New! Sign up for our free email newsletter.
Science News
from research organizations

ESO telescope images a spectacular cosmic dance

Date:
August 17, 2022
Source:
ESO
Summary:
ESO's Very Large Telescope (VLT) has imaged the result of a spectacular cosmic collision -- the galaxy NGC 7727. This giant was born from the merger of two galaxies, an event that started around a billion years ago. At its center lies the closest pair of supermassive black holes ever found, two objects that are destined to coalesce into an even more massive black hole.
Share:
FULL STORY

ESO's Very Large Telescope (VLT) has imaged the result of a spectacular cosmic collision -- the galaxy NGC 7727. This giant was born from the merger of two galaxies, an event that started around a billion years ago. At its centre lies the closest pair of supermassive black holes ever found, two objects that are destined to coalesce into an even more massive black hole.

Just as you may bump into someone on a busy street, galaxies too can bump into each other. But while galactic interactions are much more violent than a bump on a busy street, individual stars don't generally collide since, compared to their sizes, the distances between them are very large. Rather, the galaxies dance around each other, with gravity creating tidal forces that dramatically change the look of the two dance partners. 'Tails' of stars, gas and dust are spun around the galaxies as they eventually form a new, merged galaxy, resulting in the disordered and beautifully asymmetrical shape that we see in NGC 7727.

The consequences of this cosmic bump are spectacularly evident in this image of the galaxy, taken with the FOcal Reducer and low dispersion Spectrograph 2 (FORS2) instrument at ESO's VLT. While the galaxy was previously captured by another ESO telescope, this new image shows more intricate details both within the main body of the galaxy and in the faint tails around it.

In this ESO VLT image we see the tangled trails created as the two galaxies merged, stripping stars and dust from each other to create the spectacular long arms embracing NGC 7727. Parts of these arms are dotted with stars, which appear as bright blue-purplish spots in this image.

Also visible in this image are two bright points at the centre of the galaxy, another telltale sign of its dramatic past. The core of NGC 7727 still consists of the original two galactic cores, each hosting a supermassive black hole. Located about 89 million light-years away from Earth, in the constellation of Aquarius, this is the closest pair of supermassive black holes to us.

The black holes in NGC 7727 are observed to be just 1600 light-years apart in the sky and are expected to merge within 250 million years, the blink of an eye in astronomical time. When the black holes merge they will create an even more massive black hole.

The search for similarly hidden supermassive black hole pairs is expected to make a great leap forward with ESO's upcoming Extremely Large Telescope (https://elt.eso.org/) (ELT), set to start operating later this decade in Chile's Atacama Desert. With the ELT, we can expect many more of these discoveries at the centres of galaxies.

Our home galaxy, which also sports a supermassive black hole at its centre, is on a path to merge with our closest large neighbour, the Andromeda Galaxy, billions of years from now. Perhaps the resulting galaxy will look something similar to the cosmic dance we see in NGC 7727, so this image could be giving us a glimpse into the future.


Story Source:

Materials provided by ESO. Note: Content may be edited for style and length.


Cite This Page:

ESO. "ESO telescope images a spectacular cosmic dance." ScienceDaily. ScienceDaily, 17 August 2022. <www.sciencedaily.com/releases/2022/08/220817135606.htm>.
ESO. (2022, August 17). ESO telescope images a spectacular cosmic dance. ScienceDaily. Retrieved December 20, 2024 from www.sciencedaily.com/releases/2022/08/220817135606.htm
ESO. "ESO telescope images a spectacular cosmic dance." ScienceDaily. www.sciencedaily.com/releases/2022/08/220817135606.htm (accessed December 20, 2024).

Explore More

from ScienceDaily

RELATED STORIES