Three ways the universe could end - Venus Keus

2,097,742 views ・ 2019-02-19

TED-Ed


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Translator: Julie Mbeyella Reviewer: Doris Mangalu
Tunajua ya kale ya ulimwengu wetu:
00:06
We know about our universe’s past:
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00:09
the Big Bang theory predicts that all matter, time, and space
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nadharia ya Mlipuko Mkubwa inatabiri kuwa mata, muda na anga zote
00:14
began in an incredibly tiny, compact state about 14 billion years ago.
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vilianza kwa hali ya udogo sana, takribani miaka bilioni 14 iliyopita.
00:20
And we know about the present:
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Nasi tunajua kuhusu sasa:
00:22
scientists’ observations of the movement of galaxies
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mitazamo ya watafiti ya mienendo ya galaksi
00:25
tell us that the universe is expanding at an accelerated rate.
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inatuambia kwamba ulimwengu unapanuka kwa kasi sana.
00:30
But what about the future?
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Je vipi kuhusu mbeleni?
00:31
Do we know how our universe is going to end?
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Tunajua namna gani ulimwengu wetu utafikia kikomo?
00:35
Cosmologists have three possible answers for this question,
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Wanakosmolojia wana nadharia tatu za swali hili,
00:38
called the Big Freeze,
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zinazoitwa Mgando Mkubwa,
00:40
the Big Rip and the Big Crunch.
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Mraruo Mkubwa na Uchakacho Mkubwa.
00:43
To understand these three scenarios,
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Kuzielewa hizi nadharia tatu,
00:46
imagine two objects representing galaxies.
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waza vitu viwili vya kuwakilisha galaksi.
00:49
A short, tight rubber band is holding them together—
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Kamba ya mpira fupi, iliyokaza inazishikilia pamoja---
00:53
that’s the attractive force of gravity.
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hiyo ni mvuto wa nguvu ya uvutano.
00:56
Meanwhile, two hooks are pulling them apart—
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Wakati huo huo, koleo mbili zinaziachanisha---
00:59
that’s the repulsive force expanding the universe.
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hiyo ni nguvu ya muasi inayofanya ulimwengu usambae.
01:03
Copy this system over and over again,
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Nakili huu mfumo tena na tena,
01:06
and you have something approximating the real universe.
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Na una kitu kinachokaribia ulimwengu wa ukweli.
01:09
The outcome of the battle between these two opposing forces
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Matokeo ya mashindano ya hizi nguvu mbili zinazokinzana
01:13
determines how the end of the universe will play out.
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inaamua jinsi mwisho wa ulimwengu utakuwaje.
01:16
The Big Freeze scenario is what happens if the force pulling the objects apart
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Matukio ya Mgando Mkubwa ndiyo yanayotokea kama nguvu inayofanya vitu viachane
01:22
is just strong enough to stretch the rubber band until it loses its elasticity.
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ina nguvu ya kutosha ya kuisogeza kamba ya mpira hadi ipoteze uvutikaji.
01:27
The expansion wouldn’t be able to accelerate anymore,
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Kusogea hakutoweza kuongezeka tena,
01:30
but the universe would keep getting bigger.
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lakini ulimwengu utazidi kuwa mkubwa.
01:33
Clusters of galaxies would separate.
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Makundi ya galaksi yanaweza kutengana.
01:36
The objects within the galaxies–
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Vitu vilivyomo kwenye galaksi--
01:38
suns, planets, and solar systems
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jua, sayari, na mifumo wa jua
01:41
would move away from each other,
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vingeweza kutengana,
01:42
until galaxies dissolved into lonely objects
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mpaka galaksi ziyeyuke kuwa vitu vya kipekee
01:45
floating separately in the vast space.
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vikielea kwa kujitegemea kwenye anga kubwa.
01:48
The light they emit would be redshifted to long wavelengths
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Mwanga unaotoka ungeweza kuhamishwa kwenye mawimbi marefu
01:51
with very low, faint energies,
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yenye nguvu kidogo na hafifu,
01:54
and the gas emanating from them would be too thin to create new stars.
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na gesi inayotoka kwao ingekua nyembamba sana kutengeneza nyota mpya.
01:59
The universe would become darker and colder,
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Ulimwengu ungekuwa wa giza na wa baridi zaidi,
02:02
approaching a frozen state
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ukikaribia hali ya kuganda
02:03
also known as the Big Chill,
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unaojulikanana kama Ubaridi Mkubwa,
02:05
or the Heat Death of the Universe.
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au kifo cha joto cha Ulimwengu.
02:08
But what if the repulsive force is so strong
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Lakini inakuwaje kama nguvu muasi ni kubwa sana
02:11
that it stretches the rubber band past its elastic limit,
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kufanya kamba ya mpira ipanuke kupita kipimo chake,
02:15
and actually tears it?
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na iichane kabisa?
