A Grazing Encounter Between Two Spiral Galaxies

A Grazing Encounter Between Two Spiral Galaxies
From the Hubble Space Telescope
In the constellation Canis Major, two spiral galaxies are seen nearly colliding in images taken by NASA's Hubble Space Telescope and its Wide Field Planetary Camera 2. The larger and more massive galaxy is NGC 2207 (on the left), and the smaller one on the right is IC 2163. Strong tidal forces from NGC 2207 have distorted the shape of IC 2163, flinging out stars and gas into long streamers stretching out a hundred thousand light-years toward the right-hand edge of the image.
Computer simulations, by a team led by Bruce and Debra Elmegreen, demonstrate the timescale over which galactic collisions occur. In addition measurements made with the National Science Foundation's Very Large Array Radio Telescope in New Mexico reveal the motions of the galaxies and aid the reconstruction of the collision. IC 2163 is swinging past NGC 2207 in a counterclockwise direction, having made its closest approach 40 million years ago. But, IC 2163 does not have sufficient energy to escape from the gravitational pull of NGC 2207. Trapped in their mutual orbit around each other, these two galaxies will continue to distort and disrupt each other. Eventually, billions of years from now, they will merge into a single, more massive galaxy. Many present-day galaxies, including the Milky Way, were assembled from a similar process of coalescence of smaller galaxies occurring over billions of years.
The high resolution of this image reveals dust lanes in the spiral arms of NGC 2207, clearly silhouetted against IC 2163, which is in the background. Hubble also reveals a series of parallel dust filaments extending like fine brush strokes along the tidally stretched material on the right-hand side. The large concentrations of gas and dust in both galaxies may well erupt into regions of active star formation in the near future.
Image Title: A Grazing Encounter Between Two Spiral Galaxies
based on press release for PHOTO NO.: STScI-PRC99-41

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Last modified on Sunday, December 17, 2000