MessageToEagle.com - A vast structure of satellite galaxies and clusters of stars surrounding our Galaxy,
stretching out across a million light years has been discovered by astronomers from the University of Bonn in Germany .
The work challenges the existence of dark matter, part of the standard model for the evolution of the universe.
PhD student and lead author Marcel Pawlowski reports the team’s findings in a paper in the journal Monthly Notices
of the Royal Astronomical Society.
The Milky Way, the galaxy we live in, consists of around three hundred thousand million stars as well as large
amounts of gas and dust arranged with arms in a flat disk that wind out from a central bar.
The diameter of the main part of the Milky Way is about 100,000 light years, meaning that a beam of light takes
100,000 years to travel across it. A number of smaller satellite galaxies and spherical clusters of stars (so-called globular
clusters) orbit at various distances from the main Galaxy.
Conventional models for the origin and evolution of the universe (cosmology) are based on the presence of ‘dark matter’,
invisible material thought to make up about 23% of the content of the cosmos that has never been detected directly.
In this model, the Milky Way is predicted to have far more satellite galaxies than are actually seen.
In their effort to understand exactly what surrounds our Galaxy, the scientists used a range of sources from twentieth century
photographic plates to images from the robotic telescope of the Sloan Deep Sky Survey. Using all these data they assembled a
picture that includes bright ‘classical’ satellite galaxies, more recently detected fainter satellites and the younger globular clusters.
“Once we had completed our analysis, a new picture of our cosmic neighbourhood emerged”, says Pawlowski. The astronomers found
that all the different objects are distributed in a plane at right angles to the galactic disk.
The newly-discovered structure is huge, extending from as close as 33,000 light years to as far away as one million light
years from the centre of the Galaxy.
VV 340 - Two perpendicular galaxies going to collide. Image credit: NASA, ESA, Hubble
Team member Pavel Kroupa, professor for astronomy at the University of Bonn, adds “We were baffled by how well the
distributions of the different types of objects agreed with each other”. As the different companions move around the
Milky Way, they lose material, stars and sometimes gas, which forms long streams along their paths. The new results show
that this lost material is aligned with the plane of galaxies and clusters too. “This illustrates that the objects are not
only situated within this plane right now, but that they move within it”, says Pawlowski. “The structure is stable.”
The various dark matter models struggle to explain this arrangement. “In the standard theories, the satellite galaxies would
have formed as individual objects before being captured by the Milky Way”, explains Kroupa. “As they would have come from many
directions, it is next to impossible for them to end up distributed in such a thin plane structure.”
Postdoctoral researcher and team member Jan Pflamm-Altenburg suggests an alternative explanation. “The satellite galaxies and
clusters must have formed together in one major event, a collision of two galaxies.” Such collisions are relatively common and
lead to large chunks of galaxies being torn out due to gravitational and tidal forces acting on the stars, gas and dust they
contain, forming tails that are the birthplaces of new objects like star clusters and dwarf galaxies.
Arp 87 - A galaxy gets torn apart in a collision. Image credit: NASA, ESA, Hubble
Kroupa concludes by highlighting the wider significance of the new work. “Our model appears to rule out the presence of dark
matter in the universe, threatening a central pillar of current cosmological theory. We see this as the beginning of a paradigm
shift, one that will ultimately lead us to a new understanding of the universe we inhabit.”
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