Panning on the interacting galaxies Arp 87.

Hubble - graceful dance of interacting galaxies

30 October 2007

Two galaxies, containing a vast number of stars, swing past each other in a graceful dance choreographed by gravity, as seen by Hubble.

The pair of galaxies collectively known as Arp 87 is among the hundreds of interacting and merging galaxies known in our nearby Universe. The Arp 87 pair was originally discovered and catalogued by astronomer Halton Arp in the 1970s. The ‘Arp’s Atlas of Peculiar Galaxies’ is a compilation of astronomical photographs using the Palomar 200-inch Hale and the 48-inch Samuel Oschin telescopes.

Wide-field image of Leo and Arp 87

The resolution in this Hubble image shows exquisite detail and fine structure that was not observable when Arp 87 was first discovered in the 1970s.

The two main players comprising Arp 87 are NGC 3808 (the larger of the two galaxies, on the right, in the image below) and its companion NGC 3808A (on the left, in the image below). NGC 3808 is a nearly face-on spiral galaxy with a bright ring of star formation and several prominent dust arms. Stars, gas, and dust flow from NGC 3808, forming an enveloping arm around its companion. NGC 3808A is a spiral galaxy seen edge-on and is surrounded by a rotating ring that contains stars and interstellar gas clouds. The ring is situated perpendicular to the plane of the host galaxy disk and is called a ‘polar ring.’

Arp 87

As seen in other mergers similar to Arp 87, the corkscrew shape of the tidal material (or bridge of shared matter) between the two galaxies suggests that some stars and gas drawn from the larger galaxy have been caught in the gravitational pull of the smaller one.

The shapes of both galaxies have been distorted by their gravitational interaction with one another.

Interacting galaxies often exhibit high rates of star formation. Many lines of evidence – colours of their starlight, intensity of emission lines from interstellar gas, far-infrared output from heated interstellar dust – support this fact. Some merging galaxies have the highest levels of star formation we can find anywhere in the nearby Universe.

A zoom from a wide-field image of Leo towards the interacting galaxies Arp 87.

A major aspect of this excess star formation was properly revealed only when Hubble turned its imaging capabilities toward colliding galaxies. Among the observatory’s first discoveries was that galaxies with very active star formation contain large numbers of super star clusters – clusters more compact and richer in young stars than astronomers were accustomed to seeing in our galactic neighborhood.

Wide-field image of Leo and Arp 87

Arp 87 is in the constellation Leo, the Lion, approximately 300 million light-years away from Earth. These observations were taken in February 2007 with the Wide Field Planetary Camera 2. Light from isolated blue, green, red, and infrared ranges was combined to form this colour image.

Notes for editors

The Hubble Space Telescope is a project of international cooperation between ESA and NASA.

For more information, please contact:

Lars Lindberg Christensen, Hubble/ESA, Garching, Germany
E-mail: Lars @ eso.org

Ray Villard, Space Telescope Science Institute, Baltimore, USA
E-mail: Villard @ stsci.edu

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