USA 338, the NROL-91 payload, observed

NROL-91. Click image to enlarge

On 24 September 2022 at 22:25:30 UT, with half an hour delay, ULA launched NROL-91, a Delta IV Heavy with a classified payload for the NRO. The payload is probably an electro-optical reconnaissance satellite in the KH-11 lineage (for more backgrounds see the previous post).

Six hours after the launch, the payload, USA 338, made a pass over the Netherlands and around 4:17 UTC (6:17 local time) was observed by Cees Bassa from Dwingeloo and by me from Leiden. It was visible by the naked eye with a brightness around magnitude +2.5 to +3.

The image above shows it ascending over the roof of my house, passing close to the Hyades cluster in Taurus. The image was taken with a Canon EOS 80D + Samyang 1.4/35 mm lens, 5 seconds at ISO 800. The sky was clear but with sacttered clouds, as can be seen in the image.

A very preliminary orbit fit suggests a 73.59 degree inclined, 376 x 415 km orbit. The RAAN difference with USA 290, an earlier launch of similar type, is ~99 degrees. When the orbit gets better established, these figures might still change somewhat.

 

NROL-91: a new (possibly electro-optical) sister ship of USA 290

 

click map to enlarge

On 24 September 2022 at 21:53 UT, an ULA Atlas Delta IV Heavy (the last to be launched from Vandenberg) will launch from Vandenberg SFB Launch Complex 6 as NROL-91, carrying a classified payload into Low Earth Orbit for the NRO.

The launch is in southernly direction. The locations of the four hazard areas from the published Navigational Warnings (see map above and text below) are consistent with launch into an orbital inclination of 73.6 degrees, which is similar to NROL-71 from January 2019 that launched USA 290 (2019-004A). 

So the NROL-91 payload likely is a sister ship to USA 290.

Below is Navigational Warning HYDROPAC 2592/22 for the launch (note that there appears to be a clerical error in the first coordinate of area C):

122224Z SEP 22
HYDROPAC 2592/22(GEN).
EASTERN PACIFIC.
CALIFORNIA.
1. HAZARDOUS OPERATIONS:
   A. 242020Z TO 242347Z SEP, ALTERNATE
      2020Z TO 2347Z DAILY 25 THRU 27 SEP
      IN AREA BOUND BY
      33-53.00N 120-23.00W, 34-28.00N 120-40.00W,
      34-39.00N 120-40.00W, 34-39.00N 120-35.00W,
      34-27.00N 120-25.00W, 33-55.00N 120-18.00W.
   B. 242020Z TO 242345Z SEP, ALTERNATE
      2020Z TO 2345Z DAILY 25 THRU 27 SEP
      IN AREA BOUND BY
      25-18.00N 117-07.00W, 25-12.00N 117-27.00W,
      26-35.00N 117-53.00W, 26-41.00N 117-33.00W.
   C. 242020Z TO 242345Z SEP, ALTERNATE
      2020Z TO 2345Z DAILY 25 THRU 27 SEP
      IN AREA BOUND BY
      00-17.00S 121-28.00W, 00-07.00S 110-21.00W,
      03-24.00S 109-33.00W, 03-24.00S 110-21.00W.
   D. 242242Z TO 250133Z SEP, ALTERNATE
      2242Z TO 0133Z DAILY 25 THRU 27 SEP
      IN AREA BOUND BY
      17-57.00N 140-23.00W, 06-13.00N 137-52.00W,
      06-30.00N 136-25.00W, 18-15.00N 138-53.00W.
2. CANCEL THIS MSG 280233Z SEP 22.// 

A second Navigational Warning for this launch, NAVAREA XII 695/22, is identical.

The locations of the first three hazard areas A to C from the Navigational Warning are indeed very similar to those for NROL-71 in 2019: compare for example to this map for NROL-71 from this december 2018 post:

 

NROL-71 from January 2019. click to enlarge

Area D, the upper stage deorbit area, is situated slightly more south and is a bit more elongated than it was for NROL-71, for unclear reasons. The upper stage deorbit happens at the end of the first revolution. The deorbit burn might be visible from central Asia around 23:10-23:20 UTC.

In 2019, NROL-71 was launched into a 395 x 420 km, 73.6 degree inclined non-sun-synchronous orbit and I expect the orbit of the NROL-91 payload to be very similar.

Here is my pre-launch orbital estimate for the NROL-91 payload based on this assumption:

 

NROL-91                      for launch on 24 Sep 2022 at 21:53:00 UT
1 70001U 22999A   22267.91180556  .00000000  00000-0  00000-0 0    06
2 70001 073.6000 044.7175 0018421 155.1634 324.7303 15.53162541    00

 

If NROL-91 indeed launches at 21:53 UT on the 24th, the orbital planes of the payload and USA 290 will end up at a 90-degree angle to each other, as can be seen in the polar view below:

polar view of the orbital plane relative to that of USA 290. Click to enlarge

 

If the launch is scrubbed on the 24th, and if indeed this specific orbital plane at 90-degree angle to that of USA 290 is aimed for, the launch time will shift ~13 minutes earlier each day.

USA 290 at the time was widely believed to be a new generation electro-optical reconnaissance (IMINT) satellite, a follow-on on the KH-11 ENHANCED CRYSTAL program. That it was launched, as NROL-91 will be, in a non-sun-synchronous orbit is odd though, for an optical reconnaissance satellite. 

One really wonders why the sun-synchronous polar orbit typical for such missions (and typical for earlier generation KH-11 EVOLVED ADVANCED CRYSTAL missions) was dropped in favour of this new 73.6 degree orbital plane. What is the advantage of this new orbital configuration? Or are USA 290 and NROL-91 perhaps not electro-optical systems, but something else?

