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Spektr-R


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The author would like to thank Christian Cognard for editing this story.

Spektr-RG to expand horizons of X-ray astronomy

Conceived as one of three Soviet "great observatories" at the end of the 1980s, the Spektr-RG could become the main window on the Universe for the nation's astronomers. However, economic storms of the post-Soviet transition were continuously delaying and crippling the project.

Spektr RG

Above: A Spektr-RG observatory. Copyright © 2010 Anatoly Zak

Previous chapter: Spektr-R observatory

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Origin of Spektr-RG project

A brainchild of the astronomical section of the Soviet Academy of Sciences, Spektr-RG (where RG stands for Roentgen-Gamma) was designed for astrophysics research. The project was proposed by Academician Rashid Syunyaev, who previously led a team of scientists working with astronomical payload of the Kvant module onboard the Mir space station. According to one of the project veterans, the concept of the spacecraft was first formulated at a scientific symposium in 1987, which was dedicated to the 30th anniversary of the First Artificial Satellite. Along with Syunyaev, Soviet scientists Yakov Zeldovich and Roald Sagdeev stood at the roots of the project.

By mid-1990s, the Spektr-RG program involved a wide international cooperation, including 20 organizations from Denmark, UK, Germany, Italy, US, Finland, Switzerland, Israel, Hungary, Kyrgyzstan, Canada and Turkey.

The 6,000-kilogram spacecraft would carry 2,750 kilograms of scientific instruments, including five telescopes: SODART, JET-X, MART-LIME, FUVITA, TAUVEX, as well as all-sky monitors MOXE in SPIN sensitive to X-ray and gamma radiation. The Proton rocket had to carry Spektr-RG into a highly elliptical orbit with an apogee of 200,000 kilometers above the Earth surface, a perigee of 500 kilometers and an inclination 51.6 degrees toward the Equator. There, the satellite could work up to 80 hours at a time, free of interference from the Earth's radiation belts. It would take the satellite four days to complete a single orbit. The spacecraft could be pointed at up to 10 different targets a day. (403)

Despite considerable political pressure from international partners, including the weight of the Gore-Chernomyrdin agreements on space cooperation between Russia and the United States, the cash-strapped Russian government ultimately failed to fund the project. With much of science instruments and other hardware manufactured and tested, its launch date kept slipping from 1996 to 1997, 1998, 1999, 2000, 2002 and 2003, before the project was finally declared dead in February 2002. As early as 1998, Western partners spent $300 million on their participation in three Spektr observatories, with most of these funds going to Spektr-RG. As a "compensation" for the losses by foreign partners, the Russian government offered a Proton rocket to launch a similar European space telescope, known as Integral. Even some of the Russian scientists, who participated in the Spektr-RG project decided to "jump the ship" and banked on the European observatory instead. ESA provided Russian partners 25 percent of available observation time onboard Integral. (402) Ironically, the European spacecraft was launched without problems or considerable delays in 2002.

Rebirth of Spektr-RG

Developers of sophisticated payloads for the original Spektr-RG had to find new carriers for their instruments or surrender them to museums. Yet, with the improvement of Russian financial situation in the first decade of the 21st century, Spektr-RG was reborn as a smaller, cheaper project. Once the highest priority for launch among Russian space observatories, Spektr-RG was moved behind the Spektr-R (Radioastron) project. Both satellites were redesigned to use NPO Lavochkin's new standard spacecraft bus, known as Navigator. It would play a role of the service module for Spektr-RG and other space observatories.

In 2005, Roskosmos and ESA started discussion about possible installation of a pair of European instruments on Spektr-RG. These included a German ROSITA (Roentgen Survey with an Imaging Telescope Array) and the British Lobster Eye, LE, an all-sky X-ray monitor. Both of these instruments were originally considered for installation on the European Columbus module of the International Space Station, ISS. However concerns over the contamination of sensitive optics in the polluted environment around the ISS coupled with the premature demise of the Space Shuttle program killed these plans. To resolve the problem, the International Working Group was formed, involving representatives from the Moscow-based Space Research Institute, Germany's Max Planck Institute, University of Leicester in England, as well as from the European, Russian and German space agencies. The group evaluated various ways to cluster available payloads and, at one point, considered incorporating a yet another telescope built by a US-Japanese-Dutch team. However, ultimately, even the LOBSTER instrument had to be dropped from the project, due to lack of funding on the British side.

