A star is an astronomical object consisting of a luminous spheroid of plasma held together by its own gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, the brightest of which gained proper names. Astronomers have assembled star catalogues that identify the known stars and provide standardized stellar designations. The observable Universe contains an estimated 1×1024 stars,[1][2] but most are invisible to the naked eye from Earth, including all stars outside our galaxy, the Milky Way. For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the star's lifetime, and for some stars by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, its luminosity, and spectrum respectively. The total mass of a star is the main factor that determines its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the star's environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities produces a plot known as a Hertzsprung-Russell diagram (H-R diagram). Plotting a particular star on that diagram allows the age and evolutionary state of that star to be determined. A star's life begins with the gravitational collapse of a gaseous nebula of material composed primarily of hydrogen, along with helium and trace amounts of heavier elements. When the stellar core is sufficiently dense, hydrogen becomes steadily converted into helium through nuclear fusion, releasing energy in the process.[3] The remainder of the star's interior carries energy away from the core through a combination of radiative and convective heat transfer processes. The star's internal pressure prevents it from collapsing further under its own gravity. A star with mass greater than 0.4 times the Sun's will expand to become a red giant when the hydrogen fuel in its core is exhausted.[4] In some cases, it will fuse heavier elements at the core or in shells around the core. As the star expands it throws a part of its mass, enriched with those heavier elements, into the interstellar environment, to be recycled later as new stars.[5] Meanwhile, the core becomes a stellar remnant: a white dwarf, a neutron star, or, if it is sufficiently massive, a black hole. Binary and multi-star systems consist of two or more stars that are gravitationally bound and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution.[6] Stars can form part of a much larger gravitationally bound structure, such as a star cluster or a galaxy.
Ah yes, peach asked me to gather the stars and defeat bowser, but instead I will proceed to break the laws of physics and quantum tunnel through multiple objects.
Bowser:he wont get the stars they are difficult! 1 sec later*so long gay bowser Bowser how did this happen?! 1 sec before*YAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYA
@@gcm64 I can't but imma name some lakitu skip blj sblj bombomclip owless canonless (both) straight swimming (idk what it called) uuhhh there a lot of strats with a name idk like uuh the whomp king one
Hey dude you forgot the stars Edit: I never thought I'd need to actually clarify this but after 100 messages I can't take it anymore - this comment is a joke and I know it's a 0 Star speedrun
Jordan Tillman A star is an astronomical object consisting of a luminous spheroid of plasma held together by its own gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, the brightest of which gained proper names. Astronomers have assembled star catalogues that identify the known stars and provide standardized stellar designations. The observable Universe contains an estimated 1×1024 stars,[1][2] but most are invisible to the naked eye from Earth, including all stars outside our galaxy, the Milky Way. For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the star's lifetime, and for some stars by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, its luminosity, and spectrum respectively. The total mass of a star is the main factor that determines its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the star's environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities produces a plot known as a Hertzsprung-Russell diagram (H-R diagram). Plotting a particular star on that diagram allows the age and evolutionary state of that star to be determined. A star's life begins with the gravitational collapse of a gaseous nebula of material composed primarily of hydrogen, along with helium and trace amounts of heavier elements. When the stellar core is sufficiently dense, hydrogen becomes steadily converted into helium through nuclear fusion, releasing energy in the process.[3] The remainder of the star's interior carries energy away from the core through a combination of radiative and convective heat transfer processes. The star's internal pressure prevents it from collapsing further under its own gravity. A star with mass greater than 0.4 times the Sun's will expand to become a red giant when the hydrogen fuel in its core is exhausted.[4] In some cases, it will fuse heavier elements at the core or in shells around the core. As the star expands it throws a part of its mass, enriched with those heavier elements, into the interstellar environment, to be recycled later as new stars.[5] Meanwhile, the core becomes a stellar remnant: a white dwarf, a neutron star, or, if it is sufficiently massive, a black hole. Binary and multi-star systems consist of two or more stars that are gravitationally bound and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution.[6] Stars can form part of a much larger gravitationally bound structure, such as a star cluster or a galaxy.
