Primary Mirror: Features a 6.5-meter diameter primary mirror, segmented into 18 hexagonal beryllium mirrors, coated with gold for optimal infrared reflectivity.

Orbit: Operates in a halo orbit around the Sun-Earth L2 (second Lagrange) point, approximately 1.5 million km from Earth, providing a stable, cold, and unobstructed view of the cosmos.

Instruments: Equipped with four main scientific instruments: NIRCam (Near-Infrared Camera), NIRSpec (Near-Infrared Spectrograph), MIRI (Mid-Infrared Instrument), and FGS/NIRISS (Fine Guidance Sensor/Near Infrared Imager and Slitless Spectrograph).

Wavelength Range: Primarily observes in the infrared spectrum (0.6 to 28 micrometers), allowing it to penetrate cosmic dust clouds and detect the highly redshifted light from the earliest galaxies.

Sunshield: A five-layer, tennis-court-sized sunshield protects the telescope from the heat of the Sun, Earth, and Moon, keeping its instruments at extremely cold temperatures (around -233°C) essential for infrared observations.

Mission Goals: Key objectives include studying the first light and reionization epoch, the assembly of galaxies, the birth of stars and protoplanetary systems, and the characterization of exoplanets.

International Collaboration: A flagship project involving NASA (United States), the European Space Agency (ESA), and the Canadian Space Agency (CSA).

Successor to Hubble: Offers significantly improved sensitivity and angular resolution compared to the Hubble Space Telescope, particularly in the infrared wavelengths.

Deployment: Its complex deployment sequence, including the unfolding of its sunshield and primary mirror segments, was a critical engineering feat.

Primary Mirror: Features a 6.5-meter diameter primary mirror, segmented into 18 hexagonal beryllium mirrors, coated with gold for optimal infrared reflectivity.

Orbit: Operates in a halo orbit around the Sun-Earth L2 (second Lagrange) point, approximately 1.5 million km from Earth, providing a stable, cold, and unobstructed view of the cosmos.

Instruments: Equipped with four main scientific instruments: NIRCam (Near-Infrared Camera), NIRSpec (Near-Infrared Spectrograph), MIRI (Mid-Infrared Instrument), and FGS/NIRISS (Fine Guidance Sensor/Near Infrared Imager and Slitless Spectrograph).

Wavelength Range: Primarily observes in the infrared spectrum (0.6 to 28 micrometers), allowing it to penetrate cosmic dust clouds and detect the highly redshifted light from the earliest galaxies.

Sunshield: A five-layer, tennis-court-sized sunshield protects the telescope from the heat of the Sun, Earth, and Moon, keeping its instruments at extremely cold temperatures (around -233°C) essential for infrared observations.

Mission Goals: Key objectives include studying the first light and reionization epoch, the assembly of galaxies, the birth of stars and protoplanetary systems, and the characterization of exoplanets.

International Collaboration: A flagship project involving NASA (United States), the European Space Agency (ESA), and the Canadian Space Agency (CSA).

Successor to Hubble: Offers significantly improved sensitivity and angular resolution compared to the Hubble Space Telescope, particularly in the infrared wavelengths.

Deployment: Its complex deployment sequence, including the unfolding of its sunshield and primary mirror segments, was a critical engineering feat.