Interstellar space is the region between stars. It hosts a vacuum (absence of matter, < 1 atom per litre)
Cosmic rays are high-energy atomic nuclei ejected into space at extremely high velocity by supernova explosions
Objects in the Solar System
Oort Cloud
Kuiper Belt
Asteroids (Trojans, Greeks, Hildas)
Planets
Oort Cloud
A diffuse cloud of icy particles held in by the Sun's gravity past Neptune's orbit
Heliosphere
Technically delimits the edge of the Solar System, and incorporates the Kuiper Belt and planets lie within it
Most comets originate from the Kuiper Belt
Neptune forms the outer boundary of the Kuiper Belt; inside this is interplanetary space
Most asteroids lie between the orbit of Mars and Jupiter
Some asteroids (known as the Trojans and the Greeks) border Jupiter's orbit, while the Hildas lie between the main asteroid belt and Jupiter
Astronomical Unit (AU)
Distance between Earth and Sun
Terrestrial planets look markedly different from the gas giants as well as from each other
Magnetic field
The region measurably affected by the force emanating from a magnet
Earth acts as a dipole or magnet with a north pole and a south pole
Geographic poles
Places where Earth's rotational axis intersects the planet's surface
Magnetic poles
Magnetic north lies near geographic south pole; magnetic south lies near geographic north pole
Solar winds distort Earth's magnetic field into a huge teardrop away from the Sun, deflecting most solar-wind particles
Van Allen Radiation Belts occur where Earth's magnetic field starts to strengthen, trapping cosmic rays and solar-wind particles that managed to enter the magnetosphere
Particles passing through the Van Allen Belt reach Earth and follow magnetic lines to the poles causing gases to glow as aurorae
Latitude
East-west lines parallel to the equator
Longitude
North-south lines connecting poles
Atmosphere
The gaseous layer enveloping the whole Earth, containing a mixture of gases known as air
Variable amounts of water (H2O) vapour are prominent at lower elevations that form clouds, hiding about 70% of the planet's surface
Density and pressure of the atmosphere
Progressively increase towards Earth's surface due to the weight of overlying air
99% of atmospheric gas lies at lower 50 km of atmosphere; above, pressure and density are very low
Beyond 600 km, molecules no longer interact and collide like a gas; considered upper boundary of atmosphere
Layers of the atmosphere
Thermosphere
Mesosphere
Stratosphere
Troposphere
Components of the Earth System
Atmosphere
Hydrosphere
Cryosphere
Biosphere
Solid Earth
Habitable zone
Distance from Sun with temperatures between boiling and freezing points of water
Mars and Venus do not have life mostly due to the abilities of their atmospheres to trap heat
The Earth's System is dynamic and constantly moving, requiring significant energy from heat from inside the Earth, gravity, Sun's heat, and Sun's light
Earth's surface composition
30% dry land (continents and islands)
70% surface water (saline oceanic water, some fresh surface and shallow groundwater)
Ice covers land and sea
Surface has topography, i.e. variations in elevation identifying plains, mountains and valleys
Ocean floor features
Abyssal plains
Mid-ocean ridges
Deep-sea trenches
Hypsometric curve shows most of land surface is within 1 km of sea level, and most of seafloor lies between 4 km and 5 km of sea level