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Astronomy Eng
| Term | Definition |
|---|---|
| Universe began | approximately 15 billion years ago |
| Big bang theory | gravity pulled together particles until the mass was so big it exploded |
| Planet formation | clumping and gravity of particles exploded during the big bang eventually formed planets |
| The universe is | expanding, all of the galaxies |
| Galaxy | Collection of solar systems |
| Solar system | Collection of planets/celestial bodies orbiting a star(s) |
| Our galaxy | the milky way (spiral shape) |
| The asteroid belt is between | Mars and Jupiter |
| The kuiper belt is between | Neptune and outer dwarf planets |
| The sun is | at the center of our solar system, and is the closest star to us |
| Coronal mass ejection (CME) | large expulsions of plasma and magnetic field from the Sun's corona |
| Sun spots | Cooler area's on the surface of the sun caused by disturbances in the Sun's magnetic field |
| Solar cycle | Every 11 years the Sun's magnetic poles flip, causing increased magnetic field disturbances |
| Earth's magnetic field | protects us from solar radiation and emissions |
| Electromagnetic spectrum represents | Energy emitted from the sun |
| Higher frequency light waves have __ energy | more |
| Lower frequency light waves have ___ energy | less |
| Lightwaves frequency | the number of light waves that pass a point within 1 second |
| Wavelength | the distance between wave peaks |
| Amplitude | the height of a wave, higher amplitude is higher strength |
| Longer wave lengths move | slower |
| Shorter wave lengths move | faster |
| Higher frequency light waves have a __ wavelength | shorter |
| Lower frequency light waves have a __ wavelength | longer |
| Infrared light is experienced as | heat |
| Ozone layer (atmosphere) protects us from | UV light |
| Visible light | the only part of the electromagnetic spectrum that the human eye can see |
| Dopple effect | apparent change in frequency (speed) of sound or light as an object moves towards or away from an observer |
| Element fingerprint | Electromagnetic wavelength that absorbs a specific element |
| Blue shift | Object moving towards the observer appears to increase in frequency, decrease in wavelength |
| Red shift | Object moving towards the observer appears to decrease in frequency, increase in wavelength |
| Evidence supporting big bang theory | Red shift and cosmic background radiation both support that the universe is expanding and has always been expanding since the initial big bang |
| Hubble's law | the distance a galaxy or star is from the Earth is proportional to the speed at which it is moving |
| Geocentric model | Earth is the center of the solar system (old theory) |
| Heliocentric model | Sun is at the center of the solar system (current theory) |