What is going on ladies and gentlemen and welcome back to another? Bitcoin daily video today. We got three amazing things for you number one We're doing a recap from a Friday's trade setups that we gave you guys for free on Friday's video number two, we are doing a full market analysis on Bitcoin and Going over what we think might happen and what's been going on with Bitcoin and some of the other coins that we follow and number three We are giving you guys trade setups for this week. So if you missed last week's or this weekend's profits Don't worry. We got new ones for you So let's jump right in guys make sure to hit that like button Make sure to hit that subscribe button and make sure to hit that notification bell. Let's go All righty guys, so let's jump in I hope you guys are enjoying these super smooth Visuals here. I love you guys noticed But we have a new camera That's right. We've continued to make upgrades and we've continued to You know to improve our videos. So we're just working on doing that. All right, so What am I what am I looking at here? All right, here we go. So so First we're gonna go ahead and do a recap on The trades that we gave you guys these are the trade setups we gave you guys on Friday And these are there, you know the results So if you took these trade setups, this is the results You would have or you could have gotten depending where where you sold and where you entered, right? So there's just kind of a guesstimate of of what is or what could have been right? So the first one was Bitcoin. We told you guys entry point between 18.7 18.1 if you guys took that trade then that ran up all the way to 19.4,000 which would have been a 31.9 percent profit using 10x leverage now For all for all transparency reasons. We're giving you guys also there was a stop out We did stop out on this trade for a 5% was for a 0.5 percent With 10x leverage, that's 5% so we took a 5% loss on The initial entry then we re-entered it on the bounce and got made about a 32% profit on there The next trade was Ethereum The entry was that we gave you guys was 580 and it ran up to about 607 if we ran it to the top That would have been a 23% profit using 5x leverage now the same thing here on the initial entry We stopped out for about 8.5% loss, but then the winner made up for it and Overall we made money on that one Bitcoin cash was another entry. We gave you guys was that 280 support entry ran up to 293 It would have been a 23% profit if you entered that Litecoin We gave you guys at $80 support entry and it ran up to about $86 guys, so that was about 37 and a half percent profit XRP this was the biggest winner of them all it went down to about 54 55 cents and ran to about 62 That would have been a 63% profit if you use 5x Chainlink went down to about 1250 and ran up to about 1350 that would have been a 40% profit with 5x And then Tezzels and Neo as you guys can see did not hit our entries It didn't hit our support entries and it didn't hit our breakout entries either So we got no entries on those we got no results on those right?  So we got to record this a second time So we might make this one a little shorter a little faster just because we're a little tired, you know But as you guys can see here, we're looking at Bitcoin currently It's still following the same exact pattern as you guys can see it's still within this pattern here And and it's been respecting it. So from from what we can see there's just a bunch of Consolidation under the all-time highs, which is to be expected. This is a very normal thing With anything that goes up to test the all-time highs Prior to breaking it. There's usually a lot of consolidation, right? There's a lot of rejection a lot of consolidation So there's just a lot of sellers, but there's a lot of buyers as well. It's all part of the process So there's nothing to worry about guys. It's still a pennant and it's still a bullish, right? So it's a it's a flag and in a pennant And it's a bull flag. That's what it is. So we're we're still expecting this to break up You know because that's where the trend is going so we expect a full break out Eventually here Hopefully once it gets to this tip as you guys can see it has been consolidating in the consolidation range has got smaller and smaller So as long as it keeps tightening up We can expect it'll it'll confirm that it's following this this these supports and resistance line here and You know, hopefully we see that break up And so we can make some profits here. So what we're looking at for entries here We're looking at this 50-day moving average as you guys can see here. Oh It's right about it's currently right at that 19k range, right? So we're currently watching for new entries at 19,000 right now And we're gonna use about a $50 stop loss because the the this range right here is so small, right? so Because the range is so small. We're expecting the top of this range to be around 19,300 if it doesn't break out, right? so So we want to be able to take profits at 19 1 19 2 and 19 3 and then if it breaks out then we're probably gonna set up new breakout trades above 19 5 and And that'll be the next entries we have So the two entries that we're looking at right now for this week is here at the 50-day moving average as well as it's this ascending support, which is 19k and in above 1900 if it if these do not hold and it goes lower then we're looking at what the same levels We were watching this weekend, which was 1800 and down all the way down to 18 500 right so though That's a support area where you could buy if you see a bounce anywhere there going back up You could buy those entries and that's a support entry that you can use Whoo, that was a lot right? Let's go on to ethereum As you guys can see here ethereum has a basically a flat top pattern. That's what this is called So basically there's like a ascending support here and then there's just a flat top where it just keeps getting rejected Right, so that's exactly what we're looking at here. We see the ascending support We see the flat top or we've got rejected one two three times on three different tests If there is basically following Bitcoin to some degree, it's very Correlated so yeah, that's kind of what we're watching You can see that there's a moving average here in the same in these same areas So 590 is probably a place where you can take an entry using about a five dollar stop and then 600 is gonna be your first target 610 your second 620 your third Then the second breakout entry that we're looking for though Well, the breakout entry we're looking at is above 620s. That's you see that's the top of this flat top So we want a breakout above 620 so you can set orders right above 620 Or if you want to be safer you can set it above 625, but that's the that's the two entries We're watching If there is a dip for any reason and we break down below all these things Then we're looking at the same levels from the weekend, which was around 580 So we won't we want to see something like this where it drops and then we want to enter on the bounce We don't want to enter on the drop So that's pretty much it for Ethereum Bitcoin cash Bitcoin cash, I really don't like this This pattern here as you guys can see it's just kind of been weird, right? So I'm really and you can see here as well the moving averages have flipped So I would be looking for a break above the moving averages And I'd like to see these moving averages flip back So the entry would have to probably be above 295 and since 295 is so close to 300 you might as well Make that entry 300 right because of the psychological resistance there So my breakout entry the only entry that I'm currently looking at for Bitcoin cash is above $300 Light coin light coin kind of it's it's not as bad as Bitcoin cash You see here we have the impulse move up and consolidation. So it is a bull flag We need a breakout above these moving averages though So that's similar to Bitcoin flat of Bitcoin Bitcoin cash. Oh my goodness. I'm mixing up all these words So the good thing is Wait, there is