Colliding Vortices

Colliding Galaxy Pair Arp 142

NASA has released this Hubble Space Telescope composite image [taken in visible, red, and infrared light] of two galaxies colliding 326 million light years away.

The collision was originally catalogued as Arp 142 by the legendary Halton C Arp in the 1960s and as NASA wryly notes it is a “messy business”.

The weaker spiral vortex of NGC 2936 is clearly being slowly drawn in and compressed by the stronger elliptical vortex of galaxy NGC 2937.

However, it appears that NASA doesn’t believe this visual evidence presented in this image because they quaintly state that the “galaxy’s orderly spiral” is being deformed into “giant tails like stretched taffy” because of “gravitational tidal interactions”.

Once part of a flat, spiral disk, the orbits of the galaxy’s stars have become scrambled due to gravitational tidal interactions with the other galaxy. This warps the galaxy’s orderly spiral, and interstellar gas is strewn out into giant tails like stretched taffy.

Gas and dust drawn from the heart of NGC 2936 becomes compressed during the encounter, which in turn triggers star formation. These bluish knots are visible along the distorted arms that are closest to the companion elliptical. The reddish dust, once within the galaxy, has been thrown out of the galaxy’s plane and into dark veins that are silhouetted against the bright starlight from what is left of the nucleus and disk.

The companion elliptical, NGC 2937, is a puffball of stars with little gas or dust present. The stars contained within the galaxy are mostly old, as evidenced by their reddish color. There are no blue stars that would be evidence of recent star formation. While the orbits of this elliptical’s stars may be altered by the encounter, it’s not apparent that the gravitational pull by its neighboring galaxy is having much of an effect.

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