The Hunt for OTV-7

On a dark late December winter night the United States military launched its secretive X-37B spaceplane atop a Falcon 9 heavy rocket from Kennedy Space Center. After watching the rocket slip from sight and the side boosters return nothing was seen from the spaceplane until the night of February 7, 2024 when amateur satellite observer Tomi Simola found something unusual, read his story below…

Read more: The Hunt for OTV-7

Into the Dark

At 01:07 UTC December 29, 2023, the US Space Force (USSF) launched their latest X-37B spaceplane mission referred to at Orbital Test Vehicle (OTV) 7 into a highly classified secret orbit.

OTV-7 launched atop a SpaceX Falcon 9 Heavy on December 29, 2023.

Unlike earlier missions this launch was not targeting a low Earth orbit (LEO). The limited details shared to the public in Notice To Airmen (NOTAMs) revealed the spaceplane was likely targeting a high Earth orbit (HEO). Dr. Marco Langbroek conducted an analysis of the NOTAM information and shared a plausible trajectory for OTV-7.

Macro LangBroek’s analysis and suggested search trajectory for OTV-7.

Unfortunately, the time of the launch placed most of the trajectory in Earth’s shadow hiding the spaceplane from view during most of its initial coast orbit and while climbing to apogee it would be lost in the glare of the Sun during daylight.

To make the search more challenging X-37B’s are not known to emit on traditional Tracking Telemetry and Control (TT&C) radio frequency bands and likely use the National Reconnaissance Office’s (NRO) classified Satellite Data Service (SDS) and inter-satellite communications links making it exceeding difficult to track emissions from the spaceplane. 

One thing we did have going for us to search for on radio in the dark and later in the glare of the Sun was the final stage of the Falcon 9 Heavy. Given the NOTAMs revealed the rocket stage would be de-orbited over the northern Pacific Ocean thus its mission would likely carry on to at least apogee where it would conduct a de-orbit burn to lower its perigee to below the Earth’s surface to safely de-orbit the stage in the remote ocean area noted on the NOTAM.

Using Federal Communications Commission (FCC) filings we found the particular paperwork for the USSF-52 launch as submitted by SpaceX and knew that the final stage rocket should be emitting on 2232.5, 2247.5, 2255.5 and/or 2272.5MHz.

A group of amateur satellite trackers in Europe and western Australia where organized in an attempt to gather radio data from the Falcon 9’s final stage in an attempt to confirm the actual trajectory of the OTV-7 through this indirect means and hopefully allow for its optical recovery later.

Using Marco LangBroek’s search TLE, a radio observer in Western Australia was right under the suspected track of the OTV-7 and its rocket stage.

The observer in western Australia maintained vigilance for the entire expected pass of OTV-7 and its respective rocket booster. Guidance was provided to the station to conduct scans of the clear sky from 2200-2300MHz from the site using their 1m dish antenna in an effort to find the rocket booster’s emissions on S-band. We heard many signals from many other missions but nothing form OTV-7’s rocket booster. Therefore, either the rocket booster wasn’t emitting, which would be highly unlikely considering past observing experience or the trajectory guess for OTV-7 was not accurate enough to place the rocket booster in the sky above the observer in western Australia. 

To Planar Scan or Stare into Space…?

It seemed like our only chance to find OTV-7 using Marco Langbroek’s reasonable analysis of NOTAM data had resulted in failure and most likely a long search would need to be performed to find OTV-7. Two possible strategies to find OTV-7 could have been reasonably considered. One, a planar search which assumes OTV-7 was on the orbital plane Marco’s trajectory stated but it was not in the location in the plane we thought. Two, multiple observers could just stare into space and with patience OTV-7 would pass sooner or most likely later through the field of view of someone.

What is a planar search? A satellite once launched into space is in a fixed plane with respect to the stars and it will stay in that orbital plane for all practical purposes unless something adds or removes energy from the object. The effects of atmospheric drag ,solar radiation pressure, venting etc. can cause the spacecraft’s position within an orbital plane to change over time creating uncertainty of where within the orbital plane the satellite is. To recover an object in a known orbital plane one can search the plane by scanning along it for a prolonged period of time and eventually you will find your wayward satellite. However, this assumes you know the orbital plane correctly.

