Skip to main content

Hubble observes a giant planet growing as it gobbles up dust and gas

This illustration of the newly forming exoplanet PDS 70b shows how material may be falling onto the giant world as it builds up mass. By employing Hubble’s ultraviolet light (UV) sensitivity, researchers got a unique look at radiation from extremely hot gas falling onto the planet, allowing them to directly measure the planet’s mass growth rate for the first time.
This illustration of the newly forming exoplanet PDS 70b shows how material may be falling onto the giant world as it builds up mass. By employing Hubble’s ultraviolet light (UV) sensitivity, researchers got a unique look at radiation from extremely hot gas falling onto the planet, allowing them to directly measure the planet’s mass growth rate for the first time. SCIENCE: McDonald Observatory–University of Texas, Yifan Zhou (UT) ILLUSTRATION: NASA, ESA, STScI, Joseph Olmsted (STScI)

Planets come in many compositions and sizes, and they can grow considerably larger than even the gas giants in our solar system. One such giant planet, PDS 70b, is two to three times the radius of Jupiter, and around three times its mass as well. Now, Hubble has made a rare direct observation of this planet to learn about how such large planets grow.

The planet’s host star, orange dwarf PDS 70, is located 370 light-years away in the constellation of Centaurus, and this is one of the relatively few systems in which a planet has been directly imaged. Most of the time, exoplanets are detected by seeing how light coming from their host star changes, from which the presence of planets can be inferred. But occasionally, a planet is big enough to be seen directly, like the chunky PDS 70b.

Recommended Videos

Not only could Hubble observe the planet, but it could also see how fast it grows by observing radiation from hot gas which is falling toward it. The planet is moving through a cloud of dust and gas around the star, and it gathers up material as it travels. The researchers believe that although the planet is still growing, it will soon come to the end of its growth phase.

Please enable Javascript to view this content

“We just don’t know very much about how giant planets grow,” said one of the researchers, Brendan Bowler of the University of Texas at Austin, in a statement. “This planetary system gives us the first opportunity to witness material falling onto a planet. Our results open up a new area for this research.”

“This system is so exciting because we can witness the formation of a planet,” said another researcher, Yifan Zhou, also of the University of Texas at Austin. “This is the youngest bona fide planet Hubble has ever directly imaged.”

Learning about how this planet is growing can also teach us about how planets like Jupiter formed in our solar system. It too may have grown by scooping up material from a disk of dust and gas.

“Thirty-one years after launch, we’re still finding new ways to use Hubble,” Bowler said. “Yifan’s observing strategy and post-processing technique will open new windows into studying similar systems, or even the same system, repeatedly with Hubble. With future observations, we could potentially discover when the majority of the gas and dust falls onto their planets and if it does so at a constant rate.”

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
James Webb observes extremely hot exoplanet with 5,000 mph winds
This artist’s concept shows what the hot gas-giant exoplanet WASP-43 b could look like. WASP-43 b is a Jupiter-sized planet circling a star roughly 280 light-years away, in the constellation Sextans. The planet orbits at a distance of about 1.3 million miles (0.014 astronomical units, or AU), completing one circuit in about 19.5 hours. Because it is so close to its star, WASP-43 b is probably tidally locked: its rotation rate and orbital period are the same, such that one side faces the star at all times.

Astronomers using the James Webb Space Telescope have modeled the weather on a distant exoplanet, revealing winds whipping around the planet at speeds of 5,000 miles per hour.

Researchers looked at exoplanet WASP-43 b, located 280 light-years away. It is a type of exoplanet called a hot Jupiter that is a similar size and mass to Jupiter, but orbits much closer to its star at just 1.3 million miles away, far closer than Mercury is to the sun. It is so close to its star that gravity holds it in place, with one side always facing the star and the other always facing out into space, so that one side (called the dayside) is burning hot and the other side (called the nightside) is much cooler. This temperature difference creates epic winds that whip around the planet's equator.

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