HUBBLE SPACE TELESCOPE
                              DAILY REPORT #1304

PERIOD COVERED:  0000Z
Daily Status Report as of 012/0000Z

1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED:

   1.1 Completed WF/PC-2 5091 (GTO High Latitude Parallel 
       Program: Cycle 4)

       The WF/PC-2 was used in parallel with the prime science observations
to make high galactic latitude observations greater than +/-30 degrees. There
was one reported recentering event which lasted for a total of five seconds.
No other anomalies were noted.

   1.2 Completed FOS/BL 5444 (A UV Spectral Library of Metal-Poor Massive
Stars)

       The FOS (Blue Side) was used for a snapshot program to obtain
ultraviolet spectra of NS101-67, a metal-poor star in the LMC. It will be
useful for stellar atmosphere and stellar evolution studies. The observations
completed without incident. 


   1.3 Completed WF/PC-2 5562 (WF/PC-2 Cycle 4 Calibration: 
       Internal Monitor 3: Darks)

       The WF/PC-2 was used to obtain several 30-minute long, dark exposures
to provide ongoing calibration of the CCD dark current and to monitor and
characterize the evolution of hot pixels. The observations were executed as
scheduled, and no anomalies were noted. 

   1.4 Completed FOS/RD 5664 (Quasar Absorption Line Survey - Cycle 4 High)

       The Faint Object Spectrograph (Red Side) was used to make
spectrographic observations of quasi-stellar object 3C57 to look for
absorption lines due to gas in the intergalactic medium and galactic halos.
The observations were executed as scheduled, and no anomalies were noted. 

   1.5 Completed WF/PC-2 5369 (Medium Deep Survey: Cycle 4 Medium High
Galactic Latitude)

       The WF/PC-2 made a series of observations of high latitude objects as
part of a medium deep sky survey. The observations were taken in parallel
with other prime science observations. The observations were completed as
scheduled, and no anomalies were noted.


   1.6 Completed WF/PC-2 5563 (WF/PC-2 Cycle 4 Photometric Calibration
Monitor 1: UV /OPT STD.)

      The WF/PC-2 was used to make photometric calibration images of
ultraviolet standard star GRW+70D582 and monitor the photometric stability
and quantum efficiency of the WF/PC-2. The observations were executed as
scheduled, and no anomalies were noted. 

   1.7 Completed WF/PC-2 5655 (Cycle 4 Calibration: Internal Monitor 2 -
Flats Part 2)

       The WF/PC-2 was used to make both dark and visual flats. The
observations were completed as planned, and no problems were reported. 

   1.8 Completed WF/PC-2 5629 (WF/PC-2 Cycle 4 Photometric Calibration
Monitor 1C: 4-Chip STD in F170W)

       The WF/PC-2 was used to make photometric calibration observations of
the ultraviolet standard star GRW+70D582. The observations were executed as
scheduled, and no anomalies were noted. 

   1.9 Completed WF/PC-2 5476 (Continuum Snapshots of 3CR Radio Galaxies)

       The WF/PC-2 was used to make snapshot images of radio galaxy 3C29.0 as
part of a continuum survey and to study the galaxy's morphology. The
observations were executed as scheduled, and no anomalies were noted.

   1.10 Completed Two Sets of FOS/BL 5581 (Time-Resolved Spectroscopy of the
Pulsating White Dwarf DN Draconis)

        The FOS (Blue Side) was used in the rapid mode to cover the 17.1 hour
beat period of the pulsating DA white dwarf DN Draconis (aka G226-29) to
determine the index of the pulsational mode which will allow for the outer
hydrogen layer to be determined. Three recentering events were reported to
have lasting for a total of 11 seconds. No other anomalies were noted.

2.0 FLIGHT OPERATIONS SUMMARY:

   2.1 Guide Star Acquisitions: 

                            Scheduled Acquisitions : 6
                                        Successful : 6

                          Scheduled Reacquisitions : 6
                                        Successful : 6

   2.2 FHST Updates: 

                              Scheduled : 11
                             Successful : 11

   2.3 Significant HSTARs: None

   2.4 Operations Notes: 

       The ground PRS limits for Solar Array wing position were changed to a
range of 60 to 90 degrees.  Onboard, the SADE-2 was selected in the PSEA and
the SADE final try flag was disabled.

       STGT data inversions are periodically continuing.

3.0 ANOMALY STATUS:

   3.1 Significant New Anomalies: None

   3.2 Significant Unresolved Anomalies: None

4.0 SIGNIFICANT FORTHCOMING EVENTS: 

        Nothing at this time.

/DMH
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