THE SECRET SPIES IN THE SKY - Imagery, Data Analysis, and Discussions relating to Military Space
SatTrackCam Leiden (Cospar 4353) is a satellite tracking station located at Leiden, the Netherlands. The tracking focus is on classified objects - i.e. "spy satellites". With a camera, accurate positional measurements on satellites of interest are obtained in order to determine their orbits. Orbital behaviour is analysed.
This blog analyses Missile tests too.
Showing posts with label flyby. Show all posts
Showing posts with label flyby. Show all posts
Monday, 3 July 2017
Close Encounters of the Classified Kind
The Space Review has just published my paper on the close ISS flyby of US spy satelllite USA 279.
Saturday, 16 June 2012
OT: Near Earth Asteroid 2012 LZ1 fly-by imaged, June 15
On June 10, 2012, Australian Siding Spring astronomer Rob McNaught and colleagues discovered a bright Near Earth Asteroid (NEA). It got the provisional designation 2012 LZ1 and turned out to be large: it is estimated to be about 500 meter in diameter (UPDATE 22 June 2012: radar observations from Arecibo obtained during the fly-by actually showed it to be twice as large, i.e. 1 km diameter! This suggests a low albedo, which might imply a carbonaceous composition). It made it's closest approach to the earth/moon system around midnight of June 14/15. With a pass distance of 5.3 million km (a multitude of the Earth-Moon distance), this flyby was not particularly close. But because the asteroid is large, it became quite bright, ~ mag. +13.
In the early morning of June 15, some 9 hours after closest approach, I used the "remote" 37-cm F/14 Cassegrain of UoI Rigel observatory at Sonoita, Arizona, USA (MPC 857, the same telescope that I often use to image geostationary satellites) to image the asteroid (I also obtained some imagery using the larger 61-cm telescope of Sierra Stars Observatory in California).
The image above is a stack of 4 CCD images, each of 30 second exposure and spaced 5 minutes in time, obtained with the Rigel telescope. The asteroid can be seen as a set of 4 short trails lining up. It was moving at a rate of about 35"/minute near the Aquila-Capricorn border at that time and was near mag. +13.
In the early morning of June 15, some 9 hours after closest approach, I used the "remote" 37-cm F/14 Cassegrain of UoI Rigel observatory at Sonoita, Arizona, USA (MPC 857, the same telescope that I often use to image geostationary satellites) to image the asteroid (I also obtained some imagery using the larger 61-cm telescope of Sierra Stars Observatory in California).
click image to enlarge
The image above is a stack of 4 CCD images, each of 30 second exposure and spaced 5 minutes in time, obtained with the Rigel telescope. The asteroid can be seen as a set of 4 short trails lining up. It was moving at a rate of about 35"/minute near the Aquila-Capricorn border at that time and was near mag. +13.
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