Skip to main content

Hubble images a star throwing out jets of gas in a rare phenomenon

The image from the Hubble Space Telescope shared by NASA this week is a striking pair of jets spraying outward from a newly born star, formed when an unusually active star throws off streams of ionized gas. This strange-looking cosmic phenomenon is a rare sight called a Herbig-Haro object, in this case, designated HH111.

“These spectacular objects develop under very specific circumstances,” Hubble scientists write. “Newly formed stars are often very active, and in some cases they expel very narrow jets of rapidly moving ionized gas — gas that is so hot that its molecules and atoms have lost their electrons, making the gas highly charged. The streams of ionized gas then collide with the clouds of gas and dust surrounding newly formed stars at speeds of hundreds of miles per second. It is these energetic collisions that create Herbig-Haro objects such as HH111.”

A striking image from the Hubble Space Telescope featuring a relatively rare celestial phenomenon known as a Herbig-Haro object.
This striking image features a relatively rare celestial phenomenon known as a Herbig-Haro object. This particular object, named HH111, was imaged by the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 (WFC3). ESA/Hubble & NASA, B. Nisini

Hubble has previously imaged an even rarer sight, which is a pair of Herbig-Haro objects located in the constellation of Vela (the Sails). Those two objects were instrumental in astronomers understanding what these objects were for the first time, as they were previously thought to be emission nebulae. The new class of objects was named for the first two astronomers to study them in depth, George Herbig and Guillermo Haro.

Recommended Videos

To capture the image above, Hubble used its Wide Field Camera 3 (WFC3). It is difficult to image Herbig-Haro objects because even though they give out a lot of light in the visible wavelength, much of this is absorbed by the dust and gas surrounding them. So to image the object, the WFC3 looked in the infrared wavelength, in which the object still shines, but the light is no longer blocked by dust.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
A sparkling field of stars cluster together in Hubble image
This image shows just a portion of M55, the cluster as a whole appears spherical because the stars’ intense gravitational attraction pulls them together. Hubble’s clear view above Earth’s atmosphere resolves individual stars in this cluster. Ground-based telescopes can also resolve individual stars in M55, but fewer stars are visible.

A sea of stars sparkles in this image from the Hubble Space Telescope. Showing an tremendous cluster of stars called a globular cluster, this view is located in the galaxy Messier 55.

A globular cluster is a group of stars which is tens of thousands or even millions of stars, and which is held together by gravity. That's why these clusters tend to form spherical shapes as the forces of gravity hold the cluster together.

Read more
Stars sparkle in Orion Nebula in this week’s gorgeous Hubble image
The bright variable star V 372 Orionis takes center stage in this image from the NASA/ESA Hubble Space Telescope, which has also captured a smaller companion star in the upper left of this image. Both stars lie in the Orion Nebula, a colossal region of star formation roughly 1,450 light-years from Earth.

The Hubble Space Telescope is one of the great achievements in modern astronomy, still producing stunning and scientifically valuable images after more than 30 years of operation. Each week, scientists working with Hubble share an image captured by the telescope, and this week's image shows a snippet of a famous nebula along with two bright stars.

The image shows a part of the beautiful Orion Nebula, featuring the bright star V 372 Orionis just to the lower-right of the center along with a companion star to the top-left. The Orion Nebula is located 1,450 light-years away and is famous as a stellar nursery where large numbers of new stars are born.

Read more
Hubble captures rare image of a supernova as it happens
As a result of a phenomenon called gravitational lensing, three different moments in a far-off supernova explosion were captured in a single snapshot by the NASA/ESA Hubble Space Telescope. The light from the supernova, which was located behind the galaxy cluster Abell 370, was multiply lensed by the cluster’s immense gravity. This light took three different paths through the cosmic lens of the massive cluster. The three paths were three different lengths, so when the light arrived at Hubble (on the same day in December 2010), the supernova appeared at three different stages of evolution.

When a massive star runs out of fuel and approaches the end of its life, it explodes in a huge outpouring of energy called a supernova. These events can be so bright that they outshine entire galaxies, but they don't last for long -- just the blink of an eye, in cosmic terms. It's hard to capture the sudden brightness and fast dimming of a supernova event, because they are difficult to predict, but the Hubble Space Telescope recently managed to capture three different moments of a supernova in a single image.

"It is quite rare that a supernova can be detected at a very early stage, because that stage is really short," said Wenlei Chen, an author of the paper, in a statement. "It only lasts for hours to a few days, and it can be easily missed even for a nearby detection. In the same exposure, we are able to see a sequence of the images—like multiple faces of a supernova."

Read more