Space Sunday: solar events; black holes;+ updates

NASA’s Solar Dynamics Observatory captured these two views of massive solar flares, registering X5.8 and X1.5, respectively, on May 11th, 2024. Credit: NASA

We are currently approaching the mid-point in Cycle 25 of the Sun’s 11-year cyclical solar magnetic activity. These are the periods in which observable changes in the solar radiation levels, sunspot activity, solar flare and the ejection of material from the surface of the Sun, etc., go from a fairly quiescent phase (“solar minimum”) to a very active phase (“solar maximum”) before declining back to a quiescent period once more to repeat the cycle again. The “11-year” element is the average length of such cycles, as they can be both a little shorter or a little longer, depending on the Sun’s mood. They’ve likely been occurring over much of the Sun’s life, although we only really started formally observing and recording them from 1755 onwards, which is why this cycle is Cycle 25.

This cycle started in December 2019, and is expected to reach its mid-point in July 2025, before declining away in terms of activity until the next cycle commences in around 2030. Predictions as to how active it might be varied widely during the first year or so, (2019-2021), with some anticipating a fair quite cycle similar to Cycle 24; others predicted it would be more active – and they’ve been largely shown to be correct. And in this past week, the Sun has been demonstrating that while it might be middle-aged, it can still get really active, giving rise to spectacular auroras visible from around the globe.

The Aurora Australis (Southern Lights) seen over waters of Lake Ellesmere on the outskirts of Christchurch, New Zealand on May 11th, 2024. Credit: Sanka Vidanagama via Getty Images.

The cause of this activity carries the innocent name of AR3664 (“Active Region 3664”), a peppering of sunspots – dark patches on the solar surface where the magnetic field is abnormally strong (roughly 2,500 times stronger than Earth’s) – on the Sun, and one of several such groups active at this time. However, AR 3664 is no ordinary collection of sunspots. In a 3-day period between May 6th and May 9th, it underwent massive expansion, growing to over 15 Earth diameters in length (200,000 km), and at the time of writing is around 17 Earth diameters across.

This rapid expansion gave rise to a series of huge dynamic solar flares on the 10th/11th May, with the first a massive X5.8 class flare – one of the most powerful types of solar flare the Sun can produce. Accompanying the flares have been interplanetary coronal mass ejections, which since Friday have been colliding with Earth’s magnetosphere, causing geomagnetic storms and auroras, giving people spectacular night skies.

The first of these geomagnetic storms was classified G5 – the highest rating, and the first extreme storm of this type to strike our magnetosphere since October 2023, when damaged was caused to power infrastructure and services in several countries, including Sweden and South Africa. This event caused high-frequency radio blackouts throughout Asia, Eastern Europe and Eastern Africa, and disrupted GPS and other commercial satellite-directed services, although overall, the impact was fairly well managed.

Aurora Borealis (Northern Lights) seen over Vienna during the May 11th geomagnetic storm. Credit: Max Slovenchik via Getty Images

Further storms were experienced through Friday, Saturday and Sunday (10-12th May), varying between G3 and G4 as a result of further CMEs from AR 3664, together with further solar flares in the X4 range. Storms and auroras are expected to continue through until Monday, May 13th, after which AR 3664 will slip around the limb of the Sun relative to Earth.

Thus far, cycle 25 has seen daily sunspot activity around 70% higher during the peak period when compared to Cycle 24, although most of the resultant flares and CMEs have tended to be well below the extreme levels of the last few days. Whether AR 664 marks the peak of events for this cycle, or whether we’ll have more is obviously a matter for the future – but if you’ve not had the opportunity to witness the aurora, the nights of the 12th/13th May might be a good opportunity to do so!

High frequency radio blackouts occurred throughout Asia, eastern Europe and eastern Africa shortly after the X5.8 solar flare of May 11th, 2024. Credit: NOAA/SWPC

AR 3664 is, coincidentally, believed to be around the same size as the sunspot cluster thought to have been responsible for the 1859 Carrington Event, the most intense geomagnetic storm in recorded history (Cycle 10), resulting in global displays of aurora and geomagnetic storms, the latter of which massively disrupted telegraphic communications across Europe and North America (and lead to reports of telegraph operators getting electric shocks from their morse keys and still being able to send and receive messages even with their equipment disconnected from the local power supply!).

Take a Plunge into a Black Hole – Or Fly Around it

Black holes are mysterious (and oft misunderstood) objects. We all know the basics – they are regions on spacetime where gravity is so great that not even light can escape past a certain point (the event horizon) – but what would it be like to fall into one or pass into orbit around one?

In the case of the former, we may think we know the answer (stretching / spaghettification, death + a different perspective of time compare to those observing us from a safe distance), but this is not actually the case for all black holes; it comes down to the type you fall into.

In the case of stellar black holes, formed when massive stars collapse at the end of their life cycle, it’s unlikely you’ll ever actually reach the event horizon, much less fall into it; the tidal forces well beyond the event horizon will rip you apart well in advance. But in the case of supermassive black holes (SMBHs), such as the one lying at the centre of our own galaxy (and called Sagittarius A*) things are a little different.

The first direct image of a supermassive black hole, found in the galactic core of Messier 87, released in 2019 by the Event Horizon Telescope Collaboration. The orange colour is the accretion disk of matter surrounding the black hole some distance from its event horizon. Messier 87 is a giant galaxy 53 million year-years from Earth. Credit: EHO

These black holes are so mind-bogglingly big that the gravity curve is somewhat “smoother” than that of a stellar black hole, with the tidal forces more predictable, possibly allowing the event horizon to be reached and crossed (giving rise to spaghettification). Even so, trying to define what goes on in and around them is still somewhat theoretical and based on abstracted concepts drawn from indirect observation and complex maths.

So, to try to get a better handle on what the maths and theories predict should happen around something like a SMBH – such as falling into the event horizon or being able to orbit and escape such a monster, NASA astrophysicist Jeremy Schnittman – who is one of the foremost US authorities on black holes – harnessed the power of NASA’s Discover supercomputer (with over 127,000 CPU cores capable of 8,100 trillion floating point operations per second), and used available data on Sagittarius A* to generate two visual models which make for a fascinating study.

In the first, the camera takes us on a ride from a distance of some 640 million km from the SMBH (a point at which its gravity is already warping our view of the galaxy), through the accretion disk and into a double orbit around the black hole before gravity is allowed to pull the camera in and across the event horizon. It provides a unique insight into how the galaxy around us would appear, how time and space are bent (and eventually broken), whilst also offering an enticing view of another black hole phenomenon: photon rings – particles of light which are travelling fast enough to fall into orbit around the black hole and loop around it more than once before escaping again.

I’ll say no more here, the video explains itself.

In the second video (below), the camera passes around the black hole for two orbits before breaking away, just like the light particles responsible for the photon rings. As well as the visualisation of the warping effect gravity that a black hole has on light, both videos also demonstrate the time dilation effect created by the SMBH’s gravity.

In the “orbital” video, eat loop around the black hole takes – from the camera’s perspective – 30 minutes to complete. However, from the perspective of someone watching from the video’s starting point, 640 million kilometres away, each orbit appears to take 3 hours and 18 minutes. Meanwhile, in the “fall” video, from the camera’s perspective, the drop from orbit to event horizon lasts 10 minutes. However, from anywhere beyond the black hole, it never ends; the object appears to “freeze” in place the moment it touched the event horizon (even though it is ripped apart nanoseconds after crossing the event horizon).

And these dilation effects assume the black hole is static; if it happened to be rotating – then in the case of camera orbiting the black hole and then braking free, mere hours may seem to have passed – but to the observers so far away, years will have seemed to pass.

Updates

Starliner CFT-1 Delayed

Boeing’s CST-100 Starliner continues on the rocky road to flight status. As I reported in my last Space Sunday, CST-100 Calypso was due to head off to the International Space Station (ISS) on Monday, May 6th, carrying NASA astronauts Barry “Butch” Wilmore and Sunita “Suni” Williams on a Crewed Flight Test (CFT) designed to pave the way for the spacecraft to be certified for operations carrying up to 4 people at a time to / from the ISS.

