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The Kuiper Belt

The Kuiper (pronounced Ki-Per) Belt is often called our solar system's 'final frontier.' This disk-shaped region of icy debris is about 12 to 15 billion kilometers (2.8 billion to 9.3 billion miles) from our Sun. Its existence confirmed only a decade ago, the Kuiper Belt and its collection of icy objects - KBOs - are an emerging area of research in ...

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TheKuiperBelt
Biology

A Creature Only A Mother Could Love?

A creature only a mother could love isn't even much loved by its own mother. The Komodo dragon, weighing as much as 300 lbs. (136 kgs) or more, eats more than half its own weight in one meal. It ... Continue reading

MotherLove
Physics

Your Serve

NASA is well known for developing technology that makes things better, so can you believe that NASA actually did research on how to make tennis balls slower? ... Continue reading

YourServe
Chemistry

Catalysts

Chemical reactions are interactions between atoms and molecules that result in a change in their relative arrangements and interconnections. The reaction affects only individual atoms and molecules, ... Continue reading

Catalysts
Astronomy

Cosmos Provides Astronomers with Planet-Hunting Tool

If only astronomers had a giant magnifying glass in space, they might be able to uncover planets around other stars. Now they do -- sort of. Instead of magnifying a planet, astronomers used the ... Continue reading

PlanetHuntingTool

Does Anybody Really Know What Time It Is?

TimeAnybodySo, what, exactly, is the watch on your wrist, Big Ben in London, or the national atomic clock in Boulder, Colorado, actually measuring? The first definition of a second was 1/86,400 of the average solar day; in other words, a division of the average period of rotation of Earth on its axis relative to the Sun. This definition lasted until the mid-20th century, when the needs of international air and sea navigation and international communications required much more precise measurements of time. In 1956, the International Committee on Weights and Measures redefined the second to be 1/31,556,925.9747 of the length of the year 1900. This definition, known as the second of Ephemeris Time, was ratified by the General Conference on Weights and Measures in 1960. The definition was not to last very long, however, because of new developments in atomic physics.

In 1949, Harvard professor Norman Ramsey had developed a method of studying the structure of atoms by sending them through two oscillating electromagnetic fields. The procedure allowed a microwave oscillator to be synchronized with the unvarying atomic oscillations and could be used to measure the passage of time with great precision, thus providing the basis for the modern cesium atomic clock. In 1964, the International Committee on Weights and Measures acknowledged this new type of clock by provisionally defining the second based on the microwave frequency that drives the transition between two energy levels of a cesium-133 atom. In 1967, this definition became the sole definition of the second.