USA 224 has manoeuvered

During the night of June 12-13, I was doing a periodic checkup on the KH-11 Advanced Enhanced CRYSTAL satellites  USA 224 (2011-002A) and USA 314 (2021-032A) that occupy the KH-11 primary East plane. This because I expect USA 224 to manoeuvre to the secondary East plane at some point this summer, now USA 314 has recently been launched into its orbital plane as a replacement (see discussion in my earlier blogpost here).

USA 224 did not appear at the nominal time on June 13 but some 2m 20s late, indicating a manoeuvre.

Observations by David Brierley and me on June 12/13 and 13/14 have established this preliminary post-manoeuvre orbit:

USA 224                                                  255 x 998 km
1 37348U 11002A   21165.00715133 0.00014912  00000-0  12302-3 0    05
2 37348  97.8892 276.6083 0530502 157.6427 204.8870 14.81006602    06

It is clear that this is not the big plane-changing manoeuver expected, but a small regular orbit upkeeping manoeuvre: apogee was raised by some 10 km. 

From the pre- and post-manoeuvre orbit,  I calculate that the manoeuvre took place on Thursday June 10 near 14:14 UT, over the Atlantic, during crossing through the descending node and perigee. 

As usual, the manoeuvre happened while perigee was situated over the equator (when the Mean Anomaly is near 180 degrees, this is always a moment to watch out for manoeuvres). This allows to make adjustments in both orbital altitude and inclination in the same burn, with a minimum expense of fuel.

USA 314 (NROL-82) imaged

 

click to enlarge

Last Monday 26 April at 20:47:00 UT, ULA launched a classified payload for the NRO under the launch designation NROL-82. The payload is now designated USA 314. I wrote about the launch and that it is almost certainly an ADVANCED ENHANCED CRYSTAL KH-11 electro-optical reconnaissance satellite in an earlier post.

The payload was picked up on the first orbit by radio observer Scott Tilley in Canada, and next, guided by the radio observations, Cees Bassa (who is just like me in the Netherlands) optically imaged it on the second and third orbit.

Thanks to information from the radio observations, #NROL82 was caught in video observations on its second pass. It passed close to Polaris in the top left of this image at 23:45:30UTC. pic.twitter.com/HB8bSFy84e

— Cees Bassa (@cgbassa) April 27, 2021

 

I tried to image it from Leiden on the second orbit as well, but as it turns out it passed outside my camera field during that pass.

The next night, and with a more firm search orbit based on the data from the previous night available, I did succesfully image it. The photograph in top of this post was made with a Canon EOS 80D camera and Samyang 1.4/85 mm lens (at F2.0, 1600 ISO, 1 second exposure). 

I also obtained video, using the WATEC 902H2 Supreme with a 1.8/50 mm lens:

The payload is designated USA 314 (catalogue nr 48247, COSPAR 2021-032A) and as usual CSpOC does not publish orbital data. But our observations show that it is in a 528 x 755 km, 98.1 degree inclined sun-synchonous orbit.

The orbital plane is even closer to that of USA 224 than anticipated: a difference of only 1.1 degree in RAAN and 0.2 degrees in orbital inclination. The orbital altitude is somewhat different and the orbital eccentricity is less than our initial guess. Perhaps it will manoeuvre over the coming days/weeks to the same altitudes as USA 224, perhaps it will not: we will see!

So in all, the NROL-82 payload's orbit is pretty much what was expected, apart from a slightly different initial orbital altitude.

USA 224 and the new payload USA 314 currently move almost in phase, and as a result they are relatively close, with continuous sight of each other. It is well possible that USA 224 is imaging the new payload as a post-launch health checkup.

The image below shows the coplanar character of the USA 224 and USA 314 orbits, and the spatial proximity in viewing distance of each other:

click to enlarge

As I pointed out in a previous post, based on historical patterns I expect that, after a checkout-phase that may take a couple of weeks, the new USA 314 will take over from USA 224 in the KH-11 primary East orbital plane. USA 224 will then likely be manoeuvered into a lower orbit (~400 km) and its orbital plane will be moved to the 'secondary' East plane, some 10-20 degrees east in RAAN of the current orbital plane.

NROL-82: an upcoming new KH-11 EVOLVED ENHANCED CRYSTAL launch [UPDATED]

image: ULA

(updated 27 Apr 2021 with first observational orbit, see end of post)

If the weather and the launch Gods cooperate, ULA will launch a Delta IV Heavy with a classified payload for the NRO on 26 April 2021. The launch is designated NROL-82 and the payload will likely receive the designation USA 314. In a tweet from April 19, ULA mentions a prospective launch time of 20:46 UT.

Several lines of evidence lead us to believe that the payload is a KH-11 EVOLVED ENHANCED CRYSTAL optical reconnaissance satellite, colloquially also known as a 'Keyhole'. It is the kind of satellite that makes these kind of detailed pictures of areas of interest for the NRO.

A map in the ULA Mission Overview for this launch, and the Navigational Warnings issued for this launch (NAVAREA XII 173/21 and HYDROPAC 1221/21) provide information on the launch azimuth and from that the orbital inclination targetted. Likewise the position and time window of the upper stage deorbit area provides - in a very broad sense- information on the orbital altitude aimed for. Together they indicate a launch into a sun-synchronous Low Earth Orbit with an orbital inclination near 98 degrees. This is a very familiar orbit, as we will discuss later in this post.

