SUBJECTS
|
BROWSE
|
CAREER CENTER
|
POPULAR
|
JOIN
|
LOGIN
Business Skills
|
Soft Skills
|
Basic Literacy
|
Certifications
About
|
Help
|
Privacy
|
Terms
|
Email
Search
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 two-filter measure of the color - and hence temperature - of a star.
Color Index
Largest diameter
H-are Diagram
MOONS: largest size
2. The rotation period of the Earth measured relative to the stars.
quasar
Hydrostatic Equilibrium
Sidereal Day
belt
3. Where is the center of the expansion
Sidereal Day
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
cosmic fireball
Pixel
4. The gap etween saturn's A and B rings
Cassini division
cosmic fireball
solar nebula
Spectroscopy
5. Venus
hottest surface
Titus-Bode Law
Plague
Grand design spirals
6. The displacement of spectral lines to redder colors caused by the expansion of the universe.
semimajor axis
cosmological red shift
Stephen-Boltzman Law
Supercluster
7. The displacement of spectral lines to redder colors caused by the expansion of the universe.
tectonics of Earth
cosmological red shift
Ground State
smallest diameter
8. The dark - relativley smooth areas on the moon; Latin for sea
Refractor
planetary nebula
Electromagnetic Radiation: Infrared
Maria
9. The distance a moon can be from a planet before shattering from tidal forces
Coronal Loop
roche limit
homogeneous
Autumnal Equinox
10. A small chunk of rock in space
White Dwarf
meteoriod
3 reasons we orbit satellites to observe universe
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.
11. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
interstellar dust
Electromagnetic Radiation: X-Ray
MOONS: larger than mercury
Terrestrial Planets
12. 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 _____.
Prominence
Supercluster
Photometry
Flat - Remain Parallel - Exactly 1
13. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
Shepherd satellite
Population 1 vs Population 2 stars
anorthosite
radiation dominated universe
14. 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.
Kuiper belt
protostar
plate tectonics
mapping the structure of Milky Way disk
15. When material is heated and moves taking the heat energy with it
Convection
Population 1 vs Population 2 stars
Electromagnetic Radiation
Ground State
16. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Vernal Equinox
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Parallax
Ionization
17. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
synchrotron radiation
Electromagnetic Radiation
Inverse Square Law
Photon
18. Venus
Thickest atmosphere
Spectroscopic parallax
meteor
Halo
19. Poitns of gravitational stability in the orbit of a planet
Lagrangian Razor
Light Pollution
Objective Lens
Nova
20. Long - meandering cliff formed when a planet surface cools and shrinks
inferior planets
Umbra
Prominence
scarp
21. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
Gravitational Lens
mass
CNO Cycle
Io (jupiters moon)
22. 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.
Jupiters red spot
Radiative Diffusion
Parsec
Secondary Mirror
23. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
Callisto (Jupiter)
Rich Cluster
Sb spiral galaxy
Corona
24. When one side of a body always faces the planet it revolves around
Positive - Converge - Greater than 1
Precession
synchronous rotation
Galilean satellite
25. Form honeycomb like patterns surrounding empty or nearly empty voids.
Ecliptic
superclusters
We don't know. It might be but does not have to be.
most moons
26. Radiation (possibly left over from the big bang) that fills the universe. Perfect black body spectrum and tells us a bit aout how galaxies are formed.
Cosmic Microwave Background (CMB)
HII Region
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Ground State
27. What are the three possible geometries of the universe?
Open - flat - and closed.
fewest moons
radiant
Kirkwood gaps
28. Sc galaxies
Flocculent spirals
Dark Matter
Planck time
Apparent Magnitude
29. Matter that reveals itself only through its gravitational attraction.
dark matter
coma
SETI
Zenith
30. Poitns of gravitational stability in the orbit of a planet
Blackbody
Spectroscopic parallax
Lagrangian Razor
Color Index
31. 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)
Flat - Remain Parallel - Exactly 1
Doppler Shift
rotation curve = dark matter?
Triple Alpha rocess
32. The law that syas light energy from a blackbody increases as (temperature^4)
Black Hole
Stephen-Boltzman Law
Perihelion
Prominence
33. Finding a star's absolute magnitude from it's placement on an HR diagram. After finding the absolute magnitude - we measure the apparent magnitude - for a distance modulus and use this to find the distance. This method is good for finding distances t
Spectroscopic parallax
H2 Regions
Hydrostatic Equilibrium
Parallax
34. A two-filter measure of the color - and hence temperature - of a star.
Color Index
Kirchhoff's Law
Proton-proton chain
difference between maria and highlands of the moon.
35. The force of attraction between any two objects having mass
gravity
dark matter
AGN
Poor Cluster
36. The particle horizon is the farthest we can see. It exists because the universe had a beginning and thus a definite age. Light from distances farther away from the particle horizon have not had time to reach us yet.
Electromagnetic Radiation
Particle Horizon
Focal Length
chemical differentiation
37. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
Primary Mirror
Supercluster
Primary Mirror
Europa (Jupiters moon)
38. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
Color Index
Convection
quasar
Instability strip
39. The first rock-sized bodies that formed in the solar nebula from dust grains
chondrite
open star clusters
chemical differentiation
era of recombination
40. A huge sphere of tenuous gas surrounding the nucleus of a comet
coma
Metals
Triple Alpha rocess
Poor Cluster
41. The Big Bang says that the universe has not existed forever. It had a distinct beginning about 14 billion years ago called the 'Big Bang'. Therefore light from any object more than 14 billion light years away has not had time to reach us. The other p
Warning
: Invalid argument supplied for foreach() in
/var/www/html/basicversity.com/show_quiz.php
on line
183
42. Venus
planetesimal
Total Eclipse
Thickest atmosphere
Spectroscopic Parallax
43. All possible types of energy that can be emitted and absorbed by atoms.
Electromagnetic Radiation
H-are Diagram
most moons
Quasar
44. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
Focal Plane
opposition
Interstellar Extinction
Convection
45. The location of a supermassive black hole
Sunspot cycle
Nucleus
neutrino
Turn off Point
46. A point in the sky where meteors appear to come from during a shower
radiant
Hydrostatic Equilibrium
resonance
Kirkwood gaps
47. The entity responsible for spiral arms in grand-design spiral galaxies
Density Wave
Thermonuclear Fusion
blazar
Perihelion
48. A force exerted by reflecting sunlight
Degeneracy
superclusters
radiation pressure
Horizontal Branch Star
49. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
blazar
Superior planets
Oort Cloud
Gravitational Lens
50. Mercury
thinnest atmosphere
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
Synodic Day
Astronomical Unit