Tag: Spaceflight

Monday, December 21st, the winter solstice, saw Jupiter and Saturn reach their closest point of mutual approach to one another when viewed in our evening skies, in what is referred to as a great conjunction.

I covered the event in some detail in my previous Space Sunday report, noting that 2020 would see the two planets appear to come with 6 arc minutes of one another as they lay low over the south-western horizon in last light following sunset.

Unfortunately, British weather being what it tends to be, I didn’t get to see things on the night thanks to cloud and rain.  To add insult to injury, the skies were clear just 40 km away, allowing friends to witness the event on the night, while the rain and cloud continued here most of the rest of the week, preventing me from getting a further look at the two planets as they dropped ever closer to the horizon. Ho hum.

Fortunately, however, many around the world did have clear skies and captured the event using cameras equipped with telephoto lenses or attached to telescopes. I’ve included a handful of my favourites shots here.

The event was also captured on film by Jason De Freitas, who captured the space between Jupiter and Saturn being neatly “cut” by the passage of the International Space Station.

ET Probably Isn’t Radioing Us

A radio signal detected in a part of the sky that neatly aligns with our closest stellar neighbour,  Proxima Centauri, is unlikely to be of extra-terrestrial origin.

The radio burst was detected in  April-May 2019 by the Parkes Radio Telescope in  Australia, one of two radio telescopes used by the Breakthrough Listen project, which since 2015 has been listening to the one million closest stars to our own in an attempt to pick up artificial radio signals that might indicate extraterrestrial intelligence.

At the time the signal was detected, the telescope was engaged in radio observations of Proxima Cantauri, some 4.2 light years away, and a star known to have two planets orbiting it, one of which – Proxima b – is a rocky world about 1.7 times the size of Earth that sits within the star’s  habitable zone.

Parkes wasn’t listening for radio signals at the time they were picked up, but was engaged in radio observations of flare activity from the star. However, when detected, the signal was immediately intriguing due to its relatively narrow frequency – 982.002Mhz – which ruled out it being caused by known natural phenomena. In order to verify it, the Breakthrough Listen team received permission to “nod” the telescope dish.

This is a common technique used to verify radio signals that involves deliberately swinging the receiving dish away from a signal for a period of time, and then back towards it in order to see if it can be re-acquired (indicating it is not an artefact of the telescope itself), and to measure whether the signal has moved relative to the dish (which would indicate the source is likely in Earth’s orbit). In this case, the signal was reacquired, with measurements suggesting it could be emanating from Proxima b.

When news of the signal, and the on-going analysis to try to determine it’s likely point of origin / cause, was anonymously leaked recently, it was picked up by a number of media outlets and caused something of a stir. However, before ET Hunters get too excited, there are a number of additional facts to consider.

Firstly, it is devoid of any modulation – and so is likely devoid of any meaningful data, were it indeed to by an extra-terrestrial, which makes sending it a little pointless. Secondly, it was entirely transient; following the period of initial detection in April / May 2019, it was “lost”, and has never been re-acquired. Were it a deliberate signal, it would not be unreasonable to expect it to remain fairly constant in terms of detection, either by Parkes or (preferably) other centres around the world.

But the biggest counts against it being ET “‘phoning home” (or at least us), lies with the fact that the signal came from the general direction of Proxima Centauri. As our nearest, and oft-observed stellar neighbour, the star has been under observation for decades, and nary a once have we received anything amounting to an peep out of it that might suggest aliens are playing with radio systems there.

More particularly, however, is the fact that Proxima Centauri is a red dwarf star. As I’ve noted numerous times in these pages, these  M-class stars are prone to exceptionally violent solar flare. Given the close proximity of Proxima b to its star, these flares would likely, at a minimum, be bathed in hard radiation, and at worse, completely rip away the planet’s atmosphere within a period of around 100-200 million years. Therefore, it is highly unlikely the planet really is the point of origin for the signal.

instead, the most likely explanations for the signal are that it might either be something like the carrier wave from a long-forgotten piece of orbital debris of human manufacture or – mostly likely – actually originated on Earth, with conditions in the upper atmosphere serving to “bounce” it into the Parkes Telescope sphere of detection.

