A partial solar eclipse will occur on Saturday, March 19, 2072. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
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Transcription
[Intro] The sun is one of those things that you can always count on being there. Well … at least during the daytime. Usually, whenever we look up into the sky during the day, we can see the sun shining down on us, giving our planet heat and light. But sometimes you can also see the moon during the day. The moon moves around the Earth, making a full trip all the way around our planet, once every month. And during some of that month-long trip, you can see the moon only at night. But at other times, you can see it during the day. And every now and then, when you can see both the moon and the sun in the sky during the day, cool things can happen. And this week is one of those times. Because our planet is going to experience a solar eclipse! A solar eclipse happens when the moon gets right smack-dab between the sun and the Earth. When the moon does this, it blocks some of the sun’s light, and casts a gigantic shadow on the Earth. It doesn’t last for very long -- just a few minutes, really -- but when the moon blocks the light from the Sun, it can make the sky appear as dark as night -- even though it’s still day time! Now, not all eclipses are the same. They can look different, depending where on Earth you are, and where the moon’s shadow is. A total solar eclipse is when, from where you’re watching, the moon completely covers the sun in the sky. And there are also the partial solar eclipses, when the moon passes over just a little bit of the sun. When this kind of eclipse happens, the sun looks like a little chunk is missing -- like a cookie with a big bite taken out of it! Now, it’s not very often that sun, moon and the Earth line up in just the right way to create a solar eclipse. But the next one is going to happen on March 20! Not everyone in the world is going to be able to see it -- only people who happen to be in the path of the gigantic moon shadow. So where I live, in the United States, we won’t be able to see the solar eclipse. But people in Europe -- especially in the northern parts -- will get the best view. Those folks will get to see the total eclipse. Right around breakfast time, they’ll have a few minutes of darkness, almost as dark as night. People in the rest of Europe, and also parts of Asia and Africa, will see a partial solar eclipse. For them, it will look like a little bite has been taken out of the sun. And as the minutes pass, that bite will get smaller and smaller until the sun is back to its old self again. Now it’s important to remember, you should never try to look directly at an eclipse, because the rays from the sun can really damage your eyes, even when it’s partially covered up. So the next time you go outside during the day, see if you can find the moon. What does it look like? We’ll be keeping an eye out for it too here at SciShow Kids.
Related eclipses
Solar eclipses 2069–2072
This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[1]
120 | April 21, 2069 Partial |
125 | October 15, 2069 Partial |
130 | April 11, 2070 Total |
135 | October 4, 2070 Annular |
140 | March 31, 2071 Annular |
145 | September 23, 2071 Total |
150 | March 19, 2072 Partial |
155 | September 12, 2072 Total |
Saros 150
It is a part of Saros cycle 150, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on August 24, 1729. It contains annular eclipses from April 22, 2126 through June 22, 2829. There are no total eclipses in this series. The series ends at member 71 as a partial eclipse on September 29, 2991. The longest duration of annularity will be 9 minutes, 58 seconds on December 19, 2522.
Series members 11-21 occur between 1901 and 2100: | ||
---|---|---|
11 | 12 | 13 |
December 12, 1909 |
December 24, 1927 |
January 3, 1946 |
14 | 15 | 16 |
January 14, 1964 |
January 25, 1982 |
February 5, 2000 |
17 | 18 | 19 |
February 15, 2018 |
February 27, 2036 |
March 9, 2054 |
20 | 21 | |
March 19, 2072 |
March 31, 2090 |
Metonic series
The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.
21 eclipse events between June 1, 2011 and June 1, 2087 | ||||
---|---|---|---|---|
May 31 – June 1 | March 19–20 | January 5–6 | October 24–25 | August 12–13 |
118 | 120 | 122 | 124 | 126 |
June 1, 2011 |
March 20, 2015 |
January 6, 2019 |
October 25, 2022 |
August 12, 2026 |
128 | 130 | 132 | 134 | 136 |
June 1, 2030 |
March 20, 2034 |
January 5, 2038 |
October 25, 2041 |
August 12, 2045 |
138 | 140 | 142 | 144 | 146 |
May 31, 2049 |
March 20, 2053 |
January 5, 2057 |
October 24, 2060 |
August 12, 2064 |
148 | 150 | 152 | 154 | 156 |
May 31, 2068 |
March 19, 2072 |
January 6, 2076 |
October 24, 2079 |
August 13, 2083 |
158 | 160 | 162 | 164 | 166 |
June 1, 2087 |
October 24, 2098 |
References
- ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC