HUBBLE SPACE TELESCOPE
                               DAILY REPORT #1020

PERIOD COVERED:  0800 EST
Daily Status Report as of 326/1200Z.

1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED:

   1.1 Completed FOS/BL 5048 (FOS Cycle 3 Spectral Flats 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
       shutter did not open during the first observation, because of an
       earlier guide star acquisition problems. The subsequent science
       observations were received and displayed. They were reported to look
       fine.

   1.2 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.  A total of five observations were
       received and displayed in the OSS. They were reported to look okay.

   1.3 Completed WFC 4348 (Long Period Variables of M-81: 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 observation was reported to look okay.

   1.4 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 was reported to look fine.

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

       The Faint Object Spectrograph was used to make two observations of
       the Seyfert Galaxy MARK-1 (offset). The observations were monitored
       in the OSS, and the data quality was assessed. Both observations
       were reported to be normal. The binary search was successful in
       seven groups. The peakup located the target in the fifth of five
       groups.

   1.6 Completed PC 4521 (Asteroid Shape and Duplicity - Cycle 3 High)

       The Planetary Camera was used to make three snapshot images of the
       large asteroid AST-09-FELI to look for possible satellites, shapes,
       and albedo variations. The observations were executed as scheduled,
       and no anomalies were reported.

   1.7 Completed PC 4712 (WF/PC Cycle 2 Calibration: Measles Monitor)

       The Planetary Camera was used to make Earth Calibration Flat images
       to monitor of a form of contamination known as measles. The
       observations used filter F517N, both with and without filter F122M.
       The OSS monitored the observation and assessed the data quality. No
       problems were reported.

   1.8 Completed  FOC/96 3807 (Minkowski's Object)

       The Faint Object Camera (f/96) was used to make observations of
       Minkowski's object, which is a starburst region triggered by a high
       energy radio jet. The history fo star formation will be traced along
       the path of the shock front by obtaining images over a wide range of
       wavelengths. A total of eight observations were received and
       displayed. They were reported to look normal.

   1.9 Completed Three Sets of WFC 4381 (HST Medium - Deep Survey - Cycle
       3)

       The Wide Field Camera was used to make three sets of medium-deep
       high latitude sky survey observations taken in parallel with the
       prime science observations. The observations were executed as
       scheduled, and no problems were reported. The images were reported
       to look fine.

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

       The Planetary Camera was used to make two sets of Earth flat
       calibration images using different filter combinations. These images
       will be used for flat field corrections of science images made with
       the PC. No anomalies were reported.

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

       Both the Wide Field Camera and the Planetary camera were used to
       make Earth Flat calibration exposures using the wide and medium band
       filters. Ten observations were received and displayed in the OSS.
       Three images were reported to be okay, three were underexposed,
       three were saturated, and one was partially saturated.

   1.12 Completed PC 5014 (WF/PC Cycle 3 Calibration: PC Flats Narrow. 2)

       The Planetary Camera was used to make standard Earth calibrations
       images for flat fielding of PC observations. Medium and narrow
       filters were used, with and without neutral density filters. The
       observations were executed as scheduled. four images were displayed.
       Two were saturated, one was underexposed, and one was okay.

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

       The Faint Object Spectrograph (Blue Side) was used in the Rapid Mode
       to obtain high time resolution, phase dependent ultraviolet spectra
       of Vela X-1 (aka HD77581). It is expected to see pulsations and
       rapid variability in the ultraviolet P-Cycni lines. The onboard
       target acquisition was successful. No anomalies were reported.

   1.14 Completed Two Sets of PC 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. The observations were executed
       as scheduled, and no problems were reported.

   1.15 Completed PC 5017 (Internal Velocity Distribution in Globular
       Clusters Pert Three, Cycle 3)

       The Planetary Camera was used to make observations of Globular
       Cluster NGC-7078. This set of observations will be used along with
       observations from proposal 1007, to study the proper motion of this
       cluster. Observations were made at different distances from the core
       center out to ten core radii. A total of ten observations were
       received and displayed in the OSS. Nine observations were reported
       to be okay. One observation had some data missing from group #1. At
       this time the cause of the data loss is not known, but is under
       investigation.

   1.16 Completed HSP/POL 4889 (Gravitational Lens Part I - Cycle 3 High)

       The High Speed Photometer was used to make observations of quasar
       QSO2345+00 which is an apparent gravitation lens system. Both
       photometry and polarmetry observations were made to find its
       characteristic signature in variability (In the time scale of
       weeks). The observations were monitored by the OSS, and the data
       quality was assessed. The target acquisition was successful. All of
       the science observations were reported to look satisfactory.

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

       Routine Earth flat calibration exposures were taken with the Wide
       Field Camera. The observations were monitored in the OSS, and the
       data quality was assessed. A total of six observations were taken.
       Four were reported to be saturated, and two were okay.

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

       Observations were made to make a standard calibration to obtain
       Earth flats using the Wide Field Camera. A total of six observation
       were received and displayed. Two were underexposed, three were
       reported to be okay, and one was partially saturated.

   1.19 Completed WFC 5074 (WF/PC Flats 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. Two images were received and displayed in the OSS. One image
       was reported to be normal, and the other was underexposed.

2.0 FLIGHT OPERATIONS SUMMARY:

    2.1 Guide Star Acquisitions:

                            Scheduled Acquisitions : 12
                                        Successful : 12
                          Scheduled Reacquisitions : 28
                                        Successful : 28

   2.2 FHST Updates:

                              Scheduled : 30
                             Successful : 30

   2.3 Significant HSTARs: None

   2.4 Operations Note:

       The Internal Simulation #2 (EVA 1) was initiated this morning, 
Monday,
       Nov. 22, 1993 as scheduled, starting at 8am, and will run for 12 
hours.

3.0 ACTIVITIES SCHEDULED FOR NEXT REPORTING PERIOD:

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

   3.2 Complete FOS/RD/BL 5051 (FOS Cycle 3 Polarimetric Calibration)

   3.3 Complete Two Sets of PC 4902 (HST Medium - Deep Survey - Part 2: Low
       Latitude - Cycle 3 High)

   3.4 Complete Seven Sets of PC 4714 (WF/PC Cycle 2 Calibration: PC
       Internal Delta Flats)

   3.5 Complete FOS/RD 4581 (Quasar Absorption Line Survey - Cycle 3 High)

   3.6 Complete WFC 4713 (WF/PC Cycle 2 calibration: WFC Internal Delta
       Flats)

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

   3.8 Complete Two Sets of FOS/BL 5050 (Cycle 2 Internal Wavelength
       Calibration)

   3.9 Complete PC 5483 (Test of Simple Guide Star Handoff)

   3.10 Complete FOS/BL 3441 (Post Asymptotic Giant Branch Evolution in the
       Magellanic Clouds)

   3.11 Complete Two Sets of WFC 5013 (WF/PC Cycle 2 Calibration: WFC Flats
       Narrow. 2)

   3.12 Complete PC 3807 (Minkowski's Object)

4.0 ANOMALY STATUS:

   4.1 Significant New Anomalies: None

   4.2 Significant Unresolved Anomalies: None

5.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time.

/DMH                           -END- .