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Test your basic knowledge |
Cosmology
Start Test
Study First
Subject
:
science
Instructions:
Answer 50 questions in 15 minutes.
If you are not ready to take this test, you can
study here
.
Match each statement with the correct term.
Don't refresh. All questions and answers are randomly picked and ordered every time you load a test.
This is a study tool. The 3 wrong answers for each question are randomly chosen from answers to other questions. So, you might find at times the answers obvious, but you will see it re-enforces your understanding as you take the test each time.
1. A small chunk of rock in space
Horizontal Branch Star
meteoriod
Cepheid variables
aurora
2. The point directly overhead.
Electromagnetic Radiation: Ultraviolet Light
Halo
MOONS: larger than mercury
Zenith
3. Distribution of dust (tells us disk is thin) - find distances to O&B stars and H2 regions (arms are sights of star formation and OB stars live and die at location of birth) -Milky way has four arms. Sun is in spur apart from arms.
Most dense
Photosphere
belt
mapping the structure of Milky Way disk
4. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Main Sequence
Hubble constant
mass
contrast northern lowlands and the southern highlands of mars...
5. Titan
MOONS: thickest atmosphere
Spectroscopic parallax
If it is in a denser medium - such as glass - it will move slower
Halo
6. Venus (retrograde)
slowest rotation
Electromagnetic Radiation: Microwave
direct motion
Asymptotic giant Branch Star
7. A quantity measuring the stability of the Earth's atmosphere
Seeing
dark matter
meteorite
Hydrostatic Equilibrium
8. The mass of an object divided by its volume
quarks
evidence of water on mars
density
Dark matter candidates
9. The 'edge' of the universe. Light beyond this has not reached us yet.
partile horizon
resonance
Spectral Lines
Photosphere
10. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Photon
Spectroscopic Parallax
aurora
quasar
11. The Greek philosopher responsible for making the stellar magnitude scale.
tectonics of Earth
Spectroscopic parallax
Stephen-Boltzman Law
Hipparchus
12. Dying large-mass stars lose their outer layers in a violent explosion creating large - chaotic remnants. these brighten like nova but are so much brighter and only occur ONCE PER STAR
aurora
supernova
jovian
Cassini division
13. The law stating that hotter blackbodies look bluer than cooler blackbodies.
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14. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
disk
Ionization
comet
Void
15. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Big Crunch
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Kirchhoff's Law
We don't know. It might be but does not have to be.
16. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
Blackbody
Planck time
Radio Galaxy
Wein's Law
17. Star speed at outer edge of galaxy should begin to diminish - but they dont so we guess that this means there is increasing force (aka dark matter)
plate tectonics
fastest rotation
cosmological principle
rotation curve = dark matter?
18. Approximate speed of light in a vacuum
Molecular Clouds
Negative - Diverge - Less than 1
300000 KM/sec
Differential Rotation
19. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
blazar
Spectroscopy
quasar
greehouse effects
20. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
aurora
Electromagnetic Radiation
Granules
Callisto (Jupiter)
21. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
Magnification
neutrino
rotation curve = dark matter?
meteor shower
22. The act of removing an electron from an atom.
zone
Ionization
Spectroscopy
Supercluster
23. IO
Big Crunch
Density Wave
cosmological principle
MOONS: most geologically active
24. The mirror that gathers the light in a reflector
Metals
Gravitational Lens
Active Optics
Primary Mirror
25. The mirror that determines the focus configuration of a reflector
Energy Level
mare basalt
Secondary Mirror
Negative - Diverge - Less than 1
26. A star that is in the process of forming. It glows from gravitational contraction
protostar
Thermonuclear Fusion
meteorite
era of recombination
27. A telescope that uses mirrors to focus light
Disk
Reflector
Energy Level
Negative - Diverge - Less than 1
28. The seasonal shifting of a nearby star's position relative to more distant objects.
H2 Regions
mapping the structure of Milky Way disk
Parallax
plate tectonics
29. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Light Gathering Power
Electromagnetic Radiation
Halo
MOONS: thickest atmosphere
30. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
radio galaxy
fastest rotation
Neutron Star
evidence of water on mars
31. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Hydrostatic Equilibrium
Magnification
Big Crunch
Observations of distant type Ia supernovae indicate that the expansion of the universe is speeding up with time - not slowing down! So there must be a force causing this.
32. The oldest part of the Milky Way
inferior planets
cosmological red shift
hottest surface
Halo
33. The gap inthe outer portion of Saturn's A ring
differential rotation
radio lobe
Blackbody Curve
Enke gap
34. The rotation of a star or planet at different speeds at its equator and poles
Neutron Star
direct motion
differential rotation
Hyashi track
35. Electromagnetic Radiation
Winter Solstice
Chromosphere
cosmic fireball
A family of radiant energy- includes light
36. The north-south line passing directly overhead through the zenith.
Sunspot cycle
Meridian
Synodic Day
radiation pressure
37. A change in the appearance of the sun at the edge of the solar disk
Thermal Equilibrium
Yes - frozen at the poles- remains protected from the suns rays
Convection
Limb darkening
38. A word meaning 'the same in all directions.'
isotropic
synchronous rotation
Light Pollution
density waves
39. Small compact stars called white dwarfs can have material deposited on their surfaces. In time material heats up and explodes in surface nuclear reaction- star brightens - settles - repeats.
radio galaxy
Metals
Cepheid variables
nova
40. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
tectonics of Venus
Asymptotic giant Branch Star
Cepheid Variable
Light-Year
41. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Energy Level
The Big Bang Theory resolves Olber's Paradox
Spectroscopic Parallax
tectonics of Mars
42. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
Disk
Vernal Equinox
CNO Cycle
meteorite
43. The movement of the Earth's crustal plates riding on top of the mantle.
Filament
Metals
Refractor
plate tectonics
44. The equation that describes how matter equates with energy
CCD
acceleration
Light-Year
E=mc2
45. The sinking of denser elements to the center of a young molten planet
It does not have to expand into anything. It might just be that the 3 dimensions of space are getting bigger. It may also be that our 3 spatial dimensions are expanding into higher dimensions if such things exist.
Colestial Pole
supermassive black hole
chemical differentiation
46. The imaginary sphere centered on the Earth that hols the stars.
Electromagnetic Radiation
Celestial Sphere
Primary Mirror
Hubble constant
47. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
Globular Cluster
Europa (Jupiters moon)
Sunspot cycle
tectonics of Earth
48. In a FLAT UNIVERSE(our universe) - the curvature of space-time is ________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
acceleration
Kirkwood gaps
Flat - Remain Parallel - Exactly 1
thinnest atmosphere
49. In a CLOSED UNIVERSE - the curvature of space-time is _________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
critical density
open star clusters
Positive - Converge - Greater than 1
Photon
50. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
widmanstatten pattern
Emission Spectrum
Photometry
quasar