Cassini Significant Events for 04/25/07 - 05/01/07

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Cassini Significant Events 
for 04/25/07 - 05/01/07

The most recent spacecraft telemetry was acquired on Tuesday, May 1, 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, April 25 (DOY 115):

The Spacecraft Operations Office hosted a presentation to interested members
of the flight team on "Estimated Tumbling Densities for All Low-altitude
Titan Flybys in the Extended Mission."  The presentation was given by
personnel from the Attitude and Articulation Control Subsystem, with the
results to be used in the determination of minimum safe flyby altitudes.

Saturn's iconic image as a ringed planet is both the symbol and the product
of scientific discovery.  As technology advances, each closer view of the
planet has exposed new and unexpected features. At a program of the
winter/spring 2007 Earnest C. Watson Lecture Series, the Cassini Project
scientist described some of the findings that have changed our understanding
of the diverse rings and moons of Saturn, and have yielded insight into the
early history of Earth and our solar system.  The lecture, "Cassini-Huygens
at Saturn: Discovery of New Worlds, Some Familiar and Some Alien," was
presented in Beckman Auditorium on the Caltech campus in Pasadena, CA.
Caltech has offered the Watson Lecture Series since 1922, when the late
Caltech physicist Earnest Watson conceived it as a way to explain science to
the local community.

Thursday, April 26 (DOY 116):

Mission Planning has released a Consumables Report Update showing
consumables usage through Feb. 17, 2007, the end of S27, and predicted usage
out to Oct. 31, 2007, the end of S34.  All consumables usage is running at
or in some cases slightly below the expected usage rate.

Prior to April 1997, the flight team assembled a list of instrument and
spacecraft consumables to be tracked.  Since launch on Oct. 15, 1997,
Mission Planning has updated these numbers, verified whether the list to be
tracked is still complete, obtained numbers for early flight operations, and
obtained an estimate of the intended future use of these items to the end of
the prime mission. Consumable Report Updates are generated periodically to
allow visibility into the predicted end of prime mission and extended
mission margins.

The Titan 29 (T29) flyby occurred today at an altitude of 980 km with
Cassini traveling at 6.2 km/sec. Leading up to the encounter, the Optical
Remote Sensing instruments took turns capturing Titan mosaics. For the flyby
using Synthetic Aperture Radar (SAR), scatterometry, and altimetry, the
RADAR instrument imaged additional regions near Titan's north pole in an
area nicknamed the "black sea." 

The radar coverage crossed over four previous radar swaths and filled in
more of the gaps in the coverage of that area. In addition, the Composite
Infrared Spectrometer observed the lit and dark sides of Titan, looking for
hot spots and lightning. For more information and a PDF of the Mission
Description of this flyby link to: 

http://saturn.jpl.nasa.gov/news/events/titan20070426/index.cfm

Today marks the 9th anniversary of the Cassini Venus 1 flyby in April of
1998.

Friday, April 27 (DOY 117):

The S31 sequence development team has reached that point in the process
where it is determined if any part of the sequence should be tested prior to
execution on board the spacecraft.  After discussion with some of the
instrument teams and Spacecraft Operations (SCO), it was decided to run
simulations in the Integrated Test Laboratory of the Radio Science (RSS)
Saturn occultation Live Movable block on DOY 162 and Live Update Block on
DOY 178, the Titan 32 flyby on DOY 164, and the SCO gyroscope calibration on
DOY 188.

Saturday, April 28 (DOY 118):

Orbit determination has converged after processing the first tracking pass
and the telemetry from the T29 flyby.  With this information, Navigation
Team members are predicting very little improvement in the orbit estimate
after the data from the next tracking pass is processed.  Based on today's
orbit solution, Orbit Trim Maneuver (OTM) #107 had a magnitude of 0.529 m/s,
however the cost of canceling the OTM was only 0.142 m/s.  The delta V
increase is primarily in OTM #110, the T30 cleanup maneuver.  Based on the
minimal cancellation cost, the decision was made to cancel OTM-107.

Tuesday, May 1 (DOY 121):

At the final sequence approval meeting held today, S30 was approved for
uplink to the spacecraft.  The sequence leads have begun commanding to send
up the instrument expanded block files.  S30 will go active on-board on May
4.  The final development process has begun for S32

An AACS reaction wheel assembly (RWA) friction test for prime wheels 1, 2,
and 4 occurred today. For this activity, performed every three months, the
RWAs are spun up to 900 rpm in both directions and are timed as they run
down to zero. The results were quite positive, especially for wheel #1,
which has previously shown signs of increasing friction.

The topic at the Mission Planning Forum today was Extended Mission Titan
Altitudes.  Based on the tumble densities delivered by SCO/AACS/Propulsion,
and the latest atmosphere models delivered to date, the discussion centered
on whether to lower the initial 1000 km minimum flyby altitude for extended
mission that has been a baseline assumption for the tour designers so far.

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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