Sunday, September 20, 2015

Milky Way Galaxy Facts

The Milky Way Galaxy is our home galaxy in the universe. It is a fairly typical barred spiral with four major arms in its disk, at least one spur, and a newly discovered outer arm. The galactic centre, which is located about 26,000 light-years from Earth, contains at least one supermassive black hole (called Sagittarius A*), and is crossed by a bar. The Milky Way began forming around 12 billion years ago and is part of a group of about 50 galaxies called the Local Group. The Andromeda Galaxy is part of this group as are numerous smaller ones galaxies, including the Magellanic Clouds. The Local Group itself is part of a larger gathering of galaxies called the Virgo Supercluster of galaxies.

The Milky Way Galaxy

Galaxy Profile
Type: Barred Spiral
Diameter: 220,000 light-years
Mass: 400-800 billion solar masses (depending on measuring technique)
Number of Stars: at least 400 billion
Group: Local Group

Facts About The Milky Way
The Milky Way began as a series of dense regions in the early universe not long after the Big             Bang. The first stars to form were in globular clusters that still exist. They are among the oldest           stars formed in the Milky Way region.

The Milky Way has grown by merging with other galaxies through time. It is currently acquiring         stars from a very small galaxy called the Sagittarius Dwarf Spheroidal, as well as gobbling up             material from the Magellanic Clouds.

The Milky Way moves through space at a velocity of about 552 kilometres per second (343                 miles per second) with respect to the Cosmic Microwave Background radiation.

The Milky Way’s central core contains a supermassive black hole. It is commonly referred to as         Sagittarius A*. It contains the mass of about 2.6 million Suns.

The stars, gas and dust of the Milky Way all orbit the centre at a rate of about 220 kilometres per         second. This constant rate for all stars at different distances from the core implies the existence           of a shell of dark matter surrounding our galaxy.

Our galaxy will collide with Andromeda Galaxy in about 5 billion years. Some astronomers                 refer to our two galaxy as a binary system of giant spirals.

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