This post is my speculation about the payload and orbit of NROL-71. For my pre-launch search TLEs, please see: http://satobs.org/seesat/Dec-2018/0045.html I have long expected NROL-71 to launch the first Block 5 KH-11, and that has been the consensus among others who have expressed their opinion. In this post, I will review the evolution of the NRO's imagery intelligence satellites since the early 1970s, and discuss what the future may hold for KH-11, based on what is known about Block 5 KH-11, and recent improvements in the resolution of commercial imagery. The following table summarizes the evolution of the NRO's high-resolution and wide-area satellites since the early 1970s: Period High-resolution satellite Wide-area satellite ---------- ------------------------------------ ------------------------------------- From To Program Type Resolution Program Type Resolution ---- ---- -------- --------------- ---------- --------- --------------- ---------- 1971 1976 Gambit-3 Film-return 8 cm Hexagon Film-return 30 cm 1977 1984 Crystal Electro-optical 7 cm Hexagon Film-return 30 cm 1985 2018 Crystal Electro-optical 7 cm Crystal Electro-optical 28 cm The following sections provide supporting information for each entry in the table. 1. 1971-1976 Gambit-3 (aka KH-8, after the designation of its camera) was a high-resolution satellite, of the film-return type. It was first launched in 1966. It typically operated in an approximately 130 km by 400 km orbit. Its 1.1 m diameter mirror had a theoretical resolution of about 8 cm at perigee, which was achieved in the early 1970s by upgraded versions of the satellite. The NRO inadvertently confirmed this through a redaction error in a declassified copy of The GAMBIT Story, which came to light in 2012, in the following NASASpaceFlight.com forum discussion: https://forum.nasaspaceflight.com/index.php?topic=26821.80 The unredacted relevant quote: "GAMBIT's contribution to scientific and technical (S&T) Intelligence were unsurpassed. The mature system produced examples of imagery better than four inches ground-resolved distance (GRD). Furthermore, it exhibited excellent mensuration capabilities, allowing the S&T photointerpreter to perform accurate measurements on foreign weapons systems..." P.154 Remarkably, with Gambit-3, the NRO had already reached the limit on resolution imposed by atmospheric turbulence. Allen Thomson informed me that scientific papers published in the mid-1960s by David Fried and, independently, by John C. Evvard, revealed that atmospheric turbulence limits the imaging resolution achievable from Earth orbit to about 5 cm to 10 cm. Their papers are available at the following URLs: http://ntrs.nasa.gov/archive/nasa/casi.ntrs.nasa.gov/19690003603.pdf https://www.osapublishing.org/abstract.cfm?id=53168 The significance of this, is that a larger mirror would not have improved the resolution of Gambit-3, at its minimum altitude of 130 km. A larger mirror would only have been required if this distance were to be increased. Hexagon (aka KH-9, after the designation of its camera), was the medium-resolution counterpart to Gambit-3. First orbited in 1971, it was the last of the NRO's film-return spacecraft. Its theoretical resolution ranged between 20 cm at perigee and 35 cm at apogee. 2. 1977-1984 The drag experienced by Gambit-3 was severe, which limited its orbital life; however, film-capacity was the main determinant of its useful life. Once the film ran out, the spacecraft was useless. The need to return film to Earth for processing, delayed the availability of imagery for analysis. An electro-optical imager would not have these limitations. Kennen (later changed to Crystal) (aka KH-11, after the designation of its camera), was the NRO's first electro-optical spacecraft, first orbited in Dec 1976. Since it did not use film, its useful life was determined by the durability of its hardware, and its ability to counteract the effects of atmospheric drag. Spacecraft maintain altitude against drag by periodically firing thrusters to reboost their orbit, which consumes fuel. The higher the orbit, the lower the drag. So, for a given quantity of fuel, the greater the orbital altitude, the greater the useful life. KH-11 experienced far less drag than Gambit-3, by operating in a higher orbit. Its lowest altitude was about 250 km; its greatest altitude was about 500 km. Since KH-11's minimum altitude was double that of Gambit-3, it needed a mirror roughly double that of Gambit-3, to match Gambit-3's best resolution. The theoretical resolution of KH-11's 2.4 metre diameter mirror at perigee was about 7 cm (3 inches) - about the same as Gambit-3 achieved with its 1.1 m mirror from 130 km. Hexagon remained the wide-area satellite during this period. 