Whitmore and Williams departing the Neil A. Armstrong Building at Kennedy Space Centre in preparation to board the crew bus from the drive to neighbouring Canaveral Space Force Station for the (subsequently scrubbed) CST-100 launch attempt, May 6th, 2024. Credit: NASA

Only it didn’t; the launch was scrubbed some 2 hours ahead of lift-off due to issues in the flight hardware – although this time, thankfully, not with the vehicle itself. The fault lay within an oxygen relief valve in the Atlas V’s Centaur upper stage, of the Atlas V launch vehicle. The valve was cycling open and closed repeatedly and so rapidly that crew on the pad could hear it – describing is as a “buzzing” sound.

Initially, it had been hoped that the issue could be rectified without moving the vehicle back from the pad at Cape Canaveral Space Force Station, and that a launch date of May 10th could be met. However, by May 8th, attempts to reset the valve via software and control intervention had failed, and ULA – the company responsible for the Atlas V and its upper stage (ironically, the Centaur is produced by Boeing, one of the two partners in ULA) – decided the stack of rocket and Starliner would have to be rolled back to the Vertical Integration Facility (VIF) close to the pad, so the entire valve mechanism can be replaced.

Boeing’s Starliner spacecraft and its Atlas V rocket returning to the Vertical Integration Facility at Cape Canaveral Space Force Station, May 8th, 2024, so a faulty oxygen relief valve on the launch vehicle can be replaced. Credit: NASA

As a result, and at the time of writing, the launch is now scheduled to take place on Friday, May 17th, with a lift-off time targeting 23:16 UTC.

Hubble Back, TESS Down, Up, Down, Up

On April 28th, I reported that the Hubble Space Telescope (HST) had entered a “safe” mode following issues with one of its three remaining pointing gyroscopes. As noted in that piece, the gyroscopes are a vital part of HST’s pointing and steadying system, and while it generally requires three such units for Hubble to operate efficiently, it can get by at a reduced science capacity with only two – or even one, if absolutely necessary – functional gyro.

These gyros do naturally wear out – six brand new units were installed in 2009 (pairs of primary and back-up), but since then, three have permanently failed, and one of the remaining three has been having issues on-and-off since November 2023. Fortunately, in the case of that issue, and now with the April 23rd problem, engineers on Earth were able to coax the gyro back into working as expected. Thus, in the case of the latter, Hubble was back on science gathering duties with all instruments were operational on April 30th.

Hubble (l) and TESS: troubled times. Credit: Robert Lea

Quite coincidentally, another of NASA’s orbiting observatories – the Transiting Exoplanet Survey Satellite (TESS) – also entered a “safe” mode on April 23rd, 2024 – the second time in April its did so. On April 8th, 2024 TESS suddenly safed itself without any warning, and remained off-line for science operations through until April 17th, when the mission team managed to restore full service. However, what triggered the safe mode in the first place has yet to be identified; so when TESS slipped back into a safe mode on April 23rd, engineers looked to see if there was a connection. There, was – but not in the way they’d hoped.

In order to restore TESS to an operational status on April 17th, the mission team had to perform an “unloading” operation on the the flywheels used to orient and stabilise the observatory. This is a routine activity, but it requires the use of the propulsion system to correct for any excess momentum held by the flywheels that might get transferred directly to the spacecraft and cause it to lose alignment. This in turn requires the propulsion system to be properly pressurised. Unfortunately, this was not completed correctly, and the thrusters were left under-pressurised. As a result, a small amount of momentum was transferred to TESS’s orientation, gradually swinging it out of expected alignment until it reached a point where the main computer realised something was wrong, triggered the safe mode and ‘phoned home for help.

Given this, the fix was relatively simple: correctly pressurisation the propulsion system and gently nudge it to stabilise TESS once more so it is aligned in accordance with its science operations.

Space Sunday: Starliners and samples

An artist’s rendering of a CST-100 Starliner capsule and service module in low Earth orbit. Credit: NASA / Boeing

Monday, May 6th 2024 should hopefully mark the start of a new phase of crewed space launches from US soil when the long-overdue NASA Crewed Flight Test (CFT) of Boeing’s CST-100 Starliner lifts-off from Canaveral Space Force Station and heads for the International Space Station (ISS).

As I’ve noted in these updates, the Starliner is one of two commercial vehicles specifically contracted by NASA to handle crew transfers to / from the ISS (the other being the SpaceX Crew Dragon), under the the Commercial Crew Program (CCP). Like Crew Dragon, it comprises a reusable capsule powered and supported by an expendable service module. Like both NASA’s Orion capsule (which is somewhat larger) and the Crew Dragon (which is somewhat smaller), the Starliner is also capable of other missions to low-Earth orbit outside of its primary NASA function.

A comparison between NASA’s Apollo and Orion capsules, together with the commercial vehicles from Boeing (CST-100) and Dragon (SpaceX) – all seen without their service modules. Credit: G. De Chiara

Capable of carrying up to seven people (the general crew complement for an ISS Expedition crew rotation) – although normal operations will see it carry four at a time -, Starliner is designed to be used for 10 flights with a 6-month turn-around time. The system was first unveiled in 2010, and was intended to build on Boeing’s experience with NASA and the Department of Defence; with the company confident the vehicle could be flying by 2015 were NASA to fund it forthwith. However, as NASA did not grant a contract (US $4.2 billion) until 2014, the first flight (+ vehicle certification) was pushed back to 2017 – although development work on the vehicle continued between 2010-2014 due to funding via NASA’s Commercial Crew Development (CCDev) contract.

However, as as I’ve again charted in these pages, the programme has been beset with issues – many of them to Boeing’s complete embarrassment. Over confidence on Boeing’s part saw the initial uncrewed test flight(OFT-1) delayed and delayed, finally taking place in December 2019. Post-launch a number of software errors were found, including an 11-hour offset in the vehicle’s mission clock, which resulted in an over-use of propellants and leaving the vehicle unable to rendezvous with the ISS. To further software errors were detected during the flight, either of which might otherwise have resulted in the complete loss of the vehicle.

As a result, a second Orbital Flight Test was required, to be undertaken at Boeing’s expense. Again the company was bullish about things, stating they could complete it in 2020, despite NASA requesting some significant updates to the docking system (which were further exacerbated by COVID, admittedly hardly Boeing’s fault). As a result, the launch pushed back to August 2021, and things went sideways.

somehow, Boeing managed to assemble the vehicle, ship it to Canaveral Space Force Station, have ULA integrate it into its Atlas V launcher, roll it out to the pad and then realise 13 propulsion system valves were stuck in the wrong position. Rather than scrub the mission and roll the vehicle back for a complete check-out and repair, Boeing then tried to carry out a fix on the launch pad, and when that failed, at the ULA Vertical Integration Facility (VIF). Only after this (somewhat risky) options failed, did the company return the spacecraft to the factory for proper remedial action – only to then enter into an embarrassing attempt to blame-shift with propulsion system supplier Aerojet Rocketdyne.

August 22nd, 2022: harnessed against the risk of a fall down the side of the booster, Boeing technicians attempt to repair 13 propulsion valves in the OFT-2 Starliner vehicle from the High Bay of the ULA Vertical Integration Facility at Canaveral Space Force Station. Eventually, the vehicle had to be unstacked and returned to the factory for repairs. Credit: NASA

As a result, OFT-2 did not take place until May 2022, and whilst largely successful, the flight saw issues with both the Orbital Manoeuvring and Attitude Control System (OMACS) and Reaction Control System (RCS). Even so, the flight was seen as meeting all of NASA’s requirements and Starliner was cleared for a crewed test flight (CFT), initially scheduled for early 2023,  only for more issues to cause it to be pushed back. Chief among these were problems with the parachute harness linking the capsule to its descent parachute and also – most worryingly – the discovery that flammable tape had been used with electrical wiring in the vehicle (a contributing factor to the tragedy of the Apollo 1 fire in 1967). The need to subject the parachute harness to upgrades and testing, and to go through the capsule inch by inch and replace the flammable tape knocked any hope of a 2023 CFT launch on the head, and it was pushed by to April / May 2024, with May 6th eventually being selected for the launch day.

