ScienceIQ.com

How Can A Bullet-proof Vest Stop A Bullet?

Here's an experiment: take the small coil springs from a dozen or so retractable pens and roll them together in a heap until they are thoroughly tangled and entwined. Now try to pull them apart from end to end. You should find them extremely difficult to pull apart this way, as anyone who has ever tried to untangle a 'Slinky' toy will know. ...

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Medicine

Acupuncture

Traditional Chinese medicine theorizes that there are more than 2,000 acupuncture points on the human body, and that these connect with 12 main and 8 secondary pathways called meridians. Chinese ... Continue reading

Acupuncture
Biology

What’s So Different About Ferns?

Most plants reproduce by producing a flower, then seeds. Anthers, considered the male reproductive structure, hold the pollen. The ovum, the female reproductive structure inside the flower, is ... Continue reading

Ferns
Chemistry

What Makes a Candle Burn?

Have you ever wondered how a candle works? If you haven't, think about it for a while. Why does it take so long for the wick to burn down? Why does it need a wick at all? ... Continue reading

CandleLight
Engineering

Sundials, Ancient Clocks

The earliest and simplest form of sundial is the shadow stick. The time of day is judged by the length and position of the stick's shadow. Some nomadic peoples still use this method for timekeeping. ... Continue reading

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The Antennae

TheAntennaeNASA's Chandra X-ray Observatory has discovered rich deposits of neon, magnesium, and silicon in a pair of colliding galaxies known as The Antennae. The deposits are located in vast clouds of hot gas. When the clouds cool, say scientists, a great number of stars and planets should form. These results may foreshadow the fate of our own Milky Way and its future collision with the Andromeda Galaxy. When galaxies collide, direct hits between stars are extremely rare, but collisions between huge gas clouds in the galaxies trigger a stellar baby boom. Massive newborn stars race through their evolution in a few million years and explode as supernovas. Heavy elements manufactured in these stars are blown away by the explosions and enrich the surrounding gas for thousands of light years.

The supernova rate in The Antennae is about 30 times that of the Milky Way. Supernova explosions heat the gas in these galaxies to millions of degrees Celsius--so hot that they emit X-rays. Such clouds are mostly invisible to optical telescopes, but they are easy targets for the Chandra X-ray Observatory. Chandra data reveal regions of high and varying enrichment. In one cloud, for instance, magnesium and silicon are 16 and 24 times as abundant as in the Sun. As the enriched gas cools, a new generation of stars will form, and with them new planets. A number of studies indicate that clouds enriched in heavy elements are more likely to form stars with planetary systems, so in the future an unusually high number of planets may form in The Antennae. At a distance of about 60 million light years, The Antennae system is the nearest example of a collision between two large galaxies.

The collision, which began a couple of hundred million years ago, has been so violent that gas and stars from the galaxies have been ejected into the two long arcs that give the system its name. The Antennae give a closeup view of the type of collisions that were common in the crowded early universe and likely led to the formation of many of the stars that exist in the universe today. They might also provide a glimpse of the future of our Milky Way galaxy, which is on a collision course with the Andromeda galaxy. At the present rate, a crash such as the one now occurring in the Antennae could happen in about 3 billion years. Tremendous gravitational forces will disrupt both galaxies and reform them, probably as a giant elliptical galaxy peppered with hundreds of millions of young Sun-like stars. And maybe hundreds of millions of habitable planets, too. These violent crashes aren't an end, after all. They're a new beginning.