A total lunar eclipse will turn the moon red next week; will it be visible in india

New Delhi: About a year after the last total lunar eclipse, the view of the Moon sliding into Earth’s shadow will return and grace the sky. Skygazers can see the moon turning red next week.

The Moon charts a course through the southern part of Earth’s shadow and is expected to last for sixty-five minutes.

Total Lunar Eclipse 2022: When and Where to Watch

Viewers in most of North America, throughout Latin America, Western Europe, most of Africa and the eastern Pacific will see the moon darken and acquire a reddish hue from the late evening of May 15 through the early hours of May 16.

The mid-eclipse will occur on May 16 at 4:12 Universal Time (approximately 9:42 AM IST), about 1 1/2 days before the Moon reaches perigee, the point in its orbit when it is closest to Earth.

On the night of the eclipse, the Moon will appear about 12 percent larger than the apogee (farthest from Earth in its orbit). However, in all likelihood, the most committed moon watchers will follow it.

The May 15-16 eclipse can be quite dark, but look for a slight flare along the Moon’s southern limb.

Viewers may be more likely to see the summer Milky Way shining brightly during totality as the extreme brightness of the full moon is dimmed by Earth’s shadow.

The phases of an eclipse occur simultaneously for everyone, but not everyone will see a total eclipse. Weather permitting, observers in the eastern half of North America will see the entire event beginning on the evening of May 15, with a partial eclipse phase beginning approximately two hours after sunset for the East Coast and approximately one hour after sunset for the Midwest . ,

On the west coast, the Moon will be about to enter its totality as it rises at sunset. And in the northwest, the moon rises because the later phases of the eclipse are already underway. However, most of Alaska will have to sit it out.

Starting on the evening of May 15, the entire show will be watched in South America, while viewers in Western Europe and Africa will have to set their alarms to enjoy the event before dawn on May 16.

For observers in the British Isles, the Moon is completely submerged in Earth’s dark, inner shadow, while viewers in New Zealand will catch the tail end of the event on the evening of 16 May, when the Moon rises as it exits Earth’s shadow. Used to be.

Lunar eclipses, in particular, occur when the Sun, Earth, and the full Moon form a near-perfect line in space, known as syzygy. The Moon falls into Earth’s shadow, gradually darkening, until the entire lunar disk changes from a silvery gray to a terrifyingly dim orange or red. The events then occur in reverse order, until the Moon returns to full brightness.

The entire process of the eclipse of May 16 will take about five hours and 20 minutes.

There are several stages of the event, each with different things to see.

  • The Moon’s leading edge enters the lighter outer fringe of Earth’s shadow: the penumbra. You probably won’t notice anything until the Moon is about halfway across the oblique. The penumbra is the region where an astronaut standing on the Moon would see Earth covering only a portion of the Sun’s face.
  • The leading edge of the Moon enters the umbra of the Earth’s shadow cone, within which the Sun is completely hidden. You should see a dramatic darkening at the leading edge of the lunar disk. With a telescope, you can see that the sides of the umbra gradually encircle one lunar feature after another, as the entire sky begins to darken.
  • The back edge of the Moon slips into the umbra to initiate a total eclipse. But the moon won’t be completely black: some shade of intense orange or red is sure to shine. Why is it like this? Earth’s atmosphere scatters (refractors) the sunlight that cuts off its edges, bringing some of it to the eclipsed Moon. This is the same effect that happens at sunset. If you were on the Moon during a lunar eclipse, you would see that the Sun is hidden by a dark Earth, surrounded by the red light of all the world’s sunrises and sunsets at that time. The thermal brightness of red can vary greatly from one eclipse to another. Two main factors affect its brightness and color. The first is how deep the Moon goes into the umbra as it passes; The center of the womb is darker than its edges. The second factor is the state of the Earth’s atmosphere. If a large volcanic eruption has recently polluted the stratosphere with a thin global haze, a lunar eclipse can be deep red, ash brown, or sometimes nearly black. In addition, blue light is refracted through Earth’s clear, ozone-rich upper atmosphere over thick layers that produce the red sunrise-sunset hue. This ozone-blue light also colors the Moon, particularly near the edge of the umbra. You will need binoculars or binoculars to see this effect.
  • As the Moon continues to move in its orbit, events recur in the reverse order. The edge of the Moon re-emerges in the sunlight, ending totality and starting a partial eclipse again.
  • When the full Moon leaves the umbra, only the final, partial shadow remains. After some time, nothing unusual remains.
  • As the Moon moves along its orbit, the events will occur in reverse order. The lunar limbs reappear in the Sun, ending with a total solar eclipse and starting again with a partial solar eclipse.
  • When the full moon leaves the umbrella, only the last shadow of the partial shadow remains. After a while, nothing unusual remains.

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