Cassini Significant Events for 12/05/07 - 12/11/07

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Cassini Significant Events 
for 12/05/07 - 12/11/07

The most recent spacecraft telemetry was acquired on Tuesday, December 11,
from the Madrid tracking complex. The Cassini spacecraft is in an excellent
state of health and all subsystems are operating normally. Information on
the present position and speed of the Cassini spacecraft may be found on the
"Present Position" web page located at
http://saturn.jpl.nasa.gov/operations/present-position.cfm.

Wednesday, December 5 (DOY 339):

The S39 Science Operations Plan Update (SOPU) official port occurred today.
Inputs from participating instrument teams, Spacecraft Operations, and
Navigation were merged, and the reports delivered to the teams and AACS for
the end-to-end pointing analysis.

On Dec. 3, there was a large spike in Single Bit Errors (SBE) and Double Bit
Errors (DBE) on both SSRs.  Usually the SBEs run about 25-50 per hour.  This
spike lasted about 8 hours and got up to about 1850 per hour.  DBEs
typically run about 2-3 per hour.  This spike got up to 6 per hour. SBEs and
DBEs are believed to be caused by high energy particle hits. SBEs are
autonomously corrected by on-board error detection and correction (EDAC)
logic. DBEs in flight software are corrected by autonomous copies of the
code from redundant copies in the SSRs. DBEs in data regions of memory are
not corrected, but go away with the next writing of data into that area of
memory.

Thursday, December 6 (DOY 340):

With Cassini now on the outbound leg of the T38 Titan encounter, a Radio
Science (RSS) gravity science experiment, mirroring the one performed as
Cassini approached Titan on DOY 338, was executed during the downlink to
Earth.  For the remainder of the day, Imaging Science (ISS) produced images
of Saturn's smaller moons for orbital element determination and observed the
ring system, focusing on the diffuse rings and making a mosaic of the ring
system as a whole.

The S40 Aftermarket process was completed today.  However, Science Planning
is still working on reducing Cassini's requested 70m DSN coverage during the
Phoenix Entry/Descent/Landing (EDL) contention period.  Due to a hiatus in
sequence processing over the winter holidays, these changes aren't due until
Jan. 9, 2008.

Friday, December 7 (DOY 341):

As Cassini now swings outward beyond Saturn's magnetosphere, the
Magnetospheric and Plasma Science (MAPS) instruments resumed their
monitoring of solar wind conditions. The Visual and Infrared Mapping
Spectrometer (VIMS) observed bright stars to calibrate its sensors, and ISS
resumed its monitoring of Saturn's small satellites and produced a ring
mosaic.

Orbit Trim Maneuver (OTM) #137 was performed today. This is the cleanup
maneuver following the T38 encounter on Dec. 5.  The main engine burn began
at 11:15 PM PST. Telemetry immediately after the maneuver showed a burn
duration of 4.18 seconds, giving a delta-V of 0.68 m/s, as planned.   All
subsystems reported nominal performance after the maneuver.

Imaging scientists are putting together the story of how the small moons
orbiting near the outer rings of Saturn came to be. The moons began as
leftover shards from larger bodies that broke apart and filled out their
"figures" with the debris that made the rings.  For the full story link to:
http://saturn.jpl.nasa.gov/news/press-release-details.cfm?newsID=795

Uplink Operations began sending the Instrument Expanded Block files for S36
today.  Seven files for ISS, VIMS, Composite Infrared Spectrometer (CIRS),
Optical Navigation, Ultraviolet Imaging Spectrograph (UVIS), and Cassini
Plasma Spectrometer (CAPS) were sent.  The remaining files will be sent
Sunday and the background sequence will go up on Monday.  S36 will begin
execution on Friday, Dec. 14.

Sunday, December 9 (DOY 343)

Today the SSPS for the SRU-B replacement heater was tripped from OFF to
TRIPPED.  The SSPS autonomous trip response fault protection algorithm
turned it back to OFF several minutes later.   There appears to be no
correlation between this trip and the SBE and DBE activity seen earlier in
the week.

Monday, December 10 (DOY 344)

RSS performed a Saturn Occultation Operational Readiness Test (ORT) today.
There will be another ORT performed in the wee hours of the morning on Dec.
16, followed by the occultation itself later that day.

Tuesday, December 11 (DOY 345)

CIRS performed observations for determining the upper troposphere and
tropopause temperature of Saturn today.

The DOY-353 Live Movable Block (LMB) kickoff meeting was held today.  The
meeting addressed the LMB and an additional Live Inertial Vector Propagator
update with RSS as the driving instrument.  The Science Planning analysis
and recommendation is due late tonight with the Go/NoGo meeting to be held
tomorrow.

Wrap up:

Check out the Cassini web site at http://saturn.jpl.nasa.gov for the latest
press releases and images.

The Cassini-Huygens mission is a cooperative project of NASA, the European
Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a
division of the California Institute of Technology in Pasadena, manages the
Cassini-Huygens mission for NASA's Science Mission Directorate, Washington,
D.C.  JPL designed, developed and assembled the Cassini orbiter.


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