[meteorite-list] Comet ISON May Be Breaking Up

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Tue, 19 Nov 2013 10:17:46 -0800 (PST)
Message-ID: <201311191817.rAJIHk8T009697_at_zagami.jpl.nasa.gov>

http://www.mps.mpg.de/en/aktuelles/pressenotizen/pressenotiz_20131119.html

Comet ISON unfolds its wings
Max Planck Institute for Solar System Research
November 19, 2013

New images of ISON indicate that the comet lost individual fragments in
the past days.

One or more fragments may have detached from comet ISON in the past days,
as two wing-shaped features in the comet's atmosphere suggest. Scientists
from the Max Planck Institute for Solar System Research (MPS) in Germany
and the Wendelstein Observatory of the Ludwig-Maximilians-University in
Munich (Germany) discovered these features in images taken at the end
of last week. The fragmentation may offer an explanation for the comet's
recent outburst of activity.

On its journey towards the Sun, comet ISON has disappointed many hobby
astronomers in the past weeks: its brightness did not increase as strongly
as previously assumed. On November 28th, 2013 the comet will fly by the
Sun in a distance of only 1.8 million kilometers. However, on November
7th, ISON's light intensity increased abruptly; several observers announced
a sudden rise in the comet's activity.

Images of ISON taken by scientists from the MPS and the Wendelstein Observatory
now offer possible evidence for the cause of this outburst. On November
14th and 16th, 2013 the researchers aimed their telescope towards the
approaching visitor.

The researchers' analyses show two striking features within the comet's
atmosphere that protrude from the nucleus in a wing-like fashion. While
these so-called coma wings were still rather faint on November 14th, they
dominate the images taken two days later. "Features like these typically
occur after individual fragments break off the nucleus", Dr. Hermann B?hnhardt
from the MPS explains.

As does the nucleus, these fragments emit gas and dust. Where the emissions
from the comet and its fragments meet, a kind of boundary layer is formed
that often takes a wing-like form as seen from Earth. Whether or not this
fragmentation process led to the recent outburst cannot be determined
with certainty, says B?nhardt. However, in the cases of other comets,
a connection between both phenomena has been well established.

In the images taken of comet ISON, the coma wings cannot be seen with
the naked eye. Instead, numerical methods were necessary to make them
visible. To this end the researchers comb through the comet's coma looking
for spatial changes in the light intensity. The uniformly bright background
of the comet's atmosphere is numerically eliminated so as not to outshine
the fainter structures hidden beneath. "Our calculations imply that ISON
lost only one fragment or very few at the most", says B?hnhardt.

How the comet will develop in the next weeks is still unclear. "However,
according to past experience, comets that have once lost a fragment tend
to do this again", says B?hnhardt.
 
[Image]
Figure 1: This image taken on November 16th, 2013 shows ISON's atmosphere
with two wing-like features resembling the letter U. For orientation,
the comet's nucleus position is shown as a bright spot in the center.
(Credits: Wendelstein Observatory of the LMU/MPS)

Contact

Dr. Birgit Krummheuer
Press and Public Relations
Max Planck Institute for Solar System Research
Max-Planck-Stra?e 2
37191 Katlenburg-Lindau
Tel.: 05556 979 462
Fax: 05556 979 240
Mobil: 0173 3958625
Email: krummheuermps.mpg.de

Dr. Hermann B?hnhardt
Max Planck Institute for Solar System Research
Max-Planck-Stra?e 2
37191 Katlenburg-Lindau
Tel.: 05556 979 545
Email: Boehnhardtmps.mpg.de
Received on Tue 19 Nov 2013 01:17:46 PM PST