Comet ISON Unfolds Its Wings and May Have Shed Fragments

©Max Planck Institute for Solar System Research

Comet ISON

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 28, 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, the researchers aimed their telescope towards the approaching visitor.

The researchers' analyzes 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 Boehnhardt 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 Boehnhardt. 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 Boehnhardt.

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 Boehnhardt.

PIO Contact:
Dr. Birgit Krummheuer
Max Planck Institute for Solar System Research
+49 5556 979-462, cell: +49 173 3958625
krummheuer@mps.mpg.de

Science Contact:
Dr. Hermann Boehnhardt
Max Planck Institute for Solar System Research
+49 5556 979-545
boehnhardt@mps.mpg.de

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