Generated by DeepSeek V3.2| James Webb Space Telescope | |
|---|---|
| Name | James Webb Space Telescope |
| Caption | Artist's impression |
| Mission type | Astronomy |
| Operator | NASA / ESA / CSA |
| Website | https://webb.nasa.gov |
| Mission duration | 10 years (planned), 20+ years (expected) |
| Manufacturer | Northrop Grumman, Ball Aerospace |
| Launch date | 25 December 2021 |
| Launch rocket | Ariane 5 flight VA256 |
| Launch site | Guiana Space Centre |
| Orbit reference | Sun–Earth L2 point |
| Orbit regime | Halo orbit |
| Telescope type | Korsch telescope |
| Diameter | 6.5 m (21 ft) |
| Focal length | 131.4 m (431 ft) |
| Collecting area | 25.4 m² (273 sq ft) |
| Wavelength | 0.6–28.3 μm (orange to mid-infrared) |
| Instruments | NIRCam, NIRSpec, MIRI, NIRISS, FGS/NIRISS |
James Webb Space Telescope. It is a large, space-based observatory optimized for infrared astronomy and a flagship mission of NASA, developed in partnership with the European Space Agency and the Canadian Space Agency. Launched in late 2021, it is the premier observatory of the next decade, serving thousands of astronomers worldwide to explore every phase of cosmic history.
Conceived as the scientific successor to the Hubble Space Telescope, it is designed to look deeper into the universe to observe the first galaxies and see into dusty stellar nurseries where stars and planetary systems form. Its development was led by NASA's Goddard Space Flight Center, with major contributions from Northrop Grumman and an international consortium of academic and research institutions. The mission is named for James E. Webb, who served as NASA Administrator during the pivotal Apollo program.
The project's origins trace to a 1996 workshop at the Space Telescope Science Institute, with formal development beginning after the Astronomy and Astrophysics Decadal Survey of 2000 recommended it as a top priority. Facing significant technical challenges and cost overruns, the project underwent major redesigns and survived a near-cancellation vote by the United States Congress in 2011. Final assembly and testing occurred at facilities including Johnson Space Center and Northrop Grumman in Redondo Beach, California. It launched on an Ariane 5 rocket from the Guiana Space Centre on Christmas Day 2021, followed by a complex, month-long deployment sequence.
Its primary design feature is a 6.5-meter segmented beryllium primary mirror coated in gold, which unfolds after launch. A five-layer sunshield the size of a tennis court passively cools the telescope and its instruments to cryogenic temperatures. The suite of four main scientific instruments includes NIRCam (provided by the University of Arizona), NIRSpec (built by ESA with components from NASA's Goddard Space Flight Center), MIRI (a joint project of ESA and NASA's Jet Propulsion Laboratory), and NIRISS (contributed by the Canadian Space Agency).
Its core scientific goals are organized into four themes: observing the first light in the universe after the Big Bang, studying galaxy formation and evolution, understanding the birth of stars and protoplanetary disks, and investigating the origins of life through the study of exoplanet atmospheres. Early observations have already transformed fields, capturing unprecedented images of SMACS 0723, analyzing the atmosphere of WASP-96 b, and providing detailed views of the Carina Nebula and Southern Ring Nebula.
It does not orbit Earth but operates from a halo orbit around the Sun–Earth L2 Lagrange point, approximately 1.5 million kilometers away. This location provides a stable thermal environment and an unobstructed view of the cosmos. Mission operations are conducted from the Space Telescope Science Institute in Baltimore, Maryland, which also serves as the science and operations center for the Hubble Space Telescope. Communications are handled via the Deep Space Network.
While the Hubble Space Telescope observes primarily in ultraviolet and visible light, it is optimized for the infrared spectrum, allowing it to see through cosmic dust and observe highly redshifted objects. It has a significantly larger light-collecting area than Hubble but operates at much colder temperatures. Other contemporary and future observatories include the Nancy Grace Roman Space Telescope, ground-based giants like the Very Large Telescope and the future Extremely Large Telescope, and other space-based missions like the Euclid spacecraft.
Category:Space telescopes Category:NASA space probes Category:Infrared telescopes