After looking for 3 days saw it tonite from 1234UT . Date is April 5 UTC. At 12 43m 24secUT at RA 11h 12.5m , Dec +8.6degrees At 12 51m 44secUT ar RA 11h 39.5 , Dec +7.5 d At 13 22 05sec UT RA 11h 46.8min Dec +6.25d At 13 39 42secUT RA 12h 00.2min Dec +4.4d Dec drift 4.55 degrees per hour Not seen at when restarted observing at 1400UT [ should be in eclipse] The Dec drift from trakstar for 6913B is 4.25 d/hour. >From (34.97S, 138.6317E ) I am in some doubt about identification as this was some 11min in RA West, and 1.2 degrees N of the 6913B ephemeris. Can somebody suggest the most accurate programme to use with such high satellites? The orbital elements for 6913B are now 19 days old, and I am uncetain of their validity. Using my fix April 2, it is possible to say that the period is such that the object is at same RA 4minutes and 15 seconds earlier each day. This gives a slow eastward drift of say 0.1 degrees longitude per day. The declination drift means the inclination has to be similar or even a little bigger than 6913B's. The flash periodis definitely decreasing from 19.699 on march 30.57 , to 19.579 on April 5.54 I also saw another flasher, only reaching mag 6 with a period round 30 seconds and a double peak about 0.5 secs apart, but observed the original object. Tony Beresford