Eyes in the sky

Do you ever get the feeling that you're being watched? This friendly-looking object is the result of two galaxies merging into one another, complete with a pair of eyes hiding two growing supermassive black holes and a swirling grin. Such mergers are rare in our galactic neighbourhood; Mrk 739 is close enough (astronomically speaking) to study the event in detail, and thus gain a better understanding of the dramatic processes that take place during these cosmic mergers.

By using the MUSE instrument on ESO’s Very Large Telescope, the team of astronomers, led by master’s student Dusán Tubín at the Pontificia Universidad Católica de Chile, were able to study the effects of both the merger and the radiation emitted by the growing gigantic black holes. Their study answers questions about the motion of the galaxies, the age of their stars, and the elements they are made up of. They have found that one of these galaxies is much older than its companion, and that their merging process is at an early stage.

MUSE is a 3D spectrograph that takes images — known as “datacubes” — of the object being observed over thousands of wavelengths. With MUSE, astronomers are therefore able to map in great detail the properties of the objects they study, because each individual pixel contains an impressive amount of information. Obtaining these exciting insights into galaxy merging and evolution with MUSE is enough to make anyone smile.

Credit:

ESO/Tubín et al.

About the Image

Id:potw2117a
Type:Observation
Release date:26 April 2021, 06:00
Size:882 x 824 px

About the Object

Name:Mrk 739
Type:Local Universe : Galaxy : Type : Interacting
Constellation:Leo
Category:Galaxies

Image Formats

Large JPEG
102.2 KB
Screensize JPEG
104.0 KB

Zoomable


Wallpapers

1024x768
110.2 KB
1280x1024
166.1 KB
1600x1200
225.1 KB
1920x1200
253.6 KB
2048x1536
325.8 KB

Coordinates

Position (RA):11 36 28.99
Position (Dec):21° 35' 42.11"
Field of view:0.98 x 0.92 arcminutes
Orientation:North is -0.0° left of vertical

Colours & filters

BandWavelengthTelescope
Optical
B
438 nmVery Large Telescope
MUSE
Optical
g
475 nmVery Large Telescope
MUSE
Optical
r
625 nmVery Large Telescope
MUSE