Seiichi Yoshida informed me of four suspected large amplitude red variables on DSS images, noted during his researches, that were worthy of further investigation. A star at 03 59 57.70 +57 38 14.1 (2000) clearly shows very marked variation on three red plate images sourced via the USNOFS image and catalogue server at www.nofs.navy.mil/data/FchPix/ , marked variation is also seen on the three blue plates, indeed on one of these the star is actually fainter than a very close blue mag ~18 neighbouring star that is either partially obscured or in one case totally hidden by the variable star on the red plates. Variation is also seen between the two far red plates. Contemporaneous E (red) and O (blue) plates from the 1950s DSS1 survey show the object to be very much brighter indeed on the red plate, and the object is bright on the far red IVN plates. This star is most likely a Mira. (Interestingly a "blue" luminous star, LS I +57 140, lies barely half an arcmin distant south-following, which can be of similar brightness to the variable when the latter is nearer maximum (probably near red mag 14), so should give an aesthetically pleasing contrast to the naked eye at the telescope). IDENTIFICATIONS : USNOB1.0 1476-0155161 RA 2000 03h59m57.73s error 81 mas DEC2000 +57d38'14.3" error 106 mas GSC2.2 N312233258237 RA 2000 03h59m57.70s error 0.282860" DEC2000 +57d38'14.1" error 0.297817" John Greaves