Geostationary bonanza

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The images above and below are two small parts of one single image shot on May 2nd 2016, using a SamYang 1.4/85mm lens on a Canon EOS 60D with 30 seconds exposure (ISO 1000) under a very dark sky. These two image excerpts overlap in the corner: the upper right corner of the image excerpt above overlaps with the lower left corner of the image excerpt below.

Although both sub-images are only a few degrees wide, they show a bonanza of objects, including 3 classified objects.

In the image above, 11 objects including the classified SIGINT satellite PAN (2009-047A) are visible. PAN is parked next to the commercial communications satellite Yahsat 1B.

In the image below, 10 objects including two classified objects are visible: the two classified objects are the SIGINT satellite Mercury 1 (1994-054A), and the SIGINT satellite Mentor 4 (2009-001A), the latter parked next to the commercial communications satellite Thuraya 2.

The full 10 x 14 degree image, of which the images featured here are small excerpt parts, shows over 30 objects.

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Imaging a "UFO" (Ultra High Frequency Follow-On)

UFO F2 on 3 March 2016
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The image above is my first image of a UFO...

(* cue X-Files tune *)

No need to call in Mulder, however. The object in the image is a geosynchronous satellite, UFO F2 (1993-056A).

The truth is out there

The acronym 'UFO' in this case does not stand for the classic Unidentified Flying Object. It stands for Ultra High Frequency (UHF) Follow-On, the name of a class of US Navy communication satellites.

The UFO satellite constellation consists of 11 satellites (not all of them operational) in geosynchronous orbit, launched between 1993 and 2003. It serves fleet-wide communication needs for the US Navy (including its submarines, but also Marine units on land). The system is currently being replaced by the newer MUOS constellation (see a previous post) and will gradually be phased out.

UFO satellite constellation on 9 March 2016
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The first launch in the series, the launch of UFO F1 on 25 March 1993 with an Atlas 1 from Cape Canaveral, resulted in a partial failure to reach the intended geosynchronous orbit due to the failure of one of the rocket engines. The second UFO launch, UFO F2, the one imaged above, was the first truely successful launch of this satellite class.

USA 236 on 28 February 2016
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I imaged more geosynchronous objects the past week, taking advantage of clear moonless evenings. The image above shows a star field in Orion in the evening of 28 February 2016, with USA 236 (SDS 3 F7, 2012-033A), an SDS data communications satellite in geosynchronous orbit. These satellites relay data from other US military satellites, optical and radar reconnaissance satellites in Low Earth Orbits such as the KH-11 'Keyhole'/CRYSTAL, Lacrosse (ONYX) and FIA (TOPAZ), to the US.

PAN on 28 February 2016
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I also did my periodic revisit of the enigmatic SIGINT satellite PAN (2009-047A) as well (see image above). PAN is still stable at 47.7 E (see my long-term analysis here), near Yahsat 1B. The image above shows it near that satellite and a number of other commercial communications satellites in an image taken on 28 February 2016.

Mercury 1 r on 3 March 2016
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On Feb 28 and March 3, I recovered Mercury 1 r (1994-054B), the upper stage from the launch of the Mercury 1 SIGINT satellite. We had lost this object for a while, it had not been seen for 153 days when I recovered it. The image above shows it in Hydra on 3 March 2016.

USA 186 on 5 March 2016
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As spring is approaching, the visibility of satellites in Low Earth Orbit is gradually coming back for northern hemisphere observers.  This means we can take over from our lone southern hemisphere observer, Greg. The image above shows the KH-11 'Keyhole'/CRYSTAL optical reconnaissance satellite USA 186 (2005-042A) imaged on 5 March 2016.

Imaging Geostationary satellites, and PAN's past relocations

Last week saw some clear evenings, and I used one of them to image some geostationary satellites. It concerned "the usual suspects": MENTOR's, MERCURY's and the enigmatic, probably SIGINT satellite PAN (2009-047A). The latter satellite has not been moved for quite a while now: since the end of 2013 it is at longitude 47.7 E, parked close to a number of commercial comsats. In the past it was frequently relocated, taking positions next to various commercial COMSATS. In four years time between 2009-2013, it moved at least 9 times (which is a lot) to various longitudes between 33 E and 52.5 E.