For the last couple of weeks, final preparations for the launch have been taking place at both Kennedy Space Centre, where the 2-person crew have been in pre-flight quarantine (with the exception of the pre-flight team assigned to them) so as to avoid either contracting any communicable illness which might be passed to the crew on the ISS; and at Cape Canaveral Space Force Station, most recently with the roll-out of the Starliner vehicle Calypso atop its Atlas V launch vehicle.

The Boeing Starliner Calypso departs United Launch Alliance’s Vertical Integration Facility atop a ULA Atlas V rocket on May 4th, 2024, heading for Space Launch Complex 41 (SLC-41), Canaveral Space Force Station, in anticipation of its crewed launch on May 6th, 2024. Credit: Miguel J. Rodriguez Carrillo / AFP via Getty Images

The launch will mark the first used of the human-rated N22 variant of the Atlas V, and the first time any variant of the Atlas family of launch vehicles has lifted humans to space since the days of Project Mercury in the 1960s. The launch will also mark the first crewed launch from Cape Canaveral since Apollo 7 (October 1968). The mission is scheduled to last 6 days, with the crew flying the vehicle to a rendezvous and manual docking with the ISS, where they will remain for several days prior to undocking and making a return to Earth and touch down on land (Starliner does not make the more usual – for US crewed capsules – ocean splashdowns, instead using propulsive braking and an airbag, both of which operate in the last second prior to the vehicle landing, to cushion the crew).

Whilst a manual rendezvous and docking with the space station is a major goal for the mission, CFT-1 is also about getting a hands-on view of the vehicle’s capabilities and flight systems, together with an overall assessment of its human factors and handling during dynamic events (e.g. launch, docking, atmospheric re-entry and landing). For this, the crew selected for the mission are highly qualified test pilots turned astronauts in the form of mission Commander Barry “Butch” Wilmore, a Captain in the US Navy NASA, and Pilot Sunita “Suni” Williams, also a Captain in the US Navy.

Whilst Starliner is designed to be lifted to orbit from a variety of launch vehicles – ULA’s Atlas V and Delta IV and SpaceX’s Falcon 9 – all of its completed and planned NASA crew flights will be atop the N22 crew-rated version of the Atlas V. Credit: ULA

Wilmore has spent a total of 178 days in space, flying both the space shuttle (STS-129) in the Pilot’s seat, and on the Russian Soyuz vehicle, which he used in 2014 to reach the ISS as a part of the Expedition 41/42 long duration station crew. As a fleet pilot, he gained over 6,200 hours flying a range of jet fighter and interceptor aircraft and making 663 at-sea landings aboard multiple US aircraft carriers. He also flew 21 combat missions during Operation Desert Storm. As a test pilot, he was heavily involved in the certification of the T-45 Goshawk trainer (a US version of the venerable British Hawk trainer) for carrier flight training, and served as an instructor for both US Navy fixed wing aviators and pilots training at the US Air Force Test Pilot School.

Williams served in the US Navy flying rotary aircraft, flying with Helicopter Combat Support squadrons. She flew missions during Operation Desert Shield, and was a senior pilot-in-charge of a detachment of Navy helicopters flying relief and rescue missions following Hurricane Andrew in 1993. She is qualified as a pilot, a test pilot and an instructor pilot on over 30 types of rotary wing aircraft, including helicopters and the likes of the V-22 Osprey.

NASA’s Crew Flight Test (CFT) astronauts Sunita “Suni” Williams and Barry “Butch” Wilmore (right) exit the Neil A. Armstrong Operations and Checkout Building at Kennedy Space Centre wearing the Boeing Starliner pressure suits on Friday, April 26th, during a mission dress rehearsal. Credit: NASA / Frank Micheaux

As a NASA astronaut, she has flown in space no fewer than six times, for a total of 321 days 17 hours in space, 50 hours of which were spent carrying out 7 EVAs outside of the space station, marking her as one of NASA’s top five most experienced EVA astronauts. She was also the first person to run a marathon in space, officially participating in the 2007 Boston Marathon. She did this using a treadmill and bungee cords to hold her in place, completing the run distance in 4 hours 24 minutes – during which time she actually circled the Earth 3 times! She took part in the same marathon again in 2008.

Providing CFT-1 is a success and meets all of its goals, it will clear the way for crewed flight operations using Starliner to commence in 2025. No date has been set for the first operational flight, Starliner-1, but it is due to launch a 4-man crew of NASA astronauts Scott Tingle and Michael Fincke, Canadian astronaut Joshua Kutryk and Japanese astronaut Kimiya Yui on a planned 6-month stay at the space station. Once operational Starliner will fly annually on ISS missions from 2025 through 2030, splitting operations with Crew Dragon.

Whilst Starliner can – like Crew Dragon – be used for other orbital mission types, Boeing stated recently that it currently has no plans to start operating the craft commercially. However, the company is a partner in the Blue Origin-led Orbital Reef commercial space station project. This is due to commence orbital operations in the late 2020s, and Starliner is the designated crew vehicle for operations and crew flights relating to that station.

Continue reading “Space Sunday: Starliners and samples”

Space Sunday: Rocket Lab, Voyager, Hubble and SLIM

June 29th, 2019: Rocket Lab’s Electron Rocket rises from Launch Complex 1 on the Mahia Peninsula of New Zealand North Island at the start of the mission Make It Rain. Credit: Rocket Lab

Rocket Lab, the New Zealand / US commercial launch provider, is gradually increasing the annual launch cadence of its Electron rocket, as the company continues to garner a solid reputation as a provider of a reliable launch platform whilst also building-out other aspects of its business.

Founded in 2006 in New Zealand by entrepreneur Peter Beck, Rocket Lab initially developed the  Ātea (Māori for “space”) sub-orbital sounding rocket, which made its first (and only) flight in 2009 with the Manu Karere or “Bird Messenger” mission. Although a sub-orbital class of rocket, the  Ātea -1 nevertheless pushed its upper stage and payload beyond the von Kármán line, the arbitrary “boundary” between the Earth’s atmosphere and space sitting at 100 km altitude (although the Earth’s atmosphere actually extends – albeit tenuously – far further than this), technically making Rocket Lab the first private company in the Southern Hemisphere to reach space.

The company started developing Electron Rocket after being awarded a 2010 US Government contract to study the use of a small-scale launch vehicle specifically geared towards servicing the developing cubesat market – a contract which in part lead to the company relocating to the United States in 2012-13 and taking up residence in California, with its New Zealand operations becoming a wholly owned subsidiary of the US business.

Electron Rocket on the production line in 2020. The one with the Electron logo on a white background was an Electron core stage outfitted to test systems to aid in the recovery of boosters following splashdown. Credit: Peter Beck

A two-stage rocket standing 18 metres tall, Electron made its first flight in May 2017. This did not go as planned and no payload was carried, justifying the mission’s name:  It’s A Test. However, the next flight (the first of three in 2018), called Still Testing, successfully delivered a payload of cubesats to orbit, whilst the next flight, called It’s Business Time saw the commencement of commercial launch operations. At the time of writing, Electron has clocked up an impressive 42 successful flights and payload deployments out of 46 launches, with customers paying between US $5 and $10 million per launch.

While this launch rate perhaps doesn’t sound like a lot when compared to SpaceX and its Falcon family, it needs to be remembered that while much is made of the annual volume of Falcon launches, less than 25% of them are actually directly revenue generating commercial sector launches; the vast majority (an average of 60% per year for four years) have been Starlink launches, for which SpaceX absorbs the cost (approx. US $40 million a launch) for no revenue, with a further 15%+ being far more lucrative US-government related launches. By contrast – although the margin of revenue over cost is much smaller, Electron should almost double Falcon’s 4-year average of commercial launches (13.25 per annum)  in 2024, if all 21 of its commercial launches are successful (the company also has 4 government contracted launches to complete in 2024 as well).

