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Satellite Observations of the Eclipse
According to reports, geostationary satellites will report the eclipse because the moon’s penumbral shadow strikes throughout Earth. The Copernicus Sentinel-3, Himawari and GOES-16 satellites are anticipated to seize detailed photographs. The International Space Station might also report the development, as astronauts aboard have accomplished previously. The photographs taken will display the slow motion of the shadow, which can seem darker in areas the place the eclipse is maximum pronounced.
Movement of the Moon’s Shadow
As according to NASA’s Scientific Visualisation Studio, the moon’s shadow will commute from west to east because of the moon’s orbital movement. It strikes at a velocity of three,700 kilometres according to hour, which is quicker than Earth’s rotation. This reasons the shadow to look to transport in the other way of the solar’s obvious movement within the sky. The curvature of the Earth additionally impacts the shadow’s velocity and form because it strikes throughout other areas.
Viewing the Eclipse from Space
The satellites which might be situated at 36,000 kilometres above the Earth give you the absolute best view of the development. These satellites shall be shooting real-time photographs of the eclipse shadow because it strikes. Astronauts aboard the International Space Station might also seize photographs of the eclipse from orbit.
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