The Breakthrough Listen team and their partners certainly lean towards the latter as an explanation, although as noted,  they are still analysing the data gathered on the signal.

This is not a natural phenomenon—I haven’t seen the data, but if it passed BL’s tests then it’s too narrowband to be natural. It’s definitely caused by technology. But it’s almost certainly our own technology.

– Jason Wright, Professor of Astronomy and Astrophysics at Penn State University

Continue reading “Space Sunday: conjunctions, radio signals and budgets” →

For those who have not already seen it, the next two weeks present an opportunity to witness a unique event – a very close conjunction between Jupiter and Saturn.

“Conjunction” is the term astronomers used to describe two astronomical objects or spacecraft having either the same right ascension or the same ecliptic longitude, and thus when seen from Earth, appear to be close together.

With the planets, such events are not especially rare – in fact as they and the Earth circle the Sun, conjunctions between Jupiter and Saturn tend to occur once every 20 years. However, most of these only see Jupiter and Saturn close to around one degree of one another, or about one-fifth the diameter of the Moon as seen from Earth. But sometimes they appear to get much closer, creating what is referred to as a “great conjunction”. This year, the two planets will appear to be just 6 arc minutes apart as seen from Earth on December 21st, 2020; so “close” (remembering that their respective orbits around the Sun will still be separated by 883 million km), they will almost, but not quite, appear as a single point of light when seen with the naked eye.

These “great conjunctions” occur, on average, once every 300-400 years, although such is the nature of orbital mechanics, they can actually occasionally occur more frequently, or have longer time gaps between them. As it is, the last time Jupiter and Saturn appeared as close as the will be between December 20th and 22nd was in 1623, not long after Galileo had observed both planets – although he was unable to witness the event, as the rising Sun would have rendered them invisible in its glare.

What is most rare is a close conjunction that occurs in our night time sky. I think it’s fair to say that such an event typically may occur just once in any one person’s lifetime, and I think ‘once in my lifetime’ is a pretty good test of whether something merits being labelled as rare or special.

Astronomer David Weintraub

However, the two planets can appear to be much closer. In 1226, and in the skies over the Mongol Empire, when the planets appear to be just 2 arc minutes apart.

Tracing these great conjunctions back in time reveals that Jupiter and Saturn may well have played a role in the legend of the Star of Bethlehem. In 7 B.C. not one, but three great conjunctions occurred, with the two planets again being within 2 arc minutes of one another as seen from Earth.

The first occurred in May of that year, when Jupiter and Saturn appeared as a morning star over the middle east. As  the Magi were practitioners of (among other things) astronomy and astrology – both at that time pretty much joined at the hip – such an event may well have caused them to start out on their long journey towards Judea, the second conjunction, in September of the year, encouraging them to continue. The third conjunction occurred in December, 7 B.C., the time at which they were said to have met with Herod the Great.

This year’s conjunction will be not long after sunset, with the two planets located low over the south-west horizon. With a reasonable telescope or good pair of binoculars, you’ll have an ideal opportunity to see both planets and their major moons in the same field of view.  Should you do so, you’ll be looking at over 90% of the planetary mass of the entire solar system.

Beyond the 21st, the two planets will gradually move “apart” as noted, until by the 25th December, they’ll be separated in the night sky by roughly the diameter of a full Moon, and will continue to draw apart relative to Earth as they pass below the horizon.

And if you miss this close conjunction between the two, the next will be along in a relatively (and unusually) short period, occurring on March 15th 2080. The next time they’ll be as apparently close as they were in 7 B.C. will be on Christmas Day, 2874.

Continue reading “Space Sunday: Conjunctions, China & the Sun as a telescope” →

On Wednesday, December 9th, SpaceX Starship prototype SN8 finally took to the skies in what was to be a very mixed ascent to around 12.5 km altitude and return to Earth.

The much anticipated flight of the prototype vehicle, weighing approximately 672 tonnes with its partial fuel load, was far more successful than SpaceX had anticipated, even if the vehicle was lost in what SpaceX euphemistically calls a “rapid unplanned disassembly” or RUD.

