The expanding Universe
Đã giới thiệu| English | Ý nghĩa |
|---|---|
| expanding/ekˈspændɪŋ/ | Đang mở rộng |
| redshift/ˈredʃɪft/ | Dịch chuyển đỏ |
| Big Bang/bɪɡ bæŋ/ | Big Bang |
| cosmic microwave background radiation/ˈkɒzmɪk ˈmaɪkrəʊweɪv ˈbækɡraʊnd ˌreɪdɪˈeɪʃn/ | Bức xạ nền vi sóng vũ trụ |
| Hubble constant/ˈhʌbl ˈkɒnstənt/ | Hằng số Hubble |
A growing Universe
- Look far enough and every galaxy is rushing away from us.
- The whole Universe is expanding 膨胀 — and that tells us how it began.
- The clue is hidden in the colour of starlight.
Redshift 红移
- When a galaxy moves away from us, the light we receive is stretched to a longer wavelength — shifted toward the red end of the spectrum. This is redshift.
- The further away a galaxy is, the bigger its redshift.
Redshift of a distant galaxy's spectrum
The expanding Universe
v = H₀·d
Galaxies recede faster the farther they are — speed is proportional to distance.
Light from a distant galaxy is redshifted. This means the galaxy is:
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A receding source stretches the light to a longer wavelength — toward the red end of the spectrum.
How does a galaxy's redshift change with its distance?
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More distant galaxies recede faster, so they show a bigger redshift — this is the basis of Hubble's law.
The expanding Universe and the Big Bang 大爆炸
- Distant galaxies are redshifted, and further ones more so — so the galaxies are moving apart: the Universe is expanding.
- Run that backwards and everything was once together at a single point.
- This is the evidence for the Big Bang theory.
Every galaxy is moving away from us, and the farther ones move away faster — the Universe is expanding
The redshift of distant galaxies is evidence that:
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Galaxies moving apart means the Universe is expanding; running it backwards points to a single starting point — the Big Bang.
More evidence, and the age of the Universe
- Faint microwave radiation comes from every direction in space — the cosmic microwave background radiation 宇宙微波背景辐射 (CMBR). It is early radiation stretched out as the Universe expanded.
- The Hubble constant 哈勃常数 links a galaxy's recession speed $v$ and distance $d$:
- Turning it around, $\dfrac{1}{H_0}$ estimates the age of the Universe — more support for the Big Bang.
The cosmic microwave background radiation (CMBR) is found coming from every direction in space.
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The CMBR fills all of space, coming from every direction — it is early radiation stretched into microwaves as the Universe expanded.
The Hubble constant is about $H_0 = 2.0 \times 10^{-18}$ per second. Estimate the age of the Universe ($1/H_0$), in seconds.
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Age $\approx \dfrac{1}{H_0} = \dfrac{1}{2.0 \times 10^{-18}} = 5.0 \times 10^{17}\ \text{s}$ (roughly 16 billion years).
The Hubble constant $H_0$ relates a galaxy's recession speed $v$ and distance $d$ by:
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$H_0 = \dfrac{v}{d}$; its reciprocal $\dfrac{1}{H_0}$ estimates the age of the Universe.
You've got it
- redshift: light from a receding galaxy is stretched toward red; further = bigger redshift
- distant galaxies all recede → the Universe is expanding → evidence for the Big Bang
- the CMBR (microwaves from all directions) is more Big Bang evidence
- Hubble constant $H_0 = \dfrac{v}{d}$; age of the Universe $\approx \dfrac{1}{H_0}$
Write from an age estimate of 4.0 times 10 to the 17 seconds
- The Hubble constant is 2.5 times 10 to the minus 18 per second.
- Estimate the age as 1 over H0. A larger redshift means a faster recession in this model.
The Hubble constant is 2.5 times 10 to the minus 18 per second. What age estimate does 1 over H0 give, and what does a larger redshift mean?
1 divided by 2.5 times 10 to the minus 18 is 4.0 times 10 to the 17 seconds.
What age does this Hubble constant give?
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1 divided by 2.5 times 10 to the minus 18 is 4.0 times 10 to the 17 seconds.