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Hubble captures the pair of interacting galaxies Arp 87 [heic0717]

Hubble captures the pair of interacting galaxies Arp 87 [heic0717]

30 October 2007

This pair of galaxies, known collectively as Arp 87, is one of hundreds of interacting and merging galaxies known in our nearby Universe. Arp 87 was originally discovered and catalogued by astronomer Halton Arp in the 1970s. 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.

HST/WFPC2 image of the interacting galaxy pair Arp 87

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

The two main players comprising Arp 87 are NGC 3808 on the right (the larger of the two galaxies) and its companion NGC 3808A on the left. 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 orientated perpendicular to the plane of the host galaxy disk and is called a polar ring.

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 by the gravitational pull of the smaller one. The shapes of both galaxies have been distorted by their mutual gravitational interaction.

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 major aspect of this excess star formation could be 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 neighbourhood.

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 four isolated wavelength ranges (centred around 450, 555, 656 and 814 nm) was combined to form this colour image.

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

Image credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA)

Contact

Lars Lindberg Christensen
Hubble/ESA, Garching, Germany
Tel: +49-(0)89-3200-6306
Cellular: +49-(0)173-3872-621
E-mail: larseso.org

Ray Villard
Space Telescope Science Institute, Baltimore, USA
Tel: +1-410-338-4514
E-mail: villardstsci.edu

Keith Noll
Space Telescope Science Institute, Baltimore, USA
Tel: +1-410-338-1828
E-mail: nollstsci.edu

Last Update: 1 September 2019
15-Nov-2019 22:27 UT

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https://sci.esa.int/s/8OxOErA

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