SP7 - Astronomy Flashcards
What is the geocentric model and who created it?
Ptolemy made the geocentric model. This is a model of the universe with the Earth at the centre and planets and the Sun orbiting it. In Ptolemy’s model, planets moved in small circles as they orbited the Earth.
What is the heliocentric model and who created it?
Copernicus created the heliocentric model, in which the Sun is at the centre of the Solar system, and the planets orbit around it. This is the model we use today.
What is in the solar system?
- 8 planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune)
- 5 dwarf planets (Pluto, Ceres, Makemake, Haumea, Eris)
- thousands of comets (small lump of dirty ice)
- millions of asteroids (small lump of rock)
How have telescopes changed since their invention?
- they have got bigger
- they have got better magnification and resolution
- they can go into space
- they are often placed high on mountains
- can detect other waves not just light (e.g. IR telescopes)
- can take pictures
- can be attached to computers
- can be controlled robotically
Why do we put telescopes into space?
- to observe the solar system
- to take pictures in space
- to stop interference from the atmosphere (dust, weather etc.)
- ‘see’ further
- detect wavelengths blocked out by the atmosphere
- can observe Earth
- better clarity as no distortion from atmosphere
Describe the orbits of planets.
Planets orbit stars and have slightly elliptical orbits. The speed of the orbiting object therefore changes depending on the stage of the orbit it’s in. It has a closed loop orbit and it is a fixed plane. It is confined to a solar system.
Describe the orbits of moons
Moons orbit planets. They have a circular orbit which doesn’t change speed. They have a closed loop and a fixed plane. Their orbits are confined to a solar system.
Describe the orbits of comets.
Comets orbit stars with highly elliptical orbits. They therefore do change speed depending on what stage of the orbit they’re in (closer to the star = moves faster). They have a closed loop and a fixed plane but are not confined to a solar system.
What is the lifecycle of an average star?
Nebula —> Protostar —> Main sequence star —> Red giant —> White dwarf —> Black dwarf
What is the lifecycle of massive stars?
Nebula —> Protostar —> Massive main sequence star —> Red supergiant —> Supernova —> Neutron star OR Black hole
What is a nebula?
A large cloud of dust and gas containing mainly hydrogen. When the mass of the hydrogen becomes large enough, the gravity will pull the hydrogen in on itself, which will make it contract and form a ball.
What is a protostar?
A protostar is a ball of hydrogen. It continues to contract under its own gravity and as the hydrogen atoms accelerate, their kinetic energy increases. The extra kinetic energy raises the temperature of the hydrogen and the atoms collide with each other more frequently - fusion begins. Fusion turns hydrogen into helium and releases a huge amount of energy as heat and light. The protostar bursts into flame.
What is a main sequence star?
A main sequence star is in a stable phase in which gravity pulling the star in balances pressure from hot gases pushing the star out. Therefore, the size of the star stays almost constant.
What is a red giant?
Over time, the forces on a star become unbalanced. When the fusion reactions stop, the inward gravitational forces are stronger than the outward radiation pressure, causing the core of the star to collapse, the star swells and cools, turning red. This is a red giant.
What is a white dwarf?
A red giant collapses to form a white dwarf that gradually cools over time. A white dwarf is a small, very dense star that is typically the size of a planet. When a white dwarf cools, it becomes a black dwarf.