PAN amidst several commercial COMSATS on 9 December 2015 (click to enlarge)

The diagram below charts these frequent movements of PAN. Relocations typically took place about once every 6 months. Late 2013, they stopped. PAN however must still be operational, as active station-keeping is necessary for it to stay at 47.7 E.

relocations of PAN over time, 2009-2015 (click to enlarge)

Four other SIGINT satellites and a military comsat were imaged as well: Mentor 4 (2009-001A) and Mentor 6 (2012-034A), Mercury 1 (1994-054A) and Mercury 2 (1996-026A), and the military comsat Milstar 5 (2002-001A).

Mentor 4, next to commercial comsat Thuraya 2 on 9 Dec 2015 (click to enlarge)

Mentor 6 and a number of commercial satellites, close to the Orion nebula, on 9 Dec 2015

Using the remote telescope at Warrumbungle (MPC Q65) in Australia, I recently (4 December 2015) also checked-up on the recently launched US Navy COMSAT MUOS 4 (2015-044A). It is still at its check-out location over the Pacific at longitude 172 W, but some recent press statements suggest check-out has been successfully completed, and it will be moved to its operational position at longitude 75 E near India in the spring of 2016.

CLIO

On 16 September 2014, the US military launched an enigmatic satellite (2014-055A) from Cape Canaveral into a geostationary orbit. It was not disclosed for which agency the object was launched (this is information that usually is disclosed). Nor what its function would be (this is information sometimes but not always disclosed). All we know is the rather uninformative name, CLIO, that it was built by Lockheed Martin and based on their commercial A-2100 bus.

CLIO imaged on May 13, 2015 (click image to enlarge)

CLIO is currently located at longitude 108.0 E, over Indonesia, where I imaged it yesterday using the 0.51-m telescope of Warrumbungle (MPC Q65) in Australia. The image can be seen above: CLIO is positioned just north of Telkom 1 (1999 042A), an Indonesian satellite for satellite telephony. (since Telkom 1 is also built on a Lockheed A2100 bus, the brightness difference in the image above is interesting, and probably due to different attitudes (orientations) of the satellites, although it potentially could also indicate custom components on CLIO, e.g. something like a large dish antenna).

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In many ways CLIO appears similar to another enigmatic satellite,  PAN (USA 207, 2009-047A), launched in September 2009 and infamous among our amateur tracking network for its frequent repositioning.

PAN was also built by Lockheed Martin and like CLIO based on the A-2100 bus. As with CLIO, the government agency behind it was not disclosed, and no indications of its role provided. What was known, is that PAN was developed and built rapidly (in less than 3 years time) using off-the-shelf commercial parts, apparently in response to an urgent need of some undisclosed government agency (which I suspect is either the CIA or NSA). Much speculation has occurred about the role of the spacecraft. The frequent relocations (which stopped at the end of 2013) make clear it is not a simple communications or early warning platform. PAN is currently located at longitude 47.9 E over east Africa.

Because of the similarities, several analysts believe that CLIO, five years after PAN, is a follow-on to the PAN program. The two satellites are currently 60 degrees separated in longitude.

An unknown object in (near) Geostationary orbit: Express AM-5?

The evening of December 29 2013 started clear, so I did a small survey of a part of the geostationary belt. Main focus of the session was PAN, as well as Mentor 4 and 6.

Inspecting the images I found an unidentified object in near-Geostationary orbit some 4 degrees east of PAN, between Mentor 6 and NSS 5, on several images (positions here). The image below shows it near M42, the Orion nebula, near 19:17 UT:

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In addition to the UNID you can also see a classified satellite at left, Mentor 6 (2012-034A), a SIGINT satellite also known under the code name Advanced Orion. At right are two commercial geostationary satellites, NSS 5 (1997-053A) and Galaxy 26 (1999-005A).

Cees Bassa in the Netherlands and Greg Roberts in South Africa also observed what is likely the same UNID object later that night. While it is not easy to fit a reliable orbit to such a relatively short span of observations, the suggestion is an object with an inclination near 0 and a Mean Motion of about 0.92 revolutions per day, i.e. an object near Geostationary altitudes.

