HUBBLE SPACE TELESCOPE
                               DAILY REPORT #1141

PERIOD COVERED:  0700 EST
Daily Status Report as of 138/1200Z.

1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED:


   1.1 Completed GHRS/1 5373 (Excitation Processes for the Ultraviolet
       Dayglow of Jupiter: Cycle 4)

       The High Resolution Spectrograph (Side One) was used to make
       observations looking for molecular hydrogen emissions in the Jovian
       atmosphere. Four observations were received and displayed in the
       OSS. They all were reported to be okay.

   1.2 Completed WF/PC-2 5640 (Cycle 4 DD HST Observations of Comet
       Shoemaker-Levy (1993E) for May 19)

       The WF/PC-2 was used to make observations of the comet
       Shoemaker-Levy. The observations were executed as scheduled. The
       data remains on Science Tape Recorder #3, and it will be analyzed
       later. No anomalies were noted.

   1.3 Completed WF/PC-2 5446 (The Nuclei of Nearby S0 and Spiral Galaxies)

       The WF/PC-2 was used to make observations of galaxy NGC-4289. The
       observations were executed as scheduled, and the science data
       remains of Science Tape Recorder #3. It will be analyzed later. No
       anomalies were noted.

   1.4 Completed WF/PC-2 5394 (Interstellar Abundances in the SMC:
       Implications for QSO Absorption).

       The WF/PC-2 was used to make observations of the field around
       eclipsing binary star HD5980 (aka, SK78) located in NGC-346. The
       observations were executed as scheduled, and the science data
       remains of Science Tape Recorder #3. It will be analyzed later. No
       anomalies were noted.

   1.5 Completed GHRS/1 5417 (A Search for the Physical Processes
       on Jupiter)

       The High Resolution Spectrograph (Side One) was used as part of a
       program to observe atomic hydrogen emission at different latitude
       and longitudes on the planet Jupiter. The observations were executed
       as scheduled. Five observations were received and displayed. They
       were reported to look okay.  More science data remains of Science
       Tape Recorder #3. It will be analyzed later. No anomalies were
       noted.

   1.6 Completed WF/PC-2 5104 (Peculiar and Interacting Galaxies (WC01):
       Cycle 4)

       The WF/PC-2 was used to make images of galaxy APR230. The OSS
       monitored the observations, assessed and the data quality. The
       observations were executed as scheduled, and the science data
       remains of Science Tape Recorder #3. It will be analyzed later. No
       anomalies were noted.

   1.7 Completed FOS 5579 (Cycle 4 Test: To Determine FOS Polarity Mode)

       The Faint Object Spectrograph was used to make internal WAVE
       calibration observations of its polarization capabilities. The
       observations were executed as scheduled, and the science data
       remains of Science Tape Recorder #3. It will be analyzed later. No
       anomalies were noted.

   1.8 Completed WF/PC-2 5450 (Host Galaxies and Cluster Environments of
       Quasars)

       The WF/PC-2 was used to make observations of quasar QSO-121228 to
       study the properties of its host galaxy and any surrounding cluster
       environment. The observations were executed as scheduled, and the
       science data remains of Science Tape Recorder #3. It will be
       analyzed later. No anomalies were noted.

1.9 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.

   1.10 Completed FOS/RD 5441 (The Inner Regions of Quasars: Cycle 4)

       The Faint Object Spectrograph (Red side) was used to make
       observations of quasar B21351+31. The observations were executed as
       scheduled, and no anomalies were noted.


   1.11 Completed WF/PC-2 5351 (Properties of Intermediate Redshift
        Galactic Disks Causing Damped Lyman-Alpha)

       The WF/PC-2 was used to make observations to study the diffuse
       material at intermediate redshifts that is identified by absorbing
       Lyman-Alpha spectrum from quasar PKS1229-02. The observations were
       executed as scheduled, and no anomalies were noted.

2.0 FLIGHT OPERATIONS SUMMARY:

    2.1 Guide Star Acquisitions:


                            Scheduled Acquisitions : 12
                                        Successful : 12
                          Scheduled Reacquisitions : 4
                                        Successful : 4

                          FGSs #1 and #3 loss of lock at 137/1556Z.

   2.2 FHST Updates:

                              Scheduled :19
                             Successful :19

   2.3 Significant HSTARs: None

   2.4 Operations Notes:

       A quiet operational day was experienced as no anomalous activity was
       reported in any HST subsystem.

3.0 ACTIVITIES SCHEDULED FOR NEXT REPORTING PERIOD:

   3.1 Complete WF/PC-2 5479 (Subarcsecond Structure in Nearby AGNs)

   3.2 Complete WF/PC-2 5640 (Cycle 4 DD HST Observations of Comet
       Shoemaker-Levy (1993E))

   3.3 Complete WF/PC-2 5476 (Continuum Snapshots of 3CR Radio Galaxies)

   3.4 Complete GHRS/1 5417 (A Search for the Physical Processes on
       Jupiter)

   3.5 Complete WF/PC-2 5303 (Calibration of Stellar Evolutionary Ages and
       Variations in the IMF)

   3.6 Complete FOS/RD 5441 (The Inner Regions of Quasars: Cycle 4)

   3.7 Complete WF/PC-2 5369 (HST Medium-Deep Survey: Cycle 4 Medium, High
       Galactic Latitude.)

   3.8 Complete WF/PC-2 5570 (WF/PC-2 Cycle 4 Calibration: Earthflats,
       Large Set)

   3.9 Complete WF/PC-2 5446 (The Nuclei of Nearby S0 and Spiral Galaxies)

   3.10 Complete GHRS/1 5317 (Searching for circumstellar Gas Around Low
       Mass Per-Main Sequence Stars)

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-