HUBBLE SPACE TELESCOPE
                               DAILY REPORT #1010

PERIOD COVERED:  0800 EST
Daily Status Report as of 312/1200Z.

1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED:

   1.1 Completed 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 six
observations were received and displayed. One was underexposed, one was

reported to be okay, and the others were saturated
   1.2 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, and two observations were
       received and displayed. Both were reported to be saturated.

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

       The Planetary Camera was used to make four dark calibration images.
       The two exposures lasted 1200 seconds each, and the camera was
       pre-flashed before the observations. All four observations still
       remain on the science tape recorder, and will be analyzed later.

   1.4 Completed FOS/RD 3448 (Ultraviolet Evolution of Elliptical Galaxies
       at Moderate Redshifts)

       The Faint Object Spectrograph (Red Side) was used to to make
       three ultraviolet observations of the high red shifted elliptical
       galaxy A1758-7 to look for changes in the "UV rising branch". This
       feature is expected to change rapidly with the redshift of the
       galaxy, and should provide information on the hot stars which are
       believed to produce it. The observations were monitored in the OSS,
       and the data quality was assessed. The peakups for the first two
       observations had nearly identical counts in each group, so even
       though each observation chose a point to peakup on, that point
       differed little from its neighbors. The target was very extended.
       The third observation still remains on the science tape recorder,
       and will be analyzed later.

   1.5 Completed PC/WFC 5026 (WF/PC Cycle 3 Calibration: Rapid Internal

       Monitor)

       The Wide Field Camera and the Planetary Camera were used to make
       two 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 both observation are still on the
       science tape recorder.

   1.6 Completed Four Sets of WFC 4381 (HST Medium - Deep Survey - Cycle 3)

       The Wide Field Camera was used to make two 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.

   1.7 Completed GHRS/2 4536 (The Distance of High - Velocity Clouds: Cycle
       3 High)

       The High Resolution Spectrograph was used to make observations of
       quasars PG0906+597 and PG0859+533 to obtain spectra about the Mg H
       and K lines. These objects are expected to lie in front of a high
       velocity cloud. It is hoped that the distance and the velocity of
       this cloud can be found. The OSS monitored the observations, and
       assessed the data quality. No anomalies were reported.

   1.8 Completed GHRS/2 4869 (Spectroscopy of Interacting Binaries - 4185,
       Cycle 3 High)

       The High Resolution spectrograph was used to make six observations
       of the interacting binary star V-Sge. IUE spectra showed the
       possible presence of red-shifted emission at a velocity of about 700
       Km/Sec. This suggests a major mass transfer event is in process.
       The target was successfully located. The wavelength calibrations and
       spectral observations were received and displayed. All six
       observations were reported to look okay.

   1.9 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 observation was reported to look okay.

   1.10 Completed HSP/UV2 1093 (Observations of ZZ Ceti Stars)

       The High Speed Photometer was used to make ultraviolet observations
       of G117-B15A which is a pulsating white dwarf with a period of 215
       seconds. and has a visual magnitude of 15.2 . Two ultraviolet
       observations were made to obtain the star's color (i.e.,
       temperature) as a function of time. The onboard target acquisition
       was successful. Both observations were reported to look
       satisfactory.

   1.11 Completed PC 4904 (The Nuclei of Nearby S0 and Spiral Galaxies -
        III A PC Snapshot Image)

       The Planetary Camera was used to make one observations of the
       low-red-shift galaxy NGC-3769 to study its surface brightness
       profile, identify sub-arc-second scale condensations, find point
       sources, and look for gasious disk and dust lanes. The observation
       was executed without problems. The data was received and displayed.
       No problems were reported.

   1.12 Completed HSP/UV1 4810 (Constraints on Continuum Models of Active

        Nuclei: Fast Ultraviolet)

        The High Speed Photometer was used to make ultraviolet observations
        of the Seyfert galaxy NGC-4051. This galaxy has rapid variations in
        its active nuclei at X-Ray as small as 100 seconds. The target
        acquisitions left the target well centered. Two observations were
        received and displayed. No anomalies were reported.