For a time Rocket Lab toyed with (and tested) the idea of plucking Electron core stages out of the air using a helicopter and a drag line designed to snag the line between the booster’s drogue and main parafoil as it descended towards a splashdown. This idea, whilst promising, was abandoned. in 2021. Credit: Rocket Lab

Currently, Electron is not reusable, making its launch costs higher than they might be. However, the company is looking to change this by recovering spent Electron first stages after splashdown and then refurbishing and reusing their nine Rutherford motors – the rocket motors being the most expensive element of the launch vehicle. The first re-use of a refurbished Rutherford motor took place in 2023, with Electron’s 40th flight, the the company is now building on this.

As well as commercial launch customers, Rocket Lab has garnered US government contracts from NASA, the National Reconnaissance Office and the United States Space Force, with the latter in recent months awarding the company contracts worth some US $547 million to develop and launch satellites as a part of the US military’s Proliferated Warfighter Space Architecture (PWSA), a constellation of satellites from a number of suppliers which provides  communications, information gathering, target tracking, etc., to the US military in battlefield and tactical / logistical operations. In addition, Rocket Lab has provided both its US and New Zealand launch services to other governments as well, including France, South Korea and the Australian government.

Nor is the company resting on its laurels with Electron. Despite once saying he would eat his hat if Rocket Lab ever moved towards making a reusable launch system  – his belief being that if the engines could be recovered and reused, that was enough – in March 2021 Rocket Lab announced they were to commence work on a medium-lift (8 – 13 tonnes payload range) launch vehicle.

Called Neutron, the reusable vehicle was introduced to the world on March 1st, 2021 in a video which saw Peter Beck keep his promise: he ate his hat (or some of it, at least).

Neutron – unlike SpaceX’s Starship / Super Heavy – has been designed from the ground-up to meet the needs of a number of existing government and commercial markets: the growing smallsat constellation market (which in and of itself is perhaps increasing more issues they it is potentially solving); medium payloads to LEO, SSO and also to geostationary transfer orbit (GTO – e.g. to other planets); and human space flight. It will achieve all of this in a novel approach.

Classified a 2-stage launch vehicle, Neutron will not have a conventional upper stage. Instead, the payload booster and payload will be contained inside the first stage. After passing through the majority of the atmosphere and entering a post-engine shutdown ballistic flight, the upper portion of the Neutron will open to eject the payload. Once the latter is clear, Neutron will use its thrusters to flip itself away from the “upper” stage, allowing the latter to fire its motor and push the payload on to its assigned orbit. Other factors then come into play – such as the shape of the Neutron, the re-use of at least one of its motors, etc – that will allow the rocket to make a propulsive return to launch sight descent and landing.

The advantages of this approach are multiple. Incorporating the upper stage into the rocket means that it can be smaller and lighter, as it does not require the additional structural reinforcement needed for it to be the fist of the rocket as it punches its way up through the atmosphere. Similarly, the integration of the protective payload fairings into the main rocket both increases the overall structural integrity of the vehicle and means they are not simply thrown away during a launch, removing the cost of a brand new set of fairings with each launch.

A rendering of Rocket Lab’s Neutron Rocket. Credit: Rocket Lab

However, there are also potential issues with the approach which Rocket Lab will have to demonstrate they can address. For example, human-rated vehicles generally require  means by which a crew can be hauled clear should the rocket malfunction. Clearly, if you are carrying your crew inside the rocket to start with, then getting them out of it will take longer that simply blasting them clear with powerful motors, as can easily be done when they are sitting at the pointy end of the rocket.

Currently, the first Neutron flight is targeting a late 2024 launch – which is an ambitious target for a project only announced in 2021, and which requires not only the development of the launch vehicle, but its propulsion system and fabrication facilities. As such, whether Rocket Lab achieve it or not is still open to debate.

The engine for Neutron is called Archimedes engine, and it is being built by Rocket Lab at their facilities in California. Primarily constructed using 3D printing, nine Archimedes motors will power the Neutron core stage with a further motor powering the “upper” stage.

Meanwhile, ground was broken for the rocket’s production facility in April 2022 at the  Mid-Atlantic Regional Spaceport (MARS) within NASA’s Wallops Flight Facility on the eastern coast of Virginia, USA – the MARS spaceport being the base of operations for Neutron, with no plans (at present) to launch the vehicle from New Zealand or elsewhere.

In addition to launch vehicles and satellites, Rocket Lab also produces the Photon satellite bus, designed for a variety of uses, including lifting satellites to their assigned orbits and providing power and propulsion for interplanetary payloads.  Photon is an attractive vehicle for government space agencies and the private sector, as it can be flown on a variety of launch vehicles and can utilise a wide range of rocket motors, such as Rocket Lab’s other engines, the Curie and HyperCurie and those from third-party suppliers, engine selection being based on mission requirements.

As such, while Rocket Lab might be small (literally and figuratively) when compared to SpaceX’s Goliath, it is (a bit like David was in that particular fight) the one to keep an eye on.

NASA: Voyager 1  and Hubble – Good News / Bad News

After a five month period of anxiety in which the spacecraft has been sending gibberish back to Earth, NASA’s Voyager 1 spacecraft, the most distant human-made object from Earth so far made, has resumed sending understandable engineering data.

As I’ve been covering in these pages, Voyager 1 started sending this gibberish since mid-November 2023, although it has remained fully capable of receiving and acting upon instructions from Earth. This resulted both in a suspension of the spacecraft’s science activities and an inability for engineers to determine the vehicle’s overall operational state.

An artist’s rendering of Voyager 1 in interstellar space. Credit: NASA / JPL

Since then, investigations initially narrowed the potential issue as lying with one of two systems: the spacecraft’s telemetry modulation unit (TMU), responsible for sending data to Earth; or the flight data subsystem (FDS), responsible for the actual packaging of that data ready for transmission to Earth. Further work determined the issue as lying within the FDS, although exactly what has gone wrong remained a puzzle.

Then, and as I reported in March (see:  Space Sunday: starships, volcanoes and Voyagers), an engineer from NASA’s Deep Space Tracking Network (DSN), which handles all communications with NASA’s multiple deep-space missions, noticed something odd about some outlier data the communications received from Voyager 1 – it did not appear to be gibberish. Digging deeper, he realised it was actually a complete dump of the FDS’s memory.

This allows engineers to determine a single memory chip within the FDS has failed, corrupting about 3% of the system’s memory; just enough for the data packaging operation to be thrown into disarray and result in gibberish. The cause identified, the problem became how to fix it.

The most obvious means to doe so would be to tell the spacecraft not to use the corrupted memory for data processing. However, that required instructing the FDS to use other memory space – and there wasn’t a single address space in the system large enough to match the corrupted memory and manage its own data processing. As a result, the engineers broke the problem down into a series of steps.

The first step was to updated the FDS software so that the system could take the data normally handled by the corrupted data so that it could be handled through several other parts of the FDS memory, and without messing up any of the other data they had to manage. This recoding was carried out during March and April, and on April 18th, 2024, the updated software was sent to Voyager 1. Then came a nigh-on 48 hours wait for a response: it takes 22.5 hours for a signal from Earth to reach Voyager 1, which then has to execute the code, carry out the instructions related to it, and send a reply – requiring another 22.5 hours to reach Earth.

If the engineers were correct and the update correct, then the response from Voyager 1 should be an engineering update on its overall status. On April 20th, that’s exactly what the mission team at NASA’s Jet Propulsion Laboratory received, and for the first time and for the first time in five months, Voyager 1 weas once again communicating with meaningful data.

Engineers and flight team members responsible for Voyager 1’s operation respond to the confirmation that data received from the spacecraft on April 20th, 2024 confirms their initial attempt to correct a data communications issue has worked. Credit: NASA/JPL

The next steps in the process are to ensure that all science data can be similarly re-routed through the FDS to avoid the corrupted memory sent to Earth without anything becoming confused, and then finally to ensure the faulty memory is completely ignored by all FDS processing and by any of Voyager 1’s systems that interact with the FDS. These steps are expected to take several more weeks. Nevertheless, the fact that Voyager 1 is once again “transmitting in the clear”, so to speak, is welcome news.

