Recommended Posts

There's a LOT of construction coming up; the legs and fins on both Starships, the Coco FL Starship being transported to KSC, the Cocoa FL Super Heavy booster build starting (19+ ring segments are already fabbed), LC-39A modifications, etc. 

 

Busy-Busy....

  • Like 1

That's pretty awesome, it looks like it made the hop between the two pads fairly effortlessly.

 

So next is the Space X presentation which was expected to happen Mid Sept? Hopefully a Star ship prototype will be ready soon after to do hopper tests also?

7 hours ago, Skiver said:

That's pretty awesome, it looks like it made the hop between the two pads fairly effortlessly.

 

So next is the Space X presentation which was expected to happen Mid Sept? Hopefully a Star ship prototype will be ready soon after to do hopper tests also?

 

Musk will likely want to show off  an assembled Mk1 vehicle during the presentation. 

 

Starship Mk1 at Boca Chica should be getting her fins etc. soon since some airfoils were trucked in a few days ago, and pics of workers preparing the modules for them are now public.

Yeah ... diminishing returns on engine output vs fuel consumption, no matter how good Raptor becomes, will limit how heavy it can be (therefore how tall it will be). It will gain some height, though -- just not a linear scale upwards. I still think 18 meters is too wide. There's no possible way it can pack 70-100 engines ... it would destroy itself from any number of acoustic energies and other effects simply igniting all of those engines not to mention being inefficient (diminishing returns again) and way too complicated to engineer (let alone build).

 

It'd call for an upscaled Raptor design ... and I'm not certain that SpaceX is ready for that yet. They wanna get Raptor fully ironed out and flying, then evolve it over a service life of 5~10 years (or more) like they've done with the Merlin series. If they were to go that route (upscaled Raptor) they'd HAVE to get started on it NOW.

 

Now -- could Raptor see iterative gains like Merlin, where it sees double the efficiency and nearly 3x the thrust output (or more)? Sure, as long as the SpaceX boffins put in that R&D and don't cut corners. It won't just be the engine itself but the platform that'll contribute to that endeavour. The current gen of Falcon-9 is so much more than the 1.0 version that really it's only the outer shell that's anything like the first iteration (and that isn't even completely the same nowadays, what with that composite upperstage at the top 1/5th of the booster).

 

The next 20 years are going to be very interesting, development-wise and evolutionary-wise, for Starship and Super Heavy. Not sure how feasible 18m is actually gonna be though ... 

Create an account or sign in to comment

You need to be a member in order to leave a comment

Create an account

Sign up for a new account in our community. It's easy!

Register a new account

Sign in

Already have an account? Sign in here.

