Timeline of an L-type Brown Dwarf System - Planetball
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- Опубліковано 18 вер 2024
- This is an animation.
Info source: kurzgesagt.fan...
[PSR Series]Timeline of an L-type Star - Planetball
This is about the evolution of a high mass brown dwarf(Mass is 0.06x Sun) and its planets.
You can go to en.m.wikipedia... to learn about what is “L-type”
Music used:
Kevin MacLeod - Garden Music
25 is a good number, because it is 5^2.
Planetballs are basically same to polandballs, the only difference is the character, not countries, but space objects including stars, planets, moons and even galaxies.
1:35 it's Trillion and not Tillion...
well I can't change it anymore
Atleast he's using 1 trillion and not 1000 billion
@Lionel Matthew Colin Tamunu well i mean he did sirius but idk about canopus
@@AstroCatz why are likes disabled?!
Opps DogePro Wrong something UWU
_"Brown dwarfs are like a glowy gas gaint."_
"and a huge dissipointment to their moms"
Nice kurzgesagt reference
Y E S
@@Your_DoorYT "Things that would LIKE to be stars" man, that whole part was just one sick burn to brown dwarfs. :P
its nice knowing that im not the only one in this comment section to make a kurzgesagt reference, also my comment is 4 minutes less older than the video, and i didn't realize there was this comment, so don't say i copied from one of you, especially @chandra
*Timline*
*Starting system.*
0:20 Brown dwarf forming.
0:26 B c and I (the moon) form.
0:28 I has liquid water due to tidal heating.
0:34 Fusion stops in the brown dwarf.
0:57 I's oceans freeze over.
1:00 - 1:50 Nothing happens.
1:54 All the planets are lost most likely due to an interstellar encounter.
2:08 The brown dwarf fades away due to proton decay?
*End.*
Proton decay is rare ,so i think the burgundy dwarf vanishing is responsible to the white dot at the ending (probrally a neutron star
@@iapetus6110 that was a white hole that wanted it going: BYE BYE IM GOING TO THE WEST
Does proton really decay?
@@cl9408 short answer, we don't know. Long answer, if they do then it'd be long after the only thing in the universe are black holes, this brown dwarf would have collided with something else to birth a new star long before its protons would have decayed.
@@cl9408 idk maybe later when universe expansion reach the light speed
Imagine a civilization around this star.
Planets in the habitable zone around a red dwarf are tidal locked.
Edit: same for brown dwarfs
@@Kalidor99 hmm, that would make an interesting world, half burnt to a crisp, half ice world, but a thin strip of habitable land around the sunset zones. The habitable areas would be in a state of permanent sunset, would honestly look pretty cool
If Civilization able to Evolve around Hotter and Younger Massive Brown Dwarfs (since there's nothing Impossible for Life to exists) they must Leave immediately before the Browndwarf's Deuterium Fusion stops assuming like Humans if they dont kill each other in Nuclear War
@@Kalidor99 not for brown dwarfs , plus how do you know that
@@iapetus6110 gravity from a close distance from an object 80 times more massive than Jupiter would tidally lock it.
Actually there is a lecture explaining that Brown dwarfs below 75 Mjup cool down to Y type in less than 20 Gyr. (Brown Dwarfs Substellar, low-mass stars - Dominic Goodman) - thought could be useful.
According to it:
Your typical 60 Mjup BD would take about 9 Gyr to do so.
A +75 Mjup BD cools down and shrinks enough to ignite hydrogen fusion by 5 Gyr at least 2000 K temperature.
Hmm
Neat
There are 90-100 MJ brown dwarfs that do not ignite sustained hydrogen fusion but have an unsteady form of it. They cool down. a 90 MJ brown dwarfs 10 Gyr old is now (if I rememebr correctl) 2400 K in temperature and is expected to cool down by about 100K/Gyr.
(+75 Mjup) OMG I did not know that! (I know a lot about space, not everything, but I never thought I would learn this!)
