Share to: share facebook share twitter share wa share telegram print page

Spektr-R

Spektr-R
Спектр-Р
Spektr-R at the integration and test complex of Launch Pad No.31, the Baikonur Space Center in July 2011
NamesRadioAstron
Mission typeRadio telescope
OperatorRussian Astro Space Center
COSPAR ID2011-037A Edit this at Wikidata
SATCAT no.37755
Websitehttp://www.asc.rssi.ru/radioastron/
Mission durationPlanned: 5 years
Achieved: 7 years, 10 months, 11 days
Spacecraft properties
BusNavigator[1]
ManufacturerNPO Lavochkin
Launch mass3,660 kg (8,069 lb)[1]
Payload mass2,500 kg (5,512 lb)[1]
Start of mission
Launch date18 July 2011, 02:31 (2011-07-18UTC02:31) UTC[2]
RocketZenit-3F[3][4]
Launch siteBaikonur Cosmodrome Pad 45/1[2]
ContractorRoscosmos
End of mission
DisposalEquipment failure
Declared30 May 2019
Last contact11 January 2019
Orbital parameters
Reference systemGeocentric
RegimeHighly elliptical
Semi-major axis180,974.7 km (112,452 mi)
Eccentricity0.905900
Perigee altitude10,651.6 km (6,619 mi)
Apogee altitude338,541.5 km (210,360 mi)
Inclination42.46°
Period12769.93 min
RAAN67.28°
Argument of perigee244.85°
Mean anomaly3.07°
Mean motion0.1126 rev/day
Epoch24 February 2016, 23:21:29 UTC[5]
Revolution no.197
Main telescope
Diameter10 m (33 ft)[1]
Focal length4.22 m (13.8 ft)[1]
Wavelengths92, 18, 6, 1.3 cm[1]
Spektr program

Spektr-R[6] (part of RadioAstron program) (Russian: Спектр-Р) was a Russian scientific satellite with a 10 m (33 ft) radio telescope on board. It was launched on 18 July 2011[7] on a Zenit-3F launcher from Baikonur Cosmodrome, and was designed to perform research on the structure and dynamics of radio sources within and beyond the Milky Way. Together with some of the largest ground-based radio telescopes, the Spektr-R formed interferometric baselines extending up to 350,000 km (220,000 mi).

On 11 January 2019, the spacecraft stopped responding to ground control, but its science payload was described as "operational". The mission never recovered from the January 2019 incident, and the mission was declared finished (and spacecraft operations ended) on 30 May 2019.

Overview

The Spektr-R project was funded by the Astro Space Center of Russia, and was launched into Earth orbit on 18 July 2011,[3] with a perigee of 10,000 km (6,200 mi) and an apogee of 390,000 km (240,000 mi), about 700 times the orbital height of the Hubble Space Telescope at its highest point and 20 times at its lowest.[8][9] In comparison, the average distance from Earth to the Moon is 384,400 km (238,900 mi).[10] As of 2018, the satellite has a much more stable orbit with a perigee of 57,000 km (35,000 mi) and an apogee of 320,000 km (200,000 mi), with its orbit no longer intersecting the Moon's orbit and being stable for possibly hundreds or even thousands of years.

The main scientific goal of the mission was the study of astronomical objects with an angular resolution up to a few millionths of an arcsecond. This was accomplished by using the satellite in conjunction with ground-based observatories and interferometry techniques.[3] Another purpose of the project was to develop an understanding of fundamental issues of astrophysics and cosmology. This included star formations, the structure of galaxies, interstellar space, black holes and dark matter.

