HUBBLE SPACE TELESCOPE DAILY REPORT #1678 PERIOD COVERED: 0000Z (UTC) 07/18/96 - 0000Z (UTC) 07/19/96 Daily Status Report as of 201/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed FOS/RD 6577 (An Expanded Survey for Study of the = Lyman-Alpha Line and QSO Mg II Absorption) The Faint Object Spectrograph (Red Side) was used to make = observations of the QSO PKS0421+01 in order to make a survey of the = Lyman-Alpha line and the 68 Mg II absorption line system. The = observations were completed as scheduled, and no problems were reported. 1.2 Completed Three Sets of FOS/RD 6236 (FOS Cycle 5: Location of = Spectra and Wavelength Calibration: Red Side Detector) The Faint Object Spectrograph (Red Side) was used to make = calibration observations in order to determine the location of spectra = and to perform a wavelength calibration. All observations were internal. = A Taled calibration was also completed. The observations were completed = as planned, and no anomalies were reported. 1.3 Completed GHRS/2 6782 (Testing the Theory of Radiative Levitation = in DA White Dwarfs) The High Resolution Spectrograph (Side Two) was used to make = observations of the DA white dwarf star REJ1614-08 in order to test the = theory of radiative levitation. This theory predicts that for high = enough temperatures, the radiation pressure should prevent elements = heavier than H or He from sinking out of the atmosphere of the star. A = wave length calibration image was also taken. The observations were = completed as planned, and no anomalies were reported. 1.4 Completed Two Sets of WF/PC-2 6630 (The Nucleus of Comet 22P/Kopff = and Its Dust Gas Emissions) The WF/PC-2 was used to make observations of the periodic comet = 22P/Kopff in order to study the nucleus of the comet and its dust = emissions. At the minimum geocentric distance, the spatial resolution = will be about 38 KM, allowing the nucleus to be distinguished from the = coma. The observations were executed as scheduled, and no anomalies were = noted. 1.5 Completed FOS/BL 6470 (Decoding the Inner Dsik About = Beta-Pictoris) The Faint Object Spectrograph (Blue Side) was used to make = ultraviolet spectrographic observations of the disk around the star Beta = Pictoris (aka, HD39060) looking for emission lines arising in the inner = disk. The objective is to ascertain the composition of the inner disk. = The observations were completed as planned, and no problems were = reported. 2.0 FLIGHT OPERATIONS SUMMARY: 2.1 Guide Star Acquisitions: Scheduled Acquisitions : 10 Successful : 10 Scheduled Reacquisitions : 4 Successful : 4 2.2 FHST Updates: Scheduled : 10 Successful : 10 2.3 Operations Notes: There were no reported operational problems, as the HST returned = to normal science operations. 3.0 SIGNIFICANT FORTHCOMING EVENTS: Nothing at this time. /DMH