Below is a map I prepared depicting the hazard areas from these Navigational Warnings as well as the launch trajectory I calculate based on this information:

click map to enlarge

The listed times along the track are for launch at 20:46 UT into the 250 x 1020 km, 97.9 degrees inclined estimated orbit below:

 NROL-82 (USA 314)          for launch on 26 April 2021 at 20:46:00 UT
1 70002U 21999A   21116.86527778  .00000000  00000-0  00000-0 0    03
2 70002 097.8600 222.0898 0548970 157.1680 337.2110 14.78203944    02

 

The text of the Navigational Warnings:

220434Z APR 21
NAVAREA XII 173/21 (also: HYDROPAC 1221/21)
EASTERN NORTH PACIFIC.
EASTERN SOUTH PACIFIC.
CALIFORNIA.
1. HAZARDOUS OPERATIONS:
   A. 2016Z TO 2257Z DAILY 26 THRU 28 APR
      IN AREA BOUND BY
      34-38N 120-40W, 34-36N 120-30W,
      34-07N 120-39W, 34-08N 120-44W.
   B. 2016Z TO 2257Z DAILY 26 THRU 28 APR
      IN AREA BOUND BY
      22-57N 120-46W, 23-47N 125-18W,
      26-27N 124-45W, 25-36N 120-08W.
   C. 2016Z TO 2257Z DAILY 26 THRU 28 APR
      IN AREA BOUND BY
      13-28S 121-20W, 10-47S 138-34W,
      00-47S 136-41W, 03-52S 119-54W.
   D. 2253Z TO 0029Z COMMENCING DAILY
      26 THRU 29 APR IN AREA BOUND BY
      63-14S 174-16W, 32-49S 159-58W,
      33-23S 156-28W, 64-16S 168-07W.
2. CANCEL THIS MSG 300129Z APR 21.

 

Area D from the Navigational Warnings, located in the southern Pacific Ocean, appears to be the deorbit area for the Delta Cryogenic Second Stage (DCSS). The DCSS deorbit takes place some two hours after launch, just after the start of the second revolution (with the deorbit burn happening over the Arctic, near the end of the first revolution).

As mentioned above, the orbit that seems to be targetted is one that is very familiar in terms of orbital inclination and sun-synchronous character. It is the typical orbit of a KH-11 EVOLVED ENHANCED CRYSTAL electro-optical reconnaissance satellite. Several years ago I discussed the KH-11 orbital constellation in depth on this blog ("Past and future of the KH-11 Keyhole/Evolved Enhanced CRYSTAL constellation" - 2013). As a side note, the type of rocket used to launch NROL-82 is consistent with a KH-11 launch too: the Delta IV Heavy has a long history of launching KH-11's.

Currently there are at least three, and possibly four active KH-11 satellites on orbit: USA 186 (2005-042A), USA 224 (2011-002A), USA 245 (2013-043A), and possibly USA 290 (2019-004A).  The latter, USA 290, is in an odd orbit for a KH-11 and its identification as a KH-11 is open to questioning (I will discuss this later in this blog post).

Historically (see "Past and future of the KH-11 Keyhole/Evolved Enhanced CRYSTAL constellation"), new KH-11 satellites are launched into one of two primary orbital planes some 48 degrees apart in RAAN: a "primary East" plane and a "primary West" plane. The time window and the 20:46 UT launch time given by ULA for the upcoming April 26 launch corresponds well with targetting the "primary East" plane. This orbital plane results in passes around local noon and midnight. The KH-11 satellite currently occupying this orbital plane is USA 224 launched 10 years ago in 2011.

 

USA 224 imaged in June 2014. click image to enlarge

KH-11 constellation (minus USA 290), situation mid-April 2021 (polar view). Click to enlarge

 

The orbital plane of USA 224 passes over the launch site of NROL-82, Space Launch Complex 6 (SLC-6) at Vandenberg Air Force Base, around 21:20 UT on April 26. This is a difference of some 35 minutes with the launch time (20:46 UT) from the ULA tweet.

In 2011, when USA 224 itself was launched to replace USA 161 in the primary East plane, the launch occurred some 20 minutes before the USA 161 orbital plane crossed over the launch site (a similar time difference would hence see launch around 21:00 UT for the upcoming April 26 launch).

If history is our guide, the following sequence of event will likely happen. To start with, NROL-82 will be launched into the KH-11 Primary East plane, with an orbital inclination of ~97.9 degrees and orbital altitude of ~250 x 1020 km, almost co-planar with USA 224. The illustration below shows the orbital plane situation around orbit insertion. Note the similarity of the orbital planes of NROL-82 and USA 224:

 

expected situation just after launch of NROL-82. click to enlarge

 

After a check-out period of a few weeks, the NROL-82 payload (likely designated USA 314) will take over the primary plane mission from USA 224, the satellite previously occupying this orbital plane. 

Next, after USA 314 has taken over its role, USA 224 will be moved away from the primary plane, into a new orbital plane with RAAN some 10-20 degrees East of the primary plane: the so called '"secondary East plane". It will also lower its apogee and take up a ~400 km altitude orbit. In this new orbit it will continue to be operational for several years, entering its extended mission phase. 

From this moment on, for the first time since the deorbit of USA 161 in the winter of 2014-2015, all the two primary planes and all the two secondary planes will be occupied by a KH-11 again. The orbital constellation will become something like that in the image below:

Approximate KH-11 constellation after expected rearrangement later this year. Click to enlarge

 

How about USA 290?

You will have noted that after a brief initial mention, I carefully left USA 290, launched in 2019, out of the discussion so far. So what about that object? Is it a KH-11?

USA 290 (2019-004A) was launched as NROL-71 from Vandenberg on a Delta IV Heavy on 19 January 2019 (see an earlier blogpost) and it was suspected by some noted analysts to be a KH-11. It however went into a weird, 73.6 degree inclined ~400 km altitude orbit that is not sun-synchronous and nothing like previous KH-11 orbits. So, had the NRO broken with the previous 'classic' pattern of the KH-11 orbital constellation and were they trying something new?

The identification of  USA 290 as a KH-11 never has been sitting well with me. The odd orbital inclination and non sun-synchronous character of the orbit gives few reasons to think it is an IMINT mission.

In light of the apparent return to the known 'classic' KH-11 constellation with the upcoming launch of NROL-82, I have again started to foster these doubts. Maybe USA 290 isn't a KH-11 after all but something else, something experimental (readers of this blog will have noted that the past 4-5 years, a lot of NRO launches appear to be experimental, going into 'new' previously unseen types of orbit. Some of these are, I suspect, radar imaging satellites).

