Distribution:
      I am filling in for Charlie Wolf and sent the daily as an =
attachment.  It seems this presents a problem for many persons.  I am =
sending this again, not as an attachment.  If anyone has a problem reading =
this please call me at 286-3311.  Sorry for the problem!!
Dave Lychenheim


                     HUBBLE SPACE TELESCOPE

                       DAILY REPORT #1515

PERIOD COVERED:  0000Z (UTC) 11/09/95 - 0000Z (UTC) 11/13/95

Daily Status Report as of 317/0000Z

1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED:

1.1 Completed WF/PC-2 5732 (Imaging the Hot Stellar Content of Early Type =
Galaxies)

       The WF/PC-2 was used to make far ultraviolet observations of early =
type elliptical galaxy NGC-4627 to study its hot stellar contents. The =
observations were completed as planned, and no anomalies were reported.

1.2 Completed WF/PC-2 5996 (The Morphology of Field Galaxies at High =
Redshifts)

       The WF/PC-2 was used to make observations  of several field =
galaxies (Field-2217) in order to study their morphologies. The =
observations were completed as planned, and no anomalies were reported.

1.3 Completed GHRS/2 6065 (ZAMS Atmospheric Structure as a Function of =
Rotation)

       The High Resolution Spectrograph (Side Two) was used to make =
emission line spectrographic observations of the zero-age main sequence =
(ZAMS) star HD82443 in order to study its atmospheric structure as a =
function of rotation. Wavelength calibrations, internal flats, and dark =
calibration images were also taken. The observations were executed as =
scheduled, and no anomalies were noted.

1.4 Completed WF/PC-2 6311 (The Structure of Nova Shells)

       The WF/PC-2 was used to make observations of the shell of recurrent =
nova T-Pyxidis. The expansion of the shell, and the size distribution of =
the knots in the shell, will be determined. The observations were executed =
as scheduled, and no anomalies were noted.

1.5 Completed WF/PC-2 5913 (Low-Mass Binaries and Luminosity Function)

       The WF/PC-2 was used to make observations of the low-mass binary =
system SGP007 (Late Type Class M dwarf stars). The intent is to determine =
why the local stellar luminosity function is flat below Mv=3D12, while =
that found from more distant stars falls by an order of magnitude by =
Mv=3D14. The observations were executed as scheduled, and no anomalies =
were noted.

1.6 Completed FGS 6047 (Calibrating the Mass Luminosity Relation at the =
End of the Main Sequence)

       The FGS were used to make astrometric observations of star GL748 as =
part of a study to determine its mass luminosity relationship. The purpose =
is to measure the precise parallax and relative orbit of its faint =
companion. The observations were completed as planned, and no problems =
were reported.

1.7 Completed WF/PC-2 6253 (Pure Parallel Archive Program)

       The WF/PC-2 was used to execute a pure parallel program taking =
ultraviolet observations running concurrent with prime science =
observations. The intent is to search for extra-galactic sources with flux =
excesses at 3000 A0 and galactic sources with excesses at 1600 A0. The =
observations were completed as planned, and no problems were reported.

1.8 Completed GHRS/2 5857 (Is Mixing or Mass Loss the Cause of Decline in =
12C/13C)

       The High Resolution Spectrograph (Side Two) was used to make =
spectrographic observations of the halo star HD103095 to study the ratio =
of its 12C/13C Carbon and the abundance of its Boron. The results will =
influence models of evolution off of the main sequence. The observations =
were completed as planned, and no problems were reported.

1.9 Completed Two Sets of GHRS/2 5869 (Chromospheric Activity in Quiet =
stars: Halo Subdwarfs)

       The High Resolution Spectrograph (Side Two) was used to make =
spectrographic observations of the quiet stars HD84937 and HD201891 to =
study its chromospheric activity. This is a search for Mg II emission in =
low metallicity solar temperature field stars in the galactic halo. The =
observations were completed as planned, and no problems were reported.

1.10 Completed WF/PC-2 5999 (The Nuclear Structure of S0 Galaxies: A PC =
Imaging Survey)

       The WF/PC-2 was used to make observations of S0 class galaxy =
ICI-919 in order to study its nuclear structure. This is a part of a large =
survey of S0, E/S0, and S0/a class galaxies. The targets will cover a wide =
range in luminosity and environment. The observations were completed as =
planned, and no anomalies were noted.

1.11 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 NGC-40 to study their nuclei and to look for possible =
companions. The observations were executed as scheduled, and no anomalies =
were noted.

1.12 Completed FOS/BL 6038 (Winds of Massive Stars in Nearby Galaxies, the =
WR Stars)

   The Faint Object Spectrograph (Blue Side) was used to make =
spectrographic observations of the massive Wolf-Rayette star M-33-OB88-7 =
which is located in the M-33 Galaxy in order to study its stellar winds. =
The observations were completed as planned, and no problems were reported.

1.13 Completed FOS/RD 6237 (Molecular Hydrogen toward a QSO)

       The Faint Object Spectrograph (Red Side) was used tp measure the =
columen density and excitation of molecular hydrogen in a QSO.  Metal =
abundances and dust content will also be measured.  The observations =
consist of a single 8750-second expossure, plus target acquisitions.  The =
observations were completed as planed, and no problems were reported.