3. 1985-2018 As the Hexagon program drew to a close in the early 1980s, the NRO considered various options to preserve its capability. I recommend Dwayne Allen Day's excellent article on this: http://www.thespacereview.com/article/3390/1 The eventual decision was to modify the mission of KH-11 to incorporate that of Hexagon. This was accomplished, at least in part, by raising its highest altitude to about 1000 km, which afforded a wider view, but with resolution reduced to 28 cm (1 foot) - roughly that of Hexagon. The lowest altitude remained 250 km, which preserved its best resolution of 7 cm (3 inches). USA 6 was the first KH-11 to employ the higher altitude orbit. Launched in Dec 1984, it was the first of what I call the Block 2 KH-11. Whether its design was changed to facilitate the wide-area mission is unknown. USA 6 initially operated in a 700 km apogee orbit, which it raised to 1,000 km during summer and fall 1985. The 250 X 1000 km orbit remains the primary KH-11 orbit to this day. This information comes from hobbyist satellite observers and orbital analysts, who are the sole public source of precise orbital elements of these satellites. 4. Future 4.1 Commercial satellites for wide-area surveillance A quick search of the web reveals that the NGA (National Geospatial Agency) has been purchasing commercial satellite imagery since at least 2003, and has signed contracts worth many billions of dollars since then. The U.S. government regulates the resolution of imagery sold by commercial imaging satellite owners. As the best resolution permitted to be sold improved, so did the satellites. DigitalGlobe claims panchromatic 31 cm resolution from 617 km altitude, for its Worldview 3 and 4 satellites, launched in 2014 and 2016, respectively. This means that commercial satellites have now achieved approximately the resolution of the Hexagon satellite, that KH-11 replaced by raising its apogee to 1000 km. This appears to create the opportunity for KH-11 to return to its original, exclusively high-resolution imaging mission, by returning to the pre-1985 maximum apogee of 500 km. A couple of older KH-11s have done just that. 4.2 Possible Block 5 clues from KH-11s on extended mission The typical operational life of the early KH-11 was a few years. The Block 3 KH-11, first launched in 1992, extended the operational life to about 15 years. Block 4, first launched in 2001, appears to be capable of similar longevity. One Block 3 and two Block 4 satellites remain in orbit. Modern KH-11s spend roughly the first half of their life on their primary mission, at which time they are replaced by fresh satellites. The old spacecraft continue to operate for several years on extended missions, after which they are de-orbited. At any given time, there are two primary-mission spacecraft, and one or two older extended-mission spacecraft. Observations and orbital analysis by hobbyists, revealed that during 2012-2015, both of the spacecraft on extended missions (USA 161 and USA 186), manoeuvred to lower-altitude orbits, more like those used in the early years of the KH-11 program in the late 1970s and early 1980s. The extended mission would be ideal for experimentation, which led to the hypothesis that the return to a lower orbit was a clue of what to expect from the Block 5 KH-11, with NROL-71 the suspected first launch. It is known that the primary mirror of Block 5 KH-11 is the same diameter as that of the present generation, 2.4 m. Amazingly, this was openly announced: http://spacenews.com/us-intelligence-official-drops-hint-about-next-gen-spy-sat-capability/ Given that the mirror diameter will remain 2.4 m, and the resolution limit imposed by atmospheric turbulence, it is reasonable to assume that the lowest altitude would be about the same as the present, 250 km. The advantage of the reduced maximum altitude - no greater than 500 km - would be more nearly constant resolution during each revolution about the Earth. 