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卡片总数: 24内容版本: v4公开卡包更新时间: 8/1/2026

卡片预览 (24 张)

#1
正面 (问题)

what are the atmospheres of the terrestrial planets like?

背面 (解答)

• made of rocky substances • metallic core composed of mostly iron with a surrounding silicate mantle (mercury venus earth mars) • have common surface features like canyons, creaters, mountains, volcanoes • have secondary atmospheres which are gnereated through volcano or comet impact • more dense than jovian

#2
正面 (问题)

where did the water for earths oceans come from

背面 (解答)

-water came from comets and icy objects bombarding the earth

#3
正面 (问题)

why dont venus and mars have oceans

背面 (解答)

• mars is too cold, low temperatures water wouldnt be stable in liquid phase • venus is too hot to sustain water

#4
正面 (问题)

how do the jovian planets differ from earth? why are they so different?

背面 (解答)

• made of gas • jupiter and saturn contain almost entirely hydrogen and helium • different because of formation of solar system: formed behind frost line where hydrogen could condense into ice - formed farther from sun • jovian planerts are larger than earth & terrestrial planets - less dense

#5
正面 (问题)

how do we know that earth formed from the accretion of smaller rocky objects

背面 (解答)

• craters on earths surface • iron meteorite and stony meteorite • moon and mercury show evidence through meteorites

#6
正面 (问题)

where are most comets located? how do we explain the origin of comets

背面 (解答)

• comets are located in the oort cloud - 10,000x farther away from sun then earth • they originate from the oort cloud and Kupier belt • oort cloud - has icy bodies and a star can pull one out letting it fall to earth as a comet • kupier belt - composed of icy bodies (short period comets)

#7
正面 (问题)

why is the solar system flat?

背面 (解答)

• based on current obsevations, we can see solar systems beyond our own • the solar system is flat because of angular momentum

#8
正面 (问题)

what is the nebular hypothesis?

背面 (解答)

• the nebular hypothesis ocurred when the gravity contracted the solar nebula na dmost of the material collected in the center to from the protosun • remaining materials formed a thick, flattened, rotating disk within which matter gradually cooled and condensed into grain of clumps and icy, rocky material • repeated collisions resulted in the material clumping together into planets

#9
正面 (问题)

what seven wanderers did the ancient greek astronomers identify in geocentrism

背面 (解答)

• moon • mercury • venus • sun • mars • jupiter • saturn

#10
正面 (问题)

what did the Ptolemaic (geocentric) model include and why ?

背面 (解答)

• earth was the center of the solar system - motionless • believed all celestial objects orbited erath • assumed each planet moved on a small sphere of circle called an epicycle

#11
正面 (问题)

what discover made by galileo led to the downfall of geo-centrism? why?

背面 (解答)

• the discovery of the phases of venus • ptolemaic system argues that the crescent phases of venus should never be seen from earth • we are able to see phases, therefore copernican view of sun centered universe is more accurate

#12
正面 (问题)

what is retrograde motion?

背面 (解答)

• the westward motion of planets. Since Earth moves much faster than the other planets, the slower moving planets appear as if theyre going in reverse • earth moves faster than mars so when it passes mars it looks like mars is moving backwards

#13
正面 (问题)

How was retrograde motion explained in both the Ptolemaic (geocentric) and Copernican (heliocentric) models?

背面 (解答)

• geocentric: used epicycles to explain the retrograde motion - the center of the epicycle moves in large circl called a deferent • heliocentric: planets further from sun move more slowly. As earth laps mars, mars appears to go bakcward as seen by observer on earth

#14
正面 (问题)

what is keplers three laws of planetary motion?

背面 (解答)

a. Elliptical orbits (all planets move about sun in elliptical orbits) - planets are sometimes closer to sun and go fast. further away and go slow b. equal areas in equal times - describes the speed of a planet traveling in an elliptical orbit around the sun. Line between sun and planet sweeps equal areas in equal times c. period squared = distance cubed - planets in solar sytem have no linear relationship between planets orbit and distance around sun

#15
正面 (问题)

what discovery by newton verified keplers laws?

背面 (解答)

when he proposed the law of univeral gravitation. Gravitational force was the cause of Kepler’s laws

#16
正面 (问题)

what are the phases of the moon? Is the moon ever visible during the day? Start with new moon

背面 (解答)

New moon: The moon is between sun and earth - back lit waxing crescent: sunlit portion is increasing but still less than half (right side lit) first quarter: half of the moon is lit. right side waxing gibbous: more than half is lit (left side is unlit) full moon: earth sun and moon are in approximate alignment - entire sunlit part is facing us waning gibbous: light decreases, more than half lit (right side unlit third quarter: half moon is lit - left side is lit waning crescent: more is dark lit, only part of left side is lit • the moon can be seen during the day when it is in New moon as it moves away from the sun

#17
正面 (问题)

what are the differences between the crescent moon visible after sunset and the one visible before sunrise?

背面 (解答)

After sunset: moon appears very low in western sky, has low surface brightness, ddrawn curved to the right before sunrise: points eastward - drawn curved to the left

#18
正面 (问题)

what is the connection between lunar phases? why don’t eclipses happen every month?

背面 (解答)

• solar eclipses only happen when moon is in new moon phase: plane of moons orbit is aligned with earth’s orbit around sun - only happens once or twice a year • lunar eclipses only occur when moon in in full phase - planes have to align • They dont happen every month because the moon does not orbit in the same plane as earths orbital plane • more likely to see lunar eclipse

#19
正面 (问题)

what do we know about the suns visible surface and outer atmosphere & how do we know it

背面 (解答)

outer atmosphere: photosphere, chromosphere, and corone Photosphere: very active, gives off visible light strongly, has sunspotss which emerge when suns magentic field breaks through the surface Chromosphere: emits a reddish glow as hydrogen burns off. Plays a role in heat from interior to corona Corona: thrid layer of suns atmosphere. hotter than photosphere. only visible during a solar eclipse. -studied through solar exlipses and satellite devices

#20
正面 (问题)

what do we know about the suns interior and how do we know it

背面 (解答)

-suns interior is opaque -core: pure helium -radiation zone: hydrogen Convection zone: doesnt transmit light -observed throug hhelioseismology which studies suns movement/swinging. these movements are caused by sound waves

#21
正面 (问题)

how big is the sun and how does it compare to other stars

背面 (解答)

• the suns circumference is about 2,700,000 miles - you could line up 109 earths across the face of the sun • suns diameter is 100 times wider than earth, gaseous, not very dense • stars are 700 times bigger than our sun - our sun is ver y average

#22
正面 (问题)

what are the two most abundant chemical elements in the sun? How are they related to the source of the suns energy

背面 (解答)

-hyrdogen and helium - hydrogen nuclei crash together and form helium in nuclear fusion - releases gamma waves which turn into visible light

#23
正面 (问题)

what are the seven regions of the electromagnetic spectrum? what are their similarities and differences

背面 (解答)

highest energy - lowest (shortest - longest wavelength) a. gamma rays b. x ray c. ultraviolet d. visible e. infared f. microwave g. radio wave

#24
正面 (问题)

why are radio telescopes placed in desert valleys? why are optical telescopes placed on mountain tops? why are some telescopes put into orbit?

背面 (解答)

Desert valleys: humans dont emit radio waves in deserts & can get away from human interference, possible to do day or night Mountain tops: less atmosphere pollution, easier to see, less light interference from cities orbital telescopes: study visible light from space and ultraviolet telescopes study very hot stars, these lights can only be studied from space bc theyre . blocked from our atmosphere