National Aeronautics and Space Administration Logo
Follow this link to skip to the main content NASA Banner
Solar System Exploration
News & Events
This Week on Galileo: Day Two of Io 32 Encounter
This Week on Galileo: Day Two of Io 32 Encounter
16 Oct 2001
(Source: Jet Propulsion Laboratory)

Tuesday, October 16, 2001
DOY 2001/289

The hectic pace of the Io closest approach and its jam-packed observing sequence is now fully five hours behind us. Galileo has sped on to a distance of 160,000 kilometers (99,440 miles) from Io. But there are still good science observing opportunities to be taken advantage of. And take advantage of them we do!

At 12:10 a.m. PDT [See Note 1] the Photopolarimeter Radiometer instrument (PPR) turns its focus on Jupiter. The observation scans the instrument back and forth across the limb of the giant planet, mapping the temperatures of the different layers of the atmosphere.

At 12:44 a.m. the Near Infrared Mapping Spectrometer (NIMS) collects a thermal map of the entire visible disk of Io, looking for volcanos and other hot spots.

At 1:41 a.m. PPR maps the temperatures on the dark side of Europa. This is the only observation made of this icy moon on this orbit. Europa was the central focus of a series of nine orbits earlier in the Galileo mission (the orbits labelled E11 though E19). At that time, we steered the spacecraft to within 200 kilometers (124 miles) of the surface of that satellite. During this orbit, we only close to within 340,000 kilometers (211,000 miles), at 2:27 a.m., but that is still close enough to detect temperature variations across the surface features.

At this point we are finally able to take a breather, and the next observation doesn't come along until 6:58 a.m., when the Solid State Imaging camera (SSI) snaps a global color image of Io, which now fits within a single SSI frame. This view includes the volcanos Pele, Zamama, and Isum, with the Prometheus volcano appearing near the limb.

At 8:54 a.m. PPR again views Jupiter, scanning again the same patch of real estate that it viewed just after midnight. By now, that portion of the planet has rotated around so that it appears in the center of the visible disk of the planet.

By 12:29 p.m. the spacecraft has receded far enough from Jupiter (out to 15 Jupiter radii, over 1 million kilometers or 666,000 miles) that the radiation environment has cooled down considerably. At this point, the electronic noise induced in the circuitry and sensors of the star scanner detector has faded, and the control software is again instructed to look for three stars to guide it, instead of the single bright star it has relied upon for the past 47 hours.

At 12:58 p.m. SSI again images Io in color, this time with the satellite filling only a quarter of the field of view. This vista will include the volcano Loki near the terminator, or day-night boundary on the dynamic body.

At 2:31 p.m. SSI snaps another picture of the small inner satellite Amalthea. This view will also include several background stars, and will be used by the Navigation Team to help refine our knowledge of the orbit of that body. This will help us fine-tune the trajectory of the spacecraft to achieve the desired fly-by of Amalthea in November 2002.

At 2:53 p.m., and again at 8:27 p.m., NIMS acquires temperature maps of the entire visible hemisphere of Jupiter. With these two views, the scientists will be able to study the dynamics of the turbulent region in the wake of the Great Red Spot, and will have a view of both the north and south auroral regions of the planet.

Finally, at 10:21 p.m., a performance test of the spacecraft gyroscopes is executed. The electronics in the gyroscope system have proven to be very sensitive to the radiation environment sensed by the spacecraft as it flies close to Jupiter. This test will determine the extent of the degradation in the circuitry due to this most recent pass, in preparation for the planning of a spacecraft maneuver coming up on Friday.

As you can see, the pace has slacked off quite a bit now, but we're still going strong, and there's more to come!

Note 1. Pacific Daylight Time (PDT) is 7 hours behind Greenwich Mean Time (GMT). The time when an event occurs at the spacecraft is known as Spacecraft Event Time (SCET). The time at which radio signals reach Earth indicating that an event has occurred is known as Earth Received Time (ERT). Currently, it takes Galileo's radio signals 41 minutes to travel between the spacecraft and Earth. All times quoted above are in Earth Received Time.

For more information on the Galileo spacecraft and its mission to Jupiter, please visit the Galileo home page at one of the following URL's:

http://galileo.jpl.nasa.gov
http://www.jpl.nasa.gov/galileo

News Archive Search  Go!
Show  results per page
 
 
Awards and Recognition   Solar System Exploration Roadmap   Contact Us   Site Map   Print This Page
NASA Official: Kristen Erickson
Advisory: Dr. James Green, Director of Planetary Science
Outreach Manager: Alice Wessen
Curator/Editor: Phil Davis
Science Writer: Autumn Burdick
Producer: Greg Baerg
Webmaster: David Martin
> NASA Science Mission Directorate
> Budgets, Strategic Plans and Accountability Reports
> Equal Employment Opportunity Data
   Posted Pursuant to the No Fear Act
> Information-Dissemination Policies and Inventories
> Freedom of Information Act
> Privacy Policy & Important Notices
> Inspector General Hotline
> Office of the Inspector General
> NASA Communications Policy
> USA.gov
> ExpectMore.gov
> NASA Advisory Council
> Open Government at NASA
Last Updated: 12 May 2004