Spektr-R was one of the instruments in the RadioAstron program, an international network of observatories led by the Astro Space Center of the Lebedev Physical Institute.[8]

The telescope was intended for radio-astrophysical observations of extragalactic objects with ultra-high resolution, as well as researching of characteristics of near-Earth and interplanetary plasma. The very high angular resolving power was achieved in conjunction with a ground-based system of radio-telescopes and interferometrical methods, operating at wavelengths of 1.35–6.0, 18.0 and 92.0 cm.[11] Once in space, the flower-like main dish was to open its 27 'petals' within 30 minutes.[citation needed]

There was a science payload of opportunity on board, PLASMA-F, which consists of four instruments to observe solar wind and the outer magnetosphere. These instruments are the energetic particle spectrometer MEP-2, the magnetometer MMFF, the solar wind monitor BMSW, and the data collection and processing unit SSNI-2.[12]

At launch the mass of the spacecraft was 3,660 kg (8,070 lb). It was launched from the Baikonur Cosmodrome on 18 July 2011 at 02:31 UTC by a Zenit-3F launch vehicle, which is composed of a Zenit-2M with a Fregat-SB upper stage.[3][4]

On 11 January 2019, the spacecraft stopped responding to ground control. It was unknown whether the issue could be fixed, or whether the spacecraft's mission would be ended.[13] With Spektr-R's status unknown and the problems hitting the Mikhailo Lomonosov satellite, the Russian space program had no operational space observatories as of 12 January 2019. This changed with the launch of the Spektr-RG satellite in July 2019.

The mission was declared as finished on 30 May 2019.[14]

The external tank of the Fregat upper stage that delivered the Spektr-R observatory into orbit exploded on May 8, 2020, generating at least 65 trackable debris in orbit around Earth.[15]

History of the project

At the beginning of the 1980s, one of the USSR's leading developers of scientific space probes had completed a preliminary design of revolutionary, new-generation spacecraft, 1F and 2F. The main purpose of Spektr was to develop a common platform that could be used for future deep-space missions.

NPO Lavochkin hoped to use the designs of the 1F as the standard design for space telescopes. In 1982, NPO Lavochkin had completed technical blueprints for RadioAstron, a space-based radio telescope. The expectation was that the 1F and 2F spacecraft would follow the expectations of the RadioAstron mission (also known as Astron-2).


Early on, many criticized the 1F platform for its questionable astrophysics missions, even when compared to the older 4V spacecraft bus. Although the attitude control system of the 1F seemed to have little issues navigating planetary probes, its accuracy was much below the standard requirements for a high-precision telescope. To add to 1F's technical issues, the spacecraft seemed to lack electrically driven fly-wheels, which critics believed would have increased its stabilization in space. The spacecraft also failed to have a moveable solar panel system, which could track the position of the Sun without requiring the entire satellite to reposition, eventually disrupting the observations process.

It was one of three competing Spectrum missions, the others being Spektr X-Gamma and Spektr-UV [16]

On 1 August 1983, VPK, the Soviet Military Industrial Commission commissioned an official decision (number 274) titled, "On works for creation of automated interplanetary vehicles for the exploration of planets of the Solar System, the Moon and cosmic space". This document outlined a new impetus for the development of satellites. The new technical proposals submitted in mid-1984 included a gamma-ray telescope designated to register radio waves in the millimetre range. Both of these satellites incorporated rotating solar panels, a highly sensitive star-tracking operating system and fly wheels.

By the end of the 1980s, NPO Lavochkin Designer General, Vyacheslav Kovtunenko (ru), proposed to design all future astrophysics satellites on the current Oko-1 spacecraft model, designed originally to track incoming ballistic missiles. According to this plan, Oko-1 (a missile-watching infrared telescope) would eventually be replaced with scientific instruments where the satellite would be pointed towards space rather than Earth.

Observing techniques

Using a technique called very-long-baseline interferometry, it was anticipated that ground telescopes in Australia, Chile, China, India, Japan, Korea, Mexico, Russia, South Africa, Ukraine and the United States would jointly make observations with the RadioAstron spacecraft.

A selection of telescopes operating at wavelengths across the electromagnetic spectrum

The RadioAstron satellite's main 10-metre radio telescope would communicate in four different bands of radio waves with the international ground telescopes. It can also locate sources from two frequencies simultaneously.[17] The Spektr-R was also planned to include a secondary BMSV within the Plazma-F experiment, the goal of which was to measure the directions and intensity of solar wind. In May 2011, the news agency RIA Novosti reported that the BMSV instrument would indeed be on board. It was also reported that the BMSV would carry a micrometeoroid counter made in Germany.

