Kraken Reveals Itself: Astrophysicists Reconstruct the Galaxy Merger History of Our Home Galaxy


Milky Way Family Tree

Galaxies like the Milky Way formed by the merging of smaller progenitor galaxies. An international team of astrophysicists led by Dr. Diederik Kruijssen from the Centre for Astronomy at Heidelberg University has succeeded in reconstructing the merger history of our home galaxy, creating a complete family tree. To achieve this, the researchers analyzed the properties of globular clusters orbiting the Milky Way with artificial intelligence. Their investigations revealed a previously unknown galaxy collision that must have permanently altered the appearance of the Milky Way.

Globular clusters are dense groups of up to a million stars that are almost as old as the universe itself. The Milky Way hosts over 150 of such clusters. “Many of them came from smaller galaxies that later merged to form the Milky Way that we live in today,” explains Dr. Kruijssen. To study the merger history, the Heidelberg researcher and his colleague Dr. Joel Pfeffer of Liverpool John Moores University (United Kingdom) and their research groups developed a suite of advanced computer simulations, called E-MOSAICS. These simulations include a complete model for the formation, evolution, and destruction of globular clusters.

The German-British team used these simulations to relate the ages, chemical compositions, and orbital motions of the globular clusters to the properties of the progenitor galaxies in which they formed, more than ten billion years ago. By applying these insights to groups of globular clusters in the Milky Way, they not only determined how massive these progenitor galaxies were, but also when they merged with our home galaxy.

Movie of one of the E-MOSAICS simulations, showing the formation of a Milky Way-like galaxy. The grey shading shows gas fragmenting, forming stars, and falling onto the central galaxy. Newborn stars blow bubbles into the gas with their intense radiation and supernova explosions. The globular clusters are indicated by colored dots, where the color indicates the chemical composition: blue clusters have a low level of elements more massive than helium, whereas red clusters have a high level of such elements. Over time, the merging of the central galaxy with smaller, satellite galaxies brings in a large number of globular clusters. The ages, chemical compositions, and orbits of these clusters reveal the mass of the progenitor galaxy that they originally formed in, as well as the time at which it merged with the central galaxy. Together, these enabled the family tree of the Milky Way to be deciphered.
Credit: J. Pfeffer, D. Kruijssen, R. Crain, N. Bastian

MORE of the story and another associated image / click image TOP of PAGE