# How much are the benefits of installing a telescope in orbit?

I know that our atmosphere acts like a protective blanket letting only some light through while blocking others. We send telescopes to orbit to get a clearer view of space objects.

I want to know that how much is this benefit. How clear, detailed and helpful-to-study are the pictures compared to pictures from ground based telescopes?

• @fasterthanlight your edit changed the question.
– Was
Sep 23 at 15:19
• Whoops, that was too much of an edit. Sorry! Sep 23 at 15:20
• Are you most interested in the benefits for optical observations (sort-of implied by use of "pictures") vs being able to observe in that part of the electromagnetic spectrum at all ? For example, UV and X-ray astronomy is only possible from orbit as the atmosphere isn't transparent at those wavelengths... Sep 23 at 19:12
• How do you define benefits? Achievable image resolution? Up-time? Sep 23 at 21:49
• @samcarter_is_at_topanswers.xyz "How do you define benefits?" I think that's hoop to jump through too far. Why should the OP, a new user asking a question about a topic they are just starting to learn about have to stop and pre-constrain what "benefits" means and which kinds are allowed, without yet knowing which answers that might exclude. Why not just let answers outline the main benefits for astronomy?
– uhoh
Sep 24 at 0:23

## 2 Answers

Space telescopes are expensive. However they have advantages

• "Permanent" night time, often they use a solar shade to stay dark to observe ambient light
• Also the biggest advantage is no atmosphere means no atmospheric distortion

But the benefits come at a price. A amateur astronomer can build a telescope for money, homemade setups in the 10-100 thousand dollar range and laboratory grade ones cost millions or billions.

The Hubble Telescope cost 1.5 Billion dollars in 1990 dollars (3.14 in 2021 $). The replacement James Webb is now pushing 11 billion! The new "Thirty Meter telescope" will cost only$1 Billion.

How much are the benefits of installing a telescope in orbit?

In the past the benefits have been astronomical!

Sorry, I couldn't help it.

...our atmosphere acts like a protective blanket letting only some light through while blocking others...

For visible light astronomy, much of the light above the Earth reaches the ground, but astronomical seeing has limited resolution. Bigger telescopes could collect more light, but they couldn't resolve much better than a 15 cm diameter aperture.

So the 2.4 meter diameter Hubble Space Telescope delivered by far the highest resolution visible light images ever. Putting that telescope in space is one of the single biggest game changers in visible light Astronomy ever, matched only by the invention of the telescope, okay and photographic plates, and digital imaging...

How clear, detailed and helpful-to-study are the pictures compared to pictures from ground based telescopes?

Then speckle interferometry and especially adaptive optics were developed that could mostly overcome the atmospheric effects. But adaptive optics is complicated and expensive and needs computers, calibration and often artificial guide stars to work. Until recently it was only working in the near infrared, though it is pushing into the visible spectrum now.

As @RobJeffries points out the Hubble also covers some ultraviolet wavelengths that are not accessible from Earth's surface due to atmospheric absorption.

There are many other electromagnetic bands for which we must go to space to receive signals. These include UV through X-rays and most gamma rays. The atmosphere is too absorbing to to receive this radiation on the surface.

For the highest energy gamma rays however, astronomers use the Earth's atmosphere to convert the gamma rays to a shower of lower energy photons and particles then use a big array of detectors to record the shower and time the individual particles to reconstruct the direction and energy of the gamma ray.

For charged particle or cosmic ray astronomy (e.g. protons and heavier nuclei) you also must go above the atmosphere to directly measure the particles (low energy) but you can also use the Earth's atmosphere to produce a shower.

Measuring cosmic ray and gamma ray showers source

For low energy protons and nuclear cosmic rays, there is the Alpha Magnetic Spectrometer aboard the International Space Station.

At the other end of the electromagnetic spectrum, starting below 20 or 30 MHz the Earth's ionosphere becomes reflective to low frequencies. This is why short wave radio listeners can hear signals from the other side of the Earth. For these lower frequencies radio astronomers must also get above Earth's atmosphere.

Another advantage of going to space is distance!

VLBI or very long baseline interferometry is the use of radio telescopes separated by very large distances to make a synthetic aperture for very high resolution. Currently the most famous case is the Event Horizon Telescope which is "as big as the Earth" and firmly on the ground, but VLBI from space offers even larger baselines.

• This is more than my answer, thanks.
– Was
Sep 24 at 5:47
• @WalidSiddik Thanks! it's a lot for sure, but mostly summarizing what's already been written about here. If there's anything specific you feel is still unanswered please feel fee to ask for clarification or post a new question.
– uhoh
Sep 24 at 5:51