Space Physics Flashcards
1) What’s within our solar system? (2)
How did our solar system come to be?
1) Within our solar system there is one star, the Sun, plus the eight planets and the dwarf planets that orbit around the Sun. Natural satellites, the moon that orbit planets, are also part of the solar system.
- Our solar system is a small part of the Milky Way galaxy.
2) The solar system formed from gas and dust clouds that gradually become more and more concentrated because of gravitational attraction
How are stars initially formed? (3)
- Stars and dust initially formed from a cloud of dust and gas called nebula.
- The force of gravity pulls the dust and gas together to become more concentrated and form a protostar. The temperature rises as the protostar get denser and more particles collide with each other. This process transfers energy from the GPE store of the protostar to the thermal energy store
- When the temp gets high enough, hydrogen nuclei undergo nuclear fusion to form helium nuclei- this gives out huge amounts of energy which keeps the core of the star hot. A star is born.
How is the main sequence star formed?
Why do stars such as the sun radiate energy?
- Star enters a long stable period where the outward pressured caused by the nuclear fusion that tries to expand the star balances the force of gravity, pulling everything inwards. In this stable period, it’s called the main sequence star and lasts several billion years. THE FORCE OF GRAVITY AND THE RADIATION PRESSURE ARE IN BALANCE.
- Stars such as the sun radiate energy because of hydrogen fusion in the core and hence they are called main sequence stars because this is the main stage in the life of a sta
Why is the sun a ‘stable star’?
- Sun is stable because gravitational forces acting inwards balance the forces of nuclear fusion energy in the core acting outwards.
What happens to the main sequence star eventually? (2)
- Eventually, the hydrogen begins to run out in its core and the star the swells into a red giant if it is a small star or a super red giant if it’s a larger star( stars that are much bigger than the Sun)- it becomes red because the surface cools.
- Fusion of helium and other light elements in the core fuse together to form heavier elements( up to iron) are created in the core of the star
What are the two things that happens after a red giant?
- When there is no more light elements in the core, fusion stops and no more radiation is released because the star becomes unstable-> star ejects its outer layer of dust and gas and because of its own gravity, star collapses upon itself and turns from red, yellow, to white and forms a white dwarf which will gradually cool and fade away into a black dwarf.
What happens to stars much bigger than the Suns at the end of their lives after the main sequence stage? (2)
- 1) Big stars glow brightly again as they undergo more fusion and expand and contract several times, forming elements as heavier as iron in various nuclear reactions
- These stars swell out to become red supergiants and they then collapse- the matter surrounding the star’s core compresses and more and more this compresses causes t
them to explode in a supernova, forming elements heavier than iron and ejecting them into the universe to form new planets and stars; stars and life cycles produce and distribute all naturally occurring elements
What does the exploding supernova do? (2)
-Exploding supernova throws outer layers of dust and gas into space, leaving a v dense core = neutron star.
-If the star is massive enough, it will become a black hole
and the gravitational field of a black hold is so strong and super dense point in space that not even light can escape from
What is a supernova?
-explosion of a red giant where the core collapses on itself.
Outline the life cycle of stars. (3)
1) Cloud of dust and gas-> Protostar-> Main Sequence star-> Stars much bigger than Sun( Red Super Giant) or stars about the same size as the sun (red giant)
2) Red Super Giant-> Supernova-> Neutron Star or Black Hole.
3) Red Giant-> White or Black Dwarf
What is within our solar system? (4)
1) Planets- large objects that orbit a star- 8 of them0 Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune and their gravity is strong enough to have pulled in any nearby objects apart from their natural satellites.
2) Dwarf planets(pluto)- planet like objects that orbit stars.
3) Moon- natural satellites- thes orbit planets.
4) Artificial satellites- generally satellites that humans have built and they orbit the Earth
Define milky way galaxies?
A massive collection of billions of stars that are held together by gravity.
Define a satellite?
- an object that orbits a second, more massive object
What causes the planets to move around the Sun?(4)
- gravity provides the force which creates orbits and the planets move around the Sun in almost circular orbits.
- the force of gravity on the planet from the Sun act towards the centre of the Sun and this is the resultant force because no other forces act on it and this is an example of a centripetal force because it acts towards the centre of the circle.
- if an object is travelling in a circle, it is constantly changing direction which means it is constantly accelerating and the direction of the motion of any planet in a circular orbit is at right angles to the direction of the force of gravity on it- the force of gravity can lead to a change in velocity but unchanged speed- CIRCULAR MOTION
- the object keeps accelerating towards what its orbiting but the instantaneous velocity (which is at right angles to the acceleration) keeps it travelling in a circle - the force that makes this happen is provided by gravity between the planet and the sun or between the planet and its satellites..
- for a stable orbit, the radius must change if the speed changes
What does the size of the orbit depend upon on?
1) the closer you ge tto the planet, the stronger the gravitational force is and the stronger the force, the faster the orbitting objet needs to travel in order to remain in orbit.
- for an object in a stable orbit,, if the speed of the orbit changes, the radius of its orbit must do so too and faster moving objects will move in a more stable orbit with a smaller radius than slower moving ones.
therefore to stay in orbit at a particular distance, a small body must move at a particular speed around a larger boy