The skies may no longer be free for the space industry. Rocket companies like SpaceX and United Launch Alliance (ULA) may soon be required to pay a fee to support FAA oversight and airspace coordination, part of a broader effort to keep up with the growing launch industry.
A budget reconciliation bill released by Senator Ted Cruz last week proposes that the Federal Aviation Administration (FAA) begin charging licensing fees to rocket companies starting next year. The collected fees would go into a trust fund to help the FAA’s Office of Commercial Space Transportation (AST) acquire more resources needed to manage the growing number of rocket launches as it faces budget cuts for the coming year.
Today, companies like SpaceX are required to pay small fees that cover the application process for launch and reentry licenses issued by the FAA. In return, the FAA clears airspace of commercial and private flights during the rocket launches and along the path of reentry. Airlines, on the other hand, do pay fees to the FAA, which go into the Airport and Airway Trust Fund that makes up nearly half the administration’s annual budget.
The burgeoning space industry is placing an added burden on the FAA, and the authors of the proposed bill suggest it’s time for companies to start paying their dues. “You have this group of new users that are paying nothing into the system that are an increasing share of the operations, and I truly believe the current structure isn’t sustainable,” former FAA administrator Michael Huerta told NPR in an interview in May 2024.
The FAA initially waived fees for space companies to help the industry grow in its early years. Last year, SpaceX launched 134 rockets to orbit, mostly the Falcon 9, and it’s aiming to break its record with 170 launches in 2025. As a clear industry leader, SpaceX dominates the use of airspace over the U.S., while other companies like ULA carried out a total of five launches in 2024.
SpaceX executives have also been the most vocal against the FAA’s lack of resources and its inability to keep up with the growing space sector. In 2023, William Gerstenmaier, SpaceX’s vice president, spoke at a hearing by the Senate subcommittee on space and science, warning that the FAA’s licensing department is in “great distress” and “needs twice the resources it has today.”
Perhaps SpaceX didn’t anticipate that the funding for those resources would come out of the company’s own pockets. The new bill suggests the FAA charge rocket companies based on the weight of the payload per launch, starting with $0.25 per pound in 2026 and gradually increasing by approximately $0.10 every year. In 2033, companies will potentially have to pay $1.50 per pound of payload. For SpaceX, the fee for a Falcon 9 launch of the company’s Starlink satellites would amount to an average $9,400 in 2026, according to Ars Technica. SpaceX launched 89 Starlink missions in 2024, which would have cost it around $836,600 under the suggested fee guidelines.
The FAA’s AST could use that money as it faces a tight budget for 2026. The U.S. administration’s skinny budget, released last month, allocates $42 million for AST. The FAA’s overall budget request for 2026 is $22 billion, a very small portion of which will be used to expand the staffing for launch and reentry licensing. The budget for the FAA’s commercial space office increased from $27.6 million in 2021 to $42 million in 2024 to account for the increasing number of rocket launches. The AST received roughly the same budget in 2024 and 2025, without accounting for inflation or a continually growing industry. The suggested trust fund could help fill the budgeting gap for the FAA, and allow it to expand its rocket licensing operations.
Space companies have been quick to criticize regulatory bodies like the FAA for slow processes, but now it might be time for them to pay up to launch their rockets on a speedier timeline.
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![Scientists Say Some Black Holes Are Born From Other Black Holes
Since LIGO’s Nobel-winning discovery of gravitational waves—ripples in spacetime—the U.S.-based detector has been picking up on hundreds of signals from black hole mergers. And, after a decade of studying gravitational waves, researchers believe a significant fraction of black holes may come from cosmic chain reactions. A recent paper published in Physical Review Letters describes an analysis of 155 pairs of binary black holes, identified by LIGO and its sisters, Virgo and KAGRA, in Italy and Japan, respectively. According to the study, about 14% of merging black holes may be what’s called “second-generation black holes,” or black holes that form from previous mergers of two smaller black holes. This “hierarchical” backstory is vastly different from the textbook version of how black holes emerge from the explosive death of a star. “Overall in the universe, black holes are merging all the time,” Cailin Plunkett, the study’s first author and a graduate student at the Massachusetts Institute of Technology, told MIT News. “Now we’re seeing a relatively consistent picture where there’s a decent percentage of black holes that are coming from this repeated pathway.”
Tracking the invisible Gravitational waves that reach Earth’s detectors typically come from extremely intense events. Over the years, LIGO has picked up some truly perplexing signals. For example, last summer it found the most colossal black hole merger ever—and if that wasn’t wild enough, the black holes that took part in the merger lie within a cosmic “dead zone” for black holes.
This zone refers to a range of black hole masses in which, physically speaking, black holes can’t form through ordinary stellar collapse. From these discoveries, astronomers realized just how little we knew about black holes, which are challenging to investigate directly. In that sense, it was a no-brainer that the ever-growing catalog of LIGO’s gravitational signals would turn up entirely new insights about black holes. “It is increasingly clear, both from individual events and population analyses, that massive black holes exist in [this] range,” the researchers wrote in the latest paper. “These observations have spurred further investigation into mechanisms that can populate this gap.”
