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The Hubble Space Telescope has produced a close-up view of the galaxy Centaurus A. Hubble's
multi-wavelength image is the most detailed ever made of this dynamic and dusty galaxy.
Centaurus A is well known for its huge dust lanes that stretch across the entire extent
of the galaxy. Hubble's new observations are an extreme close-up of a small part of these
dust lanes. This new image is made from observations in ultraviolet, optical and near- infrared
light. The utraviolet light shows us the location of hot young stars, whereas the near infrared
light allows us to glimpse some of the details that are obscured by dust in the optical.
Astronomers think that Centaurus A must have collided and merged with another galaxy at
some point in the past. The shockwaves of this event caused hydrogen gas to coalesce
and sparked intense areas of star formation, as seen in the red patches visible here. The
turmoil of this collision also explains the warped shape of the galaxy's disc.
Looking at a broader view taken by ESO's Wide Field Imager reveals the extent of the distortion
in Cen A's shape, as well as further areas of vigorous star formation.
The galaxy contains a highly active supermassive black hole at its center. Powerful relativistic
jets release vast amounts of radio and X-ray radiation. Although Hubble can't see this,
submillimeter telescopes like APEX can see broad plumes of matter being ejected far out
from the galaxy.
At just over 11 million light-years distant, Cen A is relatively close in astronomical
terms. In fact, it's not only close, it is very bright. Amateur astronomers with a view
of the southern skies can see it with just a pair of binoculars, while those with a largish
amateur telescope can even make out the dust lanes.
But only Hubble reveals this much detail. Not only does the space telescope offer unprecedented
clarity due to its position above the distorting effects of the atmosphere: it is also able
to observe ultraviolet and infrared wavelengths with pristine clarity.