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When astronauts return to the Moon in the next few years, the plan is to have them stay for good while establishing a permanent outpost on Earth nearest celestial neighbor. Like all space missions, a lunar outpost will require fuel for long-term sustainability, but would it be better to mine fuel on the Moon or get fuel resupply from the Earth? This is what a team of researchers led by Bocconi University in Italy hope to address as they assessed both the economic and technological feasibility of deriving fuel from either the Earth or the Moon.

Mattia Pianorsi, who is a Junior Researcher of the Space Economy Laboratory at the SDA Boccini School of Management and a PhD Candidate at the University of St. Gallen, recently told Universe Today the main objective of the study was to ascertain the economic and technical feasibility of mining fuel from the Moon’s water ice deposits or from the Earth. Both options would use an orbiting depot (OD) which Pianorsi says would be used “as a distribution channel for satellites as well as rockets in space.” The OD, which is separate from NASA’s proposed Lunar Gateway and is also not mentioned in the study, would possess a maximum fuel capacity of 25 tons and be located at the Earth-Moon Lagrange Point L1 which is approximately three-quarters the distance between the Earth and the Moon.

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Orbiting depot located at the Earth-Moon Lagrange Point L1. (Credit: Sommariva et al. (2023))

For the study, the researchers conducted a Monte Carlo analysis to evaluate the risks associated with both options. For their scenario, the researchers used hypothetical variables such as a lunar mining company, a transporter/distributor company, and end-users. The hypothetical lunar mining company charges fuel at $500 per kilogram while for the Earth refueling option a transporter purchases the fuel from the Earth at a negligible cost. Both options considered fixed costs, including Design, Development, Testing, and Evaluation (DDT&E), Manufacturing, and Transportation, while the recurring costs included Refueling and Operations.

The researchers determined the Earth refueling option would involve approximately 1.5 launches of a Falcon Heavy (FH) Expendable plus propellant tank with a spacecraft refueling payload of 17.5 tons. While the OD has a capacity of 25 tons, the FH would need to bring a combined total of 26.69 tons as the remaining 1.69 tons of fuel would be used to “transfer the refilling tank with its subsystems”, according to the study. As stated, the fuel costs are negligible, but the launch costs are estimated to be $150 million per launch, putting a total refueling price tag at $227.9 million, which includes launch plus fuel costs. The estimated launch costs also totaled $6511.4 per kilogram with a total operation cost of $42.38 million per year.

For the Moon refueling option, the researchers used a hypothetical Moon shuttle built by the Cislunar Space Development Company (CSDC) with a payload of 25 tons that launches from the Moon, docks and refuels the OD to its maximum capacity of 25 tons , then returns to the lunar surface, with the assumption that zero fuel is lost during the entire process. As stated, the hypothetical lunar mining company put the fuel costs at $500 per kilogram, and the study put the total refueling price tag at $37.51 million dollars, which includes launch plus fuel costs, giving a total operation cost of $35 million per year.

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Rendering of the Moon shuttle from the Cislunar Space Development Company. (Credit: Sommariva et al. (2023))

Based on these results, the researchers concluded that refueling the OD is more affordable
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Starship | First Integrated Flight Test | Recap

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Starship gave us quite a show during the first flight test of a fully integrated Starship (S24) and Super Heavy rocket (B7) from Starbase in Texas.

On April 20, 2023 at 8:33 a.m. CT, Starship successfully lifted off from the orbital launch pad for the first time. The vehicle cleared the pad and beach as Starship climbed to an apogee of ~39 km over the Gulf of Mexico – the highest of any Starship to-date.

With a test like this, success comes from what we learn, and we learned a tremendous amount about the vehicle and ground systems today that will help us improve on future flights of Starship.

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ARABSAT BADR-8 Mission Control Audio

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This is the vehicle trajectory and mission control audio without any additional commentary. There may be very long periods of silence. For our full hosted webcast, visit

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When Black Holes Merge, They’ll Ring Like a Bell

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When two black holes collide, they don’t smash into each other the way two stars might. A black hole is an intensely curved region of space that can be described by only its mass, rotation, and electric charge, so two black holes release violent gravitational ripples as merge into a single black hole. The new black hole continues to emit gravitational waves until it settles down into a simple rotating black hole. That settling down period is known as the ring down, and its pattern holds clues to some of the deepest mysteries of gravitational physics.

Gravitational wave observatories such as the Laser Interferometry Gravitational-Wave Observatory (LIGO) have mostly focused on the inspiral period of black hole mergers. This is the period where the two black holes orbit ever closer to each other, creating a rhythmic stream of strong gravitational waves. From this astronomers can determine the mass and rotation of the original black holes, as well as the mass and rotation of the merged black hole. The pattern of gravitational waves we observe is governed by Einstein’s general relativity equations, and by matching observation to theory we learn about black holes.

General relativity describes gravity extremely well. Of all the gravitational tests we’ve done, they all agree with general relativity. But Einstein’s theory doesn’t play well with the other extremely accurate physical theory, quantum mechanics. Because of this, physicists have proposed modifications to general relativity that are more compatible with quantum theory. Under these modified theories, there are subtle differences in the way merged black holes ring down, but observing those differences hasn’t been possible. But a couple of new studies show how we might be able to observe them in the next LIGO run.

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The modified Teukolsky equation. Credit: Li, Dongjun, et al

In the first work, the team focused on what is known as the Teukolsky Equation. First proposed by Saul Teukolsky, the equations are an efficient way of analyzing gravitational waves. The equations only apply to classical general relativity, so the team developed a way to modify the equations for modified general relativity models. Since the solutions to both the Teukolsky and modified Teukolsky equations don’t require a massive supercomputer to solve, the team can compare black hole ring downs in various gravitational models.

The second work looks at how this would be done with LIGO data. Rather than focusing on general differences, this work focuses on what is known as the no-hair theorem. General relativity predicts that no matter how two black holes merge, the final merged black hole must be described by only mass, rotation, and charge. It can’t have any “hair”, or remnant features of the collision. In some modified versions of general relativity, black holes can have certain features, which would violate the no-hair theorem. In this second work, the authors show how this could be used to test general relativity against certain modified theories.

LIGO has just begun its latest observation run, so it will be a while before there is enough data to test. But we may soon have a new observational test of Einstein’s old theory, and we might just prove it isn’t the final theory of gravity after all.

Reference: Li, Dongjun, et al. “Perturbations of spinning black holes beyond General Relativity: Modified Teukolsky equation.” Physical Review X 13.2 (2022): 021029.

Reference: Ma, Sizheng, Ling Sun, and Yanbei Chen. “Black hole spectroscopy by mode cleaning.” Physical Review Letters 130.2 (2023): 141401.

The post When Black Holes Merge, They’ll Ring Like a Bell appeared first on Universe Today.

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