At last we are special by a cosmic standard! That is, we live in a galaxy – our star island, the Milky Way – that is among only four percent of similar galaxies with bright, nearby satellites. In our galaxy’s case, those satellites are the large and small Magellanic Clouds, visible from Earth’s southern hemisphere.
Stanford University astrophysicist Risa Wechsler and her team of researchers published these results in the May 20 issue of The Astrophysical Journal comparing the Milky Way to similar galaxies. The results of the study also support a leading theory – the Cold Dark Matter theory – of galaxy formation.
The findings are based on analyses of data collected from the Sloan Digital Sky Survey (SDSS). The work is the first of three papers that study the properties of the Milky Way’s two most massive satellites.
We are interested in how the Milky Way fits into the broader context of the universe. This research helps us understand whether our galaxy is typical or not, and may provide clues to its formation history.
Supported in part by the National Science Foundation (NSF), the SDSS is the most extensive survey of the optical sky performed to date. In more than eight years of operations, SDSS has obtained images covering more than a quarter of the sky, and created 3-D maps containing more than 930,000 galaxies and 120,000 quasars.
For this analysis, Wechsler’s group studied more than 20,000 galaxies with properties similar to the Milky Way, and investigated the galaxies surrounding these Milky Way “twins” to create a census of galaxies similar to the Milky Way. The work represents one of the most extensive studies of this kind ever performed.
Scientists can also compare the SDSS data to galaxies simulated by a computer model. Since they are currently unable to see all the way back to the Big Bang, this is one way researchers are trying to understand how the universe as we see it today began.
In order to learn more about possible conditions in the early universe, the group performed computer simulations to recreate the universe from specific sets of starting conditions. Then they compared their simulations to the SDSS data set. In this way, the group was able to test different theories of galaxy formation to determine whether or not each would result in a universe that matches what we see today. The results of their simulation matched the result found in the SDSS data set: just four percent of the simulated galaxies had two satellites like the Magellanic Clouds.
Nigel Sharp, of NSF’s Division of Astronomical Sciences, said:
This is an excellent example of data-enabled science. Comparing the “fake” and “real” universes is how we discriminate between successful and unsuccessful theories. This work interconnects three of the four legs of science: theory, observation, and simulation, for a powerful scientific result.
Their results also lend support to a leading theory of galaxy formation called the Cold Dark Matter (CDM) theory. This theory provides what many consider to be the simplest explanation for the arrangement of galaxies throughout the universe following the Big Bang. It assumes that most of the matter in the universe consists of material that cannot be observed by its electromagnetic radiation (dark) and whose constituent particles move slowly (cold). Dark matter, an invisible and exotic material of unknown composition, is believed to influence the distribution of galaxies in space and the overall expansion of the universe. The rarity of this aspect of the Milky Way may provide clues to its formation history.
Because the presence of two galaxies like the Magellanic Clouds is unusual, we can use them to learn more about our own galaxy.
Using their simulation, the team identified a sample of simulated galaxies that had satellites matching the Milky Way’s in terms of their locations and speeds.
The combination of large surveys of the sky like the SDSS and large samples of simulated galaxies provides a new opportunity to learn about the place of our galaxy in the universe. Future surveys will allow us to extend this study to even dimmer satellite galaxies, to build a full picture of the formation of our galaxy.
The theoretical and numerical work that produced the simulations used as a comparison for the SDSS data were supported by an award funded under the American Recovery and Reinvestment Act of 2009.
Summary: Based on data from the Sloan Digital Sky Survey (SDSS), a study by astrophysicist Risa Wechsler and her Stanford team shows that just four percent of galaxies have two satellites as bright and close by as the Milky Way’s two closest satellites, the Large and Small Magellanic Clouds. The study verifies the accuracy of simulation models and supports the CDM (cold dark matter) theory of galaxy formation. Results of the study appear in the May 20, 2011 issue of The Astrophysical Journal.