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JAMES WEBB SPACE TELESCOPE (JWST)

Telescopes are one of the remarkable inventions that changed the way we seek the Cosmos, since its invention in the 16th century, mankind has used them to find the answer to the unknown.

By Sagar TiwariPublished 4 years ago 5 min read
James Webb Space Telescope (JWST)

One such invention is the James Webb Space Telescope, which which started its journey on 24th December last year. The launch date has been rescheduled multiple times due to inevitable events.

Here's the list of the Top 7 amazing facts about the James Webb Space Telescope.

1. Named after James E. Webb

James E. Webb

This astonishing telescope is named after the second head of NASA James E. Webb, who led the agency from (1961-1968).

Under his name, is one of the most notable records. Where he supervised the historical landing mission of the first man on the surface of the moon.

His vision was to strike a balance between human space flight and science, and that's the reason that NASA Administrator Sean O\'Keefe decided that the next big telescope after Hubble should be named after him.

2. Heading to the L2 point

Lagrange Points

The James Webb Space Telescope or also known as JWST will orbit at around 374,000 - 1.5 million Km distance around the Earth and the Sun. This path in technical terms is known as L2 point or 'Lagrange point'. It will take around about 30 days to reach the orbit and the first bit of information can be expected around in 6 months of the launch.

As JWST is equipped with an advanced level of detectors and sensors than its predecessors, so it can analyze a much wider range of light than before and hence can observe a much longer Infrared wavelength.

To achieve this detectors will target near and mid-infrared wavelengths. To make it possible JWST is going to use:-

A large mirror - To collect as much light as possible

Extremely cold temperatures

Clear Line of Sight - For this L2 point is very crucial.

3. Dust Budget Crisis

For ages scientist and researcher who studies the unexplored part of the cosmos has encountered an issue and that is the cosmic dust, which is the tiny solid matter particle drifting around in space.

But JWST can solve the problem, it's doing more than just looking through the cosmic dust, it is going to solve the "Dust Budget Crisis", this is the inability to account for all the dust found throughout the universe.

Webb will be working with JAXA to observe the Infrared light from Wolf-Rayet stars that help count it. The Wolf-Rayet stars are the supermassive stars in a very late stage of stellar life, so when observed in infrared light, they release dust in a pinwheel pattern. So Webb can observe the chemical signatures produced from Wolf-Rayet stars which then tend to help scientists to understand the complex answers of early star formations and how our cosmos got so dusty.

Wolf-Rayet Stars

4. Operational temperature is between 85°C to -233°C.

Primarily James Webb Space Telescope is divided into two broad sections, the cold section that consists of the Observation function and the hot section that has the Sunshield layers.

The reason why it uses the shielded layers is that Infrared light can also be interpreted as heat, and one of the main tasks of JWST is to study the existent distant and usually faint wavelength. So engineers have to make sure that it is protected from all sources of heat.

The Hot side mainly compromises the sun shield, solar panels, Communication antennas, spacecraft buses, and star trackers. Whereas the cold side consists of primary and secondary mirrors, infrared instruments clusters, and detectors.

5. Unprecedented Goals

Being one of the most expensive projects in space history, it took more than 25 years to finally complete the projects, by the scientist, engineers, and research of the various space agencies of the USA, Canada, and EU.

This sheer hard work is to create a masterpiece. Compare to Hubble it is what Digital Microscope to the magnifying glass. Here are some of the goals set to achieve by JWST:-

  • JWST will show our universe just after 100-250 million of Big Bang (Which helps the scientist to understand the process and the structure of our universe more precisely).
  • Find the various signs for the potential life in the planetary system and the first galaxies that were formed.
  • It helps to create a 3-D model of our universe to have a better understanding.
  • It is set on the mission to find the planets and satellites outside our solar system and learn about earthlike exoplanets. (It will be able to determine their density, composition, and atmosphere for further analysis).
  • JWST can find data on up to 300 exoplanets, in comparison to its predecessors Hubble and SST that collected data of up to 100 only.

6. Enormous size and structure of JWST

Size comparison

The James Webb Space Telescope has a significant size and structure. From one end to the other it's equal to a Tennis court and nearly three-story high. The weight is around 6.2 tonnes.

The main mirror of JWST has a diameter of about 6.5 meters, and a collecting area of about 25 meters square, it has been designed to resemble the shape of a giant honeycomb with 18 sections. A special type of Beryllium 'Be' was used for its construction, which can retain its shape in low cryogenic temperatures, in addition to that the front layer of the mirror is covered with 48.25 gm of gold, which is 100 nanometers thick for best reflection of infrared radiation.

The secondary mirror is placed opposite to the main mirror, which receives lights from the main and directs it to the instruments at the rear end of the telescope, for better quality two more mirrors are placed to collect images from the surface.

The biggest element of the telescope is the sun-shield, which resembles the structure of an enormous pie, it is about 20 meters long and 7 meters wide and consists of 5 very thin layers of Kapton Polymide film which protects the mirrors and tools from direct sunlight.

7. Important components and sensors

To achieve all the desired goals JWST has some amazing components. Here is the list of some:-

  • A centralized computer controls the operation while the telescope is in its orbit.
  • NIRCam or also called (Near Infrared Camera), is the main eye of the telescope. It will help to see the oldest star in-universe or maybe create a map of dark matter.
  • Near-Infrared Spectogrpah will collect both the physical and chemical properties of various objects.
  • MIRI (Mid-Infrared instrument) will allow seeing a star being born, unknown objects of the Kuiper belt, and the search of the mysterious 9th planet.
  • NIRISS (Near-Infrared Imager and Slitless spectrograph) will be aimed to find the exoplanets and the first light of the distant object.
  • FGS (Fine Guided Sensors), are the precision point sensor to take out the higher quality images updates.
  • science

    About the Creator

    Sagar Tiwari

    I am a freelance writer with deep interst in space science and technology, always seeking to learn more and more from every aspect.

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