The RadioAstron was expected to extend into a highly elliptical orbit in the Fregat state of the Zenit rocket's launch. Spektr-R's closest point (perigee) would be 500 kilometres (310 mi) above the Earth's surface, with its apogee 340,000 kilometres (210,000 mi) away. The operational orbit would last at least nine years, with the RadioAstron never being in the Earth's shadow for more than two hours.

With its apogee as far as the orbit of the Moon, Spektr-R could be considered a deep-space mission. In fact, the gravitational pull of the Moon was expected to fluctuate the satellite's orbit in three-year cycles, with its apogee travelling between 265,000 and 360,000 kilometres (220,000 mi) from Earth and its perigee between 400 and 65,000 kilometres (250 and 40,390 mi). Each orbit would take RadioAstron around eight to nine days. This drift would vastly augment the telescope's range of vision. It was estimated that the satellite would have upwards of 80% of its potential targets within view at any one point in its orbit. The first 45 days of Spektr-R's orbit were scheduled to consist of engineering commissioning, that is, the launch of the main antenna, various systems checks and communications tests.

Spektr-R's tracking was to be handled by the RT-22 radio telescope in Pushchino, Russia. Flight control would be operated by ground stations in Medvezhi Ozera [ru] near Moscow and Ussuriysk in Russia's Far East. Other Spektr-R joint observations would be handled by ground telescopes in Arecibo, Badary, Effelsberg, Green Bank, Medicina, Noto, Svetloe, Zelenchukskaya and Westerbork.

The Spektr-R project was led by the Russian Academy of Sciences's Astro Space Center of the Lebedev Physics Institute. The radio receivers on Spektr-R were to be built in India and Australia. In earlier plans, two additional receivers were to be provided by firms under contract with the European VLBI Consortium, the EVN. These additional payloads were eventually cancelled, with the project citing old age. Similar Russian materials replaced the Indian and Australian instruments.

See also

References

  1. ^ a b c d e f "RadioAstron User Handbook" (PDF). RadioAstron Science and Technical Operations Group. 29 July 2015. Retrieved 1 August 2015.
  2. ^ a b "Запуск российского научного космического аппарата "Спектр-Р" успешно осуществлен с Байконура" [The launch of the Russian scientific spacecraft "Spektr-R" successfully carried out from Baikonur]. Roscosmos. 18 July 2011. Archived from the original on 21 September 2015. Retrieved 1 August 2015.
  3. ^ a b c d Clark, Stephen (18 July 2011). "Russian satellite on mission to peer inside black holes". Spaceflight Now. Retrieved 1 August 2015.
  4. ^ a b Graham, William (8 November 2011). "Russian Zenit-2 launches Fobos-Grunt – Battle on to save mission". NASA Spaceflight. Retrieved 1 August 2015.
  5. ^ "Spektr-R – Orbit". Heavens Above. 19 February 2016. Retrieved 19 February 2016.
  6. ^ Zak, Anatoly. "Spektr-R Radioastron". RussianSpaceWeb. Retrieved 15 August 2011.
  7. ^ Woollacott, Emma (19 July 2011). "Russia launches 'biggest-ever' space telescope". TG Daily. Archived from the original on 15 July 2018. Retrieved 19 July 2011.
  8. ^ a b "Status of the RadioAstron project development". Russian Space Science Internet. Russian Space Research Institute. Retrieved 28 February 2008.
  9. ^ "RadioAstron Mission – Orbit". Russian Space Science Internet. Russian Space Research Institute. Retrieved 28 February 2008.
  10. ^ "Earth's Moon: Facts & Figures". Solar System Exploration. NASA. 10 May 2011. Archived from the original on 7 November 2011. Retrieved 6 November 2011.
  11. ^ "RadioAstron". Roscosmos. Archived from the original on 15 August 2013. Retrieved 18 July 2011.
  12. ^ Zelenyi, L. M.; Zastenker, G. N.; Petrukovich, A. A.; et al. (March 2013). "Plasma-F experiment onboard the Spectr-R satellite". Cosmic Research. 51 (2): 73–77. Bibcode:2013CosRe..51...73Z. doi:10.1134/S0010952513020093. S2CID 121404840.
  13. ^ "Spektr-R: Russia's only space telescope 'not responding'". BBC News. 12 January 2019.
  14. ^ "Новости. "Спектр-Р": миссия закончена, обработка данных продолжается".
  15. ^ "Spektr-R mission".
  16. ^ Schilizzi, Richard.A short history of space VLBI.University of Manchester, 2012, p6
  17. ^ Weir, F. (2011, July 19). Russian telescope launch pulls national space program out of black hole. Christian Science Monitor. https://link.gale.com/apps/doc/A261832961/OVIC?u=lom_waynesu&sid=summon&xid=eb748b48