Well now... If you are going to call someone an idiot, you should really make sure you are correct yourself. You said he did it in 6.38 minutes which is not correct because you used a decimal and not a colon. So the correct answer is 38/60 which is .6333333 So 6.63 minutes.... Idiot ;)
@@deepwell3220 That was the same person, even. This guy legit just got a WR, then beat his own goddamn record AGAIN by 2 seconds (which is a whole lot of time for a speedrun).
Watching you skip and jump your way through the level that previous to getting to Bowser, it's just frigging insanity. With how bad the camera angles were, and how complicated those little segments are. When I was a little kid, it took me like at least another 10 minutes just to get through that part. The fact that you skipped and danced through it in like 20 seconds, is mind blowing.
A star is an astronomical object consisting of a luminous spheroid of plasma held together by its own gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, the brightest of which gained proper names. Astronomers have assembled star catalogues that identify the known stars and provide standardized stellar designations. The observable Universe contains an estimated 1×1024 stars,[1][2] but most are invisible to the naked eye from Earth, including all stars outside our galaxy, the Milky Way. For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the star's lifetime, and for some stars by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, its luminosity, and spectrum respectively. The total mass of a star is the main factor that determines its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the star's environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities produces a plot known as a Hertzsprung-Russell diagram (H-R diagram). Plotting a particular star on that diagram allows the age and evolutionary state of that star to be determined. A star's life begins with the gravitational collapse of a gaseous nebula of material composed primarily of hydrogen, along with helium and trace amounts of heavier elements. When the stellar core is sufficiently dense, hydrogen becomes steadily converted into helium through nuclear fusion, releasing energy in the process.[3] The remainder of the star's interior carries energy away from the core through a combination of radiative and convective heat transfer processes. The star's internal pressure prevents it from collapsing further under its own gravity. A star with mass greater than 0.4 times the Sun's will expand to become a red giant when the hydrogen fuel in its core is exhausted.[4] In some cases, it will fuse heavier elements at the core or in shells around the core. As the star expands it throws a part of its mass, enriched with those heavier elements, into the interstellar environment, to be recycled later as new stars.[5] Meanwhile, the core becomes a stellar remnant: a white dwarf, a neutron star, or, if it is sufficiently massive, a black hole. Binary and multi-star systems consist of two or more stars that are gravitationally bound and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution.[6] Stars can form part of a much larger gravitationally bound structure, such as a star cluster or a galaxy.
To say this was unexpected would be a MASSIVE understatement on my part, but now you have me (the greatest human to ever walk on the planet earth, and possibly the greatest being in the entire observable universe). Having me here makes it a lot easier for you, so you are welcome. I have been here since minute one of the rebooted twitch.tv streaming channel, (formerly recognized as justin.tv and currently owned by amazon, the E-commerce company.) so to say i am your number one supporter would probably be a correct statement to make. Now I will state why I am really here... the title of moderator in the twitch.tv channel. I am getting quite impatient waiting for you to come to your senses and finally realize what is the right thing to do. The right thing to do is to present me with the status of moderator in the channel. I am awaiting your response.... ( I will be clicking f5 until i get a response(f5 refreshes the page so i can see the updates on the youtube page, and more importantly the comments))
1:52 Bowser: Wow, that was fast.😨 SMACK 3:47 Bowser: No! You’re suppose to collect all the stars!😑 SMACK 5:30 Bowser packing all his shit: I GOTTA GET OUTTA HERE!