In our radio search for the final rocket stage which should have been very close to OTV-7, we actually compensated for this by conducting a broader search of the track and sky for some hours and would have likely found the rocket’s emissions had the orbital plane guess been close. Another factor is the timing of arriving in the orbit was fairly constrained limiting the search area along the orbit plane. This left us to conclude that OTV-7 was most likely not in the orbital plane Marco’s analysis suggested. Thus an planar search of the plane Marco suggested was likely going to be very laborious and not result in recovering OTV-7.

Marco Langbroek, Tomi Simola and Scott Tilley discuss a search strategy on X (formerly Twitter) for OTV-7.

Based on what we knew, it was agreed that staring into space may be the best strategy. You may be wondering and rightfully point out that space is pretty vast and staring at a fixed small spot may never produce results. It’s counter-intuitive but the fact is a satellite is in a fixed orbit. In this case we roughly knew the orbital geometry of our target and had a pretty good idea that if we aimed a camera at an intelligently chosen fixed spot and waited long enough the satellite would pass through and we would know it was our target because almost all other objects on orbit are known and catalogued or would be in different orbits and could be excluded. 

OTV-7’s actual passes over Tomi Simola’s observing station for 30 days. Notice the patterns in the trajectory. If you know something about the inclination and shape of the orbit you can stare at optimal places in the sky to improve your chances of the spacecraft passing through your field of view.

This is what Tomi Simola did to find OTV-7, he setup a light sensitive camera and connected it to a computer to record the results and excluded every object that passed through his field of view for literally weeks until an unidentified object passed through the field of view that matched OTV-7’s characteristics. 

On the night of February 7, 2024, Tomi Simola recovered OTV-7 and made these observations with his staring camera. Once you have even a limited set of short arc observations you can start to generate orbital elements from the data and start to narrow down the identity of the object. After consulting Mike McCants an expert on classified objects on orbit the identity was quickly firmed up as the orbital data came in on successive nights.

Tomi Simola’s discovery image of OTV-7 from February 7, 2024.

It turned out that our assumption that OTV-7 was in a different orbital plane than Marco’s reasoned guess was correct. Below you can see the dramatic difference in the sky track from the observer in western Australia for OTV-7. Much of the track was obscured by trees and other obstacles at the ground station. OTV-7 quickly passed through the ground station’s clear area of sky spent most of the pass low on the south eastern horizon obscured by trees and then as it descended from apogee passed quickly through the observable sky and disappeared…

For the record here are the initial guess TLE vs. the TLE developed from Tomi Simola’s observations of OTV-7 after it was recovered.

USSF-52 OTV 7 for launch on 29 Dec 2023 01:07:00 UTC
1 70000U 23999A 23363.06545139 .00000000 00000-0 00000-0 0 02
2 70000 074.0000 341.4480 7418186 136.2072 360.0000 02.14201823 02

OTV 7
1 58666U 23210A 24039.74420665 0.00000000 00000-0 00000-0 0 04
2 58666 59.1161 4.8483 7418435 167.3793 193.0310 2.07574710 01

An Interview with Tomi Simola on Finding OTV-7

Scott Tilley – Can you describe your observing strategy you used to recover OTV7?

Tomi Simola – Stare long enough and it will pass your Field-of-view!

Earlier I have been pointing my camera at different parts of the sky, depending on the object or area of interest. Because OTV-7 has gained great interest in the satellite watching and space technology community I elected to keep the camera stationary. Early orbital predictions showed that OTV-7 will eventually pass the FOV! As you pointed out (and it makes perfect sense), there is no point to chase a satellite when you don’t know where it is!

Scott Tilley – Can you tell us more about how you and Mike McCants came to the conclusion that the object you observed was OTV7?

Tomi Simola – After I posted my first observations to Seesat-L on February 8, Mike McCants emailed me three hours later with orbital elements for “Unknown 020724”. He could not match it with anything in his catalogues. He reckoned “it was a small piece of space debris catching sunlight just right.”