Read other articles:

Robot di pabrik Sistem tangan robot Robotika adalah satu cabang teknologi yang berhubungan dengan desain, konstruksi, operasi, disposisi struktural, pembuatan, dan aplikasi dari robot.[1] Robotika terkait dengan ilmu pengetahuan bidang elektronika, mesin, mekanika, dan perangkat lunak komputer.[2] Pemikiran tentang pembuatan mesin yang dapat bekerja sendiri telah ada sejak Era Klasik, tetapi riset mengenai penggunaannya tidak berkembang secara berarti sampai abad ke-20.[3]…

Gustav MagnussonMagnusson, 2018StatusAktifTanggal lahir1 April 1992 (umur 31)Tempat tinggalStockholm, SwediaKebangsaan SwediaTim saat iniAlliancePermainanDota 2Riwayat karir2013–2014Alliance2014–2015Team Secret2015Alliance2016–2018OG2018–2019Evil Geniuses2020–kiniAlliance Pencapaian dan penghargaan Pemenang The International (2013) Pemenang 2× Dota Major (Boston, Kiev) Gustav Magnusson (lahir 1 April 1992), lebih dikenal dengan nama s4, adalah seorang pemain profesional Dota…

Artikel ini sebatang kara, artinya tidak ada artikel lain yang memiliki pranala balik ke halaman ini.Bantulah menambah pranala ke artikel ini dari artikel yang berhubungan atau coba peralatan pencari pranala.Tag ini diberikan pada September 2015. Pantai Carnaval adalah salah satu pantai yang ada di Taman Impian Jaya Ancol, Jakarta. Pantai yang memiliki ruang terbuka yang cukup luas, disini ada Ancol Beach City. Pada tahun 2022, Formula E diadakan disini. dan beberapa kali masuk rekor Museum Reko…

Adrià Pedrosa Pedrosa with Espanyol in 2019Informasi pribadiNama lengkap Adrià Giner PedrosaTanggal lahir 13 Mei 1998 (umur 25)Tempat lahir Barcelona, SpainTinggi 172 m (564 ft 4 in)Posisi bermain Left backInformasi klubKlub saat ini EspanyolNomor 3Karier junior2004–2009 Castelldefels2009–2014 Gavà2014–2017 EspanyolKarier senior*Tahun Tim Tampil (Gol)2017–2018 Espanyol B 46 (7)2018– Espanyol 23 (2)Tim nasional‡2019– Spanyol U-21 4 (1) * Penampilan dan gol di …

Keuskupan RožňavaDioecesis RosnaviensisDieceze RoznavskaKatolik Lambang keuskupanLokasiNegaraSlowakiaProvinsi gerejawiKeuskupan Agung KošiceStatistikLuas7.000 km2 (2.700 sq mi)Populasi- Total- Katolik(per 2014)390.584205,431 (52.6%)InformasiDenominasiKatolik RomaPendirian13 Maret 1776KatedralGereja Kenaikan Maria (Rožňava)Kepemimpinan kiniPausFransiskusUskupStanislav Stolárik[1][2]PetaPeta keuskupan Keuskupan Rožňava (bahasa Slowakia:…

