Paper 1 Knowledge Gaps: Content Flashcards
What are the four types of decay?
- gamma
- beta plus
- beta minus
- alpha
Define alpha decay
If the nucleus is unstably large, it will emit a ‘package’ of two protons and two neutrons called an alpha particle
–> this is also a helium-4 nucleus
What is the effect of alpha decay on
a) the atomic number?
b) the mass number?
a) decreases by 2
b) decreases by 4
How strong is alpha decay?
- highly ionising
- weakly penetrating
Define beta minus decay
If a nucleus has too many neutrons, a neutron will turn into a proton and emit a fast-moving electron
What is the electron emitted in beta minus decay called?
beta minus (β−) particle
What is the effect of beta minus decay on
a) the atomic number?
b) the mass number?
a) increase by one
b) remains the same
How strong are both of the beta decays?
medium ionising, medium penetration
Define beta plus decay
If a nucleus doesn’t have enough neutrons, a proton will turn into a neutron and emit a fast-moving positron
What is another name for a positron?
beta plus (β+) particle
What is the effect of beta plus decay on
a) the atomic number?
b) the mass number?
a) decreases by one
b) stays the same
Define gamma decay
A nucleus will often still have excess energy after emitting an alpha/beta particle and so energy will be emitted as a gamma ray
What is the effect of gamma ray emission on
a) the atomic number?
b) the mass number?
No effect on either
How strong are gamma rays?
- highly penetrating
- weakly ionising
Define half life
The amount of time it takes for half of the sample of unstable nuclei to halve
What is the equation to calculate how many nuclei remain after a certain amount of time concerning half life?
net decline = (initial number x number after x half lives)/ initial number
Describe the life cycle of a star that has a mass similar to solar mass
- Nebula
- protostar
- main sequence star
- red giant
- white dwarf
Describe a nebula
Giant cloud of hydrogen gas and dust
How does a nebula become a protostar?
- force of gravity pulls particles closer
- until hot ball of gas is formed
- known as a protostar
How does a protostar become a main sequence star?
- density of the protostar increases
- resulting in more frequent collisions between the particles
- = temperature increases
- thermal expansion from fusion reactions occur within its core and the force of gravity keeps the star in equilibrium
How does a main sequence star turn into a red giant?
- main sequence star runs out of gas to fuse = no equilibrium
- this will cause the star to collapse
- which will increase the pressure and temperature of the core, allowing for heavier elements to form
How does a red giant star turn into a white dwarf?
Once all of the reactions are over, the star contracts and cools into a white dwarf = core collapses completely
What is the life cycle of stars that have a mass larger than solar mass?
- nebula
- protostar
- main sequence star
- red supergiant
- supernova
- neutron star or a black hole
What is the difference between a red supergiant and a red giant?
A red supergiant is much larger than a red giant