6.2.3 BETA Verified

The Universe

11 learning objectives 4 core 7 extended

1. Overview

This topic explores the vast scale of our Universe, from our home galaxy, the Milky Way, to the billions of other galaxies moving away from us. By studying the light from these distant objects, scientists have uncovered evidence for the Big Bang Theory and can even estimate the age of the Universe itself.


Key Definitions

  • The Universe: A vast collection of billions of galaxies.
  • Galaxy: A large system of billions of stars, gas, and dust bound together by gravity.
  • Milky Way: The specific galaxy that contains our Solar System.
  • Light-year: The distance light travels in one year (approximately $9.5 \times 10^{15}$ meters).
  • Redshift: The increase in the observed wavelength of electromagnetic radiation from objects moving away from the observer.
  • Cosmic Microwave Background Radiation (CMBR): (Extended) Weak microwave radiation coming from every direction in space, left over from the Big Bang.
  • Hubble Constant ($H_0$): (Extended) The ratio of the speed at which a galaxy is moving away to its distance from Earth.

Core Content

The Milky Way

  • The Universe is made up of billions of galaxies.
  • Our Solar System is a tiny part of the Milky Way galaxy.
  • The diameter of the Milky Way is approximately 100,000 light-years.
  • 📊A spiral-shaped galaxy with a label showing the Sun located on one of the outer spiral arms, far from the center.

Redshift

  • When a star or galaxy moves away from Earth, the light waves it emits are "stretched."
  • This stretching increases the wavelength, shifting the light toward the red end of the visible spectrum. This is called redshift.
  • Light from distant galaxies is redshifted compared to light emitted on Earth.

The Expanding Universe

  • Observations show that light from nearly all distant galaxies is redshifted.
  • This proves that distant galaxies are receding (moving away) from us.
  • The further away a galaxy is, the greater its redshift, meaning it is moving faster.
  • This is key evidence that the Universe is expanding and supports the Big Bang Theory (the idea that the Universe began from a single, hot, dense point).

Extended Content (Extended Only)

Cosmic Microwave Background Radiation (CMBR)

  • CMBR is microwave radiation observed at all points in space around us.
  • It was produced shortly after the Universe was formed as high-energy (short wavelength) radiation.
  • As the Universe expanded, the space itself stretched. This stretched the radiation’s wavelength into the microwave region of the electromagnetic spectrum.
  • CMBR is considered the "afterglow" of the Big Bang.

Measuring Space

  • Speed ($v$): The speed at which a galaxy moves away can be calculated from the specific change in the wavelength of its starlight (the amount of redshift).
  • Distance ($d$): The distance to very far galaxies is determined by observing the brightness of a supernova (an exploding star) within that galaxy.

The Hubble Constant and Age of the Universe

  • The speed of recession ($v$) is proportional to the distance ($d$). This is Hubble’s Law.
  • Equation: $v = H_0 d$
  • The current estimate for $H_0$ is $2.2 \times 10^{-18}$ per second ($s^{-1}$).
  • The age of the Universe can be estimated using the formula: $\text{Age} = \frac{1}{H_0}$.
  • This calculation suggests the Universe started at a single point billions of years ago.

Worked Example: Calculate the speed of a galaxy that is $2.0 \times 10^{24}$ m away.

  • $v = H_0 \times d$
  • $v = (2.2 \times 10^{-18}) \times (2.0 \times 10^{24})$
  • $v = 4.4 \times 10^6 \text{ m/s}$

Key Equations

Equation Symbols Units
$v = H_0 d$ $v$: speed, $d$: distance, $H_0$: Hubble constant $v$ (m/s), $d$ (m), $H_0$ ($s^{-1}$)
$t = \frac{1}{H_0}$ $t$: Age of the Universe $t$ (seconds)

Common Mistakes to Avoid

  • Wrong: Thinking the Sun is at the center of the Universe.
  • Right: The Sun is just one star in the Milky Way, and it is not at the center of the galaxy or the Universe.
  • Wrong: Defining redshift as a change in the speed of light.
  • Right: Redshift is a change in wavelength. The speed of light ($c$) is constant.
  • Wrong: Confusing a galaxy with a Solar System.
  • Right: A Solar System is one star and its planets; a galaxy contains billions of stars and solar systems.
  • Wrong: Thinking redshift means the light looks red to the naked eye.
  • Right: It means the wavelength is longer than expected, not necessarily that the object appears red.

Exam Tips

  1. Definitions Matter: If asked to describe redshift, always mention the "increase in observed wavelength" and that the source is "moving away/receding."
  2. Unit Conversions: In Hubble Constant calculations, ensure distance is in meters (m) and speed is in meters per second (m/s).
  3. Big Bang Evidence: If a question asks for evidence of the Big Bang, you must mention Redshift (Core) and CMBR (Extended).

Test Your Knowledge

Ready to check what you've learned? Practice with 22 flashcards covering key definitions and concepts from The Universe.

Study Flashcards