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News Release Archive:

News Release 894 of 966

May 25, 1993 12:00 AM (EDT)

News Release Number: STScI-1993-11

What Happens When Galaxies Collide? Hubble Space Telescope Finds New Surprises

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Image: Merging galaxy NGC 7252 From the Ground (left) and From Hubble (right)

Merging galaxy NGC 7252 From the Ground (left) and From Hubble (right)STScI-PRC1993-11b

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ABOUT THIS IMAGE:

[Left] Ground-based Telescopic Photograph NGC 7252 has been considered the prototypical example of a merger between two disk-shaped galaxies. The galaxy has a pair of long tails that are unambiguous evidence of the effects of gravitational tidal forces from a galaxy merger. The galaxy is nicknamed the "Atoms-for-Peace" galaxy because its stars form a bizarre loop-like structure that resembles a schematic diagram of electrons orbiting an atomic nucleus. (In December 1953, U.S. President Dwight 0. Eisenhower made his "Atoms for Peace" speech to foster peaceful applications of nuclear energy.) The galaxy is located 300 million light-years away in the constellation Aquarius.

[Right] Hubble Space Telescope Planetary Camera Image of Galaxy Core A NASA Hubble Space Telescope image of the core of the peculiar galaxy NGC 7252 reveals a striking "mini-spiral" disk of gas and stars, and about 40 exceptionally bright and young globular star clusters.

The visible light image was taken with the Wide Field and Planetary Camera (WFPC) in PC mode, on October 10, 1992. The image has been subject to computer image reconstruction. The strong spiral structure is 10,000 light-years across (3.5 arc seconds); the entire picture is 46,000 light-years across. Hubble's resolution is so good the astronomers can measure the diameters of the clusters (0.04 arc seconds, the apparent size of a dime at a distance of 60 miles). They turn out to be about 60 light-years in diameter, the same size as globular clusters that orbit our Milky Way galaxy.

The pinwheel-shaped disk of gas and young stars has an uncanny resemblance to a face-on spiral galaxy. Yet the disk is only 1/20 the diameter of the total galaxy. The disk was probably fueled by the collision.

Object Name: NGC 7252

Image Type: Astronomical/Annotated

Left Credit: Dr. Francois Schweizer, taken with 4-meter telescope at the Cerro Tololo Inter-American Observatory.

Right Credit: B. Whitmore (STScI), and NASA

Co-investigators: Francois Schweizer of the Carnegie Institution of Washington, Washington, D.C., and Claus Leitherer, Kirk Borne, and Carmelle Robert of STScI.

NEWS RELEASE IMAGES

The above montage includes these images:

NGC 7252: Spiral Disk and Globular Star Clusters at the Core of a Colliding Galaxy Image Type: Astronomical NGC 7252: Spiral Disk and Globular Star Clusters at the Core of a Colliding GalaxyPRC1993-11

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