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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. Collections of young - hot stars
synchrotron radiation
quasar
OB Associations
Celestial Sphere
2. The distance light travels in one year (=9.46x10^12km).
planetary nebula
Bok Globule
Light-Year
Extrasolar Planet
3. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
fewest moons
The Big Bang Theory resolves Olber's Paradox
Seyfert galaxy
semimajor axis
4. 1-orbit aroudn the sun 2- are in hydrostatic equilibrium and 'mostly round' 3- have not cleared debris around its orbit 4- are not satellites
Disk
Dwarf planets
Ground State
Plank's Law
5. The equation that describes how matter equates with energy
E=mc2
scarp
critical density
Resolving Power
6. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
SETI
Grand design spirals
Largest diameter
accretion disk
7. The mix of pure photon energy that emerged at the start of the universe.
Halo
Perihelion
Neutron Star
cosmic fireball
8. The apparent backward motion of a planet against the background of stars.
retrograde motion
Winter Solstice
greatest elongation
Callisto (Jupiter)
9. The rock that makes up the lunar maria
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.
Population 1 vs Population 2 stars
mare basalt
Roundest orbit
10. Approximate speed of light in a vacuum
300000 KM/sec
Inverse Square Law
Make up of the jovian planets
Parallax
11. A change in the appearance of the sun at the edge of the solar disk
Filament
synchrotron radiation
Limb darkening
Triple Alpha rocess
12. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
radio lobe
Kirchhoff's Law
Colestial Pole
Sb spiral galaxy
13. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
aphelion
Parallax
interstellar dust
H2 Regions
14. The projection of the Earth's equator onto the celestial sphere.
Parallax
jovian
Electromagnetic Radiation: Visible Light
Celestial Equator
15. When one side of a body always faces the planet it revolves around
synchronous rotation
A family of radiant energy- includes light
Seyfert galaxy
Stephen-Boltzman Law
16. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
density parameter
conjunction
Nova
planetesimal
17. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
Triple Alpha rocess
standard candle
CCD
Terrestrial Planets
18. A word used in astronomy to describe all elements besides hydrogen and helium
Largest diameter
Ammonia - methane - and water
Spectroscopic parallax
Metals
19. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Radiative Diffusion
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Make up of the terrestrial planets
Kuiper belt
20. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Filament
Ganymede (Jupiter)
bulge
Kirkwood gaps
21. 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:
Globular Cluster
A family of radiant energy- includes light
cosmology
Drake equation
22. 10 nm 10^2 nm
Celestial Equator
Electromagnetic Radiation: X-Ray
nucleus
Big Crunch
23. The material from which the solar system formed
cosmic fireball
solar nebula
molecular clouds
semimajor axis
24. Stars orvits do not define the spiral patterns - instead they are density waves that move at slower speeds (arms are defined by young O and B stars and gas clouds)
Dark Matter
Sa spiral galaxy
How is winding dilemma solved?
The Big Bang Theory resolves Olber's Paradox
25. The linear correlation between the rate of the expansion of the universe and distance. Says that as galaxies get farther away in space - the speed with which they recede from us increases. So we can measure the amount of recessional velocity and use
accretion
Focal Plane
Negative - Diverge - Less than 1
Hubble law
26. The entity from which the whole universe is postulated to have come from.
cosmic singularity
cosmological red shift
regolith
Photon
27. Venus (retrograde)
Electromagnetic Radiation: X-Ray
slowest rotation
Jupiters red spot
In an expanding universe all galaxies see all other galaxies that are not gravitationally bound to them receding away. This is what we see in the Hubble Law. We infer that the Hubble law also holds true for all other galaxies.
28. When the Sun is farthest south of the celestial equator (About December 22)
shape and color of ELLIPTICAL galaxies
Winter Solstice
gravity
Focal Length
29. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
Molecular Clouds
Flocculent spirals
critical density
Seeing
30. The sinking of denser elements to the center of a young molten planet
Cosmic Microwave Background (CMB)
dark energy
chemical differentiation
Pulsar
31. Elliptical orbits that come inside orbit of the Earth.
Nova
Apollo asteroids
Color Index
neutrino
32. The point in its orbit where a planet is farthest from the sun
aphelion
planetesimal
300000 KM/sec
Granules
33. IO
MOONS: largest size
matter dominated universe
synchrotron radiation
MOONS: most geologically active
34. A bridge of material held in position above the solar surface. They can remain for hours even days
CMB
rotation curve = dark matter?
Prominence
Photon
35. The process that powers the sun and hydrogen bombs
terrestrial planet
conjunction
Summer Solstice
Thermonuclear Fusion
36. A two-filter measure of the color - and hence temperature - of a star.
Color Index
Light-Year
Population 1 vs Population 2 stars
Primary Mirror
37. Hydrogen and helium (mainly)
open star clusters
Make up of the jovian planets
Globular Cluster
Occam's razor
38. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
critical density
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
Electromagnetic Radiation: Gamma Ray
great red spot
39. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
Positive - Converge - Greater than 1
Kuiper belt
Electromagnetic Radiation
Annular Eclipse
40. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Photometry
Halo
difference between maria and highlands of the moon.
Main Sequence
41. 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)
fastest rotation
quasar
Red Giant Branch Star
Planck time
42. A fusion process in which protons build together to form helium
gravity
Proton-proton chain
widmanstatten pattern
bulge
43. The name for the only seriously considered theory of the universe.
Plank's Law
Big Bang
Titus-Bode Law
We don't know. It might be but does not have to be.
44. Is there water on the moon?
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
Seeing
interstellar dust
Yes - frozen at the poles- remains protected from the suns rays
45. A push or a pull
zone
Photon
Precession
force
46. Saying that the sky should not get dark at night because all lines of sight end on a star meaning that the night sky should be ablaze BUT the big bang - because the universe had a beginning - says that the sky gets dark because out in space - galaxie
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47. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
synchronous rotation
Sc spiral galaxy
Umbra
coma
48. The larger bodies that formed early in teh solar nebula that were chemically differentiated
epicycle
Hydrostatic Equilibrium
planetesimal
meteor shower
49. Form honeycomb like patterns surrounding empty or nearly empty voids.
gravity
superclusters
Stephen-Boltzman Law
E=mc2
50. Rich= dense crowded cores of galaxies - poor= few members and a looser organization of galaxies
Asymptotic giant Branch Star
Light Pollution
Rich vs poor clusters
Proton-proton chain