Ted Molczan has recently suggested that USA 290 is a KH-11, and that its odd orbit is inspired by that of the notorious 'Misty' stealth IMINT satellites of the 1990-ies which were launched in ~65 degree orbits. Basically, he argues that USA 290 is a 'Misty' imaging satellite without the stealth!

I remain agnostic at best about the identity of USA 290. Perhaps, if new payloads are launched into similar orbits over the coming years, the picture will become more clear. For now, I regard USA 290 as an oddity, and not necessarily a KH-11.

UPDATE 27 Apr 2021 11:00 UT

Cees Bassa optically observed the NROL-82 payload on the 2nd and 3rd revolution. Radio observers including Scott Tilley are also tracking it.

Based on a hybrid optical/radio orbit computed by Scott Tilley, the orbital altitude is somewhat different than expected, the orbit less eccentric: but the orbital plane is even closer to that of USA 224.

The orbital plane is very close to that of USA 224 indeed: a ~1 degree difference in RAAN and 0.1 degree difference in orbital inclination.

Orbital altitude currently appears to be about 525 x 760 km, i.e. less eccentric than our initila pre-launch estimate. That of USA 224 is 256 x 997 km.

The NROL-82 payload might manoeuvre in the coming days and weeks in order to have it's apogee and perigee altitudes match with  that of USA 224.

click to enlarge

Image from Trump tweet identified as imagery by USA 224, a classified KH-11 ENHANCED CRYSTAL satellite

click to enlarge. image: US Government

The incredibly detailed image above was leaked declassified and revealed to the world by US President Donald Trump, very characteristically in a tweet, on 30 August 2019.

It shows the aftermath of the failed Iranian Safir launch of August 28/29, with considerable damage to the platform and vehicles. Obviously, there was an explosion or crash of some sort, likely an explosion of an engine or rocket stage or failed lift-off.

The image is a photograph of a printed photograph: you can see the reflection of the camera flash on the photographic print near the center of the image and the silhouet of the person photographing it. There is also some image distortion, likely because the print was curling somewhat at the edges. But the level of detail is amazing (and the original might have been even more detailed).

That level of detail quickly led to speculation: what platform took this image? A drone? A high altitude reconnaissance aircraft? A satellite?

Some initially argued that the level of detail was too high for a satellite. But as we will see in this post, it was made by a satellite, and we can even say which satellite.

The level of detail in the image is incredible and points to one of the NRO's classified KH-11 EVOLVED ENHANCED CRYSTAL electro-optical reconnaissance satellites (they are also known as ADVANCED CRYSTAL, KENNEN, and colloquially as 'KeyHole').

These are high resolution optical satellites that resemble the Hubble Space Telescope, but look down to Earth instead of to the heavens. It is known that the optics of these satellites are 2.4-meter diameter mirrors. Theoretically, from the perigee of their orbits this would yield a resolution of just under 10 cm.

Christiaan Triebert analysed the shadow directions on the image and placed the time of the image between 9 and 10 UT (August 29), or 13:30-14:30 local Iranian time. Michael Thompson pointed out on Twitter that one of the KH-11 satellites, USA 224 (2011-002A), made a pass over the launch site in that time window.

This satellite is a classified satellite, but we do know its orbit because amateur trackers track this object regularly. This is USA 224 passing over my hometown Leiden in June 2014 for example:

USA 224 passing over Leiden, 21 June 2014

This blogpost consolidates two analysis which I initially published through Twitter. I will show in this analysis that there is very little doubt that USA 224 took this image.

Matching view angles 

The map below shows how USA 224 passed almost right over the launch site at 9:43:47 UT on August 29, with a maximum elevation of 87.7 degrees. The photograph tweeted by President Trump was taken post culmination, from the location indicated by the white cross in the map above. That position is based on the analysis that now follows.

click map to enlarge

The depicted trajectory for USA 224 is based on amateur tracking data. I used elset 19239.00965638 which was ~2.5 days old at the time of the overflight. In the absence of a manoeuvre, it should be accurate to a few seconds in time along-track and very little error cross-track.

USA 224
1 37348U 11002A   19239.00965638 0.00010600  00000-0  95384-4 0    03
2 37348  97.9000 349.1166 0536016 134.6567 225.3431 14.78336728    04

The imaged launch site itself is located at 35.2346 N, 53.9210 E, altitude 936 m, and indicated by the blue dot in the map. The launch platform is part of Iran's Imam Khomeini Space Port, near Semnan.

click to enlarge. Image: US Government

Trump's image shows the platform viewed under an oblique angle, looking in a northern direction (i.e. with the satellite to the south of the site). As the launch platform is circular, we can use the ellipticity of the platform on the image to estimate the angle under which the platform was imaged. For this, we have to measure the semi-minor and semi-major axis of the ellipse (denoted Y and R in the diagram below): their ratio corresponds to the sinus of the viewing angle.

The result of this measurement is a nominal view angle of 46.03 degrees. For USA 224, this elevation with respect to the imaged site was reached at 09:44:20.7 UT (nominally), post-culmination when the satellite was to the south of the site. From the satellite ephemeris, the satellite was at an azimuth of 194.85 degrees as seen from the imaged site at that moment. The satellite's geographical position was near 33.005 N,  53.220 E at an altitude of  283 km. The range to the imaged site was 385 km.

I used these values as input in STK and simulated the view of the damaged launch platform as seen from USA 224 for 29 August 09:44:20.7 UT. The images below compare the original image from President Trump's tweet (top) and the simulated view from USA 224 (bottom):

click to enlarge

Ignoring the shadow directions, the simulated view is very similar to the actual image, pointing out that indeed the image very likely was taken by the USA 224 satellite.

