Tag: Spaceflight

China is continuing to expand its space endeavours on both the public and private fronts – drawing some flak from SpaceX fans in the process.

On Wednesday, May 28th, a Long March 3B rocket lifted-off from the Xichang Satellite Launch Centre, southwest China at 17:31 UTC, carrying aloft the Tianwen-2 explorer, bound for 469219 Kamoʻoalewa (2016 HO₃), an Apollo class, near-Earth object (NEO) and quasi-satellite of this planet.

A sample-return mission, Tianwen-2 is due to rendezvous with the 40-100 metre diameter asteroid in July 2026. It will spend some 7 months examining it and attempt to collect samples from its surface and sub-surface, using both touch-and-go (dropping briefly onto the asteroid in an attempt to gather samples before being pushed away using spring tension in the sample arm), and anchor-and-attach (literally hooking itself onto the asteroid). Departing the asteroid in April 2027, Tianwen-2 will then swing by Earth, dropping off gathered samples in a re-entry capsule in November of that year. In all, it is hoped that around 100 grams of material will be gathered from the surface and sub-surface environments of the asteroid. An interesting aspect of the mission is that Tianwen-2 will attempt to deploy a nano-rover onto the surface of 469219 Kamoʻoalewa, and place a nano-satellite in orbit around it.

The aim of the mission is to gain insight into 469219 Kamoʻoalewa, and either answer questions as to whether or not it is actually a chunk of the Moon blasted clear following an asteroid impact or, if not, it is hoped the mission will provide insight into the nature and characteristics of NEOs (particularly whether they also contain organic molecules), and allow comparative studies between the samples returns and those from Hayabush2 and OSIRIS-REx, furthering our understanding of asteroids and the role in the early solar system.

Returning the samples to earth will not be the end of Tianwen-2’s mission. Using Earth’s gravity after releasing the sample return capsule the vehicle to push itself onto a rendezvous 311P /PANSTARRS (aka P/2013 P5), which it will reach in 2031. This is an unusual object called an active asteroid – an object with an asteroid-like orbit, but exhibiting comet-like visual characteristics (such as having a tail). Estimated to be 240 metres across and with a sidereal period of 3.24 years, it was first located in 2013, and attracted attention due to its fuzzy, smudged appearance in initial images. Later that year, the Hubble Space Telescope revealed that the fuzziness was due to it having around 6 individual tails. These are thought to be the result of the asteroid is either spinning so fast, lose surface material is being thrown off of it, or that a series of “impulsive dust-ejection events” of unknown origin gave rise to a cloud of debris around the asteroid, which were then formed into the tails by solar radiation pressure.

Rather than just making a fly-by of 311P /PANSTARRS, the plan is for Tianwen-2 to use its solar-eclectic propulsion system to decelerate as it approaches the asteroid so that it can enter orbit and study it at length.

Also on May 28th, the private-venture launch company, Space Epoch, became the first Chinese company to make a sea-based vertical launch of a reusable rocket element and successfully recover it in a controlled splash-down.

The Yuanxingzhe-1 (YXZ-1 – also referred to a “Hiker 1”) is designed to be a reusable booster some 64 metres tall and capable for delivering 6.5 tonnes to a Sun-synchronous orbit (SSO). For the May 28th, flight, a test article standing 26.8 metres tall and using a single Longyun methane-liquid oxygen (methlox) motor and massing 57 tonnes, lifted-off from the sea-based Haiyang spaceport, Shandong province, at 20:40 UTC, climbing to an altitude of 2.5 km. The motor brought the vehicle to a hover before shutting down, allowing the vehicle to fall back towards the sea using four grid fins to maintain its vertical orientation. After a free descent, the motor then re-lit, slowing the vehicle and bringing it to a safe hover just a metre or so above the water. It then shut down, allowing the vehicle to gently enter the water and topple onto its side and await recovery. In all, the 125-second flight verified the broad operational parameters of the full-size Hiker-1, which will also splash-down at the end of its flights, rather than trying to land or be caught out of the air.

The flight, defined by Space Epoch as “100% successful”, immediately came under attack by SpaceX fans. The latter claimed China was merely “copying” SpaceX rather than innovating, particularly through the use of stainless steel in vehicle construction and methlox propellants, together the the use of four grid fins on the rocket for steerage / stability – as if SpaceX had any sole claim to these capabilities (they have not even patented the use of grid fins for rocket attitude control in an atmosphere).