The first attempt at a launch of the 50m tall vehicle was made on Tuesday, December 8th; but this was scrubbed after a pre-flight engine issue caused an automatic shut-down on all three Raptor motors. The second launch attempt, in the morning of Wednesday, December 9th, was aborted just 2 minutes and 6 seconds before engine ignition when a light aircraft strayed into the no-fly zone around the SpaceX facilities in Boca Chica, Texas.

However, at 16:00 CST (22:00 GMT) that day, the countdown resumed, and at 16:45:26 p.m. CST (22:45:56 GMT), the three Raptor engines on the vehicle ignited and ran up to around 80% thrust, lifting prototype SN8 into the air.

The entire flight was live streamed by SpaceX, with the initial ascent proceeding as anticipated. At 1 minute and 40 seconds into the flight, one of the Raptor engines shut down and gimballed itself away from the remaining two operating motors. 94 second later, a second of the Raptors did the same. At the time, some pundits commenting on the flight speculated the shut-down indicated something was amiss.

In actual fact, both engine shut-downs were planned. As the vehicle was flying with around 1/2 its normal fuel load, and getting lighter at the rate of 2.2 tonnes every second, the engines were shut down to reduce SN8’s thrust-to-weight ratio, naturally reducing its rate of ascent.

Even so, SN8 continued upwards under the thrust of the one remaining Raptor – Number 42, the latest and most modern Raptor engine evolution, with the vehicle’s reaction control system (RCS) firing thrusters around its hull in order to stay upright, until it reached a point where it was effectively hovering.

What happened next was one of the two most incredible sights witnessed in the testing of a space vehicle: as SN8 started to drop vertically backwards, Raptor 42 gimballed to direct its thrust at an angle, working with the RCS system to tip the entire vehicle over until it was falling more-or-less horizontally. At this point, the fore and aft flaps came into their own, working in tandem to hold the vehicle steady, much like a skydiver uses their arms and legs to maintain stability.

This skydive / bellyflop (as some unkindly refer to it) is how a Starship will make a return from orbit. Dropping into the atmosphere with the fore and aft flaps folded back against the hull to minimise their exposure to the fictional heat of atmospheric  entry, an operational starship will be protected by heat shield tiles along its underside, after which the flaps fold out, acting as air brakes to slow the vehicle’s velocity as well as keeping it stable.

Dropping back through the atmosphere for almost two minutes, SN8 then completed the second most incredible sight seen in the testing of a spacecraft when, six minutes after launch, two of the Raptor motors re-ignited, using fuel from two small “header” tanks. These, coupled with the vehicle’s RCS tipped SN8 back to an upright position just 200 metres above ground.

The idea had been for the vehicle to then descend tail-first over the landing pad, deploy its landing feet and touch-down. However, it was at this point things went wrong. With just tens of metres to go, one of the two operating engines shut down. For several seconds, the remaining engine fought to maintain vehicle stability, its exhaust plume turning bright green. Seconds later, its landing legs having failed to deploy, SN8 slammed into the landing pad and exploded in the RUD SpaceX thought might occur at some point in the flight.

Initial analysis of data from the flight suggests that the header tanks suffered a pressurisation issue that prevented them pushing sufficient fuel into the two Raptor engines, causing one to shut down completely. The green plume from the second motor is thought to be one of two things: either that a) as the motor was so starved of fuel, it started consuming itself, material inside its turbopumps turning the exhaust green; or that b) as one engine shut-down unexpectedly, the second started gimballing wildly to try an maintain the vehicle’s orientation, and in doing so, smashed its engine bell into the other motor, exposing its copper cooling circuits, which caught fire and turned the exhaust plume green.

Continue reading “Space Sunday: the flight of SN8 and a round-up” →

On Saturday, December 5th (Sunday December 6th local time in Australia), Japan’s Hyabusa2 successfully returned samples gathered from the asteroid 162173 Ryugu.

It marked the culmination of a six-year mission to reach the asteroid, gather samples and then make a return to Earth – although as I mentioned in my last Space Sunday update, the return of the samples does not mark the end of the road for Hyabusa2.

