0.1 The Possibility of a “Finite” and yet “Unbounded” Universe
From Relativity: The Special and General Theory by Albert Einstein
But speculations on the structure of the universe also move in quite another direction. The
development of non-Euclidean geometry led to the recognition of the fact, that we can cast doubt
on the infiniteness of our space without coming into conflict with the laws of thought or with
experience (Riemann, Helmholtz). These questions have already been treated in detail and with
unsurpassable lucidity by Helmholtz and Poincaré, whereas I can only touch on them briefly
here.
In the first place, we imagine an existence in two dimensional space. Flat beings with flat
implements, and in particular flat rigid measuring-rods, are free to move in a plane. For them
nothing exists outside of this plane: that which they observe to happen to themselves and to their
flat “things” is the all-inclusive reality of their plane. In particular, the constructions of plane
Euclidean geometry can be carried out by means of the rods e.g. the lattice construction,
considered in section 24. In contrast to ours, the universe of these beings is two-dimensional; but,
like ours, it extends to infinity. In their universe there is room for an infinite number of
identical squares made up of rods, i.e. its volume (surface) is infinite. If these beings say
their universe is “plane,” there is sense in the statement, because they mean that they
can perform the constructions of plane Euclidean geometry with their rods. In this
connection the individual rods always represent the same distance, independently of their
position.
Let us consider now a second two-dimensional existence, but this time on a spherical surface
instead of on a plane. The flat beings with their measuring-rods and other objects fit exactly on
this surface and they are unable to leave it. Their whole universe of observation extends
exclusively over the surface of the sphere. Are these beings able to regard the geometry
of their universe as being plane geometry and their rods withal as the realisation of
“distance”? They cannot do this. For if they attempt to realise a straight line, they will
obtain a curve, which we “three-dimensional beings” designate as a great circle, i.e. a
self-contained line of definite finite length, which can be measured up by means of a
measuring-rod. Similarly, this universe has a finite area that can be compared with the area, of a
square constructed with rods. The great charm resulting from this consideration lies in
the recognition of the fact that the universe of these beings is finite and yet has no
limits.
But the spherical-surface beings do not need to go on a world-tour in order to perceive that
they are not living in a Euclidean universe. They can convince themselves of this on
every part of their “world,” provided they do not use too small a piece of it. Starting
from a point, they draw “straight lines” (arcs of circles as judged in three dimensional
space) of equal length in all directions. They will call the line joining the free ends of
these lines a “circle.” For a plane surface, the ratio of the circumference of a circle to its
diameter, both lengths being measured with the same rod, is, according to Euclidean
geometry of the plane, equal to a constant value π, which is independent of the diameter
of the circle. On their spherical surface our flat beings would find for this ratio the
value

i.e. a smaller value than π, the difference being the more considerable, the greater is the radius of
the circle in comparison with the radius R of the “world-sphere.” By means of this relation the
spherical beings can determine the radius of their universe (“world”), even when only a relatively
small part of their worldsphere is available for their measurements. But if this part is very small
indeed, they will no longer be able to demonstrate that they are on a spherical “world” and not on
a Euclidean plane, for a small part of a spherical surface differs only slightly from a piece of a plane
of the same size.
Thus if the spherical surface beings are living on a planet of which the solar system
occupies only a negligibly small part of the spherical universe, they have no means
of determining whether they are living in a finite or in an infinite universe, because
the “piece of universe” to which they have access is in both cases practically plane,
or Euclidean. It follows directly from this discussion, that for our sphere-beings the
circumference of a circle first increases with the radius until the “circumference of the
universe” is reached, and that it thenceforward gradually decreases to zero for still further
increasing values of the radius. During this process the area of the circle continues to
increase more and more, until finally it becomes equal to the total area of the whole
“world-sphere.”
Perhaps the reader will wonder why we have placed our “beings “on a sphere rather than on
another closed surface. But this choice has its justification in the fact that, of all closed surfaces,
the sphere is unique in possessing the property that all points on it are equivalent. I admit that the
ratio of the circumference c of a circle to its radius r depends on r, but for a given value of r it is
the same for all points of the “worldsphere”; in other words, the “ world-sphere” is a “surface of
constant curvature.”
To this two-dimensional sphere-universe there is a three-dimensional analogy, namely,
the three-dimensional spherical space which was discovered by Riemann. its points are
likewise all equivalent. It possesses a finite volume, which is determined by its “radius”
(2π2R3). Is it possible to imagine a spherical space? To imagine a space means nothing else
than that we imagine an epitome of our “space” experience, i.e. of experience that we
can have in the movement of “rigid” bodies. In this sense we can imagine a spherical
space.
Suppose we draw lines or stretch strings in all directions from a point, and mark off from each of
these the distance r with a measuring-rod. All the free end-points of these lengths lie on a spherical
surface. We can specially measure up the area (F) of this surface by means of a square made
up of measuring-rods. If the universe is Euclidean, then F = 4πR2; if it is spherical,
then F is always less than 4πR2. With increasing values of r, F increases from zero up
to a maximum value which is determined by the “world-radius,” but for still further
increasing values of r, the area gradually diminishes to zero. At first, the straight lines which
radiate from the starting point diverge farther and farther from one another, but later
they approach each other, and finally they run together again at a “counter-point”
to the starting point. Under such conditions they have traversed the whole spherical
space. It is easily seen that the three-dimensional spherical space is quite analogous to
the two-dimensional spherical surface. It is finite (i.e. of finite volume), and has no
bounds.
It may be mentioned that there is yet another kind of curved space: “elliptical space.” It can be
regarded as a curved space in which the two “counter-points” are identical (indistinguishable from
each other). An elliptical universe can thus be considered to some extent as a curved universe
possessing central symmetry.
It follows from what has been said, that closed spaces without limits are conceivable. From
amongst these, the spherical space (and the elliptical) excels in its simplicity, since all points on it
are equivalent. As a result of this discussion, a most interesting question arises for astronomers and
physicists, and that is whether the universe in which we live is infinite, or whether it is finite in the
manner of the spherical universe. Our experience is far from being sufficient to enable us to answer
this question. But the general theory of relativity permits of our answering it with a moduate
degree of certainty, and in this connection the difficulty mentioned in Section 30 finds its
solution.
0.2 References
This article is derived from the Einstein Reference Archive (marxists.org) 1999, 2002. Einstein
Reference Archive which is under the FDL copyright.