no good thing. So the moving averages of flipped as well So we want to we want to see a breakout above the moving averages and up and we want to see these moving averages break And we probably want to see a break above this this right here. So that's $87. So we need something above 87 For a breakout here, right? So above 87 is a breakout entry We're not looking at to enter at any supports as of right now this moment We're not looking at any supports So eight above 87 is the only entry that we're looking at right as of today this moment for like XRP as you guys can see kind of a similar very similar to Bitcoin and Ethereum and like coin There is a big move up and then just a bunch of consolidation here. So I'm I'm saying here that once we finally get this breakout above 75 We're going to hit $1 and then at $1. I think we'll do kind of similar consolidation So that's just kind of my guess here, but but yeah for right now There's just a bunch of consolidation. We're looking for a breakout above these the moving averages And of course we want these moving averages to flip. So So we're probably looking at something at a move, you know If if it does respect this range and play the way it would play out if this it's following this range Then we should be expecting a move here soon because we're trending up We expect a move up So I want to see a break above the moving averages and I want to see a break above these highs right here So that'll set our breakout entry at 63 cents. All right So 63 cents is what we're watching for a breakout entry here.  So above 63 will put us in the clear And it'll put us at least on the road for to get to like 65 to 68 And if we were able to break that then we could look at 70 and 75 So above 63 is what I'm looking at no support entries as of now chain link Chain link kind of a similar situation here Not really interested in any supports here in this range For supports, I it would have to fall back down to this range So I'm just not interested in any of these supports right now Because of the way that this pattern is right So I'm looking for a breakout above this these moving averages and above this So we're basically talking about a break above 1360 And at that point it would pretty much put our entry above $14. So You know, we need a new high at this point You see it ran up all the way to 16 So above above probably 1425 honestly would be the safest one or even above Above 15 is probably the safest one, but we will miss out on a lot here So you can use these moving averages as a signal to entry So I would say at least above $14 for a breakout entry there Tezels Kind of a very similar pattern to chain link Not interested in any support entries here Money flow is going out of Tezels right now So I would need to see that money flow coming back in and a break of these moving averages plus a new high So I'm probably looking at a break above 250 for a Tezels entry And then Neo Same thing. There's just the same pattern as you guys can see these three these last three coins all have the same pattern They're just a drop in a bunch of consolidation not really any movement in any direction So I'm gonna need to see here at least a break above 18 for the first possible entry But really I want to break above 19 1950 really But then 20 would be there So this just depends where you want to but the first entry will be 18 Another entry would be 19 and another another breakout entry would be 20 I'm not doing any support entries here. And that's pretty much it guys looking at At the Bitcoin futures no gaps there, but we got to remember this gap from last week So that's something we're just keeping an eye on But everything else looks fine. All righty guys, that is it for today's video I hope you guys enjoyed it if you did please go ahead and hit that like button And then hit that subscribe as well if you're not subscribed yet And hit that notification bell Because it helps us continue to grow and reach more and more people which in turn makes us makes us really excited I get super excited when I see a lot of followers and views And it makes me want to make more videos and put more time into these videos and Invest more money into the studio to create to you know Produce higher quality content So as you guys can see as we if you watch the videos when we first started to where we're at now It's a huge difference. And we know we're just learning. We've never done any type of videos You know, so we're just learning as we go right now. So hopefully you guys are enjoying this content drop a comment Let us know what you think and that's pretty much it question of the day What camera do you guys think I bought? I just got a new camera in the comments Tell me what camera you think I bought whoever gets it right gets a free membership to our creating room for one month So go ahead and guess guys what camera do you think I bought? That's pretty much it guys I have nothing else to say I am done. I'm through I need water Oh, man, I will see you guys mañana peace love


Welcome back. We're continuing our discussion with Dr. Pete Sexton, who provides us with a few broad brushstrokes on the transition to no-till. It's not just simply a matter of, okay, I'm going to quit tilling and operate everything the way I did before. It's more intensive management. So it's actually, you have to be a little better manager, I think, to be successful with it. Well, anyway, I was going to say, Baz, some of the things that we've just learned from mistakes that we've made or seen, you know, one thing is you need a little more nitrogen initially because you're building your soil organic matter, so that's an investment. It's investing in capital, so to speak. That nitrogen's going into the bodies of the little microbes that went there before. Yeah, so if you were going from conventional tillage to no-till, you'd have to use a little more nitrogen on your corn. You have to be more careful with your winter annual weeds to make sure you get a good burn down in the spring. And then the other thing is you need to make sure your combine is distributing your residue evenly. Because if it's not and you're tilling, you kind of spread it around, it doesn't matter so much. If you're no-tilling and your combine's kind of sort of leaving a windrow, then that's problematic. And then the other point is maybe, you know, just make sure your residue managers and your down pressure are good on your planter. And then we find, you know, it's a little wetter in the spring, but no-till soils will hold up traffic better when it's wet. So we can get in and spray and do field work on no-till fields when we can't move at all on our tilled plots. Yeah, that's a common story that I've heard as well. So I guess those are the things I would look for. Make sure you're distributing your residue well. Make sure your corn's going to leave a little more nitrogen. And then after about somewhere after five, ten years it levels off and you don't need that extra nitrogen. But for the first five years, you know, you're building your soil organic matter, so you need another 25 pounds of nitrogen in that no-till system. Okay, so 25 pounds of nitrogen per acre, that's an increasing cost, right? Sure, but 25 units of nitrogen will cost about $9.50 an acre, which is about a third of the costs of the fall and spring tillage operations. I get that, but average costs vary and it's easy to look at cost comparison in the absence of any context. Is there someone with a little wisdom that can help us take a step back and look at the bigger picture? I have just the person. Next video we're going to visit with Dave Ollila from Butte County. See you soon.


This study found that adolescents are often consulted in the early stages of policy and guideline development but rarely involved in the later stages. This suggests that there is room for improvement when it comes to involving adolescents in the full policy and guideline development process. This article was authored by Mariam Mando, Julie Redfern, Seema Mishahi and others.