A similar “they’re just copying!” came on May 29th, when another Chinese start-up, Astronstone, announced it has received sufficient initial funding to push ahead with its design for a reusable launch vehicle. Called the AS-1, this is intended to deliver up to 10 tonnes to low-Earth orbit (LEO) when being reused and up to 15.7 tonnes in fully expendable mode. It is to utilise methlox propulsion, stainless steel construction, grid fins for descent control and is to be designed to boost-back to its launch facilities and captured by “chopsticks” mounted on the launch tower.

In this, Astronstone is not shy about taking a leaf from the SpaceX book; the only difference is that of scale: AS-1 will be a modest 70 metres tall with a 4.2 metres main diameter (roughly the height of SpaceX Super Heavy, with half the diameter), while its 10-tonne reusable payload lift capacity is well in keeping with most modern commercial launch requirements. If successful, the company plan on offering the AS-2, capable of around two or three times the payload capacity of AS-1.

NASA: Budget Fears Confirmed; Administrator Nominee Removed

Earlier in May 2025, I covered the threats to NASA’s budget under cuts being considered by the Trump administration (see: Space Sunday: of budgets and proposed cuts and Space Sunday: more NASA budgets threats). At the time, the concerns were based on a so-called “skinny” budget document released by the administration, which outlined where the cuts would fall.

On May 31st, 2025, the administration quietly published a more detailed version of its federal budget proposal. This solidifies many of the threats to NASA’s mission. It confirms the intent to slash NASA’s budget by 24%, with the majority of the cuts coming within NASA’s space science, Earth sciences, aeronautic and education areas. In real terms, and adjusted for inflation, it sees the agency’s budget reduced to levels not seen since 1961, with the potential for 5,500 job losses and possible centre closures.

The science budget zeros-out 41 in-development or in-progress science missions. These Include:

• Many NASA Earth science programmes and missions, current and future, including the decadal survey Earth System Observatory missions; cancellation of most venture-class Earth science missions; and potentially impacts to the “cyclone watching” CGNSS network currently in operation.
• The in-development DAVINCI and VERITAS missions to Venus, and the Mars Sample Return Mission (MSR – not helped by NASA repeatedly shooting itself in the foot where this is concerned).
• The operational Mars Odyssey and MAVEN Mars orbiters (ending two valuable missions and limiting relay communications with other Mars missions); the New Horizons mission; OSIRIS-APEX – a mission extension to the highly-successful OSIRIS-REx, and intended to provide information on the Earth orbit crossing asteroid (and potential future impactor) 99942 Apophis.
• Multiple astrophysics programmes and missions, including the Chandra X-Ray Observatory, the Fermi Gamma-ray Space Telescope, and multiple, low-cost but highly effective Explorer-class missions.

The budget additional calls for an effective crippling of NASA’s biological and physical sciences,  reducing its budget to just US $25 million from US $87 million, and ending cooperation with the European Space Agency on Venus and Mars missions. While the flagship Nancy Grace Roman Telescope survives cancellation, it receives just half its requested budget – US $156.6million – potentially impacting its ability to be launched in 2026.

In terms of human spaceflight, the Trump administration is apparently initiating a “bold mission of planting the American flag on Mars”, which sees some 6.38% of NASA’s total budget being steered into Mars-centric initiatives:

• US $864 million for a “Commercial Moon to Mars (M2M) Infrastructure and Transportation Program” (which as side-note, will replace SLS / Orion after Artemis 3 – assuming any such system is actually flying by then).
• A total of US $400 million to be put into a “near-term entry, descent, and landing demonstration for a human-class Mars lander”, and commercial payload deliveries to Mars.

Some of this will be offset by the cancellation of the Lunar Gateway boondoggle; however, it is hard not to see hints of the influence of the SpaceX CEO in these matters. He has been vocal in his opposition to anything other than his “grand vision” of colonising Mars, and these budget allocations, particularly the US $400 million appear to be directly tailored to SpaceX’s benefit, the company apparently prioritising landing a “human-class lander” as soon as possible, and then moving directly to cargo deliveries.

Isaacman Out

The budget details came alongside the shock announcement that the White House has withdrawn entrepreneur Jared Isaacman at its nominee to lead NASA.

Isaacman’s nomination caused mixed reactions when first announced. Whilst the majority were positive, there were also concerns over his ties to the SpaceX CEO, and the latter’s views on NASA’s future direction. During his Senate confirmation hearings, Isaacman handled the latter concerns directly, and indicated his own opposition to some of the proposals in the Trump NASA 2026 budget. As such, it was widely anticipated the Senate would confirm his appointment on June 3rd, 2025.

