Chinese Deep Space Network

Last updated

Chinese Deep Space Network
China Emblem PLA.svg
Emblem of the People's Liberation Army
Active1993;31 years ago (1993)
CountryFlag of the People's Republic of China.svg  People's Republic of China
AllegianceFlag of the Chinese Communist Party.svg Chinese Communist Party
Branch PLASSF.svg People's Liberation Army Strategic Support Force
Part ofPeople's Liberation Army Flag of the People's Republic of China.svg  People's Liberation Army
China edcp location map.svg
Red pog.svg
Kashi
Red pog.svg
Jiamusi
Red pog.svg
Kunming
Red pog.svg
Ürümqi
Red pog.svg
Miyun
Green pog.svg
FAST
Blue pog.svg
Qitai
Green pog.svg
21CMA
Green pog.svg
CSRH
Red pog.svg
Tian Ma
Red pog.svg
Sheshan
Chinese Deep Space Network and radioastronomy facilities in China   in use ·  planned ·  radioastronomy facility

The Chinese Deep Space Network (CDSN) is a network of large antennas and communication facilities that are used for radio astronomy, radar observations, and spacecraft missions of China. The CDSN is managed by the China Satellite Launch and Tracking Control Center General (CLTC) of the People's Liberation Army Strategic Support Force Space Systems Department. [1] [2] [3] [4]

Contents

The network was first needed for the lunar mission Chang'e 1, [5] [6] and since has been used to support subsequent missions to the Moon and Mars such as Chang'e 5, and Tianwen-1 missions. Similar deep space networks are run by the United States, Russia, European countries, Japan, and India.

Introduction

Nanshan 25-meter radio telescope at Xinjiang Astronomical Observatory (XAO), Chinese Academy of Sciences. XAO Nanshan 25-m radio telescope 2007-08-22.jpg
Nanshan 25-meter radio telescope at Xinjiang Astronomical Observatory (XAO), Chinese Academy of Sciences.

In principle, a Chinese deep space network has existed since 1993 with the commissioning of the Nanshan 25-meter telescope in the mountains south of Ürümqi. The 25-meter antenna of the Shanghai Astronomical Observatory was then not only able to participate in the Southern Hemisphere VLBI Experiment program, but also to form its own Chinese baseline together with Ürümqi and observe and measure distant objects.

All stations are equipped with high-precision hydrogen maser clocks and connected via powerful communication networks. All stations comply with the provisions of the Consultative Committee for Space Data Systems (CCSDS), so data exchange with the systems of other space agencies is possible despite different technical equipment.

The antennas of Sheshan, Ürümqi, Miyun, Kunming and Tianma can be interconnected to form a national association and in this way form the Chinese VLBI Network (CVN), a VLBI telescope the size of China. The evaluation of the data from the CVN takes place in the VLBI observation base Sheshan of the Shanghai Astronomical Observatory. The facilities in Shanghai and Ürümqi are also integrated into the European VLBI Network (EVN).

Network

Tianma 65-meter radio telescope at Shanghai Astronomical Observatory (SHAO), Chinese Academy of Sciences. Shanghai 65-meter Tianma Radio Telescope.jpg
Tianma 65-meter radio telescope at Shanghai Astronomical Observatory (SHAO), Chinese Academy of Sciences.

In 2007, the network consisted of:

In 2012, improvements were made to support Chang'e 3 and Chang'e 4 Moon missions, including: [7]

The Espacio Lejano Station of the Chinese Deep Space Network. Antena de la CONAE-CLTC Neuquen.jpg
The Espacio Lejano Station of the Chinese Deep Space Network.

In 2014, China and Argentina signed an agreement allowing China to construct the Espacio Lejano Station. [1] [8] The station was built in Neuquén Province, Argentina (~70°W), with a 50 million-dollar investment. The facility, a part of Chinese Lunar Exploration Program, [9] [10] was inaugurated in October 2017. [11] The station is seen by some as a symbol of China's increased role in South America's politics and economy. [12]

Since 2018, China Satellite Launch and Tracking Control General (CLTC) was a customer of the Swedish Space Corporation (SSC), which provided CLTC services, including TT&C for pre-defined civilian satellites within research, Earth observation and weather data as well as for other scientific spacecraft. [13] It was reported by Reuters on 21 September 2020 that SSC decided not to renew its contracts with China to help operate Chinese satellites from SSC's ground stations, or seek new business with China. [14]

