ScienceIQ.com

Nothing Backwards About It

Almost anyone who's seen a picture of the experimental X-29 aircraft will remember it. Its unique wings make it one of the most distinctive aircraft designs ever. Rather than sticking straight out or angling back towards the aft of the plane, the wings on the X-29 almost look like they were put on backwards. They start near the tail of the plane, ...

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NothingBackwardsAboutIt
Medicine

How Much Coffee Will Kill You?

With the spread of Starbucks franchises all the way from Portland to Poughkeepsie, Americans are getting used to paying $3 or more for a proverbial ten-cent beverage. Of course, you get a bigger cup, ... Continue reading

HowMuchCoffeeWillYou
Engineering

Pass the Basalt

Advanced composite materials technology is a field that is growing both quickly and steadily. That new fiber materials and applications will be developed is the proverbial 'no brainer'. However, ... Continue reading

PasstheBasalt
Astronomy

Jupiter's Great Red Spot - A Super Storm

The most prominent and well-known feature of the planet Jupiter is the Great Red Spot. It is not a surface feature, as the hard core of Jupiter lies at the bottom of an atmosphere that is thousands of ... Continue reading

JupiterRedSpot
Biology

Beware -- Red Tide!

Red tides occur in oceans. They are not caused by herbicides or pollutants, but by a microscopic alga. Karenia brevis, when in higher than normal concentrations, causes a red tide. This bacterium ... Continue reading

BewareRedTide

Astronomers Glimpse Feeding Of A Galactic Dragon

GalacticDragonA team of radio astronomers has found a cold ring of gas around a supermassive black hole in the fiery nuclear region of quasar galaxy 'QSO I Zw 1,' the most detailed observational evidence yet that gigantic molecular clouds fuel massive star formation in the galactic neighborhood of the black hole. A small fraction of this material might eventually find its way along streamers to the very center, just to be sacrificed to the black hole as fuel to power the brilliant quasar. The ring of gas clouds is likely the site of intense star formation as the clouds collapse under their own gravity, according to the team, and the observation is a significant first step to determining if there is a link between star formation and quasar activity.

Quasars can outshine a trillion suns, and are believed to be the fiercely bright cores of galaxies that harbor black holes weighing in at millions to billions of suns. A black hole, so named because nothing, not even light, can escape its intense gravity once past its boundary, is suspected of being the engine that powers a quasar. While many galaxies have massive black holes lurking in their centers, in quasar galaxies, the black holes 'breathe fire' as they feed on vast amounts of interstellar gas that somehow makes its way into the galactic center. The gas whirls around the black hole before plunging in, like water down a drain. This generates intense friction, heating the gas and causing it to shine brightly.

The ring of gas clouds is about 4,000 light years from the galactic center, rotating around it at about 200 kilometers per second (almost 125 miles/sec.), and contains the mass of more than a billion suns, according to the observation. Despite the unusual optical brilliance of the quasar, these are ordinary characteristics of luminous galaxies, according to the team. Other observations indicate that QSO I Zw 1 is interacting with a neighboring galaxy. Observations of closer galaxies suggest that galactic interactions (collisions and near misses) cause bursts of star formation, and the team is curious about whether such interactions ignite quasar activity as well.