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Space Giant Andromeda Galaxy circled by disk of dwarf galaxies

Giant Andromeda Galaxy circled by disk of dwarf galaxies

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First Posted: Jan 04, 2013 10:32 AM EST

A new study shows an unexpected phenomenon in our nearest giant cosmic neighbor, the Andromeda galaxy. A majority of its dwarf galaxy companions are aligned in a giant disk that appears to rotate around the bright host also known as Messier 31. The PAndAS (Pan-Andromeda Archaeological Survey) team used MegaCam on the Canada-France-Hawaii Telescope to conduct the survey, complemented by spectroscopic follow-ups with the W. M. Keck Observatory.

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"Astronomers have been observing Andromeda since Persian astronomers first noted it over a thousand years ago, but it is only in the past decade that we have truly studied it in exquisite detail with the Pan-Andromeda Archaeological Survey," said participating professor Geraint Lewis from the University of Sydney's School of Physics "The Pan-Andromeda Archaeological Survey - cutely called PAndAS - is a large project that ran between 2008 and 2011, using the Canada-France-Hawaii Telescope situated on the Mauna Kea volcano on the Big Island of Hawaii. Now that we're examining the data it collected, it is providing our first panoramic view of our closest large companion in the cosmos," explained Lewis.

Andromeda galaxy disk
(Photo : Flickr)
Andromeda galaxy, containing about one trillion stars, surrounded by smaller galaxies with only one billion stars or less.

Large galaxies like Andromeda and our own Milky Way have long been known to be orbited by an entourage of smaller galaxies. These systems -- that are individually anywhere from ten to at least hundreds of thousands times fainter that their bright hosts -- were thought to trace a path around the big galaxy that was independent of every other dwarf. The fact that astronomers now see that a majority of these little systems in fact contrive to map out an immensely large -- approximately one million light-years across -- but extremely flattened structure, implies that this understanding is grossly incorrect. Either something about how these galaxies formed, or subsequently evolved, must have led them to trace out this peculiar, coherent, structure. While dwarf galaxies are not massive, they are the most numerous galaxy type in the universe, so understanding what this is expected to shed new insight into the formation of galaxies at all masses.

The study is based on the Pan-Andromeda Archaeological Survey (PAndAS), a large project undertaken between 2008 and 2011 with MegaCam on the Canada-France-Hawaii Telescope situated on the Mauna Kea volcano on the Big Island of Hawaii. It culminates many years of effort by an international team of scientists who have discovered a large number of the satellite galaxies, developed new techniques to measure their distances, and have used the Keck telescope with colleagues to measure their radial velocities. While earlier work had hinted at the existence of this structure, the new study has demonstrated its existence to a high level of statistical confidence (99.998%), and has revealed the coherent motion.

Andromeda galaxy disk
(Photo : Nature)
The top left hand image below is a truecolour photograph (taken with the Canada-France-Hawaii Telescope) of the Andromeda galaxy, the closest giant galaxy to our own, and in many ways our Milky Way’s twin sister. Also visible in this photograph are two of its satellites (these are much smaller galaxies, containing up to about a billion stars). The study has measured the distances and velocities of 27 other such dwarf galaxies : their three-dimensional positions are shown with red spheres in the other panels. The top right hand panel depicts how these appear to us as viewed from Earth.

In the current theory of how galaxies form, the first galaxies form within large clumps of dark matter (what astronomers call "halos"). This dark matter is mysterious stuff: it is the dominant form of matter in the universe, and has not yet been directly detected, but its influence in galaxies is firmly established. These first galaxies must have been small, but over time giant galaxies like Andromeda and the Milky Way are thought to have evolved by cannibalizing their smaller neighbors. In this picture the dwarf galaxies that we see at the present day would be those ancient primordial galaxies that survived this ordeal. However, nowhere in this picture is there an explanation for why the surviving dwarfs should map out a large disk like we now see around our nearest neighbor. It appears that the smallest galaxies in the universe are intent on providing the biggest challenges to our understanding of galaxy formation.

"We don't yet know where this is pointing us" said Rodrigo Ibata, lead author on the report. "It flies in the face of our ideas about galaxy formation, but it surely is very exciting."

Andromeda is the largest galaxy of the Local Group, which consists of the Andromeda Galaxy, the Milky Way, the Triangulum Galaxy, and about 30 other smaller galaxies. Although the largest, Andromeda may not be the most massive, as recent findings suggest that the Milky Way contains more dark matter and may be the most massive in the grouping. The 2006 observations by the Spitzer Space Telescope revealed that M31 contains one trillion (10^12) stars, at least twice more than the number of stars in our own galaxy, which is estimated to be 200-400 billion.

PIO Contact:
Dr. Jean-Charles Cuillandre
Canada-France-Hawaii Telescope Corporation
+1 (808) 885-3128
jcc@cfht.hawaii.edu

Science Contact:
Dr. Rodrigo Ibata
Observatoire de Strasbourg, France
rodrigo.ibata@astro.unistra.fr
+33 3 68 85 23 91

Reference: "A vast, thin plane of corotating dwarf galaxies orbiting the Andromeda galaxy," Nature, Volume 493, Number 7430, pp. 62-65, 3 January 2013: http://www.nature.com/nature/journal/v493/n7430/full/nature11717.html

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