Finally, a Memorandum of Understanding between Roskosmos and the German Space Agency, DLR, was signed in March 2007, followed by the "Detailed Agreement," finalized at the Moscow Air and Space Show, MAKS, in August 2009. Thus, Spektr-RG became a joint Russian-German project, with a projected launch date in 2012.

Launch opportunities

The original plan was to launch a 2,000-kilogram satellite in 2011, onboard the Soyuz-2/Fregat booster into a 500-580-kilometer circular orbit with an inclination 28 degrees toward the Equator, following a liftoff from Kourou, French Guiana. Later, a Baikonur-based launch into a 600-kilometer orbit with an inclination 30 degrees was considered. Yet by 2008, a Zenit rocket, also with Fregat was deemed affordable. (By the spring of 2012, the issue remained open whether a regular Fregat or Fregat-SB version of the upper stage would be used.)

Planning a path to orbit

According to initial plans, Zenit-2SLBF/Fregat-SB would carry the 2,400-kilogram Spektr-RG spacecraft into a highly elliptical orbit around the Earth with a perigee of 491 kilometers, an apogee of 411,490 kilometers and an inclination 51.4 degrees toward the Equator. From there, Spektr-RG would use its own propulsion system and a gravitational pull of the Moon to reach a "halo" orbit around the L2 (Lagrange) point. However by mid-2012, this scenario was reportedly dropped in favor of a direct flight to the L2 point. In the absence of a reliable X-band trajectory measurement system, which engineers never had a chance to test during the ill-fated Phobos-Grunt mission, planners preferred to spend more time and propellant on the direct flight. Such trajectory would give mission control more time to assess the actual path of the spacecraft after the launch and to calculate the amount of orbit correction necessary for reaching the final destination. Planners estimated that three or four orbit corrections would be required during the mission.

In any case, Spektr-RG would likely be the first Russian (or Soviet) spacecraft reaching any of the Lagrange points, which considered as carrying great potential for new-generation scientific missions and, lately, as a destination for manned space flight (at least those around the Moon) and even competing with such traditional goals of astronauts and cosmonauts as bases on the Moon and expeditions to Mars. According to sources at Keldysh Applied Mathematics Institute, IPM, which plans trajectories of Russian space missions, a favorable launch window conserving the most of the propellant on a direct flight for Spektr-RG would open on Dec. 30, 2014.

The L2 (Lagrange) libration point behind the Earth relative to the Sun would be an ideal spot for the Spektr-RG mission. This celestial "neighborhood" provides "quiet" gravitational and magnetic conditions for the spacecraft without many disturbances and no traces of thin air slowing down the spacecraft in the low Earth orbit. Only miniscule "pressure" of light particles is expected to require a monthly action of the attitude control system.

The spacecraft would need around three months (116 days) to reach its final destination, where it was expected to spend at least four years circling L2 in a 40,000-kilometer ellipse on a mission to conduct a global survey of the sky. Three following years would be spent observing particular objects. (589) This flight trajectory located 1.5 million kilometers from Earth would essentially make Spektr-RG a deep-space mission, along with the Spektr-R radio telescope launched in 2011.

A project presentation made at the end of 2013, indicated that Fregat-SB would use two firings within 1.6 hours after launch to send Spektr-RG into an orbit with a lowest point (perigee) at an altitude of 1,020 kilometers and a highest point extending all the way to 1,415,510 kilometers from Earth -- essentially near the target Lagrange point. An empty external tank would be jettisoned during an interval between two firings. The transfer to the L2 point would last between 70 and 80 days.

Scientific mission

The scientific payload of Spektr-RG was ultimately limited to two instruments -- a 810-kilogram eRosita developed at Max Planck Institute for Extraterrestrial Physics in Munich, Germany, and a 350-kilogram Russian ART-XC telescope developed by the VNIIEF nuclear research center in the city of Sarov.

Despite its only two payloads, project scientists promised a revolutionary data in the field of the so-called high-energy astrophysics. Unlike previous orbital X-ray telescopes, such as European XMM Newton and NASA's AXAF Chandra, which were equipped with instruments with narrow angles of view, Spektr-RG would enable a wide-angle survey of the sky. Germany's eRosita, (where "e" stood for "extended" denoting much larger and powerful instrument than the originally proposed version), promised a wide-angle view at the entire range of its sensitivity and ART-XC at low-energy levels. Thus, the spacecraft could be used to compile a global map of X-ray sources, such as black holes, neutron stars and white dwarfs. According to Mikhail Pavlinsky, Deputy Director of Moscow-based Space Research Institute, IKI, Spektr-RG's eRosita would deliver sensitivity and survey depth 30 times greater than it would be possible with previous instruments. Telescope eRosita will be sensitive to electromagnetic waves from 0.3 to 10 keV and ART-XC will be registering from 6 to 30 keV.

