So i had an idea: after all star types have been covered maybe there should be a popup like "new types unlocked". Those would be L and T brown dwarves or you could throw on a hypothetical Ω type star wich isn't technically a star since instead of fusing hydrogen it feeds a black hole in the center wich spews out enough energy to keep the star from collapsing. It's difrent forces but with the same effect as regular fusion in the core of a star.
You should do a quasi star, they are basically stars that were born when the universe was still young and they have a black hole at their center. And not to mention, they are hecking big, bigger than stephenson 2-18
the editing and style of this video is one of the best, i love how the planets chat with themselves, though i wished the star had participated more. but the best part for sure was the inside of the star
I think part of the reason Gas Giants tend to form has to do with the whole binary+ pairs things being fairly common in the universe. They probably wind up not having enough material to become the binary partner star or even a brown dwarf in most cases. Well, it's either that or objects simply obtain as much mass as they can.
There should be a remake of this with a bigger planetary system As the red dwarf starts heating up towards the end of its life, planets further out would become habitable.
TIMELINE 0:29 Proto star forms 0:47 Proto Planets form 0:50 The gas giant, Alpina forms 0:51 The Rocky planets, Honga, Carol, Jafo and Pijo forms 0:52 Pijo impacts pajo 0:57 The impact creates an asteroid belt, Alpina gets thin rings 1:01 Honga moves outerward due to Alpina's gravity 1:07 The asteroid belt goes crazy and creates a late heavy bombardement 1:10 Late heavy bombardment ends 1:11 Water on Honga and Carol, they also got continents and a thicker atmosphere 1:16 Honga's and Carol's Rotation becomes chaotic 1:26 The star throws a massive solar flare 1:42 Carol's core freezes and its magnetic field dies 1:47 Carol freezes 2:07 Another massive solar flare 2:16 Honga suffers a runaway greenhouse effect 2:32 Alpina captures a rouge moon, its named Ginlo 2:39 Ginlo got a surface similar to Titan's surface 2:50 Galaxy colision 2:57 Honga looses it's magnetic field 3:01 Honga's atmosphere has been stripped away by the solar wind 3:20 A red dwarf passes by and ejects Alpina out the system 3:34 A civilization passes by and terraforms Carol 3:46 As Carol doesn't have a thick atmosphere, the water will freeze 3:56 All Carol's water freezes 4:26 A rouge gas giant enters the system 4:36 The star pulls the gas giant into it, the gas giant is destroyed, the gas giant gravity disturbed the rocky planets orbit, Honga is almost ejected and Carol almost collides with the star 4:49 Helium fusion begins 4:58 The star runs out of Hydrogen 5:09 Star begins red giant phase 5:29 The star becomes white and begins to shrink 5:34 The star starts to become a blue dwarf 5:38 The star isnt strong enough to burn Helium 5:52 The star has died 5:55 The star becomes a 🔵 dwarf 6:10 The star cools down 6:20 The universe fade 6:21 Honga and Carol have been eaten by a black hole, or dragged tothe star due to gravitational radiation 6:30 The end :)
Hello! Would be nice if you also showed the habitable zone! By the way your channel is insane, thank you, now I can't even stop watching your channel! Liked all of your videos!
0:27 a piece of nebula collapse on to its self 0:38 a proto star forms 0:47 proto planets form 0:53 planets form. Two proto collide and made an asteroid belt 1:09 a and b gets hit by asteroids. The asteroid belt is gone 1:45 b can't spin properly 2:13 a gets hit by solar flares 2:18 a doesn't has water anymore 2:39 c's biggest moon forms 2:56 a can't spin properly 3:00 a gets it's water back 3:19 c gets dragged away from the system from a star 3:31 B's ice melts 4:00 universe fades 4:44 the star starts to hack 4:59 star low hydrogen 5:26 star can't burn helium 5:54 star dies THE END
@@zachbowles4516 dunno where it is but as far as im aware it has a rather small sample size of 4,so take it with a grain of salt until its fully confirmed
@@Atula416the Titan-like moon: even worse , step father's dead , and now i have to face this evil cherry right in front of me My time has come , bye cruel universe [After the Titan-like moon said its last words ,the ultimate cherry had nommed it whole evaporating the small celestial body that could have lived forever till proton decay]
This always happens to me lol When I'm playing 0:08 error And the most painful part is when ur volume is maxed out and your mom will be awake and your ded lol
Stats for today’s star Star Type: M (red dwarf) Mass: 0.096 solar mass Lifespan: 1 trillion years or more Benefits and downsides of living in a red dwarf star system: Benefits: 1. The star has a very long lifespan, giving intelligent civilization enough time to evolve into an interstellar species 2. Very common in the universe Downsides: 1. Planets are prone to solar storms 2. Planets may be tidally locked, with one side facing the star, while the other face away from the sun. Habitability is unlikely depending on the planet’s atmosphere
It's incredible how you can make something this good on powerpoint! (honestly, I couldn't do it bcse i dunno how to make and even if I knew, I'm too lazy)🙃
@@himedo1512 Nope, big blue stars can only use the fuel in the core, but red dwarves have convection that circulates hydrogen from the core to the surface, so it is a lot more efficient
@@kerbodynamicx472 according to universe today redwarves will produce as little as 1/ 10,000th the energy of just a star the size of our sun in their lifetime. You are wrong.
The star HD 140283 is a subgiant star with an estimated age of 14.46 billion years. That might raise an eyebrow or two for those of you who remember that the age of the universe is estimated as 13.77 billion years.
They burn it very slowly--this star was listed as having two thousand times lower luminosity than our sun, and eleven times less mass. That would allow it to burn for several hundred times longer than our sun.
@@cycrothelargeplanet well if helium got ejected from the star and hydrogen fell into the star at the same time then it will live for like 600 trillion years
So G'damn well done I just can't say it loud enough! 😍 If the timeline in this video was to the same scale as the F star video, it would have to be at least 17 hours long! Edit: 6.4 days! I only figured a trillion years!
@@gamers-xh3uc Nah, look at the O star. Once you get to helium burning, you have like 1% longer to live. Then Carbon burning less than a thousand years, neon and magnesium a few years, oxygen a few months and silicon less than a day. After carbon burning starts, the star has less time to live than when the middle Ages happened.
The fact that even a red dwarf's absolute brightest and hottest moment still only produces 1/3 of Solar's luminosity is pretty insane. Just shows you how truly dim red dwarfs are compared to even our dwarf of a star
Ideas: Timeline of other star systems Future of the Solar System but with Humans How to: Planets More timelines (by the far future) Collabs (more ideas soon)
Nah not really, its is very mich expectwd gliesse 710 will pass through the ort cloud and at much it could eject dwarf planets out of suns gravitati9nal influences or throw them and some asteroids to the inner solar sistem at the very much it could affect a bit the orbit of Neptune or maybe even uranus but nothing closer to the sun.
