PDS_VERSION_ID = PDS3 RECORD_TYPE = "STREAM" ^MOVIE = "HRIV_DUST_COMA.MPG" DATA_SET_ID = "DI-C-HRIV/ITS/MRI-5-MOVIE-COLL-V1.0" PRODUCT_ID = "HRIV_DUST_COMA.MPG" PRODUCT_NAME = "DI/HRIV DUST COMA EVOLUTION - MPEG MOVIE" PRODUCT_CREATION_TIME = 2006-11-06 TARGET_NAME = "9P/TEMPEL 1 (1867 G1)" INSTRUMENT_HOST_NAME = "DEEP IMPACT FLYBY SPACECRAFT" INSTRUMENT_NAME = "DEEP IMPACT HIGH RESOLUTION INSTRUMENT - VISIBLE CCD" START_TIME = 2005-05-01 STOP_TIME = 2005-07-04 SPACECRAFT_CLOCK_START_COUNT = "UNK" SPACECRAFT_CLOCK_STOP_COUNT = "UNK" CITATION_DESC = "Farnham, T.L., DI/HRIV DUST COMA EVOLUTION - MPEG MOVIE, DI-C-HRIV/ITS/MRI-5-MOVIE-COLL-V1.0:HRIV_DUST_COMA.MPG, NASA Planetary Data System, 2006." OBJECT = MOVIE NAME = "DEEP IMPACT MOVIE: HRIV DUST COMA EVOLUTION" DATA_FORMAT = "MPEG-1" DESCRIPTION = "Animated sequence of High Resolution Instrument visibe CCD (HRIV) images showing the evolution of the dust coma of comet Tempel 1 during the approach of the Deep Impact spacecraft. The sequence starts on 1 May and extends to 4 July 2005. Frame intervals are typically four hours, though there are gaps whenever spacecraft maneuvers or calibrations took precedence, and the sampling frequency increases toward the end of the sequence. Early images show little variation, but as the spatial resolution improves, rotationally varying jets and arcs can be detected. At least ten outbursts of various strengths can also be seen during the sequence. Each image has been enhanced by dividing out an azimuthally averaged radial profile computed from the comet itself. (The profile is essentially a 1/rho profile, which steepens gradually within 300 km of the nucleus.) The circle at the center covers the PSF of the nucleus, which appears donut-shaped because of the focus problems in the HRI. The six-pointed ''star'' pattern visible close to the nucleus toward the end of the sequence is produced by diffraction of the secondary mirror mount. The date and time of each frame are shown in the upper right and the yellow marker that moves across the bottom denotes the position of that image in the rotational phase (where zero phase is defined as the time of impact, and the rotation period is 1.7 days). The field of view is about 23,000 km in the first frame, 105 km in the last frame and varies roughly linearly in between. Celestial North is to the upper right, and East is to the upper left. For more information, see ''Dust coma morphology in the Deep Impact images of Comet 9P/Tempel 1'' by Farnham, et. al (2007)." END_OBJECT = MOVIE END