A resulting catalog of X-ray sources could include a comprehensive list of galaxy clusters, which had formed since the formation of the Universe. For example, the German team had established a goal for eRosita to detect mind-boggling 100,000 clusters of galaxies, which are the largest known astronomical entities in the Universe bound by gravity. Such a comprehensive survey would enable to assess an evolution of the Universe and to calculate key cosmological phenomena, such as the Dark Energy. In addition, the instrument would enable to detect as many as 700,000 stars and three million of super-massive Black Holes throughout the entire Universe.

Spektr-RG could also detect radiation emitted by hot gas from "Dark Matter" sources, enabling to map the distribution of this mysterious substance around the Universe. (441)

It was expected that the spacecraft would spend first four years of its mission conducting a global survey of the entire sky and following three years watching small remote targets such as individual galaxies.

Potential challenges to scientific priority of Spektr-RG

Despite unique capabilities of Spektr-RG's instruments, the Russian astrophysicist S. B. Popov noted that scientific results of the observatory's mission could be diminished by delays of its launch beyond 2014. For example, potential discoveries in the field of cosmological models and large-scale structures in the Universe could be achieved with alternative instruments operating in far-infrared or sub-millimeter range of spectrum. Such data could be obtained with the European Planck orbital observatory or even with some powerful ground-based telescopes, such as South Pole Telescope.

Spacecraft development

An improved funding of the Russian space program after 2005 finally gave some confidence to developers that Spektr-RG would eventually fly. Still, the overall poor state of the Russian space science program, particularly problems in the construction of the hardware and payloads, kept pushing the launch date for the "reborn" Spektr-RG years behind schedule. Some "unfeasible ideas" in the configuration of the spacecraft were also cited by project sources as reasons for delays.

In 2004, the launch was promised in 2006, then it was delayed to the end of 2007 and to 2008. In 2008, the launch was set for Nov. 20, 2011.

As of August 2009, the earliest possible launch date for Spektr-RG was considered at the end of 2012, however by December 2010, it was likely to slip to the first quarter of 2013. (441) At the beginning of March 2011, the mission was promised to lift off in September 2013, however by December of the same year, the launch was set for Nov. 13, 2013. According to NPO Lavochkin, a three-day launch window would be available every three days.

Communications challenges

Following the Phobos-Grunt launch fiasco, all planetary exploration and science projects in Russia faced uncertain future. The mission to Phobos was to test an X-band deep-space communications system for Spektr-RG. Following the loss of the spacecraft, NPO Lavochkin considered trials of the X-band package on a small-size MKA-FKI satellite (the second or third satellite in the MKA series). Combined with delays in the delivery of Spektr-RG's scientific instruments, the launch date for the observatory slipped to 2014.

In November 2012, a representative of IKI's high-energy astrophysics department Mikhail Pavlinsky told RIA Novosti that the radio-systems onboard Spektr-RG would be re-worked to make them compatible with Western ground stations, which could back up the Russian ground control.

Building hardware

In the meantime, ISS Reshetnev in Zheleznogorsk revealed its work on the contract with NPO Lavochkin on the development of a guiding mechanism for the high-gain antenna on Spektr-RG and Luna-Glob missions. The flight version of the guiding mechanism for the antenna on Spektr-RG was scheduled for delivery to Lavochkin in 2013, ISS Reshetnev said. The same company was also building solar panels for the spacecraft.

By the spring of 2012, the VNIIEF nuclear center in the town of Sarov manufactured and tested a full-scale mass and thermal prototype of the main telescope and was working on the second (engineering) prototype of the device. A representative of the center Dmitry Litvin promised to start the construction of a fully functional ground equivalent as well as the flight version of the instrument before the end of the year. (568)

At the end of May 2012, the schedule called for the vibration tests of the Spektr-RG engineering model equipped with development mockups of main instruments to start in June or July. At the same time, development versions of Russian and German telescopes for Spektr-RG were scheduled for delivery in June and September respectively to pave the way for integrated tests. Vibration trials would be followed by electrical tests also before the end of 2012. In the meantime, the shipment of the flight version of the German-built eRosita telescope to Russia was planned for June 2013, followed by the delivery of Russian-built ART-XC in October of the same year. This timeline would enable the launch of the mission in the fall of 2014.