1.14 Completed WF/P-2 6254 (GTO Pure Parallel Program - Cycle 5)

       The WF/PC-2 was use to make random long exposures of high galactic =
fields taken in parallel with the prime science observations to obtain a =
random sample of galaxies. The observations were executed as scheduled, =
and no anomalies were noted.

1.15 Completed WF/PC-2 6225 (Resolving Dust Around Shell Stars)

       The WF/PC-2 was used to make deep image observations of A-class =
shell star HR-4368 looking for protoplanetary disks, like that around Beta =
Pic. The observations were executed as scheduled, and no anomalies were =
noted.

1.16 Completed WF/PC-2 5957 (Snapshot of 3CR Radio Galaxies)

       The WF/PC-2 was used to make observations for radio galaxy 3C264.0 =
to study the morphology of the radio galaxy. The observations were =
executed as scheduled, and no anomalies were noted.

1.17 Completed WF/PC-2 5353 (Low-Mass Binaries in the Hyades: Cycle 4 =
High)

       The WF/PC-2 was used to make images of the low-mass, late M-Class =
dwarf star RHY230 which is located in the Hyades cluster. Some of the =
companion stars may be brown dwarfs. The observations were completed as =
scheduled, and no problems were reported.

1.18 Completed WF/PC-2 6250 (WF/PC-2 Cycle 5 Calibration: Internal =
Monitor)

       The WF/PC-2 was used to make a series on internal calibration =
observations. Internal flats, biases, and K-Spot calibration images were =
taken. These observations are designed to monitor the health of the =
cameras. The observations were executed as scheduled, and no anomalies =
were noted.

1.19 Completed WF/PC-2 6114 (White Dwarf Distance and Precision Age for =
the Globular Cluster 47 Tuc)

       The WF/PC-2 was used to make observations of white dwarf star =
WD2326+049 which is located in the globular cluster 47 Tuc in order to =
study the clusters age and distance. This set of observations will be used =
to determine the distance to 47 Tuc, hopefully to an accuracy of better =
than 10%. The observations were executed as scheduled, and no anomalies =
were noted.

1.20 Completed FGS 6271 (L726-8/UV Ceti)

       The FGSs were used to make astrometric observations of the binary =
star UV Ceti to search for a short period low-mass companion around either =
component of this binary object. The observations were executed as =
scheduled, and no anomalies were reported.

1.21 Completed WF/P-2 6254 (GTO Pure Parallel Program - Cycle 5)

       The WF/PC-2 was use to make random long exposures of high galactic =
fields taken in parallel with the prime science observations to obtain a =
random sample of galaxies. The observations were executed as scheduled, =
and no anomalies were noted.

1.22 Completed WF/PC-2 5973 (The Host Galaxies of Radio Quite High =
Redshift Quasi-stellar Objects)

       The WF/PC-2 was used to make observations of the host galaxies of =
radio quite high red shift quasi-stellar object 0050-280. These data will =
be compared to existing data sets for radio-loud, high-redshift QSOs and =
ground based data on radio-quiet, low-redshift QSOs. The observations were =
executed as scheduled, and no anomalies were noted.

1.23 Completed WF/PC-2 5479 (Subarcsecond Structure in Nearby AGNs)

       The WF/PC-2 was used to make snapshot observations of the nearby =
active galactic nuclei of HEAO-1-025 to study the interactions between the =
central engine, the stars, and the interstellar matter in the AGN. The =
observations were executed as scheduled, and no anomalies were noted.

1.24 Completed WF/PC-2 5995 (Galaxies in a Very High-Z Cluster)

       The WF/PC-2 was used to image a very distant cluster of galaxies =
around 3C184 (z=3D0.996).  The purpose is to study the morphology of the =
galaxies in this cluster, and to compare them with galaxies in relatively =
nearby clusters.  This should lead to insights about the formation and =
evolution of galaxy clusters.  The observations were completed as =
scheduled, and no anomalies were noted.

1.25 Completed WF/PC-2 5974 (The Evolution of Radio Loud Quasars)

       The WF/PC-2 was used to make observations of the radio loud  large =
redshift quasar MRC1114-22. The purpose is to determine if these galaxies =
are from the same parent population as other kinds of radio galaxies =
already studied using HST. The observations were completed as scheduled, =
and no problems were reported.

2.0 FLIGHT OPERATIONS SUMMARY:

   2.1 Guide Star Acquisitions: 

                            Scheduled Acquisitions : 14
                                        Successful : 14

                          Scheduled Reacquisitions : 20
                                        Successful : 20

   2.2 FHST Updates: 

                              Scheduled : 38
                             Successful : 38

   2.3 Operations Notes: 

FOS observations affected by loss of fine lock @317:03:15z.  Documented by =
HSTAR # 5360 (affected proposal 5824).
****

3.0 SIGNIFICANT FORTHCOMING EVENTS: 

        Nothing at this time.

/DMH