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Hubble captures a dusty nursery where new baby stars are being born

Image from the NASA/ESA Hubble Space Telescope features AFGL 5180, a beautiful stellar nursery located in the constellation of Gemini.
Nestled among the vast clouds of star-forming regions like this one lie potential clues about the formation of our own solar system. This image from the NASA/ESA Hubble Space Telescope features AFGL 5180, a beautiful stellar nursery located in the constellation of Gemini (the Twins). ESA/Hubble & NASA, J. C. Tan (Chalmers University & University of Virginia), R. Fedriani (Chalmers University); Acknowledgment: Judy Schmidt

Although it recently had a scare with some faulty computer hardware, the Hubble Space Telescope is now back up and running with its normal science operations. That means we can look forward to many more breathtaking images of space captured by this venerable telescope, like the one above recently shared by NASA.

This image shows the nebula AFGL 5180, a cloud of dust located in the constellation of Gemini (the Twins), which acts as the birthplace for new stars. A huge star is being born in the center of this image, sending out jets that disrupt the dust and gas above and below it.

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Stars are born when clouds of dust like this one begin to form clumps. As more dust and gas are attracted to the clumps due to gravity, they begin to grow. Eventually, the clumps grow so large and dense that they collapse into stars. From start to finish, for a star to develop from a cloud of dust to a shining beacon, like our sun, the process takes around one million years.

Regions of relatively thick dust are essential for star formation, like this nebula. However, the dust that powers the birth of stars can be a problem for astronomers here on Earth. “Stars are born in dusty environments, and although this dust makes for spectacular images, it can prevent astronomers from seeing stars embedded in it,” Hubble scientists write. “Hubble’s Wide Field Camera 3 (WFC3) instrument is designed to capture detailed images in both visible and infrared light, meaning that the young stars hidden in vast star-forming regions like AFGL 5180 can be seen much more clearly.”

Using infrared allows astronomers to peer through the dusty veil and see what lies beneath. A similar approach has been used to peer through the clouds of Jupiter in our solar system or to see the movement of gas at the center of our galaxy.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
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

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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.

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Hubble spots a bright galaxy peering out from behind a dark nebula
The subject of this image taken with the NASA/ESA Hubble Space Telescope is the spiral galaxy IC 4633, located 100 million light-years away from us in the constellation Apus. IC 4633 is a galaxy rich in star-forming activity and also hosts an active galactic nucleus at its core. From our point of view, the galaxy is tilted mostly towards us, giving astronomers a fairly good view of its billions of stars.

A new image from the Hubble Space Telescope shows a galaxy partly hidden by a huge cloud of dust known as a dark nebula. The galaxy IC 4633 still shines brightly and beautifully in the main part of the image, but to the bottom right, you can see dark smudges of dust that are blocking the light from this part of the galaxy.

Taken using Hubble's Advanced Camera for Surveys (ACS) instrument, the image also incorporates data from the DECam instrument on the Víctor M. Blanco 4-meter Telescope, which is located in Chile. By bringing together data from the space-based Hubble and the ground-based DECam, astronomers can get a better look at this galaxy, located 100 million light-years away, and the dark dust partially obscuring it.

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