Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005dps....37.4414j&link_type=abstract
American Astronomical Society, DPS meeting #37, #44.14; Bulletin of the American Astronomical Society, Vol. 37, p.1568
Astronomy and Astrophysics
Astronomy
Scientific paper
We observed comet 9P/Tempel 1 before and after the impact in the visible from the Earth with the 1-m telescope at Pic du Midi Observatory and with the narrow angle camera (OSIRIS/NAC) aboard the ROSETTA spacecraft. The latter observations allowed an uninterrupted monitoring from 120 hrs pre-impact to 250 hrs post-impact, but at a low spatial resolution (1 pixel projected to 1500 km at the comet). The former observations offered a less extensive temporal coverage (about 3 hrs per night from June 25 to July 7) but at a higher spatial resolution (1 pixel projected to 600 km at the comet). The angle of 27 degrees between the two lines-of-sight further allowed to follow the same event from two different viewing angles. We present a combined preliminary analysis of the images obtained with both instruments. The dust production rate is monitored via two proxies, the [Afrho] parameter and the dust cross section, which is more appropriate in the case of a non-canonic coma. This indicates that the comet went back to its normal, pre-impact state within about 7 days of the impact thus showing that it did not create a detectable active region. Dust structures were found and followed in the coma and in the dust tail and we discuss their significance. Several spectral analysis of the pre-impact light curve reveal a periodic variation attributed to the rotation of the nucleus with a period of about 41 hrs.
Colas Francois
Faury Guillaume
Gutierrez Pablo
Hviid Stubbe
Jorda Laurent
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