(the simulated view uses an overhead commercial satellite image taken at another time, rendered to mimic an oblique view, hence the different shadow directions).

Cees Bassa, in an independent analysis, has calculated very similar figures for the viewing angle and from that azimuth and elevation.

Matching times

In a second analysis, I tried to improve on the time of the image derived from the shadow directions.

When projecting a line through the shadow of one of the masts at the edge of the platform, this line passes almost through the middle of the access road at top right in the image:

click to enlarge

I used this observation to measure the direction of the shadow in Google Earth. It corresponds to an approximate azimuth of 40.45 degrees, which would place the sun at an azimuth of about 220.45 degrees (+- 1 degree error or so):

click to enlarge

Looking this direction up in the solar ephemerids for the imaged site (calculated with MICA), this solar azimuth corresponds to 09:46:25 UT (Aug 29). This is only 2 minutes later than the time for which the image best matches the USA 224 view of the site, as reconstructed earlier in this post.

This again confirms that this image could very well have been taken by USA 224. Both the time matches, and the view matches.

With the uncertainties in the shadow direction measurement taken into account (including uncertainties introduced by possible image deformations), within error margins the two times match. The difference between the measured (~220.45) solar azimuth and the solar azimuth calculated for 09:44:21 UT is 0.85 degrees, i.e. under a degree and hence small.

The 09:44:21 UT  derived from matching the satellite view to the image, probably is more accurate than the time derived from the shadow analysis. This time is probably accurate to a few seconds, given that the satellite TLE used was 2.5 days old.

Why?!

And then the baffling question: why did President Trump tweet an image that otherwise would be considered highly classified?

The KH-11 satellites are classified, and so is imagery from these satellites. If an adversary gets her hands on KH-11 imagery, it reveals information about the optical capacities of these space assets.

In 1984, a Navy intelligence analyst was sent to prison for leaking three KH-11 images to the press.

Reconnaissance satellite imagery made public by the US Government itself over the past decades were either from commercial DigitalGlobe satellites, or purposely degraded in quality such as not to reveal the optical capacities of the KH-11. But now we see a US President tweet, on what appears to be a whim for the purpose of gloating, a very detailed image that as was shown in this post definitely was taken by a KH-11 satellite.

The occassion at which this happened, is eyebrow raising. A failed space launch hardly is a matter of great geopolitical concern. It is something trivial compared to e.g. imagery showing preparations for an invasion, the production of WMD, or atrocities against humanity. The latter could perhaps be argued to be a valid reason to publish imagery that also divulges the capacities of your best space-based imaging platforms: this occasion was not.

Which makes this a rather momentous occasion.

(note: there is a black block in the upper left of the image that seems to be placed there to redact some information that might have been printed there. I think it is likely this information was the time of image, space platform ID and the location of the latter. It points out that some deliberate thought was given to the release of this image, before it was tweeted).

USA 224 passing through Corona Borealis, 17 June 2014

Edit (2 Sep 2019):

In the comments, Russ Calvert makes a very valid point: the phone camera used to photograph the photographic print might also introduce some slant. But I suspect the error introduced this way is small as normally you would try as best as you can to hold the camera perpendicular to the paper you are photographing. A clear slant angle of the camera also would introduce a sharpness gradient that does not seem to be there. The good match between the image and the simulated view from the satellite also bears out that error introduced in this way is likely small.

Edit II (2 Sep 2019): 

Added two archive images of USA 224 passing through the night sky over my hometown Leiden.

Edit III (24 Sep 2019)

Between the infamous 1984 leak by Samuel Moring Lorrison and Trumps 2019 tweet, there was one other occasion that (parts of a) full resolution KH-11 imagery became public. That was an image from the Snowden files published in September 2016 as part of an article in The Intercept, which according to the annotations on it was taken on 28 January 2009 at 5:16 UT,

I had forgotten about it untill this article by Dwayne Day brought it to my attention again, and then I remembered that I had already identified this image as being taken by USA 129 (1996-072A), a now deorbitted KH-11 reconnaissance satellite.

image source: The Intercept 6 Sept 2016

In 2018 Bill Robinson geolocated the image as showing a part of Zaranj, a southern Afghanistan village on the border with Iran. I in turn was able to show that USA 129 was near this location (see Bill's blog post), in an appropriate position to make the image. As een from the position of USA 129 at 5:16 UT, Zaranj was located at a range of 368 km. Seen from Zaranj, the satellite was in azimuth 216 degrees, elevation 66 degrees at that time.

click map to enlarge

USA 290 (NROL-71)

click image to enlarge

The photograph above is not the best of images, but it does show the trail (faint) of  USA 290, the payload of the January 19 NROL-71 launch from Vandenberg. I shot it last Monday morning, February 11th.

I wrote about this odd launch earlier (here). Before the launch, it was widely suspected that this was a new electro-optical reconnaissance satellite, a block V KH-11 ADVANCED CRYSTAL ("Keyhole"). So we expected it to go in a 98-degree inclined, ~1000 x 265 km sun-synchronous orbit, the orbit typical for new primary plane additions to the KH-11 constellation.

But then the Maritime Broadcast Warnings for the launch came out, and it became clear that the splashdown and deorbit zones did not fit a launch azimuth consistent with such an orbit (see a previous post where this was discussed). Instead, it suggested a 74-degree inclined, 265 x 455 km non-sunsynchronous orbit. Which was very odd, as it was completely against expectations for a new KH-11.

click map to enlarge

The launch was postponed several times, but finally happened on 19 January, a month later than it was originally slated. The launch postponements added a new mystery: the shifting launch window times with each postponement suggested a particular orbital plane with a nodal precession of -2.27 deg/day was aimed for.