Unfortunately, things are not so good with the Hubble Space Telescope (HST), with NASA reporting it is again experience issues with its gyroscopes for the second time in the last six months – and the problem appears to lie with the space gyro that had problems in November 2023.

The gyroscopes are used to precisely point the telescope at targets and hold it steady during imaging. Originally, HST used 3 pairs of gyros, which were periodically swapped-out during servicing missions. However, the last time all six gyros were replaced was during the last servicing mission of 2009 – since the retirement of the space shuttle, NASA has not had the means to safely carry out such a mission, and in the intervening time, three of the gyros have failed completely.

The Hubble Space Telescope (HST) as seen from the departing space shuttle Atlantis, flying STS-125, the final HST Servicing Mission, in 2009. Credit: NASA

Such failures are the result of wear and tear affecting wires less than the width of a human hair and called flex leads which pass through the gyros carrying power and data. As the gyros operate, these flex leads well, flex; but they also slowly corrode as a result of this flexing and can eventually break. One sign of this possibly occurring can be seen when a gyro starts to show power fluctuations. This happened during the past week, causing the gyro to enter a “safe” mode.

As a result, and after allowing the telescope to enter a contingency mode were it can – at reduced capability – function on just two gyros for a few days, on Sunday, April 28th, 2024, NASA completely paused the telescope’s science operations in order to more fully investigate the gyro’s problems in order to try to determine if it is about to suffer a flex lead failure, or whether there is another cause of the gyro’s woes, as was the case in November 2023.

If it turns out the gyro cannot be safely restored to an operational state, NASA has indicated it will switch Hubble over to operating on just a single gyro – permanently degrading its capabilities – in order to hold the second functional gyro as a reserve against any further gyro failure.

Japan’s Moon Sniper Wakes Up – Again

As I’ve previously reported in these pages, Japan became the fifth nation to successful land a spacecraft on the Moon when its Smart Lander for Investigating Moon (SLIM – also called “Moon Sniper”) arrived on the lunar surface on January 19th, 2024. Unfortunately, the craft arrived upside down, as confirmed by images returned by one of the two micro-rovers deposited on the lunar surface as a part of the mission (see: Space Sunday: a helicopter that could; a lander on its head and  Space Sunday: More Moon (with people!) and a bit of Mars) – although precisely why it did has not been 100% confirmed.

Despite this, the vehicle was able to complete the majority of its science mission before being put in a dormant state with the onset of the long lunar night. At the time – the start of February – it was not anticipated that the craft would survive the 14 terrestrial day period without sunlight to warm it and provide energy to power its batteries. But it did; as it started to receive sunlight once more in late February, it called home.

Japan Aerospace Exploration Agency (JAXA) released this image, captured by the LEV-2 mini-rover, of their SLIM lander upside down on the Moon. Credit: JAXA

Whilst the team responsible for the spacecraft had hoped this might be the case, they were unable to get the vehicle to resume science operations and, after a further 14 terrestrial days of sunlight, SLIM went back to sleep for a second night. This time, it was not expected to wake up and the mission team disbanded – only to come back together in March 2024, when SLIM did indeed wake up as it received daylight, and started ‘phoning home and sending images, which it continued to do until night came yet again.

This time, the mission team were sure the vehicle would not call home once sunlight had returned to its landing spot and once again, they’ve been proven wrong. SLIM again ‘phoned home on April 24th, 2024, although it is unclear whether or not the mission team have been able to re-establish any of the vehicle’s science gathering activities. Even so, that the craft has thus far survived three long lunar nights again proves Japan’s prowess with their space technology.

Space Sunday: flying on Titan; bringing home samples from Mars

A 2021 rendering of NASA’s Dragonfly octocopter vehicle, now set to head to Titan in 2028. Credit: NASA / JHU/APL

NASA’s ambitious plan to fly a robotic vehicle on a moon of another world is to go ahead after receiving official confirmation in April 2024. With its cost now set at some US $3.35 billion, double its initial price estimates – largely the result of the COVID pandemic derailing the vehicle development process in 2020/21 -, the vehicle – called Dragonfly (as is the overall mission) is intended to have a 10-year primary lifespan, with 3.3 years of that time spent flying around and studying Saturn’s largest moon, Titan.

Dragonfly is a spectacular science mission with broad community interest, and we are excited to take the next steps on this mission. Exploring Titan will push the boundaries of what we can do with rotorcraft outside of Earth.

– Nicky Fox, NASA associate administrator, Science Mission Directorate, Washington D.C.

Titan is a unique target for extended study for a number of reasons. Most notably, and as confirmed by ESA’s Huygens lander and NASA’s Cassini mission, it has an abundant, complex, and diverse carbon-rich chemistry, while its surface includes liquid hydrocarbon lakes and “seas”, together with (admittedly transient) liquid water and water ice, and likely has an interior liquid water ocean. All of this means it is an ideal focus for astrobiology and origin of life studies – the lakes of water / hydrocarbons potentially forming a prebiotic primordial soup similar to that which may have helped kick-start life here on Earth.

Using a vehicle that is in situ on the surface of Titan is vital, because the moon’s dense atmosphere obscures its surface across many wavelengths, making it exceptionally hard to definitively identify the specific combinations of hydrocarbon materials present across the moon’s surface without getting very up close and personal. To do this, Dragonfly will be a unique rotary vehicle, one a good deal heavier and more complex / capable than the Ingenuity drone flown on Mars (which was an extraordinary flying vehicle – and now static weather station – on Mars).

The brainchild of Jason W. Barnes (University of Idaho) and  Ralph Lorenz (Johns Hopkins University Applied Physics Laboratory – or JHU/APL), Dragonfly is being developed for NASA by JHU/APL, with Elizabeth “Zibi” Turtle, a planetary scientist at JHU /APL serving as the mission’s principal investigator.

The craft is designed as an octocopter – an aerial vehicle with four pairs of contra-rotating rotor blades. Each pair of rotors will be powered by its own electric motor, and the craft has been design to withstand either the loss of a single rotor blade or the completely failure of and one motor powering a pair of blades. It will have an on-the-ground mass of around 450 kg (compared to Ingenuity’s 1.8 kg), and will use a mix of nuclear and battery power.

A large lithium-ion battery will provide direct power to the vehicles flight and navigation systems and to this science suite. It will provide sufficient power for the craft to travel up to 16 km on a single charge at speeds of up to 36 km/h, with a maximum airborne time of around 30 minutes per flight, and an estimated maximum altitude of 4 km – although generally the craft will fly much lower than this. The battery will be supported / recharged by a Multi-Mission Radioisotope Thermoelectric Generator (MMRTG), which will also be used to provide heat to the vehicle, particularly during Titan’s night periods when it is behind Saturn relative to the Sun, and which lasts for 8 terrestrial days. The MMRTG will additionally provide power to the vehicle’s science instruments during the night periods, allowing them to work whilst the vehicle waits out the night in order to resume flying in daylight..

Dragonfly’s remarkable flight capabilities – speed, altitude, single flight distance – are made possible by Titan’s environment: the moon’s low gravity (around 13.8% that of Earth and dense atmosphere (around 1.45 times that of Earth’s) mean that the flight power for a given mass operating on Titan is around 40 times lower than on Earth, so the vehicle can have a fairly significant mass which can be lifted by relatively low-mass, low-power motors.

A Dragonfly testbed article undergoing flight trials

The vehicle will fly a primary science suite of four packages, comprising:

  • DraGNS (Dragonfly Gamma-Ray and NeutronSpectrometer): comprising  a deuterium-tritium Pulsed Neutron Generator and a pairing of a gamma-ray spectrometer and neutron spectrometer to identify the surface composition under the vehicle.
  • DraGMet (Dragonfly Geophysicsand Meteorology Package): a suite of meteorological sensors including a seismometer.
  • DraMS (Dragonfly Mass Spectrometer): a mass spectrometer to identify chemical components, especially those relevant to biological processes, in surface and atmospheric samples.
  • DragonCam (Dragonfly Camera Suite) is a set of microscopic and panoramic cameras to image Titan’s terrain and scout for scientifically interesting landing sites.