No reason has been given by the White House for withdrawing his nomination. Some have speculated it is as a result of the recent rift between the President and the SpaceX CEO, with whom Isaacman has a strong association. Also, Isaacman’s confirmation hearing also revealed he has been a past financial supporter of the Democratic Party – something hardly likely to endear him to the White House incumbent. In a statement on the withdrawal, White House assistant press secretary Liz Houston would only say:

The Administrator of NASA will help lead humanity into space and execute President Trump’s bold mission of planting the American flag on the planet Mars. It’s essential that the next leader of NASA is in complete alignment with President Trump’s America First agenda and a replacement will be announced directly by President Trump soon.

Again, the emphasis on Mars here is loud enough to be almost deafening – and in line with the goals of the SpaceX CEO. This is not to say the the latter will now be the likely pick to head-up NASA; it is highly unlikely he would survive Senate hearings even if nominated. However, it does perhaps indicate his push for having NASA effectively abandon the International Space Station and the Artemis programme in favour of Mars have been taken to heart by a President who is all about being “first” in everything.

Thus far, all of the Trump administration proposals for NASA’s budget have been met with widespread condemnation from the aerospace, science and educations sectors in the US. Many are hoping that Congress will stop this tear-down of NASA dead in its tracks when the budget comes before the Capitol later in the year. As to Isaacman being removed as nominee, this has been received with dismay and upset within the US space industry, and leaves NASA in a continuing state of limbo.

Starship IFT9: Up and Bang Again¹

On Tuesday May 27th, 2025, SpaceX once again attempted to carry out their 9th integrated flight test (IFT-9) of their Starship / Super Heavy combination in the hope of getting the former into sub-orbital space to carry out a series of tests, and use the latter as a test article during its descent back to the Gulf of Mexico. As such, the flight had a number of distinct goals for both the booster and the starship vehicle.

• Booster (√ = success; Χ = failure):
  • Re-fly a Super Heavy for the first time – the unit used in the January 2025 test article flight (with just 4 of its 33 Raptor 2 motors replaced)  (√).
  • Attempt a new “rollover” manoeuvre after starship separation (√).
  • Test a new high angle of attack re-entry into the lower atmosphere in an attempt to use atmospheric drag to reduce velocity and reduce the need to carry propellants for propulsive braking (Χ).
  • Carry out an updated engine braking burn (Χ).
  • Splash-down in the Gulf of Mexico (Χ).
• Starship (√ = success; Χ = failure):
  • Reach a sub-orbital trajectory (√).
  • Deploy a set of 8 Starlink satellite simulators, testing the payload bay slot in the process (Χ).
  • Carry out the re-start of a sea-level Raptor engine to test de-orbit burn capabilities (Χ).
  • Make a successful re-entry into the atmosphere and test updates made to the thermal protection system and to hopefully reduce burn-through on the fore-and-aft aerodynamic flaps (Χ).
  • Splash-down in the Indian Ocean (Χ).

Lift-off was at 23:37 UTC, from the SpaceX Starbase City facilities in Texas, and proceeded to a successful staging. The booster then performed its intended roll-over and carried out a good boost-back burn. It was lost 6 minutes 20 seconds after launch, as 13 of the engines were due to fire at the start of their braking burn.

The starship vehicle continued on to its sub-orbital trajectory and successfully shut-down its motors. The deployment of the payload simulators was due at 18 minutes into the flight, but was abandoned when the deployment slot door again failed. By 30 minutes into the flight the vehicle was pitching / rolling wildly, and SpaceX confirmed they had lost all attitude control, likely the result of a propellant system leak. The vehicle subsequently made an uncontrolled re-entry over the Indian Ocean 46 minutes after launch and largely burned-up.

Whilst subject to confirmation, the propellant leak potentially hints at a vulnerability in the starship design. Most space vehicles utilise hypergolic thrusters for attitude control and fine manoeuvring. Independent of the main propulsion system, these avoid the need for complicated propellant bumps, etc.. However, the propellants are high toxic, and such systems do add mass to a vehicle. By contrast, SpaceX effectively pumps boil-off gases from the main propellant tanks around the vehicle to so-called “cold thrusters” and their own small tanks. Doing so removes the need for the majority of the mass (and engineering space) used by hypergolic thruster systems and avoids the complications of handling toxic materials during vehicle refurbishment between flights. However, the plumbing used to deliver the gases around Starship and Super Heavy is all interconnected; thus – and possibly as demonstrated with IFT-9 – there is a risk of a single leak impacting multiple attitude control thrusters.

Both the booster and the starship came down within their designated hazard zones; however, the flight will be subject to an FAA-required mishap investigation.

