How do astronomers cool infrared space telescopes?
General knowledgeIn depthAsked by Anonymous23 Oct 2026, 12:44 PM ISTUpdated
In one line
Astronomers cool infrared space telescopes by using special shields, cold materials, and sometimes liquid gases to keep them very cold so they can see heat from space clearly.
James Webb Space Telescope — NASA/ESA/CSA space infrared telescope launched in 2021 The James Webb Space Telescope, showing its large sunshield that keeps it cold. Image: Wikipedia
The rule
Infrared telescopes must be kept extremely cold to prevent their own heat from interfering with the faint heat signals (infrared light) they are trying to detect from space.
No single formula, but the key idea is: Infrared signal = Total detected signal − Telescope's own heat signal
Let's understand it simply
Imagine you are trying to see the stars at night, but someone is shining a torch right next to your eyes. You won’t see the stars well because the torch is too bright. Infrared telescopes are like your eyes, and their own heat is like the torch. If the telescope is warm, its own heat will block the faint heat coming from faraway stars and planets.
To fix this, astronomers make the telescope very cold. It’s like turning off the torch so you can see the stars better. They use special covers and coolants (cold liquids or gases) to keep the telescope colder than ice in your freezer.
Cooling methods for infrared telescopes
Passive (Sunshield, Radiative)
Active (Cryogenic)
How it works
Blocks heat, lets telescope cool by itself
Uses liquid helium or mechanical coolers
Example
JWST main mirrors
Spitzer, JWST's MIRI camera
Temperature reached
About −233°C
Up to −266°C
How it works
Sunshields: The telescope is covered with big, shiny shields that block sunlight and heat from the Sun, Earth, and Moon.
Radiative cooling: The telescope is pointed away from warm objects and lets its own heat escape into space, which is very cold.
Cryogenic cooling: Some telescopes use special coolants like liquid helium, which is much colder than ice, to cool the parts that detect infrared light.
Insulation: Layers of special materials wrap the telescope to keep outside heat from getting in.
Careful placement: The telescope is put far from Earth (like at the L2 point) so it stays in the cold shadow of its own sunshield.
Electronics kept separate: Warm electronics are kept away from the cold parts, or are specially cooled.
How JWST stays cold
Sunshield blocks sunlight and heat
Telescope faces deep space
Heat radiates away
Cryocooler cools special camera
The story behind it
Infrared astronomy became important in the late 20th century. Early telescopes on Earth could not see faint heat from space because our atmosphere and the telescope itself were too warm. In 1983, the IRAS (Infrared Astronomical Satellite) was the first to use liquid helium to cool its detectors in space. Later, missions like Spitzer and the James Webb Space Telescope (JWST) improved these methods. JWST, for example, uses a five-layer sunshield the size of a tennis court to stay cold. The need to see the universe in new ways pushed astronomers to invent better cooling tricks.
Where you see it in real life
James Webb Space Telescope (JWST) → Uses a giant sunshield and radiative cooling to reach −233°C, plus a cryocooler for its coldest camera.
Spitzer Space Telescope → Used liquid helium to cool its detectors to −271°C.
ISRO's ASTROSAT → Has ultraviolet and X-ray telescopes, but future Indian missions may use similar cooling for infrared.
Thermal cameras on Earth → Use small coolers to see heat in darkness, like night-vision goggles.
Pressure cookers → The insulation keeps heat in; in telescopes, insulation keeps heat out.
Coolers in summer → Just as you use a cooler to keep water cold, telescopes use special methods to keep themselves cold in space.
Why it matters
Sees hidden objects: Only cold telescopes can see faint heat from distant stars, planets, and galaxies.
Finds new worlds: Helps find planets around other stars (exoplanets) by their heat.
Studies the early universe: Infrared light shows us galaxies as they were billions of years ago.
Needed for future missions: Cooling technology is key for new telescopes and satellites.
Worked example
Let’s see how JWST stays cold:
Given: Sunshield blocks 99.999% of sunlight, telescope faces deep space
Step 1: Sunshield reflects and blocks heat from Sun, Earth, and Moon
Step 2: Telescope radiates its own heat away to space
Step 3: Passive cooling brings telescope to about −233°C
Step 4: Cryocooler brings the coldest camera (MIRI) to −266°C
Step 5: Result: Telescope is cold enough to see faint infrared signals
Common mistakes
Thinking space is always cold: Space is cold, but sunlight and the telescope’s own heat can warm it up quickly.
Forgetting about insulation: Just like a thermos, insulation is needed to keep the cold in (or heat out).
Assuming all telescopes use liquid helium: Some use only sunshields and radiative cooling, especially newer ones.
Believing electronics can be cold: Electronics generate heat and must be kept away from the coldest parts.
Remember it
"Infrared telescopes must be colder than space to see the universe’s heat."
Check yourself
Why do astronomers need to cool infrared telescopes?
To stop the telescope's own heat from hiding faint heat signals from space.
Name one method used to cool space telescopes.
Using a sunshield to block sunlight and keep the telescope cold.
What does a cryocooler do in a telescope like JWST?
It cools the special camera (MIRI) to very low temperatures for better infrared detection.
Why can't electronics be kept with the coldest parts of the telescope?
Because they produce heat, which would spoil the cold needed for infrared detection.
Quick recap
Infrared telescopes must be kept extremely cold to work properly.
Sunshields, radiative cooling, and cryogenic liquids are used for cooling.
JWST uses a giant sunshield and a cryocooler for its coldest camera.
Keeping the telescope cold stops its own heat from blocking faint signals.
Cooling technology is essential for seeing distant, hidden objects in space.