Skip to main content

Hubble captures a globular cluster of densely packed stars

The Hubble Space Telescope team has released another stunning space image captured by the instrument — this one of a globular cluster called NGC 1805. A globular cluster is an enormous collection of thousands of stars that are close together and bound in a spherical shape by the forces of gravity.

The stars in NGC 1805 are packed so closely that they are unlikely to have any planetary systems. They are 100 to 1,000 times closer to each other than our sun is to other stars.

Many colorful stars are packed close together in this image of the globular cluster NGC 1805, taken by the NASA/ESA Hubble Space Telescope.
Many colorful stars are packed close together in this image of the globular cluster NGC 1805 taken by the NASA/European Space Agency Hubble Space Telescope. ESA/Hubble & NASA, J. Kalirai

This image is an example of Hubble’s capabilities to not only capture light in the optical wavelength, but also in the ultraviolet and infrared wavelengths. As the Hubble scientists explain: “The striking difference in star colors is illustrated beautifully in this image, which combines two different types of light: Blue stars, shining brightest in near-ultraviolet light, and red stars, illuminated in red and near-infrared. Space telescopes like Hubble can observe in the ultraviolet because they are positioned above Earth’s atmosphere, which absorbs most of this wavelength, making it inaccessible to ground-based facilities.”

Recommended Videos

The global cluster shown here is located close to the edge of the Large Magellanic Cloud, one of the closest galaxies to the Milky Way. It is gravitationally bound to our galaxy, so it is known as a satellite galaxy. The region in question is part of the Dorado constellation, named after the Portuguese term for dolphinfish, which can be observed from the Earth’s southern hemisphere.

This particular globular cluster is notable for an unusual feature — it has both older and younger stars within it. “Usually, globular clusters contain stars which are born at the same time,” the Hubble scientists said, “however, NGC 1805 is unusual as it appears to host two different populations of stars with ages millions of years apart. Observing such clusters of stars can help astronomers understand how stars evolve, and what factors determine whether they end their lives as white dwarfs, or explode as supernovae.”

Hubble previously captured another globular cluster, Messier 62, which also has an unusual feature of being exceedingly dense at its center.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Hubble goes hunting for elusive medium-sized black holes
A Hubble Space Telescope image of the globular star cluster, Messier 4. The cluster is a dense collection of several hundred thousand stars. Astronomers suspect that an intermediate-mass black hole, weighing as much as 800 times the mass of our Sun, is lurking, unseen, at its core.

There's something odd about the black holes discovered to date. We've found plenty of smaller black holes, with masses less than 100 times that of the sun, and plenty of huge black holes, with masses millions or even billions of times that of the sun. But we've found hardly any black holes in the intermediate mass range, arguably not enough to confirm that they even exist, and it's not really clear why.

Now, astronomers are using the Hubble Space Telescope to hunt for these missing black holes. Hubble has previously found some evidence of black holes in this intermediate range, and now it is being used to search for examples within a few thousand light-years of Earth.

Read more
Hubble observes weird star system with three off-kilter, planet-forming disks
This illustration is based on Hubble Space Telescope images of gas and dust discs encircling the young star TW Hydrae. We have an oblique view of three concentric rings of dust and gas. At the centre is the bright white glow of the central star. The reddish-coloured rings are inclined to each other and are therefore casting dark shadows across the outermost ring.

Planets form from large disks of dust and gas that collect around their host stars. Billions of years ago, our solar system would have looked like a single point of bright light coming from the sun, with a disk of matter swirling around it that eventually clumped into planets. To learn about how our solar system formed, it's helpful to look at other systems that are currently going through this process -- such as TW Hydrae, a system located 200 light-years away and turned face-on toward us, making it the perfect place to observe planetary formation.

But there's something odd about the TW Hydrae system. In 2017, astronomers first noticed a strange shadow that was visible on the disk of dust and gas surrounding the star. While such shadows are typically from a planet formed within the disk, in this case the shadow's shape and movement suggested it was actually from a second disk, located within the first disk and tilted at a different angle. Now, astronomers think they have spotted evidence of a third disk, with all three stacked up and creating a complex pattern of shadows.

Read more
Hubble celebrates its 33rd birthday with stunning nebula image
Astronomers are celebrating the NASA/ESA Hubble Space Telescope’s 33rd launch anniversary with an ethereal photo of a nearby star-forming region, NGC 1333. The nebula is in the Perseus molecular cloud, and is located approximately 960 light-years away.

It will soon be the 33rd anniversary of the launch of the Hubble Space Telescope, and to celebrate this milestone, Hubble scientists have shared a stunning image taken by the telescope of a picturesque nebula. NGC 1333 is a busy stellar nursery, with new stars forming among the cloud of dust and gas located 960 light-years away.

The beautiful image of the nebula shows swirls of dark dust around glowing points of light where new stars are being born. To capture this scene, Hubble used its instruments across their full wavelengths, from ultraviolet through the optical light range and into the near-infrared. Hubble took the image using its Wide Field Camera 3 instrument, which used several filter across different wavelengths that were then assigned to colors (Blue: F475W, Green: F606W, Red: F657N and F814W) to create the colorful final result.

Read more