Cassini Significant Events 05/13/09 - 05/19/09
The most recent spacecraft telemetry was acquired on May 19 from the
Deep Space Network tracking complex at Madrid, Spain. The Cassini
spacecraft is in an excellent state of health and all subsystems are
operating normally. 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" page at:
http://saturn.jpl.nasa.gov/mission/presentposition/.
Wednesday, May 13 (DOY 133)
An encounter strategy meeting was held today to cover the period
between May 21 and June 6, Titan flybys T55 and T56, and maneuvers
197-199.
Thursday, May 14 (DOY 134)
Orbit Trim Maneuver (OTM) #195 was performed today. This is the
apoapsis maneuver setting up for the Titan 55 encounter on May 21. The
main engine burn began at 4:14 AM PDT. Telemetry immediately after the
maneuver showed the burn duration was 13.18 seconds, giving a delta-V of
2.21 m/s. All subsystems reported nominal performance after the
maneuver.
Friday, May 15 (DOY 135):
Today the Composite Infrared Spectrometer (CIRS) performed a
compositional sit and stare of Saturn¹s northern hemisphere to measure
oxygen compounds in the Saturnian stratosphere as a function of
latitude.
Over the weekend CIRS took measurements for far-infrared mapping studies
of Saturn¹s northern hemisphere and pole, the Cassini Plasma Spectrometer
led the pointing for a Magnetospheric and Plasma Science campaign to
observe the dawn-side magnetospheric boundaries at a variety of radial
distances, and the Ultraviolet Imaging Spectrograph performed day 4 of a
mosaic scan of the Saturn magnetosphere to observe atomic oxygen and
hydrogen.
Monday, May 18 (DOY 138):
Orbit Trim Maneuver (OTM) #196 was performed today. This is the
approach maneuver setting up for the Titan 55 encounter on May 21. The
reaction control subsystem burn began at 2:00 PM PDT. Telemetry
immediately after the maneuver showed the burn duration was 37.63
seconds, giving a delta-V of 47.12 mm/s. All subsystems reported nominal
performance after the maneuver.
Science Planning hosted a presentation on the science highlights for S54
with a focus on what is unique and what observations have the highest
priority. This information will help the flight team as the sequence goes
through the development process, and assist the team in making trades
should the need arise. Tomorrow the files for the first input port are
due for this sequence.
Tuesday, May 19 (DOY 139)
At less than four weeks away from uplink, it has been determined that
the S51 background sequence has grown large enough that it will be split
into two parts. Part1 has about 56,000 words and Part2 has about 51,000
words. Part1 will be sent to the spacecraft on June 10.
------------------------
To unsubscribe from Cassini Spacecraft Updates or to subscribe with a
different email address, visit:
<
http://saturn.jpl.nasa.gov/news/mailinglistsignup/ >
------------------------
This email address is not monitored. For comments and questions, please
contact Cassini Outreach at:
<
http://saturn.jpl.nasa.gov/feedback/>
------------------------
Visit the JPL Cassini home page for more information about the Cassini
Project:
<http://saturn.jpl.nasa.gov/
>
------------------------