ScienceIQ.com

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? ...

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CandleLight
Biology

Tobacco Mosaic Virus

We all know that AIDS, SARS and flu are all caused by viruses. Most people, however, don't realize that some of the earliest work on viruses was done on a common plant virus, Tobacco mosaic virus ... Continue reading

TobaccoMosaicVirus
Astronomy

Near-Earth Supernovas

Supernovas near Earth are rare today, but during the Pliocene era of Australopithecus supernovas happened more often. Their source was an interstellar cloud called 'Sco-Cen' that was slowly gliding by ... Continue reading

Supernovas
Medicine

My Aching Back

The back is an intricate structure of bones, muscles, and other tissues that form the posterior part of the body’s trunk, from the neck to the pelvis. The centerpiece is the spinal column, which not ... Continue reading

MyAchingBack
Astronomy

Neptune: The Basics

The eighth planet from the Sun, Neptune was the first planet located through mathematical predictions rather than through regular observations of the sky. When Uranus didn't travel exactly as ... Continue reading

NeptuneTheBasics

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.