I respectfully disagreed, explaining that visually the UNID was steady over the whole pass and “eyeball” magnitude similar to large USA 144 Deb (25746 / 99028C), which has passed a couple of times on a similar distance.

Next night I observed it again and very close to Mike’s earlier prediction. He told me that I’ve found the OTV-7!

Scott Tilley – Can you describe your observing equipment. What kind of camera, lens and software are you using?

Tomi Simola – I use the Watec 902H Ultimate analog video camera with a Chinese TTArtisan 50mm f1.2 lens. There is a 3D printed adapter in between. The lens was a lucky find for only 100 euros!

Tomi Simola’s camera staring into space waiting for darkness to resume the search for OTV-7.

The software is Cees Bassa’s STVID and SATTOOLS. I have the camera in an IP68 camera housing with a servo driven sunshield in front of the lens. Separate mini PC has STVID doing the capture to a NAS storage in my network. A virtual machine has a STVID and SATTOOLS installed and I use it for processing the observations.

Scott Tilley – How did you feel when you first noticed the unidentified satellite in your data?

Tomi Simola – I was browsing the images that STVID had tagged as UNID. There was one set of images (20 or so) with an object with a rather short trail, meaning it was in a higher orbit. And while scrolling the images back and front I noticed the object was “accelerating”! The trail got longer (almost doubled) at the end of the set of images! Then I knew that this was something different!

My amateurish initial analysis for a circular orbit showed it in 56.5518 inclination, 6.6 revs/day. That inclination didn’t sound like Dr Marco Langbroek’s pre-launch prediction of 74 degrees. 6.6 revolutions per day was too much for a Molniya kind of orbit. I stated my doubts in an email to Seesat-L.

Scott Tilley – When did you know that you had found OTV7? How did that feel?

Tomi Simola – After Mike McCants email where he told me the UNID was OTV-7! I might have done a wild, but private “goal celebration”!

Scott Tilley – Can you tell us about your observing site and how it makes satellite observing unique? I.e. your northern latitude and how that affects satellite illumination.

Tomi Simola – My observing site is in my south facing backyard. But there is an area where I can set up my camera and point it over the neighbours roof, pointing low at the Northern sky. Area of the sky is busy with NOSS satellites which are very predictable and they are good targets to practice observations!

My latitude is 60 North, so some satellites are more visible earlier in the spring / later in the autumn, than for those in lower latitudes.

The site is very close to an international airport, but that has no great effect in my observations.

Scott Tilley – In this process of building an observing station and operating it what have you learned and what are your next steps?

Tomi Simola – I was not that much interested in visual satellite observing until two years ago, when I found the Watec camera for a very good price! Cees Bassa’s STVID was at that time getting rapid updates. Then I started to read tutorials from www.satobs.org.

I have done some RF observations with Bassa’s STRF (interest in this was sparked by Scott Tilley’s recovery of IMAGE in 2018), but the visual side was something different. SATTOOLS and STVID are very powerful software, but learning curve is…”steepish” – especially when one has no prior experience in visual satellite tracking!

Tutorials, articles and members of the Seesat-L have helped me to understand a bit better orbital dynamics and therefore I can pre-analyze my observations a bit better now. But there is so much more in orbital dynamics, visual tracking, that only way is forward! Interesting hobby that I never thought I’d get into!

More technical side, I have to improve the Wife-Acceptance-Factor of the camera setup. Also, a motorized mount would be nice in winter time!

Scott Tilley – Why do you look up and observe the sky to monitor satellites?

Tomi Simola – My interest in space flights and satellites was sparked when I was a small boy. I was living in a small village, far from the nearest city, with a stunning night sky! Moving stars in the sky were quickly explained as satellites.

The school library had lots of old books and my favourites were translated versions of “Die Mondlandung / Moon landing, 1969”, by Herbert J. Pichler and “Man and space, (Life science library), 1972” by Arthur C. Clarke. I have read these tens of times! I later acquired these books for my ever growing space library!

In my teens I received weather satellite pictures from NOAA and old Meteor satellites and kosmonauts talking with Moscow from MIR.

Satellites are fascinating! They are so close, just 200-300 km away, but getting there requires the smartest minds on the planet!

