Close Menu
    Facebook X (Twitter) Instagram
    SciTechDaily
    • Biology
    • Chemistry
    • Earth
    • Health
    • Physics
    • Science
    • Space
    • Technology
    Facebook X (Twitter) Pinterest YouTube RSS
    SciTechDaily
    Home»Space»New Model May Rule Out the Presence of Dark Matter
    Space

    New Model May Rule Out the Presence of Dark Matter

    By Royal Astronomical SocietyApril 25, 20122 Comments6 Mins Read
    Facebook Twitter Pinterest Telegram LinkedIn WhatsApp Email Reddit
    Share
    Facebook Twitter LinkedIn Pinterest Telegram Email Reddit
    interacting galaxies
    UGC 9618, also known as VV 340 or Arp 302 consists of a pair of very gas-rich spiral galaxies in their early stages of interaction: VV 340A is seen edge-on to the left, and VV 340B face-on to the right. An enormous amount of infrared light is radiated by the gas from massive stars that are forming at a rate similar to the most vigorous giant star-forming regions in our own Milky Way. UGC 9618 is 450 million light-years away from Earth, and is the 302nd galaxy in Arp’s Atlas of Peculiar Galaxies. Credit: NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)

    Searching for dark matter and studying conventional models for the origin and evolution of the universe has led astronomers from the University of Bonn to assemble data in an effort to better understand what surrounds our galaxy. Their analysis of this data paints a new picture of our cosmic neighborhood, which appears to rule out the presence of dark matter.

    Astronomers from the University of Bonn in Germany have discovered a vast structure of satellite galaxies and clusters of stars surrounding our Galaxy, stretching out across a million light years. 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 neighborhood 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 center of the Galaxy.

    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.”

    Interacting Galaxy Pair Arp 87
    The two main players comprising Arp 87 are NGC 3808 on the right (the larger of the two galaxies) and its companion NGC 3808A on the left. NGC 3808 is a nearly face-on spiral galaxy with a bright ring of star formation and several prominent dust arms. Stars, gas, and dust flow from NGC 3808, forming an enveloping arm around its companion. NGC 3808A is a spiral galaxy seen edge-on and is surrounded by a rotating ring that contains stars and interstellar gas clouds. The ring is situated perpendicular to the plane of the host galaxy disk and is called a “polar ring.” Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)

    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.

    Pawlowski adds, “We think that the Milky Way collided with another galaxy in the distant past. The other galaxy lost part of its material, material that then formed our Galaxy’s satellite galaxies and the younger globular clusters and the bulge at the galactic center. The companions we see today are the debris of this 11 billion-year-old collision.”

    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.”

    Reference: “The VPOS: a vast polar structure of satellite galaxies, globular clusters and streams around the Milky Way” by M. S. Pawlowski, J. Pflamm-Altenburg and P. Kroupa, 8 June 2012, Monthly Notices of the Royal Astronomical Society.
    DOI: 10.1111/j.1365-2966.2012.20937.x

    Never miss a breakthrough: Join the SciTechDaily newsletter.
    Follow us on Google and Google News.

    Astronomy Cosmology Dark Matter Galaxy Galaxy Evolution Globular Cluster Milky Way Royal Astronomical Society Stars
    Share. Facebook Twitter Pinterest LinkedIn Email Reddit

    Related Articles

    The Center of Our Galaxy May Not Be a Black Hole

    Why Nearby Galaxies Are Fleeing Us: Scientists Finally Solve a 50-Year Mystery

    400-Year-Old Cosmic Mystery Solved: New Class of Ancient Star System Discovered Hiding in Our Galaxy

    Monster Black Hole Jets in a Spiral Galaxy Could Forecast the Milky Way’s Frightening Future

    Cosmic Oddity: Rare Second-Gen Star Found Beyond the Milky Way

    Dark Matter Filament in Galaxy Supercluster Directly Measured

    Galaxies are Hiding More Atomic Hydrogen Gas than Previously Calculated

    Hubble Captures New Image of Messier 9

    Large Globular Star Clusters Survive Collisions, Smaller Clusters Do Not

    2 Comments

    1. Joe on April 26, 2012 5:01 pm

      This tentative hypothesis supports the Theory of a SUPRAGOD. Atheism is boring.

      Reply
    2. Gordon Boutilier on November 30, 2012 11:26 am

      Maybe as celestail objects get farther from celestial bodies the speed at wich they travel increases because beyond the event horizon of the known universe is unbalanced charge drawing everything to it. Once the event horizon has drawn a certain amount of material , the universe collapses?
      Question do black holes accelerate at the same speed as suns ?
      The unbalanced charged omniverse behaves like a pot of bioling water. As “things” boil, universes are released and as the bubble closes “pressure”, the universe colapses.

      Reply
    Leave A Reply Cancel Reply

    • Facebook
    • Twitter
    • Pinterest
    • YouTube

    Don't Miss a Discovery

    Subscribe for the Latest in Science & Tech!

    Trending News

    Scientists Discover 132-Million-Year-Old Dinosaur Tracks on South Africa’s Coast

    Scientists Uncover the Secret Ingredient Behind the Spark That May Have Started Life on Earth

    Physicists Observe Matter in Two Places at Once in Mind-Bending Quantum Experiment

    Stanford Scientists Discover Hidden Brain Circuit That Fuels Chronic Pain

    New Study Reveals Why Ozempic Works Better for Some People Than Others

    Climate Change Is Altering a Key Greenhouse Gas in a Way Scientists Didn’t Expect

    New Study Suggests Gravitational Waves May Have Created Dark Matter

    Scientists Discover Why the Brain Gets Stuck in Schizophrenia

    Follow SciTechDaily
    • Facebook
    • Twitter
    • YouTube
    • Pinterest
    • Newsletter
    • RSS
    SciTech News
    • Biology News
    • Chemistry News
    • Earth News
    • Health News
    • Physics News
    • Science News
    • Space News
    • Technology News
    Recent Posts
    • 320 Light-Years Away, a Planet Confirms a Fundamental Cosmic Assumption
    • Astronomers Solve Decades-Long Mystery About Saturn’s Spin – “Something Strange Was Happening”
    • Scientists Uncover Strange New State of Matter Inside Uranus and Neptune
    • The Crown Jewel of Dentistry? Breakthrough Tech Could Transform Tooth Repair
    • The Surprising Non-Medical Factor That Determines Cancer Survival
    Copyright © 1998 - 2026 SciTechDaily. All Rights Reserved.
    • Science News
    • About
    • Contact
    • Editorial Board
    • Privacy Policy
    • Terms of Use

    Type above and press Enter to search. Press Esc to cancel.