@@evanderminecraft738180 Jupiter masses or higher forms a red dwarf.
@@WinVisten not always that is true for solar metallicity but at little to no metallicity it an be around 100 MJ
proto star:I’m gonna be a M ty-*turns into L type brown dwarf*
*realizes that there are stars that end up faling into L type*
*a jupiter-mass object hits the dwarf*
*proceeds to become L-Type star*
@@yellowmegablocksdogs4569 I'll assume you meant the failed L dwarfs and not the lucky ones
@@dawnsclim4382 i mean the lucky ones
Well L , T , and Y types live forever just like planets and moons ,the proto star should be glad
@@iapetus6110 no, they will eventually get vored by something with more mass
0:25 L
1:13 T
1:53 Y
Ah yes I should put the temperature in the bottom left corner next time!
Yay
When star is red is was cool 🔴
When star is white or blue is was hot ⚪️🔵
When star was orange and yellow is was normal 🌞
Nice try jadz ห่ะ
5555
@@kumpunmobile12205555
0:08 DogePro as Undyne: SCREW IT! Why should I do an intro for this video, because I won't have it anyways! NGAAHHH!!!
funny
lol
I though the 2 Brown Dwarf Were gonna collides and form a Little Red Dwarf 1:36
I will do it in T or Y
Three different -ways to die- endings
@@AstroCatz ⁰‐⁰ Seems epic
I can imagine the rocky planet yeeted straight into the gas giant ,leaving the only moon in this system traumatized till Celestial decay
@@AstroCatz what
i love how they used "L type" for failed stars
And "W type" for the largest stars
@pfftthinkpizza4144
The brown dwarf types are L-T-Y
Fun fact some very small red dwarfs such as Trappist-1, are also classified as L-type stars
Actually trappist-1 is an spectral type M8V Not An L type some can be M9.5V
TRAPPIST-1 isn't, but yes, there's some ultra-low mass red dwarfs that are very early L type. So techincally there are brown dwarf stars.
I love how the moon just smiles through all this
Life 😭😭😭
also, you mixed up the thermochemical reactions inside the brown dwarf, it would take approx 2 trillon years to exit dueterium fusion phase, and another 25 billion or so to run out of hydrgen isotpes for tritium fusion
After reaction ceases it still has to do the slow process of radiating heat
@@dawnsclim4382 this is true
Nerd
@@SouthSudanCountry Yes.
brown dwarfs are cool ngl
true
Yea like j1407b
@@npckevvo yeah the planet with the biggest rings that we know of
@@bitchesa I know it’s so cool he should make a video about that planet
I think you should do a whole bunch of different types of binary stars with planets, that would be really cool (especially if it involved a black hole)
I've always wandered what'd happen if an M-type and G-type star were in a close binary.
The g-type would go red giant, but the M-type would absorb all of the outer layers by tidally leeching it, but from there I don't really know what happens to the G/M type star beyond that point.
@@deltainfinium869 How close are we talking? Within an AU? Within the orbit of Mercury?
If we're talking within the orbit of mercury or so, the two stars would collide long before the primary's red giant phase due to chromospheric drag, which decelerates the stars over time and is the same mechanism by which the earth will likely fall into the Sun at the peak of it's red giant phase. Hence a slightly bigger star is formed which then behaves as a solitary star.
