HUBBLE SPACE TELESCOPE

                              DAILY REPORT #1413

PERIOD COVERED:  0000Z (UTC) 06/15/95 - 0000Z (UTC) 06/16/95

Daily Status Report as of 167/0000Z

1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED:

   1.1 Completed GHRS/1 5595 (GHRS ECH-A Wavelength Monitor: Cycle 4) 

       The High Resolution Spectrograph (Side 1) was used to make wavelength
spectral lamp calibration observations to measure the instrumental
characteristics of the Echelle-A spectrograph. The observations were
completed as planned, and no problems were reported. 

   1.2 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 NGC-7582 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. 

   1.3 Completed WF/PC-2  5476 (Continuum Snapshots of 3CR Radio Galaxies) 

       The WF/PC-2 was used to make snapshot images of radio galaxy 3C18.0 as
part of a continuum survey and to study the galaxy's morphology. The
observations were executed as scheduled, and no anomalies were noted.

   1.4 Completed WF/PC-2 5981 (Calibration of Nearby Type IA Supernova as
Standard Candles: NGC-4639)

       The WF/PC-2 was used to make observations of Cepheid variable stars in
Galaxy NGC-4639 (which has produced a Type IA Supernova) to calibrate the
nova's absolute brightness so that it can be used as a standard candle for
distance measurements. The observations were executed as scheduled, and no
anomalies were noted.

   1.5 Completed WF/PC-2 5985 (WF/PC-2 B-Band + Lyman Alpha Imaging of a
Cluster of Young Galaxies at Z = 2.0)
=
       The WF/PC-2 was used to make B-Band and Lyman Alpha observations
(i.e., two color images) of the young dwarf spheroidal galaxy 53W002 located
in Draco and which has a redshift of around 2.0. The observations were
executed as planned, and no problems were reported.

   1.6 Completed FOS/BL 5459 (Ultraviolet Interstellar Polarization: Cycle 4
High)

       The Faint Object Spectrograph (Blue Side) was used to make ultraviolet
spectrographic observations of the bright star HD207538 to study interstellar
polarization along the line of sight to the star. This is to study
interstellar grains that are responsible for the extinction and polarization
of the star light. The observations were executed as scheduled, and no
anomalies were reported.

2.0 FLIGHT OPERATIONS SUMMARY:

   2.1 Guide Star Acquisitions: 

                            Scheduled Acquisitions : 3
                                        Successful : 3

                          Scheduled Reacquisitions : 11
                                        Successful : 11

   2.2 FHST Updates: 

                              Scheduled : 6
                             Successful : 6

   2.3 Significant HSTARs: None

   2.4 Operations Notes: 

       No operational problems were reported.

3.0 SIGNIFICANT FORTHCOMING EVENTS: 

        Nothing at this time.

/DMH
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