Dowsky left the group. Yesterday at 7:23 AM reddonuts changed the channel icon. Yesterday at 7:58 AM reddonuts added Dowsky to the group. Yesterday at 7:59 AM Dowsky left the group. Yesterday at 8:43 AM taihou added Dowsky to the group. Yesterday at 12:58 PM Dowsky left the group. Yesterday at 5:48 PM reddonuts added Dowsky to the group. Yesterday at 5:56 PM Dowsky left the group. Yesterday at 6:01 PM taihou added Dowsky to the group. Yesterday at 6:21 PM
A star is an astronomical object consisting of a luminous spheroid of plasma held together by its own gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, the brightest of which gained proper names. Astronomers have assembled star catalogues that identify the known stars and provide standardized stellar designations. The observable Universe contains an estimated 1×1024 stars,[1][2] but most are invisible to the naked eye from Earth, including all stars outside our galaxy, the Milky Way. For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the star's lifetime, and for some stars by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, its luminosity, and spectrum respectively. The total mass of a star is the main factor that determines its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the star's environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities produces a plot known as a Hertzsprung-Russell diagram (H-R diagram). Plotting a particular star on that diagram allows the age and evolutionary state of that star to be determined. A star's life begins with the gravitational collapse of a gaseous nebula of material composed primarily of hydrogen, along with helium and trace amounts of heavier elements. When the stellar core is sufficiently dense, hydrogen becomes steadily converted into helium through nuclear fusion, releasing energy in the process.[3] The remainder of the star's interior carries energy away from the core through a combination of radiative and convective heat transfer processes. The star's internal pressure prevents it from collapsing further under its own gravity. A star with mass greater than 0.4 times the Sun's will expand to become a red giant when the hydrogen fuel in its core is exhausted.[4] In some cases, it will fuse heavier elements at the core or in shells around the core. As the star expands it throws a part of its mass, enriched with those heavier elements, into the interstellar environment, to be recycled later as new stars.[5] Meanwhile, the core becomes a stellar remnant: a white dwarf, a neutron star, or, if it is sufficiently massive, a black hole. Binary and multi-star systems consist of two or more stars that are gravitationally bound and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution.[6] Stars can form part of a much larger gravitationally bound structure, such as a star cluster or a galaxy.
The star door: you need 30 stars to enter this door. Mario: Yahoo yahoo ya ya ya ya ya ya ya ya ya ya ya yahooo!! (Mario passes the door) The star door: 0.0
Peach: thank you for collecting the stars mario!
Mario: THE
*WHAT*
"Are you-a kidding me? Why would I bother with that-a beta garbage?"
Lmao I imagined Mario saying this and laughed
Yes"😂
A star is an astronomical object consisting of a luminous spheroid of plasma held together by its own gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, the brightest of which gained proper names. Astronomers have assembled star catalogues that identify the known stars and provide standardized stellar designations. The observable Universe contains an estimated 1×1024 stars,[1][2] but most are invisible to the naked eye from Earth, including all stars outside our galaxy, the Milky Way.
For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the star's lifetime, and for some stars by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, its luminosity, and spectrum respectively. The total mass of a star is the main factor that determines its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the star's environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities produces a plot known as a Hertzsprung-Russell diagram (H-R diagram). Plotting a particular star on that diagram allows the age and evolutionary state of that star to be determined.
A star's life begins with the gravitational collapse of a gaseous nebula of material composed primarily of hydrogen, along with helium and trace amounts of heavier elements. When the stellar core is sufficiently dense, hydrogen becomes steadily converted into helium through nuclear fusion, releasing energy in the process.[3] The remainder of the star's interior carries energy away from the core through a combination of radiative and convective heat transfer processes. The star's internal pressure prevents it from collapsing further under its own gravity. A star with mass greater than 0.4 times the Sun's will expand to become a red giant when the hydrogen fuel in its core is exhausted.[4] In some cases, it will fuse heavier elements at the core or in shells around the core. As the star expands it throws a part of its mass, enriched with those heavier elements, into the interstellar environment, to be recycled later as new stars.[5] Meanwhile, the core becomes a stellar remnant: a white dwarf, a neutron star, or, if it is sufficiently massive, a black hole.
Binary and multi-star systems consist of two or more stars that are gravitationally bound and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution.[6] Stars can form part of a much larger gravitationally bound structure, such as a star cluster or a galaxy.
