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Magnitude of eclipse an annular solar eclipse has a magnitude of less than 1.0 the magnitude of eclipse is the fraction of the angular diameter of a celestial body being eclipsed This app demonstrates the relationship between eclipse magnitude (a value between 0 and 1) and percentage obscuration for solar eclipses. [1] this applies to all celestial eclipses.

Fraction of the sun's diameter the magnitude of a solar eclipse is the fraction of the sun's diameter covered by the moon The magnitude of a partial or annular solar eclipse is always between 0.0 and 1.0, while the magnitude of a total solar eclipse is always greater than or equal to 1.0, and has a theoretically maximum value of around 1.12. The magnitude of a lunar eclipse is the fraction of the moon's diameter covered by earth’s shadow

The penumbral magnitude and the umbral.

Magnitude of eclipse explained the magnitude of eclipse is the fraction of the angular diameter of a celestial body being eclipse d The core question i think is A total eclipse, especially lunar total eclipse, while the earth's umbra is much larger than the moon Then the magnitude will be larger if the center of the moon and the center of the earth's umbra are closer together see bottom figure (comparing if the moon is close to the edge of the umbra see top figure) if using definition ii

In definition i, the magnitude. A measure of the extent of an eclipse In a solar eclipse, the magnitude is the fraction of the sun's diameter that is covered by the moon If the eclipse is total, magnitude is replaced by the ratio of the apparent diameters of the moon and sun, which is always 1.00 or more during totality

The magnitude of a lunar eclipse is the fraction of the moon's diameter covered by the earth's umbra.

Footnotes [1] the instant of greatest eclipse occurs when the distance between the moon's shadow axis and earth's geocenter reaches a minimum [3] eclipse magnitude is defined as the fraction of the sun's diameter occulted by the moon The magnitude of eclipse or geometric magnitude is the fraction of the diameter of the eclipsed body which is in eclipse This applies to both solar eclipses and lunar eclipses.

The apparent sizes of the moon and the sun are both about 0.5°, or 30', but both vary because the distance between the earth and the moon varies (the distance between the earth and the sun also varies, but the effect is slight in comparison.) for an annular solar eclipse, the magnitude of the eclipse is the ratio of the apparent angular diameters of the moon to that of the sun during the. The magnitude of eclipse is the fraction of the angular diameter of a celestial body being eclipsed [1] this applies to all celestial eclipses

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