If they are far enough away from each other for this not to happen in the pre-red giant lifetime of the primary (at least 11 billion years), the primary leaves the main sequence and begins expanding, and once it reaches the roche lobe of the secondary M star, it begins feeding the secondary, gradually losing its own mass. In this case, it probably won't lose enough mass to cease fusion altogether. Instead the once-primary will eventually go through it's truncated red giant phase and collapse into a helium white dwarf. If the secondary didn't accrete enough mass to leave the main sequence earlier, it eventually falls into the roche lobe of the white dwarf, being torn apart and consumed, leaving the system contained within a solitary object. If it somehow does live long enough to leave the main sequence and begin evolving into a red giant, it will meet the same fate as the primary, having its mass eaten away by the white dwarf. The white dwarf may undergo occasional nova events, but is not in danger of going supernova, as it will not be massive enough to do so. After some time, the secondary either ends its life and collapses into a white dwarf or loses so much mass to the white dwarf primary that it ceases fusion altogether and devolves into a brown dwarf-like object, often dubbed a 'helium planet' as it is likely to consist of almost pure helium. Here, the two scenarios converge into one, as the ultimate fate for this system is to spiral into itself and merge into a single white dwarf. The end result is likely a high-mass helium white dwarf, perhaps around the mass of the present day Sirius B. The components are too light to produce white dwarfs that could one day accrete enough mass or collide to form neutron stars or type Ia supernovae.
Most white dwarf-star binaries are currently higher-mass stars and don't often involve intermediate or low mass stars, due to how long they take to begin evolving. As the universe gets older, more of these systems will be formed and new types of white dwarfs, such as high-mass helium dwarfs, will form that don't exist yet. The universe is very young still and the vast majority of all stars that have ever been born are still alive. The smallest stars that could have possibly left the main sequence by now are around 95% the mass of the Sun, and the smallest stars that could have died are perhaps very slightly less massive than the Sun, although we don't think intermediate mass stars formed until the Universe was over 1 billion years old, so it's likely that no Sun mass star has died yet, and the smallest star to die is around the mass of Alpha Centauri A at best. This least massive star to die might be considerably more massive than this considering metal-poor stars take longer to evolve and die than Pop I stars like the Sun.
@@cryoraptora303tm2 Man i didn't expect someone to actually respond! Thank you, this did correct some misconceptions i had about such systems, but man. Its kinda interesting how mass siphens back and forth as the system ages :P
@@deltainfinium869 you can research about Algol Binary star System..
It was composed of Orange Subgiant and a Blur Giant star orbiting so close to each other
It was assumed that the Orange Subgiant Stat Algol B was once a Massive Blue Giant Star that Evolved to Red Giant however its companion a Yellow Dwarf like our Sun (which is now a Blur giant) sucks much of the Outer layers of its Evolved companion Algol B and it losses half of its mass now it downgraded to Subgiant and the Sun like star upgraded to Blue giant
love the videos mate! from New Zealand!
|･ω･` )
@@AstroCatz OwO
:]
ok
I think the white dot at the end is a neutron star ,whitch is probrally responsible to the part where the 2 planets and the icy moon got thrown out of nowhere
I didn’t know brown dwarfs last that long. Thanks for showing!
Brown dwarfs live so much longer than other star types
Actually they are eternal
What program are you using for making this animations?
I am 1st to 👍you
The more and more I watch your videos the more and more I want to somehow help.
Besides that though,
Dude, really man, I can only beg you for a discord server.
Or a planetball discord server ,since he makes that type of videos
@@iapetus6110 Exactly, yes!
@@overshocklifts then i hope the mods wont be one of the stereotypical ones that can also be a simp to anime characters ,lol
Pfft, now that would depend on what DogePro would select as his mods.
@@overshocklifts it better not be one of the mods addicted to rule 34 , those stereotypes are usually cringe , not to mention they love young lolis.. , disgusting
Ik you would say ''we can beat our meat to the usual normal ones though'', but this is about planetball ,not fetish
Bro,Your videos are amazing,And Imaginating you do the animations in flipaclip or Somerhing Simillar you Have Taken Hours To do this!😳✴
The intro killed me
Umm now I put the universe in a simulation I hope nothing bad happens
A brown dwarf is almost like a succeeding star, so it’s a very hot gas giant. For example: Wolf 359.
But they are disappointments
1:11 Star starts cooling down for real
1:39 Rings dissappear completely
1:57 Planet leave the steyem
2:13 Star gets eaten
2:18 (end) Video ends
Wdym stars got eaten? you meant eaten by a black hole or proton decay?
