توينز 304 | كاس العالم مباراة السعودية ومصر كله رايح

( لا تنسى الإشتراك بالقناة عشان يجيك آخر فيديوهاتنا )
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توينز 304 | كاس العالم مباراة السعودية ومصر كله رايح
#توينز – برنامج رياضي يغطي الدوري السعودي و من تقديم التوأمين محمد و عبدالله الأحمري.

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Samsung Monitor: CJ79 Thunderbolt™ 3 Curved Monitor

World’s First Thunderbolt™ 3 Curved Monitor CJ79.
Connect to Infinite Possibilities: eye comfort and immersive performance with curved
screen, powerful multi-tasking with 21:9 ultra-wide screen, supreme picture quality with QLED, and unparalleled premium design.
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HOW TO – Make your iPhone Battery last a WEEK!

30+ TIPS & TRICKS to make your iPhone Battery last longer!
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Huge “Thank You!” to NCS for the EPIC music!
(Mostly Tobu, Alan Walker & Jim Yosef)

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5 Anime Where The Main Character Has Many Beautiful Girls

5 Anime Where Many Girls Chase After One Guy. 5 Anime Where Bunch Of Girls Fights For One Guy.

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ANIME WHERE THE PROTAGONIST HAS A HAREM. Harem-type anime series’ are as jam-packed of beautiful women as one might expect. However, the protagonist might get overwhelmed with so many females surrounding them.

This is TheGamer’s list of 5 anime where the main character has many beautiful girls!

Check out these other awesome videos!

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Most, if not all, popular anime series that regard either facing off against evil doers, chefs, demon-like entities, or witches with the power to destroy the entire world, have one thing in common, a protagonist surrounded by several cute girls with unique attributes.
In this video, we’ll be taking a look into anime series’ where there are girls that are not only beautiful, but also have ravishing personalities, demeanors and insane power or skills alike. So, sit back and relax as we take a look into some popular anime series that fit this criteria!

First is the widely popular Bleach series, which entails soul reapers with spiritual pressure facing off against hollows, quincies, arrancars and everything in between to prevent the human race from falling victim to these otherworldly entities! Ichigo Kurosaki, the main character with MANY transformations, an impressive win-loss record and a fascinating thirst to save his friends, is no stranger to being crowded by several eye-appealing females within the series.
Next up is the lewd and humorous Monster Musume, which showcases a world where humans and humanoids with animal traits have to live in harmony which, as you might guess, brings in not only chaos within Darling, the protagonist’s, home, but also makes his everyday life a living hell when the monster girls he’s surrounded by, fight over him constantly. This is also a big problem for Issei, the protagonist and male lead within High School DxD. Whichever one of these series’ you decide to watch, there is no shortage of beautiful girls!

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Script by: Chuck M.G.

Voice Over by: Justin Freitas

Edited by: Jonathan Choi

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Week 2 Highlights | Dana White’s Tuesday Night Contender Series

Check out the highlights of week 2 of Dana White’s Tuesday Night Contender Series!

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Lostvayne – The Seven Deadly Sins – MAN AT ARMS: REFORGED

Today our blacksmiths make Lostvayne from The Seven Deadly Sins series.

Lostvayne – The Seven Deadly Sins – MAN AT ARMS: REFORGED

Our team of blacksmiths and craftsman build some of your favorite weapons and some weapons that you’ve never seen before.

Filmed on Location at Baltimore Knife and Sword
http://www.baltimoreknife.com

Ever wanted to ask the Man At Arms team a question? Now you can! Go to AWEme’s Twitter: @awemechannel and use #AskABlacksmith with your question. Matt and Kerry will be answering your questions with a video reply on AWEme’s Facebook.

Kerry Stagmer – Swordsmith and Machinist
Matt Stagmer- Swordsmith / Blade Grinder
Ilya Alekseyev – Bladesmith / Armourer
John Mitchell – Shop forman / Lead fabricator
Ferenc Gregor – Carving and design
Bill Collison- Assistant Blade Grinder
Rick Janney- Assistant Smith
Tanner Saslow – Machinist/Knifemaker

Episode Produced and Directed By – Brendan Kennedy

Supervising Producer – Phil Rogers
Office Production Coordinator – Jon Michael Burgess

Baltimore Forge Crew:
Producer – Kerry Stagmer
Director of Photography – Paulius Kontijevas
Story Producer — Adam Hiner
Production Manager – Patricia Parris
Runner/PA – Mei Lin Lau Mann
Camera Op – Christopher Mariles
Set Medic – Kevin Dugard/ Rachel Obitz
1st AC – Jason Remeikis
2nd AC/DIT – Michael “MJ” Johnson
Gaffer – Steve Scott
Grip – Jeff Retburg
Swing – Paul Oh
Swing – Marc Elzey

Post Production:
Edited by — Christopher Otwell
Colorist – Patrick Burke
Post Sound – Anthony Vanchure
Lead Assistant Editors – Stephen Erdmann
Manager, Post Production Operations – Michael Gallagher
Post Production Supervisor – Gracie Hartmann

Tonight’s Sky: July 2018

This year, Mars reaches its long-awaited opposition on July 27—and is visible all night. Look for its south polar cap and dark features that shift as the planet rotates. You will also spot constellations Scorpius and Sagittarius, and the annual Delta Aquarid meteor shower.

“Tonight’s Sky” is produced by HubbleSite.org, online home of the Hubble Space Telescope. This is a recurring show, and you can find more episodes—and other astronomy videos—at http://hubblesite.org/videos/science

Kepler Supernova Remnant in Multiple Wavelengths [UltraHD]

This animation shows the remnant of Kepler’s Supernova, shown first in infrared, then visible, then low energy X-ray, then high-energy X-ray emission and finally in combination.

In 1604, astronomer Johannes Kepler noted the appearance of a new bright object in the sky, visible to the naked eye for the next 18 months. Today we know that he was seeing the death of a star 20,000 light years from Earth. It was more than ten times the mass of our sun.

Now, more than four hundred years later, several of NASA’s Great Observatories combined to produce a multi-wavelength image of the expanding remnant. Although the initial blast was caused by the implosion of the star core that rebounded to violently eject material. The supernova today can be seen as it impacts surrounding material that was likely ejected in previous episodes of losing mass into space.

The multiple wavelengths show separated layers of emission that represent different portions of the impact. Infrared (Spitzer) traces the coolest material as it is heated by the ejecta. The optical emission (Hubble) traces hot (several thousand degree) gas that is excited by the collision. The lower energy X-ray (Chandra) represents much hotter gas – up to a few million degrees, Fahrenheit, similar to the hot corona of our sun. The highest energy X-ray emission can reach tens of millions of degrees. This emission is closest to the most powerful portions of the expanding blast wave. The observations reveal that Kepler’s supernova was a “Type Ia” – a supernova caused by the transfer of material between two smaller dwarf stars. The added material brings the total mass of one of the stars beyond the critical threshold for supernova collapse.

Video: NASA, ESA, and G. Bacon (STScI)
Images: NASA, ESA, R. Sankrit and W. Blair (Johns Hopkins University)