8 - space Flashcards
cloud of dust and gas / Nebula
Stars initially form from a cloud of dust and gas called a nebula. The force of gravity pulls the dust and gas together to form a protostar.
protostar
As the star gets denser, the temperature rises and more particles collide with each other. When the temperature gets high enough, hydrogen nuclei undergo nuclear fusion (p.84) to form helium nuclei. This gives out huge amounts of energy, which keeps the core of the star hot. A star is born.
Main sequence star
The star enters a long stable period where the outward pressure
(p.67) 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 a main sequence star and it typically lasts
several billion years. The Sun is in the middle of this stable period.
red (super) giant
Eventually the hydrogen begins to run out. The star then swells into a red giant (if it’s a small star) or a red super giant (if it’s a larger star). It becomes red because the surface cools. Fusion of helium (and other elements) occurs. Heavier elements (up to iron) are created in the core of the star.
white dwarf
A small-to-medium-sized star like the Sun then becomes unstable and ejects its outer layer of dust and gas. This leaves behind a hot, dense, solid core - a white dwarf.
black dwarf
As a white dwarf cools down, it emits less and less energy. When it no longer emits a significant amount, it is called a black dwarf.
supernova
Big stars, however, start to glow brightly again as they undergo more fusion and expand and contract several times, forming elements as heavy as iron in various nuclear reactions. Eventually they’ll explode in a supernova, forming elements heavier than iron and ejecting them into the universe to form new planets and stars. Stars and their life cycles produce and distribute all naturally occurring elements.
neutron star / black hole
The exploding supernova throws the outer layers of dust and gas into space, leaving a very dense core called a neutron star. If the star is massive enough, it will become a black hole - a super dense point in space that not even light can escape from.
Planets
these are large objects that orbit a star. There are eight in our solar system.
their gravity is strong enough to have pulled in any nearby objects apart from their satellites.
Dwarf planets
These are planet-like objects that orbit stars, but don’t meet all of the rules for being a planet.
Moons
these orbit planets.
They’re a type of natural satellite (i.e. they’re not man-made).
Artificial satellites
satellites that humans have built. They generally orbit the Earth.
orbits
1) The planets move around the Sun in almost circular orbits (the same goes for the Moon orbiting the Earth).
2) If an object is travelling in a circle it is constantly changing direction, which means it is constantly accelerating. (Just like a car going around a roundabout.)
3) This also means it is constantly changing velocity (but NOT changing speed).
4) For an object to accelerate, there must be a force acting on it (p.111). This force is directed towards the centre of the circle.
5) This force would cause the object to just fall towards whatever it was orbiting, but as the object is already moving, it just causes it to change its direction.
6) The object keeps accelerating towards what it’s orbiting but the instantaneous velocity (which is at a right angle to the acceleration) keeps it travelling in a circle.
7) The force that makes this happen is provided by the gravitational force (gravity) between the planet and the Sun (or between the planet and its satellites).
orbit speed
1) The closer you get to a star or planet, the stronger the gravitational force is.
2) The stronger the force, the faster the orbiting object needs to travel to remain in orbit (to not crash into the object that it’s orbiting).
3) For an object in a stable orbit, if the speed of the object changes, the size (radius) of its orbit must do so too. Faster moving objects will move in a stable orbit with a smaller radius than slower moving ones.
red-shift
red shift is the increase in wavelength of light from galaxies as galaxies move away from us - shifted towards the red end of the spectrum.