@@Noobgrunt a white dwarf rolled around and went “yummy” to all the star’s gas
@@okavara3833 my guy , the brown dwarf evaporated like a comet , not sucked up
@@iapetus6110 oh. So it did get blown away. First time I watched it was hard to tell what was going on because the end cards were covering everything
Why are they so cute to me?
0:28 Old Sun, Saturn, Earth Without Topical Caps and Hot Moon?
Dude ,there is a bunch of solar systems ,not just ours ,also this is not our solar system ,our sun is a G-type you ugly mistake.
this is not the solar system..
Well done dogepro you have 8,500 subs
i didn't know brown dwarfs are stars, i thought they are ''a failed star that is a huge disappointment to their mums'' - kurzgesagt, i ment a gas giant planet
Yea I just noticed that I should change the title
LMAO
I personally think they are stars That dont ignite
What about M-type brown dwarf
Example: Teide 1
It's sad how everything ends eventually.
Can Brown dwarfs die?
Celestial decay , black holes ,Neutron stars , collision course with another object ,And even more ways
Drew a brown dwarf system im my sophmore geometry class because i was bored
Fun fact: instead of burning the kind of hydrogen that main sequence stars do(1 proton,1 electron), brown dwarves burn deuteriumic hydrogen(1 proton, 1 neutron, 1 electron)
At 1:37 you can see a little planet at the top of the screen
It a brown dwarf
Poor L type brown dwarf :(
don't have enough mass to turn into a star..
@Lionel Matthew Colin Tamunu u mean hydrogen!
spectral type L is not a Brown Dwarf, nor is it a Red Dwarf, It is something between the two because , in this type there are both brown Dwarfs and Red Dwarfs, that makes me think it's not a Brown Dwarf , Brown Dwarfs are the spectral type of T and Y types, I like to call these objects the Scarlet Dwarfs , or Burgundy Dwarfs because, like the Brown Dwarfs, they are neither stars nor planets, nor are Widom L-type Objects, nor are they stars or brown dwarfs. (some are stars (;)
L is between 1500K~2700K
I think this should be for bodies with 70-80J mass(red and brown dwarfs)
@@AstroCatz according to Wikipedia, they are objects sometimes like this, sometimes like the coldest Brown Dwarfs, the warmest Red Dwarfs, For me they should just be a different object, For the sake of curiosity, the smallest known star is of the L type , and the Biggest Brown Dwarf is in this type (:, plus there is another reason why it should be a different type (or star) than the only one of the Brown Dwarfs, Turns Hydrogen into Helium, Because Brown Dwarfs No, (they are heated by the mass) so. The Scarlet Dwarfs!
Maroon
@@iapetus6110 Maroon dwarf? I think so too .
@@birb2330 yea ,speaking of colors my fav is turquoise , i even made a paint of it and it matches with the picture of the color
I also like it's code
one thing to think, the gas giant moon. could have tidal heating and be massive enough to have a good atmosphere. and tidal heating could be enough to keep it warm. if its enough tidal heating
Fact: L0 - L2.5 -type stars could actually be red dwarfs
It not red dwarf it maroon dwarf
Idea Timeline Of A Binary/Trinary system idk what type stars tho maybe a binary of K-type and T-type?Cool vid but its kinda sad how short brown dwarfs live
like alpha centauri star system
@@stonerationflameration3773 yes
the glowing dot was the best part
It is probrally a neutron star
Music?
Wait i dont know an L-type star i did not even know there is an l-type star
What color is I star
@green_the_planet uhhh ok
@@realclowngamer6721 didnt u watch the vid :|
The new spectral types L, T, and Y were created to classify infrared spectra of ultra cool stars.
@@realclowngamer6721 bright red , or Maroon
There are L-type Red Dwarfs too!
OMG L-type stars actually live longer than Trappist-1🤯🤯🤯
You should do the j1407b plant system
Ah yes astronomy is biology.
