Outline of galaxies

The following outline is provided as an overview of and topical guide to galaxies:

Galaxies – gravitationally bound systems of stars, stellar remnants, interstellar gas, dust, and dark matter. The word galaxy is derived from the Greek galaxias (γαλαξίας), literally "milky", a reference to the Milky Way. Galaxies range in size from dwarfs with just a few billion (109) stars to giants with one hundred trillion (1014) stars, each orbiting its galaxy's center of mass. Galaxies are categorized according to their visual morphology as elliptical, spiral and irregular. Many galaxies are thought to have black holes at their active centers.

The Milky Way's central black hole, known as Sagittarius A*, has a mass four million times greater than the Sun. As of March 2016, GN-z11 is the oldest and most distant observed galaxy with a comoving distance of 32 billion light-years from Earth, and observed as it existed just 400 million years after the Big Bang. Previously, as of July 2015, EGSY8p7 was the most distant known galaxy, estimated to have a light travel distance of 13.2 billion light-years away.

What type of thing are galaxies?

Galaxies can be described as all of the following:

Types of galaxies

By morphological classification

Galaxy morphological classification

By nucleus

Active galactic nucleus

By emissions

By interaction

By other aspect

Nature of galaxies

Galactic phenomena

Galaxy components

Galactic cartography
Further information: Celestial cartography

Larger constructs composed of galaxies

Intergalactic phenomena

Fields that study galaxies


Galaxy catalogs

Persons influential in the study of galaxies
gollark: It's not a statement about intelligence - as far as I can tell most people have no idea how the fairly interesting technology driving this sort of thing (and basically everything *else* in computing) actually works, don't particularly care, and resist being told about it.↓ below person: this is relevant information which people considering buying it should probably know, so that they can use their money effectively
gollark: No, I mean the predictive text probably will get better at some point because of this sort of thing, and then I suppose you'll just ignore it and assume it magically gets better by magic.
gollark: This is also possible.
gollark: Oh, *you will*.
gollark: It's weird that the predictions remain moderately bad despite recent exciting advances in natural language processing.

See also

References
  1. Cosmic Year Archived 2014-04-12 at the Wayback Machine, Fact Guru, University of Ottawa
  2. Galileo Galilei, Sidereus Nuncius (Venice, (Italy): Thomas Baglioni, 1610), pages 15 and 16. English translation: Galileo Galilei with Edward Stafford Carlos, trans., The Sidereal Messenger (London, England: Rivingtons, 1880), pages 42 and 43.
  3. O'Connor, J. J.; Robertson, E. F. (November 2002). "Galileo Galilei". University of St. Andrews. Retrieved January 8, 2007.
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