Astrophysicists investigate whether the universe has a finite and connected shape.

Andrew Jaffe, professor of cosmology and astrophysics at Imperial College London, emphasized that a spacecraft could return to its original location without returning to the same moment; returning to both the original place and time would constitute a “closed timeline curve,” or time machine.
In mathematical terms, cosmic topology concerns the possible existence and properties of “unshrinkable closed loops”—paths that cannot be contracted to a point and could lead back to a traveler’s starting location after a sufficiently long journey.
The cosmic microwave background provides a particularly valuable test because it is the oldest light currently observable: it last interacted with matter roughly 380,000 years after the Big Bang.
Cosmologists have studied the cosmic microwave background since the 1960s, while advances beginning in the early 2000s enabled more detailed searches for large-scale topological signatures.
Astrophysicists are hunting for evidence that the universe might be finite and connected rather than flat and infinite in all directions. Phys.org reports that astronomers have spent decades searching for subtle patterns in ancient light and the large-scale structure of matter that could reveal whether the cosmos loops back on itself. If the universe does have this kind of topology, a spacecraft traveling far enough in one direction could theoretically return to its starting point—though not necessarily at the same time.
A crucial distinction matters in cosmic topology. Phys.org notes that Andrew Jaffe, a cosmology professor at Imperial College London, explains that a spacecraft could return to its original location without arriving at the same moment in time. Returning to both the exact place and exact time would require what physicists call a "closed timelike curve"—essentially a time machine, which remains purely theoretical.
Cosmic topology in mathematical terms means studying "unshrinkable closed loops"—paths that cannot be shrunk down to a single point. Phys.org explains these loops could theoretically lead travelers back to their starting location after journeying far enough through space. This idea stands in contrast to the current mainstream view: that the universe is flat and extends infinitely in every direction with no loops or connections.
The cosmic microwave background—the oldest light we can observe—offers astronomers their best test for topological signatures. Phys.org reports this ancient light last touched matter about 380,000 years after the Big Bang. If the universe loops back on itself, patterns in this ancient light should show repeating or unusual alignments that betray the universe's true shape.
Astronomers began studying the cosmic microwave background systematically in the 1960s. Phys.org notes that major advances started in the early 2000s, giving researchers much more detailed tools to search for large-scale topological signatures hidden in the data. Despite these efforts, current observations still broadly support the flat-universe model, though the hunt for alternative cosmic shapes continues.
Publishers
10
Articles
3
Reach
13