1. With apologies to the estate of J.R.R. Tolkien and Bilbo Baggins, Esq., formerly of The Shire

As NASA faces the threat of significant cuts in its science missions and research budgets, together with a potential overhaul of the US-led Artemis Project, China has further indicated its commitment to expanding its human presence in space, while the European Space Agency could see an increase in its budget (subject to end-of-year approval), amidst a call for Europe in general to increase its overall spending on space-based activities.

China has confirmed that it will be moving ahead with an expansion of its Tiangong space station with up to three new modules, potentially doubling its size. First hinted at in late 2022, the new modules are believed to comprise:

• An updated version of the Tianhe core module , being referred to as the expansion module, providing additional power systems, a new multi-port docking adaptor equipped to handle a range of vehicles, including the upcoming next generation crew vehicle.
• Two multi-function science modules, likely updated versions of the current Wentian, and Mengtian science modules.

The new modules are to include state-of-the-art engineering and maintenance capabilities, such as 3D printers capable for producing replacement parts used on the station (as had been introduced with the International Space Station), as well as allowing the total crew mission complement aboard the station to be expanded.

In confirming the expansion plans during a China state television interview, Wang Jue from China Aerospace Science and Technology Corporation (CASC) stated that the timeline for the expansion has yet to be confirmed, but in keeping with launches for the station to date, the modules will be flown aboard the Long March 5B booster, currently China’s most powerful launch vehicle and capable of pushing up to 25 tonnes of payload to low-Earth orbit (LEO).

Wang also confirmed that Long March 5B is itself undergoing “reliability and safety” updates – although these are not interrupting the current launch schedule. In particular, China is looking to make the re-entry of the rocket’s large first stage a more controlled affair. The country has been heavily critiqued for its Laissez-faire attitude of just allowing the first stage, which tends to fly higher than the first stages of comparable western rockets, to simply make an uncontrolled re-entry and break-up over the Pacific Ocean, rather than actually guiding it towards doing so.

Most recently, the Long March 5B has been used to launch the first batching of China’s Guowang (also called Xingwang and Hulianwang – the latter being the name of the satellite class) megaconstellation to compete with Starlink. It has taken over this role from the Long March 2 and 3 vehicles to accelerate the deployment of some 13,000 operational Hulianwang satellites of various classes. These will be placed into a range of orbits, as is the case with Starlink, allowing the system to join Starlink in further interfering with Earth-based astronomy on a global basis and adding to the amounts of pollutants dumped into the upper atmosphere annually as defunct satellites in the systems re-enter and burn-up.

The next space station related launch for Long March 5B, meanwhile, is due in 2026. This will be to deliver the free-flying Xuntian space telescope, a “Hubble class” orbital observatory. It will operate largely remotely from, but in a co-orbit with, Tiangong, the crews from which will perform routine maintenance on the telescope.

With a 2-metre diameter primary mirror offering a field of view some 300 times greater than the Hubble Space Telescope, Xuntian will be equipped with a 2.5 gigapixel imaging system and will be used to study areas including dark matter, dark energy, galaxy formation and evolution of the cosmos. China has stated the observatory will be offered for international science and research.

One major aspect of the Tiangong expansion will be the ability for the station to house larger crews, including tiakonauts from China’s partner nations. The country is due to shift its crewed spaceflight capabilities from its current Shenzhou, 3-person vehicles, to its modular, multi-function and semi-reusable Mengzhou (“Dream Vessel”) craft.

The latter, due to commence operations in 2027 or 2028, will be able to deliver up to 6 crew at a time to Tiangong (or 3 crew and a half-tonne of equipment). A further variant of the craft will form the vehicle for delivering crews of three to lunar orbit in the 2030s, who will then use the companion Lanyue (“embracing the moon”) lunar lander (launched separately) to descend to and return from the surface of the Moon, in order to achieve China’s intent to establish a permanent human presence on the Moon in the 2030s.

Rocket Lab Gains US DoD Support

Rocket Lab, the little company looking to out-SpaceX SpaceX, has gained a further boost in confidence.

Currently, the company is best known for its Electron semi-reusable launcher capable of putting 320 kg to LEO and 150 kg to Sun-synchronous orbit (SSO). However, Electron is just one element in a multi-part strategy that has enabled Rocket Lab to achieve considerable success. As well as the booster, the company has developed its own range of 3D printed rocket engines, develops satellite for customers, and has built a multi-purpose spacecraft “bus” called Proton, capable of delivering payloads to orbit or to other planets, as well as other tasks.

