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Hubble Provides New Evidence For Dark Matter Around Small Galaxies

Date:
March 13, 2009
Source:
Royal Astronomical Society (RAS)
Summary:
NASA's Hubble Space Telescope has uncovered a strong new line of evidence that galaxies are embedded in halos of dark matter.

These four dwarf galaxies are part of a census of small galaxies in the tumultuous heart of the nearby Perseus galaxy cluster. The galaxies appear smooth and symmetrical, suggesting that they have not been tidally disrupted by the pull of gravity in the dense cluster environment. Larger galaxies around them, however, are being ripped apart by the gravitational tug of other galaxies.
Credit: NASA, ESA, and C. Conselice and S. Penny (University of Nottingham)

NASA’s Hubble Space Telescope has uncovered a strong new line of evidence that galaxies are embedded in halos of dark matter.

Peering into the tumultuous heart of the nearby Perseus galaxy cluster, Hubble discovered a large population of small galaxies that have remained intact while larger galaxies around them are being ripped apart by the gravitational pull of neighbouring galaxies. The results appear in the March 1st edition of the journal Monthly Notices of the Royal Astronomical Society.

Dark matter is an invisible form of matter that accounts for most of the Universe’s mass. Astronomers have deduced the existence of dark matter by observing its gravitational influence on normal matter which consists of stars, gas, and dust.

The Hubble images provide further evidence that the undisturbed galaxies are enshrouded by a “cushion” of dark matter, which protects them from their rough-and-tumble neighbourhood.

“We were surprised to find so many dwarf galaxies in the core of this cluster that were so smooth and round and had no evidence at all of any kind of disturbance,” says astronomer Christopher Conselice of the University of Nottingham, and leader of the Hubble observations. “These dwarfs are very old galaxies that have been in the cluster a long time. So if something was going to disrupt them, it would have happened by now. They must be very, very dark matter dominated galaxies.”

The dwarf galaxies may have even a higher amount of dark matter than spiral galaxies. “With these results, we cannot say whether the dark-matter content of the dwarfs is higher than in the Milky Way Galaxy,” Conselice says. “Although, the fact that spiral galaxies are destroyed in clusters, while the dwarfs are not, suggests that is indeed the case.”

First proposed about 80 years ago, dark matter is thought to be the “glue” that holds galaxies together. Astronomers suggest that dark matter provides vital “scaffolding” for the Universe, forming a framework for the formation of galaxies through gravitational attraction. Previous studies with Hubble and NASA’s Chandra X-ray Observatory found evidence of dark matter in entire clusters of galaxies such as the Bullet Cluster. The new Hubble observations continue the search for dark matter in individual galaxies.

Observations by Hubble’s Advanced Camera for Surveys spotted 29 dwarf elliptical galaxies in the Perseus Cluster located 250 million light-years away and one of the closest galaxy clusters to Earth. Of those galaxies 17 are new discoveries.

Because dark matter cannot be seen astronomers detected its presence through indirect evidence. The most common method is by measuring the velocities of individual stars or groups of stars as they move randomly in the galaxy or as they rotate around the galaxy. The Perseus Cluster is too far away for telescopes to resolve individual stars and measure their motions. So Conselice and his team derived a new technique for uncovering dark matter in these dwarf galaxies by determining the minimum mass the dwarfs must have to protect them from being disrupted by the strong tidal pull of gravity from larger galaxies.

Studying these small galaxies in detail was possible only because of the sharpness of Hubble’s Advanced Camera for Surveys. Conselice and his team first spied the galaxies with the WIYN Telescope at Kitt Peak National Observatory outside Tucson, Arizona. Those observations, Conselice says, only hinted that many of the galaxies were smooth and therefore dark-matter dominated. “Those ground-based observations could not resolve the galaxies, so we needed Hubble imaging to nail it,” he says.

Other team members are Samantha J. Penny of the University of Nottingham; Sven De Rijcke of the University of Ghent in Belgium; and Enrico Held of the University of Padua in Italy.


Story Source:

The above story is based on materials provided by Royal Astronomical Society (RAS). Note: Materials may be edited for content and length.


Journal Reference:

  1. Penny et al. Hubble Space Telescope survey of the Perseus Cluster - I. The structure and dark matter content of cluster dwarf spheroidals. Monthly Notices of the Royal Astronomical Society, 2009; 393 (3): 1054 DOI: 10.1111/j.1365-2966.2008.14269.x

Cite This Page:

Royal Astronomical Society (RAS). "Hubble Provides New Evidence For Dark Matter Around Small Galaxies." ScienceDaily. ScienceDaily, 13 March 2009. <www.sciencedaily.com/releases/2009/03/090312093947.htm>.
Royal Astronomical Society (RAS). (2009, March 13). Hubble Provides New Evidence For Dark Matter Around Small Galaxies. ScienceDaily. Retrieved September 17, 2014 from www.sciencedaily.com/releases/2009/03/090312093947.htm
Royal Astronomical Society (RAS). "Hubble Provides New Evidence For Dark Matter Around Small Galaxies." ScienceDaily. www.sciencedaily.com/releases/2009/03/090312093947.htm (accessed September 17, 2014).

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