Next week an American military spacecraft is due to begin the first
journey to a near-Earth asteroid. During the mission, Clementine will test
technology that could one day be used to track nuclear missiles in the Earth’s
atmosphere. Although primarily a military project, the mission is a cooperative
venture between the Department of Defense and NASA. Before heading off in
late May to the tiny asteroid Geographos for a close encounter around the
end of August, Clementine will spend much of the intervening period mapping
the surface of the Moon for civilian scientists (see Diagram).
The mission, which is costing less than $80 million, was originally
conceived by the Strategic Defense Initiative Organisation as part of the
Star Wars programme. It is now controlled by the Ballistic Missiles Defense
Organisation, which replaced the SDIO last year. The BMDO admits it has
no real interest in either the Moon or Geographos, but over the past decade
Star Wars scientists have developed military technologies, such as lightweight
components and sensors for tracking missiles, that the BMDO now wants to
test in space.
Light array
For instance, parts of the spacecraft will use carbon fibres instead
of aluminium. Clementine will generate electricity using an array of solar
cells made from gallium-arsenide-germanium semiconductors – the array will
be one of the lightest ever sent into space. And it will save this energy
in a nickel hydrogen battery that has twice the storage capacity of previous
power cells. A solid state data recorder, holding three times as much information
as conventional devices, will store information from sensors designed to
detect and track incoming missiles.…
![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)


