Check out a Solar eclipse, safely

19/06/2020

 

 

This weekend, stargazers in the Eastern Hemisphere will be treated to an annular solar eclipse on the heels of the summer solstice. This type of eclipse is characterized by its stunning “ring of fire” since it’s not a total eclipse and edges of the sun can still be seen around the moon. ( source CNN )

Where to see it

The annular eclipse will begin at 12:47 a.m. ET (4:47 UTC) on June 21 and cross a skinny path that starts at sunrise in Africa and eventually moves across to China before ending at sunset over the Pacific Ocean. It will peak at 2:40 a.m. ET (6:40 UTC) and end around 4:32 a.m. ET (8:32 UTC). The partial eclipse will begin at 11:45 p.m. ET (3:45 UTC) on June 20 and end at 5:34 a.m. ET (9:34 UTC) on June 21 Check TimeandDate.com for more specific timing in your area. Stunning photos of the solar eclipse over South AmericaIt will be visible over central Africa, the southern Arabian Peninsula, Pakistan, North

 

Types of Solar Eclipses

There are 4 different types of solar eclipses. How much of the Sun’s disk is eclipsed, the eclipse magnitude, depends on which part of the Moon’s shadow falls on Earth.

  1. Partial solar eclipses occur when the Moon only partially obscures the Sun’s disk and casts only its penumbra on Earth.
  2. Annular solar eclipses take place when the Moon’s disk is not big enough to cover the entire disk of the Sun, and the Sun’s outer edges remain visible to form a ring of fire in the sky. An annular eclipse of the Sun takes place when the Moon is near apogee, and the Moon’s antumbra falls on Earth.
  3. Total solar eclipses happen when the Moon completely covers the Sun, and it can only take place when the Moon is near perigee, the point of the Moon’s orbit closest to Earth. You can only see a total solar eclipse if you’re in the path where the Moon casts its darkest shadow, the umbra.
  4. Hybrid Solar Eclipses, also known as annular-total eclipses, are the rarest type. They occur when the same eclipse changes from an annular to a total solar eclipse, and/or vice versa, along the eclipse’s path.

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