But one thing CEO Sir Peter Beck said the company would never do was move into the field of building “big” rockets – and he was so adamant in this, he promised to eat his hat if the company decided otherwise. And eat his hat he did, some four years ago, when Rocket Lab announced it was developing Neutron, a medium-lift launch vehicle (MLLV) capable of delivering up to 13 tonnes to low-Earth orbit.

As launch vehicle go, Neutron is unique. The entire first stage of the vehicle is a rocket unto itself – and fully reusable. Rather than comprise a first stage with one (or more) stages bolted on top of it and the payload on top of those, Neutron is designed to carry its “upper” stage and its payload inside itself. On reaching orbit, the nose of the vehicle opens up, allowing the “upper” stage (an expendable kick stage) with the payload attached, to be pushed clear, prior to igniting its motor.

The first launch of a Neutron vehicle is due later in 2025, and in keeping with the likes of SpaceX and Blue Origin, Rocket Lab will attempt to recover the first stage with an at-sea landing on specially adapted landing barge. But even before its first flight, Neutron has been given a double boost (no pun intended) by the US Department of Defence. The first of these is that Rocket Lab, with Neutron, has been cleared to bid for US National Security Space Launch (NSSL) contracts through to 2029. As SpaceX knows, this is a lucrative market, and Rocket Lab is the first public-traded launch company to be selected to possibly fly NSSL missions to orbit. The company has already commenced launch assurance reviews with the US military, and Beck has indicated that Rocket Lab could present bids for NSSL launches as soon as mid-2026.

In addition, the US Air Force (somewhat keen to regain some of the space high ground it has had to cede in the formation of the United States Space Force) has also selected Neutron as the test vehicle for the Rocket Experimentation for Global Agile Logistics (REGAL) initiative, intended to assess the use of rocket vehicles to rapidly deploy materiel from locations in the United States to “anywhere in the world” in what are referred to as “point-to-point” flights.

This idea was recently given a stir by the SpaceX CEO, stating that company’s Starship / Super Heavy combination would be “ideal”. While interest in the concept has remained within the USSF and USAF, the selection of Neutron for initial testing is a poke in the eye for SpaceX and one which makes a lot of sense. While Neutron cannot lift the upper end of Starship’s payload spectrum, it is entirely possible that in point-to-point operations, Starship would have its payload capacity somewhat limited. Further, Neutron is ready-made for landing on its own feet, Starship isn’t, and it doesn’t require a bloody great booster to get it (and any payload it has to carry off the ground at either end of the operation.

However, that said, the whole idea of REGAL is questionable. It’s not like you can simply lob a rocket on a ballistic flight, flip it over and land it anywhere you like. It requires quite substantial infrastructure at either end of the equation (assuming you’d like it to return to base after a flight, at least). A landing / launch platform is required; you need propellant storage and delivery / pumping capabilities; payload handing equipment, skilled personnel and facilities to undertake these and other operations. None of which can just be thrown up overnight.

As such, any idea of “point-to-point” capabilities is at best limited to complex facilities fully capable of handling the receipt and launch of the booster vehicle and payload. While this doesn’t entirely rule the idea out, it does restrict where and how such capabilities might be used; it’s hard to see such a system dropping into a FOB in a zone of conflict, or putting down right on top of a natural disaster to deliver aid – two of the promoted ideas behind REGAL. Given this, it will be interesting to see what develops as REGAL testing commences, potentially (again) in 2026.

Voyager 1: Thrusters Recovered

In another deep space piece of miracle working that would impress Montgomery Scott, NASA engineers have recovered a set of thrusters vital for communications with Earth, on their Voyager 1 spacecraft – twenty years after the system was considered defunct.

The Voyagers maintain communications with Earth via a large high-gain communications dish they carry on their “backs”. However, as they move through interstellar space, both Voyager 1 and Voyager 2 must carry out periodic “roll manoeuvres” to ensure these dishes remain  aligned with Earth for communications to continue.

These manoeuvres are carried out using small sets of thrusters on each vehicle, under the guidance of a star tracker system. The latter calculates the position of Earth and the spacecraft’s required orientation thereto by means of observing a set of notable stars the system can “see”, and using their positions to calculate where Earth is and the degree of roll the vehicle must make to re-centre the communications dish.

In 2004, the heater units required to warm the “primary” thrusters on Voyager 1 started to show signs of failure, risking a possible thruster misfire which could swing the vehicle so far off-axis, its star tracker would no longer be able to identify the stars in needed to  carry out its calculations. Because of this, operations were switched to the “back-up” thrusters.