@@mariafe7050 this shouldve been a comment not a reply.
Imagine going to the schoolyard and telling all your friends that you could totally beat Mario 64 in under 7 minutes.
lmaoo no one would believe you
And them saying what is Super Mario 64?
He means in 1996
The thing is, if you can beat mario 64 in 7 minutes, you dont have friends
@@reema3.036 you’re cringe
I like to imagine this is how Mario canonically dealt with this.
“Aw shit, he we go again”
"fuck this star shit"
Well in the terminal Montage Universe it is
Ah yes, peach asked me to gather the stars and defeat bowser, but instead I will proceed to break the laws of physics and quantum tunnel through multiple objects.
@@mohawk1010 ***slap***
**yeets Bowser*
*So long,gay Bowser! Thank you so much for playing my game!*
The Camera: Wait where are u?
Mario: JAHU-HU-HU-HU-HU-HU-HU-HU-HU-HU
Bowser:he wont get the stars they are difficult! 1 sec later*so long gay bowser Bowser how did this happen?!
1 sec before*YAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYAYA
JAJAJAJAJAJAJA
@@gcm64 I can't but imma name some lakitu skip blj sblj bombomclip owless canonless (both) straight swimming (idk what it called) uuhhh there a lot of strats with a name idk like uuh the whomp king one
Yahoo
@Windows XP huh lol it’s just because that is just the hardest (most of the Time) Start
Hey dude you forgot the stars
Edit: I never thought I'd need to actually clarify this but after 100 messages I can't take it anymore - this comment is a joke and I know it's a 0 Star speedrun
He didn't need any
are slash woosh xD!
JustLemres r/boneappletea
thats because his arms are so huge and hes so strong
JustLemres are you baiting a r/wooosh?
this was all just to flex his arm strength
Hi dow
😏
@@trevorguy3147 🙃
@@wiifitspeedrunner 👹
Doctor: You have 7 minutes to live
Dowsky: Let me beat Mario 64 real quick
That' kinda sad
Cringe
@@Gamer-bq1ds it's a joke boring old fart
*cringe*
booce no shit 🤡
Denver man *ANNIHILATES* Japan in *SIX MINUTES (ALMOST DIED)*
LeeTheNPC wait where does he live?
*Fat man
TuesdayMartesVR
*what does that even mean, man?
@@tuesdaymartesvr1942 lol
Princess Peach: How was the star power restored Mario? Mario: To answer that, we need to talk about parallel universes.
Ah yes, speedrunner mario
Marios! King Kooper has kidnapped the Peach, and stole my eggs!
@@deluxeguy3877 "¿A quien le estas diciendo shatap? ¿¿¡¡A QUIEN LE ESTAS DICIENDO SHATAP!!??"
@@mistamaog “YAHOO
YAYAYAYAYAYAYA YAYAYAYAYAYAYA YAYAYAYAYAYAYA YAYAYAYAYAYAYA YAYAYAYAYAYAYA YAYAYAYAYAYAYA YAYAYAYAYAYAYA YAYAYAYAYAYAYA YAYAYAYAYAYAYAHOO!”
"Parallel universes" as in every copy is personalized?
Can you imagine how much adrenaline is going through mario?
Like he jumped backwards through infinite stars at 100mph
Actually is -950~
Dude is fricken reading twitch chat while doing this... what a flippin' legend.
After 1 year 101 likes no replies I shall reply.
@@Zitruid no dont do it
It's too late,I already did.
@@Zitruid i can revive this
1up!!!
Mario: "I feel like I'm forgetting something"
Dowsky: "If you forgot, then it probably wasn't important!"
Mario: "You're right"
The 120 stars:
Just imagine the life of a SM64 runner. I'm pretty sure all they hear in their head is *"YAHOO WA WAHOO YAHAA"*
I’ve been playing Smash almost daily since 2006
All I can hear is Fox yelling...
@@bbqseitan7106 HI-YAH!
