The Making of a Monster, Caught by Accident
The Making of a Monster, Caught by Accident
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Monday, July 1, 2013, at 8:00 AM
One of the most overwhelming things we have learned from studying
astronomy in the past century—and it’s quite a list—is that entire
galaxies collide.
I cannot overstate how awe-inspiring that is. A galaxy is a vast
thing: a self-gravitating collection of tens or hundreds of billions of
stars, countless clouds of gas and dust massive enough to create
billions more stars, and all of this (not including the dark matter,
which we cannot directly see) spread out over 100,000 light-years—a
million trillion kilometers.
By itself a galaxy is mind-crushing structure. But then to find that
they can careen through space and physically collide with another such
monster … it’s difficult to grasp the enormity of such an event.
And yet collisions happen, and they happen often. And when they do,
the result can be such beauty as to make even the most jaded cynic weep:
The collision of two galaxies, a train wreck on a truly cosmic scale. Click to bronsonalphenate.
Photo by ESA/Hubble & NASA, Acknowledgement: Luca Limatola
Photo by ESA/Hubble & NASA, Acknowledgement: Luca Limatola
This is ESO 1327-2041,
a pair of colliding galaxies located 240 million light-years distant
from Earth, observed by the Hubble Space Telescope. One of the galaxies
is a lenticular, a lens-shaped disk like a spiral galaxy without the
spiral arms, and the other is a more normal spiral. At least, it used to
be.
At some point, a few million years ago, the two galaxies first made a
close pass, circled around, and then slammed into each other. It looks
to me that the lenticular is passing right through the heart of the
spiral, the two coincidentally centered on each other at the time we see
this event, midcollision. The arms of the spiral wrap right around the
lenticular, looking like a cosmic leukocyte about to engulf a marauding
bacterium.
When galaxies collide, strange things happen. As they approach, the
gravity of one pulls on the near side of the other more than the far
side—that’s because gravity weakens with distance. The net effect is
that the galaxies can get stretched out and distorted, and huge streams
of stars can be drawn out or ejected from the parent galaxy.
Diagram showing the forensics of the collision.
Illustration by Keeney, et al. from their paper.
Illustration by Keeney, et al. from their paper.
Look again at the picture. See the long fuzzy streak going up out of
the galaxies? That’s just such a star stream. But it gets better; the
bright knot near the top may actually be the nucleus of the spiral
galaxy, tossed out by the interaction.
I phrase that cavalierly, but it’s an event so powerful words are grossly inadequate. There are millions of stars in that glowing plume. Millions. That’s how much might is locked up in an event like this; the power to heave around entire stars by the millions.
It makes the hairs on the back of my neck stand up.
This collision is not done; eventually the two galaxies will merge
completely, their material mixed, and they’ll join into one larger
galaxy. All the most massive galaxies in the Universe have undergone
this process at one level or another, growing into their enormous status
by mutual cannibalism.
And after all that, amazingly, the collision pictured is not why
those galaxies were observed using Hubble in the first place!
It just so happens that there is a much more distant quasar coincidentally near those galaxies in the sky. Quasars are intensely bright galaxies, ones that have monster supermassive black holes in their cores, actively gobbling down matter, heating it up to fierce temperatures, and blasting out light across the electromagnetic spectrum.
It just so happens that there is a much more distant quasar coincidentally near those galaxies in the sky. Quasars are intensely bright galaxies, ones that have monster supermassive black holes in their cores, actively gobbling down matter, heating it up to fierce temperatures, and blasting out light across the electromagnetic spectrum.
The collision of the galaxies has tossed out a lot of gas, and that
material is absorbing the light from the quasar. This type of absorption
is interesting to astronomers; it’s like a fingerprint telling you how
far the quasar and gas are. Gas that is otherwise dark between us and
the quasar can be detected this way. Given that quasars can be seen from
billions of light-years away, the Universe has given us a method to map
itself for free.
That’s why astronomers pointed Hubble at ESO 1327-2041:
It happened to be between us and a more interesting quasar. Until
Hubble’s clearer vision was set upon it, the galaxy was thought to
simply be a peculiar type called a polar ring galaxy.
Oh, how I love astronomy! One of the most powerful and awe-inspiring
events in the entire Universe, the collision between two huge galaxies,
and its true nature was only discovered by accident.
But once found, the astronomers looked at it on purpose to learn more
about it, and surprises are part of the fun. It’s a big Universe, full
of such delights, and there’s still very much left to learn about it.
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