By 2018, these “back-up” thrusters (now re-designated the “primary thrusters) were encountering issues as a result of the build-up of residual material in their chambers after each use.  Steps were taken to reduce this issue by placing some of the remaining thrusters into “reserve”, the idea being to switch to the “reserve” thrusters if those remaining in operation become too unreliable for continued use.

This actually happened in September 2024 – however, it transpired that the “reserve” thrusters were already badly “clogged” with residual material. This might not have been a critical issue but for the fact that, starting in May 2025, the 70-metre diameter Deep Space Station 43 (DSS-43) radio communications dish located in Canberra, Australia, would be going off-line for a 10-month overhaul. A part of NASA’s Deep Space Communications Network (DSN), DSS-43 is the only Earth-based communications system available to NASA for communications with either of the Voyager craft.

The concern was that if Voyager 1 was allowed to continue to rely on its increasingly faulty thrusters, a misfire might occur whilst DSS-43 was offline, and the craft would be “lost” as a result of a communications breakdown. To avoid this, the decision was taken in March 2025 to try to recover the original thrusters system on the grounds that they would have 20 years less wear-and-tear and residue build-up, due to being inactive.

Even so, switching back to them would not be without risk; Voyager 1 would have to restore power to the thrusters disabled in 2004. However, with a dwindling ability to generate electrical power (since 1998, NASA has had to periodically shut-down instruments on each Voyager craft so they could maintain some degree of minimal operational and communications capability); as such there was real concern any power-up of the electrical systems on the 2004 thrusters could cause a damaging electrical surge – particularly given the previously-faulty heaters – or a thruster misfire, ending communications with Earth.

The attempt to do so was made in March 2025; it was carried out in stages designed to ensure if anything went wrong, Voyager 1 would still be capable of locating Earth again in the event of the latter occurring.  With a 46-hour lag in two-way communications between Earth and Voyager 1, the attempt was made in late Match 2025 – and proved a success.

On March 20th, 2025, mission control at the Jet Propulsion Laboratory, Pasadena, California, received the information they’d hoped: Voyager 1 had successfully brought the 2004 thruster system back on-line. There was no power spike, no issue with the thrusters firing, and Voyager 1 confirmed it had completed the test manoeuvre.

Since then, the system has continued to be monitored, and with DSS-43 due to go down for its upgrade, control was swapped from the increasingly at-risk “back-up” thrusters back to the “primary” thrusters.  This should hopefully allow Voyager 1 to maintain contact with Earth, even without it being able to receive commands of any complexity (there are narrow windows of opportunity in the DSS-43 overhaul during August and December 2025, where it could send short sequences of commands to the Voyager craft), and be ready to say “hello!” once more when full communications are resumed in 2026.

A Soviet-era space mission finally drew to a close on Saturday, May 10th, 2025 (UTC) after 53 years in space – although admittedly, that wasn’t really the plan when it was launched. Also, it’s fair to say that for the vast majority of that time, it has been little more than a hefty lump of space junk looping repeatedly around the Earth rather than doing anything useful.

However, its return marks an opportunity to recall an interesting period of the early era of the space age. A time when both the US and the Soviet Union were just starting to get to grips with lobbing humans into orbit, but when the latter already had grander designs in mind – starting with an aggressive programme to study Venus.

Initiated in 1961 – the same year as a human first flew into space – the Soviet Venus, or Venera, programme was a daring and high-stakes programme given the overall reliability and sophistication of rocket vehicles and space probes at the time. Thus, over a period of 23 years and 29 missions, it had a fair few highs and lows.

For example, of those 29 missions, 12 never even made it Venus, while several others didn’t go fully to plan. However, of those that did get to Venus, their successes were remarkable, whether or not all mission objectives were achieved:

• The first fly-by of another planet (Venera 2, 1965/66- although contact was lost prior to any data being returned).
• The first vehicle to impact the surface of Venus (Venera 3, 1965/66 and twin to Venera 2, although a failure with the carrier vehicle meant that again, no data was returned).
• The first vehicle to reach the atmosphere of another planet and return data to Earth (Venera 4, 1967).
• The first vehicles to perform a deep analysis of the atmosphere of Venus, down to an altitude of around 20 km (Venera 5 and Venera 6, 1969).
• The first vehicle to successfully land on another planet and return data from it (Venera 7, 1970).
• The first vehicles to successfully return images from the surface of Venus (Venera 9 and Venera 10, 1975).
• The first vehicles to return colour images from the surface of Venus and the first to record sounds from Venus -the wind the mechanical operations associated with the landers. (Venera 13 and Venera 14, 1982).
• The first vehicles to deploy balloons on Venus (Vega 1 and Vega 2, 1985).