The Mean Motion could suggest an old object being moved to a Graveyard Orbit. If this is the case, we haven't been able to identify which 'old' object it is yet.

Another option is that this is a new object. The only likely candidate in that case is the Russian satellite Express AM-5 which was launched on December 26th. This object seems to have been temporarily "lost" by JSpOC: as I write this (Jan 2),  Space-Track does not list orbital elements later than December 26th (when it was still in  a temporary transfer orbit).

For the moment, Mike McCants has given it the name UNK 131229 (with the acronym UNK meaning "Unknown").

This observing session also served to check on PAN (2009-047A). PAN is a highly mobile satellite and often moves position in May and December (I have written on the mystery of this satellite before). Not this time, it seems: it is still at the position it has been in for several months, forming a trio with the commercial satellites Yahsat 1B and Intelsat 10:

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Other classified objects imaged this night were the old SIGINT Mercury 1 (USA 105, "Advanced Vortex", 1994-054A), and the SIGINT Mentor 4 (USA 202, 2009-001A). Mercury 1 was placed at 48 E and recovered by me about a year ago.

click images to enlarge

During this observing session, I captured a bright irregular orange light moving across the sky: a 'Thai Lantern' ( a miniature hot-air balloon). They are the cause of many false fireball and re-entry reports. Here it is, moving through Orion while carried by the wind:

Two days earlier, on December 27, I also did my periodic check on Prowler (90-097E), using the 61-cm Cassegrain of Sierra Stars Observatory in Markleeville, California (MPC G68).

I concluded the evening of the 29th by making some shots of M31, the Andromeda Galaxy. Unfortunately, some thin haze came in after a while. The image below is a stack of 16 haze-free images of 30 seconds exposure each, with a CLS filter (against light pollution - the images were taken from Leiden town center)) and Zeiss 2.8/180mm lens piggyback on the mount of my C6:

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PAN has moved again [UPDATED]

On April 23 I wrote the following about PAN (2009-047A) and its frequent relocations in my post here:

"No doubt it will move again in the future, perhaps in May as December and May are frequently the months the satellite is moved"

I was very right with the "perhaps in May": PAN is on the move again!

Greg Roberts observing from South-Africa noted it missing at its old position on April 29. He recovered it on May 4th near the commercial geostationary Comsat Yamal 404. It is not (yet) clear whether that is its final position, or whether it is still drifting. Greg next initially thought he recovered it near the commercial comsat Yamal 404 on imagery from May 4th, but that turned out to be a mistake: as Mike McCants pointed out, the object in question was in reality the commercial geosat GSAT 8.

Ian Roberts, another South African observer, then located what likely indeed is PAN near Intelsat 12 on May 6th. Greg Roberts then managed to find it in his earlier images of May 4th as well, confirming Ian's observations.

Just goes to show that even the most secret of all satellites cannot escape the inquisitive eyes of a dedicated amateur.

PAN and Mentor 4 in March

Finally, an update on my observing activities in March. With apologies that it took so long.

In this post, early March observations of the classified geostationary satellites PAN and Mentor 4 will feature. In a second post following this one, I will report on some non-satellite observations: comet PANSTARRS and a fabulous display of Aurora borealis which I observed from Finland.


PAN and Mentor 4

As I noted on the blog before, weather has been extremely bad here since mid November 2012. Many nights were clouded, we had unusual amounts of snow, and spring set in very late (in fact, only last week).

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The few clear nights we had, usually coincided with a bright moon in the sky. As wintertime is a bad time for LEO objects at latitude 52N  (the visibility window is very short, restricted to twilight) the focus is on objects in GEO during this season: but that necessitates clear moonless nights....

On the evening of March 4 I did an attempt, which was cut short when clouds and haze moved in. The pictures came out bad, but I did manage to image PAN (2009-047A) and Mentor 4 (2009-001A), as can be seen in the picture above. Mentor 4 is a SIGINT: PAN probably is too.

PAN was moved again in December-January, this time taking up position at 42.5 E close to the commercial telecom sat Nigcomsat 1R.

