The Universe Flashcards
what is cosmology?
Cosmology is the study of the COSMOS – in other words, the universe.
What is the universe?
The universe is all existing matter, energy, space and time considered as a whole extending to the cosmic horizon.
what is the big bang theory?
▪ Before the Big Bang there was no universe, no space, no time. There simply was nothing as we know it. Absolutely nothing but energy.
▪ This energy was located in one single point of infinite density. During the Big Bang, it began to expand extremely quickly. All of the mass and energy in the universe today is still equal to this and there is evidence that the universe is continuing to expand.
▪ Cosmologists believe the universe began about 13.7 billion years ago with a massive explosion. This is considered a ‘no cause’ event.
what is the dark ages?
the last time when empty space really was empty; no planets, no suns, no galaxies, no life
Timeline of order in which celestial elements were formed
- Big Bag and Inflation
- 10-32 second - cosmic inflation ends
- 10-6 second - protons formed
- 300,000 years - first elements formed
- 400,000 years - cosmic background radiation
- 100 million years - first starts form
- 500 million years - earliest known galaxy
- 4 billion years - start formation peaks
- 9 billion years - our solar system formed
- 13.8 billion years - now
Evidence for the Big Bang?
▪ All galaxies are moving away from each other (still expanding) – this is demonstrated by red shift in light coming from distant stars. This suggests that the universe is expanding and that, if you extrapolate backwards, the universe had a beginning.
▪ Cosmic background is present everywhere and the levels exactly fit predictions based on calculations of the universe being 14 billion years old.
▪ Levels of helium in the universe are too high to have only formed by collapsing stars so must have been formed in the Big Bang explosion.
what is the doppler effect?
Doppler effect - as waves move towards you the frequency is perceived to be higher with shorter wavelength (blue shift) as it moves away frequency is perceived to be lower with longer wavelength (red shift) – although it isn’t changing!
Other Universe Models?
▪ Aristotle 380BC - Earth was at the centre of the universe, and that the sun, stars, moon, and planets all revolve around the earth in 55 concentric orbits.
▪ Copernicus 1540 AD - suggested that the sun was stationary at the centre of the universe and that all other bodies revolved around it in circular paths.
▪ And then the telescope was invented and the movement of all the visible stars could be studied…
▪ Steady State model - the universe is infinite and has always existed more or less like it is now…. And it will continue to be this way….
What is next for the universe?
- the big freeze
- the big rip
- the big crunch
- the big bounce
what is a star?
▪ Stars are massive, luminous spheres of plasma held together by gravity
what is the big freeze?
the universe will keep expanding and cooling as it has done and at some point the energy will be too dissipated to sustain life. As existing stars run out of fuel and cease to shine, the universe will slowly grow darker, one star at a time and there will be nothing but black holes. Also called heat death or maximum entropy)
what is the big rip?
is similar, in the future the distances in the universe will become infinite. At a point where the ratio between dark energy pressure and its density become less than -1 , the universe will be pulled apart.
what is the big crunch?
If the universe begins to recontract it will form a hot, dense state similar to that immediately after the Big Bang
what is the big bounce?
The Big Bounce describes a scenario of the universe expanding and then contracting – so the Big Bang was caused by the last contraction of the universe.
what is apparent magnitude?
Apparent magnitude is a measure of the brightness of a star as it appears on Earth – but this isn’t a fair comparison as some stars are very distant.
what is absolute magnitude?
Absolute magnitude is a measure of the brightness of a star if it was 10 parsecs from the Earth – better comparison.
what is the Hertzsprung – Russell Diagram?
A Hertzsprung–Russell or H–R diagram is a plot of star brightness (measured as luminosity) against star temperature/colour.
why is the Hertzsprung – Russell Diagram important?
It enables astronomers to classify the type of star they are looking at and helps them to determine many of its characteristics like how old it is, its surface temperature and the stage of its life cycle.
what does the colour of star tell you?
The colour of a star is related to its temperature: blue stars are the hottest and red stars are the coolest. Stars are given a spectral class letter based on their temperature and colour.
what is the luminosity of the star?
Stars also vary in brightness, this is called luminosity. The scale of luminosity is based around our Sun, which is given a luminosity of 1. Stars that are brighter than the Sun have a luminosity of greater than 1 and stars that are less bright than the Sun are given a luminosity of less than 1.
what is nuclear fusion?
- Stars obtain their energy through a process called nuclear fusion. This occurs when two atoms combine (or fuse) to create a new element. Because it is so hot inside the cores of stars, hydrogen atoms have enough energy to fuse together to form helium and an enormous amount of energy is released in the process. The gravitational collapse of matter triggers enormous levels of heat and pressure which triggers a nuclear fusion reaction.
- the fusion of four Hydrogen nuclei to form Helium includes a loss of mass, but this is converted into a huge amount of energy (gamma radiation)
how is matter formed?
- Formation of hydrogen and helium occurred first after the Big Bang. Other elements must be formed as a result of the lifecycle of stars.
- When the star’s supply of hydrogen is used up, it begins to convert helium into oxygen and carbon. If the star is massive enough, it will continue until it converts carbon and oxygen into neon, sodium, magnesium, sulphur and silicon. Eventually, these elements are transformed into calcium, iron, nickel, chromium, copper and others until iron is formed.
what do low mass starts tend to be?
cooler and less bright
what do high mass starts tend to be?
hotter and brighter