Large, Persistent Eclipse/Shadow On Earth?

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In summary, the conversation discusses the potential effects of a large and persistent shadow being cast on the Earth, similar to the umbra during a total solar eclipse. It is noted that the night side of the Earth is already in a permanent shadow, but if a separate shadow were to be cast, it would reduce the amount of solar radiation hitting the Earth and potentially cool the planet. The conversation also considers the impact on weather patterns and shares a personal experience of a solar eclipse causing a significant temperature drop.
  • #1
alphareign
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This may sound like a dumb question, but I have been curious about this for a while. What would happen if something cast a large and persistent shadow on the same part of earth? Say the shadow was the size of the umbra during a total solar eclipse. What would that do to the earth? I know the moon cannot do that, but if something could, then what?
 
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  • #2
Well the night side of Earth is in a permanent shadow by definition, although of course the rotation of Earth means that the shadow is not always at the same place wrt Earth's surface.
If the Earth did not rotate the darkened side would always be cooler, quite possibly frozen in parts, although I expect that this would be mitigated to some extent by atmospheric and ocean circulations.
 
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  • #3
Any "permanent" shadow of that type would reduce the amount of solar radiation striking the Earth, cooling it slightly. The Moon's shadow during an eclipse is never more than ~267 km across, and would block less than 1/5 of a percent of the Solar radiation hitting the Earth, so I wouldn't expect too much in the way of cooling. What effect such a permanent shadow spot would have on weather patterns is hard to say.
 
  • #4
Also, where the shadow is cast is also important. Normally, during a solar eclipse the area eclipsed will see some drop in temperature. If the solar eclipse happens in say Canada in February and during an unusually warm day ie 40 degrees F, the temperature will drop to below Zero, and do so as the eclipse starts to cover the sun ie you will experience a 40-50 degree drop in temperature in about an hour. This is not speculation, but an actual personal experience (year 1979).
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On a side note; because it was so warm prior to the eclipse, there was some humidity vs if it were colder, there would have been a lot less moisture in the air. This caused all the expensive cameras to freeze up. Only one or two prepackage cheap cameras actually worked (the kind that were disposable and dropped off to be processed, another item of the past).
 

1. What causes a large, persistent eclipse or shadow on Earth?

A large, persistent eclipse or shadow on Earth is caused by an object blocking the light from the Sun. This can be caused by a planet, moon, or other celestial body passing between the Sun and Earth, or by the Earth casting a shadow on itself during a solar eclipse.

2. How long can a large, persistent eclipse or shadow last on Earth?

The duration of a large, persistent eclipse or shadow on Earth depends on various factors, such as the size of the object causing the eclipse or shadow, its distance from Earth, and the speed at which it is moving. Generally, a total solar eclipse can last for a few minutes, while a lunar eclipse can last for a few hours.

3. Are large, persistent eclipses or shadows dangerous for life on Earth?

No, large, persistent eclipses or shadows are not dangerous for life on Earth. In fact, they can be quite fascinating and provide a unique opportunity for scientists to study the effects of these events on the Earth's atmosphere and environment.

4. How often do large, persistent eclipses or shadows occur on Earth?

Large, persistent eclipses or shadows on Earth occur regularly, depending on the orbit of the object causing the eclipse or shadow. For example, a solar eclipse can occur once every 18 months, while a lunar eclipse can occur multiple times in a year.

5. Can we predict when a large, persistent eclipse or shadow will occur on Earth?

Yes, scientists are able to predict when a large, persistent eclipse or shadow will occur on Earth with a high degree of accuracy. This is possible due to the precise measurements and calculations of the orbits of the objects involved in causing the eclipse or shadow.

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