Travelling at 43,190 km/h – too fast to enter orbit – the spacecraft released the 40 cm sample return capsule on the night of Friday December 4th, 2020, whilst still some 220,000 km away. With its cargo duties  discharged, Hyabusa2 performed an engine burn to start it on its way for a rendezvous with asteroid (98943) 2001 CC21 in 2026, before flying on to meet with 1998 KY26, in 2031.

With no means to slow down, the sample capsule slammed into the upper reaches of Earth’s  atmosphere at 17:28 GMT on Saturday, December 5th (the earlier  hours of Sunday December 6th in Japan and Australia). Following re-entry, that helped the capsule to slow to supersonic speeds, the capsule dropped to an altitude of 10 km before deploying its landing parachute, touching down in Australia at 17:47 GMT (04:17 a.m. local Australian time on December 6th), JAXA officials said.

Radio tracking systems deployed around the expected landing site were able to follow the capsule down allowing its landing point to be triangulated accurately so that recovery helicopters could quickly move in and retrieve the capsule and its cargo.

Following recovery, work started on capsule assessment and preparations to transfer it to the Japanese Space Agency’s (JAXA) Extraterrestrial Sample Curation Centre, a purpose-built facility designed to house and study cosmic material brought home by space missions. Here some of the samples – believed to measure just a few grams – will be studied by Japanese scientists, and some will be distributed to laboratories around the world, where scientists will study it for clues about the solar system’s early days and the rise of life on Earth.

The mission marks only the second time a dedicated sample return mission has brought samples of an extra-terrestrial body back to Earth, the first being the original Hyabusa mission, which returned samples from asteroid 25143 Itokawa in 2010. However, it will not be the last. China’s Chang’e 5 mission will shortly be on its way back to Earth with samples gathered from the Moon (see below for more), and NASA’s OSIRIS-REx will be returning samples from asteroid from 101955 Bennu in 2023.

Arecibo Collapses

When it came, it came suddenly and without warning – yet purely by chance, a drone was on hand to capture the event as it happened.

I recently wrote about the fact that, having lost a primary and secondary support cable that were helping to keep its receiving platform aloft, the Arecibo observatory had been declared unsafe and was to be decommissioned, the replacement of the primary load-bearing cables – one of three in total – being determined to be both difficult and dangerous.

Due to the risk of the 900-tonne receiving platform collapsing onto the dish, built into a hilltop karst sinkhole, it had been hoped the telescope could be decommissioned and dismantled, possibly through the use of controlled demolition, sooner rather than later, lest further cables – including one of the two remaining primary cables – gave way.

But on December  1st, before decommissioning plans could be finalised, one of the remaining suffered a catastrophic failure, sending the receiving platform plummeting into the telescope’s 305-metre diameter dish.

The event took place shortly before 07:30 in the morning, local time – and by chance, engineers were monitoring the telescope’s cable system from the main control room and via an aerial drone positioned above the cable housings on the receiving platform when the cable failed. As a result, the entire collapse was caught on camera from two locations – although the drone had to be hastily moved away from the receiving platform as the collapse started.

Swinging towards the ground on the remaining support cables, the receiving platform disassembled as it fell, the bulk falling the 150m into the aluminium dish, the support frame swinging to smash into the the side of dish, the trailing cables also doing considerable damage. Such was the force of the failure, the mass of the platform tore away the top section of one of the support towers and brought about the complete collapse of another.

Continue reading “Space Sunday: returns and a collapse” →

Sunday, November 15th saw the official start of a new era in low-Earth orbit space transportation with the launch of the NASA / SpaceX Crew-1 mission to the International Space.

Originally scheduled for launch on Saturday, November 14th, the Crew-1 mission was delayed due to weather causing concerns about the recovery of the Falcon 9 launch vehicle’s first stage. However, at 19:27 local time on Sunday (00:27 GMT on Monday, November 16th), the Falcon 9 topped by the Crew Dragon and its crew of four – NASA astronauts, Mike Hopkins, Victor Glover, Shannon Walker and Japanese astronaut Soichi Noguchi – lifted off from the SpaceX leased Pad 39A at Kennedy Space Centre, the first stage of the rocket making a successful return to Earth and landing aboard the autonomous drone ship Just Read The Instructions.

