Quiz
Astronomy 235- Dr Miroshninchenko Midterm Review 2015
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Questions in this quiz (23)
1What is the age of the Universe?
- A13 billion years
- B14 billion years
- C13 million years
- D14 million years
2Who were the most influential figures in the history of astronomy?
- AKepler and Brahe
- BEratosthenes and Ptolemy
- CGalileo and Copernicus
- DSocrates and Aristotle
- EAll of the above
3[blank_start]Eratosthenes[blank_end] was the first to measure the [blank_start]circumference[blank_end] of the Earth which helped to prove the Earth wasn't flat. Copernicus developed the heliocentric system and believed in [blank_start]perfect circle[blank_end] revolutions of the planets. Ptolemy's discoveries include developing the Ptolemaic universe model which was [blank_start]earth-centered[blank_end], [blank_start]epicycles[blank_end], and cataloging 1028 stars positions. [blank_start]Brahe[blank_end] is responsible for [blank_start]Tycho[blank_end]'s quadrant which is [blank_start]1/4[blank_end] of [blank_start]an arch[blank_end], used to measure positions, precision of the angular observant, and [blank_start]one[blank_end] second of [blank_start]an arc[blank_end]. The [blank_start]ellips[blank_end] orbit was discovered/hypothesized about by [blank_start]Kepler[blank_end]. Galileo discovered [blank_start]sunspots[blank_end], mountains and valleys on [blank_start]the moon,[blank_end] the [blank_start]four[blank_end] moons of [blank_start]Jupiter[blank_end], phases of [blank_start]venus[blank_end], and used the first telescope as a scientific instrument. Kepler is also responsible for [blank_start]3 laws[blank_end]. The first is that planets have elliptical orbits. The second is that when a planet is [blank_start]closer[blank_end] to the sun it moves [blank_start]faster[blank_end] than when it is [blank_start]further away[blank_end], and the [blank_start]third[blank_end] is that you can measure the [blank_start]orbit[blank_end] period of a planet that orbits around the sun and convert it to [blank_start]Earth years[blank_end] and then [blank_start]square[blank_end] it and the [blank_start]cubed root[blank_end] will be it's [blank_start]AU[blank_end] from the sun.
- AEratosthenes
- BKepler
- CGalileo
- DBrahe
- EPtolemy
- FTycho
- Gradius
- Hdiameter
- Icircumference
- Jsurface area
- Kelliptical
- Lrectangular
- Mirregular
- Nperfect circle
- Oheliocentric
- Psun-centered
- Qearth-centered
- Rmoon-centered
- STycho
- TBrahe
- UKepler
- VEratosthenes
- WTycho
- XEratosthenes
- YBrahe
- ZAndromeda
- AA1/2
- AB1/8
- AC1/3
- AD1/4
- AE1/16
- AFan ellipse
- AGa circle
- AHan arch
- AIan arc
- AJan ellipse
- AKa circle
- ALone
- AMtwo
- ANthree
- AOfour
- APellipse
- AQcircular
- ARirregular
- ASKepler
- ATCopernicus
- AUBrahe
- AVNewton
- AWsunspots
- AXsolar flares
- AYsun storms
- AZthe moon,
- BAVenus
- BBMars
- BCMercury
- BDJupiter's moons
- BEone
- BFfive
- BGtwo
- BHthree
- BIfour
- BJSaturn
- BKJupiter
- BLUranus
- BMNeptune
- BNMercury
- BOVenus
- BPthe moon
- BQ3 laws of gravity
- BR4 laws of gravity
- BS4 laws
- BT3 laws
- BUthird
- BVPick the other one.
- BWfurther away
- BXcloser
- BYslower
- BZfaster
- CAfurther away
- CBcloser
- CCorbit
- CDrevoltionary
- CEastronomical units
- CFlight years
- CGEarth years
- CHdivide
- CIcube
- CJsquare
- CKmultiply
- CLcubed root
- CMsquare root
- CNproduct
- COquotient
- CPlight years
- CQastronomical units
- CREarth years
- CSepicycles
- CTellipses
- CUgravity
4 Roughly, how many stars are in the Milky Way galaxy?
- A100 million
- B100 trillion
- C100 billion
- D100 thousand
5Roughly how many galaxies are there in the Universe?
- A100 million
- B100 billion
- C100 trillion
- D100 thousand
6A [blank_start]galaxy[blank_end] is a huge collection of anywhere from a few hundred million to more than a trillion [blank_start]stars[blank_end], all bound together by [blank_start]gravity[blank_end].
- Agalaxy
- Bstars
- Cgravity
7Why does the milky way look like a band from Earth? Note: outline of sight lies in the plane of the galaxy.
- AWe are in the bulge and can only see the flat arms of the galaxy.
- BWe are on the arms and cannot see anything but the rest of the arm spread out around us.
- CWe are in the bulge and cannot see anything beyond the bulge.
- DWe are on the arm and see the disk
8Retrograde motion as explained by the [blank_start]Ptolemaic[blank_end] system is where the planets orbited around the [blank_start]Earth[blank_end] but also [blank_start]orbited around[blank_end] a fixed point within a smaller [blank_start]orbit[blank_end] similar to how the [blank_start]moon orbits Earth[blank_end] and [blank_start]Earth orbits the sun[blank_end]. The [blank_start]Copernican[blank_end] system explains retrograde motion by claiming the [blank_start]planets[blank_end] orbited around [blank_start]the sun[blank_end] in [blank_start]perfect circles[blank_end].
