Hubble image archive

Supersonic Comet-Like Objects (right) in Heart of the Cartwheel Galaxy (left)

Researchers analyzing the Hubble Space Telescope's dramatic pictures of the Cartwheel galaxy have discovered immense comet-like clouds of gas speeding through the heart of the galaxy at nearly 700,000 mph.Located 500 million light-years away in the constellation Sculptor, the gal...

Date
Jan 1, 1996
Mission
Hubble Space Telescope
Archive ID
hubblesite-images-1996-36-457-image
By

Researchers analyzing the Hubble Space Telescope's dramatic pictures of the Cartwheel galaxy have discovered immense comet-like clouds of gas speeding through the heart of the galaxy at nearly 700,000 mph.

Located 500 million light-years away in the constellation Sculptor, the galaxy looks like a wagon wheel. The galaxy's nucleus is the bright object in the center of the image; the spoke-like structures are wisps of material connecting the nucleus to the outer ring of young stars. The galaxy's unusual configuration was created by a nearly head-on collision with a smaller galaxy about 200 million years ago.

This close-up image of the galaxy's nucleus reveals the comet-like knots of gas. These knots are mostly confined to the core's left side and appear as white streaks inside the blue ring. The "heads" are a few hundred light-years across; the tails are more than 1,000 light-years long, the longest of which is nearly 5,000 light-years. The structures look like comets because they probably were spawned by a collision between high-speed and slower-moving material. This collision created an arrowhead-shaped pattern called a bow shock, which is similar to the wake of a boat speeding across a lake.

Credits

Curt Struck and Philip Appleton (Iowa State University), Kirk Borne (Hughes STX Corporation), and Ray Lucas (Space Telescope Science Institute), and NASA

Image Details

About The Object
Object NameCartwheel Galaxy
R.A. Position00h 37m 41.09s
Dec. Position-33° 42' 59.0"

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Source

Image and source material are credited to the official mission archive linked below.

View on NASA.gov

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