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The Richter Magnitude Scale

Seismic waves are the vibrations from earthquakes that travel through the Earth; they are recorded on instruments called seismographs. Seismographs record a zig-zag trace that shows the varying amplitude of ground oscillations beneath the instrument. Sensitive seismographs, which greatly magnify these ground motions, can detect strong earthquakes ...

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RichterScale
Astronomy

Rossi X-ray Timing Explorer Solves Mystery of Pulsar 'Speed Limit'

Gravitational radiation, ripples in the fabric of space predicted by Albert Einstein, may serve as a cosmic traffic enforcer, protecting reckless pulsars from spinning too fast and blowing apart, ... Continue reading

RossiXrayTimingExplorer
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
Engineering

Non-Flammable Fuel?

When we're flying high above the Earth, few of us give much thought to aircraft safety. We're usually too busy wondering when lunch is going to be served. But flying safely is a goal of NASA's Glenn ... Continue reading

NonFlammableFuel
Physics

The Doppler Effect

As any object moves through the air, the air near the object is disturbed. The disturbances are transmitted through the air at a distinct speed called the speed of sound, because sound itself is just ... Continue reading

TheDopplerEffect

Big Fish

BigFishThe phrase 'big fish eat little fish' may hold true when it comes to planets and stars. Perhaps as many as 100 million of the sun-like stars in our galaxy harbor close-orbiting gas giant planets like Jupiter, or stillborn stars known as brown dwarfs, which are doomed to be gobbled up by their parent stars. Space Telescope Science Institute astronomer Mario Livio and postdoctoral fellow Lionel Siess did not directly observe the planets, because they had already been swallowed by their parent stars. But Livio did find significant telltale evidence that some giant stars once possessed giant planets that were then swallowed up. The devouring stars release excessive amounts of infrared light, spin rapidly, and are polluted with the element lithium.

About 4 to 8 percent of the stars in our galaxy display these characteristics, according to Livio and Siess. This is consistent with estimates of close orbiting giant planets, based on discoveries of extrasolar planets by radial velocity observations, which measure the amount of wobble in a star due to the gravitational tug of an unseen companion. An aging solar-type star will expand to a red giant and in the process engulf any close-orbiting planets. If the planets are the mass of Jupiter, or greater, they will have a profound effect on the red giant's evolution. First, according to Livio's calculations, such a star is bigger and brighter because it absorbs gravitational energy from the orbiting companion. This heats the star so that it puffs off expanding shells of dust, which radiate excessive amounts of infrared light.

The orbiting planet also transfers angular momentum to the star, causing it to 'spin up' to a much faster rate than it would normally have. Giant planets carry the lion's share of angular momentum in a stellar system. For example, Jupiter and Saturn contain 98 percent of the angular momentum in the solar system. Finally, a chemical tracer is the element lithium, which is normally destroyed inside stars. A newly devoured Jovian planet would provide a fresh supply of lithium to the star, and this shows up as an anomalous excess in the star's spectrum. In our solar system Jupiter is too far from the Sun to be swallowed up when the Sun expands to a red giant in about 5 billion years. However, detections of extrasolar planets do show that Jupiter-sized planets can orbit unexpectedly close to their parent stars. Some are even closer than Earth is to our Sun. These worlds are doomed to be eventually swallowed and incinerated.