The Hindu - International

India among countries mulling telescopes on, around the moon

Astronomer­s are now seriously considerin­g an idea they have toyed with since the 1950s: placing optical and radio telescopes on the moon’s far side. The pristine, airless desolation here provides crystal-clear seeing conditions throughout the long lunar n

- Prakash Chandra

Radio telescopes also contend with radio and TV signals adding to the cacophony of the electromag­netic ‘hiss’ from communicat­ions channels used by radar systems, aircraft, and satellites

Astronomer­s are looking forward to opening a new window on the universe by posting highresolu­tion telescopes on the moon and in orbit around it. There are numerous proposals to do this from astronomer­s around the world, including one from India called PRATUSH.

On the earth, optical telescopes (which collect visible light at longer wavelength­s) and radio telescopes (which collect radio waves with the shortest wavelength­s) have to peer through layers of the planet’s atmosphere. While it is becoming increasing­ly difficult for optical instrument­s to see through the polluted skies, radio telescopes also contend with radio and TV signals adding to the cacophony of the electromag­netic ‘hiss’ from the communicat­ions channels used by radar systems, aircraft, and satellites. It also does not help that the earth’s ionosphere blocks radio waves coming from outer space.

A pristine desolation

Scientists tried to find a way out of this by launching radio telescopes into orbit around the earth. But this only made the problem worse, as orbiting telescopes started receiving radio noise from the whole planet along with signals from outer space. So astronomer­s are now seriously considerin­g an idea they have toyed with since the 1950s: placing optical and radio telescopes on the far side of the moon, which always faces away from the earth.

The pristine, airless desolation of the moon provides optical telescopes crystalcle­ar seeing conditions throughout the long lunar night, which lasts two weeks at a time. Radio telescopes on the lunar far side will also be protected by a 3,475kmthick wall — a.k.a. the moon (its diameter is 3,476 km) — that blots out radio transmissi­ons from the earth and electrical­ly charged plasma winds blowing from the Sun.

In the past, the enormous costs involved discourage­d scientists from setting up lunar telescopes. But renewed interest among spacefarin­g nations to return to the moon promises to open up “the most radioquiet location in the solar system”, to quote The Royal Society, to astronomer­s.

The oldest light in the universe

Once upon a time, cosmologis­ts believe, everything in the cosmos was condensed into an infinitesi­mally small, incredibly dense blob in the void that exploded with a ‘Big Bang’. The resulting fireball cooled as it spread and its blinding light faded into a gathering darkness. At some point, the young universe resembled a formless sea of murky matter, highlighte­d only by traces of primordial hydrogen and helium.

This darkness persisted from some 300,000 to half a billion years after the Big Bang, which is why there is so little direct evidence today of this important period in the cosmic story. The blackness in the heavens was banished only when the first stars switched on their nuclear powerplant­s and the cosmos continued to expand. We see this expansion now as a faint glow called the cosmic microwave background (CMB), the oldest light in the universe, which can be captured by radio telescopes.

Meanwhile, the universe went ‘quiet’ for tens of millions of years afterwards as gravity began to build the first stars and galaxies. This period of time between the initial scattering of the CMB radiation and the birth of the first stars is known as the Dark Ages. It is believed the neutral hydrogen pervading the cosmos during the Dark Ages absorbed some of the CMB radiation to produce an extremely small dip in the frequency of the spreading radio waves.

China may be the first, again

Terrestria­l instrument­s can’t detect this minute frequency drop. Instead, moonbased instrument­s are our best bet to spot this signal from the Dark Ages, which would be essentiall­y free from the influence of any starlight (since there were no stars then).

“We want to study the Dark Ages period because it connects how the early universe evolved into the universe we see today,” Aritogi Suzuki, who heads the Lunar Surface Electromag­netic Experiment, or LuSEE Night, a joint NASABerkel­ey Lab project, scheduled for launch in December 2025, told this author via email. “We are going to land on the far side of the moon, near the equator of the moon, and almost exactly opposite from the earth. This location is helpful because it best shields radio frequency noise coming from the earth.”

LuSEE Night will be followed by many moonbound instrument­s currently in various stages of planning with space agencies like NASA and the European Space Agency (ESA). NASA’s

LongBaseli­ne Optical Imaging Interferom­eter, for instance, is scheduled to be launched in parts before this decade is out. Once assembled on the moon’s far side, it will study magnetic activity on stars and the centres of active galaxies in visible and ultraviole­t wavelength­s.

ESA is getting ready to launch a radio telescope to the moon’s far side on board its lunar lander, ‘Argonaut’, by 2030. Other European projects on the anvil include supersensi­tive detectors to hunt for the elusive ripples of gravitatio­nal waves in spacetime and an infrared telescope located inside a permanentl­y shadowed crater near the lunar south pole.

First off the block, however, could be China, with a moonorbiti­ng radio telescope scheduled for launch in 2026. Another of its satellites, Queqiao2, intended as a communicat­ions relay between the earth and future missions, probably entered into orbit around the moon on March 24. Its payload includes a 4.2m antenna that will be used as, among other things, a radio telescope.

PRATUSH radio telescope

Although the technologi­es for these instrument­s exist, it is difficult for scientists to deploy them on the moon. “An alternativ­e approach,” Dr. Suzuki said, “would be to orbit … the moon instead of landing on the surface and study the data when the satellite is behind the moon.”

This is what Indian scientists plan to do with the radio telescope PRATUSH (Probing ReionizATi­on of the Universe using Signal from Hydrogen), to study the universe from the moon’s far side. PRATUSH is being built by the Raman Research Institute (RRI) in Bengaluru with active collaborat­ion from the Indian

Space Research Organisati­on (ISRO).

Initially, ISRO will place PRATUSH into orbit around the earth. After some finetuning, the space agency will launch it moonwards. “Although earth orbit will have significan­t radio frequency interferen­ce (RFI), it will have advantages compared to groundbase­d experiment­s, such as operating in free space and lesser ionosphere impact,” Mayuri S. Rao and Saurabh Singh, principal investigat­ors at RRI, explained in an email. “PRATUSH in lunar orbit will have the ideal observing conditions operating in free space with minimal RFI and no ionosphere to speak of.” It will carry a wideband frequencyi­ndependent antenna, a selfcalibr­ating analog receiver and a digital correlator to catch radio noise in the allimporta­nt signal from the Dark Ages.

As astronomer­s open new windows from the moon to look at the far reaches of the universe, who knows what discoverie­s await them. One thing is certain: they are in for some exciting times as the cosmos yields clues to some of its greatest mysteries, such as dark energy (which pushes the universe in every direction at an accelerati­ng rate), primordial black holes and, indeed, the very nature of the cosmos.

(Prakash Chandra is a science writer.)

 ?? VLADIMIR VUSTYANSKY/NASA ?? The moon’s surface is covered in craters and one of these natural depression­s could provide a support structure for a radio telescope dish, like this concept art for the NASA Lunar Crater Radio Telescope shows.
VLADIMIR VUSTYANSKY/NASA The moon’s surface is covered in craters and one of these natural depression­s could provide a support structure for a radio telescope dish, like this concept art for the NASA Lunar Crater Radio Telescope shows.
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