Spectrum-X-Gamma
 Spektr-RG |
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| General information | |
|---|---|
| NSSDC ID | SPECXGM |
| Organization | Russian Space Research Institute |
| Major contractors | ESA, MPE, LU |
| Launch date | Q1 2014 (planned) [1] |
| Launched from | Baikonur |
| Launch vehicle | Soyuz-2/Fregat |
| Type of orbit | low Earth orbit |
| Instruments | |
| eROSITA | Wolter telescopes by MPE, Germany (extended ROentgen Survey with an Imaging Telescope Array) |
| Lobster | wide field X-ray monitor developed by Leicester University, UK |
| ART-XC | coded-mask telescopes developed by IKI and VNIIEF, Russia |
| Website | hea.iki.rssi.ru/SRG |
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Statistics as of 2011-01-23. |
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Spektr-RG (Russian for Spectrum + Röntgen + Gamma; also called Spectrum-X-Gamma, SRG, SXG) is an international high-energy astrophysics observatory, which is being built under the leadership of the Russian Space Research Institute (IKI). Spektr-RG instrumentation includes 5 telescopes spanning the energy range from the far ultraviolet to the hard X-ray, plus an all-sky monitor.
Development of an early version with the same name was canceled in 2002.[3]
Contents |
Early Spektr-RG [edit]
.png) Artist impression of the early Spektr-RG |
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| General information | |
|---|---|
| Organization | Russian Space Research Institute |
| Launch date | (canceled in 2002) [3] |
| Launched from | Baikonur |
| Launch vehicle | Proton |
| Orbit height | 200,000km apogee |
| Orbit period | 4 day |
| Instruments | |
| JET-X[4] | two co-aligned 4.4 m-long X-ray telescopes |
| TAUVEX | Ultraviolet telescope |
| EUVITA | Ultraviolet telescope |
| MART | X-ray telescope with coded-aperture instruments |
| LEPC/HEPC | gaseous position-sensitive proportional counters |
| SIXA | two solid-state Si(Li) detectors |
| SXRP | stellar X-ray polarimeter |
| MOXE | X-ray all-sky monitor |
| DIOGENE and SPIN | spectrometers for measuring gamma-ray bursts |
| gaseous scintillation proportional counter | |
| SODART[5] | high-throughput multi-mirror X-ray twin telescope of 8m focal length with changeable detectors on slides for energies between 0.1 and 20 keV |
| Bragg spectrometer | |
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Statistics as of 2011-02-04. |
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Development of an early version of Spektr-RG was started in mid-'90s and was finally canceled in 2002.[3] Initial launch date was set to 1995,[7] but later postponed as far as 2008, until it was finally cancelled in 2002.[3] However, some of the instruments have been completed, e.g., an X-ray telescope by Leicester University (JET-X)[8] and an ultraviolet telescope by Tel-Aviv University (TAUVEX).
Current Spektr-RG [edit]
The successor of the early Spektr-RG was initiated in 2005[2] and is currently in development and scheduled for launch in Q1 2014.[1] The observatory is intended to study interplanetary magnetic field, galaxies, black holes.[9]
References [edit]
- ^ a b Anatoly Zak (2011-01-23). "Spektr-RG". Russian Space Web. Retrieved 2011-02-03.
- ^ a b "Spectrum-RG/eRosita/Lobster mission definition document". Russian Space Research Institute. 2005-10-30. Retrieved 2011-02-04.
- ^ a b c d Harland, David M.; Harvey, Brian (2007), Space Exploration 2008, シュプリンガー・ジャパン株式会社, p. 96, ISBN 978-0-387-71667-1, retrieved 2011-02-04
- ^ [1]
- ^ [2]
- ^ Gunter Dirk Krebs. "Spektr-RG (SXG)". Retrieved 2011-02-04.
- ^ "Spectrum-X-Gamma". DTU Space. 2000-08-04. Retrieved 2011-02-04.
- ^ "Leicester's role in Russian satellite programme revealed as UK's largest telescope goes to Science Museum". DTU Space. 2009-06-17. Retrieved 2011-02-04.
- ^ "Russia to Restart Science in Space". Russian Federal Space Agency. 2010-08-12. Retrieved 2011-02-04.
External links [edit]
- Spectrum-X-Gamma on the internet.
- New X-Ray Telescopes Search for Galaxy Clusters and Massive Black Holes
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