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Wide Field Imager

MPG/ESO telescope
Esopia00046teles.jpg
Observatory La Silla Observatory Edit this on Wikidata
Location(s) Atacama Desert, Chile Edit this at Wikidata
Coordinates 29°15′28″S 70°44′12″W / 29.25786°S 70.736648°W / -29.25786; -70.736648Coordinates: 29°15′28″S 70°44′12″W / 29.25786°S 70.736648°W / -29.25786; -70.736648 Edit this at Wikidata
Organization European Southern Observatory
Max Planck Institute for Astronomy Edit this on Wikidata
Altitude 2,375 m (7,792 ft) Edit this at Wikidata
Built –1983 (–1983) Edit this at Wikidata
First light 22 June 1983 Edit this on Wikidata
Telescope style optical telescope
Ritchey–Chrétien telescope Edit this on Wikidata
Diameter 2.20 m (7 ft 3 in) Edit this at Wikidata
Secondary diameter 0.84 m (2 ft 9 in) Edit this at Wikidata
Angular resolution 0.3 arcsecond Edit this on Wikidata
Collecting area 3.8 m2 (41 sq ft) Edit this at Wikidata
Focal length 17.6 m (57 ft 9 in) Edit this at Wikidata
Mounting Equatorial mount Edit this at Wikidata
Website www.eso.org/public/teles-instr/lasilla/mpg22/ Edit this at Wikidata
MPG/ESO telescope is located in Chile
MPG/ESO telescope
Location of MPG/ESO telescope
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The MPG/ESO telescope is a 2.2-metre f/8.0 (17.6-metre) ground-based telescope at the European Southern Observatory (ESO) in La Silla, Chile. It was built by Zeiss and has been operating since 1984. It was on indefinite loan to the European Southern Observatory from the Max Planck Institute for Astronomy (MPIA). In October 2013 it was returned to the MPIA. Telescope time is shared between MPIA and MPE observing programmes, while the operation and maintenance of the telescope are ESO's responsibility.

The telescope hosts three instruments: the 67-million pixel Wide Field Imager with a field of view as large as the full Moon, which has taken many amazing images of celestial objects; GROND, the Gamma-Ray Burst Optical/Near-Infrared Detector, which chases the afterglows of the most powerful explosions in the Universe, known as gamma-ray bursts; and the high-resolution spectrograph, FEROS, used to make detailed studies of stars.

In November 2010 it was used to discover HIP 13044 b, marking the first time a planetary system in a stellar stream of extragalactic origin has been detected.

Messier 7 imaged by the 67-megapixel Wide Field Imager (WFI)

WFI captures the star-forming dark cloud Lupus 3

The Orion Nebula (Messier 42) captured using the WFI camera

The Jewel Box (star cluster) NGC 4755 taken with the WFI

Amazing vista of the Lagoon Nebula taken with Wide Field Imager

One square degree image of the Tarantula Nebula using the WFI


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