Everybody for us here ripping it's legacy of luminance four box NFL makes your number 12 random teams We're gonna go ahead and do our random And then we'll get started Where did the One sec that looks strange. I'm gonna double check the names real quick. I already did but something looks weird for some reason I don't know why it looks like that. Sorry guys Thought I was ready. Oh looks the same Okay, we are good. That was weird. I don't know why I don't know how to explain it. Anyway Let's go ahead and do our random We'll go eight times six and two one two three four five six seven and eight p.m. Down to mic h And the team is here One two three four five six seven and eight. What's up, Zach? Good evening. Got packers down to lions All right. It's p.m. Packers christian. W viking scott h. Niners josh.  Let's get that one going Just four Gonna forget it filled up by the end of this break. We'll break it next Jeff with a spot in the immaculate collegiate mixer that is down to 15 now. We're moving guys Everything is passed halfway full Except that mixer that's the one but it's right there. It's like right there. So see how he's assisted started today Yeah, see how that goes hope that guy's ready to work. Yeah, there's a lot of it Jalen hyatt prized prospects Addison rickety 50 for the vikings Miles murphy we should do ourselves Got orange rookie nice bijan texas color match out of 125 Orange ricky mini let's go fillies. Come on fillies Under the lights kiddle all right ryan tana hill out of 2.99 for the titans Bailey Will anderson to 100 rookie patch autograph for the texans Nice hit houston Three overall pick they're done on washington got brian breecy rookie for the uh The saints i believe the 50 249 is gonna be an errod rogers packers for the ages Under the lights after a mini here mini rookie silver joey porter jr. Steelers under the lights silver derrick henry Gallon's so long to throw in 58 pitches. They're in the fifth Smith and jigba Looking like it ramars looking looking like it Randy moss out of 150 legends for the patriots 19 of 25 anthony ritchardson under the lights autograph for the cults Baby, what a hit What a box as well Colts in the random was coal h rin thomas All right, he got a remandre stevens and a 199 patriots Cut him Cut all the patriots orange mini christ jones chiefs Out of 125 marino and toa Toa's better We'll be like Under the light shillin hurts. What do you say? We'll be like on a ten in a row super bowl Ten in a row. Hell yeah, they couldn't do it when he was playing bro. He's stunk No running backs He's been stunk. There's just dance slinging everywhere eating people up too Eight to go on pinini one now Just eight to go on pinini one Was i'm gonna have so much hair Uh legends to 100 joe name of jets Hended hooker prize prospects I don't believe it's sold out Yeah, it says four in stock Austin aqua autograph chargers to 50 Marvin mimms Yeah Maybe an order's coming through or something Uh-huh Maybe an order's coming through. Oh, yeah, still says four uh 15 to go on the I'm that collegiate mixer That's a good hitting too Got johnson and wilson a 249 jets And they had that forward spin Yeah, Paris johnson jr First letter of the first name. I think it says that in the description, right? We should say that Yep says first letter first name on it Another one came in for crown team all saints came in for one. So we're down to three on crown team all silver mini rookies don't have you on wicks for the Packers Come on Dodgers. Let's get some runs here She's a five game series. Come on Silver rookie kasha butte for the patriots Alec pierce cults. That's out of 150 Bremen up to Tankdale Texans under the lights autograph Under the lights mohomes Blast from the past of okoye All right two luminance now down to two on the crown team all Just two just two That fills up. We'll rip it next Come on freddy Yeah, it's pretty good There's bijan I don't know how it breaks like that. It's crazy Do spawn a 25 bring you for the cowboys 250 points random at the end. Oh, he froze him.  You've got parker washington rookie out over the jaguars of 350 Dude, if he was waiting on that he would have put that ball Like 480 feet away Holy cow that that pitch took some guts. That's I think he missed a little high too Dude, that was sweet. That was a sick at bat To 250 is cleal herbert for the bears tanner mckay rookie auto to 350 for the eagles James who williams lions on the jumbo jersey or not jumbo, but regular sized jersey the adequate to jersey rookie chase frown out of 175 for the bangles Shorter rookie to 200 bills And an addison dynamic. Yeah, seriously shaves.  Uh In this in the zone Where did the catcher line up because that thing I don't think they drew it out the throat right down the middle but He's got nasty stuff. So sometimes it don't matter. I guess You got him guessing, right Kirk cousins out of 100 for the vikings 250 points random to everybody at the ends Tyree wilson rookie out of 150 for the raiders michael mayer raiders rookie autograph out of 100 laurence vestige that's Bennett quentin johnson the 50 rookie for the chargers lawyer maloy as a seahawk on the gridiron grades autograph Why no patriots Damian pierce on the three color patch for houston out of 25 Debo samuel number to 150 for the niners Russ to 250 for denver And unforgettable cd lamb to 100 for dallas All right, just wanted to go on crown team all points random 250 points random to everybody here Top two spots in this random will each get 250 six times one two three four five and six chiefs bangles Quick recap. We had relics of damian pierce numbered cards of debo russ cd lamb a james williams jersey tana hill Herbert cleal herbert there kieshawn johnson and garret wilson erin rogers remandre stephenson justin shorter chase brown tyree wilson alec pierce anthony richeson to 150 congrats to the colts brandy moss curt cousins joe nameth jordan adison brian brissy autos now of michael mayer lawyer maloy tana mckay parker washington tank del austin eckler rpa will anderson jr As well as an anthony richardson under the lights autograph number 19 of 25 That'll do it. Thanks again everybody moving on now to whatever's full