Samples of surface material for examination by the science packages will be obtained using two coring drills and hoses mounted within Dragonfly’s skid, per the video below.

Further, the vehicle will be equipped with a fully autonomous flight and navigation system capable of flying it along a selected flight path, making its own adjustments to account for local conditions whilst in flight, and with sensors capable of record potential points of scientific interest along or to either side of its flight path, so the information can be relayed to Earth and factored into planning for future excursions. Flights over new terrain will likely be of an “out and back” scouting nature, the craft returning to its point of origin, allowing controllers on Earth to plan follow-up flights to locations along the flight track, taking into account any points of interest noted by the vehicle.

Currently, Dragonfly is targeting a July 2028 launch, although the launch vehicle itself has yet to be announced. It will take seven years to reach Titan, mostly likely using several gravity-assist manoeuvres around Earth to slingshot itself on its way. In this, it will be the first dedicated mission to the outer solar system not to flyby / utilise Jupiter whilst en route, as the planet will not be within the mission flight path.

On arrival at Titan, and following separation from the cruise stage that would keep it both powered and warm during the trip from Earth, Dragonfly will enter the moon’s atmosphere atop a 3.7 metre diameter heat shield, and under a protective back shell. Once in the atmosphere, a single drogue and single large main parachute will be deployed to slow the vehicle’s descent until it reaches an altitude at which the parachute is released and Dragonfly can drop clear of the back shell, enabling it to start its motors and make a first landing on Titan.

A 2017 rendering of Dragonfly’s arrival on Titan. Credit: NASA / JHU/APL

In this, the landing site for the mission has already been selected: the edge of a prominent and dark region of Titan called Shangri-La, thought to be an immense sand sea of dark, carbon-rich material.

Specifically, Dragonfly will touch down in a dune field close to the relatively young Selk impact crater, which will be the vehicles first science study location, as it contains strong indications that it was once home to deposits of liquid water (and is now surrounded by ejecta that includes water ice) and contains tholin organic compounds. After this, Dragonfly will move on into the Shangri-La, carrying out exploratory flights of up to 8 km at a time and gathering samples for analysis from diverse locations.

NASA Re-Re-Rethinks Mars Sample Return Mission

NASA is now officially seeking both internal outside support for its much-troubled Mars Sample Return (MSR) mission.

The goal of returning samples of surface and sub-surface material from Mars to Earth, where it can be subjected to much more intensive and multi-disciplinary study than can be achieved via in-situ robotic explorations, has long be sought. For NASA, the last 20 years have seen numerous ideas put forward for gathering and returning such samples from Mars, all of which have ended up being cut down in their prime due to matters of cost and stringent curbs on the US space agency’s budget – sending a vehicle to Mars with the express intent of obtaining, storing and then returning samples to Earth not being the easiest of mission profiles to plan, let alone achieve.

However, in the lead-up to the Mars 2020 mission, featuring the rover Perseverance, NASA and the European Space Agency (ESA) signed a letter of intent to jointly develop a sample return mission based around the concept of the actual sample gathering being carried out by Perseverance and deposited on the surface of Mars for collection “at a future date”. The operation to start depositing groups of these samples actually started on December 21st, 2022, with a total of 10 sample tubes being deposited relatively close together on Mars by Perseverance.

Resembling a Star Wars light sabre in an image obtained by the WATSON imager on Perseverance’s robot arm, this was the first of the sample tubes to be “dropped off” by the Mars 2020 rover (December 21st, 2022), marking the start of an initial operation to place 10 such sample tubes in a cache for collection by some future Mars Sample Return mission. Credit: NASA

Whilst this approach negated the need for the MSR to actually collect and store samples itself – in theory simplifying the mission parameters – actually settling on a final design for the mission proved difficult. By 2021, the “optimal” approach was seen as being a mission involving four unique vehicles in addition to the Mars 2020 rover. These were:

  • A NASA- built Mars lander / launch platform.
  • A NASA-built Mars Ascent Vehicle (MAV) with a specialised sample containment unit, and carried within the lander.
  • A European-built “fetch” rover with its own dedicated lander, designed to land ahead of the NASA lander and go find the sample tubes deposited by Perseverance, bring them to the NASA lander and transfer them into the sample containment unit in the MAV.
  • A European-built Earth Return Vehicle (ERV) designed to arrive in Mars orbit and await the arrival of the NASA-built MAV from the surface of Mars. This would then capture the sample unit (about the size of the basketball) after the latter had been released by the MAV, secure it and the samples inside itself and then make the return trip to Earth.

So, yeah; “simples” – not. The mission included, as identified by independent review board (IRB) charged with reviewing the mission for its overall cost-effectiveness and feasibility, no fewer than eight “break the chain” (and cause the mission to fail) first-time challenges, including the fully robotic collection and transfer of samples, the first automated launch of a vehicle from the surface of another planetary body, the first fully autonomous orbital rendezvous between two vehicles (the MAV and the ERV), and the first “pitch and catch” transfer of a sample package. However, despite this and concerns over the estimated mission cost rising to around US $4 billion, the IRB green lit the mission.

The MSR mission concept as envisioned in 2021 / early 2022 and featuring the ESA-built “fetch” rover (minus its lander).  Credit: NASA / ESA

 By July 2022, the complexities of the mission had been more fully realised, so efforts were made to “simplify” it. Specifically, the ESA “fetch” rover was eliminated from the mission – but was supplanted by the use of two Ingenuity class Mars helicopters. Fitted with wheels, these would also be delivered to Mars by the NASA lander carrying the MAV, and once there, they would fly and land in close proximity to sample tubes deposited by Perseverance, then drive up to them, pick them up and fly them back to the lander for transfer to the MAV, with the rest of the mission remaining the same.

The 2022 MSR update, with the ESA “fetch” rover removed from the mission, and replaced by two Ingenuity-class  helicopters (only one shown), which would be delivered to Mars by the NASA MSR lander and tasked with recovering sample tubes deposited by the Mars 2020 Perseverance rover. Credit: NASA / ESA

However, while this removed the need for an entire rover and lander, and meant that effectively, NASA would have two further helicopters on Mars with which they could carrying out other missions once the sample tubes had been delivered to the MAV, it didn’t actually do much to reduce complexity or mission cost – which threatened to rise to around US $8 billion.

To offset this, the planned mission time frame was revised from around 2030-31 to the mid-to-late 2030s, allowing the mission cost to be spread across a greater number of NASA fiscal years. However, by mid-2023, it was widely recognised that the mission would probably exceed the US $8 billion estimate and peak at perhaps as much as US $11 billion – gaining the mission a lot of opposition on Capitol Hill. Suggestions were made to push the mission time-fame out further, with the lander / MAV / helicopter element not launching until the early 2040s.

By mid-2023, the mission had been further revised in order to try to reduce complexity and costs. Under the new proposal, none of the sample tubes thus far used and deposited on Mars for collection by Perseverance would actually be recovered (about 24 of the 43 total). Instead, all of the remaining tubes (16 of which have yet to be used, as of the time of writing) would be retained on the rover. Then, on the arrival of the MSR lander / MAV combination, Perseverance would rendezvous with them and load its supply of sample tubes directly into the MAV’s sample capsule for onward transfer to the ERV and a return to Earth. Whilst this would limit the selection of samples compared to gathering them from the various caches the rover had made on the surface of Mars, it did both simplify the mission – NASA only having to fly the MAV-carrying lander – whilst ensuring ESA’s involvement was not wasted, as they would still supply the Earth Return Vehicle.

