Large Synoptic Survey Telescope
|Large Synoptic Survey Telescope|
|Location||El Peñón, Chile|
|Altitude||2,662.75 m (top of pier):13|
|Telescope style||Three-mirror anastigmat, Paul-Baker/Mersenne-Schmidt wide-angle|
|Diameter||8.360 (5.116 metres inner) or 27.43 (16.78 ft inner)|
|Secondary dia.||3.420 m (1.800 m inner)|
|Tertiary dia.||5.016 m (1.100 m inner)|
|Angular resolution||0.7″ median seeing limit
0.2″ pixel size
|Collecting area||35 square metres (376.7 sq ft)|
|Focal length||10.31 m (f/1.23) overall
9.9175 m (f/1.186) primary
The Large Synoptic Survey Telescope (LSST) is a planned wide-field "survey" reflecting telescope that will photograph the entire available sky every few nights. The LSST is currently in its design and mirror-development phases. As of August 2012[update], site construction has been scheduled to begin (assuming NSF and DOE FY2014 budget requests are approved) in October 2014, with engineering first light at the beginning of 2020, science first light in 2021, and full operations for a ten-year survey commencing in January 2022.
The telescope will be located on the El Peñón peak of Cerro Pachón, a 2682 metre high mountain in Coquimbo Region, in northern Chile, alongside the existing Gemini South and Southern Astrophysical Research Telescopes.
On July 18, 2012, with approval of the National Science Board, the National Science Foundation (NSF) announced its intention to advance the LSST to the final design stage. This action permits the NSF Director to include funds for LSST construction in a future budget request.
The project technology is ready for a construction start in FY 2014 and awaits construction authorization. The President’s FY2014 budget request to Congress includes construction funding for LSST, the first year of construction support for an eight-year project that will begin in July 2014.
The LSST design is unique among large telescopes (8 m-class primary mirrors) in having a very wide field of view: 3.5 degrees in diameter, or 9.6 square degrees. For comparison, both the Sun and Moon, as seen from the Earth, are 0.5 degrees across, or 0.2 square degrees. Combined with its large aperture (and thus light-collecting ability), this will give it a spectacularly large etendue of 319 m²degree².
To achieve this very wide, undistorted field of view requires three mirrors, rather than the two used by most existing large telescopes: the primary mirror (M1) will be 8.4 metres (28 ft) in diameter, the secondary mirror (M2) will be 3.4 metres (11.2 ft) in diameter, and the tertiary mirror (M3), located in a large hole in the primary, will be 5.0 metres (16 ft) in diameter. The large hole reduces the primary mirror's light collecting area to 35 square metres (376.7 sq ft), equivalent to a 6.68-metre-diameter (21.9 ft) circle. (Multiplying this by the field of view produces an etendue of 336 m²degree²; the actual figure is reduced by vignetting.)
The primary and tertiary mirrors (M1 and M3) are being constructed as a single piece of glass, the "M1M3 monolith".
Allowing for maintenance, bad weather, etc., the camera is expected to take over 200,000 pictures (1.28 petabytes uncompressed) per year, far more than can be reviewed by humans. Managing and effectively data mining the enormous output of the telescope is expected to be the most technically difficult part of the project. Initial computer requirements are estimated at 100 teraflops of computing power and 15 petabytes of storage, rising as the project collects data.
Particular scientific goals of the LSST include:
- Measuring weak gravitational lensing in the deep sky to detect signatures of dark energy and dark matter.
- Mapping small objects in the solar system, particularly near-Earth asteroids and Kuiper belt objects.
- Detecting transient optical events such as novae and supernovae.
- Mapping the Milky Way.
It is also hoped that the vast volume of data produced will lead to additional serendipitous discoveries.
Synoptic is derived from the Greek words σύν (syn "together") and ὄψις (opsis "view"), and describes observations that give a broad view of a subject at a particular time.
In January, 2008, software billionaires Charles Simonyi and Bill Gates pledged $20 million and $10 million respectively to the project. The project continues to seek a National Science Foundation grant of nearly $400 million. $7.5 million is included in the U.S. President's FY2013 NSF budget request. The Department of Energy is expected to fund construction of the digital camera component by the SLAC National Accelerator Laboratory, as part of its mission to understand dark energy.
Construction of the primary mirror, the most critical and time-consuming part of a large telescope's construction, is already well underway. The M1M3 monolith is being constructed at the University of Arizona's Steward Observatory Mirror Lab. Construction of the mold began in November 2007, mirror casting was begun in March 2008, and the mirror blank was declared "perfect" at the beginning of September 2008. As of January 2011[ref], both M1 and M3 figures have completed generation and fine grinding. Polishing has begun on M3.
The secondary mirror blank has been constructed and coarse-ground to within 40 μm of the desired shape. It is in storage, awaiting funding to complete it.
As of January 2012[update], the LSST site has been leveled, the primary mirror has been ground, while the tertiary mirror is being fine-ground. The M1M3 monolith has been polished by Steward Observatory Mirror Laboratory, and it had been expected to be completed in late 2012. The design of the telescope buildings (dome, maintenance workshop, control room and utilities) is almost complete, and numerous telescope subsystems are having their designs fine-tuned. In particular, the mirror support system, stray-light baffles, wind screen, and calibration screen have been significantly improved.
- The camera is actually at the tertiary focus, not the prime focus, but being located at a "trapped focus" in front of the primary mirror, the associated technical problems are similar to those of a conventional prime-focus survey camera.