Mr. Danny Kay, Mr. John Carlo Minate, Mr. Arthur Miller, Mr. Isaac Stern, the President of the United States and Mrs. Reagan. Thank you. Thank you. Oh, please. Well, good evening. Nancy and I are delighted to welcome you to the White House, a home that belongs to you and to all Americans. You know, when this go-to-all house was built, our country was a little more than a band of towns, a very thin band running along the eastern seaboard. People cleaned the edge of a vast and untamed continent. And when it came to art, drama, and music, Americans looked back to the old country from where most had just come. But as our nation grew and our people pushed west, plowing fields, felling forests and building new cities and towns, a new and distinctive culture began to develop, a culture that was as fertile as this new land, as bold and confident as the American people. It took on the twang of the frontier fiddle, the joy of jazz, the excellence of the new American orchestras, and the sparkle of Hollywood movies. And today our nation is crowned or greatness with grace, and we gather this evening to honor five artists who have helped her to do so. Lena Horne, when you started making movies, a columnist wrote, Lena Horne has put dignity into daring. She has given glamour, manners. Hollywood has never before seen such a combination. Neither had the world. Lena, you got your start at the age of 16 as a chorus girl at the legendary Cotton Club and then broke into the big band scene as a singer with Charlie Barnett. And during this period, one observer remarked that your voice could thaw the ice in a customer's drink. And in the 1940s, you became the first black woman ever to be signed to a long-term Hollywood contract. And you made unforgettable films like Cabin in the Sky and an American classic Stormy Weather. You often had to battle prejudice, but your work expanded the roles available to black performers. In the 1960s, you became an ardent champion of civil rights, appearing in benefits, joining protests and speaking out again and again. And through it all, you played a direct and vital role in the cause of justice. Today Lena, your voice and style are as powerful and as renowned as ever. Your recent show, Lena, the Lady and Her Music, was the longest-running one-woman show in Broadway history. And you know something, Lena, after five decades when you sing, our spine still tingle, and the ice still melts. And Arthur Miller, you grew up in Harlem, graduated from high school, and decided to study drama at the University of Michigan. You worked for two years, including a job as a shipping clerk in a warehouse to save money for your tuition. After college, you wrote radio dramas for the CBS, Columbia Workshop, and NBC's Cavalcade of America, supporting yourself by working as a truck driver and a steam-fitter in the Brooklyn Navy. Your first Broadway effort, the man who had all the luck, closed after four performances in November of 1944. Your disappointment would have made many young men give up. Not you. In 1947, you returned to Broadway with a play that no one who sees or reads will ever forget, All My Sons. Two years later, the Broadway curtain rose on a new Arthur Miller drama, one that many critics consider the greatest American play ever written, Death of a Salesman. And that play ran on Broadway for 742 performances, was made into a motion picture, and today more than three decades later is still enjoying revivals around the world. Since that brilliant work, you've continued to make rich contributions to American letters with plays like The Crucible and A View from the Bridge.  Gian Carlo Minotti. You wrote your first opera back in Italy at the age of 11. When you were 13, your mother enrolled you in a conservatory in Milan. And in 1928, when you were 17, she took you to the Curtis Institute of Music in Philadelphia, armed with a letter from the wife of conductor Arturo Toscanini. Years later, your teacher at the Curtis Institute would recall, and I quote, Early on, I told him, Gian Carlo, if I'm to teach you, we must come to an agreement, you and I. I promise you that I will be uncompromisingly severe. Do you promise to put in some very hard work? Well, Gian Carlo promised, and he abided by his agreement. And today, millions are grateful that you did. You've given a glorious medium new life with such operas as The Consul, The St. of Blaker Street, and one of the best-loved operas of all time, the Christmas classic, Amal and the Night Visitors. Gian Carlo Minotti, you have always kept your Italian citizenship.  Perhaps tonight you will allow us to claim you as an honorary American. And Isaac Stern, you were born in Russia and moved to San Francisco with your parents when you were one.  But at eight, you were fascinated by the sound of a friend playing the violin.  Your studies were paid for by a woman who recognized your promise. As you put it years later, I got my break because of the faith and belief private people showed in my work. At 11, you appeared with the San Francisco Symphony Orchestra. At 17, you debuted in New York. And by your mid-twenties, you were performing some 90 concerts a year. Today, your repertoire ranges from the classics to the moderns. And one critic has called you the only major violinist exclusively a product of American environment and training. And you've spent a lifetime showing how that American environment glitters with artistic excellence. Danny Kaye, during one of your tours in England, Prime Minister Anthony Eden remarked, Gads, sir, they treat him as if he were a nation. Born in Brooklyn, you made your acting debut at age five in the role of a watermelon seed. At 13, you left home to become a clowning busboy on the Borscht Circuit in the Catskill Mountains. In your early 20s, you joined a troop touring the Orient. Your resourcefulness on that tour became legendary. During a typhoon in Osaka, for instance, you sat on the edge of the stage, sang every song you knew, and spotlighted yourself by holding a flashlight in each hand. When that tour was over, you played nightclubs in London and throughout the American East. At Camp Tamament in Pennsylvania, you met Sylvia Fine, a pianist and composer. And her witty, sophisticated satire was perfectly suited to your delivery and led to a great collaboration. In 1940, your career soared when you stopped the Broadway show, Lady in the Dark, by performing a number in which you reeled off the names of 50 Russian composers in 38 seconds. Something else happened in 1940. Sylvia Fine became Mrs. Danny Kaye and signed by Sam Gold when you starred in a succession of hit movies, including Wonder Man, The Kid from Brooklyn, The Inspector General, The Secret Life of Walter Mitty in which you played no fewer than seven roles and the much-loved Hans Christian Anderson. Forgive me, Danny, but I can't help wishing I'd had one or two of those roles. In 1970, you returned to Broadway as Noah in Richard Rogers' musical Two by Two. And when you injured your leg, you decided that the show must go on. And for 10 and 1 half months, you performed on crutches while wearing a plaster cast. In the 1950s, Danny, you took on a new role, becoming Ambassador at Large for UNICEF, the United Nations Children's Organization. And since then, you've made scores of trips around the world on behalf of needy children and appeared at countless benefits as a guest symphony conductor. Danny Kaye, comedian, actor, singer, and conductor, you brought aid to thousands of children and helped millions of adults to feel young at heart. Each of the artists we honored tonight overcame hardship and each suffered setbacks and failures. Indeed, Isaac Stern once said that after his New York debut, and I quote, I was convinced that I didn't know my elbow from A-flat. Yet they worked long and hard, following their dreams and succeeded in bringing music, drama, and laughter into our lives. And tonight, as we appreciate their work, let us take comfort and inspiration from their lives. Lena Horne, Arthur Miller, Jean Carlo Menate, Isaac Stern, and Danny Kaye, on behalf of all Americans. Thank you. God bless you.