In September 2012, NPO Lavochkin finally published its first press-release on the status of the Spektr-RG project, announcing that it had currently conducted testing of the antenna system on the prototype of the spacecraft. According to the company, a prototype of the spacecraft for testing of its structural strength and design was manufactured. Static and transportation tests had been completed and vibration tests had been underway, Lavochkin said. In parallel, testing of the thermal-control system had been completed on the flight prototype of the spacecraft, while the assembly of another "prototype for flight testing" had been underway, Lavochkin said. The company also announced that Space Research Institute, IKI, in Moscow had manufactured the technical version of the ART-XC telescope for the spacecraft and was preparing to ship it to NPO Lavochkin. The press-release was accompanied by an undated and uncaptioned photo apparently showing one of the prototypes of the Spektr-RG observatory.

Mechanical tests of the observatory were conducted from September to December 2012.

Speaking at a conference on astrophysics in December 2012, Mikhail Pavlinsky, Deputy Director for Science at Moscow-based Space Research Institute, IKI, and the head of high-energy astrophysics department, said that the project had been moving forward quite slowly and the launch date for the mission had moved to the third quarter of 2014. Final tests of the spacecraft were scheduled for April 2014. At the same conference, a leading engineer at NPO Lavochkin Ilya Lomakin promised the delivery of the spacecraft to the launch site in the third quarter of 2014 and the launch in the fourth quarter of the same year.

Developments in 2013

By the end of May 2013, new problems required to postpone the launch of Spektr-RG from the end of 2014 to 2015. On the Russian side the biggest obstacle was presented by an X-band radio communications system for the spacecraft. According to project sources, NPO Lavochkin was considering to switch from a movable High-Gain Antenna on the spacecraft to a less-capable Medium-Gain Antenna.

On July 16, NPO Lavochkin announced that the service module for the observatory had been fully assembled with all its hardware for the exception of the radio complex, which was represented by a test version. The systems went through radio and electric tests at the company's test and checkout station, KIS. The test version of the Russian ART-XC telescope and an electric prototype of the eRosita telescope were going through initial acceptance tests, the company said. NPO Lavochkin was also completing a clean room facility to handle flight version of scientific payloads for Spektr-RG.

In the meantime, in Germany, developers hit a major problem during the integration of around 60 circuit boards with up to 30,000 individual components on the eRosita telescope. The latest tests reportedly uncovered previously unknown incompatibility between programmable radiation-resistant electronics and regular circuit boards, requiring a major redesign of onboard electronics, which would take at least a year and a half. As a result by July of 2013, the German team made a decision to postpone the delivery of flight version of eRosita to NPO Lavochkin from December 2013 until June 2015. The head of NPO Lavochkin Viktor Khartov publicly confirmed the delay at the end of August.

As of October 2013, electrical interface tests on eRosita were yet to be performed. Nevertheless by November 11, the German team integrated last of 432 mirror shells, completing seven Flight Mirror Modules of eRosita and one Spare Module.

Developments in 2014

On April 9, the Council of Chief Designers, which oversees the Spektr-RG project, reviewed the latest status of the observatory's development. The delivery of flight versions of German eRosita telescope and the Russian ART-XC telescope was set for July-October 2015, making it possible to launch the observatory in the first quarter of 2016, if no other major problems interfere with the schedule.

Around the same time, the Applied Mathematics Institute, IPM, of the Russian Academy of Sciences, which is traditionally tasked with calculating trajectories of the Russian space missions, published eight possible launch dates for the Spektr-RG from March 15, 2016, until June 30, 2016. Within this launch window, the spacecraft could be launched on the 15th and 30th of each month, according to IMP. As of June 2014, the launch of Spektr-RG was scheduled for March 26, 2016.

2015: Spektr-RG slips to 2017

At the beginning of 2015, a combination of technical problems required to postpone the launch of Spektr-RG from 2016 to March 2017. However even the new launch date stayed on the books only until around August 2015.

In February 2015, scientists involved into the Spektr-RG project reviewed the status of the Russian-built ART-XC telescope for the observatory. Another meeting, which involved the Russian-German team took place at NPO Lavochkin on May 12. The development of the scientific instruments was moving forward, but still not fast enough to keep up with the existing schedule. As of June, the delivery of the flight-worthy ART-XC instrument was apparently not expected until March 2016, at the earliest.

