| |
Space
Station Info >> The Universe
The Universe
The universe
is the entire space-time continuum in which we
exist, together with all the energy and matter
within it. Attempts to understand the universe
in this sense, on the largest possible scales,
are made in cosmology, a science that has grown
from physics and astronomy. During the second
half of the 20th century, the development of observational
cosmology, also called physical cosmology, led
to a split in the meaning of the word universe,
between observational cosmologists and theoretical
cosmologists; where the former (usually) abandon
the hope of observing the whole spacetime continuum,
the latter retain this hope, attempting to find
the most reasonable speculations for modeling
the whole of spacetime, despite the extreme difficulty
in imagining any empirical constraints on these
speculations and the possibility of crossing over
to metaphysics.
The terms known
universe, observable universe, or visible universe
are often used to describe the part of the universe
that we can see or otherwise observe. Those who
believe it is impossible to observe the whole
continuum may use our universe, referring only
to that knowable by human beings in particular.
| w
Expansion
And The Big Bang Theory
The most important result
of cosmology, that the universe is expanding,
is derived from red shift observations and
quantified by Hubble's Law. Extrapolating
this expansion back in time, one approaches
a gravitational singularity, a rather abstract
mathematical concept, which may or may not
correspond to reality. This gives rise to
the Big Bang theory, the dominant model
in cosmology today. The age of the Universe
was estimated to be about 13.7 billion (13.7
× 109) years, with a margin of error
of about 1 percent (± 200 million
years), according to NASA's Wilkinson Microwave
Anisotropy Probe (WMAP). |
|
However, this
is based on the assumption that the underlying
model used for data analysis is correct. Other
methods of estimating the age of the universe
give different ages. A fundamental aspect of the
Big Bang can be seen today in the observation
that the farther away from us galaxies are, the
faster they move away from us. It can also be
seen in the cosmic microwave background radiation
which is the much-attenuated radiation that originated
soon after the Big Bang. This background radiation
is remarkably uniform in all directions, which
cosmologists have attempted to explain by an initial
period of rapid inflation following the Big Bang.
w
Size
Of The Universe
There is disagreement over whether the universe
is finite or infinite in spatial extent and volume.
However, the observable universe, consisting of
all locations that could have affected us since
the Big Bang given the finite speed of light,
is certainly finite. The edge of the cosmic light
horizon is 13.7 billion light years distant. The
present distance (commoving distance) to the edge
of the observable universe is larger, since the
universe has been expanding; it is estimated to
be about 78 billion light years (7.8 × 1010
light years, or 7.4 × 1023 km). This would
make the comoving volume, of the known universe,
equal to 1.9 × 1033 cubic light years (assuming
this region is perfectly spherical). The observable
universe contains about 7 × 1022 stars,
organized in about 10 billion galaxies, which
themselves form clusters and super clusters. The
number of galaxies may be even larger, based on
the Hubble Deep Field observed with the Hubble
Space Telescope. Both popular and professional
research articles in cosmology often use the term
"Universe" when they really mean "observable
universe". This is because unobservable physical
phenomena are scientifically irrelevant; that
is, they cannot affect any events that we can
perceive, and therefore, it is argued, effectively
do not exist.
We live in the centre of the universe that we
observe, in apparent contradiction to the Copernican
principle which says that the Universe is more
or less uniform and it has no distinguished centre.
This is simply because light does not travel infinitely
fast, and we make observations of the past. As
we look further and further away, we see things
from epochs (times) closer and closer to the limit
of time=zero of the Big bang model. And since
light travels at the same speed in any direction
towards us, we live at the centre of our observable
universe.
Both popular
and professional research articles in cosmology
often use the term "Universe" when they
really mean "observable universe". This
is because unobservable physical phenomena are
scientifically irrelevant; that is, they cannot
affect any events that we can perceive, and therefore,
it is argued, effectively do not exist.We live
in the centre of the universe that we observe,
in apparent contradiction to the Copernican principle
which says that the Universe is more or less uniform
and it has no distinguished centre. This is simply
because light does not travel infinitely fast,
and we make observations of the past. As we look
further and further away, we see things from epochs
(times) closer and closer to the limit of time=zero
of the Big bang model. And since light travels
at the same speed in any direction towards us,
we live at the centre of our observable universe.
w
Shape
Of The Universe
An important open question of cosmology is the
shape of the universe. Mathematically, which 3-manifold
is the universe?
Firstly, whether or not the universe is flat,
i.e. whether the rules of Euclidean geometry are
valid on the largest scales, is unknown. Currently,
most cosmologists believe that the observable
universe is (nearly) flat, with local wrinkles
where massive objects distort spacetime, just
as a lake is (nearly) flat. This opinion was strengthened
by the latest data from WMAP, looking at "acoustic
oscillations" in the cosmic background radiation
temperature variations.Secondly, whether or not
the universe is multiply connected, is unknown.
The universe has no spatial boundary according
to the standard big bang model, but nevertheless
may be spatially finite (compact). This can be
understood using a two-dimensional analogy: the
surface of a sphere has no edge, but nonetheless
has a finite area. It is a two-dimensional surface
with constant curvature in a third dimension.
The 3-sphere is a three-dimensional equivalent
in which all three dimensions are constantly curved
in a fourth.
If the universe is indeed spatially finite, as
described, then traveling in a "straight"
line, in any given direction, would theoretically
cause one to eventually arrive back at the starting
point.
Strictly speaking, we should call the stars and
galaxies "views" of stars and galaxies,
since it is possible that the universe is multiply-connected
and sufficiently small (and of an appropriate,
perhaps complex, shape) that we can see once or
several times around it in various, and perhaps
all, directions. (Think of a house of mirrors.)
If so, the actual number of physically distinct
stars and galaxies would be smaller than currently
accounted. Although this possibility has not been
ruled out, the results of the latest cosmic microwave
background research make this appear very unlikely.
w
Fate
Of The Universe
Depending on the average density of matter and
energy in the universe, it will either keep on
expanding forever or it will be gravitationally
slowed and will eventually collapse back on itself
in a "big crunch". Currently the evidence
suggests not only that there is insufficient mass/energy
to cause a recollapse, but that the expansion
of the universe seems to be accelerating and will
accelerate for the whole of eternity. Other ideas
of the fate of our universe include the Big Rip,
the Big Freeze, and Heat death of the universe
theory. For a more detailed discussion of other
theories, see the ultimate fate of the universe.
w
Multiverse
There is some speculation that multiple universes
exist in a higher-level multiverse (also known
as a megaverse), our universe being one of those
universes (lower case). For example, matter that
falls into a black hole in our universe could
emerge as a "Big Bang," starting another
universe. However, all such ideas are currently
untestable and cannot be regarded as anything
more than speculation. The concept of parallel
universes is understood only when related to string
theory.
|
|