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Ted Mason (fell runner)

From Wikipedia, the free encyclopedia

Edward Thomas "Ted" Mason (born 30 January 1979) is a Yorkshire-born farmer best known for his accomplishments as a fell runner.

He grew up in Appletreewick near Grassington. He went to Burnsall V.A. Primary School, then Upper Wharfedale School in Threshfield. Upon leaving school he pursued a career as a farmer, gaining a Higher National Diploma in agriculture from Newton Rigg College, part of Askham Bryan College.

Mason is a member of the Wharfedale Harriers, the British Open Fell Runners Association (BOFRA) and the Fell Runners Association (FRA).

His fell running career began when he was ten years old, finishing last in a local race, and his first race win was at the age of nineteen at Beamsley Beacon.[1] Ted's first championship race win was in 1999 at the BOFRA Hawkswick Dash. Turning at the summit, he was lying in fifth, but he quickly gained places on the descent going on to win in 11 minutes 38 seconds, 31 seconds ahead of second place.[2]

Ted is most noted for his speed in descending, being cited by Alistair Dunn (BOFRA Champion 2006–11) as "an inspiration from the start of my fell running career. I still don't know anyone who can descend faster".[3]

Ted was crowned BOFRA Champion in 2002 and 2003, and came close to regaining the title in 2011. It was taken to the last race at Wasdale Show. Mason was leading the championship going into the race, but a result of fourth meant a finish of second overall in the series. In 2012, he was again victorious in the championship,[4] also winning in 2014[5] and 2015.[6]

In 2011, Mason achieved a number of ambitions. On 20 August he won the race most local to him, the Burnsall Classic for the first time. This fell race is one of the oldest fell races, dating beyond 1870, with the first report of it appearing in the Craven Herald in 1888.[7] Ted took a different route down the fell, going on to win by a twelve-second margin.[8] Ten days later he would go on to win the crag race at Kilnsey Show also for the first time. It was his fifteenth attempt.

Mason has made a couple of television appearances, appearing on the title screens for Look North News and more recently on The Dales hosted by Ade Edmondson on ITV, where Ted was documented training for the Burnsall Classic.

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Transcription

What would happen to you if a black hole the size of a coin suddenly appeared near you? Short answer: you’d die. Long answer: it depends. Is it a black hole with the mass of a coin, or is it as wide as a coin? Suppose a US nickel with the mass of about 5 grams magically collapsed into a black hole. This black hole would have a radius of about 10 to the power of −30 meters. By comparison, a hydrogen atom is about 10 to the power of −11 meters. So the black hole compared to an atom is as small as an atom compared to the Sun. Unimaginably small! And a small black hole would also have an unimaginably short lifetime to decay by Hawking radiation. It would radiate away what little mass it has in 10 to the power of −23 seconds. Its 5 grams of mass will be converted to 450 terajoules of energy, which will lead to an explosion roughly 3 times bigger than the atomic bombs dropped on Hiroshima and Nagasaki combined. In this case, you die. You also lose the coin. If the black hole had the diameter of a common coin, then it would be considerably more massive. In fact, a black hole with the diameter of a nickel would be slightly more massive than the Earth. It would have a surface gravity a billion billion times greater than our planet currently does. Its tidal forces on you would be so strong that they’d rip your individual cells apart. The black hole would consume you before you even realized what’s happening. Although the laws of gravity are still the same, the phenomenon of gravity that you’d experience would be very different around such dense objects. The range of the gravitational attraction extends over the entire observable universe, with gravity getting weaker the farther away you are from something. On Earth right now, your head and your toes are approximately the same distance from the center of our planet. But if you stood on a nickel-sized black hole, your feet would be hundreds of times closer to the center, and the gravitational force would be tens of thousands of times as large as the force on your head and rip you into a billion pieces. But the black hole wouldn’t stop with just you. The black hole is now a dominant gravitational piece of the Earth–Moon–Black-Hole-of-Death system. You might think that the black hole would sink towards the center of the planet and consume it from the inside out. In fact, the Earth also moves up onto the black hole and begins to bob around, as if it were orbiting the black hole, all while having swathes of mass eaten with each pass, which is much more creepy. As the Earth is eaten up from the inside, it collapses into a scattered disk of hot rock, surrounding the black hole in a tight orbit. The black hole slowly doubles its mass by the time it’s done feeding. The Moon’s orbit is now highly elliptical. The effects on the Solar system are awesome— in the Biblical sense of awesome, which means terrifying. Tidal forces from the black hole would probably disrupt the near-Earth asteroids, maybe even parts of the asteroid belt, sending rocks careening through the Solar system. Bombardment and impacts may become commonplace for the next few million years. The planets are slightly perturbed, but stay approximately in the same orbit. The black hole we used to call Earth will now continue on orbiting the Sun in the Earth’s place. In this case, you also die. This bonus video was made possible by your contributions on Patreon. Thank you so much for your support! The topic is based on a question on the AskScience subreddit and the glorious answer by Matt [Caplin?], who also worked with us on this video. Check out his blog, Quarks and Coffee, for more awesome stuff like this! If you want to discuss the video, we have our own subreddit now. To learn more about black holes or equally interesting neutron stars, click here. Subtitles by the Amara.org community

Notes

  1. ^ "Archived copy". Archived from the original on 10 April 2020. Retrieved 29 January 2012.{{cite web}}: CS1 maint: archived copy as title (link)
  2. ^ "The Official BOFRA Website". Archived from the original on 20 July 2012. Retrieved 29 January 2012.
  3. ^ "Archived copy". Archived from the original on 22 December 2015. Retrieved 29 January 2012.{{cite web}}: CS1 maint: archived copy as title (link)
  4. ^ "BOFRA Championship Positions 2012" (PDF). Archived from the original (PDF) on 17 August 2013. Retrieved 18 December 2015.
  5. ^ "BOFRA Championship Positions 2014" (PDF). Archived from the original (PDF) on 5 March 2016. Retrieved 18 December 2015.
  6. ^ "BOFRA Championship Positions 2015" (PDF). Archived from the original (PDF) on 22 December 2015. Retrieved 18 December 2015.
  7. ^ "Home". burnsallsports.co.uk.
  8. ^ Mud, Sweat and Tears: "Ted's secret is revealed!"
This page was last edited on 28 October 2023, at 18:25
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