Brown dwarves deserve attention
Brown dwarves are cool, dangit! _Literally_ "cool" as stars (?) go, but that's not what I meant. :P
Cool! Can you do C type star system? (Well, if it even exists that is...)
Edit: turns out c types are carbon fusing stars
They are red giants
@Lionel Matthew Colin Tamunu 11 SECONDS AGO!?!
@Lionel Matthew Colin Tamunu IDK!!!!!!!!
@@haniosman1323 1 MINUTE AGO??????????????
@Lionel Matthew Colin Tamunu HOLY !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! 9 MUNITES AYO!
Haha get it? Failed star? L-type brown dwarf?
hey i want a even weaker star how about the spectral class is c type stars only 60 - 40 the mass of jupiter
There are carbon giant star
L-type just saying are brown dwarf the burn same heat has the sun but there’s super nova’s Are a red lave way but there life is 198,000,369MY
brown dwarf is like a star but only uses heavier materials.
Why do they take so long to cool down
2:07 wait what
0:09 There Is A Undyne Jumpscare
L type star huh means that they hate brown dwarf cuz its L *my opinion*
We need T or a binary system with G and K or something
There was a Red dwarf and Brown Binary system called Gliese221
WEWOWEWOWEWO PWA Ambulance Coming! ⚠️⚠️⚠️⚠️ 2 planetbols sitting on the ambulance roof
sad to see the universe die
So what next? W type? T type?
Bruh he already did W
@@iapetus6110 have you checked his videos THE MAX HE DID WAS 0 TY🔵
Now I think all that’s left to do for stars is G-type stars.
G-type=solar system
@@gordonchan1108 um… no
@@tntrose7285 the sun is a G type star
1:53 the planets side away
Can you do g type of star
I like timeline of l type brown dwarf
Good ending: it upgrades to a M Type! (red dwarf)
Hey dogepro this might be to much to ask but can you do a white dwarf system even though the planets would most likely get destroyed after the death of the star. Also can you do a life of a binary system like binary b system if that’s possible and f system binary m system binary and so on and so on sorry if this is to much to take in but I would really appreciate it.
If it is a M-type's white dwarf,its planets won't be destroyed i think
Imagine We Orbited The Brown Dwarf
Doggo: nah whatever **undyne face lol**
Me:**spams bruh**
Bruh bruh bruh bruh bruh bruh bruh bruh bruh
Bro got so close to becoming a star
L dwarf. At least I live longer.
Good video, Dogepro
the L type turns into T type then Y type and black
The beginning made me upset 😢😢
I made f-g type single star system in universe sandbox and it has a terrestrial earth like planet orbiting a gas giant
Star
1.20r sun
1.20m sun
Kinda similar but there’s 3-5 planets and 1 star also it’ll die sooner
Imagine this star have infinity hidrogen
when a star shrinks to death to a glowing meteor comet
That is a netorn star
God your right that have 120ty mind bad
Whats the system and the stars, planets, name?
0:08 XD
Next time, make a video of the life cycle of Wolf-Rayet star bro😊
WR is part of the O-type main sequence stars’ evolution, not a type of main-sequence stars
L Type Stars Are Rare
-Saturn- *Jupiter when stoled the suns job*
So cute!
Great vedio
why no likes in this video? (i press the like button)
What you could have done was scroll past red dwarf and the brown dwarfs were off screen
0:34 Lithium System Now!
WHY ARE LIKES DISABLED?
I noticed that too. Why is the like/dislike ratio hidden on this one...?
Good
omg thx
Smol
Make me a planet plz
Okay. You now have a planet. It is a rocky planet in the habitable zone. Its name is Dave.
Life of Brown Dwarfs sounds like boring.
1 Tillion years 1 QuinTillion years
Newton star: I just need a friend :(
B ,C ,and C-1:ayo well you dont need to fling us,now look what you did.
1:38 Tillion
Mathematicians:
1:35 you misspelled “trillion”
I'm really early
ITS UNDYNE UNDERTALE