Spaceflights were for a long time only for superpowers and government backed institutions! They were rather rare occasions. Now, when technological advancements have brought satellites to the masses (you can almost literally buy your own satellite!), the “saturation” of the lower Earth orbit is getting more serious. I think satellite collisions are still rare, but astronomers using the whole electromagnetic spectrum (from DC to daylight and beyond) are getting frustrated with RF and visual noise in their data! Future space companies should have more responsibility to keep near space clean.

Amateur observers, not only for classified payloads, have an important task to bring these problems to the public and more importantly, to lawmakers! Good example is BLUEWALKER 3, which has a very large and visible antenna and dubious RF characteristics!

Conclusion

Once again amateur satellite observers with modest means and lots of patience find a classified object in space. We hope that sharing this story inspires others to look up and ensure the transparency in the use of space by all nations. 

Understand Doppler Analysis

We often post data online showing the results of a Doppler analysis. The concepts can be a bit intimidating to understand but with a little explanation it’s accessible to anyone.

Read more: Understand Doppler Analysis

What is the Doppler Effect?

When something emits electromagnetic radiation and is moving relative to an observer the observed wavelength of the emitting radiation will be different. Essentially when things are moving their movement effects how the waves of radiation arrive at the observer. If they are moving toward each other the wave crests successively arrive earlier thereby decreasing the wavelength observed. If the objects where moving apart then the opposite happens and the wavelength increases.

So how does this apply to observing satellites? Imagine you are at a very large train station that has an infinite number of tracks coming and going from the station in all directions. East, West, North, South and even up into the sky and down into the Earth. Further imagine you are listening to the whistles of all these trains passing through the station. Some are moving fast some slow all going in different directions. As almost everyone has experienced the pitch of the whistles note will change based on the change in velocity of the train as it passes you by. If you really pay attention you will notice the pitch of all the trains coming and going is different depending on their orientation to you, their speed and even if you decide to walk around the station and move yourself.

Using this knowledge one could use the Doppler effect to map out the train’s trajectories as they pass and determine which are which especially if they follow schedules and are on predefined routes. This is what we are doing to track satellites with the Doppler effect. Instead of whistles the satellites have radio transmitters. Instead of tracks they have orbits in which they are locked into by the force of gravity. These orbits are periodic and predictable. Therefore, if you know about how your moving and have observed data from the satellite’s radio transmitter you can compare this to a large number of guesses about the orbit it’s in and find matches that best fit the orbit. If you have a list of known satellites in known orbits you can compare that list to the data you collect to find the best match too.

All that is going on is systematically observing the change in frequency of the satellite’s radio emissions and then comparing that to a large number or educated guesses to find the best fitting guess to the data.

Understanding Doppler Analysis Plots

The following provides a brief walk through to orientate a reader on what Cees Bassa’s Satellite Tools Radio Frequency (STRF) displays as a result of a Doppler analysis of a signal. This should provide the reader with enough context to understand the display given our comments earlier.

The STRF Doppler Plot displays the raw Doppler data observed and the prediction of the Doppler from the current TLE (orbital model).

The Doppler plot noted above provides the raw Doppler frequency data (left y-axis) and the resulting range rate (line of sight velocity) on the right y-axis. The x-axis is time in Modified Julian Date (MJD).

Frequency is self evident as it’s the data we collect with our radio and antenna from the satellite. The range rate is a bit more obtuse. Range rate can also be better described as the line of sight velocity between two things. I.e. the resultant velocity at that time of perhaps two things moving with respect to each other. Doppler frequency tells us directly about this line of sight velocity and is what is actually used to compare the orbital models against.

Modified Julian Date (MJD) is a computationally friendly time system that allows for easy consecutive calculation of time based on a defined epoch (start date) of the system. MJD is used a lot in astronomy and astronautics.

Inside the plot the white lines (dots) are selected Doppler data. The grey line is the predicted Doppler curve when the object is below the observer’s horizon. The red line segments are when the object should be above the observer’s horizon.

The TLE (Two Line Element) block displays the current ‘template’ orbital elements being modelled.

