Skip to main content

Thousands of stars sparkle in this week’s Hubble image

A sky full of stars is on glorious display in this week’s image from the Hubble Space Telescope. The image shows a structure called a globular cluster, which is an enormous collection of tens of thousands or even millions of stars, tightly bound by gravity and densely packed together.

This particular globular cluster is called NGC 6638 and is located in the constellation of Sagittarius. It was taken using two of Hubble’s instruments, the Wide Field Camera 3 and the Advanced Camera for Surveys, which operate primarily in the visible light wavelength.

This star-studded image from the NASA/ESA Hubble Space Telescope shows the heart of the globular cluster NGC 6638 in the constellation Sagittarius. The star-strewn observation highlights the density of stars at the heart of globular clusters, which are stable, tightly bound clusters of tens of thousands to millions of stars. To capture the data in this image, Hubble used two of its cutting-edge astronomical instruments: Wide Field Camera 3 and the Advanced Camera for Surveys.
The heart of the globular cluster NGC 6638 in the constellation Sagittarius. ESA/Hubble & NASA, R. Cohen

These astonishing objects were difficult to study before Hubble was launched, as to be able to see each star as distinct from the rest requires very high-resolution imaging with little interference.

Recommended Videos

“Hubble revolutionized the study of globular clusters, as it is almost impossible to clearly distinguish the stars in globular clusters with ground-based telescopes,” Hubble scientists explain. “The blurring caused by Earth’s atmosphere makes it impossible to tell one star from another, but from Hubble’s location in low Earth orbit the atmosphere no longer poses a problem. As a result, Hubble has been used to study what kind of stars globular clusters are made up of, how they evolve, and the role of gravity in these dense systems.”

Globular clusters will soon be studied with another tool as well, as one such cluster called Messier 92 is the target of an early science program using the James Webb Space Telescope. The project will study star-forming regions using Webb’s NIRCam and NIRISS instruments, which look in the infrared range as opposed to Hubble’s predominantly visible-light observations.

According to lead researcher Daniel Wiesz, who spoke to Inverse about the project, Messier 92 holds some extremely ancient stars and the team is working on special imaging software to resolve individual stars within a densely packed area.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
Hubble catches a baby star pulsating in a triple star system
This NASA Hubble Space Telescope image captures a triple-star star system.

This NASA Hubble Space Telescope image shows a triple-star star system. NASA, ESA, G. Duchene (Universite de Grenoble I); Image Processing: Gladys Kober (NASA/Catholic University of America)

A gorgeous new image from the Hubble Space Telescope shows a triple star system, where three stars are working in tandem to create a reflection nebula. The trio of stars are located 550 light-years away, and include one particular star, HP Tau, that is like a younger version of our sun and will eventually grow up to be a similar hydrogen-fueled star in millions of years' time.

Read more
Celebrate Hubble’s 34th birthday with this gorgeous nebula image
In celebration of the 34th anniversary of the launch of NASA’s legendary Hubble Space Telescope, astronomers took a snapshot of the Little Dumbbell Nebula, also known as Messier 76, or M76, located 3,400 light-years away in the northern circumpolar constellation Perseus. The name 'Little Dumbbell' comes from its shape that is a two-lobed structure of colorful, mottled, glowing gases resembling a balloon that’s been pinched around a middle waist. Like an inflating balloon, the lobes are expanding into space from a dying star seen as a white dot in the center. Blistering ultraviolet radiation from the super-hot star is causing the gases to glow. The red color is from nitrogen, and blue is from oxygen.

Tomorrow, April 24, marks the 34th anniversary of the launch of the Hubble Space Telescope. For more than three decades, this venerable old telescope has been peering out into space, observing stars, galaxies, and nebulae to understand more about the universe we live in. To celebrate this birthday, Hubble scientists have shared a new image showing the striking Little Dumbbell Nebula, also known as Messier 76, which is located 3,400 light-years away.

In celebration of the 34th anniversary of the launch of NASA’s legendary Hubble Space Telescope, astronomers took a snapshot of the Little Dumbbell Nebula, also known as Messier 76, or M76, located 3,400 light-years away in the northern circumpolar constellation Perseus. NASA, ESA, STScI

Read more
Hubble discovers over 1,000 new asteroids thanks to photobombing
This NASA/ESA Hubble Space Telescope image of the barred spiral galaxy UGC 12158 looks like someone took a white marking pen to it. In reality it is a combination of time exposures of a foreground asteroid moving through Hubble’s field of view, photobombing the observation of the galaxy. Several exposures of the galaxy were taken, which is evidenced by the dashed pattern.

The Hubble Space Telescope is most famous for taking images of far-off galaxies, but it is also useful for studying objects right here in our own solar system. Recently, researchers have gotten creative and found a way to use Hubble data to detect previously unknown asteroids that are mostly located in the main asteroid belt between Mars and Jupiter.

The researchers discovered an incredible 1,031 new asteroids, many of them small and difficult to detect with several hundred of them less than a kilometer in size. To identify the asteroids, the researchers combed through a total of 37,000 Hubble images taken over a 19-year time period, identifying the tell-tale trail of asteroids zipping past Hubble's camera.

Read more