In late 2020, the Kashgar ground station was upgraded from one single 35-meter antenna to an antenna array consisting of four 35-meter antennas. The capacity of the new system was equivalent to a 66-meter antenna. [15]

Systems for radio astronomy

Five-hundred-meter Aperture Spherical Telescope (FAST) as seen from above in 2020. FAST Radio Telescope (captured from video).jpg
Five-hundred-meter Aperture Spherical Telescope (FAST) as seen from above in 2020.
Primeval Structure Telescope (PaST), also called 21 Centimeter Array (21CMA). 21-Centimetre Array pods of the Primeval Structure Telescope, pointing to the North Celestial Pole.jpg
Primeval Structure Telescope (PaST), also called 21 Centimeter Array (21CMA).

Radio astronomy, despite using similar large antennas, is a very different field than spacecraft communication. There is no need to transmit, and the receiving bands are chosen for scientific interest.

Planned or under construction stations

Relay satellites

China has several relay satellites of the Tianlian series in geostationary orbits, which can relay data to each other and to the ground, thus enabling communication with spacecraft that have no direct contact with ground stations. The technology of the relay satellites enables intermediate storage of data, a higher bandwidth of data connections, and greater sky coverage. These satellites were originally placed in orbit in 2008 for communication with the Shenzhou spacecraft of the crewed space program. But they are also used for deep-space missions, for example in 2020 for the Mars mission Tianwen-1, where the satellites Tianlian 1B and Tianlian 2A were parked for orbit tracking and the transmission of telemetry data from the probe. [28]

Moon missions

Planetary missions

See also

Related Research Articles

<span class="mw-page-title-main">Very-long-baseline interferometry</span> Comparing widely separated telescope wavefronts

Very-long-baseline interferometry (VLBI) is a type of astronomical interferometry used in radio astronomy. In VLBI a signal from an astronomical radio source, such as a quasar, is collected at multiple radio telescopes on Earth or in space. The distance between the radio telescopes is then calculated using the time difference between the arrivals of the radio signal at different telescopes. This allows observations of an object that are made simultaneously by many radio telescopes to be combined, emulating a telescope with a size equal to the maximum separation between the telescopes.

<span class="mw-page-title-main">NASA Deep Space Network</span> Network of radio communication facilities run by NASA

The NASA Deep Space Network (DSN) is a worldwide network of spacecraft communication ground segment facilities, located in the United States (California), Spain (Madrid), and Australia (Canberra), that supports NASA's interplanetary spacecraft missions. It also performs radio and radar astronomy observations for the exploration of the Solar System and the universe, and supports selected Earth-orbiting missions. DSN is part of the NASA Jet Propulsion Laboratory (JPL).

<span class="mw-page-title-main">Chinese space program</span> Space program of the Peoples Republic of China

The space program of the People's Republic of China is about the activities in outer space conducted and directed by the People's Republic of China. The roots of the Chinese space program trace back to the 1950s, when, with the help of the newly allied Soviet Union, China began development of its first ballistic missile and rocket programs in response to the perceived American threats. Driven by the successes of Soviet Sputnik 1 and American Explorer 1 satellite launches in 1957 and 1958 respectively, China would launch its first satellite, Dong Fang Hong 1 in April 1970 aboard a Long March 1 rocket, making it the fifth nation to place a satellite in orbit.

<span class="mw-page-title-main">Goldstone Deep Space Communications Complex</span> US observatory near Barstow, California

The Goldstone Deep Space Communications Complex (GDSCC), commonly called the Goldstone Observatory, is a satellite ground station located in Fort Irwin in the U.S. state of California. Operated by NASA's Jet Propulsion Laboratory (JPL), its main purpose is to track and communicate with interplanetary space missions. It is named after Goldstone, California, a nearby gold-mining ghost town.

<span class="mw-page-title-main">JAXA</span> Japans national air and space agency

The Japan Aerospace Exploration Agency (JAXA) is the Japanese national air and space agency. Through the merger of three previously independent organizations, JAXA was formed on 1 October 2003. JAXA is responsible for research, technology development and launch of satellites into orbit, and is involved in many more advanced missions such as asteroid exploration and possible human exploration of the Moon. Its motto is One JAXA and its corporate slogan is Explore to Realize.

<span class="mw-page-title-main">HALCA</span> Japanese space radio telescope

HALCA, also known for its project name VSOP, the code name MUSES-B, or just Haruka (はるか) was a Japanese 8 meter diameter radio telescope satellite which was used for Very Long Baseline Interferometry (VLBI). It was the first such space-borne dedicated VLBI mission.

