
Fast radio bursts (FRBs) are one of the strangest phenomena we’ve yet discovered in the cosmos – and they are also one of the most recent, the first one only being detected in 2007.
FRBs produce pulses in the radio part of the electromagnetic spectrum that last just a few thousandths of a second but produce as much energy as the sun does in a year. They are believed to originate within magnetars, a kind of ultra-dense neutron star (itself the collapsed remnants of a star) with an exceptionally strong magnetic fields which can warp their behaviour; however, this has yet to be confirmed.
Most FRBs have been detected originate in galaxies other than our own, and are very mixed in nature. Some FRBs emit energy just once but others can do so in repeated bursts. The thinking is that their intense bursts of energy is the result of some complex interaction between a magnetar’s massive magnetic field – trillions of times more powerful than Earth’s – and the outer layers of the neutron star itself, causing a massive explosion we later detect as radio waves.
One FRB that is known to recurring bursts is called FRB 121102, and is located in a dwarf galaxy 3 billion light-years from Earth. It was selected as a candidate for study using China’s massive Five-hundred-metre Aperture Spherical radio Telescope (FAST), which only became operational in 2020. The hope was study of FRB 121102 would reveal the secrets of these strange objects, including their source and cause. Instead, the study has actually deepened the mystery.

Prior to FAST turning its attention on FRB 121102, recorded observations by the likes of (the now defunct) Arecibo radio telescope suggested it gave off bursts of 10 radio pulses on a non-regular basis. However, FAST is so sensitive, found FRB 121102 can generate up to 117 pulses per hour, with some just a few thousandths of a second apart, with 1,652 bursts detected in the first 60 hours of observations!
Exactly how it can do this remains a mystery – but it suggests that the current theory of magnet field / star “surface” interactions is incorrect. Such interactions would generate violent outbursts of matter from the magnetar, and these would have to collapse to prevent them interfering with further bursts – and a few thousands of a second is too short a period in which this could happen.
No direct conclusions can be drawn from the study of FRB 121102; the international team behind it stating they now need to use FAST to study other repeating FRBs to see if they can find similar “hidden” bursts from them, in order that a more complete picture might start to be built up as to what might be happening, why, and how.
The “‘Fridge” That Skimmed Earth
I’ve often written about NEOs, or near-Earth objects – chunks of rock in a range of sizes from just a few metres through to a few kilometres – that orbit the Sun in a manner that means that periodically cross Earth’s orbit or can pass relatively close to us. Such is the threat posed by these objects should one of the large ones actually collide with Earth, considerable effort has been put into finding and tracking them, using their close passages to Earth to better track and predict their orbits in years to come.
As a result, many of the large NEOs have indeed been located and tracked; but there are still many hundreds, if not thousands, which, while not threatening all of civilisation on the planet, could still do much to totally ruin people’s day were they to enter the Earth’s atmosphere and explode under air pressure or even survive and strike a centre of population.
October 24th, 2021 saw a small reminder of this threat, when a chunk of rock about the size of a refrigerator and dubbed Asteroid 2021 UA1, skimmed past Earth, passing just 3,000 km above Antarctica. While the rock was too small to cause any real damage, had it entered the atmosphere, it would likely have completely burned up, it was not actually spotted until it was moving away from Earth once more, its approach having been lost in the glare of the Sun – hence why it acted as a reminder of the threat poised by larger NEOs – that we might not actually see them before them become a problem.
This is what happened in 2013, when a cometary fragment roughly 20 m across entered the Earth’s atmosphere to explode at an altitude of 26 km over the the Russian oblast of Chelyabinsk. The blast yield of explosion was 400–500 kilotons of TNT, with the shockwave it generated damaging some 7,200 buildings in six cities across the region and injuring more than 1,500 people.
The passage of Asteroid 2021 UA1 is also a timely reminder that later in November, NASA plans to launch the Double Asteroid Redirection Test (DART), an attempt to test a method for diverting asteroids by hitting them with high-speed remote-controlled vehicles, and I’ll have more of that mission in an upcoming Space Sunday report.
Selected Round-Up
Hubble Remains in Safe Mode
As I noted in my last Space Sunday update, the veritable Hubble Space Telescope (HST) entered a “safe” mode intended to protect its science capabilities on October 25th, 2021. With science activities suspended, the instruments are said to be in “good health”. However, in providing an update to the situation, NASA revealed HST actually suffered two glitches in relatively short order.

On October 23rd, the telescope’s science instruments issued an error code indicating the loss of an automated synchronisation message issued by the main computer to provide timing information to the science instruments, allowing them to properly respond to commands. This issue appeared to be corrected when a command was sent to the science instruments ordering them to reset; however, the October 25th issue appears to be related, in that “multiple losses of synchronisation messages” were reported immediately prior to the safe mode being triggered.
Right now, Hubble engineers have no idea what triggered the loss of the messages, and the focus is on trying to obtain further data from HST so a more proper diagnosis of what occurred, and what is required to bring Hubble back on-line.
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