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Pearson Edexcel IGCSE Physics Astrophysics summary notes £6.99   Add to cart

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Pearson Edexcel IGCSE Physics Astrophysics summary notes

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Pearson Edexcel IGCSE Physics Astrophysics summary notes Good for IGCSE and GCSE Edexcel board Concise, easy to use and revise from

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  • Astrophysics
  • June 25, 2023
  • 2
  • 2022/2023
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Astrophysics

Motion in the universe

 The universe is a large collection of billions of galaxies.
 A galaxy is a large collection of billions of stars.
 A solar system is a collection of planets orbiting a common star. Our solar system is in the
Milky Way galaxy.

Gravity in Space
The gravitational field strength is the force per unit mass on a body in a gravitational field and is
measured in Newtons per kilogram (N/kg). It varies with the mass and size of the body and is
therefore different on other planets and the moon compared to the Earth.
 weight = mass × gravitational field strength W = mg

Gravitational force enables the various bodies to orbit around others. For example:
 Moons orbit planets
o The orbits are slightly elliptical with near constant orbital speed
 Planets and comets orbit the Sun
o The orbits of planets are slightly elliptical with near constant orbital speed. The
orbits of comets are highly elliptical.
 Artificial satellites orbit the Earth

The greater the orbital radius or the smaller the time period, the greater the orbital speed
2× π × orbitalradius
orbital speed =
time period
Comets have a greater speed nearer to the star (when r is smaller) because the ice inside them
melts as they get closer (& warmer) - causing their mass to decrease.

Stellar evolution
 A star begins as a cloud of dust & gas called a nebula. The particles experience a weak
attraction towards each other due to gravity and begin to clump together.
 They continue to clump together until the pressure and temperature is great enough for
nuclear fusion to occur.
o Hydrogen nuclei fuse together to form helium nuclei which releases a large amount
of energy and causes a great outwards pressure
o This outwards pressure balances with the inwards pressure due to gravity and the
star is now stable and called a main sequence star
 Eventually the hydrogen in the star is used up. There is no longer enough outward pressure
from nuclear fusion, and it collapses under its
own gravitational attraction, becoming
unstable.
 If the star has a similar mass to the Sun, it
expands massively and becomes a red giant. It
then becomes a white dwarf (and finally cools
into a black dwarf).
 If the star has a mass larger than the Sun, it
expands and becomes a red super giant, before
exploding in a supernova. What remains is
either a neutron star, or if it even bigger, a black
hole

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