Untitled Document
NASA/CXC/SAO
It's often said the the
Andromeda Galaxy is like our own Milky Way. Sure, there are similarities. The
two are destined
to collide and probably merge, for one thing. And they share a similar shape,
both being spiral galaxies with central bulges loaded with stars.
But there is one big difference:
Andromeda's presumed central black hole
packs the mass of 30 million suns. The Milky Way's black hole is estimated to
be a mere 2.6 million solar masses.
You can find the supermassive
black hole in this image of Andromeda from NASA's Chandra X-ray Observatory.
See the blue dot? That's actually a relatively cool X-ray source, "only"
about a million degrees Celsius. Nobody knows what it is. When Chandra first
imaged the region in 2000, researchers thought the blue dot corresponded to
the exact center of the galaxy -- the position of the suspected central black
hole. But it should have been hotter, so the scientists were puzzled.
Just above the blue dot
is a bright yellow dot, several tens of times hotter. That's radiation from
around the black hole, astronomers now believe, based on refined Chandra imaging
in 2001 (and some help from the Hubble Space Telescope) that showed the cooler,
blue X-ray source is actually about 10 light-years south of the galactic center.
The X-rays are given off
by gas that swirls toward the gravity sink and is superheated as it approaches
the speed of light.
So what about all those
other yellow dots? They are most likely what astronomers call X-ray binary systems.
In one of these, a normal star is orbited by a dense stellar corpse, either
a stellar-mass black hole or a neutron star. The dense object siphons matter
from the normal star, setting up a miniature version of the same scenario that
generates X-rays in the supermassive black hole at the galactic center.
At just 2 million light-years
away, Andromeda is our nearest large galactic neighbor. [Learn
more about the impending collision]
-- Robert
Roy Britt
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