   1.13 Completed FOS/RD 4212 (Internal Wavelength Calibration)

       The Faint Object Spectrograph was used to make wavelength
       calibration observations for every disperser-detector combination,
       to monitor the stability of the FOS wavelength scale. A total 19
       observations were made. They all were received and displayed. No
       anomalies were noted.

   1.14 Completed FOS/RD 3791 (Quasar Absorption Line Survey: Cycle 2

        Observations)

       The Faint object Spectrograph (Red Side) was used to make
       observations of quasar PKS0003+15. This is a continuation of
       proposal FOS 2424. The target was reported to be well centered. The
       observations were reported to be okay.

   1.15 Completed WFC 5013 (WF/PC Cycle 3 Calibration: WFC Flats Narrow. 2)


       The Wide Field Camera was used to make four Earth flat calibration
       images to be used for flat fielding of WFC observations. The
       observations used the narrow band filters, both with and without
       neutral density filters. A total of four observations were received.
       All four observations were reported to be okay.

   1.16 Completed 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. Six observations were received and displayed in the OSS.
       Five observations were reported to be saturated. One observation was
       reported to look okay, but 15 segments were missing. The DCF has
       requested an LOR to see if the missing data can be recovered.

   1.17 Completed FGS 4893 (Orbital Motions of Close Binary Stars: Cycle 3

        High)

       Fine Guidance Sensor #3 was used to make astrometric observations of
       the binary star system HD32923 to obtain its orbital elements. These
       observations are important since most of the estimates of stellar
       mass are made by observing elements of these systems. The astrometry
       was monitored and no problems were seen in the telemetry.

   1.18 Completed PC 4308 (Snapshot Survey for Companions to Planetary

        Nebula Nuclei - Cycle 3 High)

       The Planetary Camera was used to make an observation of the central
       region of planetary nebula EGB5. It is possible that the central
       star in a double star. The observation still remains on the science
       tape recorder, and will be analyzed later. No anomalies were
       reported.

2.0 FLIGHT OPERATIONS SUMMARY:

    2.1 Guide Star Acquisitions:

                            Scheduled Acquisitions : 18
                                        Successful : 17

                           The Guide Star acquisition at 309/1507Z failed 
on

                           secondary FGS #@ on its first attempt. However,
                           the second attempt was successful.


                          Scheduled Reacquisitions : 30
                                        Successful : 30

   2.2 FHST Updates:

                              Scheduled : 26
                             Successful : 26

   2.3 Significant HSTARs: None

   2.4 Operations Note:

        Simulation JIS #6 (EVA 4 and 5, plus Deploy) was initiated this

        morning, Monday, Nov. 8, 1993 at 8 AM and is scheduled to last for
        59 hours. No anomalies have been reported.

3.0 ACTIVITIES SCHEDULED FOR NEXT REPORTING PERIOD:

   3.1 Complete HSP/POL 3250 (Gravitational Lenses Part 1 - Cycle 2 High)

   3.2 Complete Three Sets of Setup 4947 (DF - 224 Flight Software

       Installation 9.0 and Higher)

   3.3 Complete FGS 5068 (Linking the HIPPARCOS to the Extragalactic

       Reference Frame part 6 of 6)

   3.4 Complete FGS 4893 (Orbital Motions of Close Binary Stars - Cycle 3

       High)

   3.5 Complete GHRS/2 5041 (GHRS Sensitivity Monitor - Cycle 3)

   3.6 Complete GHRS/2 5024 (GHRS Telescope Breathing Monitor - Cycle 3)

4.0 ANOMALY STATUS:

   4.1 Significant New Anomalies:

       The MSS#1 magnetic sensor had a V2 channel saturation event on
       Friday, Nov. 7 at (311/1600Z) which lasted for 3 hours and 45
       minutes. The DF-224 automatically switched to MSS#2. The unit
       reported lower than normal temperatures during this period, and was
       in the shadow of a High Gain Antenna. The project had previously
       decided to switch to the Magnetic Field Model should an MSS Channel
       Saturate for more than three hours. The Ground System uplinked and
       initiated a Mag-Field Model in the spacecraft. The anomaly is being
       investigated. An on-orbit test of the Magnetic Field Model was
       conducted in June 1993. The MSS#1 V2 channel has since returned to a
       normal signature.

   4.2 Significant Unresolved Anomalies: None

5.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time.

/DMH                           -END-