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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. When one side of a body always faces the planet it revolves around
Convection
deferent
general star population
synchronous rotation
2. Hurricane-like vortex in southern-hemisphere winds to north and south blow in opposite directions which keep it spinning and with no subsurface features like mountians it persists.
radio lobe
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
Proton-proton chain
Jupiters red spot
3. Venus (retrograde)
Cassegrain Focus
partile horizon
Inverse Square Law
slowest rotation
4. The apparent backward motion of a planet against the background of stars.
Milky way Galaxy
retrograde motion
Proton-proton chain
tectonics of Venus
5. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
disk
Electron
tectonics of Mars
Vernal Equinox
6. The light produced when particles from the sun collide with atmospheric molecules
Brown dwarf
aurora
great red spot
Cassegrain Focus
7. Why does the earth have few craters while the moon has many?
superclusters
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
Vernal Equinox
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
8. A spectrum of light with energy at only a few wavelengths.
jovian
Big Crunch
Emission Spectrum
quarks
9. A method of finding a star's distance from its absolute magnitude and spectral type or color.
dark energy
Spectroscopic Parallax
tectonics of Mars
quarks
10. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Negative - Diverge - Less than 1
density parameter
quasar
Sc spiral galaxy
11. Light-colored high-pressure bands in Jupiter's atmosphere
Rich Cluster
zone
coma
asteroid
12. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Photometry
era of recombination
dark matter
general star population
13. The 'edge' of the universe. Light beyond this has not reached us yet.
scarp
partile horizon
How is winding dilemma solved?
Kirchhoff's Law
14. The organized effort to find life elsewhere in the universe. (Search for Extra-Terrestrial Intelligence)
Halo
Flocculent spirals
Kirchhoff's Law
SETI
15. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
shape and color of ELLIPTICAL galaxies
meteor shower
CCD
cosmology
16. The projection of the Earth's equator onto the celestial sphere.
force
Electromagnetic Radiation: Radio
Thermal Equilibrium
Celestial Equator
17. Mercury
Oort cloud
semimajor axis
Resolving Power
smallest diameter
18. 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)
Umbra
Sunspot cycle
Sunspots
Planck time
19. A telescope that uses lenses to focus light
Sunspots
Refractor
Grand design spirals
Jupiters red spot
20. The law that describes the blackbody curve - and let to quantum mechanics.
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21. The mirror that determines the focus configuration of a reflector
Secondary Mirror
fusion crust
Dwarf planets
Quasar
22. Matter that reveals itself only through its gravitational attraction
Galilean satellite
regolith
Dark Matter
thinnest atmosphere
23. A large and bright but cool star.
Red Giant
MOONS: most geologically active
mass
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
24. A quantity measuring the stability of the Earth's atmosphere
High Velocity Stars
Seeing
Instability strip
Thermal Equilibrium
25. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
comet
greehouse effects
quarks
Plague
26. A continuous spectrum of light missing energy at a few wave lengths.
quasar
dark matter
Planetary Nebula
Absorption Spectrum
27. A particle of light
Photon
meteorite
Nebula
cosmic fireball
28. First accurately measured the speed of light in a vacuum
Electron
Ole Roemer
Clouds of sufuric acid (very inhospitable and brightest object in the sky) - process called greenhouse affect traps radiation making it 900 degrees at times - spins with retrograde rotation (sun rises in west) and takes 58.4 days for it to set. Thick
radiation pressure
29. 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)
standard candle
Hydrostatic Equilibrium
Filament
rotation curve = dark matter?
30. Ganymede and Titan
bulge
MOONS: larger than mercury
Spectral Lines
Maria
31. 1. We see rapid movements or high energy radiation coming at some level from the nuclei of nearly every galaxy we have looked at. 2. We suspect that the creation of these supermassive black holes is part of the galaxy formation process.
Jupiters red spot
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Neutron Star
Electromagnetic Radiation: Visible Light
32. An energetic event taking place in the early universe
Occam's razor
CNO Cycle
Gamma-ray Burst
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
33. The faint glow of light left over from the Big Bang. cosmic microwave background are the photons that remain after the big bang that have not turned into matter.
Milky way Galaxy
CMB
Make up of the jovian planets
Planck time
34. First accurately measured the speed of light in a vacuum
Spectroscopic parallax
zone
Ole Roemer
deferent
35. The faint glow of light left over from the Big Bang. cosmic microwave background are the photons that remain after the big bang that have not turned into matter.
supernova
nova
reflection star clusters
CMB
36. A rock or iron specimen that has fallen from space
Supernova (You can be my supernova girl)
radio lobe
meteorite
open star clusters
37. The distance light travels in one year (=9.46x10^12km).
Light-Year
Horizontal Branch Star
meteor
coma
38. Loops that trace the magnetic field as it erupts from a sunspot area and arches over to an adjacent area. They glow in the light of gas pouring out of corona and falling into photosphere.
Autumnal Equinox
Negative - Diverge - Less than 1
Triple Alpha rocess
Coronal Loop
39. The location of a supermassive black hole
Cassini division
molecular clouds
Nucleus
Radiative Diffusion
40. 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 _____.
Cassini division
Electromagnetic Radiation: X-Ray
Flat - Remain Parallel - Exactly 1
partile horizon
41. The entity from which the whole universe is postulated to have come from.
cosmic singularity
H-are Diagram
Extrasolar Planet
Asymptotic giant Branch Star
42. Jupiter - Saturn - Uranus - Neptune
Objective Lens
cosmology
Jovian Planets
open star clusters
43. N=are*Fp(Ne)(Fl)(Fi)(Fc)(L) N: number of civilizations possible to communicate with are*: rate solar-like stars are created Fp: fraction of stars with planets Ne: number of planets like ours Fl: fraction of planets with life Fi: intelligent life Fc:
opposition
Gravitational Lens
Penumbra
Drake equation
44. Light scattered through the atmosphere that degrades astronomical images
Neutron Star
Light Pollution
accretion disk
greatest elongation
45. A two-filter measure of the color - and hence temperature - of a star.
Radiative Diffusion
Main Sequence
Black Hole
Color Index
46. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Coldest surface
CCD
H-are Diagram
Seyfert galaxy
47. A bright area of higher temperature that often proceeds the formation of sunspots.
Clouds of sufuric acid (very inhospitable and brightest object in the sky) - process called greenhouse affect traps radiation making it 900 degrees at times - spins with retrograde rotation (sun rises in west) and takes 58.4 days for it to set. Thick
Winter Solstice
Plague
Sunspot cycle
48. Large nebula consisting of very cold gas and dust
Big Bang
H2 Regions
Ecliptic
Molecular Clouds
49. The Greek philosopher responsible for making the stellar magnitude scale.
great dark spots
Prominence
coma
Hipparchus
50. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
Absolute Magnitude
chemical differentiation
asteroid
Ionization