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The Minor Planets

Asteroids are rocky fragments left over from the formation of the solar system about 4.6 billion years ago. Most of these fragments of ancient space rubble - sometimes referred to by scientists as minor planets - can be found orbiting the Sun in a belt between Mars and Jupiter. This region in our solar system, called the Asteroid Belt or Main Belt, ...

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MinorPlanets
Biology

Palm Trees and Prickly Pears

If you drive around Southern California you'll see a lot of palm trees and prickly pear cacti. If you drive around Southern Spain you will too! How did it happen that two places an ocean apart have ... Continue reading

PalmTreesandPricklyPears
Astronomy

A Ring Around a Dying Star

In November 2002, sky watchers were viewing the glow of meteors from the Leonid meteor shower burning up in Earth's atmosphere. They had been anticipating this celestial light show for months, ... Continue reading

ARingAroundaDyingStar
Geology

Rock, Mineral, Crystal, or Gemstone?

Rocks and minerals are all around us and used every day, perhaps without us even being aware of them. Besides making up the solid, supporting surface of the earth we live and move upon daily, rocks ... Continue reading

RockMineralCrystalGemstone
Physics

Bizarre Boiling

The next time you're watching a pot of water boil, perhaps for coffee or a cup of soup, pause for a moment and consider: what would this look like in space? Would the turbulent bubbles rise or fall? ... Continue reading

BizarreBoiling

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.