INSPIRING Kid Dance Audition Gets GOLDEN BUZZER On Britain's Got Talent 2019 | Got Talent Global 

Nationality is just color and language, we all bleed the same so, in my eyes (and I'm sure, alot of others) we are the same 😉👍 omg, I absolutely love him!!! He made me day and will be looking at this, everytime I feel down 😊❤

this would inspire me to not do this stuff

Adults should also feel proud motivated because of him

YES!!!!! I completely agree 👍

IKR

💖💖💖💗💗💗💓💓💓

'Bombay dreams'😍😍

And he is also in South movie " Naach lucky Naach"

Bombay Dreams❤

I'm America

FR THOOOOOO, THIS IS SO ACCURATE💀💀💀

so glad he's gpood0

always? are you kidding me?

"Thank You Come Again"

Naanum

Indian’s are so powerful!

wonderful you showed nothing is impossible

പിന്നല്ലാണ്ട്

And PAKISTANI like me

I hate this

I am only joking he is great 👍👍👍

Yeah I saw that movie. That movie was after this show.

Yes

Are you also proud to all the hackers and scammers in your country?

Yeah

He already was. He was also on India's got talent, he was also got a part on Ellen DeGeneres show. He was already famous before going in to Britain's got talent.

He was in movie Lakshmi

Ya I know

🧨

Not me

@@dynasty4444 هھههههه

Poda panni

EAGLE OF FIRE avanaa nee😱

Yes

Meeee!!!!

Me

ใน

Meee From Kerala

meeeeee.

U shudn really say that...it's mean....even tho I'm an Indian.

@@joel5067 bro but I didnt say bad about any other nations!!

Mate that really aint true

Nah dude i don’t believe what u just said, india isnt better than other, all nations and countries and states have talents not only india

its just rude commenting that, i mean like, im offended by ur comment

A neutron star is the collapsed core of a giant star which before collapse had a total of between 10 and 29 solar masses. Neutron stars are the smallest and densest stars, not counting hypothetical quark starsand strange stars.[1] Neutron stars have a radius of the order of 10 kilometres (6.2 mi) and a mass lower than a 2.16[2] solar masses.[3] They result from the supernova explosion of a massive star, combined with gravitational collapse, that compresses the core past white dwarf star density to that of atomic nuclei. Once formed, they no longer actively generate heat, and cool over time; however, they may still evolve further through collision or accretion. Most of the basic models for these objects imply that neutron stars are composed almost entirely of neutrons(subatomic particles with no net electrical chargeand with slightly larger mass than protons); the electrons and protons present in normal matter combine to produce neutrons at the conditions in a neutron star. Neutron stars are partially supported against further collapse by neutron degeneracy pressure, a phenomenon described by the Pauli exclusion principle, just as white dwarfs are supported against collapse by electron degeneracy pressure. However neutron degeneracy pressure is not sufficient to hold up an object beyond 0.7M☉[4][5]and repulsive nuclear forces play a larger role in supporting more massive neutron stars.[6][7] If the remnant star has a mass exceeding the Tolman-Oppenheimer-Volkoff limit, it continues collapsing to form a black hole.

@@cloroxbleach1640 thanks for telling me science?

@@thegibbatron87 mhm

@@Lewfa A black hole is a region of spacetime exhibiting such strong gravitational effects that nothing-not even particles and electromagnetic radiation such as light-can escape from inside it.[6] The theory of general relativity predicts that a sufficiently compact masscan deform spacetime to form a black hole.[7][8] The boundary of the region from which no escape is possible is called the event horizon. Although the event horizon has an enormous effect on the fate and circumstances of an object crossing it, no locally detectable features appear to be observed.[9] In many ways, a black hole acts like an ideal black body, as it reflects no light.[10][11] Moreover, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a black body of a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for black holes of stellar mass, making it essentially impossible to observe. Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace.[12]The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although its interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were long considered a mathematical curiosity; it was during the 1960s that theoretical work showed they were a generic prediction of general relativity. The discovery of neutron stars by Jocelyn Bell Burnell in 1967 sparked interest in gravitationally collapsed compact objects as a possible astrophysical reality. Black holes of stellar mass are expected to form when very massive stars collapse at the end of their life cycle. After a black hole has formed, it can continue to grow by absorbing mass from its surroundings. By absorbing other stars and merging with other black holes, supermassive black holes of millions of solar masses (M☉) may form. There is general consensus that supermassive black holes exist in the centers of most galaxies. Despite its invisible interior, the presence of a black hole can be inferred through its interaction with other matter and with electromagnetic radiation such as visible light. Matter that falls onto a black hole can form an external accretion disk heated by friction, forming some of the brightest objects in the universe. If there are other stars orbiting a black hole, their orbits can be used to determine the black hole's mass and location. Such observations can be used to exclude possible alternatives such as neutron stars. In this way, astronomers have identified numerous stellar black hole candidates in binary systems, and established that the radio source known as Sagittarius A*, at the core of the Milky Way galaxy, contains a supermassive black hole of about 4.3 million solar masses. On 11 February 2016, the LIGO collaboration announced the first direct detection of gravitational waves, which also represented the first observation of a black hole merger.[13] As of December 2018, eleven gravitational wave events have been observed that originated from ten merging black holes (along with one binary neutron star merger).[14][15] On 10 April 2019, the first ever direct image of a black hole and its vicinity was published, following observations made by the Event Horizon Telescope in 2017 of the supermassive black hole in Messier 87's galactic centre.

chip Life I can’t even dance

Agreed...

It's a great idea but you know some angry contestants might get a no vote and their friends are back stage and press that button without dec and ant knowing

awesome jawson congratulations you win a prize it’s mailing to you now 😎

I also

S

Same!

IKR

You too brother

First time not bro

It’s a dude duh

same i love Indian

@@justynaadamska3475 WTF you had written you think its a joke

Sajith Bhaskaran I’m Indian to

we are nort india but i like the dance

Malayali

yep

What happened to north and south?

Shut up before I take away your wifi

In Which

@@shivpandey8938 check this ru-vid.com/video/%D0%B2%D0%B8%D0%B4%D0%B5%D0%BE-XOg1QpXBLBw.html Movie name Lakshmi