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The BBC's December 7, 2022 SKA: Construction to begin on world's biggest telescope includes the following:

It will perform the most precise tests of Einstein's theories

and

The first major milestone should come in 2024, when four dishes in Australia and six antenna stations in South Africa are made to work seamlessly together as a basic telescope. This proof-of-principle moment will then trigger the array's full roll-out.

These may seem like two separate questions, but since it's obviously part of the press kit and PR roll-out, I think it's likely sources will have basic answers to both. So I'd like to ask for basic "SKA 101" answers to:

Question: How will the SKA "perform the most precise tests of Einstein's theories" and the Australia & South Africa arrays be "made to work seamlessly together"?

I didn't think there was any overlap in frequency between the arrays on different continents, so while they could both observe the same spot of sky at the same time, I don't see how that could be though of as working together in a "seamless" way.

Isn't registration of image data from different instruments a pretty standardized operation these days and something that one would normally do offline at a later date?

Does this seamlessness have something to do with ?

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  • $\begingroup$ It will test general relativity by monitoring pulsars which are precise as a atomic clock. also it will look for gravitational waves $\endgroup$
    – user47732
    Dec 13, 2022 at 6:24
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    $\begingroup$ @ScienceAJ how exactly does SKA monitoring pulsars test general relativity in a way that all the other pulsar monitoring telescopes (radio or X-ray) can't? Just what kind of gravitational waves can SKA look for that the ever-widening array of gravitational wave detectors already looking can't? $\endgroup$
    – uhoh
    Dec 13, 2022 at 11:50
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    $\begingroup$ @ScienceAJ the bounty "expires" in 23 hours, but there's an additional 24 hour grace period where it's invisible but can still be awarded. If you can find some additional information to expand on your comment you may have enough for an answer. $\endgroup$
    – uhoh
    Dec 15, 2022 at 22:14
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    $\begingroup$ I have a link that may be useful that i read a while ago, Link: india.skatelescope.org/gravity-einstein-pulsars. Link: sciencedirect.com/science/article/abs/pii/… $\endgroup$
    – user47732
    Dec 16, 2022 at 8:35

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To answer the first part of your question:

Einstein's theory included predictions about the nature of black holes and the delays they would cause to light travelling through space, so astronomers will aim to compare the theory with the actual measured reality - the ultimate test of General Relativity. If the two are consistent, Einstein wins again. If not, then we know there is something missing in our understanding, opening up a whole new area of astrophysics.

In this case, SKA 101 will track a gravitational wave as it passes through the universe. How you may ask?

Their rapid and regular rotations (referring to pulsars) make pulsars incredibly precise space clocks, as accurate as the best atomic clocks on Earth. They emit a pulse of radio waves like a lighthouse beam, which radio telescopes can detect from Earth. It is this accuracy, and the SKA's ability to detect even the most subtle variations in this caused by a passing gravitational wave, which will hopefully enable this breakthrough in science.

The SKA will be able to time millisecond pulsars (which are both faster and rarer than an average pulsar) typically to 100-nanosecond precision, and even better in some cases. This means it can predict a pulse’s arrival time to better than 10,000,000th of a second, a level of accuracy which is essential to spot the tiny deviations caused by a gravitational wave.

By timing a whole array of pulsars, the SKA will effectively create a cosmic observatory, tracking a gravitational wave as it passes through our galaxy.

[Bracketed phrase is own annotation]

I will also answer @uhoh's question in the comments:

@ScienceAJ how exactly does SKA monitoring pulsars test general relativity in a way that all the other pulsar monitoring telescopes (radio or X-ray) can't? Just what kind of gravitational waves can SKA look for that the ever-widening array of gravitational wave detectors already looking can't?

Answer: Because SKA 101 is the best telescope for the job. It was built to test the theory too. For example, read this short paragraph:

Back in the early 1990s astronomers asked themselves what sort of telescope would be needed to investigate the astronomical questions of the new millennium. The answer: a radio telescope with a total collecting area of one square kilometre and 50 times the sensitivity of any existing telescope. From this came the concept of the Square Kilometre Array (SKA), a project that has drawn together scientists and governments from 20 different countries, and when completed in 2030, will be the world’s biggest radio telescope.

To answer your 2nd question:

The SKA telescopes will initially comprise 131,072 antennas in Australia (known as SKA-Low), which will be built at Inyarrimanha Ilgari Bundara, on Wajarri Country in Western Australia, and 197 dishes to be built in the Karoo in South Africa (known as the SKA-Mid).

When finished, the observatory will consist of thousands of dishes and up to a million low-frequency antennas that will enable astronomers to monitor the sky in unprecedented detail and explore the first billion years after the so-called ‘dark ages’ of the Universe.

I have yet to find out why having so many telescopes enables powerful precision though.

Sources:

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