The 2023 MSR update, with Ingenuity class helicopters removed and showing the Perseverance rover directly transferring sample tube to the sample capsule of the MAV, eliminating the need for intermediary vehicles. Credit: NASA / ESA

Despite this, over mission complexities and the need for the development of two entirely new classes of robotic spacecraft (the MSR lander-come-launcher for the MAV, and the MAV itself, complete with its sample storage / containment system) meant NASA would still be looking at around a minimum US $8 billion cost – and if the timeframe for the mission were to be extended into the early 2040s, inflation would likely push the final price back up towards the US $11 billion figure.

As a result, and with NASA’s budget already being severely stressed for the 2024/25 period, the agency finally admitted defeat with its more grandiose MSR plans, and on April 15th, 2024, the US space agency issued a statement indicating it is now looking “outside the box” for the means to carry out a Mars sample return mission in a cost-effective manner and within a reasonable time-frame (i.e. before the end of the 2030s). To this end, the statement calls on all NASA centres involved in Mars exploration to work together in order to develop such a mission, whilst also indicating the agency will seek proposals for potential mission architecture from the private sector.

Currently, NASA itself has admitted it does not have firm ideas on how mission costs can be reduced, but is determined to see the sample return mission take place, viewing it as a vital precursor to any attempt at a human mission to Mars. Thus, the process for redeveloping plans and ideas is expected to run through until the latter part of autumn 2024.

Space Sunday: total eclipse and a nova

Total eclipse of the Sun. Credit: Alan Dyer/VW Pics/UIG via Getty Images

Monday April 8th 2024 marks 2024 only total solar eclipse of the year (and only one of two which might be witnessed during the year the other being an annular eclipse on October 2nd, 2024), with North America being treated to the spectacle.

A total eclipse is when the Moon crosses directly between Earth and the Sun in a manner which means it completely blocks the face of the Sun from view to those directly “under” the Moon’s path across the sky. This is the region known as the path of totality, marked by the Moon’s shadow marching its way across the face of the Earth as the Moon passes between planet and star. Within that path, the full light of the Sun is blocked for a brief period, plunging the land into twilight before the face of the Sun re-emerges from the limb of the Moon as the latter continued on in its orbit.

As I’ve mentioned before in these pages, a total solar eclipse is the most intense and fascinating of the various types of eclipse that can be observed from Earth, and they tend to occur roughly every 12-24 months, affecting different parts of the world depending on factors such as the Earth’s rotation at the time, the position of both the Sun and Moon relative to Earth, etc. Thus, not every total eclipse is necessarily so easily visible; the path of totality can often be in very remote places or over sparsely populated regions or even far out at sea.

Track of the April 8th, 2024 total solar eclipse across North America, showing the main path of totality. Michael Zeiler/GreatAmericanEclipse.com

The event on April 8th 2024, however, is a little different. The 184-km wide path of totality will extend across 15 US states, whilst its ground track across North America will include Sinaloa, Durango and Coahuila in Mexico and Ontario, Quebec (where it will brush both Toronto and Montreal respectively), New Brunswick and sweep over the Labrador coast of Newfoundland close to St. Johns. This means it will be potentially visible (weather permitting) to around 32 million people in the US alone. What’s more, and in a rarity for total eclipses, it comes just seven years after the last total eclipse was visible from the continental United States (prior to that, the previous one to occur over the contiguous US was in 1979, and the next will not be until 2044).

Upcoming total solar eclipses and their visibility on Earth. Via timeanddate.com

If you are lucky enough to lie along the path of totality, and the weather is suitable for you to view it, please keep in mind these common sense guidelines:

  • Never look directly at the Sun – even with sunglasses or by using dark material such as a bin bag or photo negative; these filters do not protect your eyes against infrared radiation and can cause permanent eye damage.
  • Only look at the sun if you have certified eclipse glasses and are wearing them.
  • Only use a telescope or binoculars to project an image of the Sun onto white card, and never use either instrument to observe the Sun directly unless you have a certified solar filter fitted.

The best way to view an eclipse if you do not have eclipse glasses or have a telescope or binoculars to project the Sun’s image onto card, is via a pinhole camera:

  1. Cut a hole in a piece of card.
  2. Tape a piece of foil over the hole.
  3. Poke a hole in the foil with a pin.
  4. Place a second piece of card on the ground.
  5. Hold the card with the foil above the piece of card on the floor to project an image of the Sun onto it, and look at the image. Do not use the pinhole to look directly at the Sun.
Eclipse Types (Moon and Sun not to scale). Credit: Cmglee

There are a number of terms common to eclipses which are worth mentioning for those who wish to follow the event, but are unfamiliar with the terminology. Specifically for a total eclipse these are:

  • The umbra, within which the object in this case, the Moon) completely covers the light source (in this case, the Sun’s photosphere).
  • The penumbra, within which the object is only partially in front of the light source.
  • Photosphere, the shiny layer of gas you see when you look at the sun.
  • Chromosphere, a reddish gaseous layer immediately above the photosphere of the sun that will peak out during the eclipse.
  • Corona, the light streams that surround the sun.
  • First contact, the time when an eclipse starts.
  • Second contact, the time when the total eclipse starts.
  • Third contact, the time when the total eclipse ends.
  • Fourth contact, the time at which the eclipse ends.
  • Bailey’s beads, the shimmering of bright specks seen immediately before the moon is about to block the sun.
  • Diamond ring, the last bit of sunlight you see right before totality. It looks like one bright spot (the diamond) and the corona (the ring).
Baily’s beads and the “diamond ring” effect seen during a solar eclipse on July 2, 2019 from the Cerro Tololo Inter-American Observatory in Chile. Credit: CTIO/NOIRLab/NSF/AURA/D. Munizaga

As noted, a total eclipse occurs when the observer is within the path of totality marked by the Moon’s shadow – which is formally called the umbra – passing along the surface of the Earth. For those in Mexico, much of the USA and Canada outside of the umbra, there is still the opportunity to see a partial solar eclipse if you are located within the penumbra.

If you are observing the eclipse (particularly along the line of totality), you might keep an eye out for some / all of the following:

  • If you look at the ground around you just before totality occurs and the Moon completely covers the disk of the Sun; you might see the phenomenon of fast-moving shadows, called shadow bands, racing across the ground under your feet. These might also occur as the Sun starts to re-emerge from behind the Moon.
  • During totality, keep an eye out for the brighter stars becoming visible during totality, together with the following planets:
    • Jupiter: roughly 30o above and to the left of the Sun / Moon.
    • Venus roughly 15o below and to the right of the Sun / Moon.
    • Saturn and Mars (both very faint) roughly 20o below Venus, close to the horizon and further to the right.
  • The very keen eyed might also be able to spot comet 12P/Pons-Brooks as a fuzzy dot just off to the right of Jupiter (although you will need to be very keen-eyed!
Sky chart showing the most conspicuous stars and planets that might be visible in the vicinity of the totally eclipsed sun. Credit: Joe Rao
  • Watch and listen to the local animals and wildlife (if present). Birds may stop singing, with some flying to their roosts, cattle might behave is if it is evening , etc., as they become confused by the local twilight.
  • During the solar eclipse, you may see colours shifting, giving familiar objects unusual hues. This natural shift in colour perception is caused by fluctuating light levels resulting from the darkening of the sun.
US Viewing probability map for the April 8th, 2024 total solar eclipse. Credit: Joe Rao

If you prefer not to watch the eclipse directly, or are not lucky enough to live along the path of totality (is the weather is pooping on you seeing it if you are), then it can be followed on-line at the following resources:

Totality Times (UTC) for Notable North American Locations

  • Mazatlán, Sinaloa, Mexico – 18:07; duration: 4 minutes 20 seconds.
  • Durango, Durango, Mexico – 18:18; duration: 3 minutes 50 seconds.
  • Piedras Negras, Coahuila, Mexico/Eagle Pass, Texas, U.S – 18:27; duration: 4 minutes, 24 seconds.
  • Dallas, Texas – 18:40; duration: 3 minutes 52 seconds.
  • Indianapolis, Indiana – 19:06; duration: 3 minutes, 51 seconds.
  • Cleveland, Ohio – 19:13; duration: 3 minutes, 50 seconds.
  • Erie, Pennsylvania – 19:16; duration: 3 minutes, 43 seconds.
  • Rochester, New York – 19:20; duration: 3 minutes, 40 seconds.
  • Niagara Falls, Ontario, Canada – 19:18; duration: 3 minutes, 31 seconds.
  • Montreal, Quebec, Canada – 19:26; duration: minutes 57 seconds.
  • Tignish, Prince Edward Island, Canada – 19:35; duration: 3 minutes, 12 seconds.
  • Catalina, Newfoundland, Canada – 19:43; duration: 2 minute, 53 seconds.