Nine minutes after launch, the Crew Dragon capsule – named Resilience by the crew – achieved an initial orbit, and the crew followed a long tradition of space flight dating back to the first manned space mission, and revealed their “zero gee indicator”, a Baby Yoda plushy toy from the TV series, The Maldorian.

The use of toys and dolls as such indicators goes back to the flight of Yuri Gagarin and his flight aboard Vostok-1 in April 1961.  Gagarin carried a small doll into orbit out of curiosity, as he wanted to see what floating in the micro-gravity of space looked like. However, his practice was copied by other Soviet cosmonauts, and in turn by NASA missions, with crews on the Crew Dragon continuing the tradition – Doug Hurley and Bob Behnken carried a plushy planet Earth on their trip to the ISS earlier in  2020 during the Crew Dragon certification flight.

While not confirmed, it is believed the selection of Baby Yoda was due to back-up crew member Kjell Lindgren. A long-time Star Wars fan, Lindgren had used a model of R2D2 as a zero-gee indicator during a 2015 Soyuz flight to the ISS and while aboard the station, persuaded the rest of the crew to dress up as Jedi Knights for a special NASA promotional poster.

It’s been a tough year. And the fact that … SpaceX and NASA were able to get our spacecraft ready to go, the rocket ready to go, throughout this year, throughout the pandemic, and all of that — we were inspired by everybody’s effort to do that. So that’s why we named Resilience, and we hope that it puts a smile on people’s faces, it brings hope to them. Baby Yoda does the same thing. I think everybody, when you see him, it’s hard not to smile, and so it just seemed appropriate.

– Mission commander Mike Hopkins explaining the choice of name for the Dragon
capsule and the selection of Baby Yoda as the zero-gee indicator.

It  took some 27 hours for Resilience to catch up with the ISS, finally rendezvousing and docking with the station at 11:01 EST on Monday, November 16th (04:01 GMT, November 17th). Following a further 2 hours of post-flight checks and preparations both in the capsule and on the station, the forward hatch on Resilience was opened and the four crew were invited aboard the ISS. In doing so, they set a new record for the space station: the first time it has been occupied by full-time crew  totalling seven  people. This is actually one more person than the ISS is designed to accommodate, so Crew-1 commander Mike Hopkins is sleeping aboard the Resilience.

The Expedition 64  crew will remain on the ISS for a 6-month rotation period, Hopkins and his crew joining NASA astronaut Kate Rubins and Russian cosmonauts Sergey Ryzhikov and Sergey Kud-Sverchkov, who arrived at the ISS on October 14th, aboard the Soyuz MS-17 – a mission which was itself a record-setter, rendezvousing with the station just three hours after launch, utilising Russia’s “ultrafast” ISS launch and rendezvous flight plan for the first time.

Once aboard the station, the crew wasted little time in getting down to work. On November 18th, Ryzhikov – currently in overall command of the ISS – and Kud-Sverchkov made a 6-hour 48-minute spacewalk that inaugurated the operational use of the Poisk “mini research” module as an airlock.

As I noted in my previous Space Sunday update, Poisk has been delivered as an airlock / docking module in 2009. It is one of two such units attached to the Russian Zvezda module, the other being the Pirs airlock / dock, deployed to the ISS in 2001. Up until the Ryzhikov / Kud-Sverchkov EVA, Poisk had only been used as a docking module, spacewalks generally being conducted via the Pirs module.

However, Pirs is due to be removed from the ISS in 2021, so it can be de-orbited to burn up in the upper atmosphere using one of the Russian Progress resupply vehicles. It is due to be replaced by the Nauka Multipurpose Laboratory Module (MLM) – although there are some doubts about this module, as its launch has been delayed so much, several of its systems are at the end of their warranty period.

In  particular, the Poisk spacewalk was to start the process of decommissioning Pirs, by moving vital communication equipment and cabling from that module and connecting them to Poisk, allowing it to become the primary Russian EVA airlock.  As  well as this work, Ryzhikov and Kud-Sverchkov retrieved hardware used to measure space debris impacts, and repositioned an instrument used to measure the residue from thruster firings. The EVA marked the 47th Russian space walk in support of ISS operations, and the 232nd ISS spacewalk overall.

Continue reading “Space Sunday: a Dragon, a telescope and a heavenly princess” →