Among these missions, some are worth a little further highlighting. For example, because it was still considered that the surface of Venus could have liquid water present, Venera 4 was designed to float in event of a splashdown, despite massing 383 kg. It was also fitted with antenna deployment locks made of sugar.

The idea behind this latter point was that if Venera 4 landed on water, the impact force might not be sufficient to trigger the release of the locking mechanism and allow the main communications antenna deploy. However, the impact on water would result in the locking mechanism being splashed with water – which would (in theory) dissolve the mechanism, allowing the antenna to be deployed!

It was initially thought that Venera 4 was the first vehicle to actually reach the surface of Venus. However, due to a combination of error margins built into some of the instruments coupled with inconsistencies between data obtained by Venera 4 and later probes, it is now believed that Venera 4 only reached somewhere between 55 and 26 km above the planet’s surface before succumbing to the harsh conditions.

Whilst Venera 5 and Venera 6 also failed to reach the surface of Venus in an operational capacity, they are remarkable as they were able to remain aloft for more than 50 minutes each, drifting under their parachutes and gathering data on the nature and composition of the planet’s atmosphere, gently descending to with 20 km of the surface before finally being overwhelmed.

The story of Venera 7 is in part one of diligence over dismissal. Immediately after receiving confirmation the vehicle was on the surface of Venus, mission controller seemed to lose all contact with the lander. Attempts were made to re-establish contact, with the recording tapes on the communications link still recording. Eventually, unable to diagnose the issue, the mission was dismissed as lost without data.

However, several weeks later, radio astronomer Oleg Rzhiga decided to review the recordings of the landing and subsequent events. In doing so, he found 23 minutes of faint, data-carrying signal had in fact received from the lander. Venera 7 hadn’t failed, it had simply been knocked off-axis on landing, resulting in its radio signal only being faintly received but passed unnoticed by mission controllers at the time.

Finally, there are the two Vega missions, remarkable for a number of reasons. “VeGa” is actually a westernisation of ВеГа, itself taken from the first two letters of the Russian for “Venus” (Венера) and Галлея (“Halley”  – or “Galleya”). This latter part of the name indicated their primary mission focus – rendezvousing with Comet Halley, which was making one of its (on average) 76-year revisits to the inner solar system.

However, in order to reach the comet, the probes would need a gravity assist from Venus. This meant that they could also piggyback Venus-centric missions, releasing them as they approached Venus for their fly-by. The Venus element comprised two landers of a similar design to earlier Venera craft, and intended to study both the atmosphere and surface of the planet. Unfortunately, turbulence encountered during descent caused the surface instruments on the Vega 1 lander to activate before touch-down, so that only the mass spectrometer returned data once on the surface. The Vega 2 lander was more successful, returning data for a period of 56 minutes, post-landing.

The more fascinating part of these missions was the use of balloons. These were released as a package by the landers at some 60 km above the surface of Venus. Parachutes initially slowed their descent to a point where, at an altitude of around 50 km, a mechanism attached to the parachute systems inflated each balloon with helium, the parachute and inflation system then being jettisoned. This allowed both balloons, each dangling a 7 kg gondola of instruments, to climb back to an altitude of some 53 km, which they drifted 11,000 km around Venus – 30%of its circumference – transmitting data to their respective Vega craft for relay to Earth. Both balloons were still actively transmitting when the Vega craft passed out of communications range, 45 minutes after the balloons started sending data.

Of the failures, the majority came, not unreasonably, in the early days of the programme. Of the first eight attempts to reach Venus between February 1961 and April 1964 (launch dates), all failed. As a result, six were never officially designated – as was the Soviet approach in the first years of their space programme (i.e. if it doesn’t have an official designation, it didn’t happen and so couldn’t have failed). Of the remaining two, one gained the Venera 1 designation, as it made it out of Earth orbit (but failed while en route to Venus) and the other being designated a “Kosmos” mission.

Originally, “Kosmos” was a catch-all designation for Soviet Earth-orbiting uncrewed missions. It was intended to obfuscate and confuse western agencies, in that it didn’t matter the object in question was a piece of test hardware or a surveillance satellite or a communications relay, or a navigation beacon, or a weather satellite or whatever. If it was orbiting the Earth, it was called “Kosmos” and given a number. In 1962, the designation was extended to include any Soviet interplanetary probe that failed to leave Earth orbit, allowing failure to be hidden in plain sight. Only after a mission was on its way to its intended destination would it be given an actual mission designation (e.g. Venera 1, etc.).