I nominated you for the Westland Mortgage Community Hero and you got it and I wrote you a letter. Dear husband, the one. Webster Stictionary says that a hero is someone who has admired for their courage, outstanding abilities and noble qualities. I nominated you to be recognized as a community hero because you are just that. You have dedicated your entire career to protecting the community. In 2003, you're one of the first Hispanic officers hired in Decatur. Throughout your career, you have served the police department in numerous capacities. But no matter what the department asks you to do, you have completed each task with the best of your ability. You have saved lives, supported people in their very worst moments, seen things that no person should ever see. And shouldered the responsibilities for telling families that a loved one has passed with both kindness and respect. People gravitate to you because they know you care. I'm always a proud police wife, but nothing makes me prouder than when people come up and thank you for what you have done for them personally or for what you have done for our community. You will always be my hero, and I love you without my heart. Love, Robin. Ladies and gentlemen, let's hear it for Officer Juan Panjuelas, today's Wesley Mortgage Community Hero.


Hey everyone, welcome back to figure fantasy. So are you stuck right now? So I'm gonna share with you guys my experience because I'm currently stuck at 160. Most of my figures are stuck at 160. So I'll show you where I am right now. So I only have one figure that is above 160 because she's in four star ready. So for you to go beyond 160, you need to upgrade or promote your figures to four star. That is actually a big challenge because let's say, for example, we want to upgrade or promote Bazzarwin. We will need a three star, a pink or a peach one of the same brand. Not necessarily the same, you know, the same type of figure. But again, it's of the same brand. And obviously, I cannot use these guys because because they are the ones that I'm using. And usually what we do is we would use father FODDR units to sacrifice for us to promote them. So what are your father units? So your father units would be your lesser units, like especially the purple ones. These guys, the purple, the striped purple. So these are your fathers that you should sacrifice for your three star. So for you to sacrifice them to three star, you need to promote them to three star first. So and that entails a lot of copies of these. So you have to get, you have to do summons, you have to do, you have to do summons here. So currently have nine, this one currently have eight. So again, do summons, get some, you can actually get some blinds guys. So the blinds get as many shards or blinds for purple as many as you can so that you could progress faster and upgrade your purples to three star. Assess how many you need per faction because again, let's say if I'm going to be, my main five is this one. So one, two, three, four, five. So if I'm going to be promoting one, two, three, four, I will need one hero from Galatea and three heroes of three star for Tenma. So again, there's a big discrepancy. You might want to transfer your level ups to other other other factions so that you would, you know, it would be the three star for every faction would be even distributed. So you could probably downgrade this and put them on the otako and get, for example, Osuke, I forgot his name, probably lower him down from the otako and upgrade him so that you have two Galatea and two Tenma left. So that, you know, charge are really hard to come by, especially if you want to concentrate on just one faction. Okay. So that is one of the things that I want you guys to, you know, to realize and try to do and also try to get some good values in the store. There are some good values in the store for your purple units. Okay. So this strategy just hear me out is going to be just temporary. You're not going to do this. This is just a switch in strategy.  You can actually you can actually purchase these in, you know, in replacement for your this one, the yellow ones up to the time that you can raise everyone to 61. It's actually your option. I'm not saying that you should do it, but this would make your progress even faster. Okay. So as well as the board, the board game store can opt to buy these again. This is just an option guys. I'm not telling you to do it. Because right now, based on my experience, if I'm stuck in a certain level, I cannot move forward to other content as well. So unless if you want to hasten up your progress, then you have to sacrifice some things first. Okay. Then you have your club store and your owner store. Your owner store. This is the one that I'm, you know, I'm telling you to get for the meantime, instead of these. So it's just a temporary solution to a temporary problem. While you're, you know, while we're waiting for, for everybody to be upgraded to go up and for everyone to reach 161, what do we do? Do we do nothing? Of course not. One of the things that you should do with your figures is to make sure that their design letters are already full. So they're already, you know, they're already prepared, just waiting for them to be 161. Make sure that almost all of them are just waiting for, for, for the upgrade to 161.  So this one, the lowest is going to be blue. The one that I'm farming right now based on my last video is actually the yellow ones already. So while you're waiting for, you know, for everybody to go beyond 161, please upgrade your gear. And also one last tip is if you have a set of, you know, set of figures already per faction, like for example, for, for Let's Red, I have already six. If you still have figures that you want to upgrade up to 160 now is the right time because you will have excess, um, excess resources. So from here, then you go to Tenma, take a look at which are you considering to put, to level up as well to 160. Then to Galatea, what I'm doing right now is actually leveling up Asteroth. So for Asteroth, I just, I'm actually leveling up his design letter and I'm running out of gold and currency. So as you can see here, I can use the sweeps and I'm going to be waiting for gold. And also for the parts, I'm also trying to make sure that I have parts for him. So again, expand your roster up to 160, expand your roster for the different, for the different brands. While you guys are waiting to go past 160 or again, the other level is going to be 181. So you can repeat this process whenever you get stock in a certain level. So that is it guys. So thank you very much. I think those are my tips for when you're stocked at 160, just farm every day, farm resources because again, once you're, you move forward from 161, you're going to need those resources, you're going to need those figures, you're going to clear certain stages again and you'll need all the help that you can get. Okay. So for those who've stocked this far, please consider subscribing because this helps my channel a lot. Also don't forget to click that bell icon so you don't miss future, future figure fantasy videos in my channel. Also guys, please put a like to this video. Thank you guys. Take care. Stay safe. This is The Warden and I'm out of here.


everybody. Here we are in part three of Prepping for a Special Project where I'm continuing to refine the painting studies that are now on the small canvases. First we're going to work some more on the face and we're going to refine our shapes and colors, our light and shadow. This is not at all where I thought initially that this face would go when I saw the inspiration photo on the magazine when I started painting it in the art journal. I had no idea but the place that it's gone, that it's going, I absolutely love. So that being said here is a fast forward of me working on the face. Next in part four you'll see some more working on the face and also working on the sunflowers and at the end of that video I'll tell you which one I decided to do on the big canvas. In part five will be me working on the big canvas, at least as much of it as I'm allowed to show you. There may not be a whole lot because I'll be working on it during the photo shoot. Anyway, enjoy. I'll be back right at the end and the shadow on the face. The lips do give me a little bit of a hard time but I do get them resolved at the very end and then next we'll work on the sunflowers. I hope you're enjoying the process with me of working on these little painting studies and working out the composition and color in these paintings and I hope it gives you some ideas of what you can do. Don't forget the most important thing besides enjoying your art and having a good time with it.  Don't forget to like, share, and subscribe and I'll see you in the next video.


