Title: The chemical composition of CO-rich comet C/2009 P1 (Garradd) at Rh = 2.4 and 2.0 AU before perihelion Authors: L. Paganini, M. J. Mumma, G. L. Villanueva, M. A. DiSanti, B. P. Bonev, M. Lippi, H. Boehnhardt
We quantified ten parent volatiles in comet C/2009 P1 (Garradd) before perihelion, through high-dispersion infrared spectra acquired with CRIRES at ESO's VLT on UT 2011 August 07 (Rh = 2.4 AU) and September 17-21 (Rh = 2.0 AU). On August 07, water was searched but not detected at an upper limit (3{\sigma}) of 2.1 x 10^28 s-1, while ethane was detected with a production rate of 6.1 x 10^26 s-1 (apparent mixing ratio > 2.90%). On September 17-21, the mean production rate for water was 8.4 x 10^28 s-1, and abundance ratios (relative to water) of detected trace species were: CO (12.51%), CH3OH (3.90%), CH4 (1.24%), C2H6 (1.01%) and HCN (0.36%). Upper limits (3{\sigma}) to abundances for four minor species were: NH3 (1.55%), C2H2 (0.13%), HDO (0.89%) and OCS (0.20%). Given the relatively large heliocentric distance, we explored the effect of water not being fully sublimated within our FOV and identified the 'missing' water fraction needed to reconcile the retrieved abundance ratios with the mean values found for "organics-normal". The individual spatial profiles of parent volatiles and the continuum displayed rather asymmetric outgassing. Indications of H2O and CO gas being released in different directions suggest different active vents and/or the possible existence of polar and apolar ice aggregates in the nucleus. The high fractional abundance of CO identifies comet C/2009 P1 as a CO-rich comet.
Comet C/2009 P1 Garradd is best seen during the early morning in February and March. The comet is visible using binoculars but fades to 8th magnitude at the end of March. The comet is close to the star Kochab in Ursa Minor on the 6th March and the "Pointers" in Ursa Major on 21st March.
This is a time-lapse video of Comet Garradd C/2009 P1 passing near the Globular Cluster M71 on August 26, 2011. 33 five-minute frames taken with a 6" Astro-Tech RC telescope and Modified Canon 450D DSLR camera were used for the video. The time lapse covers a three hour period from 9:00pm to 12:08am.
On the 2 - 3rd of September, the magnitude 7.8, comet C/2009 P1 (Garradd) will pass close to Brocchi's Cluster (the Coathanger) in the constellation Cygnus.