Skip to main content

A baby star’s energetic outburst captured by Hubble

This week’s image from the Hubble Space Telescope shows the dramatic and energetic jets given off by a young star, forming a wispy structure called a Herbig-Haro object. The image shows object HH34, located 1,250 light-years away in the Orion Nebula. The Orion Nebula is a site of active star formation and as it is bright enough to be seen even by the naked eye, it is often studied to learn about the formation of stars.

A Herbig-Haro object is formed when a young, particularly energetic star ejects particles of ionized gas in epic jets. These jets typically eject from opposite sides of the star, illuminating gas and dust around them which glows in beautiful colors. These jets are so powerful they can travel at hundreds of miles per second, meaning they spread far beyond the star and form these long, thin shapes which can be seen from great distances.

An energetic outburst from an infant star streaks across this image from the NASA/ESA Hubble Space Telescope.
An energetic outburst from an infant star streaks across this image from the NASA/ESA Hubble Space Telescope. This stellar tantrum – produced by an extremely young star in the earliest phase of formation – consists of an incandescent jet of gas traveling at supersonic speeds. As the jet collides with material surrounding the still-forming star, the shock heats this material and causes it to glow. ESA/Hubble & NASA, B. Nisini

These objects can change rapidly over short periods of time as well, just as this one has done. “Herbig–Haro objects are seen to evolve and change significantly over just a few years,” Hubble scientists write. “This particular object, called HH34, was previously captured by Hubble between 1994 and 2007, and again in glorious detail in 2015.”

If you look at the previous image of HH34, captured in 2015, you can see how the object has changed in the handful of years since then. Most astronomical objects like stars tend to change over periods of thousands of years or more, so to see an object changing so rapidly is a rarity.

By looking at objects like HH34 astronomers can learn about the formation of stars and the jets of energy they can give off. This topic will be studied in more depth using the James Webb Space Telescope, which is able to look through the clouds of dust surrounding newly-born stars using its infrared instruments, to observe the newborns up close.

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
See what James Webb and Hubble are observing right now with this tool
james webb hubble live tracker screenshot 2024 03 06 220259

If you're looking for a relaxing way to peruse the fascinating sights of space on your lunch break, then a newly updated tool from NASA has you covered. The Space Telescope Live tools show the current targets of the James Webb Space Telescope and the Hubble Space Telescope, letting you browse the cosmos from the perspective of two of the hardest-working telescopes out there.

You can visit the web-based tools at WebbTelescope for the James Webb Space Telescope and HubbleSite for the Hubble Space Telescope. Clicking on a link will bring you to a portal showing the current and past observations of the telescope and a ton of detail about the observations.

Read more
Hubble spots a massive star forming amid clouds of dust and gas
This image from the NASA/ESA Hubble Space Telescope is a relatively close star-forming region known as IRAS 16562-3959.

A stunning new image from the Hubble Space Telescope shows the birth of a new, massive star at around 30 times the mass of our sun. Nestled with a nearby star-forming region called IRAS 16562-3959, the baby star is located within our galaxy and around 5,900 light-years from Earth.

You can see the sparkle of bright stars throughout the image, with the star-forming region visible as the orange-colored clouds of dust and gas stretching diagonally across the frame. These clouds are where dust and gas clump together to form knots, gradually attracting more dust and gas, growing over time to become protostars.

Read more
Hubble spies baby stars being born amid chaos of interacting galaxies
Galaxy AM 1054-325 has been distorted into an S-shape from a normal pancake-like spiral shape by the gravitational pull of a neighboring galaxy, seen in this Hubble Space Telescope image. A consequence of this is that newborn clusters of stars form along a stretched-out tidal tail for thousands of light-years, resembling a string of pearls. They form when knots of gas gravitationally collapse to create about 1 million newborn stars per cluster.

When two galaxies collide, the results can be destructive, with one of the galaxies ending up ripped apart, but it can also be constructive too. In the swirling masses of gas and dust pulled around by the gravitational forces of interacting galaxies, there can be bursts of star formation, creating new generations of stars. The Hubble Space Telescope recently captured one such hotbed of star formation in galaxy AM 1054-325, which has been distorted into an unusual shape due to the gravitational tugging of a nearby galaxy.

Galaxy AM 1054-325 has been distorted into an S-shape from a normal pancake-like spiral shape by the gravitational pull of a neighboring galaxy, as seen in this Hubble Space Telescope image. A consequence of this is that newborn clusters of stars form along a stretched-out tidal tail for thousands of light-years, resembling a string of pearls. NASA, ESA, STScI, Jayanne English (University of Manitoba)

Read more