Galaxies

Introduction

In astronomy, a galaxy is a massive, gravitationally bound system consisting of stars, stellar remnants, an interstellar medium of gas and dust (nebulae), and dark matter, an important but poorly understood component.

 The word galaxy is derived from the Greek galaxias (γαλαξίας), literally "milky", a reference to the Milky Way. Examples of galaxies range from dwarfs with as few as ten million (107) stars to giants with one hundred trillion (1014) stars, each orbiting their galaxy's own center of mass. 


Hubble2005-01-barred-spiral-galaxy-NGC1300

Barred spiral galaxy NGC 1300 photographed by Hubble telescope.. image: wikipedia/Hubblesite

Galaxies contain varying numbers of planets, star systems, star clusters and types of interstellar clouds. In between these objects is a sparse interstellar medium of gas, dust, and cosmic rays. 


Andromeda_Galaxy_(with_h-alpha)

Telescope image of Andromeda galaxy M31 by Adam Evans -  wikimedia

Supermassive black holes reside at the center of most galaxies. They are thought to be the primary driver of active galactic nuclei found at the core of some galaxies. The Milky Way galaxy is known to harbor at least one such object.

How they are categorised

Galaxies have been historically categorized according to their apparent shape, usually referred to as their visual morphology. A common form is the elliptical galaxy, which has an ellipse-shaped light profile. Spiral galaxies are disk-shaped with dusty, curving arms. 

HubbleTuningFork

Hubble classification of Galaxies. image: wikipedia

Those with irregular or unusual shapes are known as irregular galaxies and typically originate from disruption by the gravitational pull of neighboring galaxies. Such interactions between nearby galaxies, which may ultimately result in a merger, sometimes induce significantly increased incidents of star formation leading to starburst galaxies. Smaller galaxies lacking a coherent structure are referred to as irregular galaxies.

Numbers of galaxies

There are probably more than 170 billion galaxies in the observable universe. Most are 1,000 to 100,000 parsecs in diameter and usually separated by distances on the order of millions of parsecs (or megaparsecs). Intergalactic space (the space between galaxies) is filled with a tenuous gas of an average density less than one atom per cubic meter.

 The majority of galaxies are organized into a hierarchy of associations known as galaxy groups and clusters, which, in turn usually form larger superclusters. At the largest scale, these associations are generally arranged into sheets and filaments, which are surrounded by immense voids.

Sourcehttp://en.wikipedia.org/wiki/Galaxies