The question was: why, if  NROL-71 was going into a 74-degree inclined orbit? Targetting a specific orbital plane only makes sense when the payload is part of a constellation of satellites. But NROL-71 was not targetting the orbital inclination of the existing KH-11 constellation (currently consisting of USA 186, USA 224, USA 245). And it's orbit is (as we will see) not sun-synchronous. It is very odd (and does suggest there will be future objects going into a similar orbit).

After launch on 19:10 UT on January 19th, 2019, there initially was no optical visibility as nighttime passes in the Northern hemisphere were in earth shadow.

But radio observers (a.o. Sven Grahn, Scott Tilley, Cees Bassa, Nico Jansen) quickly picked up the radiosignals of the payload at 2242.5 MHz. These showed that the payload was in a 73.6 degree inclined non-sunsynchronous ~400 km Low Earth Orbit, much as we had gleaned pre-launch from the hazard zones in the Maritime Broadcast Warnings.

As USA 290 slowly emerged from Earth shadow passes, the first optical observations were made by Russell Eberst in Scotland in the morning of 1 February. Next Leo Barhorst in the Netherlands soon followed.

These initial passes were very low in the sky, too low for my urban environment where I need elevations above 20-25 degrees to clear the rooftops. And when as February progressed the passes gradually climbed higher in the sky for my location, weather was not cooperating.

But in the morning of 11 February I finally had a clear sky, and managed to image USA 290, photographically as well as on video. As the illumination angle was not the best, the payload stayed a bit faint, but still was bright enough to register as a faint trail on the photograph (the bright star near the trail is gamma Cygni. Image taken with a Canon EOS 60D + EF 2.0/35 mm lens):

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The object showed up well on the video (WATEC 902H + Canon FD 1.8/50 mm lens), yielding good astrometry:




The optical observations helped to better define the orbit. They show USA 290 is in a 393 x 422 km, 73.6 degree inclined, non-sunsynchronous orbit.

Apart from abandoning the 97.9 degree inclined sun-synchronous orbit of the primary plane KH-11's, it also abandoned the 1000 x 260 km orbital altitude that was previously typical for new primary plane launches. The orbital altitude is closer to the extended mission, secondary plane KH-11's, the sole representative of which (USA186) currently is in a 262 x 452 km orbit.

Of course, in terms of orbital inclination and nodal precession (the non-sunsynchronous character) it doesn't compare to any of the previous KH-11.

(Note: a few year ago I wrote a series of detailed posts analysing the orbital constellation of the KH-11, and the typical changes in orbital plane and orbital altitude when a new addition to the constellation was launched: see the posts here and here).

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So, there is something new under the sun, in more than one way. While the general consensus still is that USA 290 is an electro-optical bird in the ADVANCED CRYSTAL lineage, the radical break with previous orbital structures for this series of satellites is highly interesting. It will be interesting to follow this new object, and see how things develop with future launches.

Over the last two years, the black space program in Low Earth Orbit has become much more exciting, with some new eyebrow-raising additions unlike any previous missions. Examples are USA 276, the failed Zuma launch, and now USA 290, all launches from the past 1.5 years.

I like it: just when we thought things were getting perhaps a tad predictable, we are suddenly treated to a number of surprises, resulting in new stuff to ponder and analyse.

NROL-71: an enigmatic launch [UPDATED]

(this post on NROL-71 is belated, as I was in hospital around the original launch date. Luckily, launch got postponed)

click map to enlarge

If nothing ontowards happens, the National Reconnaissance Office (NRO) will launch NROL-71, a Delta IV-Heavy with a classified payload, from Vandenberg SLC-6 on 19 December 2018 (18 December local time). [edit:] after the December 19 launch was scrubbed, a new launch attempt will take place on December 20 (December 19 local time in the USA). The December 20 launch was scrubbed as well due to a hydrogen leak in one of the boosters. A provisional new launch date is 21 December 2018 (December 20 local time in the USA) at 1:31 UT.

The new launch date will not be before 30 December 2018.

The launch was postponed three times. Originally to be launched on December 8, a communications problem aborted that launch. A renewed launch attempt the next day, was aborted only 7.5 seconds before lift-off because of a technical issue (see the video below).




A new launch attempt will take place on 19 December 2018 at 1:57 UT. As weather prospects at the moment do not look particularly good for that date, it is possible that the launch will see even further postponement. [edit:] This assessment turned out to be right: the launch was postponed due to high altitude winds. A new launch date has been set for 20 December 2018 at 1:44 UT. The December 20 launch was also aborted, due to a hydrogen leak in one of the boosters. A provisional new launch date has been set for 21 December (20 December local time in the USA) at 1:31 UT. The new launch date will not be before 30 December 2018.

NROL-71 is an odd launch. When the Maritime Broadcast Warnings for the launch came out and revealed the launch hazard areas, they contained a big surprise. The general expectation among analysts was that NROL-71 was the first of the Block V new generation KH-11 ADVANCED CRYSTAL electro-optical reconnaissance satellites. As such we expected it to go in a sun-synchronous, 97.9 degree inclined, 265 x 1000 km orbit.

But the Maritime Broadcast Warnings suggest this is NOT the case. The hazard areas are incompatible with such a sun-synchronous polar orbit. Instead, they point to a (non-sunsynchronous!) 74-75 degree inclined orbit. Not what you expect for an optical reconnaissance satellite!

The map below shows the three hazard zones. Two are directly downrange from the launch site, where the strap-on boosters and first stage splash down. The third area is the upper stage deorbit area (which is remarkably small in size), located northeast of Hawaii, with deorbit occuring near the end of the first revolution (as usual).

click map to enlarge

The trajectory depicted by the dashed line on the map is for a 74-degree inclined, 265 x 455 km orbit. Higher inclined orbits would miss the downrange splashdown zones and the upper stage deorbit area.

Ted Molczan has pointed out that the shift in launch time with each launch delay, points to a specific orbital plane and a specific aim for the rate of precession of the RAAN of -2.27 deg/day.

