What is Antumbra?


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The lighter portion of a shadow that forms at a certain distance from the object casting the shadow is called the antumbra. Planetary transits and annular solar eclipses both involve it.
The Moon and Earth’s shadows cast them into space while obstructing sunlight from reaching them, similar to other opaque objects illuminated by a light source. Umbra, penumbra, and antumbra are the three distinct areas of each shade. -Antumbra Meaning

The lighter portion of a shadow that appears beyond the umbra at a specific distance from the object casting the shadow is called the antumbra. Only when the light source’s diameter exceeds that of the object does it occur. In an antumbra, the light source’s periphery can be seen surrounding the thing casting the shadow. For instance, during a solar eclipse, when the annular is in the antumbra, the Sun’s outer edge appears as a ring of fire around the Moon.
There are two more places besides Antumbra:
– Umbra: The shadow’s dark, central region.
– Penumbra : The lighter outer part of the shadow.
A solar eclipse happens when the Moon is in the Earth’s shadow; a lunar eclipse happens when the Moon is in the Earth’s shadow. The type of eclipse depends on the type of shadow. Causes of an annual solar eclipse

The umbra, or dark core, makes up the bulk of the moon’s shadow. The umbra’s diameter decreases with increasing distance from the moon, creating a V-shaped shadow core. A total solar eclipse would happen if the Umbra touched down on Earth.
As it moves away from the Moon, another V-shaped shadow follows the umbra. The antumbra is this. Antumbra’s diameter grows with distance from the Moon, in contrast to umbra. When viewed from one side, the point where the two shadows collide takes on the appearance of an hourglass. An annular solar eclipse will occur if Antumbra touches down on Earth. -Antumbra Rarely Drops to Earth

The Moon always casts a shadow when moving through space. It typically has an antumbra. The shadow, however, does not appear if it strikes a solid object outside of the umbra’s range because the antumbra begins at a specific distance from the Moon (beyond the umbra). This is the case during a solar eclipse when the umbra of the Moon falls to Earth. This indicates that an optical solar eclipse is taking place at this very moment, somewhere in space, on the dark side of the Moon.
Because the Moon’s antumbra rarely touches the Earth’s surface, annular solar eclipses are extremely uncommon. It only covers a small portion of the earth’s surface, even during an annular solar eclipse. During an antumbra eclipse, the moon and Earth both move toward the surface of the Earth. A circular phase is therefore typically only observed along a narrow ecliptic path. – What Causes Annular Solar Eclipses?

It displays the location of the intersection of the two V-shaped shadows, where the umbras change, and where the apparent magnitude of the Sun and Moon coincide. From this vantage point, the sun and moon both appear to be of equal width. As a result, the Moon completely obscures the Sun. The Moon grows larger as it gets closer to us and the umbra, completely obscuring the Sun. Its size decreases as it moves away from the Moon and its opposition to it, making the Sun’s outer edges visible. The term “ring of fire” refers to this circumstance.
The moon’s elliptical shadow causes its distance from Earth to fluctuate every day. The distance between the closest and furthest points on Earth is approximately 50,200 km. This range includes the location where the umbra and antumbra meet. This implies that when Earth is close to the Moon, the umbra of the Moon falls to Earth. A total solar eclipse is visible at this time. On the other hand, if the Moon’s antumbra and distance from us during the lunar eclipse, we can observe an annular solar eclipse. – How Vast Is the Antumbra of the Moon?

During a lunar eclipse, the Moon’s distance from Earth determines how much of the planet’s surface is covered by the Moon’s antumbra. The antumbra grows larger the further away it is.
The Moon will appear smaller in the sky and the “ring of fire” will appear thicker if the Moon is closest to Earth at the time of the eclipse. In this case, the path of the antumbra typically reaches more than 100 km wide at the Earth’s equator. The antumbra expands in size as latitude increases because the Sun’s rays hit the Earth’s surface at a shallower angle.
If the moon is closer to Earth at the time of the eclipse, only the very tip of the moon’s V-shaped antumbra can be seen on Earth during some of the eclipse, making its diameter almost zero. The solar eclipse’s annular phase doesn’t last very long. Due to the curvature of the Earth, a circular solar eclipse may start when it first touches the planet’s surface and progress to totality over time. A hybrid solar eclipse is the name for this unusual occurrence. – Why Isn’t There an Antumbral Eclipse?

When the Moon’s surface is in the Earth’s umbra, a total or partial lunar eclipse occurs. Because of the size of the Earth and its distance from the Moon, there will never be a lunar eclipse that includes Earth’s antumbra or one in which it touches the lunar surface.
Due to Earth’s larger diameter than the Moon, the umbral shadow extends farther before the antumbra begins to form. This indicates that even when the Moon is furthest away from the Earth, the distance between them is too small for the Earth to reach the Moon before it does. During an annular solar eclipse, the Moon is small enough to form before it passes over Earth.
Although Earth’s antumbra never falls on the Moon, it sometimes reaches other planets in our solar system. For instance, Mars receives the Earth’s antumbra when the Earth, Sun, and red planet are in perfect alignment. At that instant, Earth is visible from Mars as a tiny dot in front of the Sun.

The antumbra


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