Au revoir!

March 13th, 2009 sfair Posted in Astronomy, Personal, PlanetaryRings, Saturn, Uranus Comments Off

I

will go to
Free Image Hosting at www.ImageShack.us

to study the ring system of
Free Image Hosting at www.ImageShack.us

and I’ll be right back. Maybe not.

AddThis Social Bookmark Button

Analysis of the Saturn’s F-ring Region

October 2nd, 2007 sfair Posted in Astronomy, Personal, PlanetaryRings, Saturn Comments Off

 

After a long time my Master’s Thesis is online. In this work, entitled “Analysis of the Saturn’s F-ring Region”, we analyse the influence of Prometheus and Atlas on F-ring particles and also on two diffuse rings.

The text is available in PDF format (4.3MB) (I’ll convert to djvu soon). You can download it here (90 pages, pt_br).
Comments, suggestions and job proposals are welcome :)

The abstract:

The Cassini-Huygens arrival into the Saturnian system brought a large amount of data about the satellites and rings. Two diffuse rings were found in the region between the A ring and Prometheus. R/2004 S1 is coorbital to Atlas and R/2004 S2 is close to Prometheus.
In this work we analyse the closest approach between Prometheus and both rings. As a result we have found that at each period of the satellite a gap is created in the inner F-ring’s strand and waves are formed in the further strands. Prometheus also scatters particles from F-ring and a similar behaviour occurs in the R/2004 S2 ring, with gap formation and particle scattering. The numerical simulations has shown that Prometheus does not influence the R/2004 S1 ring but Atlas is responsible for the formation of three regimes in this ring, as expected for a satellite embedded in a ring.
The determination of Lindblad and corotation resonances showed that there is an overlap of resonances in the region of the R/2004 S2 ring. Furthermore, the computation of the Lyapunov Characteristic Exponent has revealed that the R/2004 S2 ring lies in a chaotic region.
When solar radiation pressure effects are considered, micrometre-sized particles from F-ring decay and collide with Prometheus, except for few particles of 1µm which cross Prometheu’s orbit and reach the R/2004 S2 region. The solar radiation pressure affects the behavior of the R/2004 S1 ring leading to collisions between Atlas and these small particles, although some of them decay in direction of Saturn.

Keywords: F-ring, planetary rings dynamics, resonances, Lyapunov Characteristic Exponent, solar radiation pressure

AddThis Social Bookmark Button