<span class="mw-page-title-main">Haystack Observatory</span> American microwave observatory owned by MIT

Haystack Observatory is a multidisciplinary radio science center, ionospheric observatory, and astronomical microwave observatory owned by Massachusetts Institute of Technology (MIT). It is in Westford, Massachusetts, in the United States, about 45 kilometers (28 mi) northwest of Boston. The observatory was built by MIT's Lincoln Laboratory for the United States Air Force and was called the Haystack Microwave Research Facility. Construction began in 1960, and the antenna began operating in 1964. In 1970 the facility was transferred to MIT, which then formed the Northeast Radio Observatory Corporation (NEROC) with other universities to operate the site as the Haystack Observatory. As of January 2012, a total of nine institutions participated in NEROC.

<span class="mw-page-title-main">Hartebeesthoek Radio Astronomy Observatory</span> Observatory

The Hartebeesthoek Radio Astronomy Observatory (HartRAO) is a radio astronomy observatory, located in a natural bowl of hills at Hartebeesthoek just south of the Magaliesberg mountain range, and about 50 km west of Johannesburg, Gauteng, South Africa. It is a National Research Facility run by South Africa's National Research Foundation. HartRAO was the only major radio astronomy observatory in Africa until the construction of the KAT-7 test bed for the future MeerKAT array in the Meerkat National Park.

<span class="mw-page-title-main">Chinese Lunar Exploration Program</span> Lunar research program (2004 – present)

The Chinese Lunar Exploration Program, also known as the Chang'e Project after the Chinese Moon goddess Chang'e, is an ongoing series of robotic Moon missions by the China National Space Administration (CNSA). The program encompasses lunar orbiters, landers, rovers and sample return spacecraft, launched using the Long March series of rockets. A human lunar landing component may have been added to the program, after China publicly announced crewed lunar landing plans by the year 2030 during a conference in July 2023.

<span class="mw-page-title-main">Wenchang Space Launch Site</span> Launch site

The Wenchang Space Launch Site is a rocket launch site located in Wenchang on the island of Hainan, in China.

<span class="mw-page-title-main">Shanghai Astronomical Observatory</span> Observatory

Shanghai Astronomical Observatory (SHAO), is an astronomical observatory in Shanghai. It has a long history of astrometry and also operates the 25-meter (82 ft) Sheshan radio telescope as part of the Chinese VLBI array and the European VLBI Network (EVN).

The Soviet Deep Space Network is a network of large antennas and communication facilities that support interplanetary spacecraft missions, and radio and radar astronomy observations for the exploration of the Solar System and the universe during Soviet times. It was built to support the space missions of the Soviet Union. Similar networks are run by the USA, China, Europe, Japan, and India.

<span class="mw-page-title-main">Tianwen-1</span> Interplanetary mission by China to place an orbiter, lander, and rover on Mars

Tianwen-1 Chinese: 天问一号 is an interplanetary mission by the China National Space Administration (CNSA) which sent a robotic spacecraft to Mars, consisting of 6 spacecraft: an orbiter, two deployable cameras, lander, remote camera, and the Zhurong rover. The spacecraft, with a total mass of nearly five tons, is one of the heaviest probes launched to Mars and carries 14 scientific instruments. It is the first in a series of planned missions undertaken by CNSA as part of its Planetary Exploration of China program.

<span class="mw-page-title-main">2021 in spaceflight</span> Spaceflight-related events during the year 2021

The year 2021 broke the record for the most orbital launch attempts till then (146) and most humans in space concurrently (19) despite the effects of COVID-19 pandemic.

Tianwen-4, formerly known as Gan De, is a planned Chinese interplanetary mission to study the Jovian system, possibly sharing a launch with a spacecraft which will make a flyby of Uranus.

<span class="mw-page-title-main">Planetary Exploration of China</span> Chinese Solar System exploration program

The Planetary Exploration of China, also known as Tianwen, is the robotic interplanetary spaceflight program conducted by the China National Space Administration (CNSA). The program aims to explore planets of the Solar System, starting from Mars, and will be expanded to Jupiter and more in the future.

<span class="mw-page-title-main">Queqiao relay satellite</span> Chinese satellite

Queqiao relay satellite (Chinese: 鹊桥号中继卫星; pinyin: Quèqiáo hào zhōngjì wèixīng; lit. 'Magpie Bridge relay satellite'), is the first of the pair of communications relay and radio astronomy satellites for the Chinese Lunar Exploration Program. The China National Space Administration (CNSA) launched the Queqiao relay satellite on 20 May 2018 to a halo orbit around the Earth–Moon L2 Lagrangian point Queqiao is the first ever communication relay and radio astronomy satellite at this location.

