Skip to main content

This ancient, dusty galaxy gives clues to the earliest evolution of the universe

Artist’s impression of what MAMBO-9 would look like in visible light. The galaxy is very dusty and it has yet to build most of its stars. NRAO/AUI/NSF, B. Saxton

Astronomers have observed an ancient, dusty galaxy that forms stars at a tremendous rate. The galaxy is named MAMBO-9, and the light it generates traveled for around 13 billion years to reach Earth. The universe is only 13.8 billion years old, so MAMBO-9 is one of the oldest dusty galaxies yet observed.

MAMBO-9 is categorized as a dusty galaxy because it contains massive amounts of dust and gas, making it the perfect nursery for the formation of new stars. Such galaxies form stars at a rate of up to the equivalent of several thousand times the mass of our sun per year. For reference, in our galaxy stars are formed at a rate of around three solar masses per year. Another reason that MAMBO-9 is noteworthy is that astronomers previously thought that massive galaxies wouldn’t have formed in the early universe, but being both very old and very massive, this galaxy disproves that.

Recommended Videos

Locating ancient dusty galaxies is extremely challenging because the dust obscures the light from the stars which makes them hard to spot. “These galaxies tend to hide in plain sight,” lead author Caitlin Casey of the University of Texas at Austin explained in a statement. “We know they are out there, but they are not easy to find because their starlight is hidden in clouds of dust.”

To pinpoint this galaxy, Casey and her team used the Atacama Large Millimeter/submillimeter Array (ALMA) to detect the very faint starlight being given off. Thanks to ALMA’s sensitivity, Casey and her team have now been able to determine the distance of MAMBO-9. “We found the galaxy in a new ALMA survey specifically designed to identify dusty star-forming galaxies in the early universe,” said Casey. “And what is special about this observation, is that this is the most distant dusty galaxy we have ever seen in an unobstructed way.”

The astronomers were able to determine that the galaxy is not only massive, with ten times more mass from dust and gas than all the stars in the Milky Way, but it is still continuing to form stars. The amount of dust is surprising as we normally observe more stars than dust because dust is produced by dying stars. But in this case, there is much more dust than stars. Astronomers are still figuring out how so much dust could have been formed so soon after the Big Bang.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
Hubble images dusty galaxy to learn about supermassive black holes
The galaxy NGC 1022

The galaxy NGC 1022, beautifully streaked with tendrils of reddish dust, captured here in wonderful detail by the NASA/ESA Hubble Space Telescope. ESA/Hubble & NASA, A. Seth

This week's image from the Hubble Space Telescope shows the barred spiral galaxy NGC 1022, located in the constellation of Cetus. Scientists are observing this particular galaxy in order to study the relationship between the size of a galaxy and the size of the supermassive black hole at its center. They know that most galaxies, including the Milky Way, have huge black holes at their heart, but they aren't sure exactly how galaxies and supermassive black holes evolve together over time.

Read more
Impending collision of Milky Way with other galaxy is already creating new stars
A map of the Milky Way.

A newfound cluster of young stars (blue star) sits on the periphery of the Milky Way. These stars probably formed from material originating from neighboring dwarf galaxies called the Magellanic Clouds. D. Nidever; NASA

We know that in around 2 billion years' time, our galaxy will collide with a nearby satellite galaxy, the Large Magellanic Cloud (LMC). This collision will be so dramatic that it will awaken the black hole at the heart of our galaxy, causing it to gorge on nearby matter and balloon to ten times its current size. The LMC is a fairly small galaxy, but it is rich in dark matter so it has a large mass, causing the collision between the two galaxies to be catastrophic.

Read more
Astronomers search tiny galaxies to understand the evolution of black holes
Artist's conception of a dwarf galaxy

Artist's conception of a dwarf galaxy, its shape distorted, most likely by a past interaction with another galaxy, and a massive black hole on its outskirts (pullout). The black hole is drawing in material that forms a rotating disk and generates jets of material propelled outward. Sophia Dagnello, NRAO/AUI/NSF

We know that at the heart of galaxies lie enormous supermassive black holes, although exactly how these black holes formed when the universe was young is a question scientists are still investigating. Now, astronomers have new clues to this conundrum with the discovery of 13 massive black holes in dwarf galaxies relatively nearby to Earth.

Read more