A wobbly imprint The latest research represents one such investigation. During mergers, the two black holes spiral toward each other along an orbital plane. When one or both black hole spins are misaligned, the orbital plane can wobble, or “precess,” the researchers explained to MIT News. The degree to which the disk wobbles acts as a parameter from which researchers can measure the masses and spins of the merging black holes. One telling sign of hierarchical mergers is that they’re “lopsided,” meaning one of the pair has a much higher spin and mass than the other. For the study, the team created an analytic model to capture the kind of wobble that would have emerged from second-generation black holes. Around 14% of merging black holes followed this pattern, and the second-generation black holes identified had a very specific range of masses, at around 20 solar masses or 40 solar masses and above. Of mysterious origins To be fair, that might not sound like a whole lot. But it demonstrates that a sizeable portion of known black holes indeed follow this pattern. As for why, the team suspects hierarchical mergers emerge from dense stellar environments. Simply, when multiple neighboring stars die and collapse into black holes, the dense environment can make it easier for those black holes to find each other and merge. That could further lead to the formation of second-generation black holes. Theoretically, this could “repeat potentially ad infinitum, by virtue of the fact that you have a ton of stars and black holes in this really dense environment,” Plunkett said.
But an ensuing mystery concerns those black holes in the 40-and-above regime, which coincides with the aforementioned “death zones” for black hole masses. According to stellar evolution theory, black holes born of supernovas shouldn’t leave any black holes above roughly 45 solar masses, explained Plunkett. “Yet we have seen black holes that are that massive,” she mused. “And the question is: Where did they come from?” For now, it’s hard to say when we’ll get an answer to that question, if ever. But one thing seems to be clear: black holes are a lot weirder than we could ever imagine. #Scientists #Black #Holes #Born #Black #HolesBlack holes,Gravitational wave,LIGO Scientists Say Some Black Holes Are Born From Other Black Holes
Since LIGO’s Nobel-winning discovery of gravitational waves—ripples in spacetime—the U.S.-based detector has been picking up on hundreds of signals from black hole mergers. And, after a decade of studying gravitational waves, researchers believe a significant fraction of black holes may come from cosmic chain reactions. A recent paper published in Physical Review Letters describes an analysis of 155 pairs of binary black holes, identified by LIGO and its sisters, Virgo and KAGRA, in Italy and Japan, respectively. According to the study, about 14% of merging black holes may be what’s called “second-generation black holes,” or black holes that form from previous mergers of two smaller black holes. This “hierarchical” backstory is vastly different from the textbook version of how black holes emerge from the explosive death of a star. “Overall in the universe, black holes are merging all the time,” Cailin Plunkett, the study’s first author and a graduate student at the Massachusetts Institute of Technology, told MIT News. “Now we’re seeing a relatively consistent picture where there’s a decent percentage of black holes that are coming from this repeated pathway.”
Tracking the invisible Gravitational waves that reach Earth’s detectors typically come from extremely intense events. Over the years, LIGO has picked up some truly perplexing signals. For example, last summer it found the most colossal black hole merger ever—and if that wasn’t wild enough, the black holes that took part in the merger lie within a cosmic “dead zone” for black holes.
This zone refers to a range of black hole masses in which, physically speaking, black holes can’t form through ordinary stellar collapse. From these discoveries, astronomers realized just how little we knew about black holes, which are challenging to investigate directly. In that sense, it was a no-brainer that the ever-growing catalog of LIGO’s gravitational signals would turn up entirely new insights about black holes. “It is increasingly clear, both from individual events and population analyses, that massive black holes exist in [this] range,” the researchers wrote in the latest paper. “These observations have spurred further investigation into mechanisms that can populate this gap.”
A wobbly imprint The latest research represents one such investigation. During mergers, the two black holes spiral toward each other along an orbital plane. When one or both black hole spins are misaligned, the orbital plane can wobble, or “precess,” the researchers explained to MIT News. The degree to which the disk wobbles acts as a parameter from which researchers can measure the masses and spins of the merging black holes. One telling sign of hierarchical mergers is that they’re “lopsided,” meaning one of the pair has a much higher spin and mass than the other. For the study, the team created an analytic model to capture the kind of wobble that would have emerged from second-generation black holes. Around 14% of merging black holes followed this pattern, and the second-generation black holes identified had a very specific range of masses, at around 20 solar masses or 40 solar masses and above. Of mysterious origins To be fair, that might not sound like a whole lot. But it demonstrates that a sizeable portion of known black holes indeed follow this pattern. As for why, the team suspects hierarchical mergers emerge from dense stellar environments. Simply, when multiple neighboring stars die and collapse into black holes, the dense environment can make it easier for those black holes to find each other and merge. That could further lead to the formation of second-generation black holes. Theoretically, this could “repeat potentially ad infinitum, by virtue of the fact that you have a ton of stars and black holes in this really dense environment,” Plunkett said.
But an ensuing mystery concerns those black holes in the 40-and-above regime, which coincides with the aforementioned “death zones” for black hole masses. According to stellar evolution theory, black holes born of supernovas shouldn’t leave any black holes above roughly 45 solar masses, explained Plunkett. “Yet we have seen black holes that are that massive,” she mused. “And the question is: Where did they come from?” For now, it’s hard to say when we’ll get an answer to that question, if ever. But one thing seems to be clear: black holes are a lot weirder than we could ever imagine. #Scientists #Black #Holes #Born #Black #HolesBlack holes,Gravitational wave,LIGO](https://gizmodo.com/app/uploads/2026/07/black-hole-hierarchial-mergers-1280x853.jpg)
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