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Rooting for Ronda tomorrow night!!

But realistically whoever wins will be good for Women's MMA, even got Dana looking interested in this fight

If Rousey fights smarts and doesn't try to brawl with Sarah Kaufman, she'll take it easily. It was quite funny to see Cybord trying to bait Ronda into fighting her at 145. Like anyone would take that challenge, especially now, after (s)he's ****ed hot.

Main Card:

Ronda Rousey (135) vs. Sarah Kaufman (134)

Ronaldo Souza (186) vs. Derek Brunson (186)

Roger Bowling (170) vs. Tarec Saffiedine (169.5)

T.J. Cook (203) vs. Ovince St. Preux (205.5)

Lumumba Sayers (185) vs. Anthony Smith (186)

Preliminary Card:

Miesha Tate (136) vs. Julie Kedzie ( 135)

Bobby Green (155) vs. Matt Ricehouse (155)

Adlan Amagov (186) vs. Keith Berry (186)

Germaine de Randamie (144) vs. Hiroko Yamanaka (145)

Every lady made weight. But for my WMMA fix, I always turn to Invicta FC because the talent pool is (just a bit) deeper. The winner of Miesha Tate vs. Julie Kedzie fights the winner of Ronda Rousey vs. Sarah Kaufman. Rematches for everyone.

Rousey Tate 2

Tate didn't look that good at first, I really think she got lucky with that armbar, Rousey will whoop her a second time

I like what Ronda did, called Cyborg out and make her drop to 135, even tho I don't think she could do it

Rousey Tate 2

Tate didn't look that good at first, I really think she got lucky with that armbar, Rousey will whoop her a second time

I like what Ronda did, called Cyborg out and make her drop to 135, even tho I don't think she could do it

The only way Cyborg could drop to 135 was if she cut off her leg. Seeing how the division is as deep as a puddle in the sun, Rousey vs Tate 2 is the only fight available unless Carano gets her fat ass back in the cage. Sarah Kaufman was always weak to submissions and had absolutely nothing to stop Rousey from ripping her arm.

Edgar has confirmed his drop to Featherweight and wants to fight before the end of the year. So I think they should book... Frankie Edgar vs Chad Mendes. Seems to me like the best fight available and a great setup for a Top Contender Match or next in line.

  • 2 weeks later...

Two Days Late for Andrei Arlovski, ONE FC Adopts Full PRIDE Rules for Soccer Kicks

PRIDE NEVER DIE!

ONE FC is on the fast track to becoming a top tier promotion. Will Super Fight League follow suite?

Matt Mitrione Offers Himself As Jon Jones' Heavyweight Debut, Thinks He Can Beat Him

Sure, a guy that was outgrappled by Cheick Kongo in his last fight is going to ragdoll Jon Jones.

It could happen. I don't doubt the potential Mitrione holds but its delusional to think he was ragdolled omg it was all stand up and it sucked.

Dana White Says Lyoto Machida Is Fighting Dan Henderson Next

http://www.bloodyelbow.com/2012/9/14/3333942/ufc-lyoto-machida-vs-dan-henderson-dana-white-mma-news

Why? Why? Why? Why? Why?

Why not have Machida fight Alexander Gustafsson? Why does Dan have to prove his worth yet again? He isn't getting any younger. Sure, Machida should lose his spot because he turned down the fight, but why does Dan have to lose his? Who's going to fight Jones after he crumples the fat version of Vitor Belfort? Goddamn it, the LHW division is a ****ing mess again.

Saw that trailer a few weeks back, im not Kevin James biggest fan, but Bas Rutten being in this makes it a must see!

Also, the "old" guy there... it's Fonzie. Aaay! Sure hope it isn't a bait and switch and every Rutten scene is in the trailer.

What a combination, the Fonz and Bas Rutten.. If only this was incorporated into the film..

http://www.youtube.com/watch?v=P8mBe0_Ha78

People laugh about it because of the tone of the videos. But they somehow forget that if they fought Bas Rutten in the street fight, they wouldn't live to tell the tale. Ever heard the (I think it's swedish) bar fight story he told on the Joe Rogan podcast?

