A Figure-Eight in Deep Space: Hubble Image Shows Gravity Warping Distant Galaxies

A cosmic swarm

The image, released June 12, 2026, shows what NASA described as looking “somewhat like a swarm of bees returning to their hive.” The cluster is packed with galaxies bound together by gravity.

MACS0329-0211 contains large elliptical galaxies, thin edge-on spiral and lenticular galaxies, and face-on spirals with visible arms. Together, they form one of the universe’s largest gravitationally bound structures.

Gravity as a telescope

Galaxy clusters are not just collections of stars and gas. Their enormous mass bends space-time, allowing them to act as natural telescopes through gravitational lensing.

In the Hubble image, faint arcs appear in the upper-right quadrant. Those arcs are distant background galaxies whose light has been stretched and magnified by the cluster’s gravity.

Near the center, bright white intersecting curves form a distorted figure-eight shape. NASA said this may be another distant galaxy whose light was magnified and distorted by the massive cluster.

Einstein in action

Gravitational lensing is a visible confirmation of Einstein’s General Theory of Relativity. Massive objects curve space-time, and light follows that curved geometry rather than traveling in a perfectly straight line.

When alignment is especially strong, lensing can produce giant arcs, multiple images of the same galaxy, or Einstein rings. In weaker cases, astronomers use subtle distortions to map dark matter across large regions of space.

Why MACS0329-0211 matters

MACS0329-0211 sits at a redshift of about 0.4503, meaning its light left when the universe was roughly 8 billion to 9 billion years old. Its look-back time is about 5 billion years.

NASA Hubble Space Telescope image showcasing the galaxy cluster MACS0329-0211. NASA, ESA, M. Postman (STScI); Image Processing: G. Kober (NASA/Catholic University of America)

A 2024 kinematic study using Very Large Telescope spectroscopy estimated the cluster’s mass at about 9.2 × 10^14 solar masses within a radius of about 1.71 megaparsecs, or roughly 5.6 million light-years across.

The cluster was observed as part of a program studying X-ray bright galaxy clusters. Hubble used the Advanced Camera for Surveys and Wide Field Camera 3 to collect visible and infrared data.

A window into structure formation

Galaxy clusters are signposts for how the universe’s large-scale structure formed over billions of years. They also help researchers study dark matter, galaxy evolution and the assembly of massive cosmic systems.

MACS0329-0211 appears relatively relaxed overall, but studies indicate it sits in a rich environment with nearby galaxy groups and evidence of recent infall. Its brightest cluster galaxy also shows active star formation, ultraviolet emission and radio emission.

For astronomers, the value of the image extends beyond its visual drama. It captures cluster galaxies from one era of cosmic history while using gravity to reveal still more distant galaxies from earlier times.