HUBBLE SPACE TELESCOPE
                               DAILY REPORT #1019

PERIOD COVERED:  0800 EST
Daily Status Report as of 323/1200Z.

1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED:

   1.1 Completed WFC 5074 (WF/PC Cycle 3 Calibration: WFC Flats Narrow. 1)

       The Wide Field Camera was used to make Earth Flat images which will
       be used to remove pixel to pixel variations in the grain of the
       chips. Sixteen observations taken in pairs were taken for each
       filter. The OSS monitored the observations, and assessed the data
       quality. No anomalies were reported.

   1.2 Completed FOS/RD 5048 (FOS Cycle 3 Spectral Flats Fields and
       Monitor)

       The Faint Object spectrograph (Red Side) was used to make
       observations of hot white dwarf star G191-B2B (aka, WD0501+527) to
       monitor changes in the flat field characteristics of the FOS. The
       first three onboard target acquisitions were successful. During the
       fourth acquisition the FOS shutter was closed, for unknown reasons.
       The observation received only noise. The OSS chose not to open the
       shutter by uplink commands.

   1.3 Completed  PC 4902 (HST Medium - Deep Survey - Part 2: Low Latitude
       - Cycle 3 High)

       The Planetary Camera was used to make a long exposure taken in
       parallel with the prime science observation. Areas of interest are
       galactic structure and evolution. There is also the possibility of
       serendipitous discoveries.  The observation was executed as
       scheduled, and no problems were reported.

   1.4 Completed WFC 4929 (WF/PC Cycle 2: Improved Dark Calibration)

       The Planetary Camera was used to make two dark calibration images.
       The two exposures lasted 1200 seconds each, and the camera was
       pre-flashed before the observations. Both observations were reported
       to be normal exposures.

   1.5 Completed FOS/RD/BL 4694  (Stellar Content of Galaxies and Globular
       Clusters - Spectroscope)

       The Faint Object Spectrograph (Both the Red and Blue Sides) were
       used to make observations of globular cluster MII-EXT-CL which is
       located in the M-31 Galaxy (aka, Andromeda Galaxy). The G130H
       grating was used of the Blue side, and G270H and G400H were used on
       the Red Side. The observations were executed as scheduled, and no
       problems were reported.

   1.6 Completed WFC 4348 (Long Period Variables of M81: Cycle 3 Medium)

       The Wide Field Camera was used to make one image to the galaxy M-81
       (aka, NGC-3031)  to look for long period variable stars which can be
       compared to those already studied in our own galaxy and the
       Magellanic Clouds. These stars should have period of from 100 to 100
       days. The observations were executed as scheduled, and no problems
       were reported.

   1.7 Completed WFC/PC 5026 (WF/PC Cycle 3 Calibration: Rapid Internal
       Monitor)

       The Wide Field Camera and the Planetary Camera were used to make
       internal flat calibration images. These images will be used to look
       for measles and daisies (i.e., different forms of contamination),
       and to monitor scattered light. The observations were executed as
       scheduled, and no problems were reported.

2.0 FLIGHT OPERATIONS SUMMARY:

    2.1 Guide Star Acquisitions:

                            Scheduled Acquisitions : 2
                                        Successful : 2
                          Scheduled Reacquisitions : 11
                                        Successful : 11

   2.2 FHST Updates:

                              Scheduled : 8
                             Successful : 8

   2.3 Significant HSTARs: None

   2.4 Operations Note: None

3.0 ACTIVITIES SCHEDULED FOR NEXT REPORTING PERIOD:

   3.1 Complete FOS/BL 5048 (FOS Cycle 3 Spectral Flats and Monitor)

   3.2 Complete PC 4902 (HST Medium - Deep Survey - Part 2 Low Latitude -
       Cycle 3 High)

   3.3 Complete WFC 4348 (Long Period Variables of M-81: Cycle 3 Medium)

   3.4 Complete WFC/PC 5026 (WF/PC Cycle 3 Calibration: Rapid Internal
       Monitor)

   3.5 Complete FOS/RD 4941 (Geometry and Generalizability of the
       Reflective Light Model for Seyfert Galaxies)

   3.6 Complete PC 4521 (Asteroid Shape and Duplicity - Cycle 3 High)

   3.7 Complete PC 4712 (WF/PC Cycle 2 Calibration: Measles Monitor)

   3.8 Complete  FOC/96 3807 (Minkowski's Object)

   3.9 Complete Three Sets of WFC 4381 (HST Medium - Deep Survey - Cycle 3)

   3.10 Complete Two Sets of PC 5073 (WF/PC Cycle 3 Calibration: PC Flats
       Wide. 2)

   3.11 Complete Three Sets of PC 5072 (WF/PC Cycle 3 Calibration: PC Flats
       Wide. 1)

   3.13 Complete PC 5014 (WF/PC Cycle 3 Calibration: PC Flats Narrow. 2)

   3.14 Complete FOS/BL 4285 (Time-Resolved UV Spectrometry of Massive
       X-Ray Binaries: Cycle 3 High)

   3.15 Complete Two Sets of PC 4929 (WF/PC Cycle 2: Improved Dark
       Calibration)

   3.16 Complete PC 5017 (Internal Velocity Distribution in Globular
       Clusters Pert Three, Cycle 3)

   3.17 Complete HSP/POL 4889 (Gravitational Lenes Part I - Cycle 3 High)

   3.18 Complete Two Sets of WFC 5076 (WF/PC Cycle 3 Calibration: WFC Flats
       Wide. 2)

   3.19 Complete Two Sets of WFC 5075 (WF/PC Cycle 3 Calibration: WFC Flats
       Wide. 1)

   3.20 Complete WFC 5074 (WF/PC Flats Calibration: WFC Flats Narrow. 1)

4.0 ANOMALY STATUS:

   4.1 Significant New Anomalies: None

   4.2 Significant Unresolved Anomalies: None

5.0 SIGNIFICANT FORTHCOMING EVENTS:

       Internal Simulation #2 (EVA 1) is scheduled for next Monday, Nov. 
22,
       1993 starting at 8am, and is planned to run for 12 hours.

/DMH                           -END- .