The lunar eclipse on May 5 will begin at what time?
- It is now the moon’s turn to experience an eclipse, approximately two weeks after its shadowy figure crossed in front of the sun for portions of the Pacific Ocean, New Guinea, and the Indian Ocean.

On May 5, the moon almost completely disappears beneath the Earth’s shadow, testing only the penumbra, the shadow’s outermost region. The penumbra is not only light in color, but it also gets lighter as it moves farther from the umbra, the shadow’s dark essential region. Consequently, this occurrence is known as a penumbral lunar eclipse.
The lunar eclipse on May 5
Friday, May 5, will see the start of the penumbral lunar eclipse at 11:13 a.m. EDT (15:13 GMT) and its peak at 1:24 p.m. EDT (17:24 GMT). The moon will emerge from the Earth’s shadow at 3:31 p.m. EDT (1932 GMT), ending the eclipse.
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Moon’s disk’s circumference is completely submerged
No portion of the moon crosses into the Earth’s deep umbral shadow during a penumbral eclipse. Leaving no visible trace of the Earth’s shadow. This weak eclipse won’t impact the moon’s brightness much. Because it will pass through the outermost reaches of the Earth’s shadow. Unless at least two-thirds of the moon’s disk’s circumference is completely submerg. The penumbral shadow is typically faint and challenging to see. Even though the area of the moon closest to the much darker umbral shadow may darken rationally. It might not draw attention.
The Earth would appear to somewhat eclipse the sun to an astronaut standing on the moon.
The Eastern Hemisphere benefits from this eclipse, especially a portion of eastern Africa. And neighboring Madagascar as well as most of western Asia. The moon will be beneath the horizon during daylight hours. When this event takes place so that the Americas won’t see any of it. The moon’s path will be to the northward of the deep umbral shadow.

The moon will begin to enter the penumbral shadow at the time indicated in the schedule below. Which has been adjust to reflect Greenwich Mean Time (GMT). But nothing uncommon will be visible on the lunar disk at that time.
The eclipse scale, or the portion of the moon’s length that is in the lighter penumbral shadow, will be 96.4 percent at the time of the eclipse’s darkest phase.
78 miles (126 km) will separate the moon’s foremost
Only about 78 miles (126 km) will separate the moon’s foremost edge from the Earth’s umbra. As it passes through the southern portion of the penumbra. Therefore, those who are aware of looking may be able to see a vague grayish or brownish smudge or stain focused toward the moon’s upper rim for about 45 minutes. Or so, around the time of the middle of the eclipse.
Eastern Asia, Indonesia, Australia, and southern New Zealand will also be able to see the eclipse. Still, because it happens after local the early hours there, Saturday (May 6) will appear on the calendar. The moon will set in New Zealand and parts of Japan after being completely engulfed by the penumbral shadow. The eclipse won’t be visible to the rest of the world. Because this event will take place during the day and with the moon below the horizon.
If that applies to you, try not to worry too much. After all, the incident pales in comparison with other spectacular celestial displays like the recent rare hybrid solar eclipse that occurred on April 20.