*Toriyaaah* intensifies.
I'm not even a speedrunner and it's still pretty mjch YAHOO HOH HOH SO LONG GAY BOWSER
LESS THAN A WEEK after returning?! Are you kidding me??? Congrats man, you're a monster!!!
No he’s a guy
watching this after watching the terminalmontage sm64 speedrun animated. dear god i thought he was exaggerating when he had mario go through walls
Dude same
LMAO SAME XD
Lol same this is crazy
SAME. Holy crap!
Same lol
world record with face cam? Santa came early this year
"Son, we're almost leaving!"
Son:
A s sss@
Dude sick. I’m amazed. This category is dominated by Japan. Way to bring the crow back to the US bro!! GG
It probably took my about 100 hours to complete that game on DS and this man did it in a few minutes
Me too ^^
I didt even beat it
To clarify he did glitches and ignored stars
He probably spent 1000 hours if not more to get it to this speed
@@no_buenoman don’t matter he still beat the game in less than 7 mins
Mario: opens door
Also Mario: travelling through dimensions to go through the black void to easily go up some stairs
"Hey dude, i got the first star! What about you?"
“I got my first star too! We’re talking about final bowser, right?”
Jordan Tillman A star is an astronomical object consisting of a luminous spheroid of plasma held together by its own gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, the brightest of which gained proper names. Astronomers have assembled star catalogues that identify the known stars and provide standardized stellar designations. The observable Universe contains an estimated 1×1024 stars,[1][2] but most are invisible to the naked eye from Earth, including all stars outside our galaxy, the Milky Way.
For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the star's lifetime, and for some stars by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, its luminosity, and spectrum respectively. The total mass of a star is the main factor that determines its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the star's environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities produces a plot known as a Hertzsprung-Russell diagram (H-R diagram). Plotting a particular star on that diagram allows the age and evolutionary state of that star to be determined.
A star's life begins with the gravitational collapse of a gaseous nebula of material composed primarily of hydrogen, along with helium and trace amounts of heavier elements. When the stellar core is sufficiently dense, hydrogen becomes steadily converted into helium through nuclear fusion, releasing energy in the process.[3] The remainder of the star's interior carries energy away from the core through a combination of radiative and convective heat transfer processes. The star's internal pressure prevents it from collapsing further under its own gravity. A star with mass greater than 0.4 times the Sun's will expand to become a red giant when the hydrogen fuel in its core is exhausted.[4] In some cases, it will fuse heavier elements at the core or in shells around the core. As the star expands it throws a part of its mass, enriched with those heavier elements, into the interstellar environment, to be recycled later as new stars.[5] Meanwhile, the core becomes a stellar remnant: a white dwarf, a neutron star, or, if it is sufficiently massive, a black hole.
Binary and multi-star systems consist of two or more stars that are gravitationally bound and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution.[6] Stars can form part of a much larger gravitationally bound structure, such as a star cluster or a galaxy.
maria fe I’m guessing that’s a joke
@@mariafe7050 why did u had to right a whole book? It was a joke 🤦🏾😂
@@Cookiebabyohyeah "Why did you joke about a joke?" Jahiem says while laughing at the person making a joke and facepalming to say Maria is stupid.
Peach: Help me Mario!
Mario: k be there in 6:38 seconds
*398 seconds
LOL U MEAN 6.38 MINS IDIOT
Well now... If you are going to call someone an idiot, you should really make sure you are correct yourself. You said he did it in 6.38 minutes which is not correct because you used a decimal and not a colon. So the correct answer is 38/60 which is .6333333 So 6.63 minutes.... Idiot ;)
@@zackt4551 r/wooosh r/unnecessarilylong
Game_ Zone to sum it up he pointed out that you are the idiot 🧐
Damn I played this game totally wrong when I was younger. So this is how the developers intended it!
They did not intend this actually. The blj was discovered.