Within the Soviet-era Venera programme, five vehicles gained the Kosmos designation:

• Kosmos 27 (one of two Zond missions for Venus launched on March 27th, 1964, and breaking-up in the upper atmosphere 24 hours later after failing to achieve a stable orbit).
• Kosmos 96 (launched on 23rd November 1965, failed to depart Earth orbit, burned-up in the upper atmosphere on December 9th, 1965, possibly resulting in the  Kecksburg UFO incident).
• Kosmos 359 (launched on 22nd August, 1970, suffered an upper stage motor failure and re-entered the atmosphere on November 6th, 1970)
• Kosmos 482 – the cause of this article, and of which more below.

Intended to be the partner probe to Venera 8 (keeping to the naming convention to the actual run of successes), what was to become Kosmos 482 was launched on March 31st, 1972. However, a malfunction occurred as the upper stage booster motor was re-lit to transfer the probe onto its trajectory to rendezvous with Venus, and the vehicle broke up.

Some of the debris from the break-up fell to Earth in the form of 38-cm diameter, 13.6 kg titanium pressure spheres, most likely from the booster stage. These struck crop fields just outside of Ashburton, New Zealand, 48 hours after launch. However, the two larger elements of the break-up were pushed into 210 km x 9,800 km elliptical orbit around Earth, initially travelling close together, gaining the Kosmos 482 designation.

In the west, there larger of these two elements was identified as the remnants of the booster rocket and the Venus Bus, intended to provide power to the 495 kg lander. They were given the Designation 1972-023A. The smaller of the two was identified as most likely being the lander itself, clearly separated from its bus and booster, and so designated 1972-023E.

Over the next nine years, the two travelled in partnership, looping around the Earth, each pass having an increasing effect of 1972-023A, which gradually started breaking up, depositing pieces of itself to burn-up in the atmosphere (some surviving to fall on poor New Zealand again!) until it succumbed to atmosphere friction and burned-up on re-entry in mid-1981.

The lander – or 1972-023E – was made of sterner stuff, and continued to loop around Earth largely unfazed and forgotten. But each time it did make a close flyby there was exchange: a little velocity here, a little change in trajectory there. Over the decades, these little changes served to pull the craft closer and closer to Earth, such that by this year, it was looping around us once every 80-90 minutes, with its apogee and perigee both slipping into sub-200 km altitude figures. All of which meant that atmospheric entry was all but certain; the question was when? By the start of May 2025, NASA and ESA were looking to a re-entry window extending from May 9th through May 13th,which was then quickly narrowed down to the early hours of May 10th (UTC) – albeit with an initially wide margin of error (+/- 3.3 hours).

Given the orbital track of the debris, and the fact it was designed to survive the much tougher entry into the atmosphere of Venus, there were fears it could come down intact on a populated area. However, this was always unlikely, given that while it did pass over population centres each and every orbit, it also passed over large tracts of largely empty land (in human habitation terms), and even greater amounts of open ocean. Further, even if it did survive re-entry (not an absolute certainty given that both its age and the fact it would likely start tumbling during an uncontrolled atmospheric and most likely break-up / burn-up), it would not come crashing through the atmosphere at a huge velocity and explode in a massive air-burs. Rather, it would fall with a maximum velocity of around 250 km/h – enough to be decidedly upsetting if it hit a building or similar, but not enough to result in something like a city-wide disaster.

As it is, and at the time of writing, Roscosmos have stated that the vehicle re-entered the atmosphere at 06:24 UTC on May 10th over the Bay of Bengal, 560 km west of the Andaman Islands and prior to impacting the Indian Ocean somewhere west of Jakarta, Indonesia. However, this had yet to be confirmed by other agencies, although ESA indicated the vehicle potentially re-entered the atmosphere between 06:04 and 07:32 UTC, which would place its impact point most likely somewhere in the Indian or Pacific Oceans.

Kosmos 482 marked the last failure within the Soviet-era Venera programme, and its return to Earth acts as a very physical closure to that era of space history. However, it does not close the book on Russia’s ambitions where Venus is concerned. Currently, Russia is planning a return to Venus as it resumes its Venera programme with Venera D.

This mission – which is subject to a lot of ifs and maybes, already having been delayed on multiple occasions. When first conceived in 2003, it was targeting a 2013 lunch date; currently, the mission is slated for a launch no earlier than 2031, although it has yet to have its science packages finalised and developed. Comprising an orbiter and lander, if it does go ahead, Venera D (also sometimes called Venera 17) will deliver heavyweight (1.6 tonne) lander to the surface of Venus with the intentions of it being able to survive and carry out science studies for up to 3 hours after landing.