Sign In Now
  • Posts

    • It's amazing that anyone still uses this bloated trash.
    • @Sayan...I have defended you at various points as I hope you know. This headline however is utter trash...shame on you sir!
    • An actual cosmic "Eye of Sauron" had been looking straight at us all along by Sayan Sen Image by Kovin P. Vasquez via Pexels | Not representative An international team of researchers has solved a long-standing mystery surrounding a distant blazar known as PKS 1424+240, helping explain why it produces some of the brightest high-energy gamma rays and cosmic neutrinos ever observed despite appearing to have a relatively slow-moving jet. The findings were published on June 6 in Astronomy & Astrophysics Letters. The study addresses a broader challenge in astrophysics: understanding how extreme cosmic objects accelerate particles to very high energies and produce very high-energy (VHE) photons and neutrinos. PKS 1424+240 is located billions of light-years from Earth. It has attracted attention for years because it is both a powerful source of VHE gamma rays and the brightest known neutrino-emitting blazar in the sky, according to observations by the IceCube Neutrino Observatory. It is also associated with one of the strongest peaks in IceCube's nine-year neutrino sky map A blazar is a type of active galactic nucleus powered by a supermassive black hole that pulls in surrounding matter and launches jets of plasma moving close to the speed of light. What makes blazars unique is their orientation. One of their jets points almost directly toward Earth, making them appear exceptionally bright across the electromagnetic spectrum and allowing scientists to study some of the most extreme physical processes in the Universe. The scientists exclaimed it's like the 'Eye of Sauron' in deep space. Usually, the brightest gamma-ray-emitting blazars are expected to have jets that appear to move very quickly. However, radio observations of PKS 1424+240 suggested that its jet was moving much more slowly, creating a contradiction that became part of a long-running problem known as the "Doppler factor crisis." To investigate, researchers analyzed 15 years of observations from the Very Long Baseline Array (VLBA), a network of 10 radio antennas spread across the continental United States, Hawaii and St. Croix. Using a technique called Very Long Baseline Interferometry (VLBI), astronomers combine signals from widely separated radio telescopes to create a virtual Earth-sized telescope capable of revealing extremely fine details. The team combined 42 polarization-sensitive radio images collected between 2009 and 2025, creating a much deeper and more detailed view of the jet than had previously been possible. The observations were carried out as part of MOJAVE (Monitoring Of Jets in Active galactic nuclei with VLBA Experiments), a long-running program that studies the brightness, polarization and magnetic field structures of jets produced by active galaxies. The project aims to better understand how activity near supermassive black holes is linked to high-energy radiation and neutrino emission. “When we reconstructed the image, it looked absolutely stunning,” said Yuri Kovalev, lead author of the study and Principal Investigator of the European Research Council-funded MuSES project at the Max Planck Institute for Radio Astronomy. “We have never seen anything quite like it — a near-perfect toroidal magnetic field with a jet, pointing straight at us.” The image revealed an unusual geometry. The researchers found that Earth lies almost directly in line with the jet, with a viewing angle of less than 0.6 degrees. In simple terms, astronomers are looking almost straight down the jet. This turned out to be the key to the mystery. Because the jet is aimed almost directly at Earth, a relativistic effect called Doppler boosting dramatically increases its apparent brightness. The study found that this effect boosts the emission by a factor of about 30 while also making the jet appear slower than it actually is. “This alignment causes a boost in brightness by a factor of 30 or more,” said Jack Livingston, a co-author at the Max Planck Institute for Radio Astronomy. “At the same time, the jet appears to move slowly due to projection effects — a classic optical illusion.” The nearly head-on view also gave scientists a rare look at the jet's magnetic field. Using polarized radio signals, they detected a clear toroidal, or doughnut-shaped, magnetic field component. The observations suggest the jet carries an electric current and that its magnetic field helps launch, shape and stabilize the flow of plasma. Researchers believe this magnetic structure may also play a key role in accelerating particles to energies high enough to produce both gamma rays and neutrinos. “Solving this puzzle confirms that active galactic nuclei with supermassive black holes are not only powerful accelerators of electrons, but also of protons — the origin of the observed high-energy neutrinos,” Kovalev said. The research was conducted under the MuSES (Multi-messenger Studies of Energetic Sources) project, which investigates how active galactic nuclei accelerate particles and generate different cosmic signals, including light and neutrinos. Scientists say understanding how protons are accelerated and linked to neutrino production remains one of the major unanswered questions in astrophysics. The findings help explain why some blazars can appear to have slow jets while still producing extremely bright high-energy emissions. More broadly, the study strengthens the link between relativistic jets, magnetic fields, gamma rays and high-energy neutrinos. Researchers say the results provide new clues about how some of the Universe's most powerful natural particle accelerators work and offer important insights for multimessenger astronomy, which combines different types of cosmic signals to study extreme events in space. Source: European Research Council, EDP Sciences This article was generated with some help from AI and reviewed by an editor. Under Section 107 of the Copyright Act 1976, this material is used for the purpose of news reporting. Fair use is a use permitted by copyright statute that might otherwise be infringing.
    • Gotenks98 is right... Outlook (new) is absolute trash. Doesn't Mozilla have an Enterprise Version of Firebird?
  • Recent Achievements

    • One Month Later
      lamborghiniv10 earned a badge
      One Month Later
    • Week One Done
      lamborghiniv10 earned a badge
      Week One Done
    • Reacting Well
      X-No-file earned a badge
      Reacting Well
    • One Month Later
      pestcontrol46 earned a badge
      One Month Later
    • Week One Done
      pestcontrol46 earned a badge
      Week One Done
  • Popular Contributors

    1. 1
      +primortal
      510
    2. 2
      PsYcHoKiLLa
      273
    3. 3
      Skyfrog
      75
    4. 4
      +Edouard
      72
    5. 5
      FloatingFatMan
      68
  • Tell a friend

    Love Neowin? Tell a friend!