Data Set Information
DATA_SET_NAME PLUTO-CHARON MUTUAL EVENTS V3.1
DATA_SET_ID EAR-A-3-RDR-PCME-V3.1
NSSDC_DATA_SET_ID
DATA_SET_TERSE_DESCRIPTION
DATA_SET_DESCRIPTION
Data Set Overview : During the period 1985-1990, the earth entered the orbital plane of Pluto and its moon Charon, and the mutual eclipse events were observed from ground-based observatories. A subset of these data are included in this data set, and more will be added in future updates. The current version contains photoelectric photometry data from thirty-nine events observed at Mauna Kea Observatory by Tholen, CCD photometry data from fifteen events observed at Palomar Observatory by Buratti and colleagues, and photoelectric photometry data from ten events observed at McDonald Observatory by Young and Binzel.  Data :  The Mauna Kea data is in the file pcmemko.tab, and includes standard B magnitudes and errors, and Julian date at mid-observation, corrected for light-travel time. The Palomar data is in the file pcmepal.tab, and includes differential magnitudes and errors, and Julian date at mid-observation (uncorrected). The McDonald Observatory data, taken from Young (1992), includes differential B and V photometry.  Individual lightcurves are included in the subdirectory 'indiv'. These contain the same data as in the full data files. The filenaming system is as follows: obs_yyyymmdd_f.tab, where obs is an abbreviation of the observatory, yyyymmdd is the date of observation, and f is the filter.  Modification History :  In January 2002 SBN personnel calculated UTC based on the Julian dates provided and added it to the data files. At the time resolution of the Julian date (less than 1.e-05), UTC and UT are equivalent. START_TIME and STOP_TIME values were updated throughout as appropriate. No other data values were changed.  In 2008, the data from McDonald Observatory, from Young (1992) and with additional discussion of the data given in Young and Binzel (1993), was added to the data set.  In 2012, the data were broken into individual lightcurves, supplied in a separate subdirectory in addition to the original data files. This change was made to facilitate loading the data into the data Ferret.  References :  Young, E.F., An albedo and frost model of Pluto, Ph.D. thesis, Massachusetts Institute of Technology, 1992. [YOUNG1992]  Young, E.F. and R.P. Binzel, Comparative mapping of Pluto's sub-Charon hemisphere: Three least-squares models based on mutual event lightcurves, Icarus 102, 134-149, 1993. [YOUNG&BINZEL1993]
DATA_SET_RELEASE_DATE 2012-05-01T00:00:00.000Z
START_TIME 1985-01-16T11:01:21.000Z
STOP_TIME 1990-09-23T02:27:10.000Z
MISSION_NAME SUPPORT ARCHIVES
MISSION_START_DATE 2004-03-22T12:00:00.000Z
MISSION_STOP_DATE N/A (ongoing)
TARGET_NAME PLUTO
TARGET_TYPE PLANET
INSTRUMENT_HOST_ID MCD21
MCD27
OBS347T3
OBS376T1
OBS376T2
OBS445T3
INSTRUMENT_NAME TINSLEY PHOTOMETER
TINSLEY PHOTOMETER
MCDONALD P45A TWO-CHANNEL PHOTOMETER
MCDONALD P45A TWO-CHANNEL PHOTOMETER
MCDONALD P45A TWO-CHANNEL PHOTOMETER
VARIOUS GROUND-BASED DETECTORS
INSTRUMENT_ID I0390
I0390
I0391
I0391
I0391
VARGBDET
INSTRUMENT_TYPE PHOTOMETER
PHOTOMETER
PHOTOMETER
PHOTOMETER
PHOTOMETER
UNKNOWN
NODE_NAME Small Bodies
ARCHIVE_STATUS LOCALLY_ARCHIVED
CONFIDENCE_LEVEL_NOTE
Confidence Level Overview : Data Coverage and Quality :  The data set is eventually intended to be a complete collection of groundbased observations of the Pluto-Charon mutual events. At present, it contains visual photometric data from Mauna Kea Observatory, Palomar Observatory, and McDonald Observatory. The collection includes both calibrated and uncalibrated data. Additional data will be added in future updates.
CITATION_DESCRIPTION Tholen, D.J., Ed., Pluto-Charon Mutual Events V3.1. EAR-A-3-RDR-PCME-V3.1. NASA Planetary Data System, 2012.
ABSTRACT_TEXT Ground-based photometric observations of the 1985-1990 Pluto-Charon mutual events, observed from Palomar, Mauna Kea, and McDonald Observatories.
PRODUCER_FULL_NAME CAROL NEESE
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