Skip to main content

The Tarantula Nebula glows brightly in this week’s Hubble image

The Hubble Space Telescope continues to capture gorgeous views of space objects thst are shared every week, the most recent of which shows a beautiful nebula.

This week’s target is the Tarantula Nebula, technically known as 30 Doradus. Located over 160,000 light-years away in a satellite galaxy of the Milky Way called the Large Magellanic Cloud, this huge cloud of dust is exceptionally bright and is one of the busiest areas of star formation in nearby space. As new stars are born, they give off radiation that ionizes the hydrogen atoms around them, making the cloud of gas glow brightly.

A snapshot of the Tarantula Nebula (also known as 30 Doradus) is featured in this image from the NASA/ESA Hubble Space Telescope. The Tarantula Nebula is a large star-forming region of ionized hydrogen gas that lies 161,000 light-years from Earth in the Large Magellanic Cloud, and its turbulent clouds of gas and dust appear to swirl between the region’s bright, newly formed stars.
A snapshot of the Tarantula Nebula (also known as 30 Doradus) is featured in this image from the NASA/European Space Agency Hubble Space Telescope. The Tarantula Nebula is a large star-forming region of ionized hydrogen gas that lies 161,000 light-years from Earth in the Large Magellanic Cloud, and its turbulent clouds of gas and dust appear to swirl between the region’s bright, newly formed stars. ESA/Hubble & NASA, C. Murray, E. Sabbi; Acknowledgment: Y. -H. Chu

The Tarantula Nebula is not only famous for being a region of star formation. It is also a popular target for public outreach, and it has been imaged by many different famous telescopes. Last year, the James Webb Space Telescope captured its own stunning view of the nebula, and before that it was also chosen as a target for a final goodbye image from the now-retired Spitzer Space Telescope. It has also been imaged by Hubble previously, when a section of the nebula was imaged in order to study the formation of massive stars.

Recommended Videos

Both Webb and Spitzer look primarily in the infrared wavelength, which allows them to see through clouds of dust and pick out the structure of the nebula more clearly. This Hubble image, on the other hand, is taken in the visible light wavelength, which is equivalent to what the human eye would see.

Please enable Javascript to view this content

That’s why Hubble images tend to have a more pastel color palette and infrared images tend to be more saturated, because visible light is only a small slice of the electromagnetic spectrum and therefore picks up subtle variations. Infrared covers a broader swath of the spectrum, and picks out a wide range of physical processes — so when it’s translated into a visible light image, there’s high variation that equates to a wider range of colors.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
This beautiful nebula holds a starry mystery at its heart
This image, taken with the VLT Survey Telescope hosted at ESO’s Paranal Observatory, shows the beautiful nebula NGC 6164/6165, also known as the Dragon’s Egg. The nebula is a cloud of gas and dust surrounding a pair of stars called HD 148937.

A gorgeous nebula turns out to hold a surprise at its center: a pair of stars that don't match as they should. Researchers looking at the beautiful NGC 6164/6165 nebula were surprised to learn that one of the pair of stars it hosts appears to be much older than the other, giving clues to the dramatic situation in which the nebula was born.

Pairs of stars aren't unusual in nebulae, but they are typically very similar. Normally, you would expect a pair to be similar in terms of age and mass, as they would have formed around the same time. But in this nebula, located 3,800 light-years away, one member of the pair is 1.5 million years older than the other, and the younger star is also magnetic, unlike its older counterpart.

Read more
Hubble captures the dramatic jets of a baby star
FS Tau is a multi-star system made up of FS Tau A, the bright star-like object near the middle of the image, and FS Tau B (Haro 6-5B), the bright object to the far right that is partially obscured by a dark, vertical lane of dust. The young objects are surrounded by softly illuminated gas and dust of this stellar nursery. The system is only about 2.8 million years old, very young for a star system. Our Sun, by contrast, is about 4.6 billion years old.

A new image from the Hubble Space Telescope shows the drama that unfolds as a new star is born. Within a swirling cloud of dust and gas, a newly formed star is giving off powerful jets that blast away material and cut through the nearby dust of the surrounding nebula to create this stunning vista.

The image shows a system called FS Tau, located 450 light-years away in a region called Taurus-Auriga. Within this region are many stellar nurseries with new stars forming, making it a favorite target for astronomers studying star formation. But this particular system stands out for the dramatic nature of its newborn star, which has formed an epic structure called a Herbig-Haro object.

Read more
Hubble images the spooky Spider Galaxy
This image from the NASA/ESA Hubble Space Telescope shows the irregular galaxy UGC 5829.

This week's image from the Hubble Space Telescope shows an irregular galaxy, the spindly arms and clawed shape of which has led to it being named the Spider Galaxy. Located 30 million light-years away, the galaxy also known as UGC 5829 is an irregular galaxy that lacks the clear, orderly arms seen in spiral galaxies like the Milky Way.

This image from the NASA/ESA Hubble Space Telescope shows the irregular galaxy UGC 5829. ESA/Hubble & NASA, R. Tully, M. Messa

Read more