Gravity's Grin
Albert
Einstein's
general theory of relativity, published over 100 years
ago, predicted the phenomenon of gravitational lensing.
And that's what gives these distant galaxies such a whimsical
appearance,
seen
through the looking glass of X-ray and optical
image data from the Chandra and Hubble space telescopes.
Nicknamed the Cheshire Cat galaxy group, the group's two
large elliptical galaxies are suggestively framed by arcs.
The arcs are optical images
of distant background galaxies
lensed by the foreground group's total distribution
of gravitational mass.
Of course, that gravitational mass is dominated
by dark matter.
The two large elliptical "eye" galaxies represent
the brightest members of their own galaxy groups which are merging.
Their relative collisional speed of nearly 1,350 kilometers/second
heats gas to millions of degrees producing the X-ray glow shown
in purple hues.
Curiouser about
galaxy group mergers?
The Cheshire Cat
group
grins
in the constellation Ursa Major, some 4.6 billion light-years away.