Since its launch in 2009, this enigmatic satellite has frequently moved, and this is unusual. PAN was stationed at 33.0 E from late 2009 to May 2010 and then was moved to 38.0 E. It was moved again to 49.0 E in December 2010, followed by a move to 44.9 E in the spring of 2011. Then it was relocated to 39.1 E in the summer of 2011 and next moved to 52.5 E somewhere between late October 2011 and January 2012. In May 2012 it was moved back to 38.0 E. In December 2012, it moved to 42.5 E. No doubt it will move again in the future, perhaps in May as December and May are frequently the months the satellite is moved.

Note: the listed positions for PAN are based on privately archived TLE's for the satellite. The TLE source is Mike McCants and the TLE's are based on amateur observations of the satellite, notably by Greg Roberts (S-Africa), Peter Wakelin (UK), Ian Roberts (s-Africa) and me (Netherlands).

2012 in summary

It is time for a summary of the observations conducted in 2012.

I have been less active in 2012 than in previous years, logging about half the number of observational nights and obtained positions. The number of classified objects tracked however was somewhat higher.

Number of observing nights: 44
Number of obtained positions:  555
Number of classified objects tracked: 50

These data compared to previous years:

 (click diagram to enlarge)

As in previous years, springtime saw most observational activity:

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The following tables give a summary of the objects observed (with the "obs" column refering to the number of positions obtained on the object):

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Just for fun, I plotted all obtained positions on an RA/DEC map:

 (click diagram to enlarge)

So, what went on and what was special in 2012?

I continued my coverage of PAN and other geostationary satellites (well visible near declination -7.4 in the diagram above). On May 16, an unknown object in GTO (Unknown 120516) was briefly detected. In November, I found an unidentified geosynchronous object at 48 E that turned out to be the relocated object Mercury 1.

In February, a week after the lauch of the Iranian satellite Navid, I managed to photograph it in orbit.

In the last days of March, I filmed and photographed ESA's cargoship ATV-3 several times. This included vudeo and photographs less than 20 minutes after launch, when it made a deep twilight pass over Leiden. I photographed it again in September, after the ATV decoupled from the ISS again. Both times, my video and photography was featured on ESA's website.

2012 was the year of Dutch astronaut André Kuipers' 6-month stay at the ISS. I attended a live in-flight video contact at ESA/ESTEC Noordwijk on May 29. Earlier, on March 16, I listened in live to a radio contact between Kuipers (onboard ISS) and a Dutch school class with my radio receiver.

Live radio receptions were also obtained during the flight of Soyuz TMA-04M on May 16.

Mid-2012, the Japanese spy satellite IGS 1B performed an uncontrolled reentry, and over the spring and early summer I closely followed its demise, which finally took place on July 26, when I was on hollidays in Italy.

Among the new launches tracked was NROL-36, the new NOSS 3-6 duo (see here and here) launched in September. NROL-15 (a new Mentor, Mentor 5) was also tracked

October was very sad, as it saw the death of our cat, Pippi, on October 30. As related in the link, Pippi was a frequent companion during my observing sessions.

November 2012 was special, as I received the 2012 Dr J. van der Bilt Prize of the Royal Dutch Astronomical Association (KNVWS) on November 10 (see photographs here and video here).

December saw some unusual visitors to this weblog, connected to North Korea's first successful satellite launch.

I also did a number of interviews this year.

2012 was also a good asteroid year too. I discovered 3 new asteroids: 2012 SM58 in September using the 0.61-m telescope of Sierra Stars Observatory and a number of objects with Krisztián Sárneczky in the Piszkéstető (Konkoly) survey.

PAN, other Geostationary satellites, and another UNID (this time Greg's)

As reported earlier I had a prolific observing session on Geostationary satellites in the evening of November 18th, discovering amongst others an unidentified geostationary object now temporarily designated Unknown 121118 (see here and follow-up here with imagery by Greg from S-Africa: an more on it near the end of the current post).

Below is some more imagery showing various classified and unclassified objects. All images were made using a Canon EOS 60D with a SamYang 1.4/85mm lens at ISO 1000.


Unknown 20121117 (Greg's UNID)

The November 18th imagery includes imagery of a second unidentified object, Unknown 121117 discovered by Greg Roberts (CoSaTrak) from South Africa a day earlier on the 17th (a third initially reported  'unid 'by Greg turned out to be identifiable as a known object, a Chinese CZ-3C r/b). So Greg recovered my Nov 18th UNID on the 19th, and I recovered Greg's Nov 17 UNID on the 18th: nice teamwork!

