Big Bang Theory Simplified Revision Notes for Scottish Highers Physics
Revision notes with simplified explanations to understand Big Bang Theory quickly and effectively.
Learn about The Expanding Universe for your Scottish Highers Physics Exam. This Revision Note includes a summary of The Expanding Universe for easy recall in your Physics exam
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Big Bang Theory
Big Bang Theory
Introduction
The Big Bang theory is a fundamental concept in cosmology that explains the origin and evolution of the universe.
It is supported by various pieces of evidence, including redshift, the expansion of the universe, and the relationship between temperature and emitted radiation.
Redshift and Expansion
Redshift is the phenomenon where light from distant galaxies appears to shift towards longer wavelengths, indicating they are moving away from us.
The expansion of the universe, driven by dark energy, is responsible for this redshift.
While redshift and expansion support the idea of a Big Bang, they do not provide direct evidence of the event itself.
Temperature and Emitted Radiation
The relationship between temperature and emitted radiation is a crucial piece of evidence for the Big Bang theory.
In everyday life, we observe that hot objects emit visible light, with colours ranging from red to blue as their temperature increases.
Starlight can be analysed to determine the temperature of stars, usually measured in Kelvin (K), where 0 K is absolute zero (-273.15°C).
Kelvin Scale
The Kelvin scale is similar to the Celsius scale, with temperature intervals of 1 K equal to 1°C.
Absolute zero corresponds to 0 K, which is equivalent to -273.15°C.
Radiation Distribution
The distribution of radiation emitted by an object at different temperatures can be graphed.
The graph shows curves representing the radiation distribution for objects at various temperatures.
Big Bang Theory
Physics
Peak Intensity
The dotted line on the graph represents the peak intensity of radiation, also known as radiation per unit surface.
Objects at higher temperatures have shorter peak wavelengths in their spectra.
Shorter wavelengths correspond to higher frequencies and bluer colours, indicating that hotter objects emit bluer light, while cooler objects emit redder light.
Hertzsprung-Russell Diagram
The Hertzsprung-Russell (HR) diagram is a tool used in astronomy to plot the brightness of stars against their temperature.
It helps classify stars and predict their evolutionary paths.
Significance
The HR diagram is essential for understanding the life cycle of stars, including their potential to become red giants or black holes.
The evidence from the relationship between temperature and emitted radiation supports the Big Bang theory by demonstrating how the universe's temperature has changed over time.
Summary
The Big Bang theory explains the universe's origin and evolution.
Evidence such as redshift, the expansion of the universe, and the relationship between temperature and emitted radiation supports this theory.
Temperature and radiation data are crucial in understanding the universe's history and the life cycles of stars.
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