02:16
If the expansion of the universe continues to accelerate,
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Kama kutanuka kwa ulimwengu kunazidi kuongezeka,
02:19
it will eventually overcome not only the gravitational force –
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itaweza kuzidi sio tu nguvu ya uvutano --
02:23
tearing apart galaxies and solar systems–
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ikichana galaksi na mifumo ya jua--
02:26
but also the electromagnetic, weak, and strong nuclear forces
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lakini pia na nguvu hafifu ya sumaku umeme,na nguvu za nguvu za nuklia
02:30
which hold atoms and nuclei together.
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ambayo inashikilia atomu na nuklia pamoja.
02:33
As a result,
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Matokeo yake,
02:34
the matter that makes up stars breaks into tiny pieces.
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mata inayotengeneza nyota inavunjika katika vipande vidogo.
02:38
Even atoms and subatomic particles will be destroyed.
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Hata atomu na vipande vidogo vya atomu vitaharibika.
02:42
That’s the Big Rip.
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Hiyo ni Mraruo Mkubwa.
02:44
What about the third scenario,
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Vipi kuhusu tukio la tatu,
02:46
where the rubber band wins out?
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ambapo kamba ya mpira inashinda?
02:48
That corresponds to a possible future
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Ambayo ina shabihiana na uwezekano wa mbeleni
02:51
in which the force of gravity brings the universe’s expansion to a halt—
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ambapo nguvu ya uvutano inaletea kusambaa kwa ulimwengu kusimama---
02:55
and then reverses it.
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Halafu inaigeuza.
02:58
Galaxies would start rushing towards each other,
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Galaksi zitaanza kukimbizana kukaribiana,
03:01
and as they clumped together
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na zikijikusanya pamoja
03:02
their gravitational pull would get even stronger.
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nguvu zao za uvutano zingekua na nguvu zaidi.
03:06
Stars too would hurtle together and collide.
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Nyota pia zingekusanyika pamoja na kugongana.
03:09
Temperatures would rise as space would get tighter and tighter.
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Joto lingepanda kadri anga inavyozidi kujibana zaidi.
03:13
The size of the universe would plummet
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Ukubwa waa ulimwengu ungekua timazi
03:15
until everything compressed into such a small space
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hadi kila kitu kilichojikusanyika kwenye nafasi ndogo
03:19
that even atoms and subatomic particles would have to crunch together.
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mpaka hadi chembe za atomu na atomu ndogo vitajikusanyika pamoja.
03:24
The result would be an incredibly dense, hot, compact universe —
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Matokeo yatakuwa ni ulimwengu mzito, wenye joto na ulio jifunga ---
03:29
a lot like the state that preceded the Big Bang.
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kama ile hali iliyoitangulia Big Bang.
03:32
This is the Big Crunch.
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Hii ndiyo Uchakacho Mkubwa.
03:35
Could this tiny point of matter explode in another Big Bang?
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Je hii sehemu ndogo ya mata inaweza kulipuka kuwa Mlipuko Mkubwa mwingine?
03:39
Could the universe expand and contract over and over again,
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Ulimwengu unaweza kuongezeka na kujifunga tena na tena,
03:43
repeating its entire history?
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ikirudia historia yake yote?
03:45
The theory describing such a universe is known as the Big Bounce.
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Nadharia inayoeleza ulimwengu huo unajulikana kama Mruko Mkubwa.
03:50
In fact, there’s no way to tell how many bounces could’ve already happened—
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Pia hamna namna ya kujua miruko mingapi imeshatokea tayari---
03:54
or how many might happen in the future.
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au mingapi itatokea huko mbeleni.
03:57
Each bounce would wipe away any record of the universe’s previous history.
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Kila mruko itafuta mbali kumbukumbu yeyote ya historia ya ulimwengu ya nyuma.
04:03
Which one of those scenarios will be the real one?
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Matukio yapi kati ya haya yatakuwa sahihi?
04:06
The answer depends on the exact shape of the universe,
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Jibu linategemea na umbo halisi la ulimwengu,
04:09
the amount of dark energy it holds,
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kiasi cha nguvu ya gizai iliyobeba,
04:11
and changes in its expansion rate.
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na mabadiliko ya kusambaa kwake.
04:14
As of now, our observations suggest that we’re heading for a Big Freeze.
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Na kwa sasa, mitazamo yetu inapendekeza kua tunaelekea kwenye Mgando Mkubwa.
04:18
But the good news is that we’ve probably got about 10 to the 100th power years
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Japo habari njema ni kwamba tuna karibia miaka 10 mpaka nguvu ya 100
04:24
before the chill sets in —
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kabla ya ubaridi kuingia ---
04:26
so don’t start stocking up on mittens just yet.
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kwahiyo usianze kununua kinga za mkononi bado.
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