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Magnitude of an Astronomical Object

'Visual magnitude' is a scale used by astronomers to measure the brightness of a star. The term 'visual' means the brightness is being measured in the visible part of the spectrum, the part you can see with your eye (usually around 5500 angstroms). The first known catalogue of stars was made by the Greek Astronomer Hipparchus in about 120 B.C. and ...

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MagnitudeofanAstronomicalObject
Astronomy

The Strange Spin of Uranus

Directional terms like north and south make sense here on Earth. The north and south axis of the Earth is relatively perpendicular to the plane of the Earth's orbit around the sun. Actually, Earth's ... Continue reading

UranusSpin
Mathematics

Kepler's Conjecture

Take a bunch of oranges that are similar in size and try to pack them into a cardboard box. What is the most efficient orange arrangement so that you fit the most oranges into the box? Should you ... Continue reading

KeplersConjecture
Physics

Why Does A Golf Ball Have Dimples?

A golf ball can be driven great distances down the fairway. How is this possible? The answer to this question can be found by looking at the aerodynamic drag on a sphere without dimples (while it's ... Continue reading

GolfBallDimples
Chemistry

Fire Retardant Gels

Ultra-absorbent diapers, the kind that will hold massive amounts of liquids, have been used for years, without a second thought given to the materials within them. Let's face it; those materials ... Continue reading

FireRetardantGels

A New Twist on Fiber Optics

ANewTwistonFiberOpticsBy twisting fiber optic strands into helical shapes, researchers have created unique structures that can precisely filter, polarize or scatter light. Compatible with standard fiber optic lines, these hair-like structures may replace bulky components in sensors, gyroscopes and other devices. While researchers are still probing the unusual properties of the new fibers, tests show the strands impart a chiral, or 'handed,' character to light by polarizing photons according to certain physical properties. Several of these fibers, and their applications, are being developed in part with funds from the National Science Foundation Small Business Innovation Research program. In conventional optical fibers, light is transmitted from one end to the other through a round core housed within a concentric outer cladding. But, because a circular core does not develop handedness when twisted, the research team wound rectangular-core fibers to create a double helix.

When the team tested the twisted fiber, they discovered that some photons left the core and entered the cladding. Photons with the same handedness as the fiber entered the cladding whereas photons with handedness opposite that of the fiber remained in the core. With only a relatively loose twist-roughly 100 microns to form a complete turn-photons with a handedness that coincides with the fiber's twist scatter out of the core at a shallow angle and are trapped in the cladding. With a tighter twist, photons with the same handedness as the fiber scatter at a wider angle, allowing the photons to escape from the cladding into the surrounding space. Only light of a single polarization remains in the fiber. At the tightest twists, roughly one-millionth of a meter to complete a turn, photons with the same handedness as the structure are reflected backwards in the core.

Because the environment surrounding the fiber affects the wavelength of the light embedded in the cladding, 'loosely' twisted fibers can serve as sensors for pressure, temperature, torque and chemical composition. With moderately twisted fibers, researchers can manipulate the resulting polarized light in useful ways, leading to a range of applications such as gyroscopes for navigation systems, current meters for electric power stations, and chemical and materials analysis equipment. For tightly wound fibers, the amount of twist determines the precise wavelength of the light remaining in the fiber, producing light that is ideal for filter and laser applications.