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Please visit breakerwhiskey.com for more information or to send a message to Whiskey's radio. Breaker Whiskey is an Atypical Artists production created by Lauren Shippen. If you'd like to support the show, please visit atypicalartists.co/support. If you'd like to send Whiskey a message, click here. -- [TRANSCRIPT] Another message from another person out there in the black. You said: I thought it was so sad that you only saw one dog on you journey. What good is a world without dogs? Then last weekend I was shocked and heartbroken by being attacked by a large dog that the owner had said was friendly and loved everyone (owner is shocked and heartbroken,  too). So now I'm on a journey to heal, trust, and learn more about that which I thought I loved...just like Whiskey. It'll be a somewhat lonely journey, like hers, and filled with ALL of the emotions. I'm hoping it ends with belly rubs, chewed furniture legs, piddle accidents, full vacuum tanks, five am wake-ups,  and an unshakable bond. Wish me luck.

Watch this entire presentation Subscribe to Rosanne’s Channel and receive notice of each new video!   Transcript: Another answer for why we don’t credit writers is that we never really credited them equally. In the very early days of Hollywood, you can see on the bottom of this poster, it says it was written and … Continue reading "14 Charlie Brackett from Why Researching Screenwriters (has Always) Mattered [Video] (54 seconds)" Related posts: 10 Oscar Micheaux from Why Researching Screenwriters (has Always) Mattered [Video] (43 seconds) 12 Who Wrote What? from Why Researching Screenwriters (has Always) Mattered [Video] (1 minute 9 seconds) 09 Susan Y. Mason from Why Researching Screenwriters (has Always) Mattered [Video] (47 seconds)

Indoctrination was purposefully built into our current systems of education, propping up unjustifiable institutions of authority by engineering consent. But some young minds resist domestication. And some of those minds call themselves hackers.   Transcript: Another one got caught today, it’s all over the papers.  “Teenager Arrested in Computer Crime Scandal”, “Hacker Arrested after Bank…

Transcript: Another way to look at the mass density of the universe is in terms of the cosmic mass to light ratio. Mass to light ratio is defined as the ratio of the mass, in solar units, to the luminosity, in solar units, so for the Sun by definition M over L is one. In general, low mass stars have mass to light ratios greater than one, and high mass stars have ratios less than one. We know that the stellar populations typical of normal galaxies give overall mass to light ratios in the range of three to ten. This means that anywhere in the universe on larger scales where we infer mass to light ratios much above ten we must be looking at dark matter. The halos in galaxies through dynamical measurements have mass to light ratios in the range ten to fifty, groups of galaxies in the range thirty to two hundred, clusters of galaxies in the range one hundred to four hundred, and the Local Supercluster, through a very uncertain measurement, has a mass to light ratio in the range three hundred to five hundred. On all these large scales most of the mass is coming from dark matter. However, the mass to light ratio in the standard cosmology corresponding to critical mass density is one thousand five hundred. So even on the largest scales there’s not sufficient dark matter to account for a critical density; it’s a factor of three short.

Transcript: Another fundamental quantity of the big bang model is the density parameter. It’s defined as the ratio of the mean density of the universe to the density just needed to overcome the cosmic expansion. The density parameter is denoted by the Greek symbol capital omega with a subscript zero. If omega equals one the universe is flat. If omega is less than one the universe is open, and if omega is greater than one the universe is closed. Unlike the deceleration the density parameter is a purely local measurement. All that’s required is to take a large volume of space, typically fifty to a hundred megaparsecs in distance from the Milky Way, add up all the matter that’s contained, luminous and dark, divide by the volume, and compare to the critical density. The answer gives the sense of whether the universe will expand forever. The best current measurements indicate that omega is about 0.3 or only one-third of the amount of density needed to overcome the expansion. Based on these measurements the universe will expand forever.

Transcript: Another idea to explain the existence of spiral arms is called the stochastic star formation theory. In this theory the star formation in one region triggers star formation in neighboring regions of the disk like a chain reaction. For up to a hundred million years a star formation region is lit up by young stars, and during this time differential rotation, the inner part of the region moving faster than the outer part, shears the star formation region into the segment of a spiral. Overall a spiral pattern is seen, but the pattern is transient because different stars are coming and going and being born and dying over the long period of time of the lifetime of the Milky Way galaxy.

Transcript: Another reason that science cannot make statements with absolute certainty is to do with sampling or the limitations of data. Induction as a tool of the scientific method is based on generalizing from a finite set of observations or situations to a broader conclusion. If I had ten people in front of me and I asked which hand each of them wrote with and all ten said that their right hand, would I be justified in concluding that all people are right-handed? You know that the answer is no. The incidence of left-handedness in the population is about 10%, so with ten people questioned I might just be unlucky and find none that are left-handed. However with a hundred people, if I question them, I would expect ten of them to be left-handed, and the odds of finding no left-handers would be very small. Thus our ability to draw a conclusion on the incidence of left-handedness depends sensitively on the number of people asked or sampled. Astronomy has exactly the same situation. If I inspected the nearest ten stars to the sun and found them to be all of a certain type, would I be justified in concluding that that was the only type of star that existed? No, I would probably need to sample space more fully and contain larger samples of stars to make a statistical statement with any certainty. Astronomy depends on the issues of sampling as many other fields do. For instance in politics the voting intensions of tens of millions of adult Americans are based on samples of only a few thousand people. So these techniques can be used with reliability.

Transcript -- Another mosaic from Tunisia which shows the integration of local cultural references into the pattern

Transcript -- Another mosaic from Tunisia which shows the integration of local cultural references into the pattern