space physics (p8) Flashcards
describe the planets in the solar system, and the sun:
- at the centre is the sun, which is a star.
- mercury, venus, earth and mars are relatively small rocky planets.
- jupiter, saturn, uranus and neptune are much larger.
- beyond the orbit of neptune, we have a number of dawrf planets, one of which is pluto.
- the dwarf planets are extremely small.
- all orbit the sun in a slightly elliptical orbit (not a perfect circle, it’s slightly squashed)
what is the difference between asteroids and comets?
- asteroids are mostly made of rock and metal, and are mainly found in the asteroid belt (between mars and jupiter)
- comets are made mostly of ice and dust. they also orbit the sun in an elliptical orbit, and tend to be towards the edge of the solar system (beyond neptune)
what else does the solar system contain?
a number of other objects besides planets. for example, moons, asteroids and comets.
- moons are natural satellites which orbit planets.
- most planets in the solar system have at least one moon, some planets have a large number of moons.
describe the milky way galaxy:
- the solar system is just a tiny part of the milky way galaxy.
- a galaxy is a massive group of stars, most of which contain their own star systems
- in the universe, there are hundreds of billions of galaxies.
- all held together by gravity, and all the galaxies spin around the middle in the same way planets orbit the sun
describe the universe:
- scattered with galaxies, but mainly empty space (similar to galaxies)
what is the difference between a solar system and a star system?
solar system: our sun and the surrounding planets
star system: any other star and its orbiting planets
how do stars form?
- stars form from clouds of dust and gas - this is called a nebula.
- in a nebula, the gas is mainly hydrogen.
- in the first stage, gravity causes the cloud of dust and gas to collapse.
- as the dust particles move faster, the temperature rises to millions of degrees celsius (gravity ‘squeezes’ the star, meaning the particles collide more, raising the temperature), it gets more dense
- this collapsing cloud of dust and hot gas is called a protostar.
- as more particles collide and join the protostar, it gets bigger, meaning its force of gravity gets stronger, attracting even more dust and gas
- if the temperature of the protostar gets high enough, the hydrogen nuclei undergo nuclear fusion to form helium NUCLEAR FUSION
- nuclear fusion releases a lot of energy, keeping the core of the star hot
- at this point, the protostar has turned into a main sequence star.
describe what happens to a star when it undergoes nuclear fusion:
- there are two opposing forces acting within the star.
- the force of gravity acts inwards, and tends to make the star collapse.
- the energy from nuclear fusion creates a force acting outwards. this tends to make the star expand.
- the force of gravity acting inwards is balanced due to the force of fusion acting outwards.
- because these two forces are balanced, scientists would say that the star is in equilibrium, and this can result in a long stable period that lasts for billions of years
- our sun is currently in this stage
what happens to main sequence stars?
- the hydrogen nuclei had been fusing together to form helium nuclei.
- at some stage the hydrogen in the star will begin to run out, which is basically its fuel
- therefore the outward force due to fusion is less than the inward force due to gravity, causing the star to collapse inwards.
- the collapse of the star causes its temperature to increase, as it’s now a small, hot, dense ball
- now helium nuclei fuse together to create heavier elements, including all elements up to iron on the periodic table (NUCLEAR FUSION starts up again), and the star expands to form either a red giant or a red super giant
what happens to main sequence stars the same size as our sun?
- the red giant, after a short time, will become unstable and expel its outer layers of dust and gas
- this leaves behind a hot, dense, solid core which doesn’t do any nuclear fusion: white dwarf
- over time, this white dwarf gets cooler and darker as it emits all of its energy, and will transition to a black dwarf (no longer any energy to emit light, will appear dark)
what happens to main sequence stars that are much bigger than our Sun?
- once again, helium nuclei fuse together to produce heavier elements.
- once again, the red super giant stops carrying out nuclear fusion. keeps up this cycle of expanding and contracting for a while
- at the end, the star explodes - this is called a supernova.
- the temperature in a supernova explosion is incredibly high, creating elements heavier than iron.
- these elements are then distributed throughout the universe
what could happen to the star after a supernova?
- if the star was simply very big, it will condense into a very dense core, called a neutron star
- if the star was absolutely massive, it could collapse in on itself, and become a black hole
why is a black hole called a black hole?
so dense that its gravity is able to pull in any light that passes nearby. appears as a hole in the Universe, emitting no light
what are the limitations of nuclear fusion, and how are these limitations overcome?
- nuclear fusion, in any of the red giant stages, and in any of the stages up until red super giant, cannot create any elements heavier than iron.
- the temperature of a supernova explosion is high enough to create elements heavier than iron.
describe how the Earth and the moon stay in orbit of the Sun and the Earth, respectively:
- the force of gravity acting between the Sun and the Earth holds the Earth in its orbit.
- the moon also has a circular orbit around the Earth. this is called a natural satellite, and once again, the force of gravity holds the moon in its orbit.
how does the force of gravity lead to a change in velocity but not a change in speed in satellites?
as objects are orbiting the Earth in a circular motion, this means their direction is constantly changing. therefore even if its speed is remaining the same, as the direction is constantly changing, the velocity must also be constantly changing (vector quantity).
what is a satellite?
any object that orbits a celestial body, such as a star or planet
- can be either natural or artificial
define orbit:
the curved path of one celestial object/space craft around another celestial object
give an example of a natural satellite:
moon
describe geostationary satellites and general satellites:
- artificial satellites are man-made.
- used for communication and orbiting telescopes
- geostationary satellites orbit once every 24 hours, so they point at the same part of the Earth.
- other artificial satellites orbit more frequently.
describe orbits:
- the force of gravity holds objects in their orbit, and satellites are no exception.
- in the case of circular orbits, the force of gravity is leading to a change in velocity, but not a change in speed.
- therefore the satellite is constantly accelerating, as acceleration = change in velocity / time
- if the speed of a satellite changes, the orbit radius must also change.
- if the speed of the satellite increases, the radius of its orbit decreases. this is because at a higher speed, the object requires a higher force of gravity to prevent it from flying off into space. by staying closer to the Earth, the gravitational force on the object is greater, and the object remains in stable orbit.
why do objects stay in orbit?
- Newton’s first law: an object travelling at a certain velocity will continue at this velocity unless acted on by a resultant force
- the Earth is so massive and close to the moon, so it exerts a strong gravitational pull which is felt as an attractive force towards the Earth
- however, as the moon is large, and travelling fast, it has a lot of momentum in its forwards direction, so the gravitational force isn’t strong enough to completely pull it into the Earth, it can only change its direction very slightly
- the Earth is always applying this gravitational force, so always changing the moon’s direction. the moon is always orbiting around the Earth
describe the discovery of red-shift:
- in the 1900s, astronomers were looking at the light emitted from different galaxies.
- they detected that the light from very distant galaxies has an increased wavelength compared to light from closer galaxies.
what is the main point of red-shift?
from Earth, every direction we look into space, the galaxies seem to be moving further and further away from us (the Universe is expanding)
- the main evidence for this is the red shifting of light from the galaxies. the explanation is the Big Bang theory