But the astronomers were able to detect them by using a natural zoom lens in space, produced by the gravity of Abell 1689, a giant
foreground galaxy cluster.
Acting as a «natural telescope» in space, the gravity of the extremely massive
foreground galaxy cluster MACS J2129 - 0741 magnifies, brightens, and distorts the far - distant background galaxy MACS2129 - 1, shown in the top box.
Foreground galaxy clusters can warp and magnify the light of distant, background proto - galaxies, for instance, allowing cosmologists to catch glimpses of early epochs of the universe.
Not exact matches
In the end success was secured by the fact that the stone - dead
galaxy was positioned behind a
foreground cluster of other
galaxies — a
cluster which functioned as a «natural lens» by amplifying as well as enlarging the image of MACS2129 - 1.
However, through the phenomenon known as «gravitational lensing,» a massive,
foreground cluster of
galaxies acts as a natural «zoom lens» in space by magnifying and stretching images of far more distant background
galaxies.
Countless
galaxies vie for attention in this dazzling image of the Fornax
Cluster, some appearing only as pinpricks of light while others dominate the
foreground.
The highest peaks in the maps correspond the
foreground massive
clusters of
galaxies that lie 5 billion light - years away.
At these wavelengths, the
foreground cluster becomes nearly transparent, enabling the background
galaxy to be more clearly seen.
Except for a few blue,
foreground stars, these myriad stars are members of the Milky Way nuclear star
cluster, the most massive and densest stellar
cluster in the
galaxy.
Except for a few blue,
foreground stars, the stars are part of the Milky Way's nuclear star
cluster, the most massive and densest star
cluster in our
galaxy.
This «gravitational lens» magnifies
galaxies behind the
cluster, making them appear far brighter than they would if the
foreground cluster of
galaxies were not there.
Some of these
galaxies may be
foreground or background
galaxies in the vicinity of the
cluster.
It is impossible to get a good photograph of the entire
cluster because the
galaxies are faint objects scattered across 15 degrees of the sky, and a large angle photograph would be swamped by thousands of
foreground stars in our own
galaxy.
A massive
galaxy cluster called SPT - CL J0615 - 5746 sits in the
foreground of the newly discovered SPT0615 - JD.