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- Shoemaker-Levy Imaging Reports from: GALILEO, ULYSSES and VOYAGER
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- PUBLIC INFORMATION OFFICE
- JET PROPULSION LABORATORY
- CALIFORNIA INSTITUTE OF TECHNOLOGY
- NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
- PASADENA, CALIF. 91109.
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- GALILEO MISSION STATUS August 1, 1994
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- The Galileo spacecraft captured an extensive range of data on the impacts
- of the fragments of Comet Shoemaker-Levy 9 on Jupiter July 16 through 22.
- Because of its position 240 million kilometers (150 million miles) from Jupiter
- and in the direction of the impact sites on the planet's night side, Galileo
- was able to make unique direct observations of the impact events which were not
- visible from Earth.
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- The data from Galileo's science instruments were stored on the
- spacecraft's onboard tape recorder. Science teams are now carefully evaluating
- data stored on tape to select portions to be transmitted to Earth starting in
- August.
-
- The spacecraft's photopolarimeter-radiometer has already obtained and
- transmitted light-intensity readings from the impacts of comet fragments H, L
- and Q on Jupiter's far side. The B impact did not produce a significant
- indication; data from fragment P was recorded on tape for later playback.
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- Engineering telemetry indicated that Galileo's computer directed the
- imaging system, the near-infrared spectrometer, the ultraviolet spectrometer
- and plasma wave instrument to observe the impacts as planned. The camera
- observed the fragment D, E, K, N, V and W events, the infrared instrument the
- C, F, G and R impacts. Their observations are stored on tape, intended for
- gradual transmission to Earth beginning this month and continuing through
- January 1995.
-
- The spacecraft continues to operate normally, spinning at about 3 rpm and
- transmitting at 10 bits per second to ground stations of the NASA/JPL Deep
- Space Network. Galileo is about 640 million kilometers (400 million miles) from
- Earth, so that a command takes 36 minutes to reach Galileo, and the response
- another 36 minutes to return. The spacecraft will reach Jupiter on December 7,
- 1995, when its probe will descend into the Jovian atmosphere and the orbiter
- spacecraft will begin two years of observation and measurement of the planet,
- its moons and magnetosphere.
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- ULYSSES MISSION STATUS August 1, 1994
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- The Ulysses spacecraft -- currently exploring high latitude regions over
- the sun's southern pole -- has climbed to 75.5 degrees south of the sun's
- equator and is in the midst of its primary mission to examine the complex
- forces at work in these regions of space.
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- Ulysses was in a position to observe the impacts of comet Shoemaker-Levy 9
- during mid-July. At the time Ulysses had a direct line of sight to the impact
- region at 74.5 degrees south of the sun's equator. The spacecraft was about
- 375 million kilometers (230 million miles) below the ecliptic plane in which
- the planets orbit and 795 million kilometers (490 million miles) from Jupiter.
- Ulysses' unified radio and plasma wave experiment was reconfigured to provide
- the highest level of sensitivity for detecting very low frequency radio waves
- of less than 1 megahertz that might have been generated by the comet impacts.
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- Data from the impact of fragment A on July 16 through the collision of
- fragment Q on July 20 have been processed and analyzed, but no clear evidence
- of changes in radio frequencies has been detected. Jupiter normally has
- considerable activity at these frequencies. Members of the Ulysses radio
- science team will continue to watch for the more subtle or long-term effects of
- the comet collisions, but they do not anticipate much new information in the
- aftermath of the event.
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- All spacecraft operations and science experiments continue to go well.
- Ground controllers are carrying out routine data-gathering activities and
- experiment readjustments as needed. The European Space Agency's tracking
- facility at Kourou, French Guiana, has been modified and brought on-line to
- help provide 24-hour coverage of Ulysses now that it is moving into the
- sun-Earth region where the spacecraft's axial boom is illuminated by the sun.
- This illumination causes uneven heating of the boom which, in turn, causes a
- slight wobble of the spacecraft. Shortly after launch, Ulysses went through a
- period of wobbling that was finally controlled by an onboard control system
- that is used to maneuver and keep the spacecraft pointing at Earth. Ground
- controllers must be in constant contact with the spacecraft to carry out this
- technique, allowing the onboard system to detect and reduce unwanted motion.
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- Today Ulysses is traveling at a velocity of about 74,000 kilometers per
- hour (46,000 miles per hour) with respect to the sun.
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- VOYAGER MISSION STATUS August 1, 1994
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- Both the Voyager 1 and 2 spacecraft are healthy and they are continuing to
- take data on fields and particles in interplanetary space.
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- The Voyager 2 spacecraft used two of its scientific instruments to look at
- the impacts of Comet Shoemaker-Levy 9 fragments as they impacted Jupiter July
- 16-22. Both the ultraviolet spectrometer and the planetary radio astronomy
- experiments were used in the observations. Neither instrument detected any UV
- emission or radio signals during the impacts. The spacecraft began its
- observations of Jupiter on July 8 and will continue to observe the planet until
- August 17. At the time of the comet impacts, Voyager 2 was 6.1 billion
- kilometers (3.7 billion miles) from Jupiter.
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- Voyager 1 is currently 8.4 billion kilometers (5.2 billion miles) from
- Earth. Voyager 2 is 6.4 billion kilometers (4 billion miles) from Earth.
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