All right, it's Python on hardware time Yeah, so by the week the only news this week and the news to talk about is It's circuit Python day. Yes, so this Friday and just so everyone knows how this works out a data fruit I don't think we're gonna have to put up a notice on the site, but this is a company holiday There's no holidays in August So we made up one, but yeah, it's like we already had Labor day and there's Thanksgiving and then there's Christmas and then and one of the things that we know that's really important to To all of us who work is time off and being able to use that as a float holiday or being able to just take time off Because there's more to life than work and a lot of folks You know store time off or vacations and more so we wanted to have a day that everyone could take off They wanted to and so some folks are not going to be physically a data fruit But I think we're gonna have Enough folks to keep things going, but a lot of the team is working on all the online efforts This is still an online event probably will do some physical stuff in the future, but circuit Python day starts Friday August 19th, and the updated schedule is up. You could check it out on the site. It's everywhere It's on the blog. It's pretty much everywhere we can go starting in 11 a.m. Eastern time We're gonna do a circuit Python day introduction then we're gonna be celebrating code and community Panel discussion so you might see a lady Aida or I or some other folks There's gonna be a circuit Python development sprint intro video a circuit Python project built with maker Melissa Special edition circuit Python theme show and tell circuit Python 8 preview circuit Python day chat with Katnie Jeff and Dan For me guys circuit Python day game jam stream and circuit Python Development sprints no video content with that that'll just be the But if you want to take advantage of the sprints Scott and Dan will be helping people who want to contribute to the core Or you want to do some library work? Yeah Speak up early and we'll we'll be able to get you a pull request or an issue or your pet project You could get help from Dan and Scott During that time and this is last time we're gonna see Scott before he's on leave for a bit He'll be back later in the winter Yeah fall but now now's a great time to Contribute a circuit Python and get introduced as a developer and I'll I'll answer some of the questions that have come up at the end But I'll also probably do some of them real time So during psych of circuit Python day will be deals with certain products that may be featured or is it only focused on software? No, we'll have a discount code. Just look at some of the chats. I'm gonna do it that day I'm gonna just see what we have in stock and more because what I don't want to do if we're like out of a lot of stuff is say like Oh, hey, here's you know a discount code and then oh, no, this isn't the thing. We're featuring So I would just make sure that I know what I'm talking about So we'll see how things go on Friday, but there'll be a discount code for sure What it'll be for just stay tuned okay, and There's other events and things going on you can check out Blues wireless they have stuff going on The newsletter does have some interesting thing this week But you know like I said, this is all in preparation of circuit Python week this week Good news though. This is I think worth mentioning Although maybe you don't need to really pay attention to these rankings, you know But they are helpful This index that we look at all the time. This is the info world Tiob, I don't know how people pronounce it But it's a ranking of like the popularity with programming languages and Python continues to be a number one language And I don't think so, you know one of the problems is people get really polarized And dogmatic about religions like no it needs to be this one of the cool things is You don't have to commit to any of these you can try them out So the popularity of Python is probably because it's very easy to try out It's very human readable and you can get really far really fast and then there's a lot of expertise you can add Later and then you can do things like microcontrollers Almost within, you know seconds now, especially with circuit Python and micro Python So that's kind of neat and it's just it's just one of those things we see ticking up more and more and more and more So, you know, especially for young folks that are just getting in the programming Not only do they get to do some powerful things really fast, but they can also do electronics and a lot of our boards, you know Well, you you start with circuit Python or make code and then eventually, you know You're like look I want to do you know real-time operating systems and like more powerful stuff You can always move to see C++, you know, like we did streams on platform IO and we've done projects with Arduino and Zephyr and free RTOS. So there's you know, Python is I think it's good for powerful projects But it's also a great way to prototype stuff that you can then refactor and we do in a You know more compact language if necessary. Yeah, and then I'll answer a couple questions while we're here in circuit Python day land Go back to Blanka. Oh, no, I'll just stay here So the next question is Do you need any gear for circuit Python day? Not really like the good thing is like pretty much any board that runs circuit Python You can have you can order something. I guess you could potentially get it by Friday But any any electronics that you can run circuit Python on so circuit python.org slash downloads You probably have something right now. You can run on a Raspberry Pi. There's pretty much almost anything anything Pythonic. Yeah, if you want to contribute during sprints, you know, of course, it's best to have the hardware that you want to sprint on Otherwise, it's gonna be really tough. We do have some, you know issues and PRs that are documentation based and so of course you can do those without hardware, but Yeah, if you want to contribute code being able to compile and test the code on your own is gonna be really essential Okay, and then I'll answer this one Why would we have circuit Python instead of continuing with micro Python? The good news is There's both you get to decide what you want based on your needs and hardware and Expertise level so we're the biggest. I think financial supporter of circuit Python at least publicly Sorry, we'll both yeah micro Python both So we contribute to micro Python. We sell the boards in our store We sponsor micro Python, but we also needed something that Especially back in the day. This was what eight years ago now that could work on all different platforms so micro Python is very specific for very specific types of hardware and It's I'd say there's a different level of expertise usually associated with it where circuit Python is the educational version things that Get people started very quickly Massive hardware support lots of devices that's drivers lots of drivers Consistent API this is API works on a Raspberry Pi computers, and that's what our customer is expect They wanted you know for Noah just to give you an analogy They wanted an Arduino like experience, but even easier and so that's not micro Python and if you you know check out micro Python That's not what their goal of the micro Python project is luckily It's all open source so you can decide what you want and when I do see a lot of folks deploying micro Python for They'll fork micro Python They'll say this is going to be from like my device and they'll you know like Lego has a fork of micro Yeah, so that it's basically I feel like there is like there's a quick Python Well, there's like this Linuxy version like people are like oh, I need to like run Linux on something So they'll fork, you know their version of Linux and yeah, there's like 500 Yeah, and then there's very