A strange virgo Galaxy spinning in a way which defies expectations
A new Hubble Space Telescope image reveals the unusual structure and mysterious rotation of the spiral galaxy NGC 4698. Image revealed that the spiral galaxy NGC 4698 hides a strange internal arrangement, with its central region rotating in a different direction from the rest of the galaxy. The discovery, presented by ESA, offers astronomers a closer look at how galaxies can be shaped by interactions and events which happened billions of years ago. Though the spiral galaxy in the new image by the NASA/ESA Hubble Space Telescope seems serene, it hides a chaotic secret. This galaxy is NGC 4698, and it lies about 55 million light-years away in the constellation Virgo. It’s one of over one thousand galaxies in the Virgo Cluster, the nearest large cluster of galaxies bound together by gravity. As a spiral galaxy similar to our own Milky Way galaxy, NGC 4698 has spiral arms which curl around within a thin disc of stars, gas and dust. Its centre is dominated by a galactic bulge.
The spiral galaxy NGC 4698 is spinning out of sync because the stars and gas near its center rotate perpendicular (at a right angle) to the rest of its stellar disc. It belongs to the massive Virgo Cluster, which contains over a thousand galaxies. It features a central stellar bulge which extends outward from the main disc at an unusual right angle. Astronomers believe the strange rotation comes from external sources. The galaxy may have pulled in gas from an outside location, forming a new inner disc tilted against the original rotation. Evidence like a faint tail of hydrogen gas near the galaxy suggests it went through a minor collision or merger with a smaller galaxy in its past. The diffuse off-white glow of the galaxy’s bulge comes from stars smaller, older, and cooler than the massive blue stars which dot the galaxy’s outer disc. These tightly packed stars orbit a supermassive black hole containing millions of times the Sun’s mass. Scientists have found signs that this black hole is actively growing, drawing gas inward with its gravitational pull.
NGC 4698 appears at first glance to be a typical spiral galaxy with elegant arms surrounding a bright center. Yet beneath this calm appearance lies a complex structure that separates it from most known spiral galaxies. Its central bulge extends at an unusual angle compared with the galaxy’s main disk, creating a rare example of a galaxy whose components are not aligned. The ESA release explains that NGC 4698 is a spiral galaxy which looks familiar from a distance but contains a hidden complexity. Its unusual rotation pattern and tilted central bulge provide clues about interactions that may have occurred in the distant past. With a flat, starry disc and diffusely glowing centre, NGC 4698 looks a lot like a typical spiral galaxy, but this galaxy is far from normal. NGC 4698 is one of only a few known spiral galaxies with a bulge that extends out from the disc at a right angle. The elongation is faintly visible in the Hubble image, which shows the ghostly glow of the starry bulge peeking above and below the dusty disc. Astronomers believe that material from outside the galaxy may have played a role in creating this unusual arrangement. If NGC 4698 captured gas from another source, that material could have formed a new disk of gas and stars around the center at a different angle from the original galactic disk. The galaxy also shows possible signs of a previous minor merger. Observations have detected a short stream of hydrogen extending from one side of the galaxy, which could be evidence that another galaxy interaction influenced its current shape.
Astronomers have found that the culprit likely lies outside the galaxy. If NGC 4698 funneled in gas from an outside source, the newly collected gas could have formed a disc of gas and stars in the galaxy’s centre. Some observations suggest that this galaxy once experienced a minor galactic merger, as evidenced by a short ‘tail’ of hydrogen streaming from one side of the galaxy. The data used to create this image come from an observing programme (#18103; PI: Thilker) focusing on galaxies in the Virgo Cluster. The spiral galaxy NGC 4698 have a massive collection of more than one thousand galaxies held together by gravity. Like the Milky Way, it contains a thin disk made of stars, ga, and dust, along with a dense central bulge filled with older stars. The outer disk contains areas where younger, hotter stars shine with blue tones, while the central bulge produces a softer off-white glow created by older and cooler stars. This contrast reveals the different populations of stars that exist within the galaxy. What makes NGC 4698 unusual is the position of its bulge. Instead of extending along the same plane as the disk, the central structure appears tilted at nearly a right angle. Astronomers have identified only a small number of spiral galaxies with this type of configuration.
The inner stars and gas near the galaxy’s center also rotate differently from the material farther out. This mismatch indicates that the galaxy’s history involved processes capable of disturbing its original structure while allowing it to maintain its spiral appearance. Prominent red-brown dust lanes weave through the arms, which are also dotted with bright blue and reddish regions of star formation. The galaxy is set against a dark background scattered with stars and faint distant galaxies. At the center of NGC 4698 lies a supermassive black hole containing millions of times the mass of the Sun. The dense population of older stars in the bulge surrounds this powerful object, creating the bright central region visible in the Hubble image. Researchers have found indications that this black hole is actively growing by pulling gas inward through its intense gravitational field. The movement of material around the center provides scientists with information about both the black hole and the galaxy hosting it. The relationship between a galaxy and its central black hole remains one of the major areas of study in modern astronomy. Many galaxies appear to have developed alongside their central black holes, with each influencing the evolution of the other over cosmic timescales. In NGC 4698, the unusual orientation of the central region creates an opportunity to examine how black holes, gas flows, and galaxy interactions can combine to shape a galaxy’s future.
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.png)


.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.png)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)

.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)
.jpg)