- List of largest optical reflecting telescopes
- VLT Survey Telescope
- VISTA (Visible and Infrared Survey Telescope for Astronomy)
- Eric E. Mamajek (2012-10-10), Accurate Geodetic Coordinates for Observatories on Cerro Tololo and Cerro Pachon, p. 13, retrieved 2012-10-12 Measured GPS position for future site of LSST pier is WGS84 30°14′40.68″S, 70°44′57.90″W, with ±0.10" uncertainty in each coordinate.
- Charles F. Claver; et al. (2007-03-19), LSST Reference Design, LSST Corporation, pp. 64–65, retrieved 2008-12-10 The map on p. 64 shows the Universal Transverse Mercator location of the centre of the telescope pier at approximately 6653188.9 N, 331859.5 E, in zone 19J. However, those UTM coordinates appear to be using the PSAD56 (La Canoa) datum, as other assumptions do not lead to a peak. This is apparently widely used in South American UTM grids. The coordinates above translate to WGS84 .
- Victor Krabbendam; et al. (2011-01-11). "LSST Telescope and Optics Status". American Astronomical Society 217th Meeting (poster). Seattle, Washington. Retrieved 2011-01-16. This updated plan shows the revised telescope centre at 6653188.0 N, 331859.1 E (PSAD56 datum). This is the same WGS84 location to the resolution shown.
- LSST Summit Facilities, 2009-08-14, retrieved 2009-08-21
- LSST Basic Configuration, LSST Corporation, retrieved 2008-01-28
- Willstrop, R. V. (October 1, 1984), "The Mersenne-Schmidt: A three-mirror survey telescope", Monthly Notices of the Royal Astronomical Society 210 (3): 597–609, Bibcode:1984MNRAS.210..597W, ISSN 0035-8711, retrieved 2008-01-23
- Gressler, William (June 2, 2009), LSST Optical Design Summary, LSE-11, retrieved 2011-03-01
- LSST Observatory - FAQ
- LSST Timeline
- Krabbendam, Victor (2012-08-13), "LSST Project and Technical Overview", LSST All Hands Meeting, Tucson, Arizona, retrieved 2012-09-05
- Press Release LSSTC-04: Site in Northern Chile Selected for Large Synoptic Survey Telescope
- NSF Press Release 12-137
- Matt Stephens (2008-10-03), Mapping the universe at 30 Terabytes a night: Jeff Kantor, on building and managing a 150 Petabyte database, The Register, retrieved 2008-10-03
- Matt Stephens (2010-11-26), Petabyte-chomping big sky telescope sucks down baby code, The Register, retrieved 2011-01-16
- Boon, Miriam (2010-10-18), "Astronomical Computing", Symmetry Breaking, retrieved 2010-10-26
- "Google Joins Large Synoptic Survey Telescope (LSST) Project". uanews.org. January 10, 2007. Retrieved 29 April 2013.
- Dennis Overbye (January 3, 2008). "Donors Bring Big Telescope a Step Closer". The New York Times. Retrieved 2008-01-03.
- "LSST Project Office Update". March 2012. Retrieved 2012-04-07.
- "World’s largest digital camera gets green light". 2011-11-08. Retrieved 2012-04-07./
- Large Synoptic Survey Telescope gets Top Ranking, "a Treasure Trove of Discovery", LSST Corporation, 2010-08-16, retrieved 2011-01-16
- Steward Observatory Mirror Lab Awarded Contract for Large Synoptic Survey Telescope Mirror
- LSST Observatory - Site Photos
- LSST High Fire Event
- Giant Furnace Opens to Reveal 'Perfect' LSST Mirror Blank, LSST Corporation, 2009-09-02, retrieved 2011-01-16
- Cerro Pachón First Blast, LSST Corporation, March 8, 2011, retrieved 2011-04-23, "‘First Blast’, detonated on the El Peñón summit March 8th at 8:56:00 (MST) in preparation for the LSST"
- Victor Krabbendam; et al. (2012-01-09). "Developments in Telescope and Site". American Astronomical Society 219th Meeting (poster). Austin, Texas. Retrieved 2012-01-16.
- LSST.org (October 2012). "LSST E-News - Volume 5 Number 2". Retrieved 2013-04-30.
|Wikimedia Commons has media related to Large Synoptic Survey Telescope.|
- Official home page
- LSST reports and documentation
- Science & Technology brief
- New Scientist SPACE Article
- LSST Tutorials for Experimental Particle Physicists is a detailed explanation of LSST's design (as of February 2006) and weak lensing science goals that does not assume a lot of astronomy background.
- The New Digital Sky is a video of a July 25, 2006 presentation at Google about the LSST, particularly the data management issues.
- HULIQ Google participation announcement
- Ž. Ivezić et al. (2008-05-15), LSST: From Science Drivers to Reference Design and Anticipated Data Products (v1.0) 0805, p. 2366, arXiv:0805.2366, Bibcode:2008arXiv0805.2366I, retrieved 2011-01-16, this is a comprehensive overview of the LSST.
- LSST Science Collaborations; Abell, Paul A.; Allison, Julius; Anderson, Scott F.; Andrew, John R.; Angel, J. Roger P.; Armus, Lee; Arnett, David; Asztalos, S. J. (2009-10-16), LSST Science Book, Version 2.0 0912, p. 201, arXiv:0912.0201, Bibcode:2009arXiv0912.0201L, retrieved 2011-01-16, an updated and expanded overview.