The image below shows it together with a number of nearby commercial geosats (the veil-like lighter streaks in the image are cirrus clouds, who had begone to invade an initially clear sky):

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Below is one of Greg's images of the object from 17 November taken from S-Africa: in my image above taken a day later the object has drifted quite a distance more to the West.

(image courtesy Greg Roberts, CoSatTrak S-Africa)

Unknown 121117 is a truely uncatalogued object. There is nevertheless some idea about the identity of this satellite, but I am currently not allowed to provide more information.



PAN

PAN (09-047A) and the nearby commercial geosat Paksat 1R visible in Greg's Nov 17th image are visible on my Nov 18th imagery as well. The image below basically fits to the upper image above (see the Eutelsat pair visible in both images), giving you a sense how Greg's Unknown 2012117 has moved in a day time:

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I have written about PAN on this blog several times before: it is an enigmatic classified satellite that frequently relocates.


Mentor 4, Thuraya 2 and the Mentor 1r

Among the other objects imaged were the SIGINT Mentor 4 (and the nearby commercial satellite Thuraya 2), and a r/b from the Mentor 1 launch, Mentor 1r.

Mentors (the biggest geostationary satellites in existence and the biggest man-made objects in space with exception of the ISS) are relatively bright objects (typically mag. +8):

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I already posted imagery of another Mentor, Mentor 5, as well as the SIGINT Vortex 6 in an earlier post.


More on my UNID, Unknown 121118

This object in an 8.5 degree inclined geosynchronous orbit (see here and here for earlier coverage) remains 'unidentified' (i.e., is not present in public orbital catalogues such as USSTRATCOM's): we are however starting to believe it could be a classified object that has recently been moved to this location from somewhere else. It is currently positioned over 48.3 E and appears stable in longitude:

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More on the 21 September 2012 fireball: why it definitely was a meteor

I should have done this analysis earlier but did not have the time available until now. What follows now is a quick and back-of-the-envelope kind of calculation, but in my (not so) humble opinion it is adequate to the question at hand.

It concerns, of course, the splendid slow fireball seen widely over NW Europe near 21:55 UT on 21 September 2012. I posted on it before, focussing on saying "no" to the suggestion that this could have concerned a satellite reentry. In the post that now follows, I further strengthen the conclusion that it was not a satellite reentry, but a genuine meteoric fireball.

The map above gives a quick (and not particularly accurate) back-of-the-envelope reconstruction of the fireball trajectory. It is based on trajectory descriptions from Bussloo in the Netherlands and Dublin in Ireland: by taking reported altitudes (with respect to stars) and general directions of reported start and endpoints, and an assumed altitude of 50 km, the trajectory above is what approximately results. (update 19:10 UT, 24 Sep: an updated version of the map is at the bottom of this post).

The resulting trajectory is some 1000-1200 km long. In what now follows, I have taken 1100 km as the distance travelled by this fireball.

Observers near the western and eastern ends of the trajectory would probably not see the complete trajectory. Observers approximately mid-way, in mid-Britain, would potentially see most if not all of the trajectory (from experience I know you can see bright fireballs from distances of 500 km).

Observers report durations between 20-60 seconds: most video's on the web suggest a 40+ seconds duration.

It would take a reentering satellite travelling at 8 km/s (the orbital speed at decay altitudes) about 138 seconds or roughly 2.25 minutes to travel this distance. While the reported fireball durations are long, none of the reports nor videos comes even remotely close to that value.

A meteoric fireball travelling at the lowest speed possible for such an object, 11.8 km/s, would take 93 seconds to travel that distance. This is still longer than almost all of the reports suggest, but clearly getting closer.

If we take an estimated duration of 60 seconds, the 1100 km trajectory length results in a speed of  approximately 18 km/s.

18 km/s is a very reasonable speed for a slow, asteroidal origin fireball.

(it is, let me repeat, also way too fast for a satellite reentry).

Meteorite dropping fireballs typically have speeds between 11.8 and 27 km/s. A speed near 18 km/s sits squarely in the middle of that speed interval.

