[f1]Australian Grand Prix @ Albert Park


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what did that dog heidfeld do to my schumacher :cry: vengeance will be mine

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ha... don't u mean what did schu do to heidfeld

I said before the start of the race that Schu would get dirty if he couldn't get through the traffic.... suprise suprise!

yay and Fisico wins congrats to it (Y) hmm Barrichello arrives in second is very good :D, now Coulthard start amazing imo :o faster as one ray lol, can't wait to Kuala Lumpur and I hope rain a lot so Barrichello can win too :p

oh Schummy!! what's happen?? :(

judging by the replays i think that your sentence should be the other way around because Schumacher took himself out by being to agressive

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meh, it was 50/50. Heidfeld should have braked for the turn earlier (he locked up) and Schumacher shouldn't have cut him off. Either way Micheal came out on top, he now gets a fresh engine for Malaysian.

I thought it was a great race, though I will reserve judgement on the new rules. It was weird seeing no tire changes though I suppose it adds to the driver challange.

Good to see Fischella win but what is with this rule that if they dont "officially" finish the race, they can change engines without penalty? Isn't that a loophole on the rules which say that engines should last two races.

Lets wait for the next one and see what happens.

Here is a full schedule of races and tracks: BBC Sport

Also can a mod make this a sticky othervise we will be creating a new thread for each race? :rolleyes:

I hope the FIA does something bout people being pushed out of gravel traps.

Cant have one rule for one and one for another. Thats twice Schumi has been pushed out of the gravel, but there was a race last year cant rem who, but sum1 in same situation was made to retire n get out of car!

Lookin 4ward to the next race

I hope the FIA does something bout people being pushed out of gravel traps.

Cant have one rule for one and one for another. Thats twice Schumi has been pushed out of the gravel, but there was a race last year cant rem who, but sum1 in same situation was made to retire n get out of car!

Lookin 4ward to the next race

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Wasn't it Trulli or someone last year? Anyways, from what I understand they can only push the vehicle out if it poses an immediate danger to the driver or other drivers. But that really is to fuzzy.

Well Done Fisichella nice to see he held onto the first position. I fell asleep after the frist round of pits :s Dam late nice GP's

.. Well 14 days time thiere Kuala Lumpur. Cant Wait !

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as will happen here in Australia for all the remaining races.... and for Premier League soccer, and the Ashes.... no sleep for many nights this year then!

It was a good race. But unlike when watching it on TV it went really quickly. Yes, I was there. I was there with my friend, we had seats at the Capt. Arthur Waite stand. (Y)

Was really dissapointed when Schumacher got knocked out of the race, he could have got a podium finish. But it wasn't to be.

I really dislike Webber (I call him Bar-B-Que *snigger*) his attitude is just like the other australian sportsman I can't stand, Hewitt. (N)

Off to the indy in Queensland next year.

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    • 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.
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