big distributions that are made specifically with more ease of use Yeah, go bun to yeah, I'm for one way colleagues designed for another thing So I you know one of the things that I think people get trapped in is like or it's not it's and and if you look at the Entities that contribute to micro Python a to fruit being One of the bigger ones and we help with the fundraising And we fix bugs I think that's the right way to to look at open source is you're building on top of things together And there's cross-pollination of drivers and more and there's no way that micro Python is going to support Three so if you go to a circuit python.org slash downloads, that's not micro Python's mission to support every different board under the Sun In fact, there's more Circuit Python boards from other companies besides a to fruit then a to fruit boards That's that's what we wanted to do and it's neat to see that is a giant menagerie of stuff. So that's what we decided to do and the Drivers is I think the hardest part to get things to work and that's what we focused a lot on yeah, because we want to make sure all of our sensors and breakouts work and so we spend a lot of time on Having really good quality drivers that work with circuit Python But that required having a continued an API. That's the same across every board So anyways, and you know, we try to keep in step with micro Python as each release comes out So that's that's a longest answer, but that's you can also go to circuit python.org and scroll down to the bottom There's a lot of text. Okay, and that is Blinka Python on hardware Don't forget this newsletter is Available to you can be delivered every single week and get that at a to fruit daily and at a to fruit daily comm we Don't Spam you it's a separate site. It's completely different as we sell your data. No, do we want your data? Do we give your data away? Do we trade your data? No, do we do anything? No, no No, so the reason we did that is because we never wanted anyone to think if they Order something on a to fruit comm that they're gonna get a newsletter You know you have to try really hard to get an email from us But a to fruit daily is just newsletters and it's spam free ad free and that's how we do that. Okay


This effectively comes down to the question, is it possible for an object to undergo gravitational collapse? In the early days of relativity theory, most physicists, including Einstein, intuitively felt this was impossible. That some physical process would prevent the density of matter from growing large enough to create an event horizon. Even a star is a spherically symmetric ball of gas. At any spherical boundary within the star, there will be a gravitational force pressing inward, representing the weight of all the stellar material outside the boundary. We'll quantify the effect of gravity by the amount of energy required to pull the star apart. Viewing the star in cross-section, imagine we somehow take hold of the top layer of material. And working against gravity, pull it away to infinity. We continue to pull the star apart, layer by layer, until nothing is left. Calculating the total work required to disassemble the star, we find that it varies as the star mass m squared over the star radius r, multiplied by a constant, which we don't bother with here. We define the gravitational energy of the star to be the negative of this work of disassembly. General systems tend toward the state of lowest energy. If gravity was the only force acting, this would be an energy of minus infinity at r equals zero. Gravity wants the star to collapse. For the star to resist collapse and remain in equilibrium, the gravitational force must be offset by an outward pressure of equal magnitude. The primary sources of stellar pressure are first, gas pressure, analogous to earth's atmospheric pressure, although under much more extreme conditions. Gas pressure varies with temperature. At higher temperatures, gas particles are, on average, moving faster, and so transfer more momentum when they collide. Second is radiation pressure, due to transfer of momentum by the thermal emission, absorption, and scattering of electromagnetic waves inside the star. Now, both of these sources of pressure vary with temperature. At non-zero temperature, a star will radiate power into space. This must be made up by an internal power source, otherwise the star will cool. Nuclear fusion is the primary source of this power. As light nuclei fuse to form heavier nuclei, energy is released, but only up to a point. For nuclei heavier than iron and nickel, fusion requires a net input of energy, such as can occur in a supernova explosion. So even though it may take billions of years, a star is ultimately destined to exhaust all internal sources of energy and grow cold, bringing gas and radiation pressure to an end. What remains is the phenomenon sometimes referred to as the stability of matter, the fundamental explanation of why solid matter is solid, the reason why we don't fall through the floor. To be completely rigorous, we would need to solve for the quantum mechanical state of all nuclei and electrons in the frozen star and the resulting forces opposing gravity. Instead, what we'll consider is a very rough, back-of-the-envelope type calculation of what is expected to be the dominant effect at extreme densities, so-called electron degeneracy pressure. We first consider a non-relativistic analysis. Let's denote the star's radius and mass by big R and big M. Assume that each electron, with mass little m, is constrained to a region of radius little r, and that there are n sub e electrons per unit mass. In most elements, there is approximately one electron per proton neutron pair, so this is more or less a fixed value. The total number of electrons in the star is that n sub e times the star mass. This is also the volume of the star divided by the volume per electron, which varies as the cube of big R over little r. Solving this expression for little r, we find that it varies as big R over the cube root of big M. Here and in what follows, we drop physical constants and focus on the effects of the star's radius and mass. The uncertainty principle of quantum mechanics implies that if an electron is constrained to a region of dimension little r, it must have a momentum p on the order of Planck's constant h over r. Using the above expression, this varies as the cube root of the star's mass over its radius. The non-relativistic expression for kinetic energy of an electron is its momentum squared over twice its mass. This varies as the two-thirds power of star mass over the square of star radius. This kinetic energy is not dependent on the star's temperature, it's an intrinsic quantum mechanical property, even at absolute zero. Multiplying by the number of electrons, we get the total kinetic energy. Since the number of electrons varies as the star's mass, we obtain a total kinetic energy of big M to the five-thirds power over big R squared. We've already seen that the gravitational energy varies as the star's mass squared over its radius. Combining these two terms and removing a common factor, we see that for any mass, the total energy grows arbitrarily large as the radius grows arbitrarily small. From this, we conclude that gravitational collapse is impossible. Now we look at a relativistic analysis. The steps are the same until we get to the electron kinetic energy. The relativistic expression for kinetic energy is square root of p squared plus M squared minus M. For small p, this agrees with the classical expression, but for very large p, which corresponds to very small star radius, it behaves like p and not like p squared. The result is that the total kinetic energy varies as one over the star radius, not one over the radius squared.  