar 52,9% de encobrimento na cidade de Nagasaki, onde o eclipse começará às 14h28 15h28 em Brasíliaalcançará o pico às 15h45 e terminará às 16h52. É uma visão fantástica. Durante la siguiente hora y media, atravesará Oregon, Idaho, Wyoming, Montana, Nebraska, Iowa, Kansas, Misuri, Illinois, Kentucky, Tennessee, Georgia y Carolina del Norte y Carolina del Sur. Roque de los Muchachos Dakota 19:51:20 20:36 20:36 41. Si lo hacemos dentro de la penumbra, será parcial. Retrieved August 21, 2017. Motorists reported to local news outlets that it was taking them two hours to travel the 47 miles 76 km from that city to to the south, a met that normally takes 45 minutes. Eclipse solar 2017 21 agosto el 17 de agosto de 2017. An eclipse of comparable length up to 3 minutes, 8 seconds, with the longest eclipse being 6 minutes and 54 seconds occurred over the contiguous United States on along the southern portions of thefrom Hiroshima to Virginia. Veja qual é a maneira correta de se proteger: E pra quem já ficou triste porque não poderá presenciar o evento, fique tranquilo, pois teremos aqui em nosso site uma transmissão ao vivo do Grande Eclipse Solar Americano no dia 21 de agosto.
Symptoms usually occur within twenty-four hours and include eye pain and light sensitivity. No Peru, por exemplo, será de apenas 5% na cidade de Iquitos, enquanto no Equador alcançará 9% na cidade de Nueva Loja, no leste do país. El mapa muestra la zona de visibilidad del eclipse en España.
Eclipse Solar 2017 - Depending on the severity of damage, vision problems can last for several months or be permanent.
The northern and southern path limits are blue and the central line is red. You MUST be somewhere within the central path between the blue lines to see the total phase of the eclipse. The eclipse is longest on the central line red. The yellow lines crossing the path indicate the time and position of maximum eclipse at 10-minute intervals. The green marker labeled GE is the point of. The magenta marker labeled GD is the point of. This is the location where the total eclipse lasts the longest along the entire path. The magenta band on either side of the Greatest Duration marker shows a region where totality lasts within 0. In the case of the 2017 eclipse, the Greatest Duration is 2 minutes 40. This prediction does not take into account the mountains and valleys along the edge of the Moon. Detailed predictions using the show a corrected value of 2 minutes 41. 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. Note that the central line of the eclipse plotted in red is banded by different colors for hundreds of miles east and west of the marker. 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. Even in Oregon, the total eclipse still lasts 2 minutes. Good weather is the key to successful eclipse viewing - better to see a shorter eclipse from clear sky that a longer eclipse under clouds. Important Note: The eclipse predictions in this interactive map DO NOT include the effects of mountains and valleys along the edge of the Moon. Such corrections for the may change the contact times and eclipse durations by ~1-3 seconds. The exact location of may also change by ~10-20 kilometers. User Directions The zoom bar left edge of map is used to change the magnification. The four-way toggle arrows upper left corner are for navigating around the map. You can also move the map center around to reposition it by holding down the left mouse button and dragging. The two map buttons top right let you switch between map view and satellite view. Click anywhere on the map to add a red marker. A popup window appears above the marker with the calculated eclipse times and duration of annularity for that location see explanation of Eclipse Circumstances below. The 'x' in the upper right corner of the popup window closes the popup window. Additional markers can be placed anywhere on the map. Move the cursor over a marker to reveal a popup window with the eclipse times for that position. The predictions in the popup window can also be displayed in a new web page via the Eclipse Times Popup button bottom right. You can select and copy this infomation to paste into a word processor. All the markers can be removed by using the Clear Marker button below the map. Choose the Large Map check box to produce a bigger map hint: enlarge the browser window to its maximum size before selecting the Large Map check box. This option is especially useful to users with large monitors. Below the lower left corner of the map are three readouts. The third line gives the distance of the cursor from the last marker. For more information, see. Eclipse Circumstances When you click on the map a red marker is added and a popup window opens giving the Eclipse Circumstances calculated for that location. The predictions in the popup window can be divided into two sections. In the top part of the window, the decimal Latitude and Longitude of the marker are given. The Eclipse Type either , or seen from that position is given. The Duration of or Duration of lists the length of the total or annular phase in minutes and seconds. The is the fraction of the Sun's diameter eclipsed. The is the fraction of the Sun's area eclipsed. The bottom part of the window consists of a table listing the times for important stages of the eclipse. The Event column lists eclipse phase, followed by the date and time both in. Finally, the Altitude and Azimuth of the Sun is given for each event. The altitude is measured from the horizon 0° to the zenith 90°. An excellent source for weather prospects for upcoming eclipses is meteorologist Jay Anderson's. This web page approximates the curved eclipse path by using a series or straight line segments. This should prevent over-interpretation of the eclipse path accuracy. You can disable the zoom limit using the link to reload the map. The eclipse predictions presented here DO NOT include the effects of mountains and valleys along the edge of the Moon. Such corrections for the may shift the limits of the eclipse path north or south by ~1-3 kilometers, and change the eclipse duration by ~1-3 seconds. Acknowledgments All eclipse calculations are by Fred Espenak, and he assumes full responsibility for their accuracy. Candey Email: Heliospheric Physics Laboratory — Code 672 NASA's Goddard Space Flight Center, Greenbelt, Maryland 20771, USA.