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TUF 16 Finale: Roy Nelson vs. Matt Mitrione will headline

Meathead is getting back in the cage. Nelson will certainly put a beating on him or just submit him in the 1st.

I'm going to go out on a limb and say meathead will be the first to put Nelson down in the ufc.

I'm going to go out on a limb and say meathead will be the first to put Nelson down in the ufc.

He stood toe to toe with Junior dos Santos for 3 rounds. I don't think Mitrione has the power or skill to outclass JDS on the feet and KO Roy.

He stood toe to toe with Junior dos Santos for 3 rounds. I don't think Mitrione has the power or skill to outclass JDS on the feet and KO Roy.

I'm running on the notion that the accumulative affect of receiving so many headshots in ones career eventually leads to getting KO'd. Its a gamble with Matt but one day Nelson will no longer sustain those shots.

  • 2 weeks later...

UFC 157 is going to be headlined by Rousey vs Carmouche. The first WMMA fight in the UFC headlines a PPV. That's massive. The choice of opponent is pretty weak, nobody knew who Carmouche was when she fought Marloes Coenen and that situation still stands. They really should've brought in Marloes Coenen to fight Rousey. Other reasonable choices would be Alexis Davis, Shayna Baszler, Sarah McMann, Cat Zingano or Amanda Nunes, but they all suffer from the same problem as Carmouche: almost nobody has ever heard of them. Coenen's name still holds some value. Still, this is only a practice fight for Rousey vs Cyborg on a brazilian PPV card.

^^ Carmouche got the fight because she was the only one actively pushing for it in Social Media, and got what she asked for, the rest of the ladies just stood by while Carmouche talked her way into a historical fight for the UFC, but yrs she's s till a few fights from being a title contender, but she does have potential down the road

Contrasting with an absolutely terrible season, the TUF 16 Finale was AWESOME. Great fights, tons of finishes and free. What's not to like?

The UFC on FX 6 card (the TUF Australia vs UK finals), not so much. The TUF guys sucked badly, Pearson did his thing and Lombard got a gift win because Paul Harris was too dumb to take him down and fought a flat footed stand up battle. Put Lombard against Mu?oz and watch him squirm.

  • 2 weeks later...
  • 2 weeks later...
MMA fighter & TNA Wrestling star King Mo was victorious in his first Bellator MMA fight on Thursday night on Spike TV, which aired after Impact. In the quarter finals of the Bellator Light Heavyweight tournament, Mo defeated Przemyslaw Mysiala via knockout in 3:52 of the first round.

Mo looked rusty early on after being out of the cage for a full year, but found his rhythm and delivered a one-punch knockout Mysiala to advance in the tournament.

During the post-fight interview, Mo said he didn't have much of a strategy going in and he just wanted to knock the guy out.

Mo will fight Emmanuel Newton next in the semi-finals on February 21st from Salt Lake City, Utah.

Rampage sounds like he's kinda done

He was already done a while ago. But this fight sealed the deal. He looked like crap and he completely checked out in the 3rd round. Still, Bellator will probably send an offer his way to fight King Mo after he steamrolls the LHW tournament.

Pettis looked like a straight up beast. UFC 156 is coming up this weekend. I'll get the info ready.

  • 4 weeks later...

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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?
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