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The Curious Case of Centaurus A
By Wil Milan
Special to SPACE.com
posted: 06:01 am ET
01 May 2000

The Curious Case of Centaurus A

In the mid-1830s in colonial South Africa, visiting British astronomer John Herschel spotted an object that perhaps no one had ever seen before: A round, fuzzy little nebula, curious in that it seemed to have a broad dark band across its middle but otherwise unremarkable.

Herschel, who was in South Africa to catalog fuzzy objects like this, logged it in his books and later listed it in his catalog of celestial objects. This particular object didnt seem special in any way and didnt even merit a name, but only a numerical catalog designation. It eventually becomes known by its updated catalog number, NGC 5128.

100 years later

Fast forward to 1949, when astronomers in Australia working with one of the earliest radio telescopes discover a very loud source of radio noise in the southern constellation Centaurus. Not knowing what it is, the radio source becomes known as Centaurus A (the "A" indicating its the first radio source in Centaurus). After careful measurements, they determine that Centaurus A is in fact Herschels obscure little object, NGC 5128, which by now is known to be a galaxy, albeit one rather oddly shaped.

A few years later, spaceborne X-ray detectors provide our first view of the X-ray sky and they discover that Centaurus A is also a prominent source of powerful X-rays. When gamma-ray detectors are lofted into space, Centaurus A is again found to be a strong source of this ultra-powerful type of radiation. It seems there is something very strange and mysterious going on in Lord Herschels fuzzy little object.

Strange appearance

In the past 50 years, conventional telescopes also have examined Centaurus A, and theyve found it to have a very strange appearance. It appears to be a large elliptical galaxy encircled by a thick dark band of material. The odd thing about that is that large elliptical galaxies typically do not have such dark bands of dust and debris (known as "dust lanes"). Spiral galaxies typically do have such dust lanes, but Centaurus A is obviously not a spiral galaxy. It is this strange juxtaposition of characteristics that led to a theory that explains the odd characteristics of Centaurus A: Its the scene of an accident.

A cosmic crash and a fading ghost

Centaurus A is the result of an enormous galactic collision where a spiral galaxy slammed headlong into a larger elliptical galaxy, ripping the arms off the smaller galaxy and scattering parts of it as a dark band of dust around the larger elliptical. This accounts for the angled band of dust around the galaxy, as the dusty arms of the elliptical galaxy have been shredded and scattered into and around the large elliptical.

The latest evidence for this theory is a remarkable photo taken in infrared light by the orbiting European Infrared Space Observatory (ISO). Infrared light can penetrate through dust and gas that can block visible light and, like a view of a fading ghost, the ISO camera captured an image of the remaining core of the shredded spiral galaxy. It is now embedded deep in the dust and debris of the large elliptical, but the infrared image shows the core of the shredded spiral, shorn of its spiral arms but still maintaining its bar-like shape.

The lurking giant

A giant cosmic collision is certainly a dramatic event, but it turns out there is another fascinating aspect of Centaurus A: Recent radio and X-ray studies of Centaurus A reveal enormously powerful jets of superheated material being shot out of the galaxy in opposite directions at near light speed (see photos).

These spinning jets of material are thousands of light years in length, and it is the tremendous blast of energy from these jets that is generating much of the radio and X-ray radiation that makes Centaurus A such a strong source of radio noise and X-rays.

Such powerful jets have been spotted in some other galaxies as well, and their source is now well known: Such jets are the signature of a super-massive black hole in the center of the galaxy, a black hole with a mass millions of times greater than our sun. The gravitational pull of such a black hole is so powerful that material is sucked into it and around it at tremendous speeds. As the material is spinning around the black hole it can be entwined into twisting jets shooting away from the poles of the black hole, much like a cotton-candy machine can spin long twisted tendrils as the cotton ball is pulled away.

A glowing laboratory

Crashing galaxies, a giant spinning black hole, powerful glowing jets flying out of the galactic core all of these add up to what astronomers call an "active galaxy." These are galaxies that have undergone some sort of catastrophic disturbance and are now producing powerful outbursts of energy and star formation.

Most such galaxies are very distant, but Centaurus A is unique in that it is a relatively close (about 10 million light years, which is "just down the street" as galaxies go). That makes it a unique "cosmic laboratory" for studying the strange effects and high-energy physics that accompany such powerful outbursts and collisions.

The eyeball view

All its blast and thunder aside, Centaurus A is rewarding another way: Its an easy object for anyone to see, needing only a pair of binoculars or small telescope, visible low on the southern horizon in springtime (for observers in the northern hemisphere). Amateur astronomers often dub Centaurus A "the hamburger galaxy" for its curious appearance in the eyepiece. (Squint your eyes and look at the photo to understand why.)

The peaceful appearance of Centaurus A in a small telescope is a reminder of two complementary truths: That behind much of the beauty of the sky lies incomprehensible power and fury, and that maelstrom and destruction can produce a very tranquil beauty. Its our great luxury to be snug and safe a great distance from Centaurus A, enjoying its beauty and learning its mysteries without having to fear its power.

Wil Milan is an astrophotographer based in Arizona. Some of his work can be seen at http://www.astrophotographer.com/

 

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