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    • This could exactly be how our Sun ends but it's not as simple by Sayan Sen Image by Drew Rae via Pexels An international team led by Université de Montréal (University of Montreal) PhD student Érika Le Bourdais has found that the ancient white dwarf star LSPM J0207+3331 is still pulling in planetary debris, even though it has been cooling for about three billion years. White dwarfs are dense, Earth-sized stellar remnants left behind when Sun-like stars exhaust their nuclear fuel and shed their outer layers. The star, located 145 light-years away in the constellation Triangulum, is the oldest and coldest white dwarf known to have a surrounding disk of dust. The star was first spotted in 2019 by a citizen scientist through the Backyard Worlds: Planet 9 project. Its cool temperature immediately suggested that it was very old, since white dwarfs gradually lose heat over time. Using the W. M. Keck telescopes in Hawaii, astronomers later confirmed that the star shows infrared signals consistent with dust rings formed by asteroids breaking apart under its strong gravity. Such infrared excesses occur when a star emits more infrared light than expected, often because warm dust surrounding it absorbs and re-radiates energy. “This discovery challenges our understanding of planetary system evolution,” said Le Bourdais. “The fact that we still see planetary debris being accreted three billion years after the star became a white dwarf suggests that asteroids, comets, and even planets can remain in orbit around these stars for a very long time.” Spectroscopic analysis—a technique that studies light to identify the chemical elements present in an object—revealed thirteen heavy elements in the star’s atmosphere: sodium, magnesium, aluminium, silicon, calcium, titanium, chromium, manganese, iron, cobalt, nickel, copper, and strontium. Normally, heavy elements sink quickly in hydrogen-rich white dwarfs, making them hard to detect. “We expected to see only a few elements, but we found dozens!” explained Le Bourdais. The research paper adds more detail. The absence of carbon features suggests the debris came from a carbon-volatile-depleted source. The abundance pattern shows slight deficits of magnesium and silicon compared to iron but otherwise resembles Earth-like material. This points to a differentiated rocky body—one whose materials have separated into distinct layers such as a metallic core and rocky mantle—with a metallic core fraction higher than Earth’s. In other words, the star is accreting the remains of a large rocky object, similar in structure to Earth or the asteroid Vesta. “White dwarfs offer one of the only ways we can directly measure the composition of exoplanets,” said Patrick Dufour, co-author and professor at Université de Montréal. “When planetary debris come too close, they are torn apart by the star’s gravity and end up polluting its atmosphere, leaving a detailed chemical fingerprint of its composition.” The team also detected weak Ca II H & K line core emission, making this only the second known isolated polluted white dwarf to show this feature. These are specific spectral signatures produced by ionised calcium and can indicate unusual physical activity in a star’s upper atmosphere. The finding suggests that extra physical processes may be happening in or above the star’s upper atmosphere. The study stresses the importance of including heavy elements in model atmosphere calculations, since leaving them out can distort the inferred structure and lead to inaccurate stellar parameters. Earlier work suggested the star’s infrared excess came from two dust rings. The new analysis shows that a single silicate dust disk—a ring composed largely of rock-forming minerals rich in silicon and oxygen—can explain the observed signal at 11.6 μm, simplifying the picture of the system’s structure. The question of how debris ended up falling into the star so late remains open. One idea is that giant planets in the system slowly destabilised smaller bodies over billions of years. Another possibility is that a passing star disturbed the orbits of debris. “Future observations with the James Webb Space Telescope or archival data found in the European Space Agency’s Gaia mission could help distinguish between a planetary rearrangement and the gravitational effect of a close stellar encounter,” said John Debes, co-author and researcher at the Space Telescope Science Institute. Dufour noted that hydrogen-rich white dwarfs are the most common type, and the coolest among them are the oldest stars in the galaxy. “We didn't have the habit of looking for signs of accretion in them. This unique case motivates us to expand our search to more of these stars.” The findings show that even after billions of years, planetary systems can remain active and complex. Substantial accretion events—the gradual accumulation of surrounding material onto a celestial object—can still occur long after a star’s death, offering a rare window into the composition and fate of distant worlds. Source: University of Montreal, IOPScience 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.
    • Doesn't DDG mainly use Bing?
    • Given the hefty price tag this thing will likely have I doubt many everyday home users will be in the market for one especially given the current climate.
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    • +1 for Rufus. I bought NTLite a few years ago to scrape all the bloat out of Windows 11. It is not a perfect solution as there is a steep learning curve if you don't really know what you are doing (me included). I have finally got a Windows install that just works. I only keep things I use and nothing else.
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