This is over twice as fast as the RAAN precession of the KH-11 currently in orbit (0.98 deg/day, i.e. sun-synchronous).

This value for the RAAN precession apparently aimed for, puts further constraints on the orbit as in combination with the 74-degree inclination deduced from the location of the Launch Hazard areas it points to a semi-major axis of about 6735 km.

Going from the notion of KH-11-like orbital altitudes, the current typical KH-11 perigee near 265 km would then result in an apogee near 455 km. This is somewhat similar to the orbital altitude of the oldest of the KH-11 on orbit, USA 186 in the secondary West plane, which was in a 262 x 443 km orbit when we last observed it early October (it currently is invisible due to the winter blackout). This apogee would be much lower than that of the two KH-11 payloads in the primary planes, which have apogee near 1000 km, i.e. twice as high, another deviation from expectations. Normally, KH-11 are launched into a primary plane and about 265 x 1000 km orbit, and only after some years, when the payload is moved to a secondary plane (and a new payload is launched into the primary plane), is apogee lowered to ~450 km (see an earlier post here).

So, if NROL-71 is a new electro-optical reconnaissance satellite in the KH-11 series, it represents a serious deviation from past KH-11 missions. The apparent abandoning of a sun-synchronous polar orbit, is surprising, as such orbits are almost synonymous with Earth Reconnaissance. The "why" of a 74-degree orbit is mystifying too. If it does go into a 74-degree inclined orbit, it doesn't seem to be a "Multi-Sun-Synchonous-Orbit".

Alternatives have been proposed. Ted Molczan has for example suggested that, perhaps, NROL-71 could be a reincarnation of the Misty stealth satellites, warning that the unexpected orbital inclination for NROL-71 might not be the only surprise.

I myself was struck by the fact that 74-degree orbital inclination is the prograde complementary of the retrograde 106 degree inclination of the FIA Radar/TOPAZ 6 payload (USA 281,  2018-005A) launched early this year: note that 180-106 = 74. FIA Radar 6 was the first in a new block of TOPAZ radar payloads, just like NROL-71 appears to be the first in a new block of  'something'.

The previous four FIA Radars, launched into 123-degree inclined orbits, were the retrograde complementary in inclination of the prograde 57-degree Lacrosse 5 orbit, another radar satellite. The complementary character of 106-degree versus 74-degree for NROL-71, could perhaps point to NROL-71 being a Lacrosse Follow-On, as a complementary to the newest FIA block.

If NROL-71 is a Lacrosse Follow-On, its orbital altitude and brightness behavious might yield clues: Lacrosse 5 has shown a very distinct brightness behaviour.

It will be very interesting to chase this launch. If launch occurs on 19 December near 1:57 UT and weather cooperates, Europe will have visible evening twilight passes in the first few days.

Below are a couple of search orbits. All are for an assumed 74-degree orbital inclination and launch on 19 December at 1:57 UT. The first three are for KH-11 like orbital altitudes. The fourth is for a Lacrosse-like orbital altitude.

Orbit #70003 fits the hazard areas from the Maritime Broadcast Warnings best.

[EDIT: new updated search orbits below, for the new launch date, 19 Dec 20918 1:44 UT] 

[EDIT: new updated search orbits below, for the new launch date, 21 Dec 2018 1:31 UT]



NROL-71                                                 265 x 1000 km
1 70001U 18999A   18355.06319444  .00000000  00000-0  00000-0 0    00
2 70001 074.0000 184.7636 0524203 155.2439 326.4145 14.78994708    03

NROL-71                                                  265 x 500 km
1 70002U 18999A   18355.06319444  .00000000  00000-0  00000-0 0    01
2 70002 074.0000 184.7636 0173800 155.2439 324.5345 15.61785606    06

NROL-71                                                  265 x 455 km
1 70003U 18999A   18355.06319444  .00000000  00000-0  00000-0 0    02
2 70003 074.0000 184.7636 0140989 155.2439 324.3567 15.69614809    07

NROL-71                                                  715 x 725 km
1 70004U 18999A   18355.06319444  .00000000  00000-0  00000-0 0    03
2 70004 074.0000 184.8196 0007044 155.2265 327.0336 14.51731413    06



Note that deviations of many minutes in pass time and several degrees deviation in cross-track are possible on all four orbits, certainly several revolutions after launch.

USA 186 recovered

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The image above shows USA 186 (2005-042A), a KH-11 ADVANCED CRYSTAL ("Keyhole") optical reconnaissance satellite. It is cruising just below the Pleiades star cluster in this image, which I shot yesterday evening using the Samyang 1.4/85 mm lens and an exposure of 2 seconds.

USA 186 was recovered last week after being briefly lost in the Northern hemisphere winter blackout. Leo Barhorst made one or two possible detection in February, but it was Cees Bassa who unambiguously recovered it on March 13th. Two days later, I made the image above.

The arc is still short, but it appears to be in an approximately 265 x 435 km sun-synchronous orbit. The apogee is some 20 km lower than it previously was, the perigee is about 5 km higher (i.e., the current orbit is more circular than previous orbits). It's ground repeat interval is 4 days.

USA 186 is the secondary West plane satellite in the KH-11 constellation. The hunt is now on for USA 245, the primary West plane KH-11. Recovery of the primary East plane KH-11, USA 224, will have to wait untill early summer.

When I observed it yesterday it was bright (mag +1.5) and briefly flared to mag 0 near 19:32:50 UT (March 15, 2017).

USA 224 recovered: an update of the KH-11 constellation

Russell Eberst in Scotland has recovered the noon-plane KH-11 ADVANCED CRYSTAL/"Keyhole" optical reconnaissance satellite USA 224 (2011-002A) this week. The recovery happened relatively late (in 2015 it was recovered 2 months earlier).

This recovery means that, after the preliminary update last March, I can provide my periodic update on the orbits of the KH-11 constellation based on timely orbital data.

