rotates on its axisonceevery 24 hours. different stars become visible in the night skywhile others disappearbelowthehorizon
earths orbit around the sun
the earth orbits around the sun once everyyear. an observer from earth will see different stars at differenttimes because of thismotion
observer location
starsvisible in the northernhemisphere may not be visible in southernhemisphere
circumpolar stars
rotate around the celestial poles without rising or setting
seasonal stars
rise and set in the skydue to earthsrotation and its orbit
seasonal stars visibility
the tilt of the earths axis and orbit creates changing seasons which affects visibility of stars
why summers are hotter than winters
the earth is tilted toward the sun and is higherintheskycausingthedaystobelonger and warmer
why the earth exhibits seasons
the earths orbit around the sun and the tiltofitsaxis causes the sunlight to vary
whythemoonexhibitsphases
the moons position relative to the earthand the sun causes varying amounts of sunlight to illuminate its surface as seen from earth
Keplers first law
each planetmovesaround the sun in an ellipticalorbit and the sun is at onefocus. this applies to the motionofplanets in the galaxy
Keplers second law
eachplanet always sweeps out the sameamountofarea from from it tothesun.planetsmovefaster the closer they are to thesun
Keplers third law
the length of a planetsyear is proportional to the size of itsorbit. the further a planets average distance from the sun the longer its year is
what does the force of gravitydepend on?
the mass of the twoobjects and theirdistancefromeachother
retrograde motion
refers to the apparentbackwardmotion of a planetagainstthebackdrop of stars as observed from earth
geocentric model
earth is considered to be at the center of the universe, and the sun and planets orbit around it.
heliocentricmodel
the sun is at the center of the solar system and the planetsorbitaround it.
neutrinos (how we knowfusion is occurring in the sunscore)
nuclearfusion in the sunscore can be detected on earth
Helioseismology (how we knowfusion is occurring in the sunscore)
uses vibrations of the sunssurface to map its interior
basic feature of a sunspot
About half the heat of the restof the sun (55,000 degrees). They lastfromdays to weeks, then fragment and spread out.
solar cycle and how it affects earth
The solar cycle is a natural phenomenon that influences solar actively levels over a 11-yearperiod, with effects on earth'sspaceenvironment, technology, and climate
Photosphere (oftheSun)
surface of the sun, part we see, has sunspots
chromosphere (of the sun)
above the photosphere, reflects the sunsmagneticfield
corona (ofthesun)
outeratmosphere, millions of degrees
differences and similarities between terrestrial planets and earth
Earth:
- Atmosphere mostly nitrogen and oxygen
-water vapor
- One moon
-Plenty of geological activity
Terrestrial Planets:
-Mostly Rocky Surfaces
-mars has a moon
usually has some kind of water (mars Venus)
-Venus is geologically active while the others are not
jovianplanets and Jupiter
-composed of gasses
-have solidcores
-multiple moon
- extensive storms
compareJovian and terrestrialplanets
both orbit the sun, both are composed of solid and gaseousmaterials
contrastJovian and terrestrialplanets
Jovian planets are larger, further from the sun, rotate faster, have more moons, more rings
terrestrial planets
Mercury, Venus, Earth, Mars
Jovianplanets
Jupiter, Saturn, Uranus, Neptune
roles our atmosphere plays
filters radiation, sculpts the surface, traps heat, weather
what evidence do we have for human caused climate change
glaciers are melting/disappearing, temperature of the planet is going up
Jupiter major moons
Io: most geologically active
Mimas: looks like a Death Star
Ganymede: largest moon
Europa: liquid water
Saturn major moons
Titan: biggest moon
Mimas
Enceladus: liquid water vapor
why terrestrial planets formed closer to the sun and Jovian planets further from the sun
because the Jovian planets are made of gasses and it doesn't work for them to be close to the sun
how can we explore inside our solar system
space probes, satellites, rovers, telescopes
how can we explore outside out solar system
telescopes, detection methods, interstellar probes, radio astronomy
difficulties associated with human space travel
time, cost, risk
what is required for life to exist
Atmosphere, differentiated (geologicalactivity), magnetic field (proximity to sun, presence of the moon), water, climate
ways to find other life in the universe
gothere, send out signals, listen
attributes of the most easilyfound extra-solar planets
largesize,orbital period, high stellar activity, proximity to earth