More tracking of USA 245, and being flashed by ALOS

After my observations in the hours after launch on August the 28th and my observations on September 3, I observed the newly launched KH-11 Keyhole USA 245 (NROL-65, 2013-043A) again yesterday evening.

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It was brighter yesterday than during my previous observations, this time reaching an easy naked-eye brightness. Near 20:38:15 UTC it slowly brightened to mag.+1. Above is one of my images, showing it as it traverses the northern part of Cygnus.

Ten minutes earlier, I observed USA 186 (2005-042A), the KH-11 Keyhole launched in 2005 that USA 245 in time is meant to replace. For the moment, they probably will operate together in the same orbital plane for several years. The image below shows it traversing Cepheus.

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After observing USA 186 and while waiting for USA 245, a very bright (up to mag. 0), slowly and irregularly flaring object appeared near 20:33 UT. It turned out to be ALOS (2006-002A), the Japanese Earth Observation satellite that malfunctioned in 2011. It evidently is slowly tumbling. Below are two images, showing the irregular brightness variation:

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Yet another Japanese satellite failure!

The Japanese, already suffering from the major devastation of the recent earthquake, truely don't seem to catch a break.

Today news broke that yet another Japanese radar- and optical satellite has broken down on orbit. It concerns ALOS, a non-classified Earth Observation satellite including radar, visual and infrared sensing equipment.

This comes after the 2007 malfunction of the classified SAR satellite IGS 1B, which is now developing into a re-entry hazard concern for 2012 (as discussed extensively on this blog in a post from last weekend): and the 2010 malfunction of their other classified SAR satellite, IGS R2.

In the aftermath of the recent earthquake, losing their prized remote sensing satellites must really be a pain for the Japanese: this is all really at the most untimely of moments.

Unlike IGS 1B, ALOS is not a direct re-entry hazard for the near future. In a 697 x 694 km orbit (notably higher than that of the IGS-es), it will take a considerable time for it to decay.