- APtolemaic
- BCopernican
- CNewtonian
- DBraheaic
- ESun
- FEarth
- Gmoon
- Hrevolutioned around
- Icircled around
- Jorbited around
- Kaxis
- Lrevolution
- Mgravitational pull
- Norbit
- OJupiter orbits the sun
- Pthe Earth orbits the sun
- Qthe moon orbits the Earth
- RJupiter's moons orbit each other
- Sthe moon orbits around the Earth
- TEarth orbits the sun
- Uthe moon orbits the Sun
- VEarth orbits the moon
- Wthe Ptolemaic
- Xthe Eratosthenic
- Ythe Keplarian
- Zthe Copernican
- AAthe planets
- ABthe sun
- ACthe moon
- ADthe Earth
- AE+the sun
- AF+the Earth
- AG+the planets
- AH+the moon
- AIirregular patterns
- AJellipses
- AKperfect circles
- ALimperfect circles
9What is direct proof the Earth is not stationary?
- Aparallax
- Bstellar parallax
- Cthe seasons
- Dthe clouds
10What elementary (subatomic) particles make up atoms?
- Aprotons
- Bneutrons
- Celectrons
- Dboth 1 and 2
- Eboth 1 and 3
- Fboth 2 and 3
11What are the main parameters of an EM wave (wavelength, frequency, amplitude)?
- Atravel through space with a speed c=> their wavelengths ^(greek letter) and frequency f are related
- Btravel through space with a speed c=< their wavelengths ^(greek letter) and frequency f are related
- Ctravel through space with a speed c=> their wavelengths ^(greek letter) and frequency f are not related
- Dtravel through space with a speed c=< their wavelengths ^(greek letter) and frequency f are not related
12What is the place of the visible light in the electromagnetic (EM) spectrum?
- Athe beginning
- Bthe end
- Coutside of it
- Dthe middle
13How are a photon's energy and frequency (wavelength) are connected?
- AThe higher the frequency, the more energy it produces.
- BThe lower the frequency the more energy it produces.
- CThe higher the frequency the less energy it produces
14What elementary particle is responsible for emitting radiation in atoms?
- Aphoton
- Bneutron
- Cproton
- Delectron
15What does the law of conservation of angular momentum state?
- Aan external force must act on an object for momentum to occur
- Ban external force must not act on an object for momentum to occur
- Cmomentum cannot be created or destroyed it simply exists
- Dmomentum must be created by a constant application of force
16What are the consequences of the law of angular momentum?
- Ainverse correlation
- Breverse correlation
- Cfaster movement to conserve angular momentum
- Dslower movement to conserve angular momentum
17What kind of frequencies (wavelengths) and energies do different types of photons have (for example, X-rays have high frequencies, low wavelengths, and high energies)?
- ALow-energy photons, like radio photons, tend to behave more like waves, while higher energy photons (i.e. X-rays) behave more like particles.
- BI don't know
- CHigh-energy photons, like radio photons, tend to behave more like particles, while lower energy photons (i.e. X-rays) behave more like waves
18The regions of the EM spectrum are:
- A Ultraviolet radiation, Visible radiation, Infrared radiation, Terahertz radiation, and Microwave radiation
- BGamma radiation, X-ray radiation, Ultraviolet radiation, infrared radiation, and radio waves
- CGamma radiation, X-ray radiation, Ultraviolet radiation, Visible radiation, Infrared radiation, Terahertz radiation, Microwave radiation, and Radio waves
- DGamma radiation, X-ray radiation, Infrared radiation, and Radio waves
- A Ultraviolet radiation, Visible radiation, Infrared radiation, Terahertz radiation, and Microwave radiation
19What are the basic properties of all EM waves? (Electromagnetic)
- Awaves travel parallel to each other
- Bwaves travel perpendicular to each other
- Csame amplitude and wavelength
- Dsame frequency and wavelength
- Esame frequency, amplitude, and wavelength
20What happens when radiation is emitted or absorbed by an atom?
- APhotons are created
- BLight is created
- Cphotons are destroyed
- Ddarkness is created
21What mirror size do the largest telescopes in the world have?
- A10m diameter
- B20m diameter
- C100m diameter
- D1000m diameter
22Which of the following statements best describes the two principal advantages of telescopes over eyes?
- ATelescopes can collect far more light with far better angular resolution
- BTelescopes can collect far more light with far greater magnification
- CTelescopes have much more magnification and better angular resolution
- DTelescopes collect more light and are unaffected by twinkling
- E Telescopes can see farther without image distortion and can record more accurate colors
23Which of the following was not discovered by Galileo?
- Aphases of Venus
- Bstellar parallax
- Cmountains and valleys on the moon
- D4 moons of jupiter
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- Description
- Based on the study guide (2015) for Dr. Miroshninchenko's midterm exam for Astronomy 235 at UNCG.
- Author
- Courtney Swartz
- Language
- English
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