In the meantime, in Germany, engineers at the Max Planck Institute also faced technical challenges with the completion of the eRosita telescope. By August, flight versions of all mirrors, flight cameras, filter wheels and the complete structure and the cooling system for eRosita were finally delivered. Around 90 percent of necessary electronic components was also in place, however, Russian media reported problems in obtaining US-built components, which could become the subject of anti-Russian sanctions in the wake of the conflict with Ukraine.

By the end of the summer, the final calibration of the eRosita's mirrors was planned to be completed by November 15. In parallel, engineers were also assembling cameras with filter wheels and electronics, which also had to be calibrated along with their respective mirrors. Following the calibration process, each mirror-camera pair had to be integrated into the eRosita telescope. If everything went as scheduled, the instrument would be fully integrated around Christmas of 2015, followed by a series of end-to-end tests. However, the delivery of the eRosita to Russia had to be postponed from October 2015 to February 2016.

As with many other projects led by NPO Lavochkin, the scientific team providing instruments for the Spektr-RG observatory had little insight into the overall progress with the spacecraft itself. The situation was further confused by the official Russian media which tended to quote statements from Russian industry officials without any scrutiny shifting the blame for the delays in the project to international partners.

What is clear is that, NPO Lavochkin completed the assembly of the spacecraft prototype for electric and radio tests, collectively known as ERTI. Engineers also used it for the testing of the flight software. In June, RIA Novosti quoted an official at NPO Lavochkin as saying that the "first phase" of electrical tests on the Spektr-RG spacecraft had been completed. The statement indicated that the service module of the spacecraft was electrically integrated with test prototypes of scientific instruments.

By the end of 2015, the launch of Spektr-RG was postponed from the first quarter of 2017 to Sept. 25, 2017. To meet this launch date, the assembly of the spacecraft would have to be completed by July 2017, according to the head of NPO Lavochkin Sergei Lemeshevsky as quoted by RIA Novosti in December. At the time, the delivery of eRosita and ART-XS instruments was expected in April and May 2016.

There was also a potential issue with the launch of Spektr-RG on a Zenit rocket, due to Russia's conflict with Ukraine, where the launcher had been built. Although the rocket for the Spektr-RG mission was already in storage at the Russian launch site in Baikonur, Kazakhstan, the cooperation of Ukrainian specialists would be required for the successful launch campaign. Fortunately, in December 2015, the Russian-Ukrainian team demonstrated seemingly flawless performance, successfully launching the Elektro-L2 satellite on the Zenit.

Last but not least, the financial health of the project had to be ensured given the severe financial crisis in the Russian economy. Thanks to a mature state of the Spektr-RG, it emerged from the budget cuts relatively unscathed. The final version of the Federal Space Program covering the period from 2016 to 2025, which was approved at the end of 2015, allocated a total of 5,609 million rubles for the Spektr-RG project (approximately $72.76 million as of February 2016). This relatively modest amount had cover the work on the project from 2016 through the seven-year life span of the observatory in orbit until 2024:

The approved budget for the Spektr-RG project, (as of December 4, 2015):

Annual budget
Total
In millions of rubles
693.0
1,000.0
460.0
500.0
530.0
550.0
600.0
630.0
646.0
5,609.0

In addition, 28 million and 43 million rubles ($0.36 million and $0.56 million) were allocated for the launch activities of the Spektr-RG project in 2016 and 2017 respectively, which would culminate with the liftoff on the Zenit-M rocket from Baikonur.

2016: Final assembly to begin

In January 2016, NPO Lavochkin announced that the assembly of the Spektr-RG observatory would begin in the first quarter of the year. According to the company, the flight version of the spacecraft was undergoing electric and radio tests, collectively known as ERTI. NPO Lavochkin also reported that the fueling and size prototype of the spacecraft successfully completed tests in Baikonur, which revealed no need for design changes. The delivery of the two main instruments for the observatory was then expected in the second quarter of the year.

A prototype for the Russian-built ART-XS telescope was also undergoing a series of tests, while components of the flight version were in final stages of production, NPO Lavochkin said. The delivery of the ART-XS was expected in May.

Soon thereafter, Roskosmos released footage showing the preparations of the the Spektr-RG spacecraft at NPO Lavochkin. The Chief Designer of the project Vladimir Babyshkin, was quoted as saying that the flight version of the observatory temporarily equipped with test versions of its instruments and radio system, was undergoing electrical tests.

