What is Dark Energy?


    We don't know. We know how much there is, and we know some of the properties
    it must have. Other than that, dark energy is a mystery, and it's important that we
    find out more. Roughly 70% of the universe is made of dark energy. Dark matter
    makes up about 25%. Everything on Earth, everything that we have ever
    observed with all of our instruments – normal matter – adds up to less than 5% of
    the universe. Then again, maybe we shouldn't even continue call it "normal"
    matter since it's just a small fraction of the universe!

    Albert Einstein was the first person to realize that empty space is not the same as
    nothingness. Space has amazing properties, many of which are just beginning to
    be understood. The first property of space that Einstein discovered is that it is
    possible for more space to come into existence. One version of Einstein's gravity
    theory makes a second prediction: "empty space" can possess its own energy.
    This energy would not be diluted as space expands, because it is a property of
    space itself; as more space came into existence, more of this energy-of-space
    would come into existence as well. As a result, this form of energy would cause
    the universe to expand faster and faster as time passes. Unfortunately, no one
    understands why space should contain the observed amount of energy and not,
    say, much more or much less.

    But why haven't we observed it? Often, we measure differences, not absolute
    values. When we talk about the height of mountains, we are talking about how
    high they are above sea level, not the distance between the mountain top and
    the center of the earth. We assume a "floor" for these purposes. Likewise, we
    measure differences of energy in the universe – but there could be a "sea-level"
    for energy in the universe that we cannot yet measure.

    What is the nature of this energy? As scientists developed the quantum theory of
    matter, they realized that "empty space" was full of temporary ("virtual") particles
    continually forming and destroying themselves. Physicists began to suspect that
    indeed the vacuum ought to have a distinct form of energy, but they could not
    predict its magnitude.

    While theoretical physicists were trying to come to grips with dark energy,
    observational astronomers were trying to explain a bizarre result. Theories at that
    time predicted that the universe's mass should be slowly overcoming the
    momentum of the big bang, causing the expansion of the universe to slow down.
    But observations of supernovas in other galaxies were showing that the universe
    was actually expanding much faster than expected. Something was causing the
    universe to have another growth spurt!

    Theory and observation dovetailed in dark energy. The dark energy has
    presumably been around since the beginning of the universe, but its effect may
    become more dominant as the universe expands. We still do not know whether or
    how the highly accelerated expansion in the early Universe (inflation) and the
    current accelerated expansion (due to dark energy) are related.























    This diagram reveals changes in the rate of expansion since the universe's birth
    15 billion years ago. The more shallow the curve, the faster the rate of
    expansion. The curve changes noticeably about 7.5 billion years ago, when
    objects in the universe began flying apart as a faster rate. Astronomers theorize
    that the faster expansion rate is due to a mysterious, dark force that is pulling
    galaxies apart. Credit: NASA/STSci/Ann Feild [+ more]

    NASA is planning missions to find some clues to solve the mystery of dark
    energy. These missions will investigate the variation of the universe's density
    over time, and how the universe's rate of expansion has changed over time.

    What About Dark Matter?


    The image below is not a picture of dark matter. It is a picture of its effects,
    captured by the Chandra X-ray Observatory. It's a galaxy surrounded by a cloud
    of extremely hot gas. In order for the gas to stay around the galaxy, a halo of
    matter we cannot see must be holding it there with its gravity.













    Astronomy relies on light, whether this light is x-rays or radio waves or the light
    we can see with our eyes. But most of the matter in the universe is dark: it
    doesn't create its own light like stars do. (We see planets and asteroids because
    they are illuminated by the stars they orbit. These objects are not considered
    dark matter.)

    As with dark energy, we know very little about dark matter other than how much
    there is – about 25% of the universe's mass. Dark matter can be measured
    indirectly, by calculating how much mass is required to create enough gravity to
    make galaxies behave the way they do.

    There are many theories about the nature of dark matter. One says that it is
    weakly interactive massive particles (WIMPs) another says that it is massive
    compact halo objects (MACHOs).

What Is Dark Energy
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