NGC 7252: Spiral Disk and Globular Star Clusters at the Core of a Colliding Galaxy
A NASA Hubble Space Telescope (HST) 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 false-color image has been subject to computer image reconstruction. The strong spiral structure is 10,000 light-years across (7 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 globular star clusters are concentrated near the galaxy's core. Estimated to be mostly between 50 and 500 million years old, they were apparently born following the collision of two disk-shaped galaxies about a billion years ago.
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.
The globular clusters found in NGC 7252 are considered the progenitors of similar clusters that orbit our own Milky Way galaxy.
This discovery provides some of the best evidence to date for solving more than half a century of theory and conjecture about how giant elliptical galaxies form.
Co-investigators: : Francois Schweizer of the Carnegie Institution of Washington, Washington, D.C., and Claus Leitherer, Kirk Borne, and Carmelle Robert of STScI.