Astronaut Robert Curbeam spent over 6 hours in space working on the space station (Image: NASA)
Two astronauts from the space shuttle Discovery have successfully attached a huge truss to the International Space Station. The spacewalk was the first of three designed to extend and rewire the orbital outpost.
US astronaut Robert Curbeam and Sweden’s first astronaut, Christer Fuglesang, spent 6 hours and 36 minutes in space installing the two-tonne truss segment to the ISS, among other tasks.
“Christer, you knocked yourself out,” mission control told Fuglesang. “From here on the ground, we’d like to send our congratulations for a 100% successful first [spacewalk],” said astronaut Steve Robinson, speaking from mission control.
Advertisement
The spacewalk ended at 0307 GMT on Wednesday as the station passed over north Africa. The operation was particularly sensitive because the astronauts had to move the truss within centimetres of the fragile solar arrays that provide electricity to the station.
In a delicate manoeuvre, the 3.37-metre (11-foot) truss was guided by the ISS robotic arm, operated by US astronaut Joan Higginbotham. She coordinated the movements with Curbeam and Fuglesang, who bolted the structure in place.
The spacewalking pair also hooked up six cables on the space station for electricity, communications and climate control. Last on their worksheet were operations to allow enough room for new solar arrays to track the Sun’s rays in a 360° rotation.
Double power
The ISS structure is being assembled piece by piece. Construction resumed in September with the Atlantis mission, after a three-year hiatus following the 2003 Columbia disaster.
Two other spacewalks, scheduled for Thursday and Saturday, are expected to be highly complex (see ). The astronauts are tasked with rewiring the electricity and climate control of the US-made portion of the ISS from its present, temporary set-up.
The work, during which power to half of the ISS will be switched off, includes activating the solar arrays installed by the Atlantis mission, doubling the station’s present electrical output.
The current Discovery mission is one of 14 shuttle flights NASA has planned over the next four years to complete construction of the ISS by 2010, when the shuttle fleet is to be retired.
All clear
Discovery blasted off on its 12-day mission late on Saturday from Cape Canaveral, Florida, in the first night launch in four years (see Rocket’s red glare to illuminate night launch).
NASA engineers say Discovery’s heat shield has not suffered any damage. Two preliminary inspections carried out after takeoff and shortly before Discovery docked with the ISS showed no cause for concern. Such inspections on the shuttles have become routine since the Columbia tragedy.
Columbia’s heat shield was pierced by foam insulation that peeled off its fuel tank during lift-off, causing the shuttle to disintegrate during its return to Earth on 1 February, 2003, killing all seven astronauts on board.
The Return of the Space Shuttle – Learn more in our continuously updated .
![Astronomers have long known that understanding how star clusters come to be is key to unlocking other secrets of galactic evolution. Stars form in clusters, created when clouds of gas collapse under gravity. As more and more stars are born in a collapsing cloud, strong stellar winds, harsh ultraviolet radiation and the supernova explosions of massive stars eventually disperse the cloud, and their light can bear down on other star-forming regions in the galaxy. This process is called stellar feedback, and it means that most of the gas in a galaxy never gets used for star formation. Researching how star clusters develop can answer questions about star formation at a galactic scale. Now, the state of the art has been further developed with both Hubble and Webb working together to provide a broad-spectrum view of thousands of young star clusters. An international team of astronomers has pored over images of four nearby galaxies from the FEAST observing programme (#1783), trying to solve this mystery. Their results show that it is the most massive star clusters that clear away their gaseous shroud the fastest, and begin lighting their galaxy the earliest. The team identified nearly 9000 star clusters in the four galaxies in different evolutionary stages: young clusters just starting to emerge from their natal clouds of gas, clusters that had partially dispersed the gas (both from Webb images), and fully unobstructed clusters visible in optical light (found in Hubble images). With Webb???s ability to peer inside the gas clouds, they were able to then estimate the mass and age of each cluster from its light spectrum. This image shows a section of one of the spiral arms of Messier 51 (M51), one of the four galaxies studied in this work, as seen by Webb???s Near-Infrared Camera (NIRCam). The thick clumps of star-forming gas are shown here in red and orange, representing infrared light emitted by ionised gas, dust grains, and complex molecules such as polycyclic aromatic hydrocarbons (PAHs). Within these gas complexes, each tens or hundreds of light years across, Webb reveals the dense, extremely bright clusters of massive stars that have just recently formed. The countless stars strewn across the arm of the galaxy, many of which would be invisible to our eyes behind layers of dust, are also laid bare in infrared light. [Image description: A large, long portion of one of the spiral arms in galaxy M51. Red-orange, clumpy filaments of gas and dust that stretch in a chain from left to right comprise the arm. Shining cyan bubbles light up parts of the gas clouds from within, and gaps expose bright star clusters in these bubbles as glowing white dots. The whole image is dotted with small stars. A faint blue glow around the arm colours the otherwise dark background.]](https://images.newscientist.com/wp-content/uploads/2026/05/13114322/SEI_296271016.jpg)


