NASA's James Webb and Hubble telescopes have combined to create a new image of Messier 64, also known as the Black Eye Galaxy due to its distinctive dark dust band. Located about 17 million light-years away in the constellation Coma Berenices, M64 is unusual because it has gas rotating in opposite directions within different parts of the galaxy, suggesting an ancient merger with a smaller satellite galaxy over a billion years ago. The composite image reveals active star formation where these two gas systems interact, providing insights into the galaxy's complex history and evolution.
Written locally by qwen2.5:14b on 2026-09-19,
using this article's own text rather than the other coverage of the
same event (that is the story summary below).
At first glance, Messier 64 looks like a classic spiral galaxy.
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Messier → look → galaxy
Its bright centre is wrapped in sweeping arms, while a broad, dark band of dust cuts across one side of its nucleus, giving it the distinctive appearance that earned it the nickname Black Eye Galaxy.
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that → wrap → nickname
But beneath that familiar spiral shape lies something much stranger.
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something → lie → shape
Located roughly 17 million light-years from Earth in the constellation Coma Berenices, M64 is known for an unusual internal motion: gas in its outer regions rotates in the opposite direction to the gas and stars closer to the centre.
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gas → locate → centre
NASA says this counter-rotation may be a remnant of a merger involving M64 and a smaller satellite galaxy more than a billion years ago.
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rotation → say → M64
Webb sees what Hubble could not
The new composite image combines observations from the James Webb Space Telescope and Hubble Space Telescope, allowing astronomers to examine M64 across different wavelengths.
Webb’s Mid-Infrared Instrument, or MIRI, is particularly useful for studying the galaxy’s dusty regions.
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Instrument → see → regions
While the dust can appear dark in visible-light observations, infrared wavelengths allow Webb to detect radiation associated with the dust and the young stars embedded within it.
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Webb → appear → it
NASA’s APOD description notes that MIRI reveals the dust in red, while Hubble’s observations show pink regions associated with active star formation.
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observations → note → formation
That difference is important because the dark band that gives M64 its name is not simply an empty, shadowy region.
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that → give → name
It contains material involved in the ongoing process of forming new stars.
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It → contain → stars
Two gas streams moving against each other
The galaxy’s most intriguing feature is its opposing gas motion.
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feature → move → other
The gas closer to M64’s centre rotates in one direction, while gas farther out rotates in the opposite direction.
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gas → rotate → direction
Where these two systems interact, the gas can collide and become compressed.
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gas → interact → ?
That compression helps trigger the collapse of gas clouds, creating conditions favourable for new stars to form.
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stars → help → conditions
This makes M64 something of a cosmic record of its own past.
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M64 → make → past
The opposing motion is thought to have originated when a smaller galaxy interacted with and was eventually absorbed by M64.
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galaxy → oppose → M64
Astronomers have studied this unusual behaviour for decades.
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Astronomers → study → decades
NASA’s earlier Hubble observations found that the outer gas extends much farther from the centre and rotates in the opposite direction, while regions where the gas systems meet show evidence of active star formation.
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systems → find → formation
A merger hidden inside a beautiful spiral
The idea that a spiral galaxy could have undergone such a dramatic merger was significant in the study of M64.
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galaxy → hide → M64
Rather than being a completely settled system, the galaxy preserves traces of an ancient encounter in the movement of its gas.
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galaxy → settle → gas
NASA notes that M64 became important evidence that spiral galaxies can experience mergers, challenging the older assumption that their histories were comparatively peaceful.
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histories → note → assumption
The smaller galaxy involved in the event is no longer an obvious separate object.
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galaxy → involve → event
Instead, evidence of the encounter remains embedded in M64’s unusual gas dynamics.
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evidence → embed → dynamics
Why Webb’s view matters
The new Webb observations are not simply about producing a more detailed-looking photograph.
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observations → matter → photograph
Infrared observations allow astronomers to study the structure, composition and behaviour of dust that is difficult to see in visible wavelengths.
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that → allow → wavelengths
Combined with Hubble’s view, the observations provide a broader picture of how dust and star-forming regions are distributed throughout M64.
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dust → combine → M64
NASA says the Webb data will help researchers better understand the galaxy’s dust and provide additional context for reconstructing its merger history and evolution.
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researchers → say → history
For a galaxy some 17 million light-years away, its appearance may seem frozen in time.
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appearance → seem → time
Yet the Black Eye Galaxy is effectively carrying the evidence of an ancient cosmic collision within it.
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Galaxy → carry → it
What looks like a dark streak across a beautiful spiral is part of a much larger story involving two streams of gas, newly forming stars and a merger that happened more than a billion years ago.
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that → look → gas
The Aporia
