The comet's entrance coincides with
a bright CME racing away from the sun's southwestern
limb. Astronomers have been wondering what might
happen if a
CME strikes Comet ISON. This CME, however, will
probably miss. The source of the cloud is a farside
active region, which is not directly facing the
comet.
NASA's STEREO-A spacecraft is also
monitoring the comet. Click to view a high-resolution
movie (32 MB), which compresses 96 hours into less
than 1 minute:
The movie spans a 3+ day interval
from Nov. 21 to Nov. 24 roughly centered on the
period when astronomers at the IRAM telescope in
Spain recorded fading emission lines from the comet's
core. Zoom your movie-player to full screen: Although
"puffs" of material can be seen billowing
down the comet's tail, the comet itself does not
appear to be disintegrating. So what caused the
fade...?
"I will admit that I was pretty
worried yesterday morning when reports of lower
production rates came in," says Matthew Knight
of the Lowell Observatory and NASA's Comet ISON
Observation Campaign. "However, the STEREO-A
brightness has increased steadily over the subsequent
36 hr, and I'm more optimistic again. My off-the-cuff
thought is that there was an [outburst of dust,
which dampened the emission lines] from roughly
Nov 20-22, and it has returned to brightening again."
Astronomer Karl Battams of NASA's
Comet ISON Observing Campaign urges readers to remember
the following: "Comet ISON is a dynamically
new sungrazing comet, fresh in from the Oort Cloud,
and the last time we saw an object like this was
never! Furthermore, a sungrazing
comet just days from perihelion has never been studied
in this kind of detail - we're breaking new ground!
When we factor in your standard 'comets are unpredictable'
disclaimer, what we have is a huge recipe for the
unknown."
Stay tuned for updates.Source:
http://www.spaceweather.com/
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