Webb: Hubble's successor
Since its launch in , the Hubble Space Telescope has had a great impact on our understanding of the universe and the public's interest in astronomy. It has allowed us to peer further into space than ever before, take breathtakingly detailed images of planets and galaxies, and solve many of the universe's great mysteries.
The James Webb Space Telescope will be Hubble's successor, but not its replacement. The two missions have a planned overlap and will work together on new discoveries. Webb will build on Hubble's impressive legacy by helping humanity peer even deeper into the universe.
There are, however, many differences between these two space telescopes. Webb will have unique capabilities that will allow it to perform science Hubble is not able to do.
|Hubble Space Telescope||James Webb Space Telescope|
|Telescope size||About the size of a school bus||About the size of a tennis court due to its large sunshield; will need to be folded up when it launches on an Ariane 5 rocket|
|Mirror size||A single 2.4 m-wide mirror||18 hexagonal mirror segments, for a total width of 6.5 m|
|Light observed||Ultraviolet, visible and near-infrared light||Near- and mid-infrared light|
|Location||Low Earth orbit, at an altitude of 547 km||1.5 million km away from Earth (at a point in space known as Lagrange 2)|
|Maintenance||Due to its location, Hubble can be repaired and upgraded while in orbit. Astronauts famously corrected Hubble's mirror in using Canadarm, Canada's robotic arm on the American Space Shuttle.||Webb will be too far from Earth to repair, which is why it has gone through unprecedented testing.|
|Mission lifetime||Hubble was launched in and will remain operational as long as its instruments are functioning.||The minimum expected lifetime of Webb is 5 years, but it may go beyond 10 years. This will depend on how long its propellant (needed to keep Webb stable in its orbit) will last.|
Why study infrared light?
The light we can see with our eyes is composed of many wavelengths, each with its own colour—like those of a rainbow. This is called visible light and is produced by objects like our Sun and artificial lighting in our homes. However, there are many other kinds of light, such as infrared light, that our eyes cannot see. Certain objects, like cold stars and planets, shine most brightly in the infrared. Astronomers must study the infrared universe to understand these intriguing objects.
While Hubble focuses mainly on light that is visible to the human eye, Webb's four scientific instruments were specifically designed to capture infrared light. Webb will be able to peer through cosmic dust to study colder or very distant objects.
Some of the advantages of infrared observations:
- Certain objects in space like planets, red stars and brown dwarfs are too cold to emit much visible light and are most visible in the infrared.
- Because infrared light wavelengths are longer than those of visible light, they can penetrate dust clouds more easily, which allows astronomers to peer inside nebulae to see newly forming stars and planets that would otherwise remain hidden.
- The very first galaxies ever created in the universe are best observed in the infrared. Since those galaxies are very distant, their light has been stretched, in a phenomenon known as redshift, to infrared wavelengths by the time it reaches Webb.
Have you ever noticed the sound of an ambulance changing as it drives past you? It is higher pitched as it moves towards you, and lower pitched as it drives away. This effect is known at the Doppler shift: sound waves produced by an object moving towards you are compressed, while they are stretched as the waves move away from you. This same concept applies to light!
Because all galaxies are moving away from us due to the expansion of the universe, the light they produce is being stretched into longer wavelengths. This phenomenon is called cosmological redshift – "
red" because stretched light appears redder!
- About the James Webb Space Telescope
- What Webb will observe
- Canadian science observation programs for the Webb Telescope
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