1 Lunar and Solar and Eclipses

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Presentation transcript:

1 Lunar and Solar and Eclipses

2 Eclipses The Sun and Moon occasionally line up so that we have an eclipse. –These eclipses happen every year –To see a solar eclipse, you need to be on a particular part of the Earth

3 When the Earth’s shadow covers the Moon, we have a lunar eclipse

4 Three types of Lunar Eclipses Penumbral lunar eclipse—the Moon only passes through the penumbra of Earth’s shadow Partial lunar eclipse—part of the Moon passes through the umbra of Earth’s shadow Total lunar eclipse—the entire Moon passes through the umbra of Earth’s shadow Who on Earth will be able to see a lunar eclipse? Anyone who can see the Moon (anyone who is on the nighttime side of the Earth during the eclipse)

5 Images from Fred Espenak

6 Why is the Moon red during an eclipse? The Earth’s atmosphere filters some sunlight and allows it to reach the Moon’s surface The blue light is removed—scattered down to make a blue sky over those in daytime Remaining light is red or orange Some of this remaining light is bent or refracted so that a small fraction of it reaches the Moon Exact appearance depends on dust and clouds in the Earth’s atmosphere

7 Solar Eclipses When the Moon’s shadow covers part of the Earth Only happens at New Moon Three types: Annular, Partial, and Total

8 Total Solar Eclipse Observers in the “umbra” shadow see a total eclipse (safe to view the Sun); can see the corona Those in “penumbra” see a partial eclipse—not safe to look directly at Sun Only lasts a few minutes Path of Totality about 10,000 miles long, only 100 miles wide

9 Photo of a Total Eclipse

10 Annular Solar Eclipse When the Moon is too far to completely cover the Sun—the umbra doesn’t reach the Earth Sun appears as a donut around the Moon

11 Photos of an Annular Eclipse photos taken by Fred Espenak

12 Upcoming Solar Eclipses Next Total Solar Eclipse in continental USA—August 21, 2017