<span class="mw-page-title-main">Queqiao-2 relay satellite</span> Chinese satellite

Queqiao-2 relay satellite, is a second of the two communications relay and radio astronomy satellites designed to support the fourth phase the Chinese Lunar Exploration Program. The China National Space Administration (CNSA) launched the Queqiao-2 relay satellite on 20 March 2024 to a elliptical frozen orbit around the Moon to support communications from the far side of the Moon and the Lunar south pole.

References

  1. 1 2 "Eyes on the Skies: China's Growing Space Footprint in South America". Center for Strategic and International Studies . 4 October 2022. Archived from the original on 5 October 2022. Retrieved 4 October 2022.
  2. "China Satellite Launch and Tracking Control General (CLTC)". Nuclear Threat Initiative. 31 January 2013. Archived from the original on 26 May 2021. Retrieved 23 June 2021.
  3. Dinatale, Martín (8 September 2014). "Preocupa el eventual uso militar de un área espacial de China en el Sur". La Nación (in Spanish). Archived from the original on 5 September 2017. Retrieved 23 June 2021.
  4. Garrison, Cassandra (31 January 2019). "China's military-run space station in Argentina is a 'black box'". Reuters . Archived from the original on 25 January 2022. Retrieved 25 January 2022.
  5. Xie, Renjiang (14 February 2007). "Gearing up for Chang'e". Astronomy. Archived from the original on 16 March 2012. Retrieved 23 June 2021.
  6. Yan, Jianguo; Ping, Jing-Song; Li, Fei (2008). Precise orbit determination of Smart-1 and Chang'E-1. 37th COSPAR Scientific Assembly. Bibcode:2008cosp...37.1381J.
  7. "China Builds Deep Space Network" (PDF). China Science and Technology Newsletter. No. 606. 10 January 2011. Archived from the original (PDF) on 27 September 2011. Retrieved 21 June 2011.
  8. Watson-Lynn, Erin (9 June 2020). "The gravity of China's space base in Argentina". The Interpreter. Lowy Institute. Archived from the original on 11 May 2021. Retrieved 23 June 2021.
  9. "Chinese space station is "for exclusively scientific and civilian purposes": Argentine gov't". Xinhua News Agency. 30 June 2015. Archived from the original on 2 July 2015.
  10. Lee, Victor Robert (24 May 2016). "China Builds Space-Monitoring Base in the Americas". The Diplomat. Archived from the original on 10 February 2020. Retrieved 23 June 2021.
  11. Dinatale, Martín (28 January 2018). "Tras la polémica por su eventual uso militar, la estación espacial de China en Neuquén ya empezó a funcionar". Infobae (in Spanish). Archived from the original on 29 October 2020. Retrieved 2 June 2018.
  12. Londoño, Ernesto (28 July 2018). "From a Space Station in Argentina, China Expands Its Reach in Latin America". The New York Times. Archived from the original on 1 May 2020. Retrieved 23 June 2021.
  13. "Appendix for SSC's Chinese customers" (PDF). Swedish Space Corporation. Archived from the original (PDF) on 18 June 2020. Retrieved 21 September 2020.
  14. Ahlander, Johan; Barrett, Jonathan (21 September 2020). "Swedish space agency halts new business helping China operate satellites". Reuters. Archived from the original on 21 September 2020. Retrieved 21 September 2020.
  15. Li, Guoli; Lü, Binghong (18 November 2020). "我国首个深空天线组阵系统正式启用" (in Chinese (China)). Xinhua News Agency. Archived from the original on 3 June 2021. Retrieved 29 May 2021.
  16. Jin, C.; Cao, Y.; Chen, H.; Gao, J.; Gao, L.; Kong, D.; Su, Y.; Wang, M. (2006). "The Miyun 50 m Pulsar Radio Telescope". Chinese Journal of Astronomy and Astrophysics. 6: 320. doi: 10.1088/1009-9271/6/S2/59 . S2CID   120782642.
