Taking the long view: A brief history of space telescopes
- by SiliconRepublic
- Oct 25, 2024
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NGC 602. Image: ESA/Webb, NASA & CSA, P Zeidler, E. Sabbi, A Nota, M Zamani (ESA/Webb) via Flickr
Durham University’s Prof Richard Massey peers into the history of space telescopy and finds the unexpected views are often the most astounding. They were followed by Japan’s Hitomi X-ray satellite, which took 18 years to build, and the German eRosita instrument on Russia’s Spektr-RG space observatory, which took 20 years.
Similar timescales apply to the European Space Agency’s Hipparcos and Gaia space telescopes, which have mapped all the stars in the Milky Way. The Cobe and Planck missions to study the microwave-light afterglow of the Big Bang also took two decades. Precise dates depend how you count, and a few exceptions have been “faster, better, cheaper” but national space agencies are generally risk averse and slow when developing these projects.
The latest space telescopes are therefore millennials. They were designed at a time when astronomers had measured the universe’s newborn expansion following the Big Bang, and also its old-age, accelerating expansion. Their main goal now is to fill the gap – because, surprisingly, interpolations from early times to late times don’t meet in the middle.
The measured rates for the expansion of the universe are inconsistent, as are results for the clumpiness of matter in the cosmos. Both measurements create challenges for our theories of how the universe evolved.
Observing the middle age of the universe requires telescopes operating at long wavelengths, because light from distant galaxies is stretched by the time it reaches us. So, Webb has infrared zoom cameras, while the European Space Agency’s Euclid space telescope, launched in 2023, and Nasa’s Nancy Grace Roman telescope, which is set to launch in 2026, both have infrared wide-angle views.
Three buses come along at once
Most stars shine in ultraviolet and infrared colours that are blocked by the Earth’s atmosphere, as well as the colours our eyes evolved to see.
Extra colours are useful. For example, we can weigh stars on the other side of our galaxy because massive stars are bright in infrared, while smaller ones are faint – and they stay that way throughout their lifetimes. However, we know where stars are being born because only young stars emit ultraviolet light.
In addition, independent measurements of the same thing are vital for rigorous science. Infrared telescopes, for example, can work together and have already made surprising discoveries. But it’s not great for diversity that the Webb, Euclid and Roman space telescopes all see infrared colours.
Hubble’s visible light camera has just been switched off due to budget cuts. Nasa will not swing back to ultraviolet wavelengths until the 2030s, with the Ultraviolet Explorer and Habitable Worlds Observatory.
Earthly politics gets in the way, too. Data from China’s Hubble-class space telescope, Xuntian, is unlikely to be shared internationally. And in protest at Russia’s invasion of Ukraine, in February 2022 Germany switched off its eRosita X-ray instrument that had been operating perfectly, in collaboration with Russia, a million miles from Earth.
Cheap commercial launches may save the day. Euclid was to have lifted off on a Russian Soyuz rocket from a European Space Agency spaceport in French Guiana. When Russia ended operations there in tit-for-tat reprisals, Euclid’s launch was successfully switched at the last minute to a SpaceX Falcon 9 rocket.
If large telescopes can also be folded inside shoebox-size cubesat satellites, the lower cost would make it viable for them to fail. Tolerating risk creates a virtuous circle that makes missions even cheaper.
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