Credit & Copyright: Lynette
Cook
Explanation:
For astronomers,
close binary star system BD+20 307 originally stood out because it
is extremely dusty.
A substantial amount of
warm dust surrounding it causes
the system to appear exceptionally bright at
infrared wavelengths.
Of course, dust associated with planet formation is often
detected
around young stars, stars only a few
million years old.
But the BD+20 307 system has now been found to be at least a few
billion years old,
an age comparable to the age of our own Solar System.
The large amount of warm dust is
likely the debris from a relatively recent
collision of planet-sized
objects on the scale of, say, Earth and Venus,
in the BD+20 307 system.
Reminiscent of the classic scifi novel
When
Worlds Collide,
the dramatic illustration offers a depiction of
the catastrophic event.
Ironically, this indirect evidence of a destructive
planetary collision could also be the first indication that
planetary
systems can form around
close binary stars.
BD+20 307 is about 300 light-years distant toward the headstrong
constellation Aries.
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& Michigan Tech. U.
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Publikacii s klyuchevymi slovami:
binary star - dust - planets - dvoinye zvezdy - Planety u drugih zvezd
Publikacii so slovami: binary star - dust - planets - dvoinye zvezdy - Planety u drugih zvezd | |
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