Eclipse

From Conservapedia
1999 Solar eclipse

An eclipse is an astronomical event that occurs when an astronomical object is temporarily obscured, either by passing into the shadow of another body or by having another body pass between it and the viewer. An eclipse is the result of either an occultation (completely hidden) or a transit (partially hidden).

A solar eclipse is when the earth's moon passes between the sun and the earth to block the view of the sun on the earth. A lunar eclipse is when the moon passes through the shadow of the earth when the earth comes between the sun and the moon. A total eclipse completely blocks the view while a partial eclipse justs covers a portion of the viewed object.

Sun-moon configurations that produce a total (A), annular (B), and partial (C) solar eclipse

For any two objects in space, a series of lines can be drawn to explain what causes an eclipse and to predict how it will been seen at a third point in space. Typically the cross-section of the objects involved in an astronomical eclipse are roughly shaped like a circle. The region of an object's shadow during an eclipse is divided into three parts:

The umbra, within which the object completely covers the light source. For example, the moon's shadow where the sun's light is completely blocked is in the shape of a cone.
The antumbra, extending beyond the tip of the umbra, within which the object is completely in front of the light source but too small to completely cover it. Light travelling from the edges of the light source radiate beyond the shadow.
The penumbra, within which the object is only partially in front of the light source.

A total eclipse occurs when the observer is within the umbra, an annular eclipse when the observer is within the antumbra, and a partial eclipse when the observer is within the penumbra. (See diagram at left).


For spherical bodies, when the occulting object is smaller than the star, the length (L) of the umbra's cone-shaped shadow is given by:

where Rs is the radius of the star, Ro is the occulting object's radius, and r is the distance from the star to the occulting object.

Because the paths of the objects in the solar system are well understood, astronomers can predict with great accuracy when and where eclipses will be observed.

NASA jets chasing an eclipse

Because observing an occultation from a stationary position on earth may only last for a couple of minutes, scientists use jet airplanes to move instruments rapidly to compensate for the rotation of the earth. These measurements can lead to important discoveries. For example, astronomers used a jet to observe the occultation of the star SAO 158687 (also known as HD 128598) by Uranus to study its atmosphere, but unexpectly the data showed that Uranus had planetary rings.[1]

Biblical references to an eclipse[edit]

There are nine primary biblical references to an eclipse:[2]

References[edit]

  1. Elliot, J. L.; Dunham, E.; Mink, D. (1977). "The rings of Uranus". Cornell University 267: 328–330. doi:10.1038/267328a0. http://www.nature.com/nature/journal/v267/n5609/abs/267328a0.html. Retrieved June 9, 2007. 
  2. http://bible.knowing-jesus.com/topics/Eclipses

Categories: [Astronomy]


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