FIRAS
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Artist's concept of the COBE spacecraft
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| Names | Explorer 66 | ||||||||
|---|---|---|---|---|---|---|---|---|---|
| Mission type | CMBR Astronomy | ||||||||
| Operator | NASA | ||||||||
| COSPAR ID | 1989-089A | ||||||||
| SATCAT no. | 20322 | ||||||||
| Website | lambda.gsfc.nasa.gov/product/cobe | ||||||||
| Mission duration | Final: 4 years, 1 month, 5 days | ||||||||
| Spacecraft properties | |||||||||
| Manufacturer | GSFC | ||||||||
| Launch mass | 2,270 kg (5,000 lb) | ||||||||
| Dry mass | 1,408 kg (3,104 lb) | ||||||||
| Dimensions | 5.49 × 2.44 m (18.0 × 8.0 ft) | ||||||||
| Power | 542 W | ||||||||
| Start of mission | |||||||||
| Launch date | 18 November 1989, 14:34 UTC | ||||||||
| Rocket | Delta 5920-8 | ||||||||
| Launch site | SLC-2W Vandenberg | ||||||||
| End of mission | |||||||||
| Disposal | Decommissioned | ||||||||
| Deactivated | 23 December 1993 | ||||||||
| Orbital parameters | |||||||||
| Reference system | Geocentric | ||||||||
| Regime | Sun-synchronous | ||||||||
| Semi-major axis | 7,255 km (4,508 mi) | ||||||||
| Eccentricity | 0.0009394 | ||||||||
| Perigee | 877.8 km (545.4 mi) | ||||||||
| Apogee | 891.4 km (553.9 mi) | ||||||||
| Inclination | 98.9808 degrees | ||||||||
| Period | 102.5 minutes | ||||||||
| RAAN | 215.4933 degrees | ||||||||
| Argument of perigee | 52.8270 degrees | ||||||||
| Mean anomaly | 351.1007 degrees | ||||||||
| Mean motion | 14.04728277 rev/day | ||||||||
| Epoch | 21 July 2015, 15:14:58 UTC | ||||||||
| Revolution no. | 31549 | ||||||||
| Main telescope | |||||||||
| Type | off-axis Gregorian (DIRBE) | ||||||||
| Diameter | 19 cm (7.5 in) | ||||||||
| Wavelengths | Microwave, Infrared | ||||||||
| Instruments | |||||||||
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| Instruments | |
|---|---|
| DIRBE | Diffuse Infrared Background Experiment |
| FIRAS | Far-InfraRed Absolute Spectrophotometer |
| DMR | Differential Microwave Radiometer |
NASA COBE logo
The Cosmic Background Explorer (COBE /ˈkoʊbi/), also referred to as Explorer 66, was a satellite dedicated to cosmology, which operated from 1989 to 1993. Its goals were to investigate the cosmic microwave background radiation (CMB) of the universe and provide measurements that would help shape our understanding of the cosmos.
COBE's measurements provided two key pieces of evidence that supported the Big Bang theory of the universe: that the CMB has a near-perfect black-body spectrum, and that it has very faint anisotropies. Two of COBE's principal investigators, George Smoot and John Mather, received the Nobel Prize in Physics in 2006 for their work on the project. According to the Nobel Prize committee, "the COBE-project can also be regarded as the starting point for cosmology as a precision science".
Later, COBE has been followed by two more advanced spacecraft: WMAP operated from 2001-2010, and Planck from 2009-2013.
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