Note that part of north Europe  – notably the UK – will be able to witness a partial solar eclipse.

Continue reading “Space Sunday: total eclipse and a nova”

Space Sunday: starships, volcanoes and Voyagers

Plasma starts to form around the Starship’s thermal protection system as the vehicle starts to re-enter the denser part of Earth’s atmosphere, March 14th, 2024. Credit: SpaceX

Thursday, March 14th, 2024 saw SpaceX attempt the third Integrated Flight Test (IFT-3) of its massive Starship / Super Heavy launch system after the Federal Aviation Administration (FAA) granted a limited launch license to the company on March 13th.

Despite SpaceX and its followers hailing the first two launch attempts as “successes”, the short-order loss of both vehicles within 4 minutes of the launch of IFT-1 and which either vehicle achieving its core milestones in IFT-2, meant that both of those flights were extremely limited in their “success”. As a result of both, SpaceX spent considerable time reviewing the launch profile for the vehicles and making changes and improvement to both the Starship craft and Super Heavy. These resulted in IFT-3 being a broadly successful – although the loss of both vehicles at different points in the flight meant it was not an unqualified success.

Following lift-off at 13:25 UTC, with an initially perfect firing of all 33 Raptor engines on the booster, the stack of rocket and starship passed through Max-Q, the period where both experience maximum mechanical stresses as they ascend through the atmosphere, within the first minute of flight.

A clean burn: all 33 Raptors are at work as the IFT Starship / Super Heavy combination move towards Main Engine Cuto-Off (MECO). Credit: SpaceX

Even so, at 2:42 into the flight, the engines on the booster shut down and two seconds later, the starship upper stage ignited all six of its engines in a “hot staging” manoeuvre, separating from the booster after the engines had fired. This went a lot smoother than evidenced in the second launch attempt in November 2023, and the booster was this time able to change direction and execute an successful “boost back” burn – using the motors to kill its ascent velocity and push it back towards the launch site.

However, it was during the boost-back that possible hints of engine issues appeared: several of those recording and reporting on the launch noted that some of the engine exhaust plumes were tinged green, indicative of one or more engines consuming itself (green indicates the copper used in the engines is being consumed), a long-term issue with the Raptor 2. Nevertheless, the booster successfully re-oriented itself and started a planned engine-first descent towards the Gulf of Mexico and a splashdown.

For this to happen, the booster needed to slow itself by a further re-lighting several engines in a braking manoeuvre roughly a kilometres above the water. Whilst three engines did ignite, two immediately failed, and the vehicle was destroyed less than 500 metres above the Gulf – although it is not clear if the flight termination system was triggered or the booster blew itself apart. At the time of destruction, it was travelling with sufficient velocity to hit the water at 1,112 km/h.

A successful hot staging: with the super Heavy booster engines still glowing brightly, the Starship vehicle separates and moves away, the shockwaves of its exhaust ringing both vehicles after a successful engine start-up while still attached to the booster. Credit: SpaceX

Starship went on to achieve orbit, on course for a splashdown in the Indian Ocean. Travelling at around 240 km above the Earth, the vehicle carried out a test of the “Pez dispenser” payload bay door – a slot in the vehicle’s hull at the base of the payload bay and specifically designed to eject Starlink satellites (these being almost the only payload for Starship at present). Also tested was a so-called “propellant transfer” test, shunting a small amount of liquid oxygen between the vehicles’ main and header tanks.

However, SpaceX cancelled the vehicle’s planned de-orbit burn with one of its Raptor engines and instead allowed the vehicle to “go long”, continuing along its orbital track until gravity until drag caused it to re-enter the  denser part of the atmosphere for a hoped-for splashdown. In the event, and following an initially very successful re-entry, the vehicle broke apart at an altitude of around 65 km.

The orbital flight segment of the test was impressive whilst also raising questions as to Starship’s future orbital flight dynamics. Notably, throughout its half orbit of the Earth, the Starship was in a state of continuous “bbq roll”, that is, spinning around its longitudinal axis (and making it seem like the Earth was constantly looping around it on videos). Such rolls are not uncommon on space vehicles when in sunlight, as they help spread the thermal load of the Sun’s heat over the vehicle’s outer skin, preventing uneven heating (or overheating).

In the first few seconds of flight: not the white ice enveloping the Super Heavy booster and the back of Starship -the result of the hulls of both forming the outer walls of their cryogenic tanks and being so cold frost ice forms on the metal, indicative of its poor thermal regulation. Credit: SpaceX

In this respect, Starship is especially vulnerable to such thermal stresses: it is completely reliant on cryogenic propellants which tend to revert to a gaseous state (and require venting to prevent tanks being over-stressed), and it is made of stainless steel, and extremely poor thermal insulator. This is compounded by the fact that the hull of the vehicle is also the the outer surface of the propellant tanks, so outside of the thermal protection system (TPS) tiles coating one side of the vehicle and designed to protect it during re-entry in to Earth’s atmosphere, there is next to no thermal insultation between the vehicle’s propellant reserved and the Sun, thus leaving rolling the vehicle as the simplest means of regulating internal temperatures.

Even so, the rate of roll, combined with its continuous does raise questions: was the rolling seen on this flight simply an overly precautious desire to limit thermal blooming inside the vehicle, or will it be part of starship SOP in the future. If the latter, then there are going to be some significant issues to address (how are to starships supposed to pump propellants being them in they have to roll like this once mated and the fuel to be transferred from one to the other is being exposed to a severe Coriolis effect as a result of the spin? Was the spin in this instance the cause of the planned de-orbit burn being cancelled because a smooth flow of propellants to the motor to be fired could not be guaranteed?

That said, the vehicle did perform its own mini “propellant transfer”, pumping a small amount of liquid oxygen between its own tanks. However, the overall value of this test is perhaps not as significant as some SpaceX fans have stated, given it is a long way short of the 100+ tonnes of propellants at a time that will need to be transferred between vehicles when it comes to sending the proposed Starship lunar lander to the Moon .

But leaving such thoughts aside, the one undoubted spectacular element in the flight were the initial phases of re-entry into the denser atmosphere, when cameras mounted on the vehicle’s control surfaces were able to video the build-up of super-heated plasma around the craft as it slammed into the atmosphere. While this has been filmed from within various space vehicles (Apollo, shuttle, etc.), this is the first time (I believe) it has ever been recorded from outside the vehicle going through re-entry.

Another unique element of the vehicle demonstrated prior to re-entry was the use of vented gas as a means of controlling the vehicle’s orientation. As noted above, cryogenic fuels tend to “boil off” and turn gaseous unless kept perfectly chilled. This gas must then be vented in order to prevent it becoming too voluminous and rupturing its containment tank (hence why rockets using cryogenic fuels are constantly venting gasses prior to launch following propellant loading & then having to be constantly “topped off”). However, rather than just letting go of this gas in space as they do on the ground, SpaceX channel it through a series of “cold thrusters” around the starship vehicle, enabling them to use the vented gas to “steer” the vehicle, avoiding the need for more traditional (and mass-using) thrusters systems requiring their own tanks of hypergolic propellants or gas.

While overall successful, the loss of both vehicles does mean a mishap investigation overseen by the FAA has been triggered, which may delay the planned launch of another test flight originally targeted for just a few weeks time. Even so, SpaceX are to be congratulated with the results overall, carrying the company as they do a modest step forward in the system’s development.

Continue reading “Space Sunday: starships, volcanoes and Voyagers”