The US Air Force’s Global Hawk became the first pilotless aeroplane to be given permission to fly routinely in civilian airspace on Thursday.
The US Federal Aviation Administration issued the USAF and Northrop Grumman, who make the jet plane, a certificate of authorisation (COA) allowing the RQ-4 Global Hawk to enter national airspace with almost as much ease as a piloted plane.
Previously the USAF was required to file a detailed flight plan with the FAA at least 30 days in advance. Now the majority of the red tape has been cut making it possible for an unarmed Global Hawk to “file-and-fly” even on the same day. The first use of the new COA will be a flight to Germany in October.
According to Northrop Grumman, the Global Hawk’s ability to see-and-avoid other aircraft has convinced the FAA that it is safe. Moreover, during its missions Global Hawk is programmed to climb to altitudes over 60,000 feet, well above commercial traffic.
Advertisement
However, air safety campaigners are horrified. “I think this is really insane,” says Gail Dunham of the National Air Disaster Alliance, a pressure group based in Washington DC. “I understand the need to have military drones,” says Dunham. But they should be restricted to military airspace only, she says.
Pre-programmed mission
Global Hawks carry out pre-programmed missions and are monitored by pilots from the ground via a satellite link. The plane was the first pilotless aircraft to cross the Pacific Ocean, a 22-hour mission involving just two “clicks” of a mouse from the ground operator.
The previous 30-day notice period allowed time to scrutinise both the flight plan and the support infrastructure required to track and control the plane. But Northrop Grumman’s spokeswoman told New Scientist that the performance and safety record of the Global Hawk, especially during military operations in Afghanistan, has now demonstrated its reliability.
The USAF has only ever lost three Global Hawks, says Northrop Grumman. The first was during the plane’s development, when someone accidentally tested the self-destruct program. As a result the plane flew to a pre-programmed, remote location and nose-dived into ground as its operators looked on helplessly. Since then two more were lost while flying in combat zones.
However, Pentagon data on the number of crashes per hours flown show that the Global Hawk has a crash rate 50 times higher than the F-16 fighter, a plane that frequently flies more dangerous missions and at lower altitudes.
Northrop Grumman is hoping to get similar grants for its armed version of the Global Hawk. But such military grants are just the thin end of the wedge for Dunham: “My concern is that commercial airlines are interested in applications like this too.”
![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)


