The previously published
period for the variable star V1176 Sagittarii, an RR Lyrae star of type RRab,
has been confirmed for the years 1942 through 1966. Since 1966, V1176 Sgr has
undergone at least two period changes. New periods and epochs have been
determined for 1967-76 and 1977-80. V1176 Sgr was observaed via the
photographic plate collection of the Maria Mitchell Observatory.