Europe rehearses a booster built to fly itself home
A 28-metre steel cylinder stood on a pad in the far north of Sweden in late July, filled with several tonnes of liquid nitrogen chilled to nearly minus 200 degrees, and ran a full launch countdown for a flight it would not take.[1] This was the wet dress rehearsal for Themis, Europe’s first attempt at a rocket stage that climbs toward space and then flies itself back to the ground.[2] A wet dress rehearsal loads the real propellant lines and runs the real countdown, stopping just short of ignition.[1] For a continent that has watched reusable boosters land for a decade without building one, it is a late but concrete first step.[2]
01 What happened
The rehearsal ran on 23 July at the Esrange Space Centre near Kiruna, with teams from ArianeGroup and the Swedish Space Corporation working a full-day chronology.[1] Liquid nitrogen stood in for the true propellants, liquid oxygen and liquid methane, so the crews could practise the cryogenic loading, the countdown, and the safing sequence without firing the engine.[1] Cryogenic here means fluids kept so cold that they stay liquid only near a couple of hundred degrees below zero.[3] With the rehearsal behind them, the teams are setting the window for the next test, a low vertical hop.[2]
02 The machine in numbers
One Prometheus engine sits under the stage, burning liquid oxygen and liquid methane and delivering a nominal meganewton of thrust, a little over a hundred tonnes of force.[3] Its designers set a target price near one million euros, about a tenth of what an engine of the previous generation cost, reached in part by printing many of its parts rather than machining them.[4] It is meant to fly five times.[5] The demonstrator it powers, called T1H, stands 28 metres tall and 3.5 metres across, with a dry mass near 30 tonnes.[4]
03 Why coming home is hard
Coming home is a throttling problem. A booster returns nearly empty, so as its tanks drain its thrust-to-weight ratio climbs, and a single engine at full power would fling the light stage back upward.[3] Prometheus is built to throttle down to about 30 percent of full thrust for exactly that reason.[3] Methane earns its place twice over. It burns cleanly, leaving little of the soot that would foul an engine meant to fly again, and it is dense enough to keep the tanks compact.[3]
The remaining hard part is control. The stage has to close a fast loop among its sensors, the throttling engine, and its steering, and hold a falling cylinder upright until its legs meet the pad.[2] A rehearsal on the ground proves the plumbing; only a hop proves the loop.
04 What to watch
The next milestone is that first hop, a vertical rise to roughly 100 metres and back down at Esrange, the window for which the teams are defining now.[6] A larger, three-engine vehicle bound for Europe’s spaceport in French Guiana is meant to follow around 2027.[6]
- SALTO Test Campaign: Themis reusable launcher first stage prototype conducts a flight chronology rehearsal — ArianeGroup
- Major rehearsal takes Themis one step closer to flight — European Space Agency
- Prometheus (nominal 1 MN variable thrust, 30–110% throttle, liquid oxygen–methane) — European Space Agency
- Themis (launcher): 28 m tall, 3.5 m diameter, 30 t dry, one Prometheus engine — CNES
- PROMETHEUS: target unit cost 1 M€ and five reuses — CNES
- ArianeGroup and ESA target first Themis hop test (100 m vertical takeoff and landing; three-engine vehicle for French Guiana) — SatNews
The falcon that brought back the first dust from an asteroid
A spacecraft no larger than a household refrigerator settled twice onto a rock shaped like a peanut, three hundred million kilometres from home, and came back carrying dust no one had ever held.[1] The grains were the first material ever lifted from the surface of an asteroid, and they settled a long argument about where the most common meteorites come from.[2]
01 The falcon that barely made it
The mission launched in 2003 as MUSES-C and was renamed Hayabusa, the falcon, once it was safely in space.[3] Its target was Itokawa, a stony body about 535 metres long and so loosely packed that nearly two-fifths of its volume is empty space.[4] This was a rubble pile rather than a solid rock, held together by little more than its own weak gravity.[4] Reaching it was the easy part. Two of the craft’s three reaction wheels, the spinning flywheels that hold a spacecraft’s aim, failed before sampling began, stripping away the fine pointing control it needed to hover over a moving surface.[3] Hayabusa made two brief touchdowns in November 2005. The device meant to fire a pellet into the surface never worked as designed, yet grains kicked up by the contact drifted into the collection horn anyway.[2] Then a fuel line leaked, attitude control was lost, and in December 2005 the falcon fell silent.[3] Controllers regained contact weeks later and nursed the battered craft home three years behind schedule, its return leg flown on a single improvised ion engine.[3]
02 Nearly everything was new
Almost every subsystem was being asked to do something new. Ion engines were the primary propulsion, not a trim thruster. Four microwave-discharge thrusters ran on xenon at a specific impulse near 3,000 seconds, a measure of how efficiently a rocket uses its propellant, and each produced about 8 millinewtons of thrust, roughly the weight of a coin resting on a palm.[3] Sustained over years, that faint push delivered about 1,900 metres per second of velocity change across more than 35,000 cumulative thruster-hours.[3] Navigation was just as unforgiving. A radio command took many minutes to cross the gap, far too long to fly a landing by hand from Earth, so the final descent was flown autonomously, the craft judging its own height above ground no one had mapped until it arrived.[3] Sampling in near-weightlessness offered no surface to press against, so the collection depended on catching whatever the touchdown threw up.[2]
03 Why it mattered, measurably
What the mission changed can be counted. The returned container held on the order of 1,500 particles, most smaller than ten microns and the largest near 180, for a total mass under a milligram.[2] Their mineralogy matched a common class of stony meteorite almost exactly, tying the ordinary chondrites that fall to Earth to S-type asteroids like Itokawa.[1] That closed a link telescopes alone had argued over for a generation.[1] The engineering was proven too. Microwave ion propulsion had carried a payload to another world and back, and touch-and-go sampling had worked in spite of failing hardware.[3]
The clearest measure is what followed. Hayabusa flew the same ion-cruise and touch-and-go plan again as Hayabusa2, which returned 5.4 grams from the asteroid Ryugu in 2020.[5] A separate American mission used a different sampler but the same round-trip logic to bring back 121.6 grams from the asteroid Bennu in 2023, more than twice what its designers had required.[6] In under two decades, asteroid sample return went from a single sub-milligram vial to laboratories on two continents sharing more than a hundred grams of pristine rock.[5]
04 Echoes today
The template is visible in every asteroid mission since. Ion propulsion for the long cruise, an autonomous approach to a body too distant to fly by hand, and a brief touch to lift a sample are now the standard grammar of the field, and the return capsules that parachute into desert ranges trace straight back to the one that limped home half-broken.[6]
- The Science special edition on Hayabusa research reports (Itokawa grains match ordinary LL chondrites; S-type link) — JAXA/ISAS
- Analysis of the grains returned by Hayabusa (~1,500 particles, total under a milligram, sizes, collection-horn capture) — The Planetary Society
- Hayabusa Asteroid Explorer Powered by Ion Engines, IEPC-2009-267 (four microwave thrusters, ~8 mN each, Isp ~3,000 s, ~1,900 m/s total, ~35,000 thruster-hours; reaction-wheel and fuel-line failures) — Kuninaka et al.
- The Rubble-Pile Asteroid Itokawa as Observed by Hayabusa (~535 m long, bulk density ~1.9 g/cm3, ~40% porosity) — Fujiwara et al., Science
- The sample from asteroid Ryugu: 5.4 grams returned by Hayabusa2 (2020) — JAXA/ISAS
- NASA announces OSIRIS-REx bulk sample mass: 121.6 grams from Bennu (2023) — Phys.org / NASA