An analysis of 56 published radial velocities of Delta Sco that cover the interval 1903-1975, has yielded the following provisional spectroscopic period and orbital elements. The results from this study are being provided prior to the complete analysis because of the importance of the period to photometric observers. Observations from the Yerkes, Allegheny, Dominion (Ottawa), McDonald, and KPNO/CTIO Observatories were used. (The errors quoted are standard errors.) An ephemeris of predicted times of putative eclipses is also provided; a comparison to recent photometry was not done. P = 78.860 +/- 0.0017 days T = JD 2442776.075 +/- 0.17 e = 0.10 +/ -.17 w = 254.9 +/- 95.04 V0 = -12.2 +/- 1.5 km/sec K = 10.3 +/- 2.4 km/sec T Min. I = JD 2427769.523 + 78.860*E T Min. II = JD 2427728.773 + 78.860*E Some of these data occur near the predicted periastron passage in the interferometric orbit (P=10.583). Analysis of the radial velocity data, especially with regard to that orbit. Cordially, Thom Gandet -- ************************************************************************ Lizard Hollow Observatory Thomas L. Gandet, Director PO Box 77021 Tucson, AZ 85703-7021 USA ************************************************************************