(update: diagram added 14:45 UT, 24 Sep)

(click diagram to enlarge)

The 60 seconds probably represents the upper boundary value for the duration of the fireball. If we take a shorter duration of 40 seconds, the speed already increases to 27.5 km/s.

This quick back-of-the-envelope reconstruction therefore shows that this must have been a meteoric fireball, quite likely of asteroidal origin, and we definitely can exclude a satellite reentry.

The fragmentation described and filmed is not unusual for meteorite dropping fireballs (see the video's of the Peekskill meteorite fall in my previous post). The object probably entered the atmosphere under a very shallow angle, which together with the slow speed explains the unusually long duration of the event.

Meteors of this kind are rare, but they have been seen before. Think of the Peekskill meteorite fall, but also the famous 1972 daylight fireball over the Grand Tetons (that had a duration of over 100 seconds) and the Cyrilid Meteor Procession from 1913 (that lasted minutes).

Note: a previous post gives a number of other lines of evidence which likewise suggest this fireball was not man-made space debris.

UPDATE: a further update is given in a new post: a very cautious orbital solution suggests an Aten orbit.

Note 2: on how I made this quick and (emphasis) rough trajectory reconstruction. I took observations that contain clear sky locations: e.g. a sighting from Dublin stating it went "through the pan of the Big Dipper"; the description from Bussloo observatory in the Netherlands; and later adding a.o. a photo from Halifax, UK, showing it just above the tail of Ursa Major. These descriptions can be turned into directions and elevations. Next, I drew lines from these sighting points towards the indicated directions, marking distances roughly corresponding to 30, 50 and 80 km altitude as indicated by the observed elevation [ distance = altitude / tan(elevation) ]. Near the start of the trajectory I marked 50 and 80 km, for Britain and Ireland I marked 30 and 50 km. These points then provide you with a rough trajectory.
From Dublin the object passed through North towards west. From Bussloo the object started NE (azimuth 60 degrees): these are important points of information too as it shows that the object started at least as far east as the Dutch-German border (and more likely over Sleswig-Holstein in N-Germany) and had its endpoint at least as far west as the northern part of Ireland.

Above: Updated map version, 24 Sep 19:10 GMT , also showing the principle of how it was reconstructed for three sighting locations. With thanks to Ramon van der Hilst for providing more detailed information on sky trajectory as seen from Bussloo (NL) on request.

30 (mostly) geostationary objects in one image

Click image to enlarge

The image above was made by me just after midnight of June 18-19, 2012. It is a single image taken with my new Canon EOS 60D and a SamYang 1.4/85mm lens (800 ISO, 10s exposure). It was shot from the center of Leiden town.

The image shows a 11 x 14 degrees wide field low in the south-southeastern sky, between 20 and 30 degrees elevation above the horizon. Diagonally over the image runs a part of the geostationary belt, at declination -7.4 deg for my location.

In this single image, as much as 30 mostly geostationary satellites are visible: 23 commercial geostationary satellites, 1 classified military geostationary satellite (Milstar 5, 2002-001A), and 6 rocket boosters.

I did a poor job with the focus of this image, resulting in a slight unsharpness (especially near the edges of the image). Yet, the number of  objects nevertheless visible in this small piece of low southern sky is amazing!

This is just one of several images I took that night. Apart from Milstar 5, a number of other classified (military) geostationary satellites were imaged and astrometry on them obtained.



PAN in it's new position at 37.9 E

One of these objects is PAN (2009-047A), an enigmatic satellite I have written about before. Here is an image from June 18-19:

click image to enlarge

One of the curious aspects of this strange classified geostationary satellite operated by an undisclosed agency (see Dwayne Day's article in The Space Review), is that it is very frequently repositioned. It recently did so again (see my imagery of May 16, when it was still on the move). It has now stopped drifting and taken up position at 37.9 deg E (a position it has occupied before) not far from Paksat 1R, as can be seen in the image above. A stray Atlas Centaur rocket booster passed the area as well when the image was taken.


Vortex 4 and Mercury 2

Other classified objects imaged include  the older geostationary satellites Vortex 4 (1984-009A) and Mercury 2 (96-026A), the latter of which currently also is on the move (it is probably being sent to a disposal orbit after reaching the end of its operational mission):

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Vortex 4  (launched on 31 January 1984) and Mercury 2 (USA 118, launched on 24 April 1996) both are SIGINT (eaves-dropping) satellites, with the Mercury being a further advanced version of the Vortex.

