Volume 422, Number 1, July IV 2004
|Page(s)||L19 - L21|
|Published online||06 July 2004|
Letter to the Editor
Rosetta target comet 67P/Churyumov-Gerasimenko*
Postperihelion gas and dust production rates
ESA Research and Scientific Support Department, ESTEC, Postbus 299, 2200 AG Noordwijk, The Netherlands e-mail: Rita.Schulz@rssd.esa.int
2 Sterrewacht Leiden, Postbus 9513, 2300 RA Leiden, The Netherlands e-mail: firstname.lastname@example.org
3 Max-Planck-Institute for Aeronomy, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany e-mail: email@example.com
Corresponding author: R. Schulz, Rita.Schulz@rssd.esa.int
Accepted: 5 June 2004
The evolution of the activity and composition of the coma of Rosetta target comet 67P/Churyumov-Gerasimenko was studied along its postperihelion orbit from 2.29 AU to 3.22 AU. The comet had a major drop of activity between 2.5 AU and 2.9 AU, which manifested most obviously in its light curve (the brightness decreased by 3 mag), but is also confirmed by the production rates derived from spectrophotometric measurements. The strong decrease of activity indicates a change in the outgassing behaviour of the nucleus and might be due to water sublimation becoming less efficient. The spectrophotometric measurements at 2.9 AU show that the coma is at least slightly depleted in C2 with respect to CN.
Key words: comets / Rosetta / 67P/Churyumov-Gerasimenko / production rates
© ESO, 2004
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.