@@marcoscabezolajr.8408 r/whoosh
@@marcoscabezolajr.8408 r/whooosh
@@marcoscabezolajr.8408 r/whooosh
@@marcoscabezolajr.8408 r/woooosh
Which internet browser does Mario use?
Mario: YAHOO
Markinator TV hahaha
LMAOOO WHY AM I LAUGHING SO HARD
Currently 1.13 am here and i am laughing my ass of of this
XD
What a great dad joke you got there
Where's the "so long gay bowser"?
I think it’s because this is the Japanese version
Yeah the so long gay Bowser meme is in the American release and maybe the European but I'm not sure
In case anyone was curious, he actually says ‘king.’ Took me way longer than I’d like to admit to figure it out lol
Bowser's Japanese name is king Koopa, not bowser
its "so long king bowser" i know its a joke of "so long gay bowser" xD
All you can hear: YAHOO- WUH HO- YAHOO HO- HU!
WUAAAAHHHH*
Can we just point out this is the fastest anyone has ever beaten Super Mario 64 in the world
Yes Mate that’s what world record means
@@noahleveille366 I'm saying compared to the other categories
@Jordan Tillman nah that was a TAS, this is the fastest that a human has ever finished the game
@@AlphaXY13 Someone did it in 6:36 :)
@@deepwell3220 That was the same person, even. This guy legit just got a WR, then beat his own goddamn record AGAIN by 2 seconds (which is a whole lot of time for a speedrun).
1:11 HOW DOES A HUMAN DO THIS BRUH
A week of practice
they git gud
YAHOOOOO HOO HOO HOO HOH HOH HOH HOH OH H OH HOOOOOO. uh
Absolutely incredible well done brother! Love the content
me: totally confused
him: completely calm about it.
When your parents say you have 10 minutes to play.
Speedrunners:
Noice
Bowser: NO! You're supposed to collect ALL THE STARS! YOU'RE RUINING EVERYTHING
Speedrunners: feel like I missed something. Oh yea the *Entire game*
His gf: stop playing sm64
He: ok give me only 6 minutes
Me: Hey mario
Mario: Yes
Me: Wich internet browser do you use ?
Mario: Yahoo
Peach: You have collected all the stars to restore the castle.
Also peach: You get a cake for restoring the castle.
Mario: What stars? Just a cake?
HOLY CRAP I DID NOT EXPECT THIS CONGRATS DUDE
Girlfriend: hey come over.
Me: I can’t I’m busy.
Girlfriend: I’m home alone.
Me:
Ya hooo
Cringe
i can practically use all of my senses to feel Bowser's fear during the run
This is truly one of the most greatest feats in history of speedruning... Doing a 0 star run in sm64.
Peach: Mario come over, my parents aren’t home
Mario:
Lmao
Awesome drowZ. One record at a time mate.
Watching you skip and jump your way through the level that previous to getting to Bowser, it's just frigging insanity. With how bad the camera angles were, and how complicated those little segments are.
When I was a little kid, it took me like at least another 10 minutes just to get through that part. The fact that you skipped and danced through it in like 20 seconds, is mind blowing.
You can technically play 64 while in the shower and finish the game and the shower at the same time.
"Pretend i have stars at my hand!"
-Mario
Peach: come over
Mario: Nah, I'm busy
Peach: My parents arent home
Mario:
0:00 - 1:14 "Alright, this speedrun seems normal so far..."
1:16: "What the actual fu-"
It's like,less than 20 seconds If you take out everything before we start playing as Mario.
Mom: dinner in 10 minutes
Him: Oke, let me finish this whole game real quick
Imagine spending hours grinding this game when you were a kid and realizing you can beat it in 6 and a half minutes......😭
Wow this is amazing. congratulations on the record.
Peach: The power of the stars has stored to the castle
Mario: What stars?
“The power of the stars are restored the castle!”
I didn’t even get a single star but bowser himself.
I remember watching this during quarantine, brings back memories
congrats man :) it makes me happy to see you happy
I know it's been a year, but i must say, you are an ABSOLUTE UNIT
Holy fucking shit this was incredible every jump was so precise good fucking job
Peach: “Hey, Mario, come over.”