  17. Zhang, X.Z.; Piao, T.Y.; Kang, L.S.; Pang, L. (2002). Pramesh Rao, A.; Suiarup, G.; Gopal-Krishna (eds.). "Solar Observation with Miyun Radio Telescope". The Universe at Low Radio Frequencies IAU Symposium. 199: 430–431. Bibcode:2002IAUS..199..430Z. doi: 10.1017/S0074180900169517 . S2CID   118095827.
  18. 2020中国火星探测计划(根据叶院士报告整理). spaceflightfans.cn (in Chinese (China)). 14 March 2018. Archived from the original on 4 November 2019. Retrieved 23 June 2021.
  19. Sarkissian, John (6 August 2012). "The Parkes MSL EDL Track". CSIRO Parkes Observatory. Archived from the original on 21 December 2022. Retrieved 23 June 2021.
  20. Esterhuizen, S.; Asmar, S. W.; De, K.; Gupta, Y.; Katore, S. N.; Ajithkumar, B. (March 2019). "ExoMars Schiaparelli direct-to-earth observation using GMRT". Radio Science. 54 (3): 314–325. Bibcode:2019RaSc...54..314E. doi: 10.1029/2018RS006707 .
  21. Dong, Guangliang; Li, Haitao; Hao, Wanhong; Wang, Hong; Zhu, Zhiyong; Shi, Shanbin; Fan, Min; Zhou, Huan; Xu, Dezhen (April 2018). 中国深空测控系统建设与技术发展 [Development and Future of China's Deep Space TT&C System]. Journal of Deep Space Exploration (in Chinese (China)). 5 (2): 99–114. doi:10.15982/j.issn.2095-7777.2018.02.001. Archived from the original on 24 June 2021. Retrieved 23 June 2021.
  22. Morabito, David D.; Schratz, Brian; Bruvold, Kris; Ilott, Peter; Edquist, Karl; Cianciolo, Alicia Dwyer (15 May 2014). "The Mars Science Laboratory EDL Communications Brownout and Blackout at UHF" (PDF). The Interplanetary Network Progress Report. 42–197: 1–22. Bibcode:2014IPNPR.197A...1M. Archived (PDF) from the original on 25 January 2021. Retrieved 17 February 2021.
  23. "The 21 CentiMeter Array (21CMA)". National Astronomical Observatories, Chinese Academy of Sciences. Archived from the original on 19 June 2021. Retrieved 23 June 2021.
  24. Zheng, Qian; Wu, Xiang-Ping; Johnston-Hollitt, Melanie; Gu, Jun-Hua; Xu, Haiguang (1 December 2016). "Radio Sources in the NCP Region Observed with the 21 Centimeter Array". The Astrophysical Journal. 832 (2): 190. arXiv: 1602.06624 . Bibcode:2016ApJ...832..190Z. doi: 10.3847/0004-637X/832/2/190 . S2CID   118551520.
  25. O'Callaghan, Jonathan (17 January 2018). "China To Build The World's Largest Steerable Radio Telescope By 2023". IFLScience. Archived from the original on 21 April 2021. Retrieved 11 February 2018.
  26. Atkinson, Nancy (24 January 2018). "China Plans to Build the World's Largest Steerable Radio Telescope". Seeker. Archived from the original on 15 October 2021. Retrieved 11 February 2018.
  27. Mack, Eric (17 January 2018). "New biggest radio telescope to help detect alien signals". CNET. Archived from the original on 21 April 2021. Retrieved 23 June 2021.
  28. Li, Guoli; Wang, Ran (21 July 2020). "我国天基测控系统团队完成多项技术状态准备静待天问一号发射" (in Chinese). Xinhua News Agency. Archived from the original on 22 July 2020. Retrieved 23 June 2021.
  29. "Chang'e-1 – new mission to Moon lifts off". European Space Agency. 24 October 2007. Archived from the original on 16 October 2012. Retrieved 24 October 2007.
  30. "China's second moon orbiter Chang'e-2 sends data from 1.7 mln km away". Xinhua News Agency. 21 September 2011. Archived from the original on 26 September 2011. Retrieved 23 June 2021.
  31. Gray, Bill (25 August 2012). "Chang'e 2: The Full Story". The Planetary Society. Archived from the original on 26 August 2012.
  32. Jones, Andrew (23 July 2020). "Tianwen-1 launches for Mars, marking dawn of Chinese interplanetary exploration". SpaceNews. Archived from the original on 10 November 2022. Retrieved 23 July 2020.
  33. Roulette, Joey (5 February 2021). "Three countries are due to reach Mars in the next two weeks". The Verge. Archived from the original on 5 February 2021. Retrieved 7 February 2021.