Cassini Significant Events for 11/10/05 - 11/16/05

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Cassini Significant Events 
for 11/10/05 - 11/16/05

The most recent spacecraft telemetry was acquired Wednesday, November 16,
from the Goldstone tracking stations. The Cassini spacecraft is in an
excellent state of health and is 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 .

Thursday, November 10 (DOY 314):

Cassini Outreach and a Saturn Observation campaign member presented a
children's program at the Monrovia Public Library last week.  While waiting
for the rain to disperse outside, the children learned about Saturn by
making their own "Layers of Saturn" books.  This activity is the subject of
Lesson 9 for grades 1 and 2 in Cassini's Reading, Writing and Rings literacy
program.  In addition, 'Reading, Writing, and Rings' was presented to 20
educators at Mesa Union School District in Somis, California, and 108
participants in the Collaborative After School Project in Los Angeles,
California. 

Friday, November 11 (DOY 315):

Members of the Imaging Science Subsystem (ISS) are supporting deviations
from the nominal S19 uplink process.  The science team has found that the
exposures in S19 can't be properly determined until the S17 data is
available.  Because it arrives a few days after the deadline for S19
instrument expanded block files (IEB), the team must make special
arrangements.  The plan is to upload changes to exposures on some
observations after the sequence is on-board and before the S19 triggers.

Saturday, November 12 (DOY 316):

The S16 background sequence began execution today at 10:15 AM Pacific time.
The sequence runs for 34 days concluding on December 17.  Activities during
S16 include four Orbit Trim Maneuvers (OTM), numbers 42, 43, 44, and 45, one
targeted flyby of Rhea over the Thanksgiving weekend, and two non-targeted
flybys, one each of Enceladus and Helene. Sixteen optical navigation images
will be taken, periodic spacecraft engineering maintenance will be
performed, and 41 DSN tracks will be utilized.

Two live updates were identified for S16, Iapetus beginning on DOY 316 and
Rhea on DOY 330.  The DOY 316 update was cancelled on November 1.  The Go/No
Go meeting for the Rhea update is scheduled for Wednesday, November 23.

With the start of S16 and the third closest approach to Iapetus in the tour,
the Optical Remote Sensing instruments will continue the Iapetus campaign
begun in S15.  ISS continues spectrophotometry, the Ultraviolet Imaging
Spectrograph will measure UV albedo across various longitudes and phase
angles, and the Composite Infrared Spectrometer (CIRS) will continue its
Iapetus observations with high spectral resolution integration for
composition.  RADAR scatterometry and radiometry of Iapetus will also be
obtained. The Magnetospheric and Plasma Science instruments continue to
observe the dawn-side magnetospheric boundaries at a variety of radial
distances, including the bow shock, magnetopause and associated boundary
layers.

Uplink Operations sent commands to the spacecraft to perform a switch of
CIRS flight software from version 3.0.1. to 4.0.  Execution will occur on
Tuesday.

Twenty-five years ago on November 12, 1980, the Voyager 1 spacecraft had its
close encounter with Titan as it flew through the Saturnian system.  Data
returned from that mission showed Titan completely enveloped by haze that
merges with a darker cloud layer over the North Pole.  Voyager found that
Titan had a substantial atmosphere.

Sunday, November 13 (DOY 317):

Orbit trim maneuver #42 (OTM-42) was performed today. This is an apoapsis
maneuver setting up Cassini's flyby of Rhea on November 26.  The main engine
burn began at 7:16 am Pacific Time.  Telemetry immediately after the
maneuver showed the burn duration was 13.2 sec, giving a delta-V of
approximately 2.1 m/s. All subsystems reported nominal performance after the
OTM.

Monday, November 14 (DOY 318):

Every instrument team has submitted 100% of their archive data products that
were due on October 1, 2005.  In addition, the Planetary Data System (PDS)
has accepted 100% of these products for most teams, and is in the process of
reviewing the data for the rest. Instrument teams have already begun
submitting some of the data products scheduled to be delivered on January 1,
2006.

Tuesday, November 15 (DOY 319):

An encounter strategy meeting was held today covering the period from
November 26 through December 26.  This includes the Rhea 1 and Titan 9
flybys and OTMs 44-46.

The tumble densities for Titan-25 through Titan-43 were presented at the
Mission Planning Forum today.  There are currently 21 low altitude Titan
flybys scheduled between now and end of mission in 2008. The purpose of the
meeting was to present the results of the work performed thus far by the
Spacecraft team in determining tumbling and safe atmospheric densities for
these flybys.

Wednesday, November 16 (DOY 320):

A Cassini tour science talk was given on the results of the Huygens Probe
Doppler Wind experiment.

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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