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Color image of spiral galaxy.
Spiral galaxy NGC 7331 looks similar to our Milky Way.

Editor's Note: This page provides a brief overview of our Universe. For a comprehensive look at the Universe, visit NASA's Astrophysics Division.

Color illustration of cosmic dust cloud.
gas pillars in the Eagle Nebula (M16).
Color image of distant star.
The first planet discovered beyond our solar system orbits the star 51 Pegasi.
Color image showing hundres of galaxies in a single frame.
Several hundred galaxies are visible in this image.

Our sun is one of at least 100 billion stars in the Milky Way, a spiral galaxy about 100,000 light years across. The stars are arranged in a pinwheel pattern with four major arms, and we live about two-thirds of the way up one of them. Many if not most of the stars host their own families of planets. More than a thousand of these extrasolar (or exoplanets) have been discovered and thousands more are awaiting confirmation.

All of the stars in the Milky Way orbit a supermassive black hole at the galaxy's center, which is estimated to be some 4 million times as massive as our sun. Fortunately, it is a safe distance of around 28,000 light years away Earth. The Milky Way zips alonga galactic orbit at an average speed of about 514,000 miles per hour (828,000 km/hr). It takes about 230 million years for our solar system to make one revolution around the galactic center.

Beyond Our Galaxy

The Milky Way is part of the Local Group, a neighborhood about 10 million light years across, consisting of more than 30 galaxies that are gravitationally bound to each other. Aside from our galaxy, the most massive one in this group is Andromeda, which appears to be on course to collide with the Milky Way in about 4 billion years.

Scientists studying galaxies observed that the stars in the outer parts are orbiting the galactic centers just as quickly as the stars further in, a violation of Newton's well-established laws of gravitation. They deduced that something other than the stars and clouds of gas and dust known to comprise galaxies was providing extra gravity –
lots of it. They calculated that there must be five times as much of this mysterious dark matter, detectable only by its gravitational pull, as there is of the matter we already knew about.

The Local Group is only one of many, many clusters of galaxies, and they are all moving away from each other as more and more space comes into being between them. This means the universe, itself, is expanding. That discovery is what led to the theory of the Big Bang origin of the universe.

Scientists expected that the gravitational attraction of everything in the universe would put the brakes on the rate of expansion, and eventually the expansion would stop or even reverse. But in the 1990s, scientists discovered that the expansion is actually getting faster. The force responsible for this surprising acceleration was dubbed dark energy. No one is sure what it is, but one possibility is that it is energy contained within the very vacuum of space.

Since matter and energy are equivalent (as expressed in Einstein's famous equation, E=MC2) scientists have been able to calculate that whatever dark energy is, it comprises about 68 percent of everything in the universe. Dark matter accounts for another 27 percent, leaving only five percent for protons, neutrons, electrons and photons – in other words, everything we see and understand.

Scientists calculate that there are at least 100 billion galaxies in the observable universe, each one brimming with stars. On a very large scale, they form a bubbly structure, in which vast sheets and filaments of galaxies surround gargantuan voids.

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Last Updated: 6 May 2014