In addition, a newer SIGINT satellite was imaged as well,  Mentor 4 (2009-001A, one that frequently features in this observational blog, as it is bright and easy to observe), and the object designated by our amateur network as  UNK 060616 (probably an old r/b).


Prowler, AEHF 1 and DSP F15 imaged from Winer observatory, USA

While the above imaging was all done from my home in the Netherlands, I also imaged a few objects 'remotely' using the UoI Rigel (MPC 857) 37-cm Cassegrain telescope at Winer Observatory, Sonoita, Arizona, USA.

The enigmatic Prowler (1990-097E), a clandestine launch from Space Shuttle mission STS-38 which has featured on this blog more often (read the intriguing story of Prowler here; plenty of suspense!) was imaged on June 19 and 22. On June 19 I also imaged the military communications satellite AEHF 1 (2010-039A), and on June 22 the old DSP Infra-red early-warning satellite DSP F15 (1990-095A). Images of these objects below:

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Comet 185P/Petriew

In addition to all these satellites, two  Solar System Minor Bodies were imaged: 2012 LZ1 and 185P/Petriew.

I posted imagery of the June 15 fly-by of Near Earth Asteroid (NEA) 2012 LZ1 here before in my previous post, and obtained more astrometry on this object on subsequent nights. In addition, I obtained some imagery on the faint periodic comet 185P/ Petriew on June 22. Below is a stack of 5 images of 45s exposure each:

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Not a pretty picture, but the comet was near magnitude +17 to +18! My astrometry has been included in MPEC 2012-M33 (22 June).


New camera: a Canon EOS 60D

I had completely forgotten to mention this: during the second half of May, my EOS 450D camera broke down. During a macro-session on Dragonflies, the shutter broke. Much to my regret.

I had the choice between having the shutter repaired (expensive), or buying a new camera. I choose the latter option, as the new generation of EOS cameras performs notably better than the 450D, especially in performance at high ISO (less noise). So I decided to upgrade.

The choice I made was for the Canon EOS 60D, an 18 MP DSLR with Digic IV processor. So far (and having mostly used it for "normal" photography for now) I very much like it!

Before I can use it on satellites in Low Earth Orbit, I'll first have to complete a calibration program with the camera. This calibration entails the delay between the moment you press the shutter button and the exposure is actually taken; and the real duration of exposures (a "10 second" exposure is not exactly 10.00 seconds). I have some preliminary calibration results by now, but it will take some time before I have final results and can start to use the camera regularly on satellites. For geostationary satellites (where the timing accuracy isn't that much of a factor; rather the astrometry is) the preliminary results I have mean I can already use it (as has been done, see this post).

PAN is on the move, and detection of an unknown object in near-GEO

Last Wednesday evening (16 May) saw very clear skies. Combined with the absence of moonlight, an ideal situation to target geostationary objects, which are low in the sky for me at 52 N. As they are low  and I am in an urban environment, I need a very transparent sky.

Normally I use the 2.8/180mm Zeiss Sonnar, but this time I went for the SamYang 1.4/85mm. The limiting magnitude of this fine lens is only slightly less than that of the 180mm, but the FOV is twice as large (10 x 14 degrees). It is a geostationary magnet: in one single image I counted 20 geostationary or near-geostationary objects! In total, the session (a sweep of some 25 degrees of equatorial sky in the S-SE, at elevations of 15 to 25 degrees) recorded 38 objects: 7 classifieds, 30 unclassifieds and one unknown.


An UNKNOWN object on May 16

As part of the session, an object in near-Geostationary space was serendipitously observed that cannot be matched to any known object (for recorded positions, see here). It was slowly moving near the commercial geosats Eutelsat 36A and Eutelsat 36B (00-028A and 09-065A) and was captured on several images, small parts of four of which are shown below (note the movement relative to the stable Eutelsats):

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As Heavensat with the latest orbital catalogues loaded showed nothing in this position I initially logged it as a 'UNID'. Then a check with Ted's IDSat software resulted in a very superficial match with the DSP F20 cover (00-024E), but a clearly non-linear delta T suggested this could be a spurious match (see the questionmark and note under my data report here).  Next Mike McCants contacted me, it was indeed a spurious match in his opinion as his analysis of my data suggested an approximate orbit that does not match the DSP F20 cover at all. So for now, the object is designated as UNKNOWN 120516.

