Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005dps....37.6608f&link_type=abstract
American Astronomical Society, DPS meeting #37, #66.08; Bulletin of the American Astronomical Society, Vol. 37, p.772
Astronomy and Astrophysics
Astronomy
Scientific paper
The opposition surge of Saturn's rings has been measured from a long-term, uniform series of observations with the Hubble Space Telescope's (HST) Wide Field and Planetary Camera 2 (WFPC2). Extending from 1996--2005, the measurements spanned nearly the full range of ring opening (3o<|B|<26o) and solar phase (0o<α <6o) angles accessible from the Earth, using UBVRI filters. The rings were observed 3--7 times per year, concentrating on near opposition. The spatial resolution of the Planetary Camera (PC), ≃300 km/pixel, enabled us to measure radial variations in the opposition surge in the main rings. During a particularly favorable alignment of the Sun, Earth, and Saturn in January 2005, we observed the rings at exact opposition, with the minimum phase angle limited only by the angular semidiameter of the Sun as seen from Saturn (≃0.02o), accounting for solar limb-darkening. The opposition surge is quite strong throughout the entire ring system, with a narrow spike near exact opposition: [I/F(0o)]/[I/F(0.5o)]=1.4 for the C ring, and 1.3 for the A and B rings, with a weak wavelength dependence. The opposition surge results from a combination of mutual interparticle shadowing and intrinsic brightening (for example, due to coherent backscatter or regolith shadowing). From photometric models that account for particle size distributions, ring volume filling factors, and multiple scattering (Salo et al., this meeting), we find that the mutual shadowing effect saturates at α <0.5o, and we attribute the sharp core of the opposition surge to intrinsic brightening. For example, for B=23o, between α =0o and 6o, the mutual shadowing contribution to the opposition surge [I/F(0o)]/[I/F(6o)] is 1.1 in the C ring and 1.23 in the B ring; the intrinsic brightening is 1.78--1.8 in the C ring and 1.39--1.46 in the B ring, decreasing slightly with increased wavelength.
Dones Luke
French Richard G.
McGhee Colleen Anne
Salo Heikki
Verbiscer Anne
No associations
LandOfFree
HST Observations of the Opposition Effect in Saturn's Rings 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 HST Observations of the Opposition Effect in Saturn's Rings, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and HST Observations of the Opposition Effect in Saturn's Rings will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-953207