Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
Scientific paper
2009-11-29
Astronomy and Astrophysics
Astrophysics
Earth and Planetary Astrophysics
31 pages, 13 figures, accepted for publication in MNRAS
Scientific paper
Comet 133P/Elst-Pizarro is the first-known and currently best-characterised member of the main-belt comets, a recently-identified class of objects that exhibit cometary activity but which are dynamically indistinguishable from main-belt asteroids. We report here on the results of a multi-year monitoring campaign from 2003 to 2008, and present observations of the return of activity in 2007. We find a pattern of activity consistent with the seasonal activity modulation hypothesis proposed by Hsieh et al. (2004, AJ, 127, 2997). Additionally, recomputation of phase function parameters using data in which 133P was inactive yields new IAU parameters of H_R=15.49+/-0.05 mag and G_R=0.04+/-0.05, and linear parameters of m_R(1,1,0)=15.80+/-0.05 mag and Beta=0.041+/-0.005 mag/deg. Comparison between predicted magnitudes using these new parameters and the comet's actual brightnesses during its 2002 and 2007 active periods reveals the presence of unresolved coma during both episodes, on the order of ~0.20 of the nucleus cross-section in 2002 and ~0.25 in 2007. Multifilter observations during 133P's 2007 active outburst yield mean nucleus colours of B-V=0.65+/-0.03 mag, V-R=0.36+/-0.01 mag, and R-I=0.32+/-0.01 mag, with no indication of significant rotational variation, and similar colours for the trail. Finally, while 133P's trail appears shorter and weaker in 2007 than in 2002, other measures of activity strength such as dust velocity and coma contamination of nucleus photometry are found to remain approximately constant. We attribute changes in trail strength to the timing of observations and projection effects, thus finding no evidence of any substantial decrease in activity strength between 2002 and 2007.
Hsieh Henry H.
Jewitt David
Lacerda Pedro
Lowry Stephen C.
Snodgrass Colin
No associations
LandOfFree
The Return of Activity in Main-Belt Comet 133P/Elst-Pizarro does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Return of Activity in Main-Belt Comet 133P/Elst-Pizarro, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Return of Activity in Main-Belt Comet 133P/Elst-Pizarro will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-148553