Interesting Facts About Galaxies

                                              Galaxies

        A Galaxy is a huge mass of stars, nebulae, and interstellar material. The smallest galaxies contain about 100, 000 stars, while the largest contain up to 3, 000 billion stars. There are three main types of galaxy, classified according to their shape: elliptical, which are oval shaped; spiral, which has arms spiraling outwards from a central bulge and irregular, which have no obvious shape. Sometimes, the shape of a galaxy is distorted by a collision with another galaxy. Quasars are thought to be galactic nuclei but are so far away that their exact nature is still uncertain. They are compact, highly luminous objects in the outer reaches of the known Universe: while the furthest known "ordinary" galaxies are about 12 billion light years away, the furthest known quasar is about 13 billion light year away. Active galaxies, such as Seyfert galaxies and radio galaxies, emit intense radiation. In a Seyfert galaxy, this radiation comes from the galactic nucleus; in a radio galaxy, it also comes from huge lobes on either side of the galaxy. The radiation from active galaxies and quasars is thought to be caused by material falling into central black holes.

Anatomy of the Universe

ANATOMY OF THE UNIVERSE

         The UNIVERSE CONTAINS EVERYTHING that exists, from the tiniest subatomic particles to galactic superclusters. Nobody knows how big the Universe is, but astronomers estimate that it contains at least 125 billion galaxies, each comprising an average of 100 billions stars. The most widely accepted theory about the origin of the Universe is the Big Bang theory, which states that the Universe came into being in a huge explosion - the Big Bang - that took place between 10 and 20 billion years ago. The Universe initially consisted of a very hot, dense fireball of expanding, cooling gas. After about one million years, the gas began to condense into localized clumps called protogalaxies. During the next five billion years, the protogalaxies continued condensing, forming galaxies in which stars were being born. Today, billions of years later, the Universe as a whole is still expanding, although there are localized areas in which objects are held together by gravity; for example, many galaxies are found in clusters. The Big Bang theory is supported by the discovery of faint, cool background radiation coming evenly from all directions. This radiation is believed to be Bing Bang. Small "ripples" in the temperature of the cosmic background radiation are thought to be evidence of slight fluctuations in the density of the early Universe, which resulted in the formation of galaxies. Astronomers do not yet know if the Universe is "closed", which means it will eventually stop expanding and begin to contract, or if it is "open", which means it will continue expanding forever.