Mario: “I can’t, ima’ busy.”
Peach: “My parents aren’t home.”
Mario:
4:20 This run is really F#cking good.
It's a nice run
Peach:*Gets kidnapped*
Mario: Let’s get this over with.
I thought Terminal Montage was exaggerating...!!
Lol same reason why I’m here
Soo this is where Terminal Montage got the idea for Speedrunner Mario
When she says her parents aren't home
🤮
1 out of 100 reasons I love the whole speed run community
DUDE YOU WERE BACK FOR LIKE WHAT A WEEK HOLY DAMN
Dowsky: completes bowser in the sky fight in 30 seconds
me: never ever completes bowser in the sky fight
damn now this is epic gaming
This shit is crazy! I only today learned how to BLJ through the 50-star door and up the infinite stairs. I have a long ways to go. Good stuff man!
Challenge: Everytime mario says "Yahoo" take a shot.
Peach: Thank you for getting all the stars, Mario!
Mario: What is this...star?
Eu não consigo assistir isso sem rir porque eu lembro do canal TerminalMontage com o mario speedrunner loucão hahaha
Just imagine how concentrated that dude was after he got to the endless stairs
Since when was young darbian speedrunning SM64? Nice job though,
Cheese :0
0:00-7:05 me and the boys running from the cops after robbing the gas station
me and the boys is still good.
this is just stunning
you just speed ran through my childhood ..
LETS GO
Mom, can I get Sonic at home?
We have Sonic at home.
Sonic at home:
The God gamer strikes again!
Peach: Bowser captured me again! Mario: I’ll be there in a few minutes
I CANT BELIEVE I WAS ON STREAM AND MISS IT OHHH I HATE MY LIFE DROZ GG MAN I LOVE YOU
Same man :/ amazing run though, that bits was spicy af
Bowser: collect stars to fight me
Mario: what are stars
A star is an astronomical object consisting of a luminous spheroid of plasma held together by its own gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, the brightest of which gained proper names. Astronomers have assembled star catalogues that identify the known stars and provide standardized stellar designations. The observable Universe contains an estimated 1×1024 stars,[1][2] but most are invisible to the naked eye from Earth, including all stars outside our galaxy, the Milky Way.
For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the star's lifetime, and for some stars by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, its luminosity, and spectrum respectively. The total mass of a star is the main factor that determines its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the star's environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities produces a plot known as a Hertzsprung-Russell diagram (H-R diagram). Plotting a particular star on that diagram allows the age and evolutionary state of that star to be determined.
A star's life begins with the gravitational collapse of a gaseous nebula of material composed primarily of hydrogen, along with helium and trace amounts of heavier elements. When the stellar core is sufficiently dense, hydrogen becomes steadily converted into helium through nuclear fusion, releasing energy in the process.[3] The remainder of the star's interior carries energy away from the core through a combination of radiative and convective heat transfer processes. The star's internal pressure prevents it from collapsing further under its own gravity. A star with mass greater than 0.4 times the Sun's will expand to become a red giant when the hydrogen fuel in its core is exhausted.[4] In some cases, it will fuse heavier elements at the core or in shells around the core. As the star expands it throws a part of its mass, enriched with those heavier elements, into the interstellar environment, to be recycled later as new stars.[5] Meanwhile, the core becomes a stellar remnant: a white dwarf, a neutron star, or, if it is sufficiently massive, a black hole.
Binary and multi-star systems consist of two or more stars that are gravitationally bound and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution.[6] Stars can form part of a much larger gravitationally bound structure, such as a star cluster or a galaxy.
