P6 - space phy Flashcards
(52 cards)
how does the days work
-sun goes from east to west because of the earth’s rotation on its own axis
what controls the tides
moon
why can you see the moon at night
-it reflects the sun’s light
time taken for the moon to completely orbit around the earth
27.5 days/ 1 month
moon phases
-the moon’s orbit relative to the earths change, results in varying sunlight on different parts of the moon
-its a natural satellite of earth
time taken for the earth to completely orbit around the sun
365 days
seasons
-caused by the earth’s axis being tilted so different hemispheres receive varying amounts of sunlight = diff seasons
eg. summer & winter/ spring & autumn
-countries near the equator don’t have seasons as they receive direct sunlight all year
-the further the country from the equator, the more noticeable the season changes
order of the 8 planets from the Sun
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-Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune
-rocky planets - Mercury, Venus, Earth, Mars
-gas giants - Jupiter, Saturn, Uranus, Neptune
-Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto have moons
-there’s an asteroid belt btw Mars & Jupiter
what orbits the Sun
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-dwarf planets - Pluto, Eris
-moons that orbit planets
-asteroids & meteoroids
-comets
what hold the celestial objects that the orbit the sun
-the sun’s gravitational pull
-greater the distance, the weaker the gravitational pull, slower orbital speed
-planets size affects the gravitational pull
heaviest object in the solar system
sun
what are moons
natural satellites that orbit planets
what are asteroids & meteoroids
lumps of rock
what are comets
-at their farthest distance form the Sun, they’re made of frozen gas, rocks & dust
-as they move to the sun, they warm up & release a trail of gas & dust behind them
-orbits the sun in irregular paths
origins of the solar system
from a nebula, a large rotating cloud of gas & dust
accretion disk
flat rotating disk made by the spinning motion of the nebula
formation of planets
-planets were formed from the leftover material from the nebula that wasn’t drawn into the sun’s gravitational pull
-through accretion, smaller particles (gas & dust) were pulled tgt by gravity to form larger rocks = Rocky planets
-the heat of the sun pushed the lighter materials away from it to form Gas Giants
speed of light
3 x 10^8 meters per second
elliptical
the shape of the the orbits around the sun
eccentricity
how much the orbit path deviates from a perfect circle
why are orbits elliptical
-at the start, the object travels past the sun due to its own momentum from the big bang
-When it gets close to the sun, the sun’s gravity pulls it
-the object speeds up & its kinetic energy carries it to its furthest point of the orbit
-the object then slows down & is pulled back to the sun again
formula for orbital speed
2πr
——— = orbital speed (meter per second)
t
-orbital speed - speed of a planet in an orbit around the sun
-r - orbital radius - average distance from the planet to the sun
-t - orbital period - time taken for 1 complete orbit
define star
-ball of hot gas & plasma that is powered by nuclear fusion in its core
-usually has hydrogen & helium
define nuclear fusion
process of merging small nuclei into larger -nuclei to release energy
-needs high temp & pressure to start