Wide-field Infrared Survey Explorer

Wide-field Infrared Survey Explorer (WISE, observatory code C51, Explorer 92 and SMEX-6) is a NASA infrared astronomy space telescope in the Explorers Program launched in December 2009. WISE discovered thousands of minor planets and numerous star clusters. Its observations also supported the discovery of the first Y-type brown dwarf and Earth trojan asteroid. WISE performed an all-sky astronomical survey with images in 3.4, 4.6, 12 and 22 μm wavelength range bands, over ten months using a 40 cm (16 in) diameter infrared telescope in Earth orbit.

Wide-field Infrared Survey Explorer
WISE spacecraft
NamesExplorer 92
SMEX-6
NEOWISE
Near-Earth Object WISE
Mission typeInfrared telescope
OperatorNASA / JPL
COSPAR ID2009-071A
SATCAT no.36119
Websitewww.nasa.gov/wise
Mission duration10 months (planned)
14 years, 1 month and 30 days (in progress)
Spacecraft properties
SpacecraftExplorer XCII
Spacecraft typeWide-field Infrared Survey Explorer
BusRS-300
ManufacturerBall Aerospace & Technologies
Launch mass661 kg (1,457 lb)
Payload mass347 kg (765 lb)
Dimensions2.85 × 2 × 1.73 m (9 ft 4 in × 6 ft 7 in × 5 ft 8 in)
Power551 watts
Start of mission
Launch date14 December 2009, 14:09:33 UTC
RocketDelta II 7320-10C (Delta 347)
Launch siteVandenberg, SLC-2W
ContractorUnited Launch Alliance
Entered service2010
End of mission
Decay date2025 (planned)
Orbital parameters
Reference systemGeocentric orbit
RegimeSun-synchronous orbit
Perigee altitude488.3 km (303.4 mi)
Apogee altitude494.8 km (307.5 mi)
Inclination97.50°
Period94.45 minutes
Main telescope
Diameter40 cm (16 in)
Wavelengths3.4, 4.6, 12 and 22 µm
Instruments
Four infrared detectors
Explorer Program
 

After its solid hydrogen coolant depleted, it was placed in hibernation mode in February 2011. In 2013, NASA reactivated the WISE telescope to search for near-Earth objects (NEO), such as comets and asteroids, that could collide with Earth. The reactivation mission was called Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE). As of August 2023, NEOWISE is 40% through the 20th coverage of the full sky.

Science operations and data processing for WISE and NEOWISE take place at the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena, California. The WISE All-Sky (WISEA) data, including processed images, source catalogs and raw data, was released to the public on 14 March 2012, and is available at the Infrared Science Archive.

The NEOWISE mission is expected to end by early-2025 and the satellite to reentry some time after.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.