We see that if the star's mass is small, the constant will be positive, so the energy would again approach positive infinity as the radius approaches zero. However, if the mass is large enough, the constant will be negative, and the energy will approach negative infinity as the radius approaches zero. That is, the star will undergo gravitational collapse. This phenomenon is called the Chandrasekhar limit. After Subramanian Chandrasekhar, who derived it rigorously in a series of papers starting in 1931, he was able to solve for the ultimate radius of a star as a function of its mass, and showed that this radius is zero if the mass exceeds a certain limit. Current calculations set this limit at about 1.4 times the mass of our sun. Now, the process of stellar evolution is typically dynamic and often violent, resulting in some of the star's mass being ejected as a planetary nebula, supernova remnant, or in some other phenomenon. However, if the mass of the remaining core is above the Chandrasekhar limit, then it will not be able to resist gravitational collapse. But what does it collapse to? The answer is, not necessarily a black hole. By the 1930s, a theoretical picture of nuclear physics was emerging. Nuclear were known to contain protons and neutrons. It was thought possible that under certain conditions an electron could be captured by a nucleus, converting one of the protons to a neutron with the emission of a neutrino. This process of electron capture was observed and reported in 1937 by Luis Alvarez. The implication was that in a collapsing star all electrons and protons might combine in this manner, leaving an object composed of nothing but neutrons, what we now call a neutron star. This led to a consideration of the stability of neutron stars through neutron degeneracy pressure. In 1939, Oppenheimer and Volkov analyzed the problem and showed that there is an upper limit to the mass of a neutron star, beyond which it will undergo gravitational collapse. They concluded, actual stellar matter after the exhaustion of thermonuclear sources of energy will, if massive enough, contract indefinitely. This limit is not as well defined as the Chandra Shekhar limit, because the physics is more extreme and not as well understood. It's thought to be less than about three solar masses. Currently, the largest known neutron star has an estimated mass about twice that of the sun. A neutron star over this limit might collapse to a black hole. Another hypothetical possibility is the transformation of neutrons into a collection of free quarks, forming a quark star. Currently, there is no substantial evidence of quark stars. Even if such things did exist, they would have their own upper mass limit. And since quarks are elementary particles, there should be no further transformations possible, and we would finally have a collapse into a black hole. So, it seems that there is no theoretical process that can stop a large enough star from ultimately forming a black hole through gravitational collapse. Someone who pushed back against the idea of black holes was Albert Einstein. Someone ironically, since it was his theory that predicted them. In 1939, he published a paper claiming, The Schwarzschild Singularity does not appear for the reason that matter cannot be concentrated arbitrarily, and this is due to the fact that otherwise, the constituting particles would reach the velocity of light. His argument was based on assuming the particles of a collapsing star would follow essentially circular orbits. He remarked, Although the theory given here treats only clusters whose particles move along circular paths, it does not seem to be subject to reasonable doubt that more general cases will have analogous results. But, Einstein was wrong, and we've already seen why in our previous discussion of orbits around a black hole. It's true that there is a radius outside the event horizon, where the velocity of a circular orbit is the speed of light. And it's true that no circular orbits smaller than this are possible. However, it does not follow that an in-falling particle passing through this radius would have to travel faster than light. In fact, we've already calculated such orbits. They're not circular, they're spirals. And, as we've shown, a particle can fall in radially. Both of these processes are well described by relativity theory. Regardless of how bizarre they may have seemed to Einstein and others, no known physical process has been found that could keep a black hole from forming. Given that they are theoretically possible, the obvious question then is, can we detect black holes? By definition, we cannot see a black hole. Classically, they do not emit any radiation for us to detect. So any evidence for their existence will have to be circumstantial. What they do produce is a very strong gravitational field. If a visible object moves through that field, it will exhibit an acceleration that indicates both the mass and distance of the black hole. Due to breakthroughs in observational technology, astronomers are now able to view and track stars near the center of our Milky Way galaxy. What they've seen are several stars orbiting an invisible central object. From these orbits, the object's mass has been determined to be some 4 million solar masses. Moreover, the orbit's place and upper limit on its size, roughly the size of our solar system. A supermassive black hole is the only known object consistent with these observations. Other evidence for black holes can come from an accretion disk. If material falls into a black hole, it can accelerate to near the speed of light. These high speeds and violent collisions produce tremendous heat, which in turn generates radiation. Temperatures of millions of degrees are possible, which can produce intense x-ray emissions.  The radiation burst associated with material falling into an accretion disk is called an x-ray nova. However, this by itself is not evidence of a black hole. The intense gravity of a neutron star can also produce an accretion disk in x-ray nova. But there's a key difference illustrated in this figure. As material spirals in through the accretion disk, the radiation it produces is ever more redshifted. If the central object is a black hole, this redshifting continues without end, and the material disappears into the event horizon. However, a neutron star has a solid surface, and the in-spirits of a black hole star has a solid surface, and the in-spiriling material ultimately strikes this, producing an additional characteristic x-ray burst. It's the lack of this final burst that provides evidence that the central object has no solid surface. And the only massive object without a solid surface is a black hole. Finally, gravitational waves were recently observed by the laser interferometer Gravitational Wave Observatory. These bear the characteristic signature of merging black holes, and cannot be explained by any other known process.


Another 1,050 Russian soldiers and officers were confirmed as killed or wounded in action in the past day alone, reports the general staff of Ukraine's armed forces. Russia lost another 12 tanks and 75 UAVs over the past day. The UK Ministry of Defence said the number of dead and wounded reflects Moscow's commitment to attritional warfare. Both Kiev and Moscow shrouded their causality counts in secrecy, due to the effects they can have on army morale, populations at home and how the war is. Perceived Abroad. Each side can overestimate the number of enemy dead and wounded, meanwhile. The Ukrainian Defence Ministry says about how many pieces of equipment its forces had managed to destroy in the first 24 months of the war started by Vladimir Putin. In the post, it said on Monday, 13,000 Russian armored combat vehicles have been destroyed since the beginning of the full-scale invasion. It's, on average, more than 500 armored vehicles per month. Russian warriors destroy Russian weapons with incredible speed. Bravo, the Defence Ministry added.