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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: 7:45  
clear_day Transit: 11:48  
SunsetSet: 15:51 south
sunny DaytimeWhat's Visible Now?
Solar Eclipses » 

Solar Eclipse of April 20 2023 from Panguipulli, Chile

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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 Hybrid Solar Eclipse of April 20 2023 will be visible from there.

Eclipse Map from Panguipulli, Chile
Eclipse KML paths provided by Xavier M. Jubier (http://xjubier.free.fr/)
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Eclipse Visibility from Panguipulli, Chile
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Finder chart of
This diagram shows how the Hybrid Solar Eclipse of April 20 2023 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 Panguipulli, Chile
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Start of Hybrid Eclipse from Panguipulli, Chile
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Maximum Eclipse from Panguipulli, Chile
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End of Hybrid Eclipse from Panguipulli, Chile
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End of Partial Eclipse from Panguipulli, Chile
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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 Hybrid Solar Eclipse of April 20 2023

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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