Objects like this do not spontaneously materialize, and there is no recent launch that can account for this object. It is therefore likely an old object being relocated. According to Mike, one possible (but by far not certain) option is that it is the classified object Mercury 1 (94-054A, or USA 105), which has not been observed for some time, being retired and relocated to a graveyard orbit.

Unfortunately, both Greg Roberts in South Africa and me here in the Netherlands were clouded out last night and today, so follow-up using Mike's approximate search orbits is troublesome for the moment.


PAN being relocated again

Another classified geostationary object on the move again is the enigmatic PAN (09-047A). This object has an unusual history of frequent relocations, moving to and fro in longitude each few months. It was at 44.9 E in the spring of 2011, then relocated to 39.1 E in the summer of 2011 and next moved to 52.5 E somewhere between late October 2011 (I still observed it at 39.1E on 23 October 2011) and January 2012, when Greg Roberts noted it missing after which Ian Roberts recovered it at 52.5 E early February.

And now its is moving again: Greg Roberts was the first to note this on May 10 and recovered it on May 14 and May 16 while it was and is moving towards 39.1 E (a position it has previously occupied). I imaged it near 39.1 E too on Wednesday evening May 16. Below is a part of one of the images, showing PAN and several commercial geostationary objects, as well as two old rocket boosters in GTO:

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 Other classified (near-)  geostationary objects observed this evening were the SIGINT Vortex 6 (89-035A, also in the process of being relocated), the SIGINT Mentor 4 (09-001A), it's rocket (09-001B), the Milstar 5 communication satellite (02-001A), the DSCS 3-13 R2 rocket (03-008C) and the DSP early-warning satellite DSP F23 (07-054A).

Apart from these geostationary objects, I observed the LEO object USA 186 (05-042A, a KH-12 Keyhole) as well that evening, in its new orbit after it manoeuvered earlier this year.

FIA Radar 1 through the Pleiades, and Geostationary satellites in Orion

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The picture above (10s exposure taken with a Canon 450D and SamYang 1.4/85 mm lens) shows the classified military Radar reconnaissance satellite FIA Radar 1 (10-046A) sailing smack through the Pleiades last Friday.

Friday evening started clear, and I took the opportunity do so some observing. Using the SamYang 1.4/85 mm and the Carl Zeiss Jena Sonnar MC 2.8/180mm, I not only obtained the picture of FIA Radar 1 above, but I also targetted some geostationary satellites, imaging several of them in Orion.

Among the targets were the classified military communication satellite Milstar 5 (02-001A), the SDS data relay satellite USA 227 (11-011A) and the SIGINT satellite Mentor 2 (98-029A). Two other classified objects were captured as by-catch of these objects: the SIGINT satellite Vortex 6 (89-035A) and the object "Unknown 110623" (11-674A), an amateur-discovered object in GTO that is probably a spent rocket booster of a military launch. Note how it created a tiny trail in the image below as it was moving northwards through Orion.

The images below show these objects. Milstar 5, Vortex 6, UNK 110623 plus the two non-classified commercial communication satellites Eutelsat W2 (98-056A) and Intelsat New Dawn (11-016A) are all in the same 10-degree wide 85mm image. The stars of Orion's belt are visible in the top of the image, and Milstar 5 is close to the Orion Nebula. Orion's belt stars are visible at left in the Mentor 2 image as well.

click images to enlarge

 

In one of the other images taken last Friday evening, another commercial geostationary communication satellite, Intelsat 4 (95-040A) was captured while it briefly flared brightly at about 18:58:30 UTC (27 Jan).

The FIA radar and a number of geostationary objects (Mentor 2, Mentor 4) and the NOSS 3-3 r/b were imaged by me two weeks earlier as well, observations on January 14 and 15 which I had not reported here earlier. I also tried to relocate PAN, which recently has been relocated again but so far has not been recovered, although both Greg in South Africa and I in the Netherlands have tried.