The Two Line Element block displays the current ‘template’ orbital elements being modelled. If you want to learn more see my article on Basic Orbital Dynamics. The user can use template orbits, old orbits to update and also change the settings based on knowledge and intuition.

The Fitted Elements block allows the user to choose which elements should be fitted for the best fit to the data.

The fitted elements block allows the user to select which elements should be fitted for the best fit to the data. Careful selection of these given understanding of the orbital dynamics allows the user to find the best correct fit to a data set.

The Sky Track block provides a visualization of the satellites path through the observer’s sky during the times data is present.

The sky track block allows the user to visualize the satellite’s path through the observer’s sky during times data is present. This is helpful when comparing to other data sources like antenna position etc.

Analysis Results block provides the basic results of the current Doppler analysis.

The analysis results block provides the basic summary of the current Doppler analysis. Measurements is the total number of Doppler samples in the analysis. Frequency is the measured spacecraft emitted frequency once Doppler is accounted for. The rms is Root Mean Square error of the data compared to the model. TCA is Time of Closest Approach to the observing station performing the analysis. The name and COSPAR # for the observing station is next. The RED 8049 means that observing station 8049 data is present. If another station also contributed data their number and a different colour would be used to represent that.

To understand how good or bad an analysis is look at the rms number. The lower the better.

How Accurate is Doppler Analysis?

Accurate Doppler analysis relies on the observer recording very accurate frequency samples of the observed satellite signal. Therefore, using a very accurate clock for timing is required. In my case I use a GPS referenced oscillator to perform this function. This leads to the other source of error the spacecraft itself. Most spacecraft in Earth orbit and in Lunar orbit don’t usually have super stable radio oscillators. The reason is they don’t usually need this as the control stations will use other methods of determining the range and range rate to the spacecraft like two-way Doppler that uses a transponder on the spacecraft and therefore eliminates the spacecraft’s oscillator as a source of error. However, in our case we are limited to the one-way Doppler and must deal with the errors. If you want to learn more read NASA JPL’s Range and Doppler Tracking Observables.

Mysterious ‘Pips’ from the Chinese JILIN Constellation

Why is an imaging satellite constellation acting like a mobile-satellite communications system?

China’s first self-developed commercial remote sensing satellite system known as JILIN is sending strange wideband data pips in a quiet piece of spectrum on L-band. The JILIN system is operated by Chang Guang Satellite Technology Company in Beijing. No public references have been found by the author about what these emissions from the satellites purpose is.

Continue reading “Mysterious ‘Pips’ from the Chinese JILIN Constellation”

You can call me Dmitry Meyer…

History Repeats Itself

Russia operates a constellation of satellites in high Earth orbit called Meridian (меридиан). These satellites perform a critical communications purpose for Russia as much of its land mass is not well served by geostationary satellites. Therefore, you would think this constellation would be held to the highest operational level. Well it’s not as radio amateurs have observed. This fact could raise questions about Russia’s ability and preparedness to act on their recent veiled threats of nuclear war.

Continue reading “You can call me Dmitry Meyer…”

Chang’e 5 Returns to the Moon

Chang’e 5 has quietly departed from the Sun-Earth L1 point to enter a distant retrograde orbit (DRO) of the Moon, a first.

Pre-empting NASA’s planned 1st use of the orbit during Exploration Mission 1 later this year.

Silence from China.

Off Station

In mid August 2021, the Chang’e 5 service module without any notice was noted to not be on station near the Sun-Earth L1 point where it had been since mid-March 2021. Observers were quick to reacquire the spacecraft’s X-band beacon and it was not long before it was clear from the data that Chang’e 5 was headed back to the Earth-Moon system where it would ultimately enter a Distant Retrograde Orbit (DRO) of the Moon.

Continue reading “Chang’e 5 Returns to the Moon”

Basic Orbital Dynamics

There has been a recent surge in interest in a software package written by Cees Bassa known as ‘strf’, Sattools Radio Frequency.  Once over the initial installation and basic usage hump users quickly reach a wall about how to use the software because of a limited understanding of orbital dynamics.  I hope this brief post will help users understand some of the basic concepts so they can use strf as a tool.

Continue reading “Basic Orbital Dynamics”

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