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STAR Sacramento. If so, these huge stars would have quickly consumed their supply of fuel and became supernovae , releasing heavy elements into the interstellar medium.
Such stars are likely to have existed in the very early universe i. Within a billion years of a galaxy's formation, key structures begin to appear.
Globular clusters , the central supermassive black hole, and a galactic bulge of metal-poor Population II stars form. The creation of a supermassive black hole appears to play a key role in actively regulating the growth of galaxies by limiting the total amount of additional matter added.
During the following two billion years, the accumulated matter settles into a galactic disc. The cycle of stellar birth and death slowly increases the abundance of heavy elements, eventually allowing the formation of planets.
The evolution of galaxies can be significantly affected by interactions and collisions. Mergers of galaxies were common during the early epoch, and the majority of galaxies were peculiar in morphology.
However, gravitational stripping of the interstellar gas and dust that makes up the spiral arms produces a long train of stars known as tidal tails.
Although the Milky Way has never collided with a galaxy as large as Andromeda before, evidence of past collisions of the Milky Way with smaller dwarf galaxies is increasing.
Such large-scale interactions are rare. As time passes, mergers of two systems of equal size become less common. Most bright galaxies have remained fundamentally unchanged for the last few billion years, and the net rate of star formation probably also peaked about ten billion years ago.
Spiral galaxies, like the Milky Way, produce new generations of stars as long as they have dense molecular clouds of interstellar hydrogen in their spiral arms.
At the end of the stellar age, galaxies will be composed of compact objects : brown dwarfs , white dwarfs that are cooling or cold " black dwarfs " , neutron stars , and black holes.
Eventually, as a result of gravitational relaxation , all stars will either fall into central supermassive black holes or be flung into intergalactic space as a result of collisions.
Deep sky surveys show that galaxies are often found in groups and clusters. Solitary galaxies that have not significantly interacted with another galaxy of comparable mass during the past billion years are relatively scarce.
Only about five percent of the galaxies surveyed have been found to be truly isolated; however, these isolated formations may have interacted and even merged with other galaxies in the past, and may still be orbited by smaller, satellite galaxies.
Isolated galaxies [note 2] can produce stars at a higher rate than normal, as their gas is not being stripped by other nearby galaxies.
On the largest scale, the universe is continually expanding, resulting in an average increase in the separation between individual galaxies see Hubble's law.
Associations of galaxies can overcome this expansion on a local scale through their mutual gravitational attraction. These associations formed early, as clumps of dark matter pulled their respective galaxies together.
Nearby groups later merged to form larger-scale clusters. This on-going merger process as well as an influx of infalling gas heats the inter-galactic gas within a cluster to very high temperatures, reaching 30— megakelvins.
Most galaxies are gravitationally bound to a number of other galaxies. These form a fractal -like hierarchical distribution of clustered structures, with the smallest such associations being termed groups.
A group of galaxies is the most common type of galactic cluster, and these formations contain a majority of the galaxies as well as most of the baryonic mass in the universe.
If there is insufficient kinetic energy , however, the group may evolve into a smaller number of galaxies through mergers.
Clusters of galaxies consist of hundreds to thousands of galaxies bound together by gravity. Superclusters contain tens of thousands of galaxies, which are found in clusters, groups and sometimes individually.
At the supercluster scale , galaxies are arranged into sheets and filaments surrounding vast empty voids. The Hercules-Corona Borealis Great Wall , currently the largest structure in the universe found so far, is 10 billion light-years three gigaparsecs in length.
The Milky Way and the Andromeda Galaxy are the two brightest galaxies within the group; many of the other member galaxies are dwarf companions of these two.
The peak radiation of most stars lies in the visible spectrum , so the observation of the stars that form galaxies has been a major component of optical astronomy.
It is also a favorable portion of the spectrum for observing ionized H II regions , and for examining the distribution of dusty arms.
The dust present in the interstellar medium is opaque to visual light. It is more transparent to far-infrared , which can be used to observe the interior regions of giant molecular clouds and galactic cores in great detail.
Water vapor and carbon dioxide absorb a number of useful portions of the infrared spectrum, so high-altitude or space-based telescopes are used for infrared astronomy.
The first non-visual study of galaxies, particularly active galaxies, was made using radio frequencies. The ionosphere blocks signals below this range.
Ultraviolet and X-ray telescopes can observe highly energetic galactic phenomena. Ultraviolet flares are sometimes observed when a star in a distant galaxy is torn apart from the tidal forces of a nearby black hole.
The existence of supermassive black holes at the cores of galaxies was confirmed through X-ray astronomy. From Wikipedia, the free encyclopedia.
This article is about the astronomical structure. For our galaxy, see Milky Way. For other uses, see Galaxy disambiguation.
Gravitationally bound astronomical structure. Main article: Milky Way. Main article: Galaxy morphological classification.
Main article: Elliptical galaxy. Main articles: Spiral galaxy and Barred spiral galaxy. Main article: Dwarf galaxy.
Main article: Interacting galaxy. Main article: Starburst galaxy. Main article: Active galactic nucleus. Main article: Blazar.
Main article: Low-ionization nuclear emission-line region. Main article: Seyfert galaxy. Main article: Quasar. Main article: Luminous infrared galaxy.
Main article: Galaxy formation and evolution. XDF view field compared to the angular size of the Moon. Several thousand galaxies, each consisting of billions of stars , are in this small view.
XDF view: Each light speck is a galaxy, some of which are as old as XDF image shows from left fully mature galaxies, nearly mature galaxies from five to nine billion years ago , and protogalaxies , blazing with young stars beyond nine billion years.
Main article: Future of an expanding universe. Seyfert's Sextet is an example of a compact galaxy group.
The largest structures in the universe are larger than expected. Are these actual structures or random density fluctuations?
Play media. Hubble Legacy Field second video . See also: Observational astronomy. This ultraviolet image of Andromeda shows blue regions containing young, massive stars.
Dark galaxy Galactic orientation Galaxy formation and evolution Illustris project List of galaxies List of nearest galaxies Luminous infrared galaxy Outline of galaxies Supermassive black hole Timeline of knowledge about galaxies, clusters of galaxies, and large-scale structure UniverseMachine.
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