HUBBLE SPACE TELESCOPE

                       DAILY REPORT #1514

PERIOD COVERED:  0000Z (UTC) 11/08/95 - 0000Z (UTC) 11/09/95

Daily Status Report as of 313/0000Z

1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED:

1.1 Completed FOS/RD 6314 (QSO Broad Abs Line Region Gas)

       The Faint Object Spectrograph (Red Side) was used to obtain UV =
spectra of a QSO with broad absorption lines (BALs).  These BALs are =
believed to be produced by highly ionized gas moving out from the QSO at =
high velocity.  A UV spectrum of this target is needed to follow the shape =
of the continuum into the far UV.  The observation was executed as =
scheduled, and no anomalies were noted.

1.2 Completed WF/PC-2 6332 (The Circumnuclear Regions of Seyfert Galaxies =
LRF Part: Cycle 4 Medium)

       The WF/PC-2 and the linear ramp filter (LRF) were used to make =
observations for the circumnuclear regions of Seyfert galaxy FR680N18 in =
both emission and continuum.  From the data the PI expects to derive =
sufficient evidence to confirm or refute a suggested model of Seyfert Type =
2 galaxies.  The observations were executed as scheduled, and no anomalies =
were noted.

1.3 Completed WF/PC-2 6099 (Black Holes and Cores of Galaxies)

       The WF/PC-2 was used to search for possible black holes in the =
cores of nearby early-typr galaxies.  The WF/PC-2 will be used to obtain =
high resolution images of several galaxies to identify those with bright =
cores, and to provide sufficiently accurate coordinates for the FOS, which =
will be used to measure the velocity dispersion around selected galaxies.  =
The acquisition for this proposal, at 312/051449Z, failed to fine lock =
back-up on FGS-2 only.  The re-acquisition, at 312/064748Z, experienced the=
 same result.  HSTAR 5358 was written to document these events.  =
Otherwise, the observations were executed as scheduled, and no further =
anomalies were noted.

1.4 Completed WF/PC-2 5914 (The Formation History of Globular Clusters in =
M-33)

       The WF/PC-2 was used to make V and I observations of  globular =
cluster NGC-598-C20 AND NGC-598-R14 which is located in the M-33 galaxy in =
order to study its formation history.  Color-magnitude diagrams made from =
these images will be examined for evidence of a  parameter other than =
metallicity that influences the evolutionary development of stars.  The =
observations were executed as scheduled, and no anomalies were noted.

1.5 Completed WF/PC-2 6187 (WF/PC-2 Cycle 5 Calibration: Earth Flats)

       The WF/PC-2 was used to make Earth streak-flat calibration images. =
These streak-flats will be used to produce flat fields, to map the OTA =
illumination pattern and, in combination with other data, to produce new =
superflats.  The observations were completed as planned, and no problems =
were reported.

1.6 Completed WF/PC-2 6060 (The Structure of Nova Shells)

       The WF/PC-2 was used to make observations of the nova shell around =
GK-Perseus in order to study its structure.  The goal is to determine =
whether these shells are broken into knots, and if so, to determine the =
size distribution of the knots.  The observations were completed as =
planned, and no anomalies were noted.

1.7 Completed WF/PC-2 6119 (Snapshot Survey for Companions of Planetary =
Nebula Nuclei)

       The WF/PC-2 was used to make snapshot survey observations of =
planetary nebulus IW1 to study their nuclei and to look for possible =
companions.  The observations were executed as scheduled, and no anomalies =
were noted

2.0 FLIGHT OPERATIONS SUMMARY:

   2.1 Guide Star Acquisitions: 

                            Scheduled Acquisitions : 5
                                        Successful : 5

                          Scheduled Reacquisitions : 10
                                        Successful : 10

   2.2 FHST Updates: 

                              Scheduled : 7
                             Successful : 7

   2.3 Operations Notes: 

       Operations were uneventfully conducted from the SAMS back-up =
facility for four hours last night.

3.0 SIGNIFICANT FORTHCOMING EVENTS: 

        Nothing at this time.