Note: 1. I worked hard until 113 pages 2. Mistake: sorry for the disturbing noise its just a piano zelda game over and i forgot to pause the music division
Mistakes you made 1. Red dwarfs (m types) die at 3 trillion years in its lifespan 2. Red dwarfs also cannot burn heluim because it is to small to support it (so instead of growing then shinking it slowly shrinks down to a white dwarf when its out of hydrogen 3. O types cant get planets because they take all the matter (thats why their so big) 4. when the stars were dying it was going like 6M, 5.9M, 6M, 5.9M on the timeline 5. the black hole wouldve consumed the red dwsrf very quickly. end (pls try to fix these)
heres some mistakes you should fix. 1. Red dwarf's is the only star that do not grow before they die. 2. Red dwarf's live for 10 Trillion year's. 3. Red dwarf's is the only star that do not super nova but shrinks to white dwarf instead. 4. White dwarf's cooldown for 1 Quadtillion year's. 5. Black hole's will evaporate in 10^44 year's, for super massive is 10^100. For these list you should fix.
1. If mass is about 0.3 Sun masses the star is not convective and will expand to red supergiant after finishing burning hydrogen in its core. 2. Depends on mass - trillions of years for the least massive ones. 3. More massive stars up to 8-12 Sun masses also do not go supernova - they simply lose their outer layers during thermal pulses in AGB phase.
![Seungmin "그렇게, 천천히, 우리(As we are)" | [Stray Kids : SKZ-PLAYER]](http://i.ytimg.com/vi/kAzmhLHePqU/mqdefault.jpg)
Note:
1. I worked hard until 113 pages
2. Mistake: sorry for the disturbing noise its just a piano zelda game over
and i forgot to pause the music division
Uh you made the M star live less then a thousandth of its life 💀
And M types shrink and don’t get bigger / don’t expand
M type stars cant burn its helium
Some M0 and M1 stars are massive enough to burn helium.
The red dwarf should have died 1 trillion years to 9 trillion years
Proxima?
@@Ncn08825 4 Trillion years is its lifespan
congratulations
O
1:50
AAAAAAAW
4:47
OMG NO H!
3:43
Mistakes you made
1. Red dwarfs (m types) die at 3 trillion years in its lifespan
2. Red dwarfs also cannot burn heluim because it is to small to support it (so instead of growing then shinking it slowly shrinks down to a white dwarf when its out of hydrogen
3. O types cant get planets because they take all the matter (thats why their so big)
4. when the stars were dying it was going like 6M, 5.9M, 6M, 5.9M on the timeline
5. the black hole wouldve consumed the red dwsrf very quickly.
end (pls try to fix these)
What about 9.4 and 9.5 b
3 seems not true, planets mass is nothing compared to mass of red dwarfs, let alone o type stars
Bruh
0:27 z
Nah I'd win.
:( AAAAA BLACK HOLE!!!!!
2:24
/e pin also congrats
Thanks
@@Exon_ThePlanetball what is the app your using on PC?
@@Yuudachi-ChPowerPoint
and bandicam for record
@@Exon_ThePlanetball oh ok
M types only grow a tiny bit if at all
It’s good but M type stars don’t explode, they shrink
thats a mistake
@@Exon_ThePlanetball that’s true M type stars shrink but if thrips have a mass of over 0.3 Suns then they will become orange giants like K type stars
White dwarfs always form without explosion, more massive stars simply lose their outer layers due to thermal pulses during AGB phase.
Red dwarfs below 0.3 Sun masses become hotter up to 8-10 000K and increase their luminosity, then collapse to white dwarfs.
Even G and K type stars don't supernova, they only give out planetary nebulae.
Music used
Kevin macleod = Exotic battle
Kevin Macleod = Division
Kevin Macleod = Hitman
Kevin Macleod = Stages of grief
app name?
Powerpoint
Fun fact:Did you know Iron is not I? It is actually Fe.
Ferrum in Latin.🙂
heres some mistakes you should fix.
1. Red dwarf's is the only star that do not grow before they die.
2. Red dwarf's live for 10 Trillion year's.
3. Red dwarf's is the only star that do not super nova but shrinks to white dwarf instead.
4. White dwarf's cooldown for 1 Quadtillion year's.
5. Black hole's will evaporate in 10^44 year's, for super massive is 10^100.
For these list you should fix.
Before shrinking red dwarfs become hotter up to 8-10 000 K and more luminous, so called blue dwarf.
If an red dwarf has an mass of around > 0,30 M, they become red subgiants
@@F2r2923 They become red giants.
1. If mass is about 0.3 Sun masses the star is not convective and will expand to red supergiant after finishing burning hydrogen in its core.
2. Depends on mass - trillions of years for the least massive ones.
3. More massive stars up to 8-12 Sun masses also do not go supernova - they simply lose their outer layers during thermal pulses in AGB phase.
Even G and K type stars don't supernova, they only give out planetary nebulae.
How did supernova not destroy all planets
because its a binary
and ba moved far away from aa