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A Complete Guide to the Solar System and the Night Sky
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public Observing fromLocation: Greenwich, United Kingdom edit_location_alt
north SunriseRise: 7:52  
clear_day Transit: 11:51  
SunsetSet: 15:49 south
sunny DaytimeWhat's Visible Now?
Solar Eclipses » 

Solar Eclipse of December 24 1916 from Lugazi, Uganda

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You can search for any other location by typing into the search field below, or by clicking on any point on the map below to find out when and how the Partial Solar Eclipse of December 24 1916 will be visible from there.

Eclipse Map from Lugazi, Uganda
Eclipse KML paths provided by Xavier M. Jubier (http://xjubier.free.fr/)
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Eclipse Visibility from Lugazi, Uganda
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Finder chart of
This diagram shows how the Partial Solar Eclipse of December 24 1916 will look like at the instant of maximum eclipse from Loading... (Loading...).
Move the blue pin on the map above to change the location.
Please keep in mind that in this sky chart the North direction points upwards. The Online Planetarium provides a realistic interactive visualization which properly takes into account the rotation of the sky caused by the local observing point on Earth.
Start of Partial Eclipse from Lugazi, Uganda
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Start of Partial Eclipse from Lugazi, Uganda
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Maximum Eclipse from Lugazi, Uganda
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End of Partial Eclipse from Lugazi, Uganda
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End of Partial Eclipse from Lugazi, Uganda
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Thee eclipse KML paths used for the maps visualization on this site are provided by Xavier M. Jubier (http://xjubier.free.fr/)

Sky Chart of Partial Solar Eclipse of December 24 1916

The sky chart below shows the location in the sky of the Moon, the Sun and the planets at the time of maximum eclipse. The portion of the sky represented in this sky chart is 50°x25°

In case of a total solar eclipse this chart can be useful to determine which planets are visible during the totality phase. Please keep in mind that in this sky chart the North direction (increasing Declination) points upwards. The Online Planetarium provides a realistic interactive visualization which properly takes into account the rotation of the sky caused by the local observing point on Earth.

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