In the meantime, engineers at the Max Planck Institute in Germany were completing the final calibration of the eRosita instrument, before its delivery to Russia sometimes after April 2016.

Next chapter: Spektr-UF observatory

 


APPENDIX

Evolution of the Spektr-RG mission:

- as of 2009 as of 2012 as of 2014 as of 2015
Launch year 2012 (The 2013 was considered as more realistic) 2014 2016 March 26 2017 Sept. 25
Spacecraft mass 2,400 kilograms 2,385 kilograms (dry mass: 2,115 kg) - -
Payload mass 1,100 kilograms 1,100 kilograms - -
Payloads eRosita and ART-XC X-ray telescopes eRosita and ART-XC X-ray telescopes eRosita and ART-XC X-ray telescopes eRosita and ART-XC X-ray telescopes
Spacecraft bus (platform) Navigator Navigator Navigator Navigator
Projected mission lifetime From three to seven years 7.5 years 7.5 years No less than 7 years
Electrical power available for the payload 680 Watts nearly 700 Watts - -
Onboard propellant mass ? 360 kilograms - -
Launch vehicle Zenit or Soyuz-2-1b with Fregat upper stage Zenit with Fregat or Fregat-SB Zenit with Fregat or Fregat-SB -
Operational orbit L2 Libration point (approximately 1.5 million kilometers from Earth) in the Sun-Earth system L2 Libration point in the Sun-Earth system L2 Libration point in the Sun-Earth system -

 

Specifications of science instruments onboard Spektr-RG (589):

- eRosita ART-XC
Sensitivity range 0.3 - 10 keVolts 6 - 30 keVolts
View angle 1 degree 30 minutes
Angular resolution 15 seconds 45 seconds
Sensor area 2,400 square centimeters per 1 keVolts 450 square centimeters per 8 keVolts
Mass 810 kilograms ?

 

Spektr-RG development team:

Organization Location Role in the project
NPO Lavochkin Moscow Prime contractor
VNIIEF nuclear research center Sarov ART-XC X-ray telescope
Max Planck Institute Germany eRosita telescope
ISS Reshetnev Zheleznogorsk A guiding mechanism of the high-gain antenna, solar panels

 

Expected total targets cataloged by Spektr-RG:

Galaxy clusters
100,000
Active galactic cores (super-massive black holes)
3,000,000
Stars emitting in X-ray range
500,000
White dwarfs
more than 100,000

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Writing and photography by Anatoly Zak

Last update: February 2, 2016

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IMAGE ARCHIVE

Spektr

The original architecture of the Spektr-RG spacecraft planned during 1990s. Credit: IKI


JET-X

Spektr-RG's sophisticated JET-X telescope became a museum exhibit. Click to enlarge. Copyright © 2010 Anatoly Zak


yamal

One proposed architecture of the Spektr-RG observatory was based on the Yamal communications satellite. Credit: IKI


early

The second incarnation of the Spektr-RG observatory intended for launch on the Soyuz rocket. Credit: NPO Lavochkin


orbit

The final design of the Spektr-RG observatory. Credit: NPO Lavochkin


Spektr RG

A one-to-four model of the Spektr-RG satellite. Click to enlarge. Copyright © 2010 Anatoly Zak


eRosita

A European-built eRosita telescope designed for the Spektr-RG mission. Click to enlarge. Copyright © 2009 Anatoly Zak


eRosita

A general layout of the eRosita instrument. Credit: Max Planck Institute


transparent

A general layout of the ART-XC instrument. Credit: IKI


Navigator bus

A hexagon-shaped Navigator spacecraft bus was expected to serve as a base of the Spektr-RG mission. Credit: IKI


L2

The Spektr-RG observatory is expected to watch the Universe from the L2 position located "behind" the Earth relative to the Sun as illustrated in this graphic. Credit: Credit: Max Planck Institute


assembly

A prototype of the Spektr-RG satellite under assembly circa 2009. Credit: NPO Lavochkin


RG

A photo released on Sept. 18, 2012, apparently showed one of the full-scale prototypes of the Spektr-RG observatory. Credit: NPO Lavochkin


e-Rosita

The assembly of eRosita telescope circa 2012. Credit: Max Planck Institute


ART

The ART-XC telescope during testing circa 2012. Credit: Max Planck Institute


testing

A footage released at the beginning of 2016, shows what appears to be a test prototype of the Russian-built ART-XC telescope electrically connected to the Navigator service module (right). Click to enlarge. Credit: Roskosmos


 

 

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