Gamma-ray
bursts (GRBs) that make up the newly discovered ring were observed using a
variety of space- and ground-based observatories. They appear to be at very
similar distances from us -- around 7 billion light years -- in a circle 36°
across on the sky, or more than 70 times the diameter of the Full Moon. This
implies that the ring is more than 5 billion light years across, and according
to Prof Balazs there is only a 1 in 20,000 probability of the GRBs being in
this distribution by chance.
Most current models
indicate that the structure of the cosmos is uniform on the largest scales.
This 'Cosmological Principle' is backed up by observations of the early
universe and its microwave background signature, seen by the WMAP and Planck
satellites. Other recent results and this new discovery challenge the
principle, which sets a theoretical limit of 1.2 billion light years for the
largest structures. The newly discovered ring is almost five times as large.
If the ring represents a
real spatial structure, then it has to be seen nearly face-on because of the
small variations of GRB distances around the object's centre. The ring could
though instead be a projection of a sphere, where the GRBs all occurred within
a 250 million year period, a short timescale compared with the age of the
universe.
A spheroidal ring
projection would mirror the strings of clusters of galaxies seen to surround
voids in the universe; voids and string-like formations are seen and predicted
by many models of the cosmos. The newly discovered ring is however at least ten
times larger than known voids.
Prof Balazs comments:
"If we are right, this structure contradicts the current models of the
universe. It was a huge surprise to find something this big -- and we still
don't quite understand how it came to exist at all."
The team now want to find
out more about the ring, and establish whether the known processes for galaxy
formation and large scale structure could have led to its creation, or if
astronomers need to radically revise their theories of the evolution of the cosmos.
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