> Of course this will be a BWGS top-priority object. Many of this Zenit second stages began their flash period life time with a period of about 0.4s. I hope this will be a fast flasher as well. This is a totally random thought, but has anyone looked to see if there's any correlation between the 14th-order resonance-induced fluctuations in orbital decay rate and flash rate for these objects? I can't really think of any reason there should be, but with the amount of data that must be available by now it might be worth a quick look. ------------------------------------------------------------------------- Subscribe/Unsubscribe info, Frequently Asked Questions, SeeSat-L archive: http://www.satobs.org/seesat/seesatindex.html
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