Credit: ESA/Hubble & NASA
This delicate smudge in deep space is far more
turbulent than it first appears. Known as IRAS 14348-1447 — a name
derived in part from that of its discoverer, the Infrared Astronomical Satellite
(IRAS for short) — this celestial object is actually a combination of
two gas-rich spiral galaxies. This doomed duo approached one another too
closely in the past, gravity causing them to affect and tug at each
other and slowly, destructively, merge into one. The image was taken by Hubble’s Advanced Camera for Surveys (ACS).
IRAS 14348-1447 is located over a billion light-years away from us. It is one of the most gas-rich examples known of an ultraluminous infrared galaxy, a class of cosmic objects that shine characteristically — and incredibly — brightly in the infrared part of the spectrum. Almost 95% of the energy emitted by IRAS 14348-1447 is in the far-infrared!
The huge amount of molecular gas
within IRAS 14348-1447 fuels its emission, and undergoes a number of
dynamical processes as it interacts and moves around; these very same
mechanisms are responsible for IRAS 14348-1447’s own whirling and
ethereal appearance, creating prominent tails and wisps extending away
from the main body of the galaxy.
Source: ESA/Hubble/News
