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How do you make a galaxy without dark matter

March 28, 2018

[TORONTO] A team of astronomers has discovered a unique galaxy--the first of its kind--that appears to contain virtually no dark matter. It is an exceptional find since galaxies are commonly thought to contain more dark matter than the ordinary matter that makes up a galaxy's stars, gas and dust.

Also, it is generally accepted that galaxies first formed from concentrations of dark matter that act like "galaxy starters." They gravitationally attract ordinary, or baryonic, matter which eventually settles within the extant cloud of dark matter.

So, finding a galaxy with no dark matter raises the question: if the galaxy has no dark matter, how did it form?

"We thought all galaxies were made up of stars, gas and dark matter mixed together, but with dark matter always dominating," says Prof. Roberto Abraham from the University of Toronto and co-author of the Nature paper describing the discovery. "Now it seems that at least some galaxies exist with lots of stars and gas and hardly any dark matter. It is pretty bizarre."

According to the paper's lead author, Prof. Pieter van Dokkum from Yale University, "It challenges the standard ideas of how we think galaxies work. This result also suggests that there may be more than one way to form a galaxy." The paper appears in the March 29 issue of the journal Nature.

The newly discovered galaxy is called NGC1052-DF2, or DF2 for short. In addition to the dearth of dark matter, DF2 is unusual in another way: it is roughly the size of our Milky Way Galaxy, but contains only 1/200 the number of stars.

It was first identified as a peculiar object using the Dragonfly Telescope Array, a ground-breaking instrument for detecting very faint astronomical objects, conceived of and built by van Dokkum and Abraham.

Dragonfly is a multi-lens array that uses commercially available telephoto lenses with specially-coated optical glass that reduces scattered light. Having grown from a three-lens array in 2013, it now comprises 48 lenses and is the world's largest, all-refracting telescope. Previously, van Dokkum, Abraham and their collaborators used the array to discover a new class of galaxies known as Ultra-Diffuse Galaxies (UDG).

Once the team identified the unusual nature of DF2, they conducted follow-up observations. From the W.M. Keck Observatory, they measured the velocity of clusters of stars (called globular clusters) within DF2 and found they were moving slower than expected. Using these velocities, they calculated the galaxy's mass and determined that the visible stars, gas and dust in DF2 accounted for most of the mass and that there was only 1/400th the amount of dark matter expected.

Follow-up observations with the Hubble Space Telescope revealed DF2's other unusual qualities. Unlike typical spiral galaxies, DF2 has no dense, central region; nor spiral arms or a disk. And unlike elliptical galaxies, it has no central black hole.

"I spent an hour just staring at the Hubble image," says van Dokkum, "This thing is astonishing: a gigantic blob that you can look through. It's so sparse that you see all of the galaxies behind it. It is literally a see-through galaxy."

DF2 is located in a cluster of galaxies that is dominated by a giant elliptical galaxy designated NGC 1052. The astronomers speculate that the birth and formation of DF2 in the dynamic environment of the cluster could have been influenced by the giant galaxy. Or, a cataclysmic event within DF2 such as an eruption of star formation could have cleared the galaxy of all its gas and dark matter.

"We're currently undertaking a survey to find more objects like DF2," says Abraham. "Dragonfly is good at finding these sorts of objects. Maybe we're only seeing the tip of the iceberg."
-end-
Paper: A Galaxy Lacking Dark Matter

CONTACT INFORMATION:

Prof. Roberto Abraham
Department of Astronomy & Astrophysics
Dunlap Institute for Astronomy & Astrophysics (Associate)
University of Toronto
p: 416-946-7289
e: abraham@astro.utoronto.ca

Chris Sasaki
Communications Coordinator | Press Officer
Dunlap Institute for Astronomy & Astrophysics
University of Toronto
p: 416-978-6613
e: csasaki@dunlap.utoronto.ca
w: dunlap.utoronto.ca

The Dunlap Institute for Astronomy & Astrophysics at the University of Toronto is an endowed research institute with over 70 faculty, postdocs, students and staff, dedicated to innovative technology and instrumentation, ground-breaking research, world-class training, and public engagement. The research themes of its faculty and Dunlap Fellows span the Universe and include: optical, infrared and radio instrumentation; Dark Energy; large-scale structure; the Cosmic Microwave Background; the interstellar medium; galaxy evolution; cosmic magnetism; and time-domain science.

The Dunlap Institute, Department of Astronomy & Astrophysics, Canadian Institute for Theoretical Astrophysics, and Centre for Planetary Sciences comprise the leading centre for astronomical research in Canada, at the leading research university in the country, the University of Toronto.

The Dunlap Institute is committed to making its science, training and public outreach activities productive and enjoyable for everyone, regardless of gender, sexual orientation, disability, physical appearance, body size, race, nationality or religion.

Dunlap Institute for Astronomy & Astrophysics

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