Space Physics Flashcards
Our solar system
One star - the Sun
Eight planets and dwarf planets that orbit the Sun
Natural satellites - moons that orbit planets
Part of the Milky Way Galaxy
Formation of the Sun
The Sun was formed from a cloud of dust and gas (nebula) pulled together by gravitational attraction
Fusion reactions in the Sun
When the Sun’s core became hot enough and dense enough, nuclear fusion reactions began
A star like the Sun is at equilibrium - gravity tends to pull it inwards, and radiation pressure from the nuclear reactions tends to expand it outwards
Life cycle of a star
All stars begin life in the same way
A cloud of dust and gas, also known as a nebula, is mainly comprised of hydrogen
This then becomes a protostar, which goes on to become a main sequence star
Following this, stars develop in different ways depending on their size
Sequence determining the life cycle of a star
Stars the same size as the Sun
Red giant star —- white dwarf —- black dwarf
Stars much bigger than the Sun
Red super giant star —- supernova —- neutron star, or a black hole (depending on size)
Formation of new elements
Elements heavier than iron are formed in a supernova explosion of high mass stars