HUBBLE SPACE TELESCOPE DAILY REPORT #962 PERIOD COVERED: 0800 EST Daily Status Report as of 243/1200Z. 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed WFC 4713 (WF/PC Cycle 2 Calibration: WFC Internal Delta Flats) The Wide Field Camera was used to make a total of four internal flat calibrations images. The first image was saturated, and the other three were reported to look okay. 1.2 Completed WFC 4385 (Spectroscopy and Imagery of Orion's Nebula - Cycle 3 High) The Wide Field Camera was used to make image of regions in the Orion Nebula to learn more about its small structure at short wavelengths. The onboard target acquisition failed, and a status buffer error message was generated. An HSTAR was written. A corrective point maneuver was successfully calculated, and uplinked to the spacecraft. Subsequent observations were received and displayed. They were reported to look okay. The was also one recentering event which was reported to have occurred in one of the later observations. 1.3 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, however, it was filed as being bad due to a recentering event. 1.4 Completed PC 4140 (WF/PC Cycle 2 Calibration: Rapid Internal Monitor - Part 2) The WFPC was used to make two internal flat calibrations images to check for new forms of contamination (i.e., Daises and measles), and to check for the possible return of quantum efficiency hysteresis. Both observations completed as scheduled, and no problems were reported. They were reported to look okay. 1.5 Completed FGS 4935 (Parallaxes of Hyades Cluster Members - Cycle 3 High) The Fine Guidance Sensors were used to make astrometric observations of stars VA383 and PCEN383 which is located in the Hyades cluster to obtain a definitive calibration of its population I zero-age main sequence members. The observation appeared to executed with no problems. 1.6 Completed FOS/RD 4545 (Outgassing From Ceres - Cycle 3 High) The Faint Object Spectrograph was used to make observations of the asteroid CERES to help confirm an IUE observations which detected OH emissions from the asteroid. The Decision observation was received in real-time and indicated that the target was perfectly centered. No pointing correction maneuver was necessary. The first science observation was received in the OSS and displayed for the investigator. The observations are still ongoing at this time. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 5 Successful : 4 FGS #1 failed to acquirer fine lock at 243/0549Z, and successfully obtained course track back-up. There were no indications of vehicle errors. Scheduled Reacquisitions : 10 Successful : 10 2.2 FHST Updates: Scheduled : 7 Successful : 7 2.3 Significant HSTARs: None 2.4 Operations Note: None 3.0 ACTIVITIES SCHEDULED FOR NEXT REPORTING PERIOD: 3.1 Complete FOS/RD 4545 (Outgassing of Ceres - Cycle 3 High) 3.2 Complete WFC 4929 (WF/PC Cycle 2 : Improved Dark Calibration) 3.3 Complete WFC/PC 5026 (WF/PC Cycle 3 Calibration: Rapid Internal Monitor) 3.4 Complete FOC/96 4546 (Imaging of UV Bright Stars in the galactic Bulge) 3.5 Complete Three Sets of WFC 4713 (WF/PC Cycle 2 Calibration: WFC Internal Delta Flats) 3.6 Uplink Updated Ephemeris Tables, Per MOSES 2871 3.7 Complete PC 4712 (WF/PC Cycle 2 Calibration: Measles Monitor) 3.8 Complete WFC 5013 (WF/PC Cycle Flats Narrow. 2) 3.9 Complete PC 4714 (WF/PC Cycle Calibration: PC Internal Delta Flats) 3.10 Complete FOS/BL 4662 (Exploring Trition's UV Spectrum: The First 1800-2500 AO UV Survey) 4.0 ANOMALY STATUS: 4.1 Significant New Anomalies: None 4.2 Significant Unresolved Anomalies: None 5.0 SIGNIFICANT FORTHCOMING EVENTS: The JIS #2 Simulation will be initiated today (Tuesday, Aug. 31, 1993 at 2200Z). The simulation will cover sequences 50 through 60 (PREP FOR SA RETRACT through SAFE MCU), and should last for approximately 37 hours. /DMH -END-