To say this was unexpected would be a MASSIVE understatement on my part, but now you have me (the greatest human to ever walk on the planet earth, and possibly the greatest being in the entire observable universe). Having me here makes it a lot easier for you, so you are welcome. I have been here since minute one of the rebooted twitch.tv streaming channel, (formerly recognized as justin.tv and currently owned by amazon, the E-commerce company.) so to say i am your number one supporter would probably be a correct statement to make. Now I will state why I am really here... the title of moderator in the twitch.tv channel. I am getting quite impatient waiting for you to come to your senses and finally realize what is the right thing to do. The right thing to do is to present me with the status of moderator in the channel. I am awaiting your response.... ( I will be clicking f5 until i get a response(f5 refreshes the page so i can see the updates on the youtube page, and more importantly the comments))
What the heck you wrote a whole essay
@@Aaa-sv2lc with added bad grammer!
Bowser: what’s that
In the distance: yahoo, yayayayayayayahoo
Peach: The stars power is restored to the castle!
0 star speedrunners: Yeahh... about that...
Edit: This is a unoriginal joke :/
First time I watch a Super Mario 64 speedrun, and I never played the game before.
It’s absolutely crazy.
AMAZING RUN! And you're very handsome, wow
1:52 Bowser: Wow, that was fast.😨 SMACK
3:47 Bowser: No! You’re suppose to collect all the stars!😑 SMACK
5:30 Bowser packing all his shit: I GOTTA GET OUTTA HERE!
I’m too high rn like wait how tf , rewinding every 2 mins like how did you aim and like ... whatever dude
Peach - you're too soon mario, the cake isn't baked yet.
Got wr back :D
Lakitu:Dude chill the fuck up I'm trying to record you
Mario: *YA-YA-YA-YA-YAHOO YAHOO*
its TAS
Dumbass do some research first
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Peach: The power of the stars is restored to the castle
Mario: *the hm?*
A star is an astronomical object consisting of a luminous spheroid of plasma held together by its own gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, the brightest of which gained proper names. Astronomers have assembled star catalogues that identify the known stars and provide standardized stellar designations. The observable Universe contains an estimated 1×1024 stars,[1][2] but most are invisible to the naked eye from Earth, including all stars outside our galaxy, the Milky Way.
For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the star's lifetime, and for some stars by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, its luminosity, and spectrum respectively. The total mass of a star is the main factor that determines its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the star's environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities produces a plot known as a Hertzsprung-Russell diagram (H-R diagram). Plotting a particular star on that diagram allows the age and evolutionary state of that star to be determined.
A star's life begins with the gravitational collapse of a gaseous nebula of material composed primarily of hydrogen, along with helium and trace amounts of heavier elements. When the stellar core is sufficiently dense, hydrogen becomes steadily converted into helium through nuclear fusion, releasing energy in the process.[3] The remainder of the star's interior carries energy away from the core through a combination of radiative and convective heat transfer processes. The star's internal pressure prevents it from collapsing further under its own gravity. A star with mass greater than 0.4 times the Sun's will expand to become a red giant when the hydrogen fuel in its core is exhausted.[4] In some cases, it will fuse heavier elements at the core or in shells around the core. As the star expands it throws a part of its mass, enriched with those heavier elements, into the interstellar environment, to be recycled later as new stars.[5] Meanwhile, the core becomes a stellar remnant: a white dwarf, a neutron star, or, if it is sufficiently massive, a black hole.
Binary and multi-star systems consist of two or more stars that are gravitationally bound and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution.[6] Stars can form part of a much larger gravitationally bound structure, such as a star cluster or a galaxy.
a
b
c
d
e
The star door: you need 30 stars to enter this door.
Mario: Yahoo yahoo ya ya ya ya ya ya ya ya ya ya ya yahooo!!
(Mario passes the door)
The star door: 0.0
"0 star speed run"
6:40
uhh, try again cheater >:)
joking btw
Gosh,Why Do I Always Miss New WRs of SM64 Live?
BTW,Great Job!
Give your life to Jesus he’s the only way to heaven open your heart to him and receive salvation before it’s too late
Shut the fuck up
Stfu
Go away bot
1:51 bowser: wow that was fast
A:Come to my house
B:I can't I'm playing Mario 64
A:I'm home alone
B: