Cassini Significant Events for 07/27/06 - 08/02/06

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Cassini Significant Events 
for 07/27/06 - 08/02/06

The most recent spacecraft telemetry was acquired Wednesday, August 2, 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.crm .

Thursday, July 27 (DOY 208):

It was reported in the Cassini Significant Events last week that the
atmospheric density measured at Titan 16 was higher than expected. The Titan
Atmospheric Modeling Working Group (TAMWG) met this morning to discuss this
result and assess whether the altitudes selected for upcoming encounters are
still acceptable. At the conclusion of the meeting, the TAMWG recommended no
changes to the altitudes of upcoming encounters. The new T16 data point has
not fundamentally changed our understanding of Titan's atmospheric profile,
except to indicate a less steep falloff in density at high latitudes.
Cassini only has one future Titan flyby at very high latitude, Titan 32.
Much like T16, this encounter is at 84 deg N latitude with a closest
approach at 950 km, so it should be safe as well.

One of the things that presents a challenge to Cassini scientists and
sequence developers is attempting to respond to new scientific discoveries
as they arise.  Background sequence S24 completed Science Operations Plan
Implementation in March 2004.  At that time the basic sequence was delivered
to the project file repository.  Science Planning was chartered to archive a
sequence that if necessary would fly on the spacecraft "as is."  Now roll
the clocks forward to July 27, 2006.  S24 has been through both the
Aftermarket Process and the Science Operations Plan Update Process.  It is
currently in final development prior to uplink.  The first of four phases of
that development process is complete.  But, due to the discovery of lakes
near Titan's north pole over the weekend, RADAR has requested re-pointing of
their T19 observation to cover more of the same region.  What to do?

It was decided to stick with the process and have RADAR submit their
pointing changes in the third phase.  Although this decreases the number of
iterations available to get the pointing right, it allows the other
instruments and AACS time to properly assess any impacts they might have.
To support the development of this observation, an interim set of sequence
products was produced with the new RADAR pointing, to give AACS time to
evaluate it and make a c-kernel available to teams that might wish to
examine it.  At this time S24 is on track for final approval in September,
and it is hoped to have lakes in its future.

Friday, July 28 (DOY 209):

Science data archive deliveries for data acquired during the period of July
through September 2005 are now complete.  The next archive delivery port is
October 1.

The official port occurred today for S25 as part of the Science Operations
Plan (SOP) Update process.  The merged products are currently being run
through end-to-end pointing validation by AACS.  The Project Briefing and
Waiver Disposition Meeting is scheduled for August 9.  The SOP Update
product is handed off to the sequence leads on August 11 for the final
development process.

Monday, July 31 (DOY 212):

The Cassini RADAR image of Titan's methane lakes is Astronomy Picture of the
Day today.

Tuesday, August 1 (DOY 213):

Orbit Trim Maneuver (OTM) #69, an apoapsis maneuver setting up for the Titan
17 encounter on September 7, was performed today.  This main engine burn
began at 2:30 PM PDT.  Telemetry immediately after the maneuver showed a
burn duration of 33.8 seconds, giving a delta-V of 5.4 m/sec.   All
subsystems reported nominal performance after the maneuver.  A contingency
DSS-15 track that had been retained for the DOY 214 backup OTM-69 window in
case the DSS-14 antenna went red was released at the successful completion
of the burn.  Cassini thanks MGS, MER and Odyssey for their help in making
this track available. The next OTM is scheduled for September 4.

Solar Conjunction occurs when the Sun is between the spacecraft and Earth.
This year it will last from August 2 through August 12, and is a time of
reduced commanding and downlink capability.  Cassini enters Solar
Conjunction tomorrow with a separation angle of 4 degrees. During
conjunction, communications with the spacecraft become degraded due to
interference from the sun.  For the next ten days the Spacecraft Operations
and Mission Support and Services offices will participate in a campaign
where a command file consisting of 10 no-op commands will be uplinked to the
spacecraft ten times daily.  This will allow the teams to obtain link
characterizations and accumulate statistics for uplink reliability at
decreased separation angles. With the exception of these no-op command
files, Spacecraft Operations has asked for and received a command
moratorium.  Additional commands will only be sent in the event of an
emergency. On Saturday, the spacecraft will be turned so that the High Gain
Antenna is continuously pointed to Earth, and 1896bps telemetry continues
while separation is less than 2 deg.   Normal playback downlink rates will
resume on August 10.

There is a great write up on conjunction on the Cassini web site.  For more
information link to:  http://saturn.jpl.nasa.gov/home/index.cfm

Cassini's "For Educators" website has a hands-on activity called
"Monitoring the Sun's Corona."  Scroll down the Saturn in your Kitchen and
backyard section to  "Saturn System Science" to find it.
http://saturn.jpl.nasa.gov/education/edu-58-kitchen.cfm.  In this activity,
students of all ages will learn how, during solar conjunction, scientists
use the relative positions of the Sun, Earth, and a spacecraft to study the
Sun's corona, or outer region.

Wednesday, August 2 (DOY 214):

An artist's rendition of the methane rain on Titan is Astronomy Picture of
the Day today


The data obtained by the six Huygens experiments is now archived in the
European Space Agency (ESA) Planetary Science Archive (PSA). A copy of the
archived data set is also available in the NASA Planetary Data System (PDS).
The data is now accessible by the scientific community and the general
public for downloads. This represents a major milestone in the Huygens
mission. Data from the Aerosol Collector and Pyrolyser (ACP), Doppler Wind
Experiment (DWE), Gas Chromatograph Mass Spectrometer (GCMS), and Huygens
Atmospheric Structure Instrument (HASI) is accessible along with
housekeeping data, calibration information, and documentation necessary to
understand and process the products, and to carry out scientific analyses.
Data from the Descent Imager Spectral Radiometer (DISR), Surface Science
Package (SSP),  and the final Huygens entry and descent trajectory data is
to be released in the September-October timeframe.   To access the data,
link to:
http://atmos.nmsu.edu/data_and_services/atmospheres_data/Huygens/Huygens.htm
l

A Cassini Saturn Orbit Insertion +2 Years celebration was held in Von Karman
auditorium today for the Cassini Flight team.  Talks were given by the
laboratory director Charles Elachi, and by two surprise celebrities, Robert
Picardo and Bill Nye.  An additional presentation was given by Outreach who
read to the flight team some of the comments that the public has sent to the
Cassini web site letting us know how much they appreciate what Cassini is
doing, and looking forward to the next two years of prime mission and
extended mission after that.  The flight team says "THANKS" back to the
public.  We are looking forward to it too!

Your coffee table will never be the same.  Outreach has promised the flight
team that they will let us know as books on Cassini/Saturn are published.
The first one is a beauty called Saturn: A New View in hardcover.  The
pictures are phenomenal.  The book has not yet been released but may be
ordered and will ship as it arrives at distributors.  See your local
bookstore - either electronic or traditional.

The July 20 "Cassini Real-time Operations" presentation from the Von Karman
Lecture Series is online at the JPL public website as a RealPlayer
downloadable: http://www.jpl.nasa.gov/events

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 Spsce 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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