Gustavo Jiménez Gustavo Jiménez (lahir di Cerro de Pasco, Pasco, tahun 1886 - meninggal di Paiján, La Libertad, 14 Maret 1933) adalah seorang kolonel Peru yang menjabat sebagai Presiden Peru selama enam hari pada tahun 1931. Jiménez mengorganisir salah satu dari beberapa pemberontakan yang menyebabkan jatuhnya pemerintahan Augusto B. Leguía. Setelah pencalonan Jenderal Luis Miguel Sánchez Cerro sebagai presiden sementara yang baru, Jiménez terus mendukung hal itu meski ia tidak setuju den…

إن تخليق اليوريا (والمواد العضوية الأخرى) من المركبات غير العضوية كانت تدحض فرضية vitalist وهي أن الكائنات الحية فقط يمكن أن تخلق هذه المركبات . المذهب الحيوي هو الاعتقاد بأن «الكائنات الحية تختلف اختلافًا جوهريًا عن الكيانات غير الحية لأنها تحتوي على بعض العناصر غير المادية أو …

Miss VenezuelaTanggal pendirian1952TipeKontes kecantikanKantor pusatCaracas, VenezuelaLokasi VenezuelaJumlah anggota Miss UniverseMiss WorldMiss InternationalBahasa resmi Bahasa SpanyolPresidenOsmel SousaSitus webSitus web resmi Miss Venezuela adalah kontes kecantikan yang diadakan di Venezuela sejak tahun 1952.[1] Kontes ini diselenggarakan untuk memilih wakil Venezuela di kontes kecantikan Miss Universe, Miss World, dan Miss International. Sejak tahun 2013, kontes ini dipecah menj…

Cet article est une ébauche concernant un zoologiste ou un botaniste. Vous pouvez partager vos connaissances en l’améliorant (comment ?) selon les recommandations des projets correspondants. Consultez la liste des tâches à accomplir en page de discussion. Hermann zu Solms-LaubachBiographieNaissance 23 décembre 1842LaubachDécès 24 novembre 1915 (à 72 ans)StrasbourgNationalité hessoiseFormation Université Martin-Luther de Halle-WittembergActivités Botaniste, paléontologue, …

Student society in Lund, Sweden Not to be confused with Göteborgs nation, Uppsala.Göteborgs NationStudent nationLund UniversityGöteborg Nation's nation house                                       LocationÖstra Vallgatan 47, Lund, SwedenLatin nameNatio GothoburgensisAbbreviationGBFounded1682NamesakeGothenburg, SwedenInspektorAndreas IngehammarProinspektorMonica LarsdotterMembershi…

Voce principale: Associazione Sportiva Dilettantistica Civitavecchia Calcio 1920. Associazione Calcio CivitavecchiaStagione 1978-1979Sport calcio Squadra Civitavecchia Allenatore Roberto Melchiorri poi Nicola Petrovic Presidente Giovanni Fattori Serie C28º posto nel girone A. Maggiori presenzeCampionato: Parasmo (34) Miglior marcatoreCampionato: Fallone (5) 1977-1978 1979-1980 Si invita a seguire il modello di voce Questa pagina raccoglie le informazioni riguardanti l'Associazione Calcio C…

  لمعانٍ أخرى، طالع بارانا (توضيح). بارانا - Paraná   بارانا (ولاية) الموقع الجغرافي سميت باسم نهر بارانا  تاريخ التأسيس 1889  تقسيم إداري البلد البرازيل[1][2] العاصمة كوريتيبا  بارانا خصائص جغرافية إحداثيات 24°40′S 51°37′W / 24.67°S 51.62°W / -24.67; -51.62   […