4.3 Block 5 KH-11 NROL candidates The only publicly known candidates to launch Block 5 KH-11 satellites are the upcoming NROL-71, and NROL-82, scheduled for 2020. Both are Delta 4-Heavy launches from VAFB. Two of the existing generation of KH-11 were launched by Delta 4-Heavy, but they were designed for the less powerful Titan IV. The payloads of NROL-71 and 82 would be the first that could have been designed to take full advantage of Delta 4-Heavy, perhaps to carry a greater fuel load, which would enable them to operate for a longer time in a 250 km by 500 km, or lower orbit, than previous KH-11s. My confidence that NROL-71 and 82 would launch the first Block 5 KH-11 satellites is based on the following: A. The following 2009 article reported that Lockheed Martin had begun pre-acquisition work on the next generation electro-optical satellite, and was expected to receive the contract in 2011 for a "two-satellite system," that would "be an evolutionary upgrade of the satellites Lockheed Martin has been building for decades." It would have a 2.4 metre diameter primary mirror - same as that of Block 4: https://spacenews.com/us-intelligence-official-drops-hint-about-next-gen-spy-sat-capability/ B. First launch dates in 2018 (NROL-71) and 2020 (NROL-82) seem reasonable for a program begun in 2012. As precedent, consider that Lockheed Martin was awarded the final pair of the Block 4 electro-optical satellites about 2005, and they were launched in 2011 and 2013. C. A budget document leaked by Edward Snowden revealed the start of a new program, Evolved Enhanced CRYSTAL System, with FY12 funding of $1.2 billion, and $1.5 billion in FY13. Assuming (as a guess) average annual spending of $1.3 billion through FY17, the total cost could be nearly $8 billion, or about $4 billion per satellite. D. Electro-optical satellites relay imagery to Earth via SDS (satellite data system, aka Quasar satellites). Historically, the first launches of a new generation of SDS tended to herald a new block of KH-11 satellite. The first two SDS 2 satellites were launched in 1989 and 1990, and the first Block 3 KH-11 satellite was launched in 1992. The first two SDS 3 satellites were launched in 2000 and 2001, and the first Block 4 KH-11 satellite was launched in 2001. The first SDS 4 satellite was launched in 2016 (USA 269 on NROL-61), and the second one in 2017 (USA 279 on NROL-52). We know they are a new generation because optical and radio tracking by my fellow hobbyists revealed a spin-rate in GTO (geo-stationary transfer orbit), consistent with Boeing's BSS-702 or 702HP bus. (The 3rd gen SDS employed Boeing's older HS-601 or 601HP bus, which spun at a different rate in GTO.) The SDS 4 launches in 2016 and 2017 appear to have paved the way for Block 5 KH-11 launches in 2018 and 2020, consistent with the above pattern. E. The Block 4-2 spacecraft has been on its primary mission for more than 7.5 years, the third longest after Block 4-1 (9.3 years) and Block 3-3 (8.84 years); therefore, it probably is about due to be replaced. 5. NROL-71 Pre-launch clues The NOTAMs revealed that the orbit of NROL-71 will indeed be different than that of recent KH-11s. It will enter a 74 deg orbit, instead of the sun-synchronous orbits (SSO) of all previous KH-11s, inclined at approximately 97 deg or 98 deg, depending upon their altitude. I continue to believe that the payload is the first Block 5 KH-11, but it will not orbit in either of the existing standard KH-11 planes. This radical change may be explained by a desire/need for imagery taken under more varied illumination conditions than occur with an SSO. Therefore, the NRO and NGA may have decided to employ an MSSO (Multi Sun-Synchronous Orbit). For my latest ideas and analysis on this and other clues, please see my post of search elements: http://satobs.org/seesat/Dec-2018/0045.html The orbit of NROL-71 almost certainly will be inclined at or near 74 deg. The remaining big question is its orbital dimensions. Will it be the 250 x 1000 km employed since 1985, or have recent improvements in the resolution of commercial imagery enabled the return to the 250 x 500 km pre-1985 orbit? Or will it be something entirely different? Ted Molczan _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-lReceived on Sat Dec 08 2018 - 22:25:11 UTC
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