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Friday, November 12, 2010

Dark Matter 1, MOND 0

NASA recently used Hubble's Advanced Camera for Surveys to chart the distribution of matter in the massive galaxy cluster Abell 1689. Part of what they found was that the cluster was much more dense in non-visible matter than anticipated, which was easily demonstrated by the actual amount of gravitational lensing observed relative to the apparent mass of the visible light portions of the cluster.

The article neglects to mention one very important result of this data: this may be the proverbial final nail in the coffin for Modified Newtonian Dynamics (MOND), thereby eliminating the best and most reasonable alternative explanation for the discrepancy between Newtonian Dynamics and the observed rotation of galaxies, other than dark matter. It would be a stretch to say that this proves the existence of dark matter conclusively, but dark matter now stands as the unchallenged front-runner to explain the observed behavior of galaxies.

Kind of sad for that, I've been a big fan of MOND. But, that's how science works. 

From the NASA website:

Astronomers using NASA's Hubble Space Telescope took advantage of a giant cosmic magnifying glass to create one of the sharpest and most detailed maps of dark matter in the universe. Dark matter is an invisible and unknown substance that makes up the bulk of the universe's mass.

The new dark matter observations may yield new insights into the role of dark energy in the universe's early formative years. The result suggests that galaxy clusters may have formed earlier than expected, before the push of dark energy inhibited their growth. A mysterious property of space, dark energy fights against the gravitational pull of dark matter. Dark energy pushes galaxies apart from one another by stretching the space between them, thereby suppressing the formation of giant structures called galaxy clusters. One way astronomers can probe this primeval tug-of-war is through mapping the distribution of dark matter in clusters.

A team led by Dan Coe at NASA's Jet Propulsion Laboratory in Pasadena, Calif., used Hubble's Advanced Camera for Surveys to chart the invisible matter in the massive galaxy cluster Abell 1689, located 2.2 billion light-years away. The cluster's gravity, the majority of which comes from dark matter, acts like a cosmic magnifying glass, bending and amplifying the light from distant galaxies behind it. This effect, called gravitational lensing, produces multiple, warped, and greatly magnified images of those galaxies, like the view in a funhouse mirror. By studying the distorted images, astronomers estimated the amount of dark matter within the cluster. If the cluster's gravity only came from the visible galaxies, the lensing distortions would be much weaker.

Based on their higher-resolution mass map, Coe and his collaborators confirm previous results showing that the core of Abell 1689 is much denser in dark matter than expected for a cluster of its size, based on computer simulations of structure growth. Abell 1689 joins a handful of other well-studied clusters found to have similarly dense cores. The finding is surprising, because the push of dark energy early in the universe's history would have stunted the growth of all galaxy clusters.

"Galaxy clusters, therefore, would had to have started forming billions of years earlier in order to build up to the numbers we see today," Coe explains. "At earlier times, the universe was smaller and more densely packed with dark matter. Abell 1689 appears to have been well fed at birth by the dense matter surrounding it in the early universe. The cluster has carried this bulk with it through its adult life to appear as we observe it today."


The entire NASA article is here.

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