Anglo-Irish physician, naturalist and collector (1660–1753) This article is about the physician and collector. For the Member of Parliament, see Hans Sloane (MP). SirHans SloaneBt FRSPortrait by Stephen Slaughter13th President of the Royal SocietyIn office1727–1741Preceded byIsaac NewtonSucceeded byMartin FolkesPresident of the Royal College of PhysiciansIn office1719–1735Preceded byJohn BatemanSucceeded byThomas Pellett Personal detailsBorn(1660-04-16)16 April 1660Killyleagh, Irel…

Damiano Longhi Longhi al Padova nel 1990 Nazionalità  Italia Altezza 173 cm Peso 69 kg Calcio Ruolo Allenatore (ex centrocampista) Squadra Padova Termine carriera 2002 - giocatore Carriera Giovanili 1982-1984 Modena Squadre di club1 1984-1987 Modena77 (4)1987-1989 Padova60 (3)1989-1990 Pescara36 (0)1990-1996 Padova204 (22)1996-1997 Hércules13 (0)1997 Reggiana13 (0)1997-1998 Castel di Sangro28 (9)1998-2001 Treviso49 (2)2002 Fiorenzuola2 (0)…

Рабулеилат. Rabuleii Подданство Древний Рим Гражданская деятельность децимвир, народный трибун Военная деятельность полководец Рабулеи (лат. Rabuleii, gens Rabuleia) — древний римский род, очевидно, имевший и патрицианскую, и плебейскую ветви. Деятельность известных представител…

Brazilian footballer (born 1971) In this Portuguese name, the first or maternal family name is de Paula and the second or paternal family name is Nunes. Paulo Nunes Personal informationFull name Arílson de Paula NunesDate of birth (1971-10-30) 30 October 1971 (age 52)Place of birth Pontalina, BrazilHeight 1.74 m (5 ft 9 in)Position(s) Second strikerYouth career FlamengoSenior career*Years Team Apps (Gls)1991–1994 Flamengo 45 (30)1995–1997 Grêmio 44 (27)1997 Benfica …

ХристианствоБиблия Ветхий Завет Новый Завет Евангелие Десять заповедей Нагорная проповедь Апокрифы Бог, Троица Бог Отец Иисус Христос Святой Дух История христианства Апостолы Хронология христианства Раннее христианство Гностическое христианство Вселенские соборы Ни…

  「俄亥俄」重定向至此。关于其他用法,请见「俄亥俄 (消歧义)」。 俄亥俄州 美國联邦州State of Ohio 州旗州徽綽號:七葉果之州地图中高亮部分为俄亥俄州坐标:38°27'N-41°58'N, 80°32'W-84°49'W国家 美國加入聯邦1803年3月1日,在1953年8月7日追溯頒定(第17个加入联邦)首府哥倫布(及最大城市)政府 • 州长(英语:List of Governors of {{{Name}}}]]) • …

British independent think tank Institute for GovernmentFormation2008TypeThink tankHeadquarters2 Carlton Gardens, London, SW1Y 5AALocationLondon, EnglandDirectorHannah WhiteWebsitewww.instituteforgovernment.org.uk Carlton Gardens The Institute for Government (IfG[1]) is a British independent think tank which aims to improve government effectiveness through research and analysis. Based at 2 Carlton Gardens in central London and founded as a charity in 2008,[2] it was initially fund…

SMK Negeri 8 JakartaInformasiDidirikan30 September 1965 [1]AkreditasiA (Unggul)[2]Nomor Pokok Sekolah Nasional20102597Kepala SekolahDrs. Dadan Sabrudin M.M.Jurusan atau peminatanBisnis Manajemen dan PariwisataRentang kelasX-XIIKurikulumKurikulum 2013 RevisiJumlah siswa1.060 Peserta DidikStatusSekolah Menengah Kejuruan NegeriAlamatLokasiJl. Pejaten Raya, Kompleks Depdikbud, RT.07/RW.06, Pejaten Barat, Jakarta Selatan, DKI Jakarta,  IndonesiaTel./Faks.(021) 7996493Ko…

Kembali kehalaman sebelumnya