Cassini Significant Events 09/22/10 - 09/28/10
The most recent spacecraft telemetry was acquired on Sept. 28 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. 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, Sept. 22 (DOY 265)
Port 3 products were due today as part of the S65 Sequence
Implementation Process (SIP). The products will be merged and sent out to
the flight team for review.
This week in science, the Ultraviolet Imaging Spectrograph (UVIS),
Composite Infrared Spectrometer (CIRS) and the Visual and Infrared
Mapping Spectrometer (VIMS) took advantage of two stellar occultation
opportunities and performed a collaborative observation of Saturn's
atmosphere. In the first occultation, UVIS, CIRS and VIMS used the star
"alpha-orionis", more commonly called "Betelgeus", to
produce detailed spectral profiles of Saturn's atmosphere. Then, for the
second occultation, UVIS used "Beta Orionis", more commonly
called "Rigel", to study Saturn's atmosphere in ultraviolet
wavelengths. Following the occultations, CIRS took a 6 hour observation
tracking the limb of Saturn during periapse, the closest point of the
orbit around Saturn. This will allow studies of the thermal structure of
Saturn's stratosphere by means of limb sounding in the mid-infrared
wavelength. UVIS performed a scan across Saturn's atmosphere and
hemisphere to form spectral images.
Thursday, Sept. 23 (DOY 266)
Real time command procedure SCO-1794 to normalize the Command and
Data Subsystem (CDS) Solid State Recorder (SSR) load successfully went
through final Integrated Test Laboratory (ITL) end-to-end test today.
Normalization makes all four copies of the CDS flight software on the
SSRs equivalent.
Non-targeted flybys of Enceladus, Calypso, and Polydeuces occurred
today.
A new movie and images showing Saturn's shimmering aurora over a two-day
period are helping scientists understand what drives some of the solar
system's most impressive light shows. The movie and images are part of a
new study that, for the first time, extracts auroral information from the
entire catalogue of Saturn images taken by the visual and infrared
mapping spectrometer instrument (VIMS). For more information on this
subject and images, link to:
http://saturn.jpl.nasa.gov/news/cassinifeatures/feature20100923b/
Friday, Sept. 24 (DOY 267)
The Titan 72 encounter occurred today at an altitude of 8,175
kilometers and a speed of 5.7 km/sec. This flyby is the first in a series
of high-altitude Titan flybys over the next year and a half. During this
high altitude flyby, VIMS mapped at a resolution of 5 kilometers per
pixel an equatorial region of the trailing hemisphere known as Belet. The
resulting mosaic will complement the mosaics obtained during T-66 and
T-67. After closest approach, VIMS performed a global mapping of Titan
looking for clouds at northern mid-latitudes and near the poles. The
imaging science subsystem (ISS) rode along with VIMS throughout. For more
information link to:
http://saturn.jpl.nasa.gov/mission/flybys/titan20100924/.
Monday, Sept. 27 (DOY 270)
A kickoff meeting was held today for the S67 SIP. Port 1 for the
first set of input files from the teams occurs Oct. 12.
Five real time command procedures for the Attitude and Articulation
Control Subsystem (AACS) A8.8.0 flight software load successfully went
through final ITL end-to-end test today; testing will continue through
Oct. 1.
Cassini is once again Astronomy Picture of the Day (APOD). A repeat of
Cassini¹s 2007 image of Saturn¹s auroras by VIMS is today's Astronomy
Picture of the Day. To go to the image, link to:
http://antwrp.gsfc.nasa.gov/apod/ap100927.html.
Turning a midsummer night's dream into reality, NASA's Cassini spacecraft
begins its new mission extension -- the Cassini Solstice Mission --
today. The mission extension will take Cassini a few months past Saturn's
northern summer solstice through September 2017. It will enable
scientists to study seasonal changes and other long-term weather changes
on Saturn and its moons. For more information on this subject, link
to:
http://saturn.jpl.nasa.gov/news/cassinifeatures/feature20100927/.
Tuesday, Sept. 28 (DOY 271)
Orbit Trim Maneuver #263, the T72 clean-up maneuver scheduled for
today, was cancelled. There was no impact to science or overall
delta-V.
Today is the start of Superior Conjunction, which will continue through
Oct. 3. The Sun-Earth-Probe (SEP) angle will be less than 3 degrees
during this time. The minimum SEP angle of 2.12 degrees will take place
on Sept. 30.
The most recent Cassini-Huygens Analysis and Results of the Mission
(CHARM) teleconference was held Sept. 28. The topic:
"Satellite-magnetosphere interactions at Jupiter and Saturn." A
PDF of the presentation package may be obtained at:
http://saturn.jpl.nasa.gov/video/products/MultimediaProductsCharm/
.
An audio recording of the presentation was made and will be linked to the
same location within a few days.
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