Source: Wikipedia

Types of Lunar Eclipses

An eclipse of the Moon (or lunar eclipse) can only occur at Full Moon, and only if the Moon passes through some portion of Earth’s shadow. That shadow is actually composed of two cone-shaped components, one nested inside the other. The outer or penumbral shadow is a zone where the Earth blocks part but not all of the Sun’s rays from reaching the Moon. In contrast, the inner or umbral shadow is a region where the Earth blocks all direct sunlight from reaching the Moon.

Astronomers recognize three basic types of lunar eclipses:

1. Penumbral Lunar Eclipse
+ The Moon passes through Earth’s penumbral shadow.
+ These events are of only academic interest because they are subtle and hard to observe.

2. Partial Lunar Eclipse
+ A portion of the Moon passes through Earth’s umbral shadow.
+ These events are easy to see, even with the unaided eye.

3. Total Lunar Eclipse
+ The entire Moon passes through Earth’s umbral shadow.
+ These events are quite striking due to the Moon’s vibrant red color during the total phase (totality).

When an eclipse of the Moon takes place, everyone on the night side of Earth can see it. About 35% of all eclipses are of the penumbral type which are very difficult to detect, even with a telescope. Another 30% are partial eclipses which are easy to see with the unaided eye. The final 35% or so are total eclipses, and these are quite extrordinary events to behold.

Why is the Moon Red During a Total Lunar Eclipse?

During a total lunar eclipse, the Earth blocks the Sun’s light from reaching the Moon. Astronauts on the Moon would then see the Earth completely eclipse the Sun. (They would see a bright red ring around the Earth as they watched all the sunrises and sunsets happening simultaneousely around the world!) While the Moon remains completely within Earth’s umbral shadow, indirect sunlight still manages to reach and illuminate it. However, this sunlight must first pass deep through the Earth’s atmosphere which filters out most of the blue colored light. The remaining light is a deep red or orange in color and is much dimmer than pure white sunlight. Earth’s atmosphere also bends or refracts some of this light so that a small fraction of it can reach and illuminate the Moon.

The total phase of a lunar eclipse is so interesting and beautiful precisely because of the filtering and refracting effect of Earth’s atmosphere. If the Earth had no atmosphere, then the Moon would be completely black during a total eclipse. Instead, the Moon can take on a range of colors from dark brown and red to bright orange and yellow. The exact appearance depends on how much dust and clouds are present in Earth’s atmosphere. Total eclipses tend to be very dark after major volcanic eruptions since these events dump large amounts of volcanic ash into Earth’s atmosphere. During the total lunar eclipse of December 1992, dust from Mount Pinatubo rendered the Moon nearly invisible.

Source: www.MrEclipse.com

All total eclipses start with a penumbral followed by a partial eclipse, and end with a partial followed by a penumbral eclipse (the total eclipse is sandwiched in the middle). The penumbral phases of the eclipse are quite difficult to see, even with a telescope. However, partial and total eclipses are easy to observe, even with the naked eye.

What Causes an Eclipse of the Moon?

According to the US National Aeronautics and Space Administration (NASA), there will be four lunar eclipses to behold this year. The Feb. 9 lunar eclipse was the first of four this year. The next penumbral lunar eclipses will be on July 7 and August 6. The first three will also be penumbral while the last on Dec. 31 will be a partial lunar eclipse where a part of the moon will pass the earth’s umbra, or the part where the Earth completely blocks the Sun.

Source: Inquirer.net

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How it works?

—Magnetic Fuel Saver through directional magnetic field is a “charged” or energy field. When liquids or gases flow through this charged field, the charged particles of the atoms that form the molecules are “excited” (become more active) and realign in the direction of the magnetic field. This increased molecular activity caused by the directional magnetic “energy” field will cause molecular clusters to break up, where clusters form, or cause individual molecules to more aggressively and more completely combine with other compounds or atoms as in the case of fuel molecules (hydrocarbons). This allows the fuel molecules to more readily and more completely combine with oxygen during combustion (burn) in the firing chamber or cylinder of a combustion engine.

—Magnetic Fuel Saver makes use of its unique Ultra Power technology shield and focus the optimum magnetic field strength onto the fuel line  that is desirable to cause the fuel molecules to break apart. More importantly, the hydocarbons are broken up so that HC + radicals are formed which would readily combined with air O2- to give an efficient combustion.

—Other devices may not create the “specifically directed magnetic field” necessary for proper interaction with fuel flowing in the gas line. In addition, magnetic strength loss from heat causes a dramatic loss in a magnets ability to effectively condition fuels. A “random” magnetic field, which other devices rely upon, particularly if weakened by the normal heat generated by an engine, may or may not reach the fuel, resulting in inconsistent performance at best.

Simply, Magnetic Fuel Saver technology to work effectively on combustion powered engines, the magnetic field must penetrate the fuel line at a sufficient strength to cause a significant degree of reaction to directly affect the fuel molecules. Random magnetic fields, by definition, are non-directional and therefore effectiveness is severely limited.

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