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Centaurus A

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Centaurus A is a unique and highly active galaxy located in the constellation of Centaurus. It is known by several names, including NGC 5128 and Caldwell 77. This galaxy is significant because it is the closest radio galaxy to Earth. It is also the closest BL Lac object, which is a type of active galaxy. Because of its proximity, professional astronomers study its active galactic nucleus very closely.

Centaurus A is the fifth-brightest galaxy in the sky. This brightness makes it an excellent target for amateur astronomers. However, it is only visible from the southern hemisphere and low northern latitudes.

The galaxy possesses a very peculiar morphology, or physical shape. To observers on Earth, it appears as a lenticular or elliptical galaxy. A lenticular galaxy is a shape that sits between elliptical and spiral galaxies. What makes Centaurus A stand out is a dark dust lane that seems to be superimposed over the galaxy.

StuctureCenA-EN
StuctureCenA-EN

This strange structure was first noted by John Herschel in 1847. He described it as two elliptical nebulae separated by a broad, dark band. Many scientists believe this shape is the result of a cosmic merger. This occurs when two galaxies collide and combine into one.

At the heart of Centaurus A lies a supermassive black hole. This black hole has a mass of 55 million solar masses. This means it is as heavy as 55 million of our Sun. The black hole produces a relativistic jet, which is a stream of matter ejected at extreme speeds. The inner parts of this jet move at about half the speed of light.

StuctureCenA-EN
StuctureCenA-EN

These jets emit energy across different wavelengths. The radio jets are massive, stretching over a million light-years in length. The X-ray jets are much shorter, reaching thousands of light-years. X-rays are created further out when the jet collides with surrounding gases. This collision creates highly energetic particles.

Astronomers believe Centaurus A is a starburst galaxy. A starburst galaxy is a place where stars are forming at a very high rate. This intense burst of star formation is likely caused by a galactic collision. Models suggest that a large elliptical galaxy collided with a smaller spiral galaxy. This collision likely triggered the creation of many new stars. Over 100 star formation regions have been identified within the dusty disk. The bulge of the galaxy is mostly made of older, red stars.

ESO Centaurus A LABOCA
ESO Centaurus A LABOCA

The history of observing Centaurus A is quite long. The Scottish astronomer James Dunlop discovered the galaxy in 1826. He made this discovery while working at the Parramatta Observatory in Australia. In 1949, researchers John Gatenby Bolton, Bruce Slee, and Gordon Stanley identified it as an extragalactic radio source. In 1954, Walter Baade and Rudolph Minkowski suggested the merger theory. This theory explained why the galaxy looked so disturbed. Later, the Hubble Space Telescope discovered young blue stars along the central dust band in 1990.

Many different telescopes have provided new details about this galaxy. In 1979, the Einstein Observatory detected an X-ray jet coming from the nucleus. The Chandra X-ray Observatory identified over 200 new point sources in 1999. In 2006, the Spitzer Space Telescope found a parallelogram-shaped structure made of dust. The H.E.S.S. Observatory in Namibia detected high-energy gamma emissions in 2009. We have even observed individual stars exploding within the galaxy. For example, Robert Evans discovered a Type Ia supernova named SN 1986G in 1986.

Supernova 1986 G in the peculiar, southern galaxy Centaurus A (NGC 5128) (eso8608a)
Supernova 1986 G in the peculiar, southern galaxy Centaurus A (NGC 5128) (eso8608a)

Centaurus A is a vital part of a larger cosmic structure. It sits at the center of one of two subgroups in the Centaurus A/M83 Group. This group is located within the much larger Virgo Supercluster. The other subgroup in this group is centered around the Messier 83 galaxy. Studying Centaurus A helps scientists understand how different types of galaxies interact. While collisions between spiral galaxies are common, the effects of an elliptical and a spiral galaxy merging are not fully understood. This makes Centaurus A a key subject for learning about galactic evolution.

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File:ESO Centaurus A LABOCA.jpg
ESO Centaurus A LABOCA.jpg
Centaurus A EN.webm
File:StuctureCenA-EN.png
StuctureCenA-EN.png
File:Supernova 1986 G in the peculiar, southern galaxy Centaurus A (NGC 5128) (eso8608a).jpg
Supernova 1986 G in the peculiar,...
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