In various previous post to this blog, I outlined how the KH-11 constellation consists of two primary orbital planes, the primary East and West planes; and originally two, now one, secondary orbital plane(s). Of the latter secondary planes, only one, the secondary West plane, is left after the de-orbit of USA 161 late 2014.

The past decade or so, the primary planes have been 48-49 degrees apart in RAAN. That is still the case: USA 224 and USA 245, the primary East and West plane KH-11's, are currently 49 degrees apart in RAAN.

The secondary planes used to be either 10 or 20 degrees from the corresponding primary plane in RAAN, but since mid-2014 the secondary West plane (currently USA 186) has moved further out, to 24 degrees West of the primary orbital plane.

As I have outlined before on this blog, the secondary plane(s) differ in orbital altitudes from the primary planes. The current configuration:


         perigee   apogee    l time   repeat
Sat        km        km      d node   (days)   plane
USA 186    261       454     08:05      3      secondary W
USA 224    262      1007     12:58      4      primary E
USA 245    266      1000     09:42      4      primary W

Given are the apogee and perigee altitudes of the satellites, the average local time they pass through their descending node (an indication of around what time they pass a given area - all satellites in the constellation are sun-synchronous, i.e. they pass  at a similar solar elevation each day), the repeat interval of the ground track in days, and the plane they orbit in.

What can be seen is that the secondary plane satellite, USA 186, is in a much more circular orbit with a much lower apogee (454 km), compared to the two primary satellites (~1000 km). Perigee altitudes of all three satellites are similar. I have speculated on the reason for this apogee difference of the secondary plane satellite at the end of a previous post.

The West plane satellites, USA 186 and USA 245, make morning passes, about 1h45m after each other. The East plane satellite, USA 224, makes passes about an hour after local noon.

The current orbital configuration has been more or less stable since mid-2014 (or more exactly, since USA 161 was de-orbitted late 2014).

USA 186 rising, and revisiting the KH-11 constellation

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The image above shows the KH-11 ADVANCED CRYSTAL/"KeyHole" optical reconnaissance satellite USA 186 (2005-042A) rising over the roof of my house in late twilight of March 28, 2016.

It had passed perigee at 260 km altitude just 10 minutes earlier and was at about 285 km altitude when I photographed it. At that low an altitude, it races over the sky (these are 5 second images with a 50mm lens). Clearly visible by the naked eye, I watched it rise over the roof, and then slowly flare to mag. -1 near 19:17:55 UT:

USA 128 186 flaring near 19:17:55 UT (March 28, 2016)
click image to enlarge

USA 186 is the oldest of the remaining KH-11 ADVANCED CRYSTAL satellites. After the de-orbit of  USA 161 late 2014, there are now three KH-11's left on-orbit:  

(a)  USA 186  (2005-042A) pictured here;
(b)  USA 224  (2011-002A), and;
(c)  USA 245  (2013-043A).

USA 224, the primary East plane satellite, and USA 245, the primary West plane satellite, are separated by 48.7 degrees in RAAN. USA 186, the secondary West plane satellite, is 24.3 degrees (half the separation of the two primary satellites) West of USA 245 in RAAN:

click to enlarge

All the orbits are sun-synchronous, meaning that they maintain an orbital precession coupled to the daily precession of the sun.This ensures that they make passes at roughly the same time each day, imaging terrain with roughly similar solar elevations. This helps interpret imagery, as the shadow patterns will be similar on images from nearby days and changes in shadow pattern will stand out.  

USA 224, the primary East plane satellite in the constellation, makes daily passes around 13h local solar time. It's ground track repeats each 4 days. USA 245, the primary West plane satellite, makes daily passes around 9:45h local solar time, also with a ground track repeating each 4 days. USA 186, the secondary west plane satellite, makes daily passes around 8h local time, with a repeating ground track each 10 days.

Basic data ():

sat      orbit           mlt DN    repeat  plane 

USA 124  265 x 1009 km*  13:00     4 days  primary E
USA 245  268 x 1020 km   09:45     4 days  primary W
USA 186  260 x 456  km   08:05    10 days  secondary W

* September 2015 (sat not yet recovered in 2016)

("mlt DN" means mean "local time of passage through Descending Node") 

Note that due to the winter blackout in the Northern hemisphere we haven't observed USA 224 for seven months: the orbit shown here assumes it has kept up its September 2015 orbit. We will know for sure when we recover the object in early summer.

The previous secondary West plane satellite in the constellation, USA 129 (de-orbited in late April of 2014) used to make passes near 9h local time. By changing the RAAN difference between the primary and secondary satellite from 10 degrees to 24.3 degrees after USA 186 moved from the primary to the secondary plane and took over from USA 129 following the launch of USA 245 (see earlier post here and links theirin), the pass time was shifted to one that occurs one hour earlier.

As can be seen in the table above, all current KH-11's have perigee at a roughly similar altitude of ~260-270 km. The primary plane satellites have apogee at ~1010-1020 km. The secondary plane satellite has a much lower apogee, at ~455 km altitude.

The exact reason why the secondary plane KH-11's lower their apogee is unclear. USA 129 was the first to lower apogee connected to its move from the primary West plane to the secondary West plane in 2006. USA 161 repeated this pattern in 2011 when it was moved from the primary East plane to the secondary East plane (since the de-orbit of USA 161 late 2014, this latter secondary East plane no longer exists). Various options can be considered:

(a) some operational constraint, e.g. aim for a particular ground-track repeat interval;

(b) some operational constraint, e.g. related to image resolution (this is unlikely);

(c) some operational constraint, e.g.different imaging role compared to the primary plane satellites;

(d) making it easier to de-orbit the satellite near end-of-life: if fuel